Start time (UTC),Duration,Date ,Team,SPASS Type,Target,Request Name,Library Definition,Title,Description,,,,,, ,,,,,,,,,,,,,,, 2004-135T18:40:00,000T01:00:00,14-May-04,ADMIN,Prime,Saturn,TEST333,,,Milestone.,,,,,, 2004-135T18:40:00,000T09:22:00,14-May-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-135T18:40:00,025T20:57:59,14-May-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust exploration - saturn,"for prograde dust (Saturn cent.): -z2E, -x 21;-18.6 AM=52",,,,,, 2004-135T18:40:00,000T10:37:00,14-May-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-135T18:40:00,027T09:21:59,14-May-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: -X to sun, with either -Y to Saturn, or Saturn in S/C X, Z plane. This allows pick up ions to be measure, along with either Saturn ENA, or upstream ion events.",,,,,, 2004-135T18:40:00,002T23:52:00,14-May-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-135T20:01:00,000T02:30:00,14-May-04,ISS,Prime,rings(general),DIFSATSRC,Diffuse ring satellite search,OBSERVATIONS OF DIFFUSE RINGS AND SATELLITES PRE-S,"OBSERVATIONS OF DIFFUSE RINGS AND SATELLITES AT LOW PHASE BEFORE SOI; LAST CHANCE BEFORE FINAL SOI TRAJECTORY IS SET. THIS SET MAY HAVE 2 POINTINGS AT EACH ANSA, REPEAT L,R,L,R. EACH POINTING HAS 28 IMAGES AS: 2 SATELLITE EXP, 10 DIFFUSE RING EXP/POL/FILT, 2 SATELLITE EXP.",,,,,, 2004-135T20:01:00,000T02:30:00,14-May-04,VIMS,SPASS Rider,rings(general),DIFSATSRC,Diffuse ring satellite search,Early search for E Ring,"Rider on ISS E Ring/satellite search. 1-sec exposures, IR + VIS. Dimensions selected to fit ISS dwell times. Additional short exposures. 21 Mbits/hour. Further details TBD.",,,,,, 2004-135T22:31:00,000T04:16:00,14-May-04,UVIS,Prime,Saturn,MOS04PER,Linear mosaic,MOSAIC_09_PER_04,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit perpendicular to the Saturn Equator. 2) Slew about the Z-axis from Saturn Center to +MOS Orb. 3) Step 20 times using 1.75mrad increments about the Z-axis to -MOS Orb for 7200s. Stare for 360s during each step increment. 4) Step 14 times using 1.75mrad increments about the Z-axis toward +MOS Orb for 3600s. Stare for 360s during each step increment. 5) Slew back to Saturn Center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 16.88mrad.,,,,,, 2004-136T02:47:00,000T02:30:00,15-May-04,ISS,Prime,rings(general),DIFSATSRC,Diffuse ring satellite search,OBSERVATIONS OF DIFFUSE RINGS AND SATELLITES PRE-S,"OBSERVATIONS OF DIFFUSE RINGS AND SATELLITES AT LOW PHASE BEFORE SOI; LAST CHANCE BEFORE FINAL SOI TRAJECTORY IS SET. THIS SET MAY HAVE 2 POINTINGS AT EACH ANSA, REPEAT L,R,L,R. EACH POINTING HAS 28 IMAGES AS: 2 SATELLITE EXP, 10 DIFFUSE RING EXP/POL/FILT, 2 SATELLITE EXP.",,,,,, 2004-136T02:47:00,000T02:30:00,15-May-04,VIMS,SPASS Rider,rings(general),DIFSATSRC,Diffuse ring satellite search,Early search for E Ring,"Rider on ISS E Ring/satellite search. 1-sec exposures, IR + VIS. Dimensions selected to fit ISS dwell times. Additional short exposures. 21 Mbits/hour. Further details TBD.",,,,,, 2004-136T04:02:00,013T19:58:00,15-May-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-136T05:17:00,000T10:06:00,15-May-04,CIRS,Prime,Saturn,TEMPSIT,Thermal map,CIRS_000SA_TEMPSIT,"Early temperature map of Saturn, starting when Saturn subtends ~5 mrad. With a 2 mrad pointing uncertainty, 3 array positions covers the disk",,,,,, 2004-136T05:17:00,000T10:06:00,15-May-04,ISS,SPASS Rider,Saturn,TEMPSIT,Thermal map,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-136T05:17:00,000T05:00:00,15-May-04,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required. Includes 2 hours for IFC cal and range checks.",,,,,, 2004-136T10:17:00,006T15:30:00,15-May-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-136T13:08:00,000T08:00:00,15-May-04,RSS,SPASS Rider,Earth,USO,Ultra stable oscillator,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. Last 4 hours required to be tracked at DSS-25 in 1-way mode. Last 4 hours are also desired to be tracked at DSS-14 in 1-way mode.,,,,,, 2004-136T15:23:00,000T00:30:00,15-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-136T17:08:00,000T09:00:00,15-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-136T17:53:00,000T06:00:00,15-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-136T18:00:00,000T02:17:00,15-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-137T03:00:00,000T02:17:00,16-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-137T03:23:00,000T11:37:00,16-May-04,UVIS,Prime,Saturn,MOS10PE,Linear mosaic,MOSAIC_10_PER_04,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with Saturn Spin Axis. 2) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Step 77 times using 0.115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 3) Step 77 times about the Z-axis using .115 deg increments for 7200s to +MOS Orb. Stare for 94s during each step increment. 4) Step 77 times about the Z-axis using .115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 5) Step 77 times about the Z-axis using .115 deg increments for 7200s to +MOS Orb. Stare for 94s during each step increment. 6) Step 77 times about the Z-axis using .115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 7) Slew back to Saturn Center. Return to WAYPOINT pointing. Stare for remaining observation time. MOS Orb (+/-range): 77.27mrad.,,,,,, 2004-137T15:00:00,000T00:20:00,16-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-137T15:20:00,000T00:30:00,16-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 001 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [HY-DI-EN-HE-PA (602, 604, 607, 612, 617)]",,,,,, 2004-137T17:05:00,000T09:00:00,16-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-137T17:50:00,000T06:00:00,16-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-138T03:20:00,000T03:57:00,17-May-04,UVIS,Prime,Saturn,MOS10PE,Linear mosaic,MOSAIC_10_PER_05,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Slew about the Z-axis from Saturn Center to +MOS Orb. 3) Step 77 times about the Z-axis using 0.115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 4) Step 38 times about the Z-axis using .115 deg increments for 3600s to Saturn Center. 5) Reset pointing for the WAYPOINT. Stare for remaining observation time. MOS Orb (+/-Range): 77.27mrad.,,,,,, 2004-138T07:17:00,000T00:30:00,17-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-138T07:47:00,000T00:30:00,17-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 002 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [DI-AT-CP-PM-JA (604, 610, 614, 615, 616)]",,,,,, 2004-138T09:32:00,000T09:00:00,17-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-138T10:17:00,000T06:00:00,17-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-138T18:32:00,004T07:15:00,17-May-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-138T19:47:00,000T12:06:00,17-May-04,CIRS,Prime,Saturn,TEMPSIT,Thermal map,CIRS_000SA_TEMPSIT,"Early temperature map of Saturn, starting when Saturn subtends ~5 mrad. With a 2 mrad pointing uncertainty, 3 array positions covers the disk",,,,,, 2004-138T19:47:00,000T12:06:00,17-May-04,ISS,SPASS Rider,Saturn,TEMPSIT,Thermal map,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-138T20:00:00,000T02:17:00,17-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-139T07:53:00,000T07:50:00,18-May-04,UVIS,Prime,Saturn,MOS10PE,Linear mosaic,MOSAIC_10_PER_06,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Slew about the Z-axis from Saturn Center to +MOS Orb. 3) Step 77 times about the Z-axis using .115 deg step increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 4) Step 77 times about the Z-axis for 7200s to +MOS Orb. Stare for 94s during each step increment. 5) Step 77 times about the Z-axis for 7200s to -MOS Orb. Stare for 94s during each step increment. 6) Step 38 times about the Z-axis for 3600s to Saturn Center. Stare for 94s during each step increment. 7) Reset pointing for the WAYPOINT. Stare for remaining observation time. MOS Orb (+/-Range): 77.27mrad.,,,,,, 2004-139T16:58:00,000T09:00:00,18-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-139T18:00:00,000T02:17:00,18-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-140T03:00:00,000T02:17:00,19-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-140T03:13:00,000T11:26:00,19-May-04,UVIS,Prime,Saturn,MOS10PE,Linear mosaic,MOSAIC_10_PER_07,UVIS mosaic. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin axis. 2) Slew about the Z-axis from Saturn Center to +MOS Orb. 3) Step 77 times about the Z-axis using .115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 4) Step 77 times about the Z-axis using .115 deg increments for 7200s to +MOS Orb. Stare for 94s during each step increment. 5) Step 77 times about the Z-axis using .115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 6) Step 77 times about the Z-axis using .115 deg increments for 7200s to +MOS Orb. Stare for 94s during each step increment. 7) Step 77 times about the Z-axis using .115 deg increments for 7200s to -MOS Orb. Stare for 94s during each step increment. 8) Slew back to Saturn Center and reset pointing for WAYPOINT. Stare for remaining observation time. MOS ORB (+/-Range): 77.27mrad.,,,,,, 2004-140T14:39:00,000T00:30:00,19-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-140T15:09:00,000T00:30:00,19-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 003 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EN-JA-PM-PA-EP (602, 610, 611, 616, 617)]",,,,,, 2004-140T16:54:00,000T09:00:00,19-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-141T03:09:00,000T03:57:00,20-May-04,UVIS,Prime,Saturn,MOS11PA,Linear mosaic,MOSAIC_11_PAR_01,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 2) Slew about the Z-axis from Saturn Center to +MOS Orb. 3) Step 28 times about the Z-axis using .114 deg step increments for 7200s to -MOS Orb. Stare for 257s during each step increment. 4) Step 14 times about the Z-axis using .114 deg step increments for 3600s to Saturn Center. Stare for 257s during each step increment. 5) Reset pointing for Saturn Center and stare for remaining observation time. MOS Orb (+/-Range): 27.86mrad,,,,,, 2004-141T07:06:00,000T00:30:00,20-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-141T07:36:00,000T00:30:00,20-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 004 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-TL-EN-PA-EP (602, 611, 613, 615, 617)]",,,,,, 2004-141T09:21:00,000T09:00:00,20-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-141T19:36:00,000T12:00:00,20-May-04,CIRS,Prime,Saturn,TEMPSIT,Thermal map,CIRS_000SA_TEMPSIT,"Early temperature map of Saturn, starting when Saturn subtends ~5 mrad. With a 2 mrad pointing uncertainty, 3 array positions covers the disk",,,,,, 2004-141T19:36:00,000T12:00:00,20-May-04,ISS,SPASS Rider,Saturn,TEMPSIT,Thermal map,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-142T07:36:00,000T07:56:00,21-May-04,UVIS,Prime,Saturn,MOS11PA,Linear mosaic,MOSAIC_11_PAR_02,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. 2) Step 28 times about the Z-axis using .114 deg step increments for 7200s to -MOS Orb. Stare for 257s during each step increment. 3) Step 28 times about the Z-axis using .114 deg step increments for 7200s to +MOS Orb. Stare for 257s during each step increment. 4) Step 28 times about the Z-axis using .114 deg step increments for 7200s to -MOS Orb. Stare for 257s during each step increment. 5) Step 14 times about the Z-axis using .114 deg increments for 3600s to Saturn Center. Stare for 257s during each step increment. 6) Reset pointing for Saturn Center and stare for remaining observation time. MOS Orb (+/-Range): 27.86mrad.,,,,,, 2004-142T16:47:00,000T09:00:00,21-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-142T17:32:00,000T06:00:00,21-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-143T01:47:00,001T16:24:00,22-May-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-143T01:47:00,001T16:24:00,22-May-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-143T03:00:00,000T04:34:00,22-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-143T03:02:00,000T00:30:00,22-May-04,ISS,Prime,Titan,MOVIEOP,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-143T03:02:00,000T00:30:00,22-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,Titan Light Curve,"Titan Light Curve, Observtion #1, ride along with ISS",,,,,, 2004-143T03:32:00,000T01:51:00,22-May-04,UVIS,Prime,Titan,MOS11PAA,Linear mosaic,MOSAIC_11_PAR_03a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 129s during each step increment. 3) Slew back to Titan. Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-143T05:23:00,000T00:30:00,22-May-04,ISS,Prime,Titan,MOVIEPP,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-143T05:23:00,000T00:30:00,22-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #2","Titan Light Curve, Observation #2, ride along with ISS",,,,,, 2004-143T05:53:00,000T02:00:00,22-May-04,UVIS,Prime,Titan,MOS11PAB,Linear mosaic,MOSAIC_11_PAR_03b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-143T07:53:00,000T00:30:00,22-May-04,ISS,Prime,Titan,MOVIEPP,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-143T07:53:00,000T00:30:00,22-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #3","Titan Light Curve, Observation #3, ride along with ISS",,,,,, 2004-143T08:23:00,000T02:00:00,22-May-04,UVIS,Prime,Titan,MOS11PAC,Linear mosaic,MOSAIC_11_PAR_03C,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn +/-Range): 27.86mrad.,,,,,, 2004-143T10:23:00,000T00:30:00,22-May-04,ISS,Prime,Titan,MOVIEPP,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-143T10:23:00,000T00:30:00,22-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #4","Titan Light Curve, Observation #4, ride along with ISS",,,,,, 2004-143T10:53:00,000T02:00:00,22-May-04,UVIS,Prime,Titan,MOS11PAD,Linear mosaic,MOSAIC_11_PAR_03d,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-143T12:00:00,000T04:34:00,22-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-143T12:53:00,000T00:30:00,22-May-04,ISS,Prime,Titan,MOVIEPP,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-143T12:53:00,000T00:30:00,22-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #5","Titan Light Curve, Observation #5, ride along with ISS",,,,,, 2004-143T13:23:00,000T01:05:00,22-May-04,UVIS,Prime,Titan,MOS11PAE,Linear mosaic,MOSAIC_11_PAR_03E,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Stare at WAYPOINT for observation duration.,,,,,, 2004-143T14:28:00,000T00:30:00,22-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-143T14:58:00,000T00:30:00,22-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 005 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-EN-CP-PM-PA (602, 611, 614, 616, 617)]",,,,,, 2004-143T16:43:00,000T09:00:00,22-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-143T17:28:00,000T06:00:00,22-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-144T02:58:00,000T00:30:00,23-May-04,ISS,Prime,Titan,MOVIEQQ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-144T02:58:00,000T00:30:00,23-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #6","Titan Light Curve, Observation #6, ride along with ISS",,,,,, 2004-144T03:00:00,000T04:34:00,23-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-144T03:28:00,000T02:00:00,23-May-04,UVIS,Prime,Titan,MOS11PAA,Linear mosaic,MOSAIC_11_PAR_04A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to -MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to +MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-144T05:28:00,000T00:30:00,23-May-04,ISS,Prime,Titan,MOVIEQQ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-144T05:28:00,000T00:30:00,23-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #7","Titan Light Curve, Observation #7, ride along with ISS",,,,,, 2004-144T05:58:00,000T00:58:00,23-May-04,UVIS,Prime,Titan,MOS11PAB,Linear mosaic,MOSAIC_11_PAR_04b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation.,,,,,, 2004-144T06:56:00,000T00:30:00,23-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-144T07:26:00,000T00:30:00,23-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 006 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [TL-EP-AT-PM-JA (610, 611, 613, 615, 616)]",,,,,, 2004-144T09:11:00,000T09:00:00,23-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-144T09:56:00,000T06:00:00,23-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-144T10:00:00,000T06:51:00,23-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 96 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-144T18:11:00,007T08:18:00,23-May-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-144T18:11:00,005T23:37:00,23-May-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-144T19:26:00,000T12:00:00,23-May-04,CIRS,Prime,Saturn,TEMPSIT,Thermal map,CIRS_000SA_TEMPSIT,"Early temperature map of Saturn, starting when Saturn subtends ~5 mrad. With a 2 mrad pointing uncertainty, 3 array positions covers the disk",,,,,, 2004-144T19:26:00,000T12:00:00,23-May-04,ISS,SPASS Rider,Saturn,TEMPSIT,Thermal map,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-144T20:00:00,000T02:17:00,23-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-145T07:26:00,000T00:30:00,24-May-04,ISS,Prime,Titan,MOVIERR,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 6 images every 10 minutes,,,,,, 2004-145T07:26:00,000T00:30:00,24-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #8","Titan Light Curve, Observation #8, ride along with ISS",,,,,, 2004-145T07:56:00,000T02:00:00,24-May-04,UVIS,Prime,Titan,MOS11PAA,Linear mosaic,MOSAIC_11_PAR_05A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to -MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to +MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-145T09:56:00,000T00:30:00,24-May-04,ISS,Prime,Titan,MOVIERR,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 6 images every 10 minutes,,,,,, 2004-145T09:56:00,000T00:30:00,24-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #9","Titan Light Curve, Observation #9, ride along with ISS",,,,,, 2004-145T10:26:00,000T02:00:00,24-May-04,UVIS,Prime,Titan,MOS11PAB,Linear mosaic,MOSAIC_11_PAR_05b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to -MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to +MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-145T12:26:00,000T00:30:00,24-May-04,ISS,Prime,Titan,MOVIERR,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 6 images every 10 minutes,,,,,, 2004-145T12:26:00,000T00:30:00,24-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #10","Titan Light Curve, Observation #10, ride along with ISS",,,,,, 2004-145T12:56:00,000T02:00:00,24-May-04,UVIS,Prime,Titan,MOS11PAC,Linear mosaic,MOSAIC_11_PAR_05C,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to -MOS Orb. Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s to +MOS Orb. Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 129s during each step increment. 4) Reset pointing and stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-145T14:56:00,000T00:25:00,24-May-04,ISS,Prime,Titan,MOVIERS,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 6 images every 10 minutes,,,,,, 2004-145T14:56:00,000T00:25:00,24-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #11","Titan Light Curve, Observation #11, ride along with ISS",,,,,, 2004-145T16:36:00,000T09:00:00,24-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-145T17:00:00,000T02:17:00,24-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-145T17:21:00,000T06:00:00,24-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL0,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-146T02:51:00,000T00:30:00,25-May-04,ISS,Prime,Titan,MOVIESS,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-146T02:51:00,000T00:30:00,25-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #12","Titan Light Curve, Observation #12, ride along with ISS",,,,,, 2004-146T03:21:00,000T02:00:00,25-May-04,UVIS,Prime,Titan,MOS11PAA,Linear mosaic,MOSAIC_11_PAR_06a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s from Titan to +MOS Orb (increasing DEC angles). Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s toward Titan. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 27.86mrad.,,,,,, 2004-146T05:21:00,000T00:30:00,25-May-04,ISS,Prime,Titan,MOVIESS,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-146T05:21:00,000T00:30:00,25-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #13","Titan Light Curve, Observation #13, ride along with ISS",,,,,, 2004-146T05:51:00,000T02:00:00,25-May-04,UVIS,Prime,Titan,MOS11PAB,Linear mosaic,MOSAIC_11_PAR_06b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s from Titan to +MOS Orb (increasing DEC angles). Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114deg increments for 1800s toward Titan. Stare for 129s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 27.86mrad.,,,,,, 2004-146T07:51:00,000T00:30:00,25-May-04,ISS,Prime,Titan,MOVIESS,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-146T07:51:00,000T00:30:00,25-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #14","Titan Light Curve, Observation #14, ride along with ISS",,,,,, 2004-146T08:21:00,000T02:00:00,25-May-04,UVIS,Prime,Titan,MOS11PAC,Linear mosaic,MOSAIC_11_PAR_06c,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s from Titan to +MOS Orb (increasing DEC angles). Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s toward Titan 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 27.86mrad.,,,,,, 2004-146T10:21:00,000T00:30:00,25-May-04,ISS,Prime,Titan,MOVIESS,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-146T10:21:00,000T00:30:00,25-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #15","Titan Light Curve, Observation #15, ride along with ISS",,,,,, 2004-146T10:51:00,000T02:00:00,25-May-04,UVIS,Prime,Titan,MOS11PAD,Linear mosaic,MOSAIC_11_PAR_06D,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s from Titan to +MOS Orb (increasing DEC angles). Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 129s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 27.86mrad.,,,,,, 2004-146T12:51:00,000T00:30:00,25-May-04,ISS,Prime,Titan,MOVIESS,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-146T12:51:00,000T00:30:00,25-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #16","Titan Light Curve, Observation #16, ride along with ISS",,,,,, 2004-146T13:21:00,000T00:57:00,25-May-04,UVIS,Prime,Titan,MOS11PAE,Linear mosaic,MOSAIC_11_PAR_06E,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation,,,,,, 2004-146T14:18:00,000T00:30:00,25-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-146T14:48:00,000T00:30:00,25-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 007 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-DI-PM-EN-JA (602, 604, 610, 616, 617)]",,,,,, 2004-146T16:33:00,000T09:00:00,25-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-147T02:48:00,000T00:30:00,26-May-04,ISS,Prime,Titan,MOVIETT,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-147T02:48:00,000T00:30:00,26-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #17","Titan Light Curve, Observation #17, ride along with ISS",,,,,, 2004-147T03:18:00,000T02:00:00,26-May-04,UVIS,Prime,Titan,MOS11PAA,Linear mosaic,MOSAIC_11_PAR_07A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator. 2) Step 28 times about the Z-axis using 0.114 deg increments for 3600s from Titan to +MOS Orb (increasing DEC angles). Stare for 129s during each step increment. 3) Step 14 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 129s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 27.86mrad.,,,,,, 2004-147T05:18:00,000T00:30:00,26-May-04,ISS,Prime,Titan,MOVIETT,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-147T05:18:00,000T00:30:00,26-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #18","Titan Light Curve, Observation #18, ride along with ISS",,,,,, 2004-147T05:48:00,000T00:57:00,26-May-04,UVIS,Prime,Titan,MOS11PAB,Linear mosaic,MOSAIC_11_PAR_07b,"Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, parallel to the orbital plane. 1) Slew from Titan to START RA/DEC: 36.89/11.32 deg. 2) Step 28 times using 0.114 deg increments. Step in the direction of decreasing declination angles in the XY plane. Stare during each step increment. Total mosaic time 2700 seconds. 3) Slew back to Titan and reset pointing. Stare for remaining observation time.",,,,,, 2004-147T06:45:00,000T00:30:00,26-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-147T07:15:00,000T00:30:00,26-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 008 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-HY-DI-MI-HE (601, 604, 607, 612, 615)]",,,,,, 2004-147T09:00:00,000T09:00:00,26-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-147T19:15:00,000T12:00:00,26-May-04,ISS,Prime,rings(general),SATSRCHBP,Ansa movie,"ANSA MOVIE FOR SATELLITE SEARCHES, PRE PHOEBE IN R","ANSA MOVIE FOR SEARCHING FOR SATELLITES IN RING GAPS ON APPROACH. ONE NAC, ALTERNATE ANSAE, EVERY 12 MINUTES.",,,,,, 2004-148T07:15:00,000T00:30:00,27-May-04,ISS,Prime,Titan,MOVIEUU,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-148T07:15:00,000T00:30:00,27-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #19","Titan Light Curve, Observation #19, ride along with ISS",,,,,, 2004-148T07:45:00,000T02:00:00,27-May-04,UVIS,Prime,Titan,MOS11PEA,Linear mosaic,MOSAIC_11_PER_01A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 96 times about the Z-axis using 0.119 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 37.5s during each step increment. 3) Step 48 times about the Z-axis using .119 deg increments for 1800s toward Titan. Stare for 37.5s during each step increment. 3) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/-Range): 99.69mrad.,,,,,, 2004-148T09:45:00,000T00:30:00,27-May-04,ISS,Prime,Titan,MOVIEUU,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-148T09:45:00,000T00:30:00,27-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #20","Titan Light Curve, Observation #20, ride along with ISS",,,,,, 2004-148T10:15:00,000T02:00:00,27-May-04,UVIS,Prime,Titan,MOS11PEB,Linear mosaic,MOSAIC_11_PER_01b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 96 times about the Z-axis using 0.119 deg increments for 3600s from Titan to -MOS ORB. Stare for 37.5s during each step increment. 3) Step 48 times about the Z-axis using .119 deg increments for 1800s toward Titan. Stare for 37.5s during each step increment. 3) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/-Range): 99.69mrad.,,,,,, 2004-148T12:15:00,000T00:30:00,27-May-04,ISS,Prime,Titan,MOVIEUU,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-148T12:15:00,000T00:30:00,27-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #21","Titan Light Curve, Observation #21, ride along with ISS",,,,,, 2004-148T12:45:00,000T02:00:00,27-May-04,UVIS,Prime,Titan,MOS11PEC,Linear mosaic,MOSAIC_11_PER_01c,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 96 times about the Z-axis using 0.119 deg increments for 3600s from Titan to -MOS ORB. Stare for 37.5s during each step increment. 3) Step 48 times about the Z-axis using .119deg increments for 1800s toward Titan. Stare for 37.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 99.69mrad.,,,,,, 2004-148T14:45:00,000T00:26:00,27-May-04,ISS,Prime,Titan,MOVIEUV,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-148T14:45:00,000T00:26:00,27-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #22","Titan Light Curve, Observation #22, ride along with ISS",,,,,, 2004-148T16:26:00,000T10:47:00,27-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-149T03:13:00,000T03:40:00,28-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-149T11:41:00,000T00:30:00,28-May-04,ISS,Prime,Titan,MOVIEVV,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-149T12:11:00,000T01:55:00,28-May-04,UVIS,Prime,Titan,MOS11PEE,Linear mosaic,MOSAIC_11_PER_02e,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation,,,,,, 2004-149T14:06:00,000T00:30:00,28-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-149T14:36:00,000T00:30:00,28-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 009 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-HY-HE-CP-PA (607, 610, 612, 614, 617)]",,,,,, 2004-149T16:21:00,000T09:00:00,28-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-150T00:00:00,013T04:02:00,29-May-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-150T02:00:00,013T02:02:00,29-May-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-150T02:36:00,000T00:30:00,29-May-04,ISS,Prime,Titan,MOVIEWW,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-150T02:36:00,000T00:30:00,29-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #28","Titan Light Curve, Observation #28, ride along with ISS",,,,,, 2004-150T03:06:00,000T02:00:00,29-May-04,UVIS,Prime,Titan,MOS11PEA,Linear mosaic,MOSAIC_11_PER_03A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 96 times about the Z-axis using 0.119 deg increments for 3600s from Titan (decreasing RA angles) to -MOS Orb. Stare for 37.5s during each step increment. 3) Step 48 times about the Z-axis using .119 deg increments for 1800s toward Titan. Stare for 37.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 99.69mrad,,,,,, 2004-150T05:06:00,000T00:30:00,29-May-04,ISS,Prime,Titan,MOVIEWW,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-150T05:06:00,000T00:30:00,29-May-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #29","Titan Light Curve, Observation #29, ride along with ISS",,,,,, 2004-150T05:36:00,000T00:57:00,29-May-04,UVIS,Prime,Titan,MOS11PEB,Linear mosaic,MOSAIC_11_PER_03b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation,,,,,, 2004-150T06:33:00,000T00:30:00,29-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-150T07:03:00,000T00:30:00,29-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 010 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-EN-TL-JA-PM (602, 610, 613, 615, 616)]",,,,,, 2004-150T07:33:00,000T00:23:00,29-May-04,UVIS,Non-SPASS,SpacecraftActivity,PIM,Periodic Instrument maintenance,UVIS PIM in S01,"This is an engineering activity. Start time should be around doy 150, but can be moved by several days (30) if needed. Any orientation is Ok. Does not require SSR allocation.",,,,,, 2004-150T08:48:00,000T09:00:00,29-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-150T17:48:00,001T08:41:00,29-May-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-150T19:03:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T19:33:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T20:03:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T20:33:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T21:03:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T21:33:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T22:03:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T22:33:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T23:03:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-150T23:33:00,000T00:30:00,29-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T00:03:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T00:33:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T01:03:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T01:33:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T02:03:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T02:33:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T03:03:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T03:33:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T04:03:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T04:33:00,000T00:30:00,30-May-04,ISS,Prime,Saturn,2X1CH4NAC,Photometry,Saturn Methane imaging,Methane Band Photometry,,,,,, 2004-151T05:03:00,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T05:32:48,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T06:02:36,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T06:32:24,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T07:02:12,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T07:32:00,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T08:01:48,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T08:31:36,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T09:01:24,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T09:31:12,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T10:01:00,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T10:30:48,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T11:00:36,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T11:30:24,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T12:00:12,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T12:30:00,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T12:59:48,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T13:29:36,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T13:59:24,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T14:29:12,000T00:29:48,30-May-04,ISS,Prime,Saturn,2X1PLRNCC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color,,,,,, 2004-151T16:14:00,000T09:00:00,30-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-151T17:00:00,000T02:17:00,30-May-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-152T02:29:00,000T11:27:00,31-May-04,RPWS,Prime,Saturn,ANTCAL,Antenna calibration,RPWS Post-Probe Release Antenna Cal.,"Repeat of portion of Jupiter RPWS antenna calibration. Require two eleven hour periods during the approach phase. Attitude, rotate about offset axis of spacecraft in such a way that the RPWS antenna directions sweep through Saturn once per turn.",,,,,, 2004-152T02:29:00,000T11:27:00,31-May-04,MAG,Non-SPASS,Saturn,ANTCAL,Antenna calibration,Offset Calibration using RPWS rolls,Use RPWS rolls to perform an offset calibration of the MAG sensors,,,,,, 2004-152T13:56:00,000T00:30:00,31-May-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-152T13:56:00,001T12:22:00,31-May-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-152T13:56:00,001T12:22:00,31-May-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-152T14:26:00,000T00:30:00,31-May-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 011 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EN-AT-EP-DI (602, 604, 611, 615, 617)]",,,,,, 2004-152T16:11:00,000T09:00:00,31-May-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-152T16:56:00,000T06:00:00,31-May-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-153T02:26:00,000T10:37:00,1-Jun-04,ISS,Prime,rings(general),SATSRCHBP,Ansa movie,"ANSA MOVIE FOR SATELLITE SEARCHES, PRE PHOEBE IN R",ANSA MOVIE FOR SEARCHING FOR SATELLITES IN RING GAPS ON APPROACH(PRE PHOEBE ENCOUNTER),,,,,, 2004-153T14:18:00,000T12:00:00,1-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-154T02:18:00,002T16:24:00,2-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-154T02:18:00,002T15:09:00,2-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-154T02:18:00,000T01:00:00,2-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-154T04:00:00,000T02:17:00,2-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-154T04:33:00,000T00:30:00,2-Jun-04,ISS,Prime,Titan,MOVIEZZ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-154T04:33:00,000T00:30:00,2-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #30","Titan Light Curve, Observation #30, ride along with ISS",,,,,, 2004-154T05:03:00,000T02:00:00,2-Jun-04,CIRS,Prime,Saturn,MIRCMPSTA,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITA,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-154T07:03:00,000T00:30:00,2-Jun-04,ISS,Prime,Titan,MOVIEZZ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-154T07:03:00,000T00:30:00,2-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #31","Titan Light Curve, Observation #31, ride along with ISS",,,,,, 2004-154T07:33:00,000T02:00:00,2-Jun-04,CIRS,Prime,Saturn,MIRCMPSTB,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITA,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-154T09:33:00,000T00:30:00,2-Jun-04,ISS,Prime,Titan,MOVIEZZ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-154T09:33:00,000T00:30:00,2-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #32","Titan Light Curve, Observation #32, ride along with ISS",,,,,, 2004-154T10:03:00,000T02:00:00,2-Jun-04,CIRS,Prime,Saturn,MIRCMPSTC,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITC,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-154T12:03:00,000T00:30:00,2-Jun-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-154T12:33:00,000T00:30:00,2-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 012 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EP-DI-PM-JA (604, 610, 611, 616, 617)]",,,,,, 2004-154T14:18:00,000T13:00:00,2-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-154T15:00:00,000T02:17:00,2-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-155T04:00:00,000T02:17:00,3-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-155T04:33:00,000T01:56:00,3-Jun-04,UVIS,Prime,Titan,MOS12PAA,Linear mosaic,MOSAIC_12_PAR_01A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing DEC angles). Stare for 88s during each step increment. 3) Step 20 times about the Z-axis using .114 deg increments for 1800s towards Titan. Stare for 88s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/-Range): 40.79mrad,,,,,, 2004-155T06:29:00,000T00:30:00,3-Jun-04,ISS,Prime,Titan,MOVIEAAA,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-155T06:29:00,000T00:30:00,3-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #33","Titan Light Curve, Observation #33, ride along with ISS",,,,,, 2004-155T06:59:00,000T02:00:00,3-Jun-04,UVIS,Prime,Titan,MOS12PAB,Linear mosaic,MOSAIC_12_PAR_01b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing DEC angles). Stare for 88s during each step increment. 3) Step 20 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 88s during each step increment. 3) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 40.79mrad,,,,,, 2004-155T08:59:00,000T00:30:00,3-Jun-04,ISS,Prime,Titan,MOVIEAAA,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-155T08:59:00,000T00:30:00,3-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #34","Titan Light Curve, Observation #34, ride along with ISS",,,,,, 2004-155T09:29:00,000T02:00:00,3-Jun-04,UVIS,Prime,Titan,MOS12PAC,Linear mosaic,MOSAIC_12_PAR_01C,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing DEC angles). Stare for 88s during each step increment. 3) Step 20 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 88s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 40.79mrad,,,,,, 2004-155T11:29:00,000T00:30:00,3-Jun-04,ISS,Prime,Titan,MOVIEAAA,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-155T11:29:00,000T00:30:00,3-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #35","Titan Light Curve, Observation #35, ride along with ISS",,,,,, 2004-155T11:59:00,000T01:46:00,3-Jun-04,UVIS,Prime,Titan,MOS12PAD,Linear mosaic,MOSAIC_12_PAR_01d,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing DEC angles). Stare for 88s during each step increment. 3) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 40.79mrad,,,,,, 2004-155T13:45:00,000T00:30:00,3-Jun-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-155T14:15:00,000T00:30:00,3-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 013 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EP-EN-AT-PM (602, 611, 615, 616, 617)]",,,,,, 2004-155T16:00:00,000T09:00:00,3-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-155T16:45:00,000T06:00:00,3-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-155T17:00:00,000T04:34:00,3-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-156T02:00:00,000T04:34:00,4-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-156T02:15:00,000T00:30:00,4-Jun-04,ISS,Prime,Titan,MOVIEBBB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-156T02:15:00,000T00:30:00,4-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #36","Titan Light Curve, Observation #36, ride along with ISS",,,,,, 2004-156T02:45:00,000T02:00:00,4-Jun-04,CIRS,Prime,Saturn,MIRCMPSTA,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITA,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-156T04:45:00,000T00:30:00,4-Jun-04,ISS,Prime,Titan,MOVIEBBB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-156T04:45:00,000T00:30:00,4-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #37","Titan Light Curve, Observation #37, ride along with ISS",,,,,, 2004-156T05:15:00,000T01:00:00,4-Jun-04,CIRS,Prime,Saturn,MIRCMPSTB,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITB,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-156T06:15:00,000T00:27:00,4-Jun-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-156T06:42:00,000T00:30:00,4-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 014 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [DI-HE-JA-CP-TL (604, 610, 612, 613, 614)]",,,,,, 2004-156T08:27:00,000T09:00:00,4-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-156T09:00:00,000T04:34:00,4-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-156T09:12:00,000T06:00:00,4-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-156T17:27:00,000T01:15:00,4-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-156T18:00:00,000T02:17:00,4-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-156T18:42:00,000T11:30:00,4-Jun-04,RPWS,Prime,Saturn,ANTCAL,Antenna calibration,RPWS Post-Probe Release Antenna Cal.,"Repeat of portion of Jupiter RPWS antenna calibration. Require two eleven hour periods during approach. Attitude, rotate about x-axis of spacecraft in such a way that the RPWS antenna directions sweep through Saturn once per turn.",,,,,, 2004-156T18:42:00,000T11:30:00,4-Jun-04,MAG,Non-SPASS,Saturn,ANTCAL,Antenna calibration,Offset Calibration using RPWS rolls,Use RPWS rolls to perform an offset calibration of the MAG sensors,,,,,, 2004-157T06:12:00,000T00:30:00,5-Jun-04,ISS,Prime,Titan,MOVIECCC,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-157T06:12:00,000T00:30:00,5-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #38","Titan Light Curve, Observation #38, ride along with ISS",,,,,, 2004-157T06:12:00,004T09:26:00,5-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-157T06:12:00,002T11:05:00,5-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-157T06:42:00,000T02:00:00,5-Jun-04,CIRS,Prime,Saturn,FIRCMPSTA,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-157T08:42:00,000T00:30:00,5-Jun-04,ISS,Prime,Titan,MOVIECCC,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-157T08:42:00,000T00:30:00,5-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #39","Titan Light Curve, Observation #39, ride along with ISS",,,,,, 2004-157T09:12:00,000T02:00:00,5-Jun-04,CIRS,Prime,Saturn,FIRCMPSTB,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-157T11:12:00,000T00:30:00,5-Jun-04,ISS,Prime,Titan,MOVIECCC,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-157T11:12:00,000T00:30:00,5-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #40","Titan Light Curve, Observation #40, ride along with ISS",,,,,, 2004-157T11:42:00,000T02:26:00,5-Jun-04,CIRS,Prime,Saturn,FIRCMPSTC,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-157T14:08:00,000T00:30:00,5-Jun-04,ISS,Prime,Titan,MOVIECCD,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-157T14:08:00,000T00:30:00,5-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #41","Titan Light Curve, Observation #41, ride along with ISS",,,,,, 2004-157T15:53:00,000T09:00:00,5-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-157T16:38:00,000T06:00:00,5-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-157T17:00:00,000T02:17:00,5-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-158T02:00:00,000T02:17:00,6-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-158T02:08:00,000T00:40:00,6-Jun-04,ISS,Prime,Titan,MOVIECDD,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-158T02:08:00,000T00:40:00,6-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #42","Titan Light Curve, Observation #42, ride along with ISS",,,,,, 2004-158T02:48:00,000T02:00:00,6-Jun-04,CIRS,Prime,Saturn,MIRCMPSTA,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITA,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-158T04:48:00,000T00:30:00,6-Jun-04,ISS,Prime,Titan,MOVIEDDD,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-158T04:48:00,000T00:30:00,6-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #43","Titan Light Curve, Observation #43, ride along with ISS",,,,,, 2004-158T05:18:00,000T02:00:00,6-Jun-04,CIRS,Prime,Saturn,MIRCMPSTB,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITB,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-158T07:18:00,000T00:30:00,6-Jun-04,ISS,Prime,Titan,MOVIEDDD,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-158T07:18:00,000T00:30:00,6-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #44","Titan Light Curve, Observation #44, ride along with ISS",,,,,, 2004-158T07:48:00,000T02:00:00,6-Jun-04,CIRS,Prime,Saturn,MIRCMPSTC,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITC,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-158T09:48:00,000T00:30:00,6-Jun-04,ISS,Prime,Titan,MOVIEDDD,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-158T09:48:00,000T00:30:00,6-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #45","Titan Light Curve, Observation #45, ride along with ISS",,,,,, 2004-158T10:18:00,000T02:47:00,6-Jun-04,CIRS,Prime,Saturn,MIRCMPSTD,Sit and stare to derive composition,CIRS_000SA_MIRCMPSITD,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-158T11:50:00,000T08:00:00,6-Jun-04,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS PIM (Ka-TWTA Maintenance),RSS PIM. Pointing=Not Applicable. DSN Tracking=None.,,,,,, 2004-158T13:05:00,000T00:30:00,6-Jun-04,ISS,Prime,Titan,MOVIEDDE,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-158T13:05:00,000T00:30:00,6-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #46","Titan Light Curve, Observation #46, ride along with ISS Changed start time to match TOL 4/8/03, DPC",,,,,, 2004-158T13:35:00,000T00:30:00,6-Jun-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-158T14:05:00,000T00:30:00,6-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 015 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-PM-AT-JA-PA (610, 611, 615, 616, 617)]",,,,,, 2004-158T15:50:00,000T09:00:00,6-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-158T16:35:00,000T03:00:00,6-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-158T17:00:00,000T02:17:00,6-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-159T02:00:00,000T02:17:00,7-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-159T02:05:00,000T00:30:00,7-Jun-04,ISS,Prime,Titan,MOVIEEEE,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-159T02:05:00,000T00:30:00,7-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #47","Titan Light Curve, Observation #47, ride along with ISS",,,,,, 2004-159T02:35:00,000T02:00:00,7-Jun-04,UVIS,Prime,Titan,MOS12PAA,Linear mosaic,MOSAIC_12_PAR_05a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 88s during each step increment. 3) Step 20 times about the Z-axis using .114 deg increments for 1800s to Titan. Stare for 88s during each step increment. 4)Reset pointing and stare for remaining observation time. MOS Orb (Saturn +/- Range): 40.79mrad,,,,,, 2004-159T04:35:00,000T00:30:00,7-Jun-04,ISS,Prime,Titan,MOVIEEEE,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-159T04:35:00,000T00:30:00,7-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #48","Titan Light Curve, Observation #48, ride along with ISS",,,,,, 2004-159T05:05:00,000T00:57:00,7-Jun-04,UVIS,Prime,Titan,MOS12PAB,Linear mosaic,MOSAIC_12_PAR_05b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for observation duration,,,,,, 2004-159T06:02:00,000T00:30:00,7-Jun-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-159T06:32:00,000T00:30:00,7-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 016 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-EN-DI-HY-HE (602, 604, 607, 612, 614)]",,,,,, 2004-159T08:17:00,000T09:00:00,7-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-159T09:00:00,000T02:17:00,7-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-159T09:02:00,000T03:00:00,7-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-159T17:17:00,001T22:21:00,7-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-159T18:00:00,000T02:17:00,7-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-159T18:32:00,000T00:30:00,7-Jun-04,ISS,Prime,Titan,MOVIEEEB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-159T18:32:00,000T00:30:00,7-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #49","Titan Light Curve, Observation #49, ride along with ISS",,,,,, 2004-159T19:02:00,000T02:00:00,7-Jun-04,UVIS,Prime,Titan,MOS12PAA,Linear mosaic,MOSAIC_12_PAR_06A,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 88s during each step increment. 3) Step 20 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 88s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 40.79mrad,,,,,, 2004-159T21:02:00,000T00:30:00,7-Jun-04,ISS,Prime,Titan,MOVIEEEB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-159T21:02:00,000T00:30:00,7-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #50","Titan Light Curve, Observation #50, ride along with ISS",,,,,, 2004-159T21:32:00,000T02:00:00,7-Jun-04,UVIS,Prime,Titan,MOS12PAB,Linear mosaic,MOSAIC_12_PAR_06b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 88s during each step increment. 3) Step 20 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 88s during each step increment. 3) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 40.79mrad,,,,,, 2004-159T23:32:00,000T00:30:00,7-Jun-04,ISS,Prime,Titan,MOVIEEEB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-159T23:32:00,000T00:30:00,7-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #51","Titan Light Curve, Observation #51, ride along with ISS",,,,,, 2004-160T00:02:00,000T02:56:00,8-Jun-04,UVIS,Prime,Titan,MOS12PAC,Linear mosaic,MOSAIC_12_PAR_06C,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Slew about the Z-axis from Titan to +MOS Orb. Align slit parallel with the Saturn Equator 2) Step 41 times about the Z-axis using 0.114 deg increments for 3600s to -MOS Orb. Stare for 88s during each step increment. 3) Step 21 times about the Z-axis for 1800s to Titan. 4) Reset pointing for waypoint. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 40.79mrad,,,,,, 2004-160T02:58:00,000T00:30:00,8-Jun-04,ISS,Prime,Titan,MOVIEFFF,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-160T02:58:00,000T00:30:00,8-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #52","Titan Light Curve, Observation #52, ride along with ISS",,,,,, 2004-160T03:28:00,000T02:00:00,8-Jun-04,CIRS,Prime,Saturn,MIRCMPSTA,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-160T05:28:00,000T00:30:00,8-Jun-04,ISS,Prime,Titan,MOVIEFFF,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-160T05:28:00,000T00:30:00,8-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #53","Titan Light Curve, Observation #53, ride along with ISS",,,,,, 2004-160T05:58:00,000T02:00:00,8-Jun-04,CIRS,Prime,Saturn,MIRCMPSTB,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-160T07:58:00,000T00:30:00,8-Jun-04,ISS,Prime,Titan,MOVIEFFF,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-160T07:58:00,000T00:30:00,8-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #54","Titan Light Curve, Observation #54, ride along with ISS",,,,,, 2004-160T08:28:00,000T02:00:00,8-Jun-04,CIRS,Prime,Saturn,MIRCMPSTC,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-160T10:28:00,000T00:30:00,8-Jun-04,ISS,Prime,Titan,MOVIEFFF,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-160T10:28:00,000T00:30:00,8-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #55","Titan Light Curve, Observation #55, ride along with ISS",,,,,, 2004-160T10:58:00,000T02:00:00,8-Jun-04,CIRS,Prime,Saturn,MIRCMPSTD,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-160T12:58:00,000T00:30:00,8-Jun-04,ISS,Prime,Titan,MOVIEFFF,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-160T12:58:00,000T00:30:00,8-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #56","Titan Light Curve, Observation #56, ride along with ISS",,,,,, 2004-160T13:28:00,000T01:00:00,8-Jun-04,CIRS,Prime,Saturn,MIRCMPSTE,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-160T15:43:00,000T09:00:00,8-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-160T16:28:00,000T06:00:00,8-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-160T17:00:00,000T04:34:00,8-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-161T01:58:00,000T00:30:00,9-Jun-04,ISS,Prime,Titan,MOVIEGGG,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-161T01:58:00,000T00:30:00,9-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #57","Titan Light Curve, Observation #57, ride along with ISS",,,,,, 2004-161T02:00:00,000T04:34:00,9-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-161T02:28:00,000T02:00:00,9-Jun-04,CIRS,Prime,Saturn,FIRCMPSTA,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-161T04:28:00,000T00:30:00,9-Jun-04,ISS,Prime,Titan,MOVIEGGG,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-161T04:28:00,000T00:30:00,9-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #58","Titan Light Curve, Observation #58, ride along with ISS",,,,,, 2004-161T04:58:00,000T02:00:00,9-Jun-04,CIRS,Prime,Saturn,FIRCMPSTB,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-161T06:58:00,000T00:30:00,9-Jun-04,ISS,Prime,Titan,MOVIEGGG,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-161T06:58:00,000T00:30:00,9-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #59","Titan Light Curve, Observation #59, ride along with ISS",,,,,, 2004-161T07:28:00,000T02:00:00,9-Jun-04,CIRS,Prime,Saturn,FIRCMPSTC,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-161T09:28:00,000T00:30:00,9-Jun-04,ISS,Prime,Titan,MOVIEGGG,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-161T09:28:00,000T00:30:00,9-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #60 (DPC)","Titan Light Curve, Observation #60 (DPC), ride along with ISS",,,,,, 2004-161T09:58:00,000T02:55:00,9-Jun-04,CIRS,Prime,Saturn,FIRCMPSTD,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-161T12:53:00,000T00:30:00,9-Jun-04,ISS,Prime,Titan,MOVIEGGH,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-161T12:53:00,000T00:30:00,9-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #61 (DPC)","Titan Light Curve, Observation #61 (DPC), ride along with ISS",,,,,, 2004-161T13:23:00,000T00:30:00,9-Jun-04,ISS,Prime,Other,RETARGETS,Retargetable observation,RETARGETABLES FOR SATELLITES DISCOVERED ON APPROAC,RETARGETABLES FOR SATELLITES DISCOVERED DURING APPROACH(START 0 TO PHOEBE ENCOUNTER),,,,,, 2004-161T13:53:00,000T00:30:00,9-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 017 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [TL-EN-JA-PM-AT (602, 610, 613, 615, 616)]",,,,,, 2004-161T15:38:00,001T12:24:00,9-Jun-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust exploration,"for prograde dust (Saturn cent.): -z2E, -x 21;-18.6 AM=52",,,,,, 2004-161T15:38:00,001T12:24:00,9-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps). End was tied to Phoebe-2hrs = 163T17:33:37. Removed epoch for SOPU/SSUP.,,,,,, 2004-161T15:38:00,001T12:24:00,9-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-161T15:38:00,000T09:00:00,9-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-161T16:23:00,000T03:00:00,9-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-162T01:53:00,000T11:44:00,10-Jun-04,ISS,Prime,Phoebe,FULROTIN,,Phoebe pre-encounter global mapping,"Turn -Y to Phoebe; shift back-and-forth between CIRS FP3, FP1, and UVIS FUV about every hour (about 20 min dwell for each position) (total of 34 positions). Do clr and color filter during FP3, clr filter observations during FUV pointings. Turn back to WP.",,,,,, 2004-162T01:53:00,000T11:44:00,10-Jun-04,CIRS,SPASS Rider,Phoebe,FULROTIN,,,"CIRS rider on ISS distant full rotation observation (AD typ 0.2 mrad). CIRS: center detectors, coadd, FP1 and FP3 only, 38 RTI, shutter closed occasionally during periods where FP1 is on Phoebe, to calibrate FP3. Lego table #790. Timings (UT) are: --------------------- > The detailed timeline for pointing is (absolute SCET): > > 01:53 UTC: Request start, turn to CIRS FP3 > 02:00 UTC (approx.): CIRS FP3 (only 11m instead of 20m) > 02:11 UTC: CIRS FP1 - shutter closed > 02:31 UTC: UVIS FUV > 02:53 UTC: CIRS FP3 > 03:13 UTC: CIRS FP1 > 03:33 UTC: UVIS FUV > 03:55 UTC: CIRS FP3 (includes first ISS) > 04:15 UTC: CIRS FP1 > 04:35 UTC: UVIS FUV > 04:57 UTC: CIRS FP3 > 05:17 UTC: CIRS FP1 - shutter closed > 05:37 UTC: UVIS FUV > 05:59 UTC: CIRS FP3 > 06:19 UTC: CIRS FP1 > 06:39 UTC: UVIS FUV > 07:01 UTC: CIRS FP3 > 07:21 UTC: CIRS FP1 > 07:41 UTC: UVIS FUV > 08:03 UTC: CIRS FP3 > 08:23 UTC: CIRS FP1 - shutter closed > 08:43 UTC: UVIS FUV > 09:05 UTC: CIRS FP3 > 09:25 UTC: CIRS FP1 > 09:45 UTC: UVIS FUV > 10:07 UTC: CIRS FP3 > 10:27 UTC: CIRS FP1 > 10:47 UTC: UVIS FUV > 11:09 UTC: CIRS FP3 > 11:29 UTC: CIRS FP1 - shutter closed > 11:49 UTC: UVIS FUV > 12:11 UTC: CIRS FP3 > 12:31 UTC: CIRS FP1 > 13:51 UTC: UVIS FUV > 13:13 UTC: CIRS FP3 (only ~17m instead of 20m) > 13:30 UTC (approx.): turn to WP > 13:37 UTC: Request end > --------------------",,,,,, 2004-162T01:53:00,000T11:44:00,10-Jun-04,UVIS,SPASS Rider,Phoebe,FULROTIN,,ICYLON full Phoebe rotation,RIDER TO ISS REQUEST,,,,,, 2004-162T01:53:00,000T11:44:00,10-Jun-04,VIMS,SPASS Rider,Phoebe,FULROTIN,,Phoebe,Multiple VIMS cubes over one complete Phoebe rotation,,,,,, 2004-162T13:37:00,000T00:30:00,10-Jun-04,ISS,Prime,Titan,APPROACH,Aproach imaging,Titan Approach Imaging,"Point to Titan, run through sequence of filters most likely to be of use, determine which are best.",,,,,, 2004-162T13:37:00,000T00:30:00,10-Jun-04,CIRS,SPASS Rider,Titan,APPROACH,Aproach imaging,,Titan observation,,,,,, 2004-162T13:37:00,000T00:30:00,10-Jun-04,VIMS,SPASS Rider,Titan,LIGHTC,Titan light curve,Lightcurve (DPC),"Titan Light Curve, Observation #62 (DPC), ride along with ISS Added 4/8/03, DPC",,,,,, 2004-162T15:22:00,000T11:00:00,10-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-162T16:07:00,000T03:00:00,10-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-163T02:22:00,000T01:40:00,11-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-163T04:02:00,000T15:01:37,11-Jun-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-163T04:02:00,000T15:16:37,11-Jun-04,CDA,Non-SPASS,Phoebe,SURVEY,Magnetospheric survey,Phoebe dust survey,dust survey data rate = 100 bps power = 12 W,,,,,, 2004-163T04:02:00,000T14:31:37,11-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,INMS Ops. Test,Ride with prime instrument,,,,,, 2004-163T04:02:00,000T13:31:37,11-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps). End was tied to Phoebe-2hrs = 163T17:33:37. Removed epoch for SOPU/SSUP.,,,,,, 2004-163T04:02:00,000T14:21:03,11-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-163T04:02:00,000T15:04:37,11-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-163T04:40:00,000T00:43:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,Group #2 CIRS PRIME requests,"AD=0.68 mrad; phase=87; LT=6.5; (-22, 87); duration 00:43. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T04:40:00,000T08:38:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T05:23:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES0,Low resolution imaging,Phoebe Approach Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 6 NAC color, 3 NAC polarizer filters)",,,,,, 2004-163T05:23:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES0,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, shutter closed. Calibration only: ca. 5 min. 38 RTI, 10 min 96 RTI.",,,,,, 2004-163T05:39:00,000T02:52:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.72 mrad; phase=87; LT=6.5; (-22, 126); duration 02:52. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T08:31:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1A,Low resolution imaging,Phoebe Approach Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-163T08:31:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1A,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-163T08:47:00,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.93 mrad; phase=87; LT=6.5; (-22, 247); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T08:47:00,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 12x12, 640ms, 160 ms, 10 of each cube",,,,,, 2004-163T09:18:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1B,Low resolution imaging,Phoebe Approach Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-163T09:18:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1B,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-163T09:18:00,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 12x12, 320ms",,,,,, 2004-163T09:34:00,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.01 mrad; phase=87; LT=6.5; (-22, 277); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T09:34:00,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 12x12, 640ms, 160 ms, 10 of each cube",,,,,, 2004-163T10:05:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1C,Low resolution imaging,Phoebe Approach Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-163T10:05:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1C,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-163T10:05:00,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 12x12, 320ms",,,,,, 2004-163T10:21:00,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.09 mrad; phase=87; LT=6.5; (-22, 308); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T10:21:00,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 24x12, 640ms, 160 ms, 6 cubes of each",,,,,, 2004-163T10:52:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1D,Low resolution imaging,Phoebe Approach Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-163T10:52:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1D,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-163T10:52:00,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 12x12, 320ms",,,,,, 2004-163T11:03:37,000T03:00:00,11-Jun-04,RADAR,SPASS Rider,Phoebe,WARMDAT,RADAR warmup,"Warmup, with bits",Warmup the instrument in an opmode that allows RADAR operation as well as collects RADAR data.,,,,,, 2004-163T11:03:37,000T04:31:00,11-Jun-04,RADAR,Non-SPASS,Phoebe,REUBITS,Data volume adjustment,REU bits request,REU bits,,,,,, 2004-163T11:08:00,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.19 mrad; phase=87; LT=6.5; (-22, 338); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T11:08:00,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 24x12, 160ms and 640ms 6 cubes of each",,,,,, 2004-163T11:39:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1E,Low resolution imaging,Phoebe Approach Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-163T11:39:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1E,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-163T11:39:00,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low-res and ir hi-res, 12x12, 320ms",,,,,, 2004-163T11:55:00,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.32 mrad; phase=87; LT=6.5; (-22, 8); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T11:55:00,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 24x12, 160ms and 640ms 6 cubes of each",,,,,, 2004-163T12:26:00,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1F,Low resolution imaging,Phoebe Approach Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-163T12:26:00,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1F,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, shutter closed. Calibration only: ca. 5 min. 38 RTI, 10 min 96 RTI.",,,,,, 2004-163T12:26:00,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low-res and ir hi-res, 12x12, 320ms",,,,,, 2004-163T12:42:00,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.47 mrad; phase=87; LT=6.5; (-22, 39); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.),center detectors.",,,,,, 2004-163T12:42:00,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 24x12, 160ms and 640ms 6 cubes of each",,,,,, 2004-163T13:13:00,000T00:05:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1G,Low resolution imaging,Phoebe Approach Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-163T13:13:00,000T00:05:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1G,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:05. CIRS: center detectors, 96 RTI.",,,,,, 2004-163T13:13:00,000T00:05:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi-res and ir hi-res, 12x12, 320ms",,,,,, 2004-163T14:03:37,000T01:31:00,11-Jun-04,RADAR,Prime,Phoebe,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Phoebe.,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2004-163T15:34:37,000T00:36:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1J,Low resolution imaging,Phoebe Approach Global Color Mapping,"Turn -Y to Phoebe; Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-163T15:34:37,000T00:36:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12 x12 320ms",,,,,, 2004-163T15:54:37,000T00:47:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T16:10:37,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP3REGION,CIRS FP3 regional map,FP3 map,"AD=2.96 mrad; phase=86; LT=6.6; (-22, 172); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T16:10:37,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"36 x36 hi res vis and ir, one each of 640 and 160ms",,,,,, 2004-163T16:41:37,000T00:16:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1K,Low resolution imaging,Phoebe Approach Global Mapping,Do 1x1 mosaic (3 NAC clr) filters; do 9 dark frames (for HIRESC inbound color data),,,,,, 2004-163T16:41:37,000T00:16:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1K,Low resolution imaging,Rider on ISS low resolution 30 degree longitude co,"ISS rider; duration 00:16. CIRS: blink, shutter closed. Calibration only: ca. 5 min. 38 RTI, 10 min 96 RTI.",,,,,, 2004-163T16:41:37,000T00:47:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T16:41:37,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320 ms",,,,,, 2004-163T16:57:37,000T00:31:00,11-Jun-04,CIRS,Prime,Phoebe,FP3REGION,CIRS FP3 regional map,FP3 map,"AD=3.85 mrad; phase=85; LT=6.6; (-22, 202); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T16:57:37,000T00:31:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 36x36,640 ms, and 160ms 1 cube each",,,,,, 2004-163T17:28:37,000T00:15:00,11-Jun-04,ISS,Prime,Phoebe,LOWRES1L,Low resolution imaging,Phoebe Approach Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-163T17:28:37,000T00:15:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES1L,Low resolution imaging,Rider on ISS low resolution 30 degree longitude co,"ISS rider; duration 00:15. CIRS: blink, 38 RTI.",,,,,, 2004-163T17:28:37,000T00:35:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T17:28:37,000T00:16:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis hi and ir hi res, 12x12, 320ms",,,,,, 2004-163T17:33:37,000T04:00:00,11-Jun-04,MAG,Non-SPASS,Phoebe,PHTAR,Phoebe targeted flyby,Phoebe targeted flyby,Monitor the interaction of Phoebe with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field. Starttime was tied to Phoebe LMB epoch - 2 hours (163T17:33:37). This has been removed for SOPU/SSUP.,,,,,, 2004-163T17:43:37,000T00:20:00,11-Jun-04,CIRS,Prime,Phoebe,FP3REGION,CIRS FP3 regional map,FP3 map,"AD=5.45 mrad; phase=85; LT=6.6; (-21, 231); duration 00:20. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T17:43:37,000T00:20:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi-res, 48 x 48 320 ms",,,,,, 2004-163T18:03:37,000T00:08:00,11-Jun-04,ISS,Prime,Phoebe,MEDRESA,Medium resolution global mapping,Phoebe Approach Mapping and Color,Do 2x1 NAC mosaic (clear filters),,,,,, 2004-163T18:03:37,000T00:08:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,MEDRESA,Medium resolution global mapping,ISS rider,"ISS rider; duration 00:08. CIRS: blink, 38 RTI.",,,,,, 2004-163T18:03:37,000T00:08:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T18:03:37,000T00:08:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12 x 12, 320ms",,,,,, 2004-163T18:11:37,000T00:13:00,11-Jun-04,CIRS,Prime,Phoebe,FP3EWMAPN,,FP3 EW map (north),"AD=7.29 mrad; phase=84; LT=6.6; (-21, 248); duration 00:13. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T18:11:37,000T00:13:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T18:11:37,000T00:13:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi-res, 36x36, 320ms and 160ms, 1 of each",,,,,, 2004-163T18:24:37,000T00:14:00,11-Jun-04,ISS,Prime,Phoebe,MEDRESB,Medium resolution global mapping,Phoebe Approach Mapping,Do 3x2 NAC clear mosaic + 3-color WAC context,,,,,, 2004-163T18:24:37,000T00:14:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,MEDRESB,Medium resolution global mapping,ISS rider,"ISS rider; duration 00:14. CIRS: blink, 38 RTI.",,,,,, 2004-163T18:24:37,000T00:14:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T18:24:37,000T00:14:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-163T18:33:37,000T02:00:00,11-Jun-04,MIMI,SPASS Rider,Phoebe,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,Part of RS MAPS Campaign. Icy moon encounter in solar wind. Pointing: -X to sun.,,,,,, 2004-163T18:33:37,000T03:00:00,11-Jun-04,RADAR,SPASS Rider,Phoebe,WARMNODAT,RADAR warmup,"Warmup, no bits.",Warmup the instrument in an opmode that allows RADAR operation. But in a telemetry mode that does not allow collection of RADAR data.,,,,,, 2004-163T18:33:37,000T02:00:00,11-Jun-04,INMS,Non-SPASS,Phoebe,ENCOUNTER,MAPS Campaign,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-163T18:38:37,000T00:12:00,11-Jun-04,CIRS,Prime,Phoebe,FP3NITMAP,CIRS FP3 nighttime map,FP3 nighttime map,"AD=11.00 mrad; phase=82; LT=6.7; (-21, 264); duration 00:12. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T18:38:37,000T00:12:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T18:38:37,000T00:12:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi-res, 36x36, 320ms and 80ms, 1 of each",,,,,, 2004-163T18:50:37,000T00:21:00,11-Jun-04,ISS,Prime,Phoebe,HIRESA,High resolution image,Phoebe High Resolution Mosaics and High-res color,"Do high-res NAC mosaics (3x2 and 6-frame), 4 WAC filter 1x1 context for both; 3-color NAC at last footprint",,,,,, 2004-163T18:50:37,000T00:21:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,HIRESA,High resolution image,ISS rider,"ISS rider; duration 00:21. CIRS: blink, 38 RTI.",,,,,, 2004-163T18:50:37,000T00:21:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T18:50:37,000T00:21:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms,",,,,,, 2004-163T19:03:37,000T01:00:00,11-Jun-04,CAPS,SPASS Rider,Phoebe,ENCOUNTER,MAPS Campaign,MAPS 000PH Campaign,Part of 000PH MAPS Campaign. Observe interaction between Phoebe and the solar wind,,,,,, 2004-163T19:06:37,000T00:54:00,11-Jun-04,RPWS,Non-SPASS,Phoebe,PHCA,Phoebe closest approach,Phoebe closest approach observations,"RPWS observations in the immediate vicinity of Phoebe, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. No pointing requirement.",,,,,, 2004-163T19:11:37,000T00:10:00,11-Jun-04,CIRS,Prime,Phoebe,FP1NITMAP,CIRS FP1 dark side map,FP3 nighttime map,"AD=25.92 mrad; phase=75; LT=7.0; (-19, 277); duration 00:10. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink, shutter closed.",,,,,, 2004-163T19:11:37,000T00:10:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T19:11:37,000T00:10:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi-res, 36x36, 320ms",,,,,, 2004-163T19:18:37,000T00:30:00,11-Jun-04,CDA,Non-SPASS,Phoebe,PHODUST,Phoebe dust observation,Dust envelope around Phoebe,"Study dust envelope around Phoebe. CDA boresight must be orientated toward the Phobe dust RAM (see CDA TOST white paper for definition). Our pointing requirements are met by various orientations. It seems to be inpossible to share the observation with the ORS instruments. Estimated data volume: 7.5 Mbits, data rate: 4192 bps, power: 19.5 W (with articulation), 11 W (without articulation)",,,,,, 2004-163T19:21:37,000T01:07:00,11-Jun-04,ISS,Prime,Phoebe,HIRESC,High resolution image,Phoebe High Resolution Mosaics and Color,"Do highest-res NAC mosaics (8 footprints inbound, 9 outbound) plus WAC context; outbound also 19 color + 6 polarizer highres NAC.",,,,,, 2004-163T19:21:37,000T01:07:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,HIRESC,High resolution image,ISS rider,"INCLUDES CLOSEST APPROACH (from DIGIT this is at 19:33:37). At start of observation: AD=43.8, phase=66, LT=8.0, (-15, 273); at C/A: AD=109.0, phase=24, LT=11.0, (11, 220); at end of observation: AD=11.0, phase=88, LT=18.0, (23, 167). Duration 01:07. CIRS: 38 RTI (15.5 cm-1, 4.75 sec), blink; shutter closed last 00:07.",,,,,, 2004-163T19:21:37,000T01:07:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T19:21:37,000T01:07:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-163T19:49:00,000T01:48:21,11-Jun-04,CDA,Non-SPASS,Phoebe,SURVEY,Magnetospheric survey,Phoebe dust survey,dust survey data rate = 100 bps power = 12 W,,,,,, 2004-163T20:00:37,001T02:31:23,11-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-163T20:03:37,001T02:29:39,11-Jun-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-163T20:22:03,001T02:09:57,11-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-163T20:28:37,000T00:15:00,11-Jun-04,CIRS,Prime,Phoebe,FP3DAYMAP,CIRS FP3 daytime map,FP3 daytime map,"AD=11.04 mrad; phase=88; LT=18.1; (23, 167); duration 00:15. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T20:28:37,000T00:15:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T20:28:37,000T00:15:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi-res, 48x48, 320ms",,,,,, 2004-163T20:33:37,005T03:33:23,11-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-163T20:43:37,000T00:10:00,11-Jun-04,ISS,Prime,Phoebe,MEDRESD,Medium resolution global mapping,Phoebe Departure Mapping and regional color,"Do 2x1 NAC mosaic, then 1x1 regional short wavelength color (12 NACs from UV1 to GRN)",,,,,, 2004-163T20:43:37,000T00:10:00,11-Jun-04,CIRS,SPASS Rider,Phoebe,MEDRESD,Medium resolution global mapping,ISS rider,"ISS rider; duration 00:10. CIRS: blink, 38 RTI.",,,,,, 2004-163T20:43:37,000T00:10:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T20:43:37,000T00:10:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-163T20:53:37,000T00:39:00,11-Jun-04,CIRS,Prime,Phoebe,FP3NITMAP,CIRS FP3 nighttime map,FP3 nighttime map,"AD=7.59 mrad; phase=89; LT=18.0; (23, 181); duration 00:39. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), blink.",,,,,, 2004-163T20:53:37,000T00:39:00,11-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-163T20:53:37,000T00:39:00,11-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi-res, 36x36, 640, 160ms 2 of each",,,,,, 2004-163T21:33:37,000T04:15:00,11-Jun-04,RADAR,Prime,Phoebe,2SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Phoebe. #2,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2004-163T21:33:37,001T00:58:23,11-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps). Starttime was tied to Phoebe LMB + 4hrs (163T21:33:37). Has been removed for SOPU/SSUP.,,,,,, 2004-163T21:33:37,000T04:15:00,11-Jun-04,RADAR,Non-SPASS,Phoebe,REUBITS,Data volume adjustment,REU bits request,REU bits,,,,,, 2004-163T21:38:37,000T04:15:00,11-Jun-04,CDA,Non-SPASS,Phoebe,PHODUST,Phoebe dust observation,study of Phoebe dust environment,"Study dust in the vincinity of Phoebe. Ride along with RADAR. Secondary axis: -x = (ra: 283.6, dec: 50.6) @ 21:35, -x = (ra: 284.9, dec: 51.7) @ 23:00 Power: 11 W. Data rate: 200 bps.",,,,,, 2004-164T01:54:00,003T22:12:59,12-Jun-04,CDA,Non-SPASS,DustRAM direction,RETRO,MAPS retrograde campaign,retrograd dust exploration,dust anti-RAM: -z2E and a) -x 18 ; -5 AM=97 b) -x 120 ; -67 AM=261,,,,,, 2004-164T02:33:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2A,Low resolution imaging,Phoebe Departure Global Color Mapping,"Turn -Y to Phoebe; do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-164T02:33:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2A,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T02:33:00,000T09:37:00,12-Jun-04,UVIS,SPASS Rider,Phoebe,ICYMAP,Icy satellite surface map,ICYMAP: Phoebe UV Map,UV albedo of Phoebe's surface,,,,,, 2004-164T02:33:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T02:49:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.39 mrad; phase=92; LT=18.0; (22, 48); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T02:49:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T03:20:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2B,Low resolution imaging,Phoebe Departure Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-164T03:20:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2B,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: cnter detectors, shutter closed. Calibration only: ca. 5 min. 38 RTI, 10 min 96 RTI.",,,,,, 2004-164T03:20:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T03:36:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.25 mrad; phase=92; LT=18.0; (22, 78); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T03:36:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T04:07:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2C,Low resolution imaging,Phoebe Departure Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-164T04:07:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2C,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T04:07:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T04:23:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.14 mrad; phase=92; LT=18.0; (22, 108); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T04:23:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T04:54:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2D,Low resolution imaging,Phoebe Departure Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-164T04:54:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2D,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T04:54:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T05:10:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=1.05 mrad; phase=92; LT=18.0; (22, 139); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T05:10:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T05:41:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2E,Low resolution imaging,Phoebe Departure Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-164T05:41:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2E,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T05:41:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T05:57:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.97mrad; phase=92; LT=18.0; (22, 169); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T05:57:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T06:28:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2F,Low resolution imaging,Phoebe Departure Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-164T06:28:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2F,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T06:28:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T06:44:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.90mrad; phase=92; LT=18.0; (22, 199); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T06:44:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T07:15:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2G,Low resolution imaging,Phoebe Departure Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-164T07:15:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2G,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T07:15:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T07:31:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.84mrad; phase=92; LT=18.0; (22, 230); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T07:31:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T08:02:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2H,Low resolution imaging,Phoebe Departure Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-164T08:02:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2H,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T08:02:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T08:18:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.79mrad; phase=92; LT=18.0; (22, 260); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T08:18:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T08:49:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2I,Low resolution imaging,Phoebe Departure Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters)",,,,,, 2004-164T08:49:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2I,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T08:49:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T09:05:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.74mrad; phase=92; LT=18.0; (22, 290); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T09:05:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T09:36:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2J,Low resolution imaging,Phoebe Departure Global Mapping,Do 1x1 mosaic (3 NAC clr filters),,,,,, 2004-164T09:36:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2J,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T09:36:00,000T00:16:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis and ir hi res, 12x12, 320ms",,,,,, 2004-164T09:52:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.70mrad; phase=93; LT=17.9; (22, 321); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T09:52:00,000T00:31:00,12-Jun-04,VIMS,SPASS Rider,Phoebe,PHOEBE,Phoebe observation,Phoebe,"vis low res and ir hi res, 12x12, 640ms and 160ms. Do 12 of each time",,,,,, 2004-164T10:23:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2K,Low resolution imaging,Phoebe Departure Global Color Mapping,"Do 1x1 mosaic (3 NAC clr, 12 NAC color, 6 NAC polarizer filters). Do 6 dark frames for LOWRES color observations.",,,,,, 2004-164T10:23:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2K,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, 96 RTI.",,,,,, 2004-164T10:39:00,000T00:31:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.67mrad; phase=93; LT=17.9; (22, 351); duration 00:31. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T11:10:00,000T00:16:00,12-Jun-04,ISS,Prime,Phoebe,LOWRES2L,Low resolution imaging,Phoebe Departure Global Mapping,Do 1x1 mosaic (up to 3 NAC clr filters). Do up to 21 dark frames for LOWRES color observations.,,,,,, 2004-164T11:10:00,000T00:16:00,12-Jun-04,CIRS,SPASS Rider,Phoebe,LOWRES2L,Low resolution imaging,Rider on ISS low resolution longitude coverage.,"ISS rider; duration 00:16. CIRS: center detectors, shutter closed. Calibration only: ca. 5 min. 38 RTI, 10 min 96 RTI.",,,,,, 2004-164T11:26:00,000T00:44:00,12-Jun-04,CIRS,Prime,Phoebe,FP13LTCRV,CIRS FP13 light curve,FP13 Light Curve,"AD=0.63mrad; phase=93; LT=17.9; (22, 21); duration 00:44. CIRS: 38 RTI (4.75 sec, 15.5 cm-1 res.), center detectors.",,,,,, 2004-164T13:32:00,000T02:28:00,12-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-164T16:30:00,000T02:30:00,12-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-164T22:32:00,006T23:20:00,12-Jun-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-164T22:32:00,003T01:35:00,12-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-164T22:32:00,003T01:35:00,12-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-164T22:33:00,004T01:34:00,12-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-164T23:50:00,000T00:30:00,12-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 087 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EN-DI-HY-HE-EP (602, 604, 607, 611, 612)]",,,,,, 2004-165T00:20:00,000T00:30:00,13-Jun-04,ISS,Prime,Titan,MOVIEHHH,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-165T00:50:00,000T02:00:00,13-Jun-04,UVIS,Prime,Titan,MOS12PEA,Linear mosaic,MOSAIC_12_PER_04a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-165T02:50:00,000T00:30:00,13-Jun-04,ISS,Prime,Titan,MOVIEHHH,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-165T03:20:00,000T02:00:00,13-Jun-04,UVIS,Prime,Titan,MOS12PEB,Linear mosaic,MOSAIC_12_PER_04b,. Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/- Range): 159.17mrad.,,,,,, 2004-165T05:20:00,000T00:30:00,13-Jun-04,ISS,Prime,Titan,MOVIEHHH,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-165T05:50:00,000T00:40:00,13-Jun-04,UVIS,Prime,Titan,MOS12PEC,Linear mosaic,MOSAIC_12_PER_04c,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation.,,,,,, 2004-165T07:52:00,000T09:00:00,13-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-165T08:37:00,000T03:00:00,13-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-165T18:07:00,000T00:30:00,13-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 090 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-CP-DI-PM-JA (604, 610, 614, 616, 617)]",,,,,, 2004-165T18:37:00,000T00:30:00,13-Jun-04,ISS,Prime,Titan,MOVIEIII,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-165T19:07:00,000T02:00:00,13-Jun-04,UVIS,Prime,Titan,MOS12PEA,Linear mosaic,MOSAIC_12_PER_05a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-165T21:07:00,000T00:30:00,13-Jun-04,ISS,Prime,Titan,MOVIEIII,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-165T21:37:00,000T02:00:00,13-Jun-04,UVIS,Prime,Titan,MOS12PEB,Linear mosaic,MOSAIC_12_PER_05b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-165T23:37:00,000T00:30:00,13-Jun-04,ISS,Prime,Titan,MOVIEIII,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-166T00:07:00,000T02:00:00,14-Jun-04,UVIS,Prime,Titan,MOS12PEC,Linear mosaic,MOSAIC_12_PER_05c,.Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-166T02:07:00,000T00:30:00,14-Jun-04,ISS,Prime,Titan,MOVIEIII,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-166T02:37:00,000T02:00:00,14-Jun-04,UVIS,Prime,Titan,MOS12PED,Linear mosaic,MOSAIC_12_PER_05d,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-166T04:37:00,000T00:30:00,14-Jun-04,ISS,Prime,Titan,MOVIEIII,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-166T05:07:00,000T02:00:00,14-Jun-04,UVIS,Prime,Titan,MOS12PEE,Linear mosaic,MOSAIC_12_PER_05e,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/-Range): 159.17mrad.,,,,,, 2004-166T07:07:00,000T00:30:00,14-Jun-04,ISS,Prime,Titan,MOVIEIII,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-166T07:37:00,000T02:00:00,14-Jun-04,UVIS,Prime,Titan,MOS12PEF,Linear mosaic,MOSAIC_12_PER_05f,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-166T09:37:00,000T04:15:00,14-Jun-04,VIMS,Prime,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2. Time of observation (hours) = 3.75. Volume (Mbits) = 61.9. Mosaic of entire ring system near apoapse. Sunlit face. Mosaic size 1x2. Also 8 radial scans 64x12 across lit ring ansa in high-res mode. Exposures 80 msec and 320 msec.",,,,,, 2004-166T09:37:00,000T04:15:00,14-Jun-04,CIRS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Rider on VIMS ring mosaic,FP1 integrations on main rings during VIMS ring mosaics,,,,,, 2004-166T15:07:00,000T09:00:00,14-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-167T00:00:00,001T00:00:00,15-Jun-04,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination Data rate set to near zero -- overlaps normal science data observations, so produces no additional data volume.",,,,,, 2004-167T01:22:00,000T00:30:00,15-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 094 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-AT-TL-EN-JA (602, 610, 611, 613, 615)]",,,,,, 2004-167T01:52:00,000T00:30:00,15-Jun-04,ISS,Prime,Titan,MOVIEJJJ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-167T02:22:00,000T02:00:00,15-Jun-04,UVIS,Prime,Titan,MOS12PEA,Linear mosaic,MOSAIC_12_PER_06a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-167T04:22:00,000T00:30:00,15-Jun-04,ISS,Prime,Titan,MOVIEJJJ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-167T04:52:00,000T02:00:00,15-Jun-04,UVIS,Prime,Titan,MOS12PEB,Linear mosaic,MOSAIC_12_PER_06b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-167T06:52:00,000T00:30:00,15-Jun-04,ISS,Prime,Titan,MOVIEJJJ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-167T07:22:00,000T02:00:00,15-Jun-04,UVIS,Prime,Titan,MOS12PEC,Linear mosaic,MOSAIC_12_PER_06c,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn +/-Range): 159.17mrad.,,,,,, 2004-167T09:22:00,000T00:30:00,15-Jun-04,ISS,Prime,Titan,MOVIEJJJ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-167T09:52:00,000T02:00:00,15-Jun-04,UVIS,Prime,Titan,MOS12PED,Linear mosaic,MOSAIC_12_PER_06d,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-167T11:52:00,000T00:30:00,15-Jun-04,ISS,Prime,Titan,MOVIEJJJ,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-167T12:22:00,000T01:30:00,15-Jun-04,UVIS,Prime,Titan,MOS12PEE,Linear mosaic,MOSAIC_12_PER_06e,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation.,,,,,, 2004-167T15:07:00,000T09:00:00,15-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-168T00:07:00,003T15:44:59,16-Jun-04,CDA,Non-SPASS,DustRAM direction,RETRO,MAPS retrograde campaign,retrograd dust exploration,dust anti-RAM: -z2E and a) -x 18 ; -5 AM=97 b) -x 120 ; -67 AM=261,,,,,, 2004-168T00:07:00,002T23:45:00,16-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-168T00:07:00,002T23:45:00,16-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-168T01:22:00,000T00:30:00,16-Jun-04,ISS,Prime,Other,SATELLORA,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 097 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-EN-PM-PA-EP (602, 611, 615, 616, 617)]",,,,,, 2004-168T01:52:00,000T00:30:00,16-Jun-04,ISS,Prime,Titan,MOVIEKKK,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-168T02:00:00,000T02:17:00,16-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-168T02:22:00,000T02:00:00,16-Jun-04,UVIS,Prime,Titan,MOS12PEA,Linear mosaic,MOSAIC_12_PER_07a,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-168T04:22:00,000T00:30:00,16-Jun-04,ISS,Prime,Titan,MOVIEKKK,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-168T04:52:00,000T02:00:00,16-Jun-04,UVIS,Prime,Titan,MOS12PEB,Linear mosaic,MOSAIC_12_PER_07b,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-168T06:52:00,000T00:30:00,16-Jun-04,ISS,Prime,Titan,MOVIEKKK,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-168T07:22:00,000T02:00:00,16-Jun-04,UVIS,Prime,Titan,MOS12PEC,Linear mosaic,MOSAIC_12_PER_07c,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. 1) Align slit parallel with the Saturn Spin Axis. 2) Step 160 times about the Z-axis using 0.114 deg increments for 3600s from Titan to -MOS Orb (decreasing RA angles). Stare for 22.5s during each step increment. 3) Step 80 times about the Z-axis using .114 deg increments for 1800s toward Titan. Stare for 22.5s during each step increment. 4) Slew back to Titan and reset pointing. Stare for remaining observation time. MOS Orb (Saturn+/-Range): 159.17mrad.,,,,,, 2004-168T09:22:00,000T00:30:00,16-Jun-04,ISS,Prime,Titan,MOVIEKKK,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds,,,,,, 2004-168T09:52:00,000T01:30:00,16-Jun-04,UVIS,Prime,Titan,MOS12PED,Linear mosaic,MOSAIC_12_PER_07d,Linear mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on. Stare at waypoint for duration of observation.,,,,,, 2004-168T11:22:00,000T02:30:00,16-Jun-04,VIMS,Prime,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2, Time of observation (hours) = 2.0, Volume (Mbits) = 45 Mosaic of entire ring system near apoapse. Sunlit face. Mosaic size 1x2. Also 3 radial scans 64x12 across lit ring ansa in high-res mode, exposures 80 msec and 320 msec.",,,,,, 2004-168T11:22:00,000T02:30:00,16-Jun-04,CIRS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Rider on VIMS ring mosaic,FP1 integrations on main rings during VIMS ring mosaics,,,,,, 2004-168T15:07:00,000T09:00:00,16-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-168T16:00:00,000T02:17:00,16-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-169T00:07:00,000T15:00:00,17-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-169T00:07:00,002T15:45:00,17-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-169T01:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Titan,APPROACH,Aproach imaging,Titan Approach Imaging,"Point to Titan, run through sequence of filters most likely to be of use, determine which are best.",,,,,, 2004-169T01:22:00,000T00:30:00,17-Jun-04,CIRS,SPASS Rider,Titan,APPROACH,Aproach imaging,Titan rider,Titan rider,,,,,, 2004-169T01:52:00,000T03:00:00,17-Jun-04,CIRS,Prime,Saturn,FIRCMPSIT,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT006_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-169T06:07:00,000T09:00:00,17-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-169T15:07:00,002T06:45:00,17-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-169T16:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T16:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T17:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T17:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T18:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T18:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T19:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T19:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T20:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T20:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T21:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T21:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T22:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T22:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T23:22:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-169T23:52:00,000T00:30:00,17-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-170T00:22:00,000T00:30:00,18-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-170T00:52:00,000T00:30:00,18-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-170T01:00:00,000T11:23:00,18-Jun-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 160 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2004-170T01:22:00,000T00:30:00,18-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-170T01:52:00,000T00:30:00,18-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-170T02:22:00,000T01:15:00,18-Jun-04,ISS,Prime,Saturn,2X2PLRNC,Polarimetry,Saturn polarimetry,NAC Polarimetery & Color & methane imaging,,,,,, 2004-170T03:37:00,000T10:00:00,18-Jun-04,CIRS,Prime,Saturn,MIRCMPSIT,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Composition study at 0.5cm-1. Make sure FP1, FP3, & FP4 are on Saturn. After other requests were cut we need more pre-SOI integration time on FP1. If all FP's do not fit on the portion of Saturn unobscured by rings, then divide the time between FP1 on Saturn (5 hours) and FP3/4 on Saturn (5 hours).",,,,,, 2004-170T14:52:00,000T09:00:00,18-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-170T15:45:00,000T06:00:00,18-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-170T23:52:00,000T16:00:00,18-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-170T23:52:00,000T16:00:00,18-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-171T01:07:00,000T00:30:00,19-Jun-04,ISS,Prime,Rhea,PRESOIA,Pre-SOI imaging,Rhea pre-SOI observation (leading side),Turn -Y to Rhea; do 1x1 mosaic 2 NAC clear plus multiple NAC color and polarizer filters; do dark frames; turn to WP.,,,,,, 2004-171T01:07:00,000T00:30:00,19-Jun-04,CIRS,SPASS Rider,Rhea,PRESOIA,Pre-SOI imaging,Rhea rider,"Rhea rider on ISS. AD=0.21, phase=63, (-17, 121). Duration 00:30. CIRS: 38 RTI, center detectors. No data 00:00 to 00:17 (data rate multiplier 0.42); data, shutter open 00:17 to 00:29; shutter closed 00:20 to 00:30.",,,,,, 2004-171T01:37:00,000T10:30:00,19-Jun-04,CIRS,Prime,Saturn,FIRCMPSIT,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-171T12:07:00,000T00:30:00,19-Jun-04,ISS,Prime,Titan,APPROACH,Aproach imaging,Titan Approach Imaging,"Point to Titan, run through sequence of filters most likely to be of use, determine which are best.",,,,,, 2004-171T12:07:00,000T00:30:00,19-Jun-04,CIRS,SPASS Rider,Titan,APPROACH,Aproach imaging,Titan rider,Titan rider,,,,,, 2004-171T12:37:00,000T02:00:00,19-Jun-04,VIMS,Prime,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2, Time of observation (hours) = 2.0, Volume (Mbits) = 45 Mosaic of entire ring system near apoapse. Sunlit face. Mosaic size 1x2. Also 3 radial scans 64x12 across lit ring ansa in high-res mode, exposures 80 msec and 320 msec.",,,,,, 2004-171T12:37:00,000T02:00:00,19-Jun-04,CIRS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Rider on VIMS ring mosaic,FP1 integrations on main rings during VIMS ring mosaics,,,,,, 2004-171T14:37:00,000T01:15:00,19-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,OPNAV rider for deep space,Any pointing O.K. Deep space during OPNAV turns,,,,,, 2004-171T15:52:00,000T06:00:00,19-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-171T15:52:00,000T05:59:59,19-Jun-04,CDA,Non-SPASS,DustRAM direction,RETRO,MAPS retrograde campaign,retrograd dust exploration,dust anti-RAM: -z2E and a) -x 18 ; -5 AM=97 b) -x 120 ; -67 AM=261,,,,,, 2004-171T15:52:00,000T06:00:00,19-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-171T15:52:00,000T06:00:00,19-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-171T15:52:00,000T06:00:00,19-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-171T15:52:00,000T06:00:00,19-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-171T21:52:00,002T20:40:00,19-Jun-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-171T21:52:00,002T20:40:00,19-Jun-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-171T21:52:00,000T00:23:00,19-Jun-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-171T21:52:00,002T02:20:00,19-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-171T21:52:00,002T20:40:00,19-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-171T21:52:00,002T20:40:00,19-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-171T22:15:00,002T01:37:00,19-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-171T23:07:00,000T00:30:00,19-Jun-04,ISS,Prime,Dione,PRESOIB,Pre-SOI imaging,Dione pre-SOI observation,Turn -Y to Dione; do 1x1 NAC mosaic 1 clear + 12 color + 6 polarizer filters; turn to WP,,,,,, 2004-171T23:07:00,000T00:30:00,19-Jun-04,CIRS,SPASS Rider,Dione,PRESOIB,Pre-SOI imaging,Dione rider,Dione rider,,,,,, 2004-171T23:07:00,000T00:30:00,19-Jun-04,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-171T23:37:00,000T05:30:00,19-Jun-04,CIRS,Prime,Saturn,FIRCMPSIT,Sit and stare to derive composition,CIRS_000SA_FIRCMPSIT001_PRIME,"Measure oxygen compounds (H2O) in stratosphere. Search for new tropospheric species (HCP, H2S, H2Se, Halides). Measure hydrogen dimers and PH3. Determine HD/H2. FP1 to Saturn.",,,,,, 2004-172T05:07:00,000T02:00:00,20-Jun-04,VIMS,Prime,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2, Time of observation (hours) = 2.0, Volume (Mbits) = 45 Mosaic of entire ring system near apoapse. Sunlit face. Mosaic size 1x2. Also 3 radial scans 64x12 across lit ring ansa in high-res mode, exposures 80 msec and 320 msec.",,,,,, 2004-172T05:07:00,000T02:00:00,20-Jun-04,CIRS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Rider on VIMS ring mosaic,FP1 integrations on main rings during VIMS ring mosaics,,,,,, 2004-172T07:07:00,000T01:15:00,20-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,OPNAV rider for deep space,Any pointing O.K. Deep space during OPNAV turns,,,,,, 2004-172T08:22:00,000T06:00:00,20-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-172T08:22:00,000T06:00:00,20-Jun-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-172T15:37:00,000T02:00:00,20-Jun-04,VIMS,Prime,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2, Time of observation (hours) = 2.0, Volume (Mbits) = 45 Mosaic of entire ring system near apoapse. Sunlit face. Mosaic size 1x2. Also 3 radial scans 64x12 across lit ring ansa in high-res mode, exposures 80 msec and 320 msec.",,,,,, 2004-172T15:37:00,000T02:00:00,20-Jun-04,CIRS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Rider on VIMS ring mosaic,FP1 integrations on main rings during VIMS ring mosaics,,,,,, 2004-172T17:37:00,000T00:20:00,20-Jun-04,ISS,Prime,Tethys,PRESOIC,Pre-SOI imaging,Tethys pre-SOI observation,Turn to Tethys; 2x NAC clear + 23 NAC color/polarization filters; turn to WP,,,,,, 2004-172T17:37:00,000T00:20:00,20-Jun-04,CIRS,SPASS Rider,Tethys,PRESOIA,Pre-SOI imaging,Tethys rider,Tethys rider,,,,,, 2004-172T17:37:00,000T00:20:00,20-Jun-04,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-172T17:57:00,000T16:30:00,20-Jun-04,ISS,Prime,rings(general),SATSRCHAP,Ansa movie,"ANSA MOVIE FOR SATELLITE SEARCHES, POST PHOEBE IN","ANSA MOVIE,1 X 2,C RING AND A RING REGION, FOR SEARCHING FOR SATELLITES IN RING GAPS ON APPROACH(POST PHOEBE ENCOUNTER)",,,,,, 2004-172T17:57:00,000T16:30:00,20-Jun-04,CIRS,SPASS Rider,rings(general),SATSRCHAP,Ansa movie,CIRS_000_SATSRCHAP rider,Ride with ISS during SATSRCH,,,,,, 2004-173T10:27:00,000T00:40:00,21-Jun-04,ISS,Prime,Other,DIONERHEA,,Dione (leading) and Rhea (trailing side) pre-SOI c,Turn -Y to Dione; do 1x1 mosaic 2 NAC clear plus 23 NAC color/ polarizer filters. Turn -Y to Rhea; do 1x1 mosaic 2 NAC clear plus 23 NAC color and polarizer filters. Turn to WP,,,,,, 2004-173T10:27:00,000T00:20:00,21-Jun-04,CIRS,SPASS Rider,Dione,PRESOIA,Pre-SOI imaging,Dione rider,Dione rider,,,,,, 2004-173T10:27:00,000T00:40:00,21-Jun-04,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-173T10:47:00,000T00:20:00,21-Jun-04,CIRS,SPASS Rider,Rhea,PRESOIB,Pre-SOI imaging,Rhea rider,rhea rider,,,,,, 2004-173T11:07:00,000T01:30:00,21-Jun-04,ISS,Prime,rings(general),RINGPHOTM,Ring photometry,RING PHOTOMETRY ON APPROACH,RING PHOTOMETRY DURING LATE APPROACH BETWEEN PHOEBE AND SOI,,,,,, 2004-173T11:07:00,000T01:30:00,21-Jun-04,CIRS,SPASS Rider,rings(general),RINGPHOTM,Ring photometry,Rider on ISS ring photometry,FP3 and FP4 integrations on main rings during ISS ring mosaics,,,,,, 2004-173T11:07:00,000T01:30:00,21-Jun-04,VIMS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"ISS Rider. Cube Size (X,Z) = 12*12, Time per SC pointing (mins) = 2.5, Number of SC pointings = 16, Time of observation (hours) = 1.5, Volume (Mbits) = 10. Mosaic of entire ring system near apoapse. Sunlit face. Mosaic size 4x4. Exposures 80 msec and 320 msec. Data vol is enough for an extra 16 cubes.",,,,,, 2004-173T12:37:00,000T01:00:00,21-Jun-04,ISS,Prime,Other,ENHYTE,,"Enceladus, Hyperion, and Tethys pre-SOI color obs","Turn to satellite; do 2x NAC clear + 23 NAC color/polarization filters for each of the three satellites, then return to WP. Each satellite gets same amount of dwell time.",,,,,, 2004-173T12:37:00,000T00:20:00,21-Jun-04,CIRS,SPASS Rider,Enceladus,PRESOI,Pre-SOI imaging,Enceladus rider,Enceladus rider,,,,,, 2004-173T12:37:00,000T01:00:00,21-Jun-04,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-173T12:57:00,000T00:20:00,21-Jun-04,CIRS,SPASS Rider,Hyperion,PRESOI,Pre-SOI imaging,Hyperion rider,Hyperion rider,,,,,, 2004-173T13:17:00,000T00:20:00,21-Jun-04,CIRS,SPASS Rider,Tethys,PRESOIB,Pre-SOI imaging,Tethys rider,Tethys rider,,,,,, 2004-173T13:37:00,000T01:15:00,21-Jun-04,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,OPNAV rider for deep space,Any pointing O.K. Deep space during OPNAV turns,,,,,, 2004-173T23:52:00,000T18:40:00,21-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-174T00:12:00,000T07:30:00,22-Jun-04,CIRS,Prime,RingB,COMP,Sit and stare to derive composition,CIRS_000RB_COMP,"B ring composition: Stare at West ansa, 90 deg phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-174T00:12:00,000T07:30:00,22-Jun-04,CIRS,SPASS Rider,RingB,COMP,Sit and stare to derive composition,CIRS_000RB_COMP_SI,Support imaging for long integration on A ring and C rings,,,,,, 2004-174T00:12:00,000T07:30:00,22-Jun-04,VIMS,SPASS Rider,rings(general),RINGMOS,Ring mosaic,Ring Mosaic during rev 0,"Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 1. FP1 stares at B ring near apoapse. Sunlit face. Also 10 radial cubes 64x12 across lit ring ansa in high-res mode. Volume (Mbits) = 34 . Exposures 80 msec and 320 msec.",,,,,, 2004-174T00:12:00,000T05:00:00,22-Jun-04,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required. Includes 2 hours for IFC cal and range checks. Final calibration before SOI.",,,,,, 2004-174T05:12:00,000T13:20:00,22-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-174T07:42:00,000T01:22:00,22-Jun-04,ISS,Prime,Other,TIMIIA,,"Titan, Mimas, and Iapetus pre-SOI (approach) color","Turn NAC to Titan; do 26 NAC images for filter testing; turn NAC to Mimas; do 1 clear + 13 color + 6 polarizer filters (all NAC 1x1); turn NAC to Iapetus, do 19 color + 6 polarizer + 2 clear filters (all NAC 1x1); turn to WP.",,,,,, 2004-174T07:42:00,000T00:30:00,22-Jun-04,CIRS,SPASS Rider,Titan,APPROACH,Aproach imaging,Titan rider,Titan rider,,,,,, 2004-174T07:42:00,000T00:13:00,22-Jun-04,VIMS,SPASS Rider,InstrumentCalibration,FSW20MST,Flight software test,VIMS FSW 20ms Anonoly Test,Flight software test.,,,,,, 2004-174T07:55:00,000T00:13:00,22-Jun-04,VIMS,SPASS Rider,InstrumentCalibration,FSW20MST,Flight software test,VIMS FSW 20ms Anonoly Test,Flight software test.,,,,,, 2004-174T08:08:00,000T00:13:00,22-Jun-04,VIMS,SPASS Rider,InstrumentCalibration,FSW20MST,Flight software test,VIMS FSW 20ms Anonoly Test,Flight software test.,,,,,, 2004-174T08:12:00,000T00:30:00,22-Jun-04,CIRS,SPASS Rider,Mimas,PRESOI,Pre-SOI imaging,Mimas rider,Mimas rider,,,,,, 2004-174T08:21:00,000T00:13:00,22-Jun-04,VIMS,SPASS Rider,InstrumentCalibration,FSW20MST,Flight software test,VIMS FSW 20ms Anonoly Test,Flight software test.,,,,,, 2004-174T08:34:00,000T00:13:00,22-Jun-04,VIMS,SPASS Rider,InstrumentCalibration,FSW20MST,Flight software test,VIMS FSW 20ms Anonoly Test,Flight software test.,,,,,, 2004-174T08:42:00,000T00:22:00,22-Jun-04,CIRS,SPASS Rider,Iapetus,PRESOI,Pre-SOI imaging,Iapetus rider,Iapetus rider,,,,,, 2004-174T08:47:00,000T00:13:00,22-Jun-04,VIMS,SPASS Rider,InstrumentCalibration,FSW20MST,Flight software test,VIMS FSW 20ms Anonoly Test,Flight software test.,,,,,, 2004-174T18:32:00,000T11:05:00,22-Jun-04,CAPS,SPASS Rider,Saturn,PRESOIOBS,Pre-SOI imaging,Observations during SOI & SOI quiet period,"Observe Saturn's magnetosphere during first pass through the system (i.e. pre-SOI quiet period) Rate changes during this period are all done inside an IEB; multiple requests are necessary to model data volume. Rate left unchanged from original request based on May 24, 2002 email from Bill Kurth. This assumes high activity days will be allowed.",,,,,, 2004-174T18:32:00,005T10:50:00,22-Jun-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-174T18:32:00,000T00:23:00,22-Jun-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-174T18:32:00,000T04:28:00,22-Jun-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-174T18:32:00,000T05:28:00,22-Jun-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-174T18:32:00,000T05:05:00,22-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-174T18:55:00,000T05:05:00,22-Jun-04,INMS,Non-SPASS,Saturn,OPSTEST,,MAPS Survey,Ride with prime instrument,,,,,, 2004-174T23:00:00,008T04:02:00,22-Jun-04,MAG,SPASS Rider,Other,SOINTFLD,MAG internal field measurements,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field during SOI. It is timed to start just before the beginning of the SOI critical sequence. Note pointing constraints only apply with 4Rs.,,,,,, 2004-174T23:00:00,000T01:00:00,22-Jun-04,MIMI,SPASS Rider,Other,CONFIGURE,Huygens probe support,Configure for SOI Quiet,Configure MIMI for SOI Quiet (data and power carried in another request),,,,,, 2004-174T23:37:00,000T00:23:00,22-Jun-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-174T23:40:00,000T00:01:00,22-Jun-04,UVIS,Non-SPASS,Saturn,SOISLEEP,Huygens probe support,UVIS TO SLEEP PRIOR TO SOI CRITICAL SEQUENCE,UVIS to go to sleep prior to SOI critical sequence,,,,,, 2004-174T23:45:00,000T00:09:50,22-Jun-04,ISS,Non-SPASS,Other,SOIQUIET,Huygens probe support,put ISS to sleep for SOI activity,placeholder activity put into CIMS to remenind ISS to go into sleep for SOI,,,,,, 2004-174T23:52:00,000T00:02:00,22-Jun-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,VIMS to SLEEP for SOI,VIMS to SLEEP for SOI,,,,,, 2004-174T23:59:15,000T00:00:00,22-Jun-04,CIRS,Non-SPASS,Other,SOISLEEP,Huygens probe support,sleep/mute placeholder for post-SOI,Go to sleep pre-SOI,,,,,, 2004-175T00:00:00,005T05:22:00,23-Jun-04,MIMI,SPASS Rider,co-rotation,SOIQUIET,Huygens probe support,Pre-SOI QUIET Campaign,"Part of MAGDYN MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-175T00:00:00,008T03:15:00,23-Jun-04,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,SLEEP between Instr test and SOI,SLEEP/MUTE for PCO14,,,,,, 2004-175T00:00:00,006T19:00:00,23-Jun-04,RPWS,Non-SPASS,Saturn,PRESOI,Pre-SOI imaging,RPWS SOI Critical Sequence Observations,"RPWS Observations during the SOI critical sequence, including the periapsis period. By requirement, this request covers the full 8-day quiet period.",,,,,, 2004-175T05:37:00,001T02:23:00,23-Jun-04,CAPS,SPASS Rider,Saturn,PRESOIOBS,Pre-SOI imaging,Observations during SOI & SOI quiet period,"Observe Saturn's magnetosphere during first pass through the system (i.e. pre-SOI quiet period) Rate changes during this period are all done inside an IEB; multiple requests are necessary to model data volume. Rate left unchanged from original request based on May 24, 2002 email from Bill Kurth. This assumes high activity days will be allowed.",,,,,, 2004-176T08:00:00,001T15:37:00,24-Jun-04,CAPS,SPASS Rider,Saturn,PRESOIOBS,Pre-SOI imaging,Observations during SOI & SOI quiet period,"Observe Saturn's magnetosphere during first pass through the system (i.e. pre-SOI quiet period) Rate changes during this period are all done inside an IEB; multiple requests are necessary to model data volume. Rate left unchanged from original request based on May 24, 2002 email from Bill Kurth. This assumes high activity days will be allowed.",,,,,, 2004-177T23:37:00,001T18:23:00,25-Jun-04,CAPS,SPASS Rider,Saturn,PRESOIOBS,Pre-SOI imaging,Observations during SOI & SOI quiet period,"Observe Saturn's magnetosphere during first pass through the system (i.e. pre-SOI quiet period) Rate changes during this period are all done inside an IEB; multiple requests are necessary to model data volume. Rate left unchanged from original request based on May 24, 2002 email from Bill Kurth. This assumes high activity days will be allowed.",,,,,, 2004-179T18:00:00,000T11:22:00,27-Jun-04,CAPS,SPASS Rider,Saturn,PRESOIOBS,Pre-SOI imaging,Observations during SOI & SOI quiet period,"Observe Saturn's magnetosphere during first pass through the system (i.e. pre-SOI quiet period) Rate changes during this period are all done inside an IEB; multiple requests are necessary to model data volume. Rate left unchanged from original request based on May 24, 2002 email from Bill Kurth. This assumes high activity days will be allowed.",,,,,, 2004-180T05:22:00,001T13:38:00,28-Jun-04,CAPS,SPASS Rider,Saturn,PRESOIOBS,Pre-SOI imaging,Observations during SOI & SOI quiet period,"Observe Saturn's magnetosphere during first pass through the system (i.e. pre-SOI quiet period) Rate changes during this period are all done inside an IEB; multiple requests are necessary to model data volume. Rate left unchanged from original request based on May 24, 2002 email from Bill Kurth. This assumes high activity days will be allowed.",,,,,, 2004-180T05:22:00,001T13:38:00,28-Jun-04,MIMI,SPASS Rider,co-rotation,SOIQUIET,Huygens probe support,Pre-SOI QUIET Campaign,"Part of MAGDYN MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-180T05:22:00,001T04:38:00,28-Jun-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-181T10:00:00,003T00:00:00,29-Jun-04,CDA,Non-SPASS,DustRAM direction,SOI,Saturn orbit insertion,SOI,"prograde dust,HRD measurements around SOI",,,,,, 2004-181T19:00:00,000T20:40:00,29-Jun-04,MIMI,SPASS Rider,co-rotation,SOIQUIET,Huygens probe support,Pre-SOI QUIET Campaign,"Part of MAGDYN MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-181T19:00:00,000T20:12:00,29-Jun-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-181T19:00:00,001T05:42:00,29-Jun-04,RPWS,Non-SPASS,Saturn,SOINBOUND,,RPWS inbound to SOI,RPWS comprehensive observations during SOI-29 hours inbound to ARPC.,,,,,, 2004-182T15:12:00,000T09:05:00,30-Jun-04,CAPS,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,Rings and Satellites Campaign,"Observe the plasma interaction with the E ring and icy satellites. NOTE: This change in data rate must be inside a long-running IEB, not in the background sequence (SOI critical sequence requirement.)",,,,,, 2004-182T15:40:00,000T11:26:40,30-Jun-04,MIMI,SPASS Rider,co-rotation,SOIQUIET,Huygens probe support,Pre-SOI QUIET Campaign,"Part of MAGDYN MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-183T00:17:00,000T02:49:40,1-Jul-04,CAPS,SPASS Rider,Saturn,SOIOBS,,Observations during SOI,"Monitor instrument status SOI burn, with all high voltages down. NOTE: This mode change must be inside a long-running IEB, not in the background sequence (SOI critical sequence requirement.)",,,,,, 2004-183T00:42:00,000T00:10:00,1-Jul-04,RPWS,Non-SPASS,Saturn,SOIARPC,Ascending ring plane crossing,RPWS SOI ARPC,Acquire high resolution waveforms during SOI ARPC for use in dust impact counts (and crude mass determination).,,,,,, 2004-183T00:52:00,000T00:20:00,1-Jul-04,RPWS,Non-SPASS,Saturn,SOIINNER,,RPWS Inbound Inner SOI measurements,Comprehensive measurements above rings after SOI APRC and before the SOI burn.,,,,,, 2004-183T01:12:00,000T01:40:00,1-Jul-04,RPWS,Non-SPASS,Saturn,SOIBURN,Saturn orbit insertion burn,RPWS observations during SOI burn,"Provides continuing coverage over the rings during SOI ME burn. Concentrates on direction-finding of SED which should be unaffected by the burn. Includes comprehensive measurements of full spectrum, as well",,,,,, 2004-183T02:52:00,000T00:14:40,1-Jul-04,RPWS,Non-SPASS,Saturn,SOIINNER,,RPWS observation over rings,Continues comprehensive observations over rings after the SOI ME burn and before the end of the critical sequence.,,,,,, 2004-183T03:02:00,000T07:49:00,1-Jul-04,MAG,SPASS Rider,Other,SOINTFLD,MAG internal field measurements,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field during SOI. It is timed to start just before the beginning of the SOI critical sequence. Note pointing constraints only apply with 4Rs.,,,,,, 2004-183T03:06:40,000T00:49:50,1-Jul-04,CAPS,SPASS Rider,rings(general),RINGS,Ring observation,Observations of ring ionosphere,"Observe the ring ionosphere from the end of SOI (over the B ring), through ring plane crossing, and out to post-SOI downlink (~3 RS)",,,,,, 2004-183T03:06:40,000T01:01:35,1-Jul-04,ISS,SPASS Rider,rings(general),SOISPTURN,,RING OBS'S DURING SOI - G POINTING (RINGSCAN001),IMAGING OF RINGS DURING SOI G POINTING.,,,,,, 2004-183T03:06:40,000T00:17:30,1-Jul-04,VIMS,SPASS Rider,rings(general),RINGSCANG,Ring radial scan,Ring radial scan during SOI,"Stellar_occ mode, star_finding OFF, IR_only. tau_IR = 160 msec, time per cube = 11.4 min. Time of observation (after turn) = 13:25 min. Observe throughout turn & science period, to minimize loss of SOI data. Data vol incl VIS data in case design is reworked later.",,,,,, 2004-183T03:06:40,000T00:47:35,1-Jul-04,RPWS,Non-SPASS,Saturn,SACA,Saturn closest approach,RPWS POST SOI Saturn Periapsis,"RPWS post-SOI periapsis observations to study lightning, ring, and the inner magnetosphere phenomena.",,,,,, 2004-183T03:06:41,000T01:44:19,1-Jul-04,MIMI,SPASS Rider,DustRAM direction,POSTBURN,,MIMI Ring Interaction Science,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-183T03:06:55,000T00:15:00,1-Jul-04,CAPS,Non-SPASS,SpacecraftActivity,CONFIGCHG,Huygens probe support,Config after SOI critical sequence,Change instrument state placeholder for a change after the SOI critical sequence,,,,,, 2004-183T03:07:10,000T00:16:50,1-Jul-04,UVIS,SPASS Rider,rings(general),RINGSCANG,Ring radial scan,,Highest spatial resolution UV spectral mapping of Saturn's rings. Spatial variation of UV albedo and water absorption edge indicative of scattering center size scale.,,,,,, 2004-183T03:07:25,000T00:03:20,1-Jul-04,CIRS,Non-SPASS,Other,SOIWAKE,Huygens probe support,wake/unmute placeholder for post-SOI,Wake and un-mute post-SOI. Note power transients!,,,,,, 2004-183T03:07:40,000T00:01:00,1-Jul-04,ISS,Non-SPASS,Other,POSTSOI,Huygens Probe support,put ISS to sleep for SOI activity,ISS wake after SOI,,,,,, 2004-183T03:07:50,000T02:17:10,1-Jul-04,CIRS,SPASS Rider,rings(general),SOIRINGS,,CIRS_000RI_SOIRINGS,"Radial scan of main rings during SOI, deep space time during turns included also.",,,,,, 2004-183T03:09:10,000T00:02:00,1-Jul-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode after SOI,VIMS to Active after SOI,,,,,, 2004-183T03:15:00,000T00:03:00,1-Jul-04,INMS,Non-SPASS,Saturn,CVRJET,Instrument cover jettison,INMS Cover Jettison,The protective cover for INMS shall be released upon Cassini SOI.,,,,,, 2004-183T03:18:00,000T00:03:00,1-Jul-04,INMS,Non-SPASS,Saturn,CVRJET,Instrument cover jettison,INMS Cover Jettison,The protective cover for INMS shall be released upon Cassini SOI.,,,,,, 2004-183T03:21:00,000T00:33:30,1-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-183T03:24:00,000T00:30:30,1-Jul-04,UVIS,SPASS Rider,rings(general),RINGSCANA,Ring radial scan,,Highest spatial resolution UV spectral mapping of Saturn's rings. Spatial variation of UV albedo and water absorption edge indicative of scattering center size scale.,,,,,, 2004-183T03:24:10,000T00:30:20,1-Jul-04,VIMS,SPASS Rider,rings(general),RINGSCANA,Ring radial scan,Ring radial scan of A ring during SOI,"Cube Size (X,Z) = 64*1, Tau_IR = 160 ms, Tau_VIS = 10.2 s, Time per SC pointing (sec) = 10.7, Number of SC pointings = 170 Time of observation (min) = 30.3.",,,,,, 2004-183T03:54:15,000T00:06:31,1-Jul-04,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2004-183T03:54:30,000T00:09:00,1-Jul-04,INMS,SPASS Rider,Saturn,RINGCOMP,Ring composition,INMS Ring Compostion,This request looks 'down' the magnetic field lines (compensating for the velocity of the SC and the particles we're looking for).,,,,,, 2004-183T03:54:30,000T00:13:45,1-Jul-04,VIMS,SPASS Rider,rings(general),WAKE,,A Ring wake observation during SOI,"Stellar_occ mode, star_finding OFF, IR_only. tau_IR = 160 msec, time per cube = 11.4 min. Time of observation (between turns) = 3:40. Observe throughout turn & science periods, to minimize loss of SOI data. Data vol incl VIS data in case design is reworked later.",,,,,, 2004-183T03:56:30,000T00:08:32,1-Jul-04,CAPS,SPASS Rider,rings(general),RINGS,Ring observation,Observations of ring ionosphere,"Observe the ring ionosphere from the end of SOI (over the B ring), through ring plane crossing, and out to post-SOI downlink (~3 RS)",,,,,, 2004-183T03:56:30,000T00:01:00,1-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,RATE4K,Data volume adjustment,Change logical telemetry rate to 4 kbps,Change logical telemetry rate to 4 kbps. Explicitly in CIMS to make sure timing works with S&ER-5a TLM change and keep automatic command generation from exploding.,,,,,, 2004-183T04:00:46,000T00:08:29,1-Jul-04,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2004-183T04:03:30,000T00:04:45,1-Jul-04,INMS,SPASS Rider,Saturn,RINGCOMP,Ring composition,INMS Ring Compostion,This request looks into Dust Ram (for Neutral Particles),,,,,, 2004-183T04:05:02,000T00:45:58,1-Jul-04,CAPS,SPASS Rider,rings(general),RINGS,Ring observation,Observations of ring ionosphere,"Observe the ring ionosphere from the end of SOI (over the B ring), through ring plane crossing, and out to post-SOI downlink (~3 RS)",,,,,, 2004-183T04:05:02,000T00:01:00,1-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,RATE16K,Data volume adjustment,Change logical telemetry rate to 16 kbps,Change logical telemetry rate to 16 kbps. Explicitly in CIMS to make sure timing works with S&ER-5a TLM change and keep automatic command generation from exploding.,,,,,, 2004-183T04:08:15,000T10:31:45,1-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-183T04:09:15,000T00:44:45,1-Jul-04,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2004-183T04:51:00,000T00:30:00,1-Jul-04,CAPS,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,Rings and Satellites Campaign,Observe the plasma interaction with the E ring and icy satellites.,,,,,, 2004-183T04:51:00,000T01:34:00,1-Jul-04,MIMI,SPASS Rider,DustRAM direction,POSTBURN,,MIMI Ring Interaction Science,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-183T04:54:00,000T00:22:00,1-Jul-04,ISS,Prime,rings(general),ARINGLIT,A ring observation,POST-SOI POST-RPLXING HI RES A RING OBSERVATION,"HI RES OUTER A RING IMAGING POST SOI,POST RING PLANE CROSSING. MOSAIC (1x9) FROM F RING TO MIMAS 5:3 IVR AT 131,900 KM, SKIPPING REGION BETW/ F RING AND A RING. ALL POSITIONS ARE BOTSIMS",,,,,, 2004-183T04:54:00,000T00:22:00,1-Jul-04,UVIS,SPASS Rider,rings(general),RANSASCN,,,Highest spatial resolution UV spectral mapping of Saturn's rings. Spatial variation of UV albedo and water absorption edge indicative of scattering center size scale.,,,,,, 2004-183T04:54:00,000T00:22:00,1-Jul-04,VIMS,SPASS Rider,rings(general),ARINGLIT,A ring observation,"SOI radial scan, high phase, lit face after DRPX","32*32 cubes, tau_IR=80 msec, tau_VIS=2.5 sec, time per cube = 95 sec (?), up to 10 ISS pointings. Data vol allows for continuous imaging.",,,,,, 2004-183T04:54:00,000T00:12:00,1-Jul-04,RPWS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,RPWS INNER MAGNETOSPHERE,Outbound inner magnetosphere observations following desending ring plane crossing.,,,,,, 2004-183T05:06:00,000T01:19:00,1-Jul-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Set up RPWS for inner magnetosphere survey, attitude N/A, any OPMODE and science TLM mode including RPWS.",,,,,, 2004-183T05:21:00,000T20:00:00,1-Jul-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-183T05:26:00,000T09:50:00,1-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-183T06:25:00,000T19:00:00,1-Jul-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-183T06:25:00,000T17:45:00,1-Jul-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Set up RPWS for inner magnetosphere survey, attitude N/A, any OPMODE and science TLM mode including RPWS.",,,,,, 2004-183T10:51:00,000T14:30:00,1-Jul-04,MAG,SPASS Rider,Other,SOINTFLD,MAG internal field measurements,MAG_Internal_Field_Measurements,"This request will yield unique observations of Saturns internal magnetic field during SOI. The whole request is timed to start just before the beginning of the SOI critical sequence, this is the TOST portion. Note pointing constraints only apply with 4Rs.",,,,,, 2004-183T14:40:00,000T10:45:00,1-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-183T15:16:00,000T09:50:00,1-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-184T00:10:00,000T01:11:00,2-Jul-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-184T01:21:00,000T04:09:21,2-Jul-04,MAG,SPASS Rider,Other,SOINTFLD,MAG internal field measurements,MAG_Internal_Field_Measurements,"This request will yield unique observations of Saturns internal magnetic field during SOI. The whole request is timed to start just before the beginning of the SOI critical sequence, this is the TOST portion. NOTE: pointing constraints only apply within 4Rs. NOTE: This is the T0min request.",,,,,, 2004-184T01:21:00,000T18:56:00,2-Jul-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-184T01:21:00,000T18:56:00,2-Jul-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-184T01:25:00,000T16:35:00,2-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-184T01:25:01,000T06:07:10,2-Jul-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-184T01:56:21,000T01:34:00,2-Jul-04,ISS,Prime,Titan,2X2WIND,Wind observation,Titan T0 imaging,Surface/winds/clouds,,,,,, 2004-184T01:56:21,000T01:34:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_01,"Ride-along with ISS. Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, -x to sun.",,,,,, 2004-184T01:56:21,000T01:34:00,2-Jul-04,VIMS,SPASS Rider,Titan,SPOLEA,South pole campaign,Titan global mapping,"IR:32x64 double res, vis 32x32 single res; Titan global mapping of surface (south-polar area at 220 km/pxl)",,,,,, 2004-184T03:30:21,000T01:22:00,2-Jul-04,CIRS,Prime,Titan,TEMPMAP,Thermal map,CIRS_000TI_TEMPMAP038,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, -x aligned E/W toward sun (E-W slews)",,,,,, 2004-184T03:30:21,000T01:22:00,2-Jul-04,CIRS,SPASS Rider,Titan,TEMPMAP,Thermal map,CIRS_000_TI_TEMPMAP101,"ISS NAC support imaging, 2 images per integration (~2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2004-184T04:52:21,000T00:24:00,2-Jul-04,ISS,Prime,Titan,2X2WIND,Wind observation,Titan T0 imaging,Surface/winds/clouds,,,,,, 2004-184T04:52:21,000T00:24:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_011,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-184T04:52:21,000T00:24:00,2-Jul-04,VIMS,SPASS Rider,Titan,SPOLEA,South pole campaign,Titan global mapping,"Titan global mapping as a ridealong with ISS. 48 square double res images. If ISS is mosaicing, do 12 square.",,,,,, 2004-184T05:16:21,000T01:24:00,2-Jul-04,CIRS,Prime,Titan,TEMPMAP,Thermal map,CIRS_000TI_TEMPMAP042,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, -x aligned E/W toward sun (E-W slews)",,,,,, 2004-184T05:16:21,000T01:24:00,2-Jul-04,CIRS,SPASS Rider,Titan,TEMPMAP,Thermal map,CIRS_000_TI_TEMPMAP102,"ISS NAC support imaging, 2 images per integration (~2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2004-184T05:30:21,000T08:00:00,2-Jul-04,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T0 Flyby,"T0 is formally the first Titan encounter of the mission although the closest approach is at a very large distance of 338082 km. Because of the large flyby distance the emphasis is not on Titan science but on the exploration of the region around Titan's orbit. This is important in connection with an accurate definition of the external field contributions to the magnetic field measurements around Saturn closest approach, the prime objective of which is the determination od Saturn's internal magnetic field. NOTE: Data rate is composed of continuous 494 bps (8 vps) plus bursts of 1976 bps (32 vps). NOTE: This is the T0min request.",,,,,, 2004-184T06:40:21,000T00:24:00,2-Jul-04,ISS,Prime,Titan,2X2WIND,Wind observation,Titan T0 imaging,Surface/winds/clouds,,,,,, 2004-184T06:40:21,000T00:24:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_010,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-184T06:40:21,000T00:24:00,2-Jul-04,VIMS,SPASS Rider,Titan,SPOLEA,South pole campaign,Titan global mapping,"Titan global mapping as a ridealong with ISS. 48 square double res images. If ISS is mosaicing, do 12 square.",,,,,, 2004-184T07:04:21,000T01:26:00,2-Jul-04,CIRS,Prime,Titan,TEMPMAP,Thermal map,CIRS_000TI_TEMPMAP044,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, -x E/W toward sun (E-W slews)",,,,,, 2004-184T07:04:21,000T01:26:00,2-Jul-04,CIRS,SPASS Rider,Titan,TEMPMAP,Thermal map,CIRS_000_TI_TEMPMAP103,"ISS NAC support imaging, 2 images per integration (~2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2004-184T07:04:21,000T01:26:00,2-Jul-04,UVIS,SPASS Rider,Titan,TEMPMAP,Thermal map,UVIS Rider to CIRS TEMPMAP,UVIS Rider to CIRS TEMP Map,,,,,, 2004-184T07:32:10,000T00:58:11,2-Jul-04,MIMI,SPASS Rider,Titan,T0INBND,,MAPS 000TI(T0) Campaign,"Part of 000TI(T0) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-184T08:30:21,000T00:09:00,2-Jul-04,ISS,Prime,Titan,2X2WIND,Wind observation,Titan T0 imaging,Surface/winds/clouds,,,,,, 2004-184T08:30:21,000T00:09:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_004,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-184T08:30:21,000T02:00:00,2-Jul-04,MIMI,SPASS Rider,Titan,T0CLOSE,,MAPS 000TI(T0) Campaign,"Part of 000TI(T0) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-184T08:30:21,000T00:09:00,2-Jul-04,VIMS,SPASS Rider,Titan,SPOLEA,South pole campaign,Titan global mapping,"Titan global mapping as a ridealong with ISS. 48 square double res images. If ISS is mosaicing, do 12 square.",,,,,, 2004-184T08:39:21,000T00:51:00,2-Jul-04,VIMS,Prime,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #63","Titan Light Curve, Observation #63.Changes made 5/19/02 by Buratti as per TOST and ISS agreements.",,,,,, 2004-184T08:39:21,000T00:51:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_01,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-184T08:39:21,000T00:51:00,2-Jul-04,ISS,SPASS Rider,Titan,LIGHTC,Titan light curve,Titan T0 imaging,Photometry/polarimetry,,,,,, 2004-184T09:30:21,000T01:00:00,2-Jul-04,ISS,Prime,Titan,SPOLEB,South pole campaign,"Titan T0 2x3 mosaic, S pole",Turn -Y to Titan; do 2X3 mosaic with multiple NAC filters at each footprint,,,,,, 2004-184T09:30:21,000T01:00:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_01,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-184T09:30:21,000T01:00:00,2-Jul-04,VIMS,SPASS Rider,Titan,SPOLEB,South pole campaign,Titan global mapping,"IR:32x64 double res, vis 32x32 single res; Titan global mapping of surface (south-polar area at 170 km/pxl)",,,,,, 2004-184T10:00:00,012T02:55:00,2-Jul-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-184T10:30:21,000T04:00:00,2-Jul-04,CIRS,Prime,Titan,TEMPMAP,Thermal map,CIRS_000TI_TEMPMAP01,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, -X aligned E/W toward sun (E/W slews)",,,,,, 2004-184T10:30:21,000T04:00:00,2-Jul-04,CIRS,SPASS Rider,Titan,TEMPMAP,Thermal map,CIRS_000_TI_TEMPMAP104,"ISS NAC support imaging, 2 images per integration (~4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2004-184T10:30:21,000T04:00:00,2-Jul-04,ISS,SPASS Rider,Titan,TEMPMAP,Thermal map,Titan T0 imaging,Photometry/polarimetry,,,,,, 2004-184T10:30:21,000T01:01:49,2-Jul-04,MIMI,SPASS Rider,Titan,T0OUTBND,,MAPS 000TI(T0) Campaign,"Part of 000TI(T0) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-184T10:30:21,000T04:00:00,2-Jul-04,UVIS,SPASS Rider,Titan,TEMPMAP,Thermal map,UVIS Rider to CIRS TEMPMAP,UVIS Rider to CIRS TEMP Map,,,,,, 2004-184T10:30:21,000T04:00:00,2-Jul-04,VIMS,SPASS Rider,Titan,TEMPMAP,Thermal map,CIRS Temp Map,Titan global mapping as a ridealong with CIRS There will be pauses in mosaic for ISS/VIMS,,,,,, 2004-184T11:32:21,000T08:44:39,2-Jul-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-184T13:30:21,000T06:50:39,2-Jul-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps). NOTE: This is the T0min request.,,,,,, 2004-184T14:30:21,000T00:45:00,2-Jul-04,VIMS,Prime,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #62","Titan Light Curve, Observation #62. Changes made by Buratti as per TOST agreements.",,,,,, 2004-184T14:30:21,000T00:45:00,2-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_01,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-184T14:30:21,000T00:45:00,2-Jul-04,ISS,SPASS Rider,Titan,LIGHTC,Titan light curve,Titan T0 imaging,Photometry/polarimetry,,,,,, 2004-184T15:15:21,000T01:45:00,2-Jul-04,CIRS,Prime,Titan,TEMPMAP,Thermal map,CIRS_000TI_TEMPMAP01,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, -x aligned E/W toward sun (slews e/w)",,,,,, 2004-184T15:15:21,000T01:45:00,2-Jul-04,CIRS,SPASS Rider,Titan,TEMPMAP,Thermal map,CIRS_000_TI_TEMPMAP105,"ISS NAC support imaging, 2 images per integration (~2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2004-184T17:51:00,000T02:45:00,2-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-184T17:51:00,000T02:45:00,2-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-184T18:00:00,000T00:23:00,2-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-184T18:23:00,001T04:43:00,2-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-184T20:17:00,001T05:02:00,2-Jul-04,MIMI,SPASS Rider,co-rotation,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS MAGDYN Campaign,"Part of MAGDYN MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-184T20:17:00,002T02:49:00,2-Jul-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-184T20:17:00,001T02:49:00,2-Jul-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-184T20:21:00,001T02:45:00,2-Jul-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-184T20:36:00,000T01:24:00,2-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,OPNAV rider for deep space,Any pointing O.K. Deep space during OPNAV turns,,,,,, 2004-184T22:00:00,000T02:45:00,2-Jul-04,CIRS,Prime,rings(general),SHADLMP,Saturn ring shadow observation,CIRS_000RB_ShadLMP,"Longitudinal scan of ring in the early mission (highest temperature contrasts), in and around shadow, Low Phase, dawn side. -Y to ring, +Z perpendicular to rings (if not possible, +Z parallel to pole)",,,,,, 2004-184T22:00:00,000T02:45:00,2-Jul-04,CIRS,SPASS Rider,rings(general),SHADLMP,Saturn ring shadow observation,CIRS_000RI_SHADLMP_SI,"Support imaging for ring shadow observation, multiple scans",,,,,, 2004-185T01:00:00,000T02:15:00,3-Jul-04,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADIRCOMPINT_01,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 0.0. POINTING: -y to Titan, x away from sun PIC",,,,,, 2004-185T01:00:00,000T02:15:00,3-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000_TI_FIRNADCMP017,"ISS NAC support imaging, 2 images per integration (~2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2004-185T01:00:00,000T02:15:00,3-Jul-04,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging/Titan imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2004-185T03:15:00,000T00:45:00,3-Jul-04,VIMS,Prime,Titan,LIGHTC,Titan light curve,"Titan Light Curve, Obs #65","Titan Light Curve, Observation #65. Added 5/19/02 by Buratti as per TOST agreement.",,,,,, 2004-185T03:15:00,000T00:45:00,3-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADCMP_01,"Obtain information on CO, HCN, CH4. Integrate on disk. POINTING: -y to Titan, x away from sun.",,,,,, 2004-185T03:15:00,000T00:45:00,3-Jul-04,ISS,SPASS Rider,Titan,LIGHTC,Titan light curve,Titan T0 imaging,Photometry/polarimetry,,,,,, 2004-185T04:00:00,000T06:00:00,3-Jul-04,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000TI_FIRNADIRCOMPINT_01,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 0.0. POINTING: FP1 to Titan, x away from sun, PIC.",,,,,, 2004-185T04:00:00,000T06:00:00,3-Jul-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_000_TI_FIRNADCMP001,"ISS NAC support imaging, 2 images per integration (~4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2004-185T04:00:00,000T06:00:00,3-Jul-04,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging/Titan T0 imaging),Photometry/polarimetry,,,,,, 2004-185T04:00:00,000T06:00:00,3-Jul-04,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,UVIS Rider to CIRS Far Nadir Comp,UVIS Rider to CIRS Far-IR Nadir Comp,,,,,, 2004-185T04:00:00,000T06:00:00,3-Jul-04,VIMS,SPASS Rider,Titan,FARIRMAP,Far Infrared map,CIRS Far IR Map,Titan global mapping as a ridealong with CIRS There will be pauses in mosaic for ISS/VIMS,,,,,, 2004-185T10:00:00,000T01:00:00,3-Jul-04,ISS,Prime,Titan,1X2WIND,Wind observation,Titan T0 imaging,Surface/winds/clouds,,,,,, 2004-185T10:00:00,000T01:00:00,3-Jul-04,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,CIRS_013TI_MIDIRTMAP07,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, x to pole",,,,,, 2004-185T10:00:00,000T01:00:00,3-Jul-04,VIMS,SPASS Rider,Titan,MAP,,"Titan Light Curve, Obs #65","Ridealong with ISS Map. If they are doing NAC, take 12 X 12 high res., If WAC do 38 square high res.",,,,,, 2004-185T11:00:00,000T01:30:00,3-Jul-04,CIRS,SPASS Rider,Iapetus,MIDIRTMAP,Mid infrared thermal map,CIRS_013TI_MIDIRTMAP07,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, x to pole",,,,,, 2004-185T11:20:00,000T01:10:00,3-Jul-04,ISS,Prime,Iapetus,TERRAINCA,Terra incognita observation,Iapetus terra incognita (south hem) low phase obs,Turn -Y to Iapetus; Do 1x1 mosaic 2 NAC clear + 4 NAC color + 3 NAC polarizer filters; custom handoff to NAV at -Y to Iapetus,,,,,, 2004-185T14:06:00,000T09:00:00,3-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-185T15:00:00,000T06:00:00,3-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-185T23:06:00,000T01:25:00,3-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,OPNAV rider for deep space,Any pointing O.K. Deep space during OPNAV turns,,,,,, 2004-185T23:06:00,001T00:00:00,3-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-185T23:06:00,000T03:25:00,3-Jul-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-185T23:06:00,001T23:45:00,3-Jul-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-186T00:31:00,000T02:00:00,4-Jul-04,UVIS,Prime,rings(general),IMPACT,,,Use UVIS HSP and FUV to detect flashes from meter-sized interplanetary impactors on rings to constrain flux of important impact population for ring origin/evolution.,,,,,, 2004-186T00:31:00,000T02:00:00,4-Jul-04,CIRS,SPASS Rider,rings(general),URIMPACT,,CIRS_000RI_URIMPACT_SI,Support imaging for long integration on A ring and C rings,,,,,, 2004-186T00:31:00,000T02:00:00,4-Jul-04,CIRS,SPASS Rider,rings(general),URIMPACT,,CIRS_000_RI_URIMPACT rider with UVIS,"Ride with URIMPACT, staring at B ring shadow",,,,,, 2004-186T00:31:00,000T02:00:00,4-Jul-04,ISS,SPASS Rider,rings(general),IMPACT,,URIMPACT spoke and F ring images day 186,"WACs for F ring at beginning (R ansa), and during UVIS shadow stare (L ansa), and at end (R ansa) to catch emerging spokes. Added one dark current.",,,,,, 2004-186T00:31:00,000T02:00:00,4-Jul-04,VIMS,SPASS Rider,rings(general),IMPACT,,F Ring during UVIS impact observations,F Ring observations during UVIS searches for ring impacts.,,,,,, 2004-186T01:19:01,004T10:41:00,4-Jul-04,MIMI,SPASS Rider,co-rotation,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS MAGDYN Campaign,"Part of MAGDYN MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-186T02:31:00,000T10:10:00,4-Jul-04,CIRS,Prime,rings(general),COMP,Sit and stare to derive composition,CIRS_000RI_COMP,"Stare at West ansa, low phase, lit face, 5 hrs on C ring, 5 hrs on A ring -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-186T02:31:00,000T10:10:00,4-Jul-04,CIRS,SPASS Rider,rings(general),COMP,Sit and stare to derive composition,CIRS_000RI_COMP_SI,Support imaging for long integration on A ring and C rings,,,,,, 2004-186T02:31:00,000T05:00:00,4-Jul-04,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required. Includes 2 hours for IFC cal and range checks. First calibration after SOI.",,,,,, 2004-186T07:31:00,008T05:29:00,4-Jul-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-186T12:41:00,000T01:25:00,4-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,OPNAV rider for deep space,Any pointing O.K. Deep space during OPNAV turns,,,,,, 2004-186T14:06:00,000T09:00:00,4-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-186T23:06:00,006T23:30:00,4-Jul-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-186T23:06:00,000T00:23:00,4-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-186T23:29:00,002T00:31:00,4-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-186T23:36:00,000T04:14:00,4-Jul-04,ISS,Prime,Iapetus,TERRAINCC,Terra incognita observation,Iapetus terra incognita (south hem) low phase obs,Turn -Y to Iapetus; do 1x1 NAC mosaic 20 clear + 66 color + 18 polarizer + 15 WAC color filters; turn to WP,,,,,, 2004-186T23:36:00,000T04:14:00,4-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-186T23:36:00,000T01:00:00,4-Jul-04,VIMS,SPASS Rider,Iapetus,TERRAINCC,Terra incognita observation,Iapetus southern hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-187T13:51:00,000T09:00:00,5-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-187T14:45:00,000T06:00:00,5-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-187T22:51:00,005T14:45:00,5-Jul-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-188T14:00:00,000T06:00:00,6-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-189T00:00:00,000T00:23:00,7-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-189T00:23:00,001T23:37:00,7-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-189T09:00:00,000T06:00:00,7-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-190T12:00:00,004T01:00:00,8-Jul-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-191T00:00:00,000T00:23:00,9-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-191T00:23:00,001T23:37:00,9-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-193T00:00:00,000T00:23:00,11-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-193T00:23:00,001T23:37:00,11-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-193T13:36:00,000T23:24:00,11-Jul-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-193T13:36:00,000T09:00:00,11-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-193T14:45:00,000T06:00:00,11-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-193T22:36:00,000T14:24:00,11-Jul-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-194T13:00:00,002T00:08:00,12-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-194T13:00:00,002T00:00:00,12-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-194T13:00:00,002T00:07:00,12-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-194T13:00:00,002T00:02:00,12-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-194T13:36:00,000T09:00:00,12-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-194T14:45:00,000T06:00:00,12-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-195T00:00:00,000T00:23:00,13-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-195T00:06:00,000T01:00:00,13-Jul-04,ISS,Prime,Iapetus,SOUTHHEMB,Southern hemisphere imaging,Iapetus terra incognita (south hem) obs.,Turn -Y to Iapetus; Do 1x1 mosaic 2 NAC clear + 4 NAC color + 3 NAC polarizer filters; turn to WP.,,,,,, 2004-195T00:06:00,000T01:00:00,13-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-195T00:06:00,000T01:00:00,13-Jul-04,VIMS,SPASS Rider,Iapetus,SOUTHHEMB,Southern hemisphere imaging,Iapetus southern hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-195T00:23:00,001T12:34:00,13-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-195T01:06:00,000T04:25:00,13-Jul-04,UVIS,Prime,Saturn,MOS00WA,Apoapsis mosaic,MOSAIC_APO_01_21b,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to Saturn spin axis. 1) Slew about the Z-axis from Saturn center to +MOS orb. 2) Drift at a rate of .0156 mrad/sec about the Z-axis toward -MOS orb for 14000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/- range from Saturn Center): 123.77 mrad.",,,,,, 2004-195T06:06:00,000T09:00:00,13-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-195T16:31:00,000T10:30:00,13-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-195T16:31:00,000T10:30:00,13-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-195T16:31:00,000T10:30:00,13-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-196T03:01:00,000T03:25:00,14-Jul-04,UVIS,Prime,Saturn,MOS00WA,Apoapsis mosaic,MOSAIC_APO_01_21c,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS orb. 2) Drift at a rate of .0148 mrad/sec about the Z-axis towards +MOS orb for 11700s. 3) Slew Back to Saturn center and reset pointing. Stare for remaining observation time. MOS ORB (+/-range from Saturn Center): 117.92 mrad.",,,,,, 2004-196T06:26:00,000T05:00:00,14-Jul-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-196T06:26:00,000T05:00:00,14-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-196T06:26:00,000T05:00:00,14-Jul-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-196T12:54:00,000T00:06:00,14-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,SLEEP,Instrument to sleep mode,Sleep for Probe activity,sleep instrument,,,,,, 2004-196T12:55:00,000T09:49:00,14-Jul-04,CDA,SPASS Rider,Other,PCOMUTE,Mute instrument for Probe Checkout,Probe Checkout Mute,Sleep/Mute Unmute/Active for PCO,,,,,, 2004-196T12:56:00,000T00:17:00,14-Jul-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder for PCO14,"Put CIRS to sleep/mute for PCO#14 CIRS to sleep at epoch - 00:17, mute by epoch -00:06",,,,,, 2004-196T12:57:00,000T00:10:00,14-Jul-04,INMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,PCO 14 SLEEP,SLEEP/MUTE for PCO14,,,,,, 2004-196T12:58:00,000T00:09:50,14-Jul-04,ISS,Non-SPASS,Earth,SLEEPMUTE,Huygens probe support,put ISS to sleep for probe activity,placeholder activity put into CIMS to remenind ISS to go into sleep for probe activity at request of MAG TWT,,,,,, 2004-196T13:00:00,000T09:42:00,14-Jul-04,MIMI,SPASS Rider,co-rotation,PCOMUTE,Mute instrument for Probe Checkout,Probe Checkout Mute,SLEEP/MUTE for PCO,,,,,, 2004-196T13:02:00,000T09:49:00,14-Jul-04,RPWS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,RPWS Sleep and Mute for Probe activity,"RPWS sleep/mute for Probe activity, followed by unmute/sleep.",,,,,, 2004-196T13:04:00,000T00:03:00,14-Jul-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (PCO 14),UVIS to go to sleep/mute for PCO 14 (MGTWT request),,,,,, 2004-196T13:05:00,000T00:08:00,14-Jul-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE,VIMS to SLEEP/ MUTE for PCO14_PSAON,,,,,, 2004-196T13:07:00,000T00:01:00,14-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,MUTE,Instrument to sleep mode,Mute for Probe activity,mute biu,,,,,, 2004-196T13:07:00,000T09:35:00,14-Jul-04,INMS,Non-SPASS,SpacecraftActivity,MUTE,Instrument to sleep mode,PCO 14 MUTE,SLEEP/MUTE for PCO14,,,,,, 2004-196T13:07:00,000T09:35:00,14-Jul-04,MAG,Non-SPASS,SpacecraftActivity,PROBEMUTE,Huygens Probe support,Mute/Unmute for PCO14,"Mute instrument for probe patch load, unmute at end. NOTE: MAG does not go to sleep for probe activities, other instruments do",,,,,, 2004-196T13:13:00,000T09:23:00,14-Jul-04,PROBE,Non-SPASS,Earth,PCO14,Probe Checkout,Post-SOI Probe Checkout,"Regular Probe Checkout. X-band downlink required. The following Orbiter instruments will be ON, in sleep mode, and muted prior to PSA ON: CDA, CAPS, ISS, MIMI, RPWS, MAG, UVIS, and VIMS; other orbiter instruments OFF.",,,,,, 2004-196T22:42:00,001T01:34:00,14-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-196T22:42:00,000T00:01:00,14-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,UNMUTE,Huygens probe support,UnMute at Probe activity,unmute biu,,,,,, 2004-196T22:42:00,000T00:07:00,14-Jul-04,MIMI,SPASS Rider,co-rotation,PCOUNMUTE,Huygens probe support,Probe Checkout Mute,UNMUTE/ACTIVE after PCO UNMUTE at request start. Active 7 minutes later,,,,,, 2004-196T22:42:00,000T00:04:00,14-Jul-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,wake/unmute placeholder for PCO14,"UNMUTE. Note power transients! unmute at 00:06, wake at epoch+00:09",,,,,, 2004-196T22:42:00,000T00:04:00,14-Jul-04,INMS,Non-SPASS,SpacecraftActivity,UNMUTE,Huygens probe support,PCO 14 UNMUTE,SLEEP/MUTE for PCO14,,,,,, 2004-196T22:42:00,000T00:07:00,14-Jul-04,ISS,Non-SPASS,Earth,WAKESLEEP,Wakeup instrument from sleep mode,wake up ISS after probe activity,placeholder activity put into CIMS to remind ISS to wake up after probe activity at request of MAG TWT,,,,,, 2004-196T22:42:00,001T16:09:00,14-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-196T22:42:00,000T00:11:00,14-Jul-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after PCO 14,Unmute/go to active after PCO 14 (MAGTWT request),,,,,, 2004-196T22:42:00,000T00:15:00,14-Jul-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode,VIMS to UnMute and Active at PCO14_PSAOFF,,,,,, 2004-196T22:43:00,000T02:16:00,14-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,WakeUp at Probe activity,wake up,,,,,, 2004-196T22:43:00,000T02:16:00,14-Jul-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,WakeUp at Probe activity,wake up,,,,,, 2004-196T22:44:00,001T16:07:00,14-Jul-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-196T22:46:00,000T00:23:00,14-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,Ride with prime instrument,,,,,, 2004-196T22:49:00,001T16:02:00,14-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-196T22:51:00,001T16:00:00,14-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-196T23:09:00,001T23:51:00,14-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-197T01:26:00,000T00:55:00,15-Jul-04,UVIS,Prime,Saturn,MOS00WA,Apoapsis mosaic,MOSAIC_APO_01_05,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew from Saturn Center about the Z-axis to +MOS orb. 2) Drift at a rate of .0143 mrad/sec about the Z-axis towards -MOS orb for 3000S. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS ORB (+/- range from Saturn Center): 113.77 mrad.",,,,,, 2004-197T02:21:00,000T10:30:00,15-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-197T02:21:00,000T10:30:00,15-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-197T13:21:00,000T09:00:00,15-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-197T23:51:00,000T01:00:00,15-Jul-04,ISS,Prime,Iapetus,SOUTHHEME,Southern hemisphere imaging,Iapetus terra incognita (south hem) obs.,Turn -Y to Iapetus; Do 1x1 mosaic 2 NAC clear + 4 NAC color + 3 NAC polarizer filters,,,,,, 2004-197T23:51:00,000T01:00:00,15-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-197T23:51:00,000T01:00:00,15-Jul-04,VIMS,SPASS Rider,Iapetus,SOUTHHEME,Southern hemisphere imaging,Iapetus southern hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-198T00:06:00,004T21:26:00,16-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-198T00:51:00,000T04:25:00,16-Jul-04,UVIS,Prime,Saturn,MOS00WB,Apoapsis mosaic,MOSAIC_APO_01_05a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn center to +MOS orb and rotate +64 mrad in the YZ plane. 2) Drift at a rate of .0424 mrad/sec about the Z-axis toward -MOS orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS ORB (+/- range): 318.29 mrad",,,,,, 2004-198T05:51:00,000T09:00:00,16-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-198T14:51:00,008T23:31:00,16-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-198T14:51:00,008T23:31:00,16-Jul-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-198T14:51:00,003T00:00:00,16-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-198T14:51:00,003T00:00:00,16-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-198T16:16:00,000T10:30:00,16-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-198T16:16:00,000T10:30:00,16-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-198T16:16:00,000T10:30:00,16-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-198T16:30:00,000T04:33:30,16-Jul-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 2000 bps from SWSKR.,,,,,, 2004-198T23:00:00,000T00:23:00,16-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-198T23:23:00,000T22:58:00,16-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-199T02:46:00,000T04:55:00,17-Jul-04,UVIS,Prime,Saturn,MOS00WB,Apoapsis mosaic,MOSAIC_APO_01_05b,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS orb. 2) Drift at a rate of .0410 mrad/sec about the Z-axis toward -MOS orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS ORB (+/- RANGE): 307.25 mrad.",,,,,, 2004-199T07:41:00,000T05:00:00,17-Jul-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-199T07:41:00,000T05:00:00,17-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-199T07:41:00,000T05:00:00,17-Jul-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-199T13:21:00,000T09:00:00,17-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-199T22:21:00,001T00:00:00,17-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-199T23:41:00,000T02:25:00,17-Jul-04,UVIS,Prime,Saturn,MOS00WB,Apoapsis mosaic,MOSAIC_APO_01_05c,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS orb and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0399 mrad/sec about the Z-axis in the direction toward -MOS orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/- range): 299.22 mrad",,,,,, 2004-200T02:06:00,000T10:30:00,18-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-200T02:06:00,000T10:30:00,18-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-200T13:21:00,000T09:00:00,18-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-200T22:21:00,000T00:23:00,18-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-200T22:44:00,001T23:37:00,18-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-200T23:51:00,000T01:00:00,18-Jul-04,ISS,Prime,Iapetus,SOUTHHEMH,Southern hemisphere imaging,Iapetus terra incognita (south hem) obs.,Turn -Y to Iapetus; Do 1x1 mosaic 8 NAC clear + 9 NAC color + 6 NAC polarizer + 15 WAC color filters,,,,,, 2004-200T23:51:00,000T01:00:00,18-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-200T23:51:00,000T01:00:00,18-Jul-04,VIMS,SPASS Rider,Iapetus,SOUTHHEMH,Southern hemisphere imaging,Iapetus southern hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-201T00:51:00,000T04:25:00,19-Jul-04,UVIS,Prime,Saturn,MOS00WC,Apoapsis mosaic,MOSAIC_APO_01_05d,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS orb and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0387 mrad/sec about the Z-axis toward +MOS orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/- range): 290.44 mrad.",,,,,, 2004-201T05:51:00,000T09:00:00,19-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-201T14:51:00,002T23:45:00,19-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-201T14:51:00,002T23:45:00,19-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-201T16:16:00,000T10:30:00,19-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-201T16:16:00,000T10:30:00,19-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-201T16:16:00,000T10:30:00,19-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-201T16:30:00,000T04:33:30,19-Jul-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 2000 bps from SWSKR.,,,,,, 2004-202T02:46:00,000T04:55:00,20-Jul-04,UVIS,Prime,Saturn,MOS00WC,Apoapsis mosaic,MOSAIC_APO_01_06,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn center to -MOS orb. 2) Drift at a rate of .0376 mrad/sec about the Z-axis to +MOS orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/- range): 282.29 mrad.",,,,,, 2004-202T02:46:00,000T09:55:00,20-Jul-04,VIMS,SPASS Rider,Saturn,SATURN,Saturn global map,,Saturn Global,,,,,, 2004-202T07:41:00,000T05:00:00,20-Jul-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-202T07:41:00,000T05:00:00,20-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-202T07:41:00,000T05:00:00,20-Jul-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-202T13:06:00,000T09:00:00,20-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-202T14:41:00,000T06:00:00,20-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-202T21:32:00,004T16:50:00,20-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-202T22:21:00,000T00:23:00,20-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-202T22:44:00,001T23:37:00,20-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-202T23:41:00,000T02:25:00,20-Jul-04,UVIS,Prime,Saturn,MOS00WC,Apoapsis mosaic,MOSAIC_APO_01_06a,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS orb and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0368 mrad/sec about the Z-axis toward +MOS orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS ORB (+/- range): 276.28 mrad.",,,,,, 2004-203T02:06:00,000T10:30:00,21-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-203T02:06:00,000T10:30:00,21-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-203T13:06:00,000T09:00:00,21-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-203T23:36:00,000T01:00:00,21-Jul-04,ISS,Prime,Iapetus,SOUTHHEMK,Southern hemisphere imaging,Iapetus terra incognita (south hem) obs.,Turn -Y to Iapetus; Do 1x1 mosaic NAC clear + 4 NAC color + NAC polarizer filters.,,,,,, 2004-203T23:36:00,000T01:00:00,21-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-204T00:36:00,000T04:25:00,22-Jul-04,UVIS,Prime,Saturn,MOS00WD,Apoapsis mosaic,MOSAIC_APO_01_06b,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn center to +MOS orb. 2) Drift at a rate of .0360 mrad/sec about the Z-axis toward -MOS orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/- range): 269.70.",,,,,, 2004-204T05:36:00,000T09:00:00,22-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-204T14:36:00,002T23:46:00,22-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-204T14:36:00,002T23:46:00,22-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-204T16:01:00,000T10:30:00,22-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-204T16:01:00,000T10:30:00,22-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-204T16:01:00,000T10:30:00,22-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-204T16:30:00,000T06:51:00,22-Jul-04,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). 96 B cycles duration. Data is in addition to 2000 bps from SWSKR.,,,,,, 2004-204T22:21:00,000T00:23:00,22-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-204T22:44:00,001T23:37:00,22-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-205T02:31:00,000T04:55:00,23-Jul-04,UVIS,Prime,Saturn,MOS00WD,Apoapsis mosaic,MOSAIC_APO_01_06c,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z axis to +MOS orb and rotate -64mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0351 mrad/sec about the Z-axis toward -MOS orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/- range): 263.45 mrad.",,,,,, 2004-205T02:31:00,000T09:55:00,23-Jul-04,VIMS,SPASS Rider,Saturn,SATURN,Saturn global map,,Saturn Far Encounter Global Mosaic #5,,,,,, 2004-205T07:26:00,000T05:00:00,23-Jul-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-205T07:26:00,000T05:00:00,23-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-205T07:26:00,000T05:00:00,23-Jul-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-205T12:52:00,000T09:00:00,23-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-205T14:26:00,000T06:00:00,23-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-205T23:26:00,000T02:25:00,23-Jul-04,UVIS,Prime,Saturn,MOS00WD,Apoapsis mosaic,MOSAIC_APO_01_06d,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS ORB and rotate +64 mrad in the YZ plane from Saturn Center 2) Drift at a rate of .0345 mrad/sec about the Z-axis in the direction of -MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 258.81 mrad",,,,,, 2004-206T01:51:00,000T10:30:00,24-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-206T01:51:00,000T10:30:00,24-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-206T12:52:00,000T09:00:00,24-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-206T22:21:00,000T00:23:00,24-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-206T22:44:00,001T23:37:00,24-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-206T23:22:00,000T01:00:00,24-Jul-04,ISS,Prime,Iapetus,SOUTHHEMN,Southern hemisphere imaging,Iapetus terra incognita (south hem) obs.,Turn -Y to Iapetus; Do 1x1 mosaic NAC clear + NAC color + NAC polarizer filters,,,,,, 2004-206T23:22:00,000T01:00:00,24-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-207T00:22:00,000T04:25:00,25-Jul-04,UVIS,Prime,Saturn,MOS00WE,Apoapsis mosaic,MOSAIC_APO_01_06e,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned with Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center 2) Drift at a rate of .0338 mrad/sec about the Z-axis in the direction of +MOS orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/- Range): 253.67 mrad",,,,,, 2004-207T05:22:00,000T09:00:00,25-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-207T14:22:00,004T13:10:00,25-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-207T14:22:00,002T23:45:00,25-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-207T14:22:00,005T07:09:59,25-Jul-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,new (sponge bits),"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-207T14:22:00,004T13:10:00,25-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-207T14:22:00,004T13:10:00,25-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-207T15:47:00,000T10:30:00,25-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-207T15:47:00,000T10:30:00,25-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-207T15:47:00,000T10:30:00,25-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-208T02:17:00,000T04:55:00,26-Jul-04,UVIS,Prime,Saturn,MOS00WE,Apoapsis mosaic,MOSAIC_APO_01_06f,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb and -64 mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0332 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 248.77 mrad.",,,,,, 2004-208T07:12:00,000T05:00:00,26-Jul-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-208T07:12:00,000T05:00:00,26-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-208T07:12:00,000T05:00:00,26-Jul-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-208T12:52:00,000T09:00:00,26-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-208T14:12:00,000T06:00:00,26-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-208T22:21:00,000T00:23:00,26-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-208T22:44:00,001T23:37:00,26-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-208T23:12:00,000T02:25:00,26-Jul-04,UVIS,Prime,Saturn,MOS00WE,Apoapsis mosaic,MOSAIC_APO_01_06g,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to Saturn spin axis. 1) Slew about Z to -MOS Orb and rotate +64mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0327 mrad/sec about the Z-axis toward +MOS orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 245.09 mrad.",,,,,, 2004-209T01:37:00,000T10:30:00,27-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-209T01:37:00,000T10:30:00,27-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-209T12:52:00,000T09:00:00,27-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-209T23:22:00,000T01:00:00,27-Jul-04,ISS,Prime,Iapetus,TRAILSIDA,Satellite trail side imaging,Iapetus early trailing side obs.,Turn -Y to Iapetus; Do 1x1 mosaic 2 NAC clear filters; Turn to WP.,,,,,, 2004-209T23:22:00,000T01:00:00,27-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-210T00:22:00,000T04:25:00,28-Jul-04,UVIS,Prime,Saturn,MOS00WF,Apoapsis mosaic,MOSAIC_APO_01_06h,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb and rotate -64mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0321 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/- Range): 240.97 mrad",,,,,, 2004-210T05:07:00,000T09:00:00,28-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-210T14:07:00,001T13:25:00,28-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-210T15:47:00,000T10:30:00,28-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-210T15:47:00,000T10:30:00,28-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-210T15:47:00,000T10:30:00,28-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-210T22:21:00,000T00:23:00,28-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-210T22:44:00,001T22:25:00,28-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-211T02:17:00,000T04:55:00,29-Jul-04,UVIS,Prime,Saturn,MOS00WF,Apoapsis mosaic,MOSAIC_APO_01_06i,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0316 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/- Range): 237.05mrad",,,,,, 2004-211T07:12:00,000T05:00:00,29-Jul-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-211T07:12:00,000T05:00:00,29-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-211T07:12:00,000T05:00:00,29-Jul-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-211T12:12:00,000T02:25:00,29-Jul-04,UVIS,Prime,Saturn,MOS00WF,Apoapsis mosaic,MOSAIC_APO_01_06l,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb and rotate +64mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0312 mrad/sec about the Z-axis toward -MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 234.10mrad",,,,,, 2004-211T14:37:00,000T10:30:00,29-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-211T14:37:00,000T10:30:00,29-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-212T03:32:00,000T18:00:00,30-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-212T03:32:00,000T18:00:00,30-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-212T03:32:00,000T18:00:00,30-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-212T03:32:00,000T18:00:00,30-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-212T03:32:00,000T09:00:00,30-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-212T05:32:00,000T06:00:00,30-Jul-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-212T12:32:00,000T09:00:00,30-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-212T21:09:00,000T00:23:00,30-Jul-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,Memory Dump,Ride with prime instrument,,,,,, 2004-212T21:32:00,005T14:01:00,30-Jul-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-212T21:32:00,001T13:20:00,30-Jul-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-212T21:32:00,027T18:41:00,30-Jul-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,"prograde dust, day 174: -z2E and -x 26.9; -24.6 AM=42 (60deg from +x2NEP) geometry changes fast, -x pointing only valid at beginning in the first days.",,,,,, 2004-212T21:32:00,000T01:22:00,30-Jul-04,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,STARTUP,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2004-212T21:32:00,001T13:20:00,30-Jul-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-212T21:32:00,001T13:20:00,30-Jul-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-212T22:54:00,005T00:06:00,30-Jul-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-212T23:07:00,000T01:00:00,30-Jul-04,ISS,Prime,Iapetus,TRAILSIDB,Satellite trail side imaging,Iapetus early trailing side obs.,Turn -Y to Iapetus; Do 1x1 mosaic 3 NAC clear filters,,,,,, 2004-212T23:07:00,000T01:00:00,30-Jul-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-213T00:07:00,000T04:25:00,31-Jul-04,UVIS,Prime,Saturn,MOS00WG,Apoapsis mosaic,MOSAIC_APO_01_06M,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb and rotate -64mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0308 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-range): 230.81mrad.",,,,,, 2004-213T05:07:00,000T09:00:00,31-Jul-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-213T15:32:00,000T10:30:00,31-Jul-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-213T15:32:00,000T10:30:00,31-Jul-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-213T15:32:00,000T10:30:00,31-Jul-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-214T02:02:00,000T04:55:00,1-Aug-04,UVIS,Prime,Saturn,MOS00WG,Apoapsis mosaic,MOSAIC_APO_01_06n,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center. 2) Drift at a rate of .0304 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 227.64mrad.",,,,,, 2004-214T06:57:00,000T03:25:00,1-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-214T06:57:00,000T03:25:00,1-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-214T06:57:00,000T03:25:00,1-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-214T10:52:00,004T17:45:00,1-Aug-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-214T10:52:00,004T17:45:00,1-Aug-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-214T10:52:00,004T17:45:00,1-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-214T10:52:00,000T12:00:00,1-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-214T13:57:00,000T06:00:00,1-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-214T22:52:00,000T02:00:00,1-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-215T01:22:00,000T09:00:00,2-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-215T01:22:00,000T09:00:00,2-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-215T01:22:00,000T09:00:00,2-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-215T10:52:00,000T06:00:00,2-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-215T10:52:00,000T06:00:00,2-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-216T00:22:00,000T01:00:00,3-Aug-04,ISS,Prime,Iapetus,TRAILSIDC,Satellite trail side imaging,Iapetus early trailing side obs.,Turn -Y to Iapetus; Do 1x1 mosaic 3 NAC clear filters; turn to WP,,,,,, 2004-216T00:22:00,000T01:00:00,3-Aug-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-216T01:22:00,000T01:30:00,3-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 006 TH OBSERVATIO","DIFFUSE RINGS IN REV 000, GO WEST TEMPLATE DOY 215-218",,,,,, 2004-216T03:22:00,000T12:00:00,3-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-216T16:52:00,000T09:30:00,3-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-216T16:52:00,000T09:30:00,3-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-216T16:52:00,000T09:30:00,3-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-217T02:22:00,000T08:42:00,4-Aug-04,UVIS,Prime,Saturn,MOS00WH,Apoapsis mosaic,MOSAIC_APO_01_06q,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb and rotate +64mrad in the YZ plane from Saturn Center. 2) Drift at a rate of .0293 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Rotate -64mrad in the YZ Plane. Drift at the indicated rate about Z for 15000s toward +MOS Orb. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 220.02mrad",,,,,, 2004-217T11:52:00,000T11:30:00,4-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-217T13:42:00,000T06:00:00,4-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-217T23:00:00,000T00:33:00,4-Aug-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-217T23:33:00,001T15:34:00,4-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-218T00:52:00,000T09:30:00,5-Aug-04,ISS,Prime,Star,CALSTARA,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2004-218T00:52:00,000T09:10:00,5-Aug-04,CAPS,SPASS Rider,InstrumentCalibration,CALIBRATE,Calibration,CAPS Calibration,"CAPS periodic gain test and calibration. The specified rate and data volume are the delta above the CAPS solar wind campaign rate (2000 bps), and the rate is the average over the entire request (current plans are to conduct the test in two different rates.)",,,,,, 2004-218T10:52:00,000T12:00:00,5-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-218T11:33:00,000T17:04:00,5-Aug-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-219T00:22:00,000T03:45:00,6-Aug-04,ISS,Prime,Phoebe,040PHO,Spectrophotometry,Phoebe Spectrophotometry and Multi-Color,Do during 0.4 Phoebe rotations 5 1x1 mosaics (109 images),,,,,, 2004-219T00:22:00,000T03:45:00,6-Aug-04,UVIS,SPASS Rider,Phoebe,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-219T04:37:00,000T09:00:00,6-Aug-04,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind while ORS instruments simultaneously observer Saturn's aurora,,,,,, 2004-219T04:37:00,000T09:00:00,6-Aug-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-219T04:37:00,000T09:00:00,6-Aug-04,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,MAPS SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2004-219T04:37:00,000T09:00:00,6-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-219T04:37:00,000T09:00:00,6-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-219T13:37:00,021T02:39:00,6-Aug-04,CAPS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS solar wind/aurora campaign,MAPS magnetospheric survey,,,,,, 2004-219T13:37:00,000T01:30:00,6-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-219T13:37:00,000T09:47:00,6-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-219T13:37:01,000T09:47:00,6-Aug-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-219T15:07:00,000T02:00:00,6-Aug-04,UVIS,Prime,Star,ALPVIR,Alpha Virginis occultation,USTRCAL02,INSTANCE OF USTRCAL02. Stellar Calibration: alpha Virginis,,,,,, 2004-219T15:07:00,000T02:00:00,6-Aug-04,ISS,SPASS Rider,Star,ALPVIR,Alpha Virginis occultation,ISS Sensitivity monitor,Periodic standard star image to monitor ISS sensitivity,,,,,, 2004-219T15:07:00,003T07:53:00,6-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-219T15:07:00,000T07:53:00,6-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-219T15:30:00,000T09:06:08,6-Aug-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 128 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2004-219T17:07:00,000T10:55:00,6-Aug-04,CIRS,Prime,Saturn,MIRCMPSIT,Sit and stare to derive composition,CIRS_000SA_MIRCMPSIT,"Measure oxygen compounds (CO2) in stratosphere as a function of latitude to determine whether rings are the source. Search for new stratospheric hydrocarbons (C3H4, C4H2). Determine isotopic ratios (CH3D/CH4, 12C/13C). FP3/4 to Saturn. Z parallel to Saturn pole direction.",,,,,, 2004-219T17:07:00,000T10:55:00,6-Aug-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,Saturn Far Global Mosaic Early Start,Saturn Far Encounter Global Mosaic. Ride-along with CIRS.,,,,,, 2004-219T23:00:00,000T05:00:00,6-Aug-04,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required. Includes 2 hours for IFC cal and range checks.",,,,,, 2004-219T23:24:00,020T16:51:00,6-Aug-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-219T23:24:00,000T14:13:00,6-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-220T04:00:00,000T09:37:00,7-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-220T04:37:00,000T09:00:00,7-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-220T06:07:00,000T06:00:00,7-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Saturn south pole,,,,,, 2004-220T13:37:00,008T07:01:00,7-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-220T13:37:00,008T07:01:00,7-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-220T15:17:00,000T10:30:00,7-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-220T15:17:00,000T10:30:00,7-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-220T15:17:00,000T10:30:00,7-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-220T15:17:00,000T10:30:00,7-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #16,Saturn Far Encounter Global Mosaic #7,,,,,, 2004-221T01:47:00,000T04:55:00,8-Aug-04,UVIS,Prime,Saturn,MOS00SWAA,Apoapsis mosaic,MOSAIC_APO_01_07,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0283 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 212.03mrad",,,,,, 2004-221T06:42:00,000T05:00:00,8-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-221T06:42:00,000T05:00:00,8-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-221T06:42:00,000T05:00:00,8-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-221T06:42:00,000T05:00:00,8-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #8,Saturn Far Encounter Global Mosaic #8,,,,,, 2004-221T12:12:00,000T08:55:00,8-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-221T13:42:00,000T06:00:00,8-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Saturn South Pole Template,Deep Space Cal,,,,,, 2004-221T22:42:00,000T02:25:00,8-Aug-04,UVIS,Prime,Saturn,MOS00SWAA,Apoapsis mosaic,MOSAIC_APO_01_07a,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0281 mrad/sec about the Z-axis toward -MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 210.57mrad",,,,,, 2004-222T01:07:00,000T10:30:00,9-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-222T01:07:00,000T10:30:00,9-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-222T01:07:00,000T10:30:00,9-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #9,Saturn Far Encounter Global Mosaic #9,,,,,, 2004-222T12:07:00,000T09:00:00,9-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-222T22:37:00,000T01:00:00,9-Aug-04,ISS,Prime,Iapetus,TRAILSIDE,Satellite trail side imaging,Iapetus early trailing side obs.,Turn -Y to Iapetus; Do 1x1 mosaic 3 NAC clear filters,,,,,, 2004-222T22:37:00,000T01:00:00,9-Aug-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-222T23:00:00,000T00:33:00,9-Aug-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-222T23:33:00,004T23:27:00,9-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-222T23:37:00,000T04:25:00,9-Aug-04,UVIS,Prime,Saturn,MOS00SWAB,Apoapsis mosaic,MOSAIC_APO_01_07b,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0279 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 208.94mrad",,,,,, 2004-222T23:37:00,000T04:25:00,9-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAB,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-223T04:32:00,000T08:50:00,10-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-223T15:02:00,000T10:30:00,10-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-223T15:02:00,000T10:30:00,10-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-223T15:02:00,000T10:30:00,10-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-223T15:02:00,000T10:30:00,10-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #10,Saturn Far Encounter Global Mosaic #10,,,,,, 2004-224T01:32:00,000T04:55:00,11-Aug-04,UVIS,Prime,Saturn,MOS00SWAB,Apoapsis mosaic,MOSAIC_APO_01_07c,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center. 2) Drift at a rate of .0277 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb(+/-Range): 207.39mrad.",,,,,, 2004-224T01:32:00,000T04:55:00,11-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAB,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-224T06:27:00,000T05:00:00,11-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-224T06:27:00,000T05:00:00,11-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-224T06:27:00,000T05:00:00,11-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-224T06:27:00,000T05:00:00,11-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #11,Saturn Far Encounter Global Mosaic #11,,,,,, 2004-224T11:57:00,000T08:55:00,11-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-224T13:27:00,000T06:00:00,11-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Saturn South Pole Template,Deep Space Cal,,,,,, 2004-224T22:27:00,000T02:25:00,11-Aug-04,UVIS,Prime,Saturn,MOS00SWAB,Apoapsis mosaic,MOSAIC_APO_01_07d,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0277 mrad/sec about the Z-axis toward +MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 204.93mrad",,,,,, 2004-225T00:52:00,000T10:30:00,12-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-225T00:52:00,000T10:30:00,12-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-225T00:52:00,000T10:30:00,12-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #12,Saturn Far Encounter Global Mosaic #12,,,,,, 2004-225T11:52:00,000T09:00:00,12-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-225T22:22:00,000T01:00:00,12-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 001 TH OBSERVATIO","DIFFUSE RINGS IN REV 000, GO WEST TEMPLATE",,,,,, 2004-225T22:22:00,000T01:00:00,12-Aug-04,CIRS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,"Diffuse Rings, Go West Template Ridealong","Ridealong on ISS diffuse rings, Go West Template",,,,,, 2004-225T23:22:00,000T04:25:00,12-Aug-04,UVIS,Prime,Saturn,MOS00SWAC,Apoapsis mosaic,MOSAIC_APO_01_07e,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0273 mrad/sec about the Z-axis towarad -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 204.93mrad",,,,,, 2004-225T23:22:00,000T04:25:00,12-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAC,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-226T04:17:00,000T09:00:00,13-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-226T14:47:00,000T10:30:00,13-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-226T14:47:00,000T10:30:00,13-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-226T14:47:00,000T10:30:00,13-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-226T14:47:00,000T10:30:00,13-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #13,Saturn Far Encounter Global Mosaic #13,,,,,, 2004-227T01:17:00,000T04:55:00,14-Aug-04,UVIS,Prime,Saturn,MOS00SWAC,Apoapsis mosaic,MOSAIC_APO_01_07f,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0271 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 203.70mrad.",,,,,, 2004-227T01:17:00,000T04:55:00,14-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAC,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-227T06:12:00,000T05:00:00,14-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-227T06:12:00,000T05:00:00,14-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-227T06:12:00,000T05:00:00,14-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-227T06:12:00,000T05:00:00,14-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #14,Saturn Far Encounter Global Mosaic #14,,,,,, 2004-227T11:42:00,000T09:00:00,14-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-227T13:12:00,000T06:00:00,14-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Saturn South Pole Template,Deep Space Cal,,,,,, 2004-227T22:12:00,000T02:25:00,14-Aug-04,UVIS,Prime,Saturn,MOS00SWAC,Apoapsis mosaic,MOSAIC_APO_01_07g,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0270 mrad/sec about the Z-axis toward -MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 202.79mrad.",,,,,, 2004-227T23:00:00,000T00:33:00,14-Aug-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-227T23:33:00,004T23:27:00,14-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-228T00:37:00,000T10:30:00,15-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-228T00:37:00,000T10:30:00,15-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-228T00:37:00,000T10:30:00,15-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #15,Saturn Far Encounter Global Mosaic #15,,,,,, 2004-228T11:38:00,000T09:00:00,15-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-228T20:38:00,000T16:25:00,15-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-228T20:38:00,000T16:25:00,15-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-228T22:08:00,000T01:00:00,15-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 002 TH OBSERVATIO","DIFFUSE RINGS IN REV 000, GO WEST TEMPLATE",,,,,, 2004-228T22:08:00,000T01:00:00,15-Aug-04,CIRS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,"Diffuse Rings, Go West Template Ridealong","Ridealong on ISS diffuse rings, Go West Template",,,,,, 2004-228T22:30:00,000T06:49:36,15-Aug-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 96 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2004-228T23:08:00,000T04:25:00,15-Aug-04,UVIS,Prime,Saturn,MOS00SWAD,Apoapsis mosaic,MOSAIC_APO_01_07h,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center. 2) Drift at a rate of .0269 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 201.79mrad.",,,,,, 2004-228T23:08:00,000T04:25:00,15-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAD,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-229T04:03:00,000T09:00:00,16-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-229T05:33:00,000T06:00:00,16-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep Space Cal,,,,,, 2004-229T13:03:00,005T07:20:00,16-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-229T13:03:00,005T07:20:00,16-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-229T14:33:00,000T10:30:00,16-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-229T14:33:00,000T10:30:00,16-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-229T14:33:00,000T10:30:00,16-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-229T14:33:00,000T10:30:00,16-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #16,Saturn Far Encounter Global Mosaic #16,,,,,, 2004-230T01:03:00,000T04:55:00,17-Aug-04,UVIS,Prime,Saturn,MOS00SWAD,Apoapsis mosaic,MOSAIC_APO_01_07i,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn center and rotate -64mrad in YZ plane. 2) Drift at a rate of .0268 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb(+/-Range): 200.85mrad.",,,,,, 2004-230T01:03:00,000T04:55:00,17-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAD,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-230T05:58:00,000T05:00:00,17-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-230T05:58:00,000T05:00:00,17-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-230T05:58:00,000T05:00:00,17-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-230T05:58:00,000T05:00:00,17-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #17,Saturn Far Encounter Global Mosaic #17,,,,,, 2004-230T11:28:00,000T09:00:00,17-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-230T12:58:00,000T06:00:00,17-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Saturn South Pole Template,Deep Space Cal,,,,,, 2004-230T21:58:00,000T02:25:00,17-Aug-04,UVIS,Prime,Saturn,MOS00SWAD,Apoapsis mosaic,MOSAIC_APO_01_07j,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0268 mrad/sec about the Z-axis toward +MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-range): 200.16mrad.",,,,,, 2004-231T00:23:00,000T10:30:00,18-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-231T00:23:00,000T10:30:00,18-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-231T00:23:00,000T10:30:00,18-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #18,Saturn Far Encounter Global Mosaic #18,,,,,, 2004-231T11:38:00,000T09:00:00,18-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-231T22:08:00,000T01:00:00,18-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 003 TH OBSERVATIO","DIFFUSE RINGS IN REV 000, GO WEST TEMPLATE",,,,,, 2004-231T22:08:00,000T01:00:00,18-Aug-04,CIRS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,"Diffuse Rings, Go West Template Ridealong","Ridealong on ISS diffuse rings, Go West Template",,,,,, 2004-231T23:08:00,000T04:25:00,18-Aug-04,UVIS,Prime,Saturn,MOS00SWAE,Apoapsis mosaic,MOSAIC_APO_01,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .027 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 199.43mrad",,,,,, 2004-231T23:08:00,000T04:25:00,18-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAE,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-232T04:03:00,000T08:50:00,19-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-232T14:33:00,000T10:30:00,19-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-232T14:33:00,000T10:30:00,19-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-232T14:33:00,000T10:30:00,19-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-232T14:33:00,000T10:30:00,19-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #19,Saturn Far Encounter Global Mosaic #19,,,,,, 2004-232T23:00:00,000T00:33:00,19-Aug-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-232T23:33:00,003T22:20:00,19-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-233T01:03:00,000T04:55:00,20-Aug-04,UVIS,Prime,Saturn,MOS00SWAE,Apoapsis mosaic,MOSAIC_APO_01,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0265 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 198.76mrad.",,,,,, 2004-233T01:03:00,000T04:55:00,20-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWAE,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-233T05:58:00,000T05:00:00,20-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-233T05:58:00,000T05:00:00,20-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-233T05:58:00,000T05:00:00,20-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-233T05:58:00,000T05:00:00,20-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #20,Saturn Far Encounter Global Mosaic #20,,,,,, 2004-233T11:28:00,000T08:55:00,20-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-233T12:58:00,000T06:00:00,20-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Saturn South Pole Template,Deep Space Cal,,,,,, 2004-233T21:58:00,000T02:25:00,20-Aug-04,UVIS,Prime,Saturn,MOS00SWAE,Apoapsis mosaic,MOSAIC_APO_01,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0264 mrad/sec about the Z-axis toward -MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 198.29mrad.",,,,,, 2004-234T00:23:00,000T10:30:00,21-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-234T00:23:00,000T10:30:00,21-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-234T00:23:00,000T10:30:00,21-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #21,Saturn Far Encounter Global Mosaic #21,,,,,, 2004-234T11:23:00,000T09:00:00,21-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-234T20:23:00,000T16:30:00,21-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-234T20:23:00,000T16:30:00,21-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-234T21:53:00,000T01:00:00,21-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 004 TH OBSERVATIO","DIFFUSE RINGS IN REV 000, GO WEST TEMPLATE",,,,,, 2004-234T21:53:00,000T01:00:00,21-Aug-04,CIRS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,"Diffuse Rings, Go West Template Ridealong","Ridealong on ISS diffuse rings, Go West Template",,,,,, 2004-234T22:30:00,000T04:33:04,21-Aug-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2004-234T22:53:00,000T04:25:00,21-Aug-04,UVIS,Prime,Saturn,MOS00SWA,Apoapsis mosaic,MOSAIC_APO_01_07k,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate 64mrad in the YZ plane. 2) Drift at a rate of .0264 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 197.80mrad.",,,,,, 2004-234T22:53:00,000T04:25:00,21-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWA,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-235T03:53:00,000T09:00:00,22-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-235T05:23:00,000T06:00:00,22-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep Space Cal,,,,,, 2004-235T12:53:00,008T07:01:00,22-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-235T12:53:00,005T03:23:00,22-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-235T14:18:00,000T10:30:00,22-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-235T14:18:00,000T10:30:00,22-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-235T14:18:00,000T10:30:00,22-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-235T14:18:00,000T10:30:00,22-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #1,Saturn Far Encounter Global Mosaic #1,,,,,, 2004-236T00:48:00,000T04:55:00,23-Aug-04,UVIS,Prime,Saturn,MOS00SWA,Apoapsis mosaic,MOSAIC_APO_01_07l,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center. 2) Drift at a rate of .0263 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 197.38mrad",,,,,, 2004-236T00:48:00,000T04:55:00,23-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWA,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-236T05:43:00,000T03:30:00,23-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-236T05:43:00,000T03:30:00,23-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-236T05:43:00,000T03:30:00,23-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-236T05:43:00,000T03:30:00,23-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #1,Saturn Far Encounter Global Mosaic #2,,,,,, 2004-236T09:53:00,000T12:00:00,23-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-236T21:53:00,000T23:45:00,23-Aug-04,INMS,Non-SPASS,Saturn,PTOTM,MAPS survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-236T23:23:00,000T09:45:00,23-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-236T23:23:00,000T09:45:00,23-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-236T23:26:00,000T09:45:00,23-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #1,Saturn Far Encounter Global Mosaic #3,,,,,, 2004-237T09:38:00,000T12:00:00,24-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-237T21:38:00,000T00:33:00,24-Aug-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-237T22:11:00,002T14:27:00,24-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Ride with prime instrument,,,,,, 2004-237T22:38:00,000T01:00:00,24-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 005 TH OBSERVATIO","DIFFUSE RINGS IN REV 000, GO WEST TEMPLATE",,,,,, 2004-237T22:38:00,000T01:00:00,24-Aug-04,CIRS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,"Diffuse Rings, Go West Template Ridealong","Ridealong on ISS diffuse rings, Go West Template",,,,,, 2004-237T23:38:00,000T03:25:00,24-Aug-04,UVIS,Prime,Saturn,MOS00SWB,Apoapsis mosaic,MOSAIC_APO_01_07n,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0263 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.89mrad.",,,,,, 2004-237T23:38:00,000T03:25:00,24-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWB,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-238T03:38:00,000T09:00:00,25-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-238T14:03:00,000T10:30:00,25-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-238T14:03:00,000T10:30:00,25-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-238T14:03:00,000T10:30:00,25-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-238T14:03:00,000T10:30:00,25-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #1,Saturn Far Encounter Global Mosaic #4,,,,,, 2004-239T00:33:00,000T04:55:00,26-Aug-04,UVIS,Prime,Saturn,MOS00SWB,Apoapsis mosaic,MOSAIC_APO_01_07o,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0262 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.74mrad.",,,,,, 2004-239T00:33:00,000T04:55:00,26-Aug-04,ISS,SPASS Rider,Saturn,MOS00SWB,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-239T05:28:00,000T05:00:00,26-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-239T05:28:00,000T05:00:00,26-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-239T05:28:00,000T05:00:00,26-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-239T05:28:00,000T05:00:00,26-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #5,Saturn Far Encounter Global Mosaic #5,,,,,, 2004-239T10:58:00,000T09:00:00,26-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-239T12:28:00,000T06:00:00,26-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Deep Space Calibration,,,,,, 2004-239T21:28:00,000T02:25:00,26-Aug-04,UVIS,Prime,Saturn,MOS00SWB,Apoapsis mosaic,MOSAIC_APO_01_07p,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0262 mrad/sec about the Z-axis toward -MOS Orb 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.74mrad",,,,,, 2004-239T23:53:00,000T10:30:00,26-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-239T23:53:00,000T10:30:00,26-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-239T23:53:00,000T10:30:00,26-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #6,Saturn Far Encounter Global Mosaic #6,,,,,, 2004-240T11:09:00,000T09:00:00,27-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-240T12:38:00,002T09:22:00,27-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-240T16:15:00,007T07:45:00,27-Aug-04,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,"Part of SW1 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observes the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2004-240T16:16:00,007T07:44:00,27-Aug-04,CAPS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS solar wind/aurora campaign,MAPS magnetospheric survey,,,,,, 2004-240T16:16:00,003T03:38:00,27-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-240T16:20:00,015T19:15:00,27-Aug-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,Survey measurements of dust,,,,,, 2004-240T21:39:00,000T01:00:00,27-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 001 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO WEST TEMPLATE",,,,,, 2004-240T22:39:00,000T04:25:00,27-Aug-04,UVIS,Prime,Saturn,MOS0ASWC,Apoapsis mosaic,MOSAIC_APO_01_08,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center. 2) Drift at a rate of .0262 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.67mrad.",,,,,, 2004-240T22:39:00,000T04:25:00,27-Aug-04,ISS,SPASS Rider,Saturn,MOS0ASWC,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-241T03:34:00,000T09:00:00,28-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-241T14:04:00,000T10:30:00,28-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-241T14:04:00,000T10:30:00,28-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-241T14:04:00,000T10:30:00,28-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-241T14:04:00,000T10:30:00,28-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #7,Saturn Far Encounter Global Mosaic #7,,,,,, 2004-242T00:34:00,000T04:55:00,29-Aug-04,UVIS,Prime,Saturn,MOS0ASWC,Apoapsis mosaic,MOSAIC_APO_01_08a,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0262 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.67mrad.",,,,,, 2004-242T00:34:00,000T04:55:00,29-Aug-04,ISS,SPASS Rider,Saturn,MOS0ASWC,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-242T05:29:00,000T05:00:00,29-Aug-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-242T05:29:00,000T05:00:00,29-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-242T05:29:00,000T05:00:00,29-Aug-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-242T05:29:00,000T05:00:00,29-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #8,Saturn Far Encounter Global Mosaic #8,,,,,, 2004-242T10:59:00,000T09:00:00,29-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-242T21:29:00,000T02:25:00,29-Aug-04,UVIS,Prime,Saturn,MOS0ASWC,Apoapsis mosaic,MOSAIC_APO_01_08b,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0262 mrad/sec about the Z-axis toward +MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.87mrad",,,,,, 2004-242T22:00:00,000T00:33:00,29-Aug-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-242T22:33:00,004T23:27:00,29-Aug-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-242T23:54:00,000T10:30:00,29-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-242T23:54:00,000T10:30:00,29-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-242T23:54:00,000T10:30:00,29-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #9,Saturn Far Encounter Global Mosaic #9,,,,,, 2004-243T10:54:00,000T09:00:00,30-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-243T12:29:00,000T06:00:00,30-Aug-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Deep Space Calibration,,,,,, 2004-243T19:54:00,000T16:25:00,30-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-243T19:54:00,000T16:25:00,30-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-243T22:54:00,000T01:00:00,30-Aug-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 002 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO WEST TEMPLATE",,,,,, 2004-243T23:30:00,000T02:16:32,30-Aug-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2004-243T23:54:00,000T02:55:00,30-Aug-04,UVIS,Prime,Saturn,MOS0ASWD,Apoapsis mosaic,MOSAIC_APO_01_08c,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0263 mrad/sec about the Z-axis toward -MOS Orb for 8500s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 197.00mrad",,,,,, 2004-243T23:54:00,000T02:55:00,30-Aug-04,ISS,SPASS Rider,Saturn,MOS0ASWD,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-244T03:19:00,000T09:00:00,31-Aug-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-244T12:19:00,003T11:41:00,31-Aug-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-244T12:19:00,003T11:41:00,31-Aug-04,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW1 Campaign,Part of SW1 MAPS Campaign. Observe solar wind plasma waves and Saturn radio emissions while ORS instruments simultaneously observe Saturn's aurora and other MAPS observe solar wind conditions.,,,,,, 2004-244T13:49:00,000T10:30:00,31-Aug-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-244T13:49:00,000T10:30:00,31-Aug-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-244T13:49:00,000T10:30:00,31-Aug-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-244T13:49:00,000T10:30:00,31-Aug-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #1,Saturn Far Encounter Global Mosaic #10,,,,,, 2004-245T00:19:00,000T04:55:00,1-Sep-04,UVIS,Prime,Saturn,MOS0ASWD,Apoapsis mosaic,MOSAIC_APO_01_08d,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0263 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 197.26mrad",,,,,, 2004-245T00:19:00,000T04:55:00,1-Sep-04,ISS,SPASS Rider,Saturn,MOS0ASWD,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-245T05:14:00,000T05:00:00,1-Sep-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-245T05:14:00,000T05:00:00,1-Sep-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-245T05:14:00,000T05:00:00,1-Sep-04,ISS,SPASS Rider,Saturn,AURORAB,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-245T05:14:00,000T05:00:00,1-Sep-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #11,Saturn Far Encounter Global Mosaic #11,,,,,, 2004-245T10:44:00,000T09:00:00,1-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-245T12:14:00,000T06:00:00,1-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep space cal,Deep Space Calibration,,,,,, 2004-245T21:14:00,000T02:25:00,1-Sep-04,UVIS,Prime,Saturn,MOS0ASWD,Apoapsis mosaic,MOSAIC_APO_01_08e,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0263 mrad/sec about the Z-axis toward -MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 197.54mrad.",,,,,, 2004-245T23:39:00,000T10:30:00,1-Sep-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-245T23:39:00,000T10:30:00,1-Sep-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-245T23:39:00,000T10:30:00,1-Sep-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #12,Saturn Far Encounter Global Mosaic #12,,,,,, 2004-246T10:39:00,000T09:00:00,2-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-246T21:09:00,000T01:00:00,2-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO WEST TEMPLATE, 003 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO WEST TEMPLATE",,,,,, 2004-246T22:09:00,000T04:25:00,2-Sep-04,UVIS,Prime,Saturn,MOS0ASWE,Apoapsis mosaic,MOSAIC_APO_01_08f,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate -64mrad in the YZ plane. 2) Drift at a rate of .0264 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 197.93mrad.",,,,,, 2004-246T22:09:00,000T04:25:00,2-Sep-04,ISS,SPASS Rider,Saturn,MOS0ASWE,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-247T03:04:00,000T09:00:00,3-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-247T13:34:00,000T10:30:00,3-Sep-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-247T13:34:00,000T10:30:00,3-Sep-04,CIRS,SPASS Rider,Saturn,SPTEMPL10,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-247T13:34:00,000T10:30:00,3-Sep-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-247T13:34:00,000T10:30:00,3-Sep-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #13,Saturn Far Encounter Global Mosaic #13,,,,,, 2004-247T22:00:00,000T00:33:00,3-Sep-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-247T22:33:00,002T04:32:00,3-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-248T00:00:00,008T11:35:00,4-Sep-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-248T00:00:00,001T19:40:00,4-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-248T00:00:00,008T11:35:00,4-Sep-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-248T00:00:00,001T19:40:00,4-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-248T00:04:00,000T04:55:00,4-Sep-04,UVIS,Prime,Saturn,MOS0ASWE,Apoapsis mosaic,MOSAIC_APO_01_08g,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0265 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 198.41mrad",,,,,, 2004-248T00:04:00,000T04:55:00,4-Sep-04,ISS,SPASS Rider,Saturn,MOS0ASWE,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-248T04:59:00,000T05:00:00,4-Sep-04,UVIS,Prime,Saturn,AURORAB,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 5 hours. A similar request (auroralA) is identical except it repeats for 10.5 hours.",,,,,, 2004-248T04:59:00,000T05:00:00,4-Sep-04,CIRS,SPASS Rider,Saturn,SPTEMPL05,South pole imaging,Saturn South Pole Template,Saturn south pole,,,,,, 2004-248T04:59:00,000T05:00:00,4-Sep-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #14,Saturn Far Encounter Global Mosaic #14,,,,,, 2004-248T10:29:00,000T09:00:00,4-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-248T11:59:00,000T06:00:00,4-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Saturn South Pole Template,Deep Space Calibration,,,,,, 2004-248T20:59:00,000T02:25:00,4-Sep-04,UVIS,Prime,Saturn,MOS0ASWE,Apoapsis mosaic,MOSAIC_APO_01_08h,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about Z to -MOS Orb from Saturn Center. 2) Drift at a rate of .0265 mrad/sec about the Z-axis toward +MOS Orb for 6700s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 198.87mrad.",,,,,, 2004-248T23:24:00,000T03:30:00,4-Sep-04,UVIS,Prime,Saturn,AURORAA,Saturn aurora movie,Saturn south pole auroral scan,"This observation is a repetative half-hour unit for imaging Saturn's south pole during the go-west template in apoapse 0/A. It uses the GENMOS_P module. It starts with a scan from left limb to central meridian, stop at central meridion for 7 minutes, continue scan to right limb and a fast slew back to left limb. The full duration is 30 minutes. This repeats 21 times for 10.5 hours. A similar request (auroralB) is identical except it repeats for 5.0 hours.",,,,,, 2004-248T23:24:00,000T03:30:00,4-Sep-04,ISS,SPASS Rider,Saturn,AURORAA,Saturn aurora movie,go west saturn pole movie,Saturn south pole movie,,,,,, 2004-248T23:24:00,000T03:30:00,4-Sep-04,VIMS,SPASS Rider,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global Mosaic #15,Saturn Far Encounter Global Mosaic #15,,,,,, 2004-249T02:54:00,000T07:00:00,5-Sep-04,CAPS,Prime,InstrumentCalibration,SWCAL,CAPS solar wind beam calibration,CAPS Solar Wind Beam Calibration,"CAPS solar wind beam calibration. Need pointing -x to sun, roll +/- 85 degrees about Y. Need 16kbps. Need to be placed late in this subphase since we need to have the solar wind beam as narrow as possible (and on average the beam is narrower the farther we are from the sun).",,,,,, 2004-249T10:40:00,000T09:00:00,5-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-249T19:40:00,000T16:25:00,5-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-249T19:40:00,000T16:25:00,5-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-249T21:10:00,000T01:00:00,5-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 004 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-249T21:30:00,000T04:33:04,5-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 700 bps survey.,,,,,, 2004-249T22:10:00,000T04:25:00,5-Sep-04,UVIS,Prime,Saturn,MOS0AGEA,Apoapsis mosaic,MOSAIC_APO_01_08i,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0266 mrad/sec about the z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 199.49mrad.",,,,,, 2004-249T22:10:00,000T04:25:00,5-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEA,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-250T03:05:00,000T09:00:00,6-Sep-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,Survey 18 a,06/14/2004 - Erin changed time of request. Received additional sponge bits and thus must make adjustments to CIMS request FSW Testing,,,,,, 2004-250T03:05:00,000T09:00:00,6-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-250T12:05:00,001T07:25:00,6-Sep-04,INMS,Non-SPASS,Saturn,SURVEYB,MAPS survey,Suvery 19 b,06/14/2004 - Erin changed time of request. Received additional sponge bits and thus must make adjustments to CIMS request FSW testing,,,,,, 2004-250T12:05:00,005T07:05:00,6-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-250T12:05:00,005T07:05:00,6-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-250T13:35:00,000T20:25:00,6-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-250T13:35:00,000T20:25:00,6-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-250T13:35:00,000T20:25:00,6-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-250T13:35:00,000T20:25:00,6-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #1",Saturn Far Encounter Global Mosaic under Go-East Template #1. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-251T10:30:00,000T09:00:00,7-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-251T12:00:00,000T06:00:00,7-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-251T19:30:00,000T23:55:00,7-Sep-04,INMS,Non-SPASS,Saturn,PTOTM003,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-251T21:00:00,000T05:15:00,7-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-251T21:00:00,000T05:15:00,7-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-251T21:00:00,000T05:15:00,7-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-251T21:00:00,000T05:15:00,7-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #2",Saturn Far Encounter Global Mosaic under Go-East Template #2. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-252T02:15:00,000T07:30:00,8-Sep-04,UVIS,Prime,Saturn,MOS0AGEA,Apoapsis mosaic,MOSAIC_APO_01_08j,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about Z to +MOS Orb from Saturn Center. 2) Drift at a rate of .0268 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about Z for 9500s toward +MOS orb. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 201.02mrad.",,,,,, 2004-252T02:15:00,000T04:55:00,8-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEA,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-252T10:25:00,000T09:00:00,8-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-252T19:25:00,000T00:33:00,8-Sep-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-252T19:58:00,002T23:12:00,8-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-252T20:55:00,000T01:00:00,8-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 005 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-252T21:55:00,000T04:25:00,8-Sep-04,UVIS,Prime,Saturn,MOS0AGEB,Apoapsis mosaic,MOSAIC_APO_01_08k,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .0270 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 201.70mrad.",,,,,, 2004-252T21:55:00,000T04:25:00,8-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEB,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-253T02:50:00,000T09:00:00,9-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-253T13:20:00,000T20:25:00,9-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-253T13:20:00,000T20:25:00,9-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-253T13:20:00,000T20:25:00,9-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-253T13:20:00,000T20:25:00,9-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #3",Saturn Far Encounter Global Mosaic under Go-East Template #3. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-254T10:15:00,000T09:00:00,10-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-254T11:00:00,000T06:00:00,10-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-254T20:45:00,000T05:15:00,10-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-254T20:45:00,000T05:15:00,10-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-254T20:45:00,000T05:15:00,10-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-254T20:45:00,000T05:15:00,10-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #4",Saturn Far Encounter Global Mosaic under Go-East Template #4. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-255T02:00:00,000T07:30:00,11-Sep-04,UVIS,Prime,Saturn,MOS0AGEB,Apoapsis mosaic,MOSAIC_APO_01_08l,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .0272 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Rotate -64mrad in the YZ plane. Drift at indicated rate toward -MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 203.74mrad.",,,,,, 2004-255T02:00:00,000T04:55:00,11-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEB,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-255T10:10:00,000T09:00:00,11-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-255T19:10:00,000T16:25:00,11-Sep-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,SURVEY 019A,06/14/2004 - Erin created request. Received additional sponge bits and thus must make adjustments to CIMS request Will be performing FSW testing,,,,,, 2004-255T19:10:00,000T16:25:00,11-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-255T19:10:00,000T16:25:00,11-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-255T20:40:00,000T01:00:00,11-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 006 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-255T21:30:00,000T04:33:04,11-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 700 bps survey rate.,,,,,, 2004-255T21:40:00,000T04:25:00,11-Sep-04,UVIS,Prime,Saturn,MOS0AGEC,Apoapsis mosaic,MOSAIC_APO_01_09,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0273 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 204.61mrad",,,,,, 2004-255T21:40:00,000T04:25:00,11-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEC,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-256T02:35:00,000T09:00:00,12-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-256T11:35:00,001T22:10:00,12-Sep-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-256T11:35:00,001T21:58:00,12-Sep-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,Survey measurements of dust,,,,,, 2004-256T11:35:00,000T01:22:00,12-Sep-04,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,STARTUP,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2004-256T11:35:00,001T22:10:00,12-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-256T11:35:00,001T22:03:00,12-Sep-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-256T11:35:00,000T12:25:00,12-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-256T12:57:00,001T20:38:00,12-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-256T13:05:00,000T20:25:00,12-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-256T13:05:00,000T20:25:00,12-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-256T13:05:00,000T20:25:00,12-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-256T13:05:00,000T20:25:00,12-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #5",Saturn Far Encounter Global Mosaic under Go-East Template #5. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-257T00:00:00,001T00:00:00,13-Sep-04,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2004-257T10:00:00,000T09:00:00,13-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-257T10:10:00,000T06:00:00,13-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-257T20:30:00,000T04:37:00,13-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-257T20:30:00,000T04:37:00,13-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-257T20:30:00,000T04:37:00,13-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-257T20:30:00,000T04:37:00,13-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #6",Saturn Far Encounter Global Mosaic under Go-East Template #6. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-258T00:00:00,000T09:40:00,14-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-258T01:07:00,000T05:30:00,14-Sep-04,UVIS,Prime,Saturn,MOS0AGEC,Apoapsis mosaic,MOSAIC_APO_01_09a,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate -64mrad in the YZ plane. 2) Drift at a rate of .0276 mrad/sec about the Z-axis toward -MOS Orb for 15000s. 3) Rotate +128mrad in the YZ plane. Drift at the indicated rate toward +MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 207.23mrad.",,,,,, 2004-258T01:07:00,000T04:55:00,14-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEC,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-258T09:32:00,000T00:06:00,14-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,SLEEP,Instrument to sleep mode,Sleep for Probe activity,sleep instrument,,,,,, 2004-258T09:33:00,000T09:31:00,14-Sep-04,CDA,Non-SPASS,Saturn,PCO,Probe Checkout,ProbeCheckOut,CDA Sleep/Mute Unmute/Active pointing: NA; datavolume=0 MB,,,,,, 2004-258T09:34:00,000T00:17:00,14-Sep-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder,"Put CIRS to sleep/mute for PCO#15, sleep and mute (at epoch-00:06?)",,,,,, 2004-258T09:35:00,000T00:10:00,14-Sep-04,INMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,INMS Sleep and Mute for Probe C/O,null,,,,,, 2004-258T09:38:00,000T09:24:00,14-Sep-04,MIMI,SPASS Rider,co-rotation,PCOMUTE,Mute instrument for Probe Checkout,Probe Checkout Mute,"SLEEP/MUTE for PSA; SLEEP 13 minutes before PSA_ON (at REQUEST START), MUTE 7 minutes later. Duration lasts until UNMUTE, at 6 minutes after PSA_OFF, ACTIVE 7 minutes later.",,,,,, 2004-258T09:40:00,000T09:31:00,14-Sep-04,RPWS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,RPWS Sleep and Mute for Probe activity,"RPWS sleep/mute for Probe activity, followed by unmute/sleep.",,,,,, 2004-258T09:42:00,000T00:03:00,14-Sep-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (PCO 15),UVIS to go to sleep/mute for PCO 15 (MGTWT request),,,,,, 2004-258T09:43:00,000T00:05:00,14-Sep-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE,VIMS to SLEEP/ MUTE,,,,,, 2004-258T09:45:00,000T00:01:00,14-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,MUTE,Instrument to sleep mode,Mute for Probe activity,mute instrument,,,,,, 2004-258T09:45:00,000T09:17:00,14-Sep-04,INMS,Non-SPASS,SpacecraftActivity,MUTE,Instrument to sleep mode,INMS Mute for Probe C/O,null,,,,,, 2004-258T09:45:00,000T09:17:00,14-Sep-04,MAG,Non-SPASS,SpacecraftActivity,PROBEMUTE,Huygens Probe support,Mute/Unmute for Probe Checkout 15,"Mute instrument for probe checkout, unmute at end. NOTE: MAG does not go to sleep for PCO, other instruments do",,,,,, 2004-258T09:51:00,000T09:05:00,14-Sep-04,PROBE,Non-SPASS,Earth,PCO15,Probe Checkout,Probe Checkout #15,"Preheating Probe Checkout; MTU Test. This activity, if moved, should remain five days away from Battery Depassivation 1, for thermal reasons. X-band downlink required. The following Orbiter instruments will be ON, in sleep mode, and muted prior to PSA ON: CDA, CAPS, ISS, MIMI, RPWS, MAG, UVIS, and VIMS; other orbiter instruments OFF. The checkout data recorded on the SSR should be played back on a different pass.",,,,,, 2004-258T10:06:00,000T00:09:50,14-Sep-04,ISS,Non-SPASS,Earth,SLEEPMUTE,Huygens probe support,put ISS to sleep for probe activity,placeholder activity put into CIMS to remenind ISS to go into sleep for probe activity at request of MAG TWT,,,,,, 2004-258T19:02:00,000T00:01:00,14-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,UNMUTE,Huygens probe support,Unmute after Probe activity,wake up & unmute biu,,,,,, 2004-258T19:02:00,000T00:07:00,14-Sep-04,MIMI,SPASS Rider,co-rotation,PCOUNMUTE,Huygens probe support,"Probe Checkout Un-Mute, Active","UNMUTE/ACTIVE post- PSA; UMNUTE 6 minutes after PSA_OFF (at REQUEST START), ACTIVE 7 minutes later.",,,,,, 2004-258T19:02:00,004T17:52:00,14-Sep-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-258T19:02:00,000T00:04:00,14-Sep-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,wake/unmute placeholder,"UNMUTE. Note power transients! unmute at 00:06, wake at epoch+00:09",,,,,, 2004-258T19:02:00,000T00:04:00,14-Sep-04,INMS,Non-SPASS,SpacecraftActivity,UNMUTE,Huygens probe support,INMS UnMute after Probe C/O,null,,,,,, 2004-258T19:02:00,000T00:07:00,14-Sep-04,ISS,Non-SPASS,Earth,WAKESLEEP,Wakeup instrument from sleep mode,wake up ISS after probe activity,placeholder activity put into CIMS to remind ISS to wake up after probe activity at request of MAG TWT,,,,,, 2004-258T19:02:00,002T23:54:00,14-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-258T19:02:00,000T00:11:00,14-Sep-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after PCO 15,Unmute/go to active after PCO 15 (MAGTWT request),,,,,, 2004-258T19:02:00,000T00:18:00,14-Sep-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode,VIMS to ACTIVE,,,,,, 2004-258T19:03:00,000T02:16:00,14-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,WakeUp after Probe activity,wake up & unmute biu,,,,,, 2004-258T19:04:00,002T23:51:59,14-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-258T19:06:00,002T17:51:00,14-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-258T19:09:00,004T17:38:00,14-Sep-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-258T19:11:00,002T23:45:00,14-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-258T20:56:00,000T01:00:00,14-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 007 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-258T21:56:00,000T03:55:00,14-Sep-04,UVIS,Prime,Saturn,MOS0AGED,Apoapsis mosaic,MOSAIC_APO_01_09b,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .0279 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 208.33mrad.",,,,,, 2004-258T21:56:00,000T03:55:00,14-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGED,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-259T02:21:00,000T09:00:00,15-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-259T12:51:00,000T20:25:00,15-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-259T12:51:00,000T20:25:00,15-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-259T12:51:00,000T20:25:00,15-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-259T12:51:00,000T20:25:00,15-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #7",Saturn Far Encounter Global Mosaic under Go-East Template #7. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-260T09:46:00,000T09:00:00,16-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-260T11:26:00,000T06:00:00,16-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-260T20:16:00,000T05:15:00,16-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-260T20:16:00,000T05:15:00,16-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-260T20:16:00,000T05:15:00,16-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-260T20:16:00,000T05:15:00,16-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #8",Saturn Far Encounter Global Mosaic under Go-East Template #8. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-261T01:31:00,000T07:30:00,17-Sep-04,UVIS,Prime,Saturn,MOS0AGED,Apoapsis mosaic,MOSAIC_APO_01_09c,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate -64mrad in the YZ plane. 2) Drift at a rate of .0284 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Rotate +128mrad in the YZ plane. Drift at the indicated rate toward -MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for the remaining observation time. MOS Orb (+/-Range): 212.94mrad.",,,,,, 2004-261T01:31:00,000T04:55:00,17-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGED,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-261T09:56:00,000T09:00:00,17-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-261T12:57:00,000T00:33:00,17-Sep-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-261T13:30:00,001T23:14:00,17-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-261T18:56:00,000T16:25:00,17-Sep-04,CAPS,Non-SPASS,Saturn,SURVEY2,MAPS survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-261T18:56:00,000T16:25:00,17-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-261T18:56:00,000T16:25:00,17-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-261T18:56:00,000T16:25:00,17-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-261T20:26:00,000T01:00:00,17-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 008 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-261T20:26:00,000T01:00:00,17-Sep-04,UVIS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,UV Ring Spectroscopy,,,,,,, 2004-261T21:26:00,000T04:25:00,17-Sep-04,UVIS,Prime,Saturn,MOS0AGEE,Apoapsis mosaic,MOSAIC_APO_01_09e,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate -64mrad in the YZ plane. 2) Drift at a rate of .0284 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 212.94mrad.",,,,,, 2004-261T21:26:00,000T04:25:00,17-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEE,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-261T22:21:00,000T08:00:00,17-Sep-04,RSS,SPASS Rider,Earth,USOBSC,RSS HGA boresight calibration,RSS USO Characterization plus Boresight Calibratio,RSS USO characterization plus Boresight Cal. Pointing=XBAND to Earth + two crosshair maneuvers. Last 4 hours required to be tracked at DSS-55 in 1-way mode. Last 4 hours are also desired to be tracked at DSS-63 in 1-way mode.,,,,,, 2004-261T23:00:00,000T02:16:32,17-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-262T02:21:00,000T09:00:00,18-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-262T05:21:00,000T01:00:00,18-Sep-04,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,RSS Boresight Calibration,RSS HGA Boresight Calibration. Pointing: XBAND to Earth + two crosshair maneuvers,,,,,, 2004-262T06:21:00,000T05:00:00,18-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-262T11:21:00,001T01:33:00,18-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-262T11:21:00,001T01:28:00,18-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-262T11:21:01,001T01:20:59,18-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-262T12:51:00,000T20:25:00,18-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-262T12:51:00,000T20:25:00,18-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-262T12:51:00,000T20:25:00,18-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-262T12:51:00,000T20:25:00,18-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #9",Saturn Far Encounter Global Mosaic under Go-East Template #9. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-263T12:41:00,000T00:06:00,19-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,SLEEP,Instrument to sleep mode,Sleep for Probe activity,sleep instrument,,,,,, 2004-263T12:42:00,000T02:26:00,19-Sep-04,CDA,Non-SPASS,Saturn,PCO,Probe Checkout,ProbeCheckOut,Mute for PCO. Sleep/Mute Unmute/Active Commands for CDA pointing: NA; datavolume=0 MB,,,,,, 2004-263T12:43:00,000T00:17:00,19-Sep-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder,Put CIRS to sleep/mute for DEPASS,,,,,, 2004-263T12:44:00,000T00:10:00,19-Sep-04,INMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,INMS Sleep and Mute for Probe C/O,null,,,,,, 2004-263T12:45:00,000T00:09:50,19-Sep-04,ISS,Non-SPASS,Earth,SLEEPMUTE,Huygens probe support,put ISS to sleep for probe activity,placeholder activity put into CIMS to remenind ISS to go into sleep for probe activity at request of MAG TWT,,,,,, 2004-263T12:47:00,000T02:19:00,19-Sep-04,MIMI,SPASS Rider,co-rotation,PCOMUTE,Mute instrument for Probe Checkout,Probe SLEEP,"SLEEP/MUTE for Probe depassivation of batteries. SLEEP 13 minutes before PSA_ON (at request start), MUTE 7 minutes later. Duration lasts until UNMUTE, at 6 minutes after PSA_OFF, ACTIVE 7 minutes later. Both epoch relative.",,,,,, 2004-263T12:49:00,000T02:26:00,19-Sep-04,RPWS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,RPWS Sleep and Mute for Probe activity,"RPWS sleep/mute for Probe activity, followed by unmute/sleep.",,,,,, 2004-263T12:51:00,000T00:03:00,19-Sep-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (Probe depassivation),UVIS to go to sleep/mute for probe depassivation,,,,,, 2004-263T12:52:00,000T00:05:00,19-Sep-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE,VIMS to SLEEP/ MUTE,,,,,, 2004-263T12:54:00,000T00:01:00,19-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,MUTE,Instrument to sleep mode,Mute for Probe activity,mute instrument,,,,,, 2004-263T12:54:00,000T02:12:00,19-Sep-04,INMS,Non-SPASS,SpacecraftActivity,MUTE,Instrument to sleep mode,INMS Mute for Probe Depassivation,null,,,,,, 2004-263T12:54:00,000T02:12:00,19-Sep-04,MAG,Non-SPASS,SpacecraftActivity,PROBEMUTE,Huygens Probe support,Mute/Unmute for Probe Depassivation,"Mute instrument for probe checkout, unmute at end. NOTE: MAG does not go to sleep for PCO, other instruments do",,,,,, 2004-263T13:30:00,000T01:30:00,19-Sep-04,PROBE,Non-SPASS,Earth,DEPASSIV1,Huygens probe support,Probe Battery Depassivation - 1,Prepare Probe batteries for primary mission. X-band downlink required. Orbiter instruments off/sleep/mute as for probe checkouts. This activity must remain at least five days from probe checkout F15 for thermal reasons.,,,,,, 2004-263T15:06:00,000T00:01:00,19-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,UNMUTE,Huygens probe support,Unmute after Probe activity,wake up & unmute biu,,,,,, 2004-263T15:06:00,000T00:07:00,19-Sep-04,MIMI,SPASS Rider,co-rotation,PCOUNMUTE,Huygens probe support,"Probe Checkout Un-Mute, Active","UNMUTE/ACTIVE post- PSA; UMNUTE 6 minutes after PSA_OFF (at REQUEST START), ACTIVE 7 minutes later.",,,,,, 2004-263T15:06:00,028T18:24:00,19-Sep-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-263T15:06:00,000T00:04:00,19-Sep-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,wake/unmute placeholder,"UNMUTE. Note power transients! unmute at 00:06, wake at epoch+00:09",,,,,, 2004-263T15:06:00,000T00:04:00,19-Sep-04,INMS,Non-SPASS,SpacecraftActivity,UNMUTE,Huygens probe support,INMS UnMute after Probe Depassivation,null,,,,,, 2004-263T15:06:00,000T00:07:00,19-Sep-04,ISS,Non-SPASS,Earth,WAKESLEEP,Wakeup instrument from sleep mode,wake up ISS after probe activity,placeholder activity put into CIMS to remind ISS to wake up after probe activity at request of MAG TWT,,,,,, 2004-263T15:06:00,001T03:35:00,19-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-263T15:06:00,000T00:11:00,19-Sep-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after probe dep.,Unmute/go to active after probe depassivation,,,,,, 2004-263T15:06:00,000T00:05:00,19-Sep-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode,VIMS to ACTIVE,,,,,, 2004-263T15:07:00,000T02:16:00,19-Sep-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,WakeUp after Probe activity,wake up & unmute biu,,,,,, 2004-263T15:08:00,001T03:32:59,19-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-263T15:10:00,001T03:31:00,19-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-263T15:13:00,015T08:47:00,19-Sep-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-263T15:15:00,001T03:26:00,19-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-263T20:16:00,000T05:15:00,19-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-263T20:16:00,000T05:15:00,19-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-263T20:16:00,000T05:15:00,19-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-263T20:16:00,000T05:15:00,19-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #10",Saturn Far Encounter Global Mosaic under Go-East Template #10. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-264T01:31:00,000T07:30:00,20-Sep-04,UVIS,Prime,Saturn,MOS0AGEE,Apoapsis mosaic,MOSAIC_APO_01_09f,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .0289 mrad/sec about the Z-axis toward -MOS Orb 15000s. 3) Rotate -64mrad in the YZ plane. Drift at the indicated rate about the Z-axis toward +MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 216.92mrad.",,,,,, 2004-264T01:31:00,000T04:55:00,20-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEE,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-264T09:41:00,000T09:00:00,20-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-264T18:41:00,000T16:25:00,20-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-264T18:41:00,000T16:25:00,20-Sep-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,MAPS Survey,Mag Survey,,,,,, 2004-264T18:41:00,000T16:25:00,20-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-264T18:41:00,000T16:25:00,20-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-264T20:11:00,000T01:00:00,20-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 009 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-264T20:11:00,000T01:00:00,20-Sep-04,UVIS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,UV Ring Spectroscopy,,,,,,, 2004-264T20:45:00,000T04:33:04,20-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-264T21:11:00,000T04:25:00,20-Sep-04,UVIS,Prime,Saturn,MOS0AGEF,Apoapsis mosaic,MOSAIC_APO_01_09h,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate -64mrad in the YZ plane. 2) Drift at a rate of .0291 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 218.57mrad.",,,,,, 2004-264T21:11:00,000T04:25:00,20-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEF,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-265T02:06:00,000T09:00:00,21-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-265T11:06:00,001T01:51:00,21-Sep-04,INMS,Non-SPASS,Saturn,SURVEYB,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-265T11:06:00,002T07:21:00,21-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-265T11:06:00,002T07:21:00,21-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-265T11:06:01,002T07:20:58,21-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-265T12:36:00,000T20:25:00,21-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-265T12:36:00,000T20:25:00,21-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-265T12:36:00,000T20:25:00,21-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-265T12:36:00,000T20:25:00,21-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #11",Saturn Far Encounter Global Mosaic under Go-East Template #11. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-266T09:31:00,000T09:00:00,22-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-266T11:11:00,000T06:00:00,22-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-266T12:57:00,000T00:33:00,22-Sep-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-266T13:30:00,001T04:57:00,22-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-266T20:01:00,000T05:15:00,22-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-266T20:01:00,000T05:15:00,22-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-266T20:01:00,000T05:15:00,22-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-266T20:01:00,000T05:15:00,22-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #12",Saturn Far Encounter Global Mosaic under Go-East Template #12. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-267T01:16:00,000T07:30:00,23-Sep-04,UVIS,Prime,Saturn,MOS0AGEF,Apoapsis mosaic,MOSAIC_APO_01_09j,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .0298 mrad/sec about the Z-axis toward +MOS Orb for 15000s. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis toward -MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 223.43mrad.",,,,,, 2004-267T01:16:00,000T04:55:00,23-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEF,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-267T09:27:00,000T09:00:00,23-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-267T18:27:00,000T16:25:00,23-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-267T18:27:00,000T16:25:00,23-Sep-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-267T18:27:00,000T16:25:00,23-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-267T18:27:00,000T16:25:00,23-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-267T19:57:00,000T01:00:00,23-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 010 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-267T19:57:00,000T01:00:00,23-Sep-04,UVIS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,UV Ring Spectroscopy,,,,,,, 2004-267T20:30:00,000T04:33:04,23-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-267T20:57:00,000T04:25:00,23-Sep-04,UVIS,Prime,Saturn,MOS0AGEG,Apoapsis mosaic,MOSAIC_APO_01_09k,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to +MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .0301 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 225.46mrad.",,,,,, 2004-267T20:57:00,000T04:25:00,23-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEG,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-268T01:52:00,000T09:00:00,24-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-268T10:52:00,002T07:35:00,24-Sep-04,INMS,Non-SPASS,Saturn,SURVEYB,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-268T10:52:00,000T23:55:00,24-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-268T10:52:00,002T07:35:00,24-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-268T10:52:01,002T07:34:58,24-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-268T12:22:00,000T20:25:00,24-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-268T12:22:00,000T20:25:00,24-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-268T12:22:00,000T20:25:00,24-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-268T12:22:00,000T20:25:00,24-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #13",Saturn Far Encounter Global Mosaic under Go-East Template #13. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-269T09:17:00,000T09:00:00,25-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-269T10:47:00,000T06:05:00,25-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-269T16:52:00,000T18:05:00,25-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-269T19:47:00,000T05:15:00,25-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-269T19:47:00,000T05:15:00,25-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-269T19:47:00,000T05:15:00,25-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-269T19:47:00,000T05:15:00,25-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #14",Saturn Far Encounter Global Mosaic under Go-East Template #14. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-270T01:02:00,000T07:30:00,26-Sep-04,UVIS,Prime,Saturn,MOS0AGEG,Apoapsis mosaic,MOSAIC_APO_01_09l,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0309 mrad/sec about the Z-axis to -MOS Orb for 15000s. 3) Rotate -64mrad in the YZ plane. Drift at indicated rate toward +MOS Orb for 9500s. 4) Slew back to Saturn center and resest pointing. Stare for remaining observation time. MOS Orb (+/-Range): 231.38mrad.",,,,,, 2004-270T01:02:00,000T04:55:00,26-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEG,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-270T09:27:00,000T09:00:00,26-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-270T10:57:00,000T06:05:00,26-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-270T17:02:00,000T01:25:00,26-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-270T18:27:00,000T16:25:00,26-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-270T18:27:00,000T16:25:00,26-Sep-04,INMS,Non-SPASS,Saturn,SURVEYC,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-270T18:27:00,000T16:25:00,26-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-270T18:27:00,000T16:25:00,26-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-270T19:57:00,000T01:00:00,26-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 011 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-270T19:57:00,000T01:00:00,26-Sep-04,UVIS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,UV Ring Spectroscopy,,,,,,, 2004-270T20:30:00,000T06:49:36,26-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-270T20:57:00,000T04:25:00,26-Sep-04,UVIS,Prime,Saturn,MOS0AGEH,Apoapsis mosaic,MOSAIC_APO_01_09n,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .0312 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 233.88mrad.",,,,,, 2004-270T20:57:00,000T04:25:00,26-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEH,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-271T01:52:00,000T09:00:00,27-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-271T10:52:00,002T07:19:59,27-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-271T10:52:00,000T02:05:00,27-Sep-04,INMS,Non-SPASS,Saturn,SURVEYD,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-271T10:52:00,002T07:20:00,27-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-271T10:52:00,002T07:20:00,27-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-271T12:22:00,000T20:25:00,27-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-271T12:22:00,000T20:25:00,27-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-271T12:22:00,000T20:25:00,27-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-271T12:22:00,000T20:25:00,27-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #15",Saturn Far Encounter Global Mosaic under Go-East Template #15. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-271T12:57:00,000T00:33:00,27-Sep-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-271T13:30:00,002T04:42:00,27-Sep-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-272T09:17:00,000T09:00:00,28-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-272T10:57:00,000T06:00:00,28-Sep-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-272T19:47:00,000T05:15:00,28-Sep-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-272T19:47:00,000T05:15:00,28-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-272T19:47:00,000T05:15:00,28-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-272T19:47:00,000T05:15:00,28-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #16",Saturn Far Encounter Global Mosaic under Go-East Template #16. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-273T01:02:00,000T07:30:00,29-Sep-04,UVIS,Prime,Saturn,MOS0AGEH,Apoapsis mosaic,MOSAIC_APO_01_09o,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .0322 mrad/sec about the Z-axis for 15000s to +MOS Orb. 3) Rotate -64mrad in the YZ plane. Drift at the indicated rate toward -MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 241.13mrad.",,,,,, 2004-273T01:02:00,000T04:55:00,29-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEH,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-273T09:12:00,000T09:00:00,29-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-273T18:12:00,000T16:25:00,29-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-273T18:12:00,000T16:25:00,29-Sep-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-273T18:12:00,000T16:25:00,29-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-273T18:12:00,000T16:25:00,29-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-273T19:42:00,000T01:00:00,29-Sep-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 012 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-273T19:42:00,000T01:00:00,29-Sep-04,UVIS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,UV Ring Spectroscopy,,,,,,, 2004-273T20:30:00,000T06:49:36,29-Sep-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-273T20:42:00,000T04:25:00,29-Sep-04,UVIS,Prime,Saturn,MOS0AGEI,Apoapsis mosaic,MOSAIC_APO_01_09q,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0326 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 244.16mrad.",,,,,, 2004-273T20:42:00,000T04:25:00,29-Sep-04,ISS,SPASS Rider,Saturn,MOS0AGEI,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-274T01:37:00,000T09:00:00,30-Sep-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-274T10:37:00,002T02:20:00,30-Sep-04,INMS,Non-SPASS,Saturn,SURVEYB,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-274T10:37:00,004T13:23:00,30-Sep-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-274T10:37:00,004T13:23:00,30-Sep-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-274T10:37:01,011T00:03:58,30-Sep-04,CDA,Non-SPASS,DustRAM direction,SURPCOPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-274T12:07:00,000T20:25:00,30-Sep-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-274T12:07:00,000T20:25:00,30-Sep-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-274T12:07:00,000T20:25:00,30-Sep-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-274T12:07:00,000T20:25:00,30-Sep-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #17",Saturn Far Encounter Global Mosaic under Go-East Template #17. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-275T09:02:00,000T09:00:00,1-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-275T19:32:00,000T05:15:00,1-Oct-04,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-275T19:32:00,000T05:15:00,1-Oct-04,CIRS,SPASS Rider,Saturn,ISSPCKT03,Saturn movie,Saturn Movie Pickets,Movie picket rider,,,,,, 2004-275T19:32:00,000T05:15:00,1-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVIEB,Saturn movie,ISS 2X2MOVIEB Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEB observation,,,,,, 2004-275T19:32:00,000T05:15:00,1-Oct-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #18",Saturn Far Encounter Global Mosaic under Go-East Template #18. 5.25-hour duration. 3 pickets acquired over these 5.25 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 3 observations * 2 exposures * 64*64*352*12 = 105 mbits,,,,,, 2004-276T00:47:00,000T07:30:00,2-Oct-04,UVIS,Prime,Saturn,MOS0AGEI,Apoapsis mosaic,MOSAIC_APO_01_09r,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate -64mrad in the YZ plane. 2) Drift at a rate of .0115 mrad/sec about the Z-axis for 15000s to -MOS Orb. 3) Rotate +128mrad in the YZ plane. Drift at indicated rate toward +MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 86.00mrad.",,,,,, 2004-276T00:47:00,000T04:55:00,2-Oct-04,ISS,SPASS Rider,Saturn,MOS0AGEI,Apoapsis mosaic,UVIS Ride-along for dark images,Ride along during system scans take 5 dark images,,,,,, 2004-276T08:58:00,000T09:00:00,2-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-276T12:57:00,000T00:33:00,2-Oct-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-276T13:30:00,004T23:27:00,2-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-277T01:23:00,000T09:00:00,3-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-278T08:48:00,000T09:00:00,4-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-279T00:00:00,006T10:54:00,5-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-279T00:00:00,006T17:29:00,5-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-279T00:00:01,006T17:06:59,5-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-279T08:43:00,000T09:00:00,5-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-279T19:13:00,000T01:00:00,5-Oct-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 014 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-279T20:13:00,000T04:25:00,5-Oct-04,UVIS,Prime,Saturn,MOS0AGEK,Apoapsis mosaic,MOSAIC_APO_01_10c,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to +MOS Orb and rotate +64mrad in the YZ plane. 2) Drift at a rate of .0124 mrad/sec about the Z-axis toward -MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb(+/-Range): 92.85mrad.",,,,,, 2004-280T01:13:00,000T09:00:00,6-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-280T12:00:00,000T00:30:00,6-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 120 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EP-TL-EN-DI (602, 604, 611, 613, 617)]",,,,,, 2004-280T12:30:00,000T03:00:00,6-Oct-04,ISS,Prime,Saturn,SATSYSTEM,Saturn system image,Saturn system PR observation,"Do observations of satellites (NAC), Saturn, and rings (NAC and WAC), turn to WP. For a detailed description, see notes entry field.",,,,,, 2004-280T15:30:00,000T00:30:00,6-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 121 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-JA-CP-PM-PA (610, 614, 615, 616, 617)]",,,,,, 2004-280T16:30:00,000T09:00:00,6-Oct-04,UVIS,Prime,Star,URXICET,Stellar occultation,URSTAR,Instance of URSTAR. This very slow occultation near apoapse provides an excellent opportunity for high resolution studies of low optical depth regions in the rings. This part of the occultation covers the ring system interior to the B Ring.,,,,,, 2004-281T02:00:00,000T05:50:00,7-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-281T03:30:00,000T06:00:00,7-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-281T08:20:00,000T07:20:00,7-Oct-04,UVIS,Prime,Star,URXICET,Stellar occultation,URSTAR,Instance of URSTAR. This very slow occultation near apoapse provides an excellent opportunity for high resolution studies of low optical depth regions in the rings. This part of the occultation covers the ring system exterior to the B Ring.,,,,,, 2004-281T12:57:00,000T00:33:00,7-Oct-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-281T13:30:00,003T21:13:00,7-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-281T16:26:00,000T01:15:00,7-Oct-04,ISS,Prime,Iapetus,GLOBCOLA,Global coverage observation,Iapetus global color observation,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 25 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn -Y to WP,,,,,, 2004-281T16:26:00,000T01:15:00,7-Oct-04,CIRS,SPASS Rider,Iapetus,GLOBCOLA,Global coverage observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.6 mrad, long~245 (Roncevaux Terra), phase~45.",,,,,, 2004-281T16:26:00,000T01:15:00,7-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-281T16:26:00,000T01:15:00,7-Oct-04,VIMS,SPASS Rider,Iapetus,GLOBCOLA,Global coverage observation,Iapetus southern anti-Saturn hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-281T20:00:00,000T00:30:00,7-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 124 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-AT-DI-EP-EN (602, 604, 611, 615, 616)]",,,,,, 2004-281T20:30:00,000T10:45:00,7-Oct-04,ISS,Prime,Phoebe,002PHO,Phoebe spectrophotometery,Phoebe Spectrophotometry,"Turn -Y to Phoebe, do during one Phoebe rotation 6 1x1 mosaics, 4 color, 3 polarizer filters, turn to WP.",,,,,, 2004-281T20:30:00,000T10:45:00,7-Oct-04,UVIS,SPASS Rider,Phoebe,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-282T08:44:00,000T09:00:00,8-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-282T19:14:00,000T01:00:00,8-Oct-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 015 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-282T20:14:00,000T04:15:00,8-Oct-04,UVIS,Prime,Saturn,MOS0AGEL,Apoapsis mosaic,MOSAIC_APO_01_10f,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to -MOS Orb. Rotate -64mrad in the YZ Plane. 2) Drift at a rate of .0134 mrad/sec about the Z-axis toward +MOS Orb for 13900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 100.18mrad.",,,,,, 2004-283T00:59:00,000T09:00:00,9-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-283T11:34:00,000T07:00:00,9-Oct-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:30.",,,,,, 2004-283T11:34:00,000T09:10:00,9-Oct-04,CAPS,SPASS Rider,InstrumentCalibration,CALIBRATE,Calibration,CAPS Calibration,"CAPS periodic gain test and calibration. The specified rate and data volume are the delta above the CAPS survey rate (1000 bps), and the rate is the average over the entire request (current plans are to conduct the test in two different rates.)",,,,,, 2004-283T11:34:00,000T20:25:00,9-Oct-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets,,,,,, 2004-283T11:34:00,000T07:00:00,9-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-283T11:34:00,000T20:25:00,9-Oct-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #23",Saturn Far Encounter Global Mosaic under Go-East Template #23. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-283T18:34:00,000T00:30:00,9-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 129 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-EN-DI-JA-PA (602, 604, 610, 616, 617)]",,,,,, 2004-283T19:04:00,000T04:00:00,9-Oct-04,ISS,Prime,Saturn,2X2MOVI2A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:30.",,,,,, 2004-283T19:04:00,000T04:00:00,9-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI2A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-283T23:04:00,000T00:30:00,9-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 130 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [TL-AT-PM-EP-HE (611, 612, 613, 615, 616)]",,,,,, 2004-283T23:34:00,000T05:30:00,9-Oct-04,ISS,Prime,Saturn,2X2MOVI3A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:30.",,,,,, 2004-283T23:34:00,000T05:30:00,9-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI3A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-284T05:04:00,000T00:30:00,10-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 131 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-AT-PM-EN-JA (602, 610, 611, 615, 616)]",,,,,, 2004-284T05:34:00,000T02:25:00,10-Oct-04,ISS,Prime,Saturn,2X2MOVI4A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:30.",,,,,, 2004-284T05:34:00,000T02:25:00,10-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI4A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-284T08:29:00,000T09:00:00,10-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-284T09:59:00,000T06:00:00,10-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-284T19:59:00,000T00:30:00,10-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 133 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-PM-AT-HE-JA (610, 612, 614, 615, 616)]",,,,,, 2004-284T20:29:00,000T10:50:00,10-Oct-04,UVIS,Prime,Saturn,MOS0AGEL,Apoapsis mosaic,MOSAIC_APO_01_10i,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to +MOS Orb. Rotate +64mrad in the YZ Plane. 2) Drift at a rate of .0143 mrad/sec about the Z-axis for 15000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 15000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis toward -MOS Orb for 7000s. 5) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb(+/-Range): 106.81mrad.",,,,,, 2004-285T07:19:00,000T00:30:00,11-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 134 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-EN-TL-DI-PA (602, 604, 611, 613, 617)]",,,,,, 2004-285T10:41:00,000T06:19:00,11-Oct-04,CDA,Non-SPASS,Saturn,PPL,Huygens Probe support,Probe Patch Load,Mute for PPL. Sleep/Mute Unmute/Active Commands pointing: NA; datavolume=0 MB,,,,,, 2004-285T10:42:00,000T00:17:00,11-Oct-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder,"Put CIRS to sleep/mute for probe patch load, mute at epoch -00:06",,,,,, 2004-285T10:43:00,000T00:10:00,11-Oct-04,INMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,INMS Sleep and Mute for Probe C/O,null,,,,,, 2004-285T10:44:00,000T00:09:50,11-Oct-04,ISS,Non-SPASS,Earth,SLEEPMUTE,Huygens probe support,put ISS to sleep for probe activity,placeholder activity put into CIMS to remenind ISS to go into sleep for probe activity at request of MAG TWT,,,,,, 2004-285T10:50:00,000T00:03:00,11-Oct-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (Probe Patch Load),UVIS to go to sleep/mute for Probe Patch Load (MGTWT request),,,,,, 2004-285T10:51:00,000T00:05:00,11-Oct-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE,VIMS to SLEEP/ MUTE,,,,,, 2004-285T10:53:00,000T06:07:00,11-Oct-04,INMS,Non-SPASS,SpacecraftActivity,MUTE,Instrument to sleep mode,INMS Mute for Probe Patch,null,,,,,, 2004-285T10:54:00,000T06:05:00,11-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-285T16:59:00,000T00:30:00,11-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-285T17:00:00,000T00:28:59,11-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-285T17:00:00,000T00:04:00,11-Oct-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,wake/unmute placeholder,"UNMUTE. Note power transients!, unmute at 00:06, wake at epoch+00:09",,,,,, 2004-285T17:00:00,000T00:04:00,11-Oct-04,INMS,Non-SPASS,SpacecraftActivity,UNMUTE,Huygens probe support,INMS UnMute after Probe Patch,null,,,,,, 2004-285T17:00:00,000T00:07:00,11-Oct-04,ISS,Non-SPASS,Earth,WAKESLEEP,Wakeup instrument from sleep mode,wake up ISS after probe activity,placeholder activity put into CIMS to remind ISS to wake up after probe activity at request of MAG TWT,,,,,, 2004-285T17:00:00,000T00:11:00,11-Oct-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after probe patch load,Unmute/go to active after probe patch load (MAGTWT request),,,,,, 2004-285T17:00:00,000T00:05:00,11-Oct-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode,VIMS to ACTIVE,,,,,, 2004-285T17:04:00,000T00:25:00,11-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-285T17:07:00,002T23:45:00,11-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-285T17:29:00,000T16:15:00,11-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-285T17:29:00,000T16:15:00,11-Oct-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-285T17:29:00,000T16:15:00,11-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-285T17:29:00,000T16:15:00,11-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-285T18:59:00,000T01:15:00,11-Oct-04,ISS,Prime,Iapetus,GLOBCOLB,Global coverage observation,Iapetus global color observation,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 25 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn -Y to WP,,,,,, 2004-285T18:59:00,000T01:15:00,11-Oct-04,CIRS,SPASS Rider,Iapetus,GLOBCOLB,Global coverage observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.75 mrad, long~220 (Roncevaux Terra), phase~58.",,,,,, 2004-285T18:59:00,000T01:15:00,11-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-285T18:59:00,000T01:15:00,11-Oct-04,VIMS,SPASS Rider,Iapetus,GLOBCOLB,Global coverage observation,Iapetus,Multiple 640ms 12x12 cubes (double resolution),,,,,, 2004-285T20:14:00,000T00:30:00,11-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 136 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EN-JA-PM-AT (602, 610, 615, 616, 617)]",,,,,, 2004-285T20:30:00,000T04:33:04,11-Oct-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-285T20:44:00,000T03:30:00,11-Oct-04,UVIS,Prime,Saturn,MOS0AGEM,Apoapsis mosaic,MOSAIC_APO_01_11b,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +64mrad in the YZ Plane. 2) Drift at a rate of .0147 mrad/sec about the Z-axis toward -MOS Orb for 10600s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 109.96mrad.",,,,,, 2004-286T00:44:00,000T09:00:00,12-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-286T09:44:00,000T03:13:00,12-Oct-04,INMS,Non-SPASS,Saturn,SURVEYB,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-286T09:44:00,002T00:55:00,12-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-286T09:44:00,002T07:30:00,12-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-286T09:44:01,002T00:41:59,12-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-286T11:14:00,000T06:25:00,12-Oct-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-286T11:14:00,000T11:40:00,12-Oct-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets with SATELORBS,,,,,, 2004-286T11:14:00,000T06:25:00,12-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-286T11:14:00,000T20:25:00,12-Oct-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #25",Saturn Far Encounter Global Mosaic under Go-East Template #25. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-286T12:57:00,000T00:33:00,12-Oct-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-286T13:30:00,001T20:58:00,12-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-286T17:39:00,000T00:30:00,12-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 139 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-EN-PM-AT-EP (602, 610, 611, 615, 616)]",,,,,, 2004-286T18:14:00,000T04:40:00,12-Oct-04,ISS,Prime,Saturn,2X2MOVI2A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-286T18:14:00,000T04:40:00,12-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI2A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-286T22:54:00,000T00:30:00,12-Oct-04,ISS,Prime,Iapetus,GLOBMAPC,Global coverage mapping,Iapetus global mapping,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 3 NAC color filters; turn to WP,,,,,, 2004-286T22:54:00,000T00:30:00,12-Oct-04,CIRS,SPASS Rider,Iapetus,GLOBMAPC,Global coverage mapping,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.75 mrad, long~230 (Roncevaux Terra), phase~65.",,,,,, 2004-286T22:54:00,000T00:30:00,12-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-286T23:29:00,000T04:40:00,12-Oct-04,ISS,Prime,Saturn,2X2MOVI3A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-286T23:29:00,000T08:05:00,12-Oct-04,CIRS,SPASS Rider,Saturn,ISSPCKT2I,Saturn movie,Saturn Movie pickets,Saturn Movie pickets and SATELORBs.,,,,,, 2004-286T23:29:00,000T04:40:00,12-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI3A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-287T04:09:00,000T00:30:00,13-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 140 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EP-EN-JA-DI (602, 604, 610, 611, 617)]",,,,,, 2004-287T04:39:00,000T02:55:00,13-Oct-04,ISS,Prime,Saturn,2X2MOVI4A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-287T04:39:00,000T02:55:00,13-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI4A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-287T08:14:00,000T09:00:00,13-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-287T08:44:00,000T06:00:00,13-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-287T18:49:00,000T00:30:00,13-Oct-04,ISS,Prime,Iapetus,LIMBTOPOD,Limb topography and geodesy observation,Iapetus limb topography and geodesy obs.,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 3 NAC color filters,,,,,, 2004-287T18:49:00,000T00:30:00,13-Oct-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOD,Limb topography and geodesy observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.1 mrad, long~220 (Roncevaux Terra), phase~80.",,,,,, 2004-287T18:49:00,000T00:30:00,13-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-287T19:19:00,000T01:20:00,13-Oct-04,ISS,Prime,Iapetus,HILLSPHEC,Hill sphere observation,Iapetus Hill sphere observation,Do 5x5 NAC clear filter mosaic of Hill sphere around Iapetus two times.,,,,,, 2004-287T19:19:00,000T01:20:00,13-Oct-04,CIRS,SPASS Rider,Iapetus,HILLSPHEC,Hill sphere observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.05 mrad, long~230 (W. Cassini Regio), phase~80.",,,,,, 2004-287T19:19:00,000T01:20:00,13-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-287T20:50:00,000T00:30:00,13-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 142 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [TL-PM-AT-EP-PA (611, 613, 615, 616, 617)]",,,,,, 2004-287T22:00:00,000T00:45:00,13-Oct-04,ISS,Prime,rings(general),RNGPHOTMA,Ring photometry,RING PHOTOM,3X3 NACS IN 5 COLORS ON RIGHT ANSA;,,,,,, 2004-287T22:45:00,000T01:00:00,13-Oct-04,RADAR,SPASS Rider,Other,ENGTEST,Engineering test,Engineering Test of Diagnostic Modes,Engineering test of diagnostic modes on the flight unit.,,,,,, 2004-288T00:04:00,000T07:30:00,14-Oct-04,UVIS,Prime,Saturn,MOS0AGEM,Apoapsis mosaic,MOSAIC_APO_01_11c,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0159 mrad/sec about the Z-axis for 15000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-Axis toward +MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 119.21mrad.",,,,,, 2004-288T10:26:00,000T06:21:00,14-Oct-04,CDA,Non-SPASS,Saturn,PPL,Huygens Probe support,Probe Patch Load BU,Mute for PPL. Sleep/Mute Unmute/Active activities for CDA pointing: NA; datavolume=0 MB,,,,,, 2004-288T10:27:00,000T00:17:00,14-Oct-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder,"Put CIRS to sleep/mute for probe patch load BU, mute at epoch -00:06",,,,,, 2004-288T10:28:00,000T00:10:00,14-Oct-04,INMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,INMS Sleep and Mute for Probe C/O,null,,,,,, 2004-288T10:29:00,000T00:09:50,14-Oct-04,ISS,Non-SPASS,Earth,SLEEPMUTE,Huygens probe support,put ISS to sleep for probe activity,placeholder activity put into CIMS to remenind ISS to go into sleep for probe activity at request of MAG TWT,,,,,, 2004-288T10:35:00,000T00:03:00,14-Oct-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE for probe patch backup,UVIS to go to sleep/mute for probe patch backup,,,,,, 2004-288T10:36:00,000T00:05:00,14-Oct-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE,VIMS to SLEEP/ MUTE,,,,,, 2004-288T10:38:00,000T06:07:00,14-Oct-04,INMS,Non-SPASS,SpacecraftActivity,MUTE,Instrument to sleep mode,INMS Mute for Probe Patch Back Up,null,,,,,, 2004-288T10:39:00,000T06:05:00,14-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-288T16:44:00,000T00:30:00,14-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-288T16:45:00,000T00:04:00,14-Oct-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,wake/unmute placeholder,"UNMUTE. Note power transients!, unmute at 00:06, wake at epoch+00:09",,,,,, 2004-288T16:45:00,000T00:04:00,14-Oct-04,INMS,Non-SPASS,SpacecraftActivity,UNMUTE,Huygens probe support,INMS UnMute after Probe Patch BackUp,null,,,,,, 2004-288T16:45:00,000T00:07:00,14-Oct-04,ISS,Non-SPASS,Earth,WAKESLEEP,Wakeup instrument from sleep mode,wake up ISS after probe activity,placeholder activity put into CIMS to remind ISS to wake up after probe activity at request of MAG TWT,,,,,, 2004-288T16:45:00,000T00:11:00,14-Oct-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after patch backup,Unmute/go to active after probe depassivation,,,,,, 2004-288T16:45:00,000T00:05:00,14-Oct-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode,VIMS to ACTIVE,,,,,, 2004-288T16:47:00,000T00:26:59,14-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,Dust Survey,survey measurement of dust,,,,,, 2004-288T16:49:00,002T20:08:00,14-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-288T16:52:00,003T16:38:00,14-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-288T17:14:00,000T16:30:00,14-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,Dust Survey,survey measurement of dust,,,,,, 2004-288T17:14:00,000T16:30:00,14-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-288T17:14:00,000T16:30:00,14-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-288T18:44:00,000T04:40:00,14-Oct-04,UVIS,Prime,Saturn,MOS0AGEN,Apoapsis mosaic,MOSAIC_APO_01_11d,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate +64mrad in the YZ Plane. 2) Drift at a rate of .0165 mrad/sec about the Z-axis toward +MOS Orb for 14800s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 123.40mrad.",,,,,, 2004-288T19:00:00,000T04:33:04,14-Oct-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-288T23:24:00,000T00:45:00,14-Oct-04,ISS,Prime,rings(general),RNGPHOTMA,Ring photometry,RING PHOTOMETRY OF RING ANSA,3X3 NACS IN 4 COLORS ON RIGHT ANSA,,,,,, 2004-288T23:24:00,000T00:45:00,14-Oct-04,UVIS,SPASS Rider,rings(general),RNGPHOTMA,Ring photometry,UV Ring Spectroscopy,,,,,,, 2004-288T23:24:00,000T00:45:00,14-Oct-04,VIMS,SPASS Rider,rings(general),RNGPHOTMA,Ring photometry,Ring Mosaic,TBD,,,,,, 2004-289T00:44:00,000T09:00:00,15-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-289T09:44:00,002T07:16:00,15-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-289T09:44:00,002T07:16:00,15-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-289T09:44:01,002T07:15:58,15-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,Dust Survey,survey measurement of dust,,,,,, 2004-289T11:14:00,000T06:25:00,15-Oct-04,ISS,Prime,Saturn,2X2MOVIEA,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-289T11:14:00,000T11:25:00,15-Oct-04,CIRS,SPASS Rider,Saturn,ISSPCKT20,Saturn movie,Saturn Movie pickets,Saturn Movie pickets and SATELORBS.,,,,,, 2004-289T11:14:00,000T06:25:00,15-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVIEA,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-289T11:14:00,000T20:25:00,15-Oct-04,VIMS,SPASS Rider,Saturn,FRGLOB,Saturn far encounter global mosaic,"Saturn Far Global Mosaic, Go-East Template #27",Saturn Far Encounter Global Mosaic under Go-East Template #27. 20-hour duration. 12 pickets acquired over these 20 hours. ISS movie pickets each last 1:00. Then CD CIRS observations for 45 minutes. Total cycle time is 1:45. Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits,,,,,, 2004-289T17:39:00,000T00:30:00,15-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 147 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [HE-PM-AT-PA-JA (610, 612, 615, 616, 617)]",,,,,, 2004-289T18:14:00,000T04:25:00,15-Oct-04,ISS,Prime,Saturn,2X2MOVI2A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-289T18:14:00,000T04:25:00,15-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI2A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-289T22:39:00,000T01:00:00,15-Oct-04,ISS,Prime,Iapetus,GLOBCOLF,Global coverage observation,Iapetus global color and global mapping observatio,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 25 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn -Y to WP,,,,,, 2004-289T22:39:00,000T01:00:00,15-Oct-04,CIRS,SPASS Rider,Iapetus,GLOBCOLF,Global coverage observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.2 mrad, long~200 (W. Cassini Regio), phase~95.",,,,,, 2004-289T22:39:00,000T01:00:00,15-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-289T22:39:00,000T01:00:00,15-Oct-04,VIMS,SPASS Rider,Iapetus,GLOBCOLF,Global coverage observation,Iapetus southern anti-Saturn hemisphere,Multiple 640ms 12x12 cubes (double resolution),,,,,, 2004-289T23:39:00,000T04:30:00,15-Oct-04,ISS,Prime,Saturn,2X2MOVI3A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-289T23:39:00,000T08:00:00,15-Oct-04,CIRS,SPASS Rider,Saturn,ISSPCKT2I,Saturn movie,Saturn Movie pickets,Saturn Movie pickets and SATELORBS.,,,,,, 2004-289T23:39:00,000T04:30:00,15-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI3A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-290T04:09:00,000T00:30:00,16-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 149 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-EN-TL-PM-DI (602, 604, 611, 613, 616)]",,,,,, 2004-290T04:44:00,000T02:55:00,16-Oct-04,ISS,Prime,Saturn,2X2MOVI4A,Saturn movie,Go east global Saturn movie,"2X2 Saturn mosaic + spoke movie, repeat every 1:45.",,,,,, 2004-290T04:44:00,000T02:55:00,16-Oct-04,UVIS,SPASS Rider,Saturn,2X2MOVI4A,Saturn movie,ISS 2X2MOVIEA Rider,UVIS EUV and FUV riding along with ISS 2X2MOVIEA observation,,,,,, 2004-290T08:15:00,000T09:00:00,16-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-290T18:45:00,000T00:45:00,16-Oct-04,ISS,Prime,Iapetus,LIMBTOPOG,Limb topography and geodesy observation,Iapetus limb topography and geodesy obs.,Turn -Y to Iapetus; Do 1x1 mosaic 2 NAC clear + 3 NAC color filters,,,,,, 2004-290T18:45:00,000T00:45:00,16-Oct-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOG,Limb topography and geodesy observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.28 mrad, long~200 (W. Cassini Regio), phase~100.",,,,,, 2004-290T18:45:00,000T00:45:00,16-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-290T18:45:00,000T00:45:00,16-Oct-04,VIMS,SPASS Rider,Iapetus,LIMBTOPOG,Limb topography and geodesy observation,Iapetus southern anti-Saturn hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-290T19:30:00,000T04:00:00,16-Oct-04,ISS,Prime,Iapetus,HILLSPHEF,Hill sphere observation,Iapetus Hill sphere observation,Do 5x5 NAC clear filter mosaic of Hill sphere around Iapetus two times.,,,,,, 2004-290T19:30:00,000T04:00:00,16-Oct-04,CIRS,SPASS Rider,Iapetus,HILLSPHEF,Hill sphere observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.3 mrad, long~210 (W. Cassini Regio), phase~100.",,,,,, 2004-290T19:30:00,000T04:00:00,16-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-290T23:49:00,000T07:30:00,16-Oct-04,UVIS,Prime,Saturn,MOS0AGEN,Apoapsis mosaic,MOSAIC_APO_01_12,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .0183 mrad/sec about the Z-axis for 15000s to +MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate toward -MOS Orb for 9500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 137.18mrad.",,,,,, 2004-291T08:00:00,000T09:00:00,17-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-291T12:57:00,000T00:33:00,17-Oct-04,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-291T13:30:00,000T03:30:00,17-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-291T17:00:00,000T16:30:00,17-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,Dust Survey,survey measurement of dust,,,,,, 2004-291T17:00:00,000T16:30:00,17-Oct-04,INMS,Non-SPASS,Saturn,SURVEYA,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-291T17:00:00,000T16:30:00,17-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-291T17:00:00,000T16:30:00,17-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-291T18:45:00,000T01:00:00,17-Oct-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 018 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-291T18:45:00,000T01:00:00,17-Oct-04,UVIS,SPASS Rider,rings(general),DIFFUSRNG,Diffuse ring observation,UV Ring Spectroscopy,,,,,,, 2004-291T19:00:00,000T06:49:36,17-Oct-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-291T19:45:00,000T00:45:00,17-Oct-04,ISS,Prime,Iapetus,GLOBMAPH,Global coverage mapping,Iapetus global mapping,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 3 NAC color filters; turn to WP.,,,,,, 2004-291T19:45:00,000T00:45:00,17-Oct-04,CIRS,SPASS Rider,Iapetus,GLOBMAPH,Global coverage mapping,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.25 mrad, long~200 (W. Cassini Regio), phase~100.",,,,,, 2004-291T19:45:00,000T00:45:00,17-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-291T19:45:00,000T00:45:00,17-Oct-04,VIMS,SPASS Rider,Iapetus,LIMBTOPOH,Limb topography and geodesy observation,Iapetus southern anti-Saturn hemisphere,Multiple 640ms 12x12 cubes,,,,,, 2004-291T20:30:00,000T00:30:00,17-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 154 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-DI-EN-AT-JA (602, 604, 610, 615, 617)]",,,,,, 2004-291T21:00:00,000T02:55:00,17-Oct-04,UVIS,Prime,Saturn,MOS0AGEO,Apoapsis mosaic,MOSAIC_APO_01_12a,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0192 mrad/sec about the Z-axis toward -MOS Orb for 8500s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 143.64mrad.",,,,,, 2004-292T00:30:00,000T09:00:00,18-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-292T09:30:00,005T23:31:00,18-Oct-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-292T09:30:00,010T08:14:00,18-Oct-04,CDA,Non-SPASS,DustRAM direction,SURAFTPPL,Dust survey,dust survey,Survey measurements of dust,,,,,, 2004-292T09:30:00,000T01:22:00,18-Oct-04,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,STARTUP,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2004-292T09:30:00,004T07:16:00,18-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps). Request includes clear of DPU timetagged buffer (commands left within from S2 SOI).,,,,,, 2004-292T09:30:00,004T07:16:00,18-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-292T09:30:00,004T07:16:00,18-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-292T10:52:00,004T22:24:00,18-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-292T11:00:00,000T20:25:00,18-Oct-04,CIRS,Prime,Saturn,COMPSITA,Sit and stare at one location to derive composition,CIRS_00ASA_COMPSITA13,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-292T11:00:00,000T20:25:00,18-Oct-04,ISS,SPASS Rider,Saturn,COMPSITA,Sit and stare at one location to derive composition,"Shutter, Linearity and RBI calibration",Linearity and Shutter cal and RBI cal,,,,,, 2004-292T11:00:00,000T20:25:00,18-Oct-04,UVIS,SPASS Rider,Saturn,COMPSITA,Sit and stare at one location to derive composition,UVIS Rider to CIRS Far Nadir Comp,UVIS Rider to CIRS Far-IR Nadir Comp,,,,,, 2004-292T11:00:00,000T20:25:00,18-Oct-04,VIMS,SPASS Rider,Saturn,GLOMAP,Saturn global map,Saturn GlobalMap: CIRS Ridealong,Saturn Global Map. Ridealong for first 20 hours of CIRS COMPSIT observation,,,,,, 2004-293T08:00:00,000T09:00:00,19-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-293T09:30:00,000T06:00:00,19-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-293T18:30:00,000T13:00:00,19-Oct-04,CIRS,Prime,Saturn,COMPSITB,Sit and stare at one location to derive composition,CIRS_00ASA_COMPSITB13,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-293T18:30:00,000T13:00:00,19-Oct-04,ISS,SPASS Rider,Saturn,COMPSITB,Sit and stare at one location to derive composition,Saturn BOTSIM imaging,Photometry/polarimetry,,,,,, 2004-293T18:30:00,000T13:00:00,19-Oct-04,UVIS,SPASS Rider,Saturn,COMPSITB,Sit and stare at one location to derive composition,UVIS Rider to CIRS Far Nadir Comp,UVIS Rider to CIRS Far-IR Nadir Comp,,,,,, 2004-293T18:30:00,000T13:00:00,19-Oct-04,VIMS,SPASS Rider,Saturn,GLOMAP,Saturn global map,Saturn GlobalMap: CIRS Ridealong #2,Saturn Global Map. Ridealong for first 20 hours of CIRS COMPSIT observation,,,,,, 2004-294T08:00:00,000T09:00:00,20-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-294T18:30:00,000T01:00:00,20-Oct-04,ISS,Prime,Iapetus,GRAYLITEK,Graylight observstion,Iapetus graylight observation,Turn to Iapetus; do 1x1 mosaic at various exposure times,,,,,, 2004-294T18:30:00,000T01:00:00,20-Oct-04,CIRS,SPASS Rider,Iapetus,GRAYLITEK,Graylight observstion,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~1.0 mrad, long~190 (W. Cassini Regio), phase~150.",,,,,, 2004-294T18:30:00,000T01:00:00,20-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-294T19:30:00,000T01:00:00,20-Oct-04,ISS,Prime,Iapetus,LIMBTOPOK,Limb topography and geodesy observation,Iapetus limb topography and geodesy obs.,Do 1x1 mosaic 2 NAC clear + 3 NAC color filters + various exp times for graylight; turn to WP.,,,,,, 2004-294T19:30:00,000T01:00:00,20-Oct-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOK,Limb topography and geodesy observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.9 mrad, long~170 (W. Cassini Regio), phase~150.",,,,,, 2004-294T19:30:00,000T01:00:00,20-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-294T20:30:00,000T00:30:00,20-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 163 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-DI-HE-AT-EP (604, 610, 611, 612, 615)]",,,,,, 2004-294T21:00:00,000T02:45:00,20-Oct-04,UVIS,Prime,Saturn,MOS0AGEP,Apoapsis mosaic,MOSAIC_APO_01_14a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-Axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .0238 mrad/sec about the Z-axis toward +MOS Orb for 7900s. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 177.50mrad",,,,,, 2004-295T00:15:00,000T09:00:00,21-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-295T11:45:00,000T01:00:00,21-Oct-04,ISS,Prime,Iapetus,LIMBTOPOL,Limb topography and geodesy observation,Iapetus limb topography and geodesy obs.,Turn -Y to Iapetus; do 1x1 mosaic 3 NAC clear + 3 NAC color filters for limbtopo; do various exp. times for graylight imaging; do two more NAC clear for limbtopo.,,,,,, 2004-295T11:45:00,000T01:00:00,21-Oct-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOL,Limb topography and geodesy observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.9 mrad, long~160 (W. Cassini Regio), phase~150.",,,,,, 2004-295T11:45:00,000T01:00:00,21-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-295T12:45:00,000T01:00:00,21-Oct-04,ISS,Prime,Iapetus,GRAYLITEL,Graylight observstion,Iapetus graylight observation,Do 1x1 mosaic NAC clear filters at various exposure times; do 2 NAC clear for limbtopo; turn to WP.,,,,,, 2004-295T12:45:00,000T01:00:00,21-Oct-04,CIRS,SPASS Rider,Iapetus,GRAYLITEL,Graylight observstion,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.9 mrad, long~180 (W. Cassini Regio), phase~160.",,,,,, 2004-295T12:45:00,000T01:00:00,21-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-295T13:45:00,000T00:30:00,21-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 166 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-PM-EN-DI-EP (602, 604, 611, 616, 617)]",,,,,, 2004-295T14:46:00,000T16:00:00,21-Oct-04,ISS,Prime,rings(general),RNGHAZARD,Diffuse ring satellite search,RING HAZARD AND SATELLITE SEARCH,SEARCH FOR DIFFUSE RINGS AND NEW SATELLITES AT EACH ANSAE WITH SINGLE WACS,,,,,, 2004-296T06:46:00,000T00:30:00,22-Oct-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,Early tour Hyperion color observation,"Turn to Hyperion; do multi-color NAC images; turn to WP. Was orbit determination, but changed to a satellite observation at SOP update.",,,,,, 2004-296T07:46:00,000T09:00:00,22-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-296T09:16:00,000T06:00:00,22-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-296T16:46:00,001T16:15:00,22-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-296T16:46:00,001T16:15:00,22-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-296T16:46:00,001T16:15:00,22-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-296T18:20:00,000T01:00:00,22-Oct-04,ISS,Prime,rings(general),DIFFUSRNG,Diffuse ring observation,"DIFFUSE RINGS, GO EAST TEMPLATE, 020 TH OBSERVATIO","DIFFUSE RINGS IN REV 00A, GO EAST TEMPLATE",,,,,, 2004-296T18:30:00,000T02:16:32,22-Oct-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-296T19:20:00,000T01:00:00,22-Oct-04,ISS,Prime,Iapetus,LIMBTOPOM,Limb topography and geodesy observation,Iapetus limb topography and geodesy obs.,Turn -Y to Iapetus; do 1x1 mosaic 2 NAC clear + 3 NAC color filters for limbtopo; do 5 NAC for dust search; do 2 NAC clear for limbtopo.,,,,,, 2004-296T19:20:00,000T01:00:00,22-Oct-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOM,Limb topography and geodesy observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.85 mrad, long~140 (W. Cassini Regio), phase~160.",,,,,, 2004-296T19:20:00,000T01:00:00,22-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-296T20:20:00,000T01:00:00,22-Oct-04,ISS,Prime,Iapetus,GRAYLITEM,Graylight observstion,Iapetus graylight observation,Do 1x1 mosaic 7 NAC clear filters (varying exposure times),,,,,, 2004-296T20:20:00,000T01:00:00,22-Oct-04,CIRS,SPASS Rider,Iapetus,GRAYLITEM,Graylight observstion,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.85 mrad, long~170 (W. Cassini Regio), phase~165.",,,,,, 2004-296T20:20:00,000T01:00:00,22-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-296T21:20:00,000T01:00:00,22-Oct-04,ISS,Prime,Iapetus,DUSTSEAR,Dust observation,Iapetus very high-phase Hill sphere obs.,Do 10 NAC clear and 5 NAC UV3 filter images (combined with polarizers); do 1 NAC clear for limbtopo; turn to WP,,,,,, 2004-296T21:20:00,000T01:00:00,22-Oct-04,CIRS,SPASS Rider,Iapetus,DUSTSEAR,Dust observation,Iapetus rider,"Integrate FP3, FP4 at high spectral resolution (0.5 cm-1). AD~0.8 mrad, long~140 (W. Cassini Regio), phase~165.",,,,,, 2004-296T21:20:00,000T01:00:00,22-Oct-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-296T22:20:00,000T01:25:00,22-Oct-04,UVIS,Prime,Saturn,MOS0AGEP,Apoapsis mosaic,MOSAIC_APO_01_15,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Drift at a rate of 0.0369 mrad/s about the z-axis from Saturn Center for 4100s toward -MOS Orb. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 221.48mrad.",,,,,, 2004-297T00:16:00,000T09:00:00,23-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-297T01:16:00,000T06:00:00,23-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-297T09:16:00,000T23:45:00,23-Oct-04,INMS,Non-SPASS,Saturn,PSTOTM004,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-297T10:46:00,000T12:45:00,23-Oct-04,ISS,Prime,Titan,MOVIEA,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 9 images every hour for duration,,,,,, 2004-297T10:46:00,000T12:45:00,23-Oct-04,VIMS,SPASS Rider,Titan,MOVIEA,Surface/winds/cloud movie,"Titan Movie, ridealong with ISS",Titan movie ride-along with ISS. Part 1 of 4 parts.,,,,,, 2004-298T00:01:00,000T09:00:00,24-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-298T09:01:00,001T07:30:00,24-Oct-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-298T09:01:00,001T05:49:00,24-Oct-04,INMS,Non-SPASS,Saturn,PSTOTM4BU,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-298T09:01:00,001T07:30:00,24-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-298T09:01:00,001T07:30:00,24-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-298T09:01:00,001T07:30:00,24-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-298T10:31:00,000T01:30:00,24-Oct-04,ISS,Prime,rings(general),RADCOLOR,Radial color scan,RING RADIAL COLOR SCAN,"RADIAL COLOR SCAN, 15 COLORS, NAC",,,,,, 2004-298T10:31:00,000T01:30:00,24-Oct-04,VIMS,SPASS Rider,rings(general),COMPLOLIT,Low phase sunlit ring radial scan,"radial scan, low phase, lit face.","Cube Size (X,Z) = 64*12 hires, 80 msec, + 12*12, 320 msec, Time per SC pointing (mins) = 3 Number of SC pointings = 16?, Time of observation (hours) = 1.5, Desc = ISS rider with ISS RAD_COLOR001 observation.",,,,,, 2004-298T12:01:00,000T11:55:00,24-Oct-04,ISS,Prime,Titan,MOVIEB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 9 images every hour for duration,,,,,, 2004-298T12:01:00,000T14:55:00,24-Oct-04,VIMS,SPASS Rider,Titan,MOVIEB,Surface/winds/cloud movie,"Titan Movie, ridealong with ISS",Titan movie ride-along with ISS. Part 2 of 4 parts.,,,,,, 2004-298T23:56:00,000T00:20:00,24-Oct-04,ISS,Prime,Titan,MOVIEB1,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 9 images every hour for duration,,,,,, 2004-298T23:56:00,000T03:00:00,24-Oct-04,RADAR,SPASS Rider,Other,WARMUP,RADAR warmup,"Distant Titan Latitude Study, Southern Latitudes",Warmup for calibration and science data collection.,,,,,, 2004-299T00:16:00,000T02:40:00,25-Oct-04,ISS,Prime,Titan,MOVIEB2,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 9 images every hour for duration,,,,,, 2004-299T02:56:00,000T01:20:00,25-Oct-04,RADAR,Prime,Titan,SOUTH7CAL,Distant Titan radiometery and calibration,"Distant Titan Radiometry, Southern Latitudes",Obtain distant Titan radiometer science and calibration data. One of a set that provides coverage of Titan southern latitude variation along with some obtainable associated longitude variation.,,,,,, 2004-299T04:16:00,000T00:10:00,25-Oct-04,ISS,Prime,Titan,MOVIEB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 9 images.,,,,,, 2004-299T04:16:00,000T00:10:00,25-Oct-04,VIMS,SPASS Rider,Titan,MOVIEB,Surface/winds/cloud movie,"Titan Movie, ridealong with ISS",Titan movie ride-along with ISS. Part 3 of 4 parts.,,,,,, 2004-299T04:26:00,000T01:40:00,25-Oct-04,RADAR,Prime,Titan,SOUTHSCAT,Distant Titan radiometery and calibration,"Distant Titan Scatterometry, Southern Latitudes",Obtain distant Titan scatterometry science and calibration data. One of a set that provides coverage of Titan southern latitude variation along with some obtainable associated longitude variation.,,,,,, 2004-299T06:06:00,000T00:55:00,25-Oct-04,ISS,Prime,Titan,MOVIEB,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds. 9 images twice.,,,,,, 2004-299T06:06:00,000T00:55:00,25-Oct-04,VIMS,SPASS Rider,Titan,MOVIEB,Surface/winds/cloud movie,"Titan Movie, ridealong with ISS",Titan movie ride-along with ISS. Part 4 of 4 parts.,,,,,, 2004-299T07:31:00,000T09:00:00,25-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-299T09:01:00,000T06:00:00,25-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCALTMP,Deep space calibration,Deep Space Calibration,Deep space cal.,,,,,, 2004-299T14:50:00,000T12:40:23,25-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-299T16:31:00,000T20:59:09,25-Oct-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-299T16:31:00,000T19:27:16,25-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps.,,,,,, 2004-299T16:31:00,000T20:59:09,25-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-299T16:31:01,000T21:13:46,25-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-299T17:16:09,000T00:14:00,25-Oct-04,ISS,Prime,Titan,LRMONITOR,Long range monitor,Long Range NAC Monitoring of Surface and Atmospher,"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2004-299T17:16:09,000T00:14:00,25-Oct-04,VIMS,SPASS Rider,Titan,ISS,,Dark_Side VIMS_4868,Ridealong with ISS Image. 64X64,,,,,, 2004-299T17:30:09,000T05:15:00,25-Oct-04,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2004-299T17:30:09,000T05:15:00,25-Oct-04,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (6 integrations total = 12 frames, 0.5 Mb/frame)",,,,,, 2004-299T17:30:09,000T05:15:00,25-Oct-04,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"wind/cloud motions, 3-12 km/px, 3 images/timestep in CB1 filter to increase SNR, 12-bit lossless",,,,,, 2004-299T17:30:09,000T05:15:00,25-Oct-04,VIMS,SPASS Rider,Titan,MIDIR,Mid infrared thermal map,Dark_Side VIMS_4868,Ridealong with CIRS MID IR Temp map. Mode will be 64 square for entire period.,,,,,, 2004-299T22:45:09,000T01:15:00,25-Oct-04,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,NMA (NAC Monitoring of Surface and Atmosphere),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2004-299T22:45:09,000T01:15:00,25-Oct-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,,Ride-along with ISS.,,,,,, 2004-299T22:45:09,000T01:15:00,25-Oct-04,VIMS,SPASS Rider,Titan,ISS,,Dark_Side VIMS_4868,Ridealong with ISS Monitor (both NAC & WAC). 64X64 all the way.,,,,,, 2004-300T00:00:09,000T04:00:00,26-Oct-04,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2004-300T00:00:09,000T04:00:00,26-Oct-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2004-300T00:00:09,000T04:00:00,26-Oct-04,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"wind/cloud motions, 3-12 km/px, 3 images/timestep in CB1 filter to increase SNR, 12-bit lossless",,,,,, 2004-300T00:00:09,000T04:00:00,26-Oct-04,VIMS,SPASS Rider,Titan,FARIRNAD,,Dark_Side VIMS_4868,Ridealong with CIRS Far IR nadir comp map. Sit and stare. Mode will be 64 square for entire period.,,,,,, 2004-300T03:30:23,000T10:59:46,26-Oct-04,INMS,Non-SPASS,Titan,TAINBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-300T04:00:09,000T06:30:00,26-Oct-04,VIMS,Prime,Titan,MEDRES,Medium resolution global mapping,Med_Res_Regional VIMS_4868,"Medium resolution global mapping. Start sequence with 64X64, and then do a 3X2 mosaic (64 hi-res mode) with at least 2 integration times.",,,,,, 2004-300T04:00:09,000T06:30:00,26-Oct-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,,Ride-along with VIMS. 1 minute dwells.,,,,,, 2004-300T04:00:09,000T06:30:00,26-Oct-04,ISS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,WMO (WAC Movie),"wind/cloud motions, 3-12 km/px, 3 images/timestep in CB1 filter to increase SNR, 12-bit lossless",,,,,, 2004-300T04:00:09,000T06:30:00,26-Oct-04,UVIS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2004-300T10:15:09,000T03:27:00,26-Oct-04,RADAR,SPASS Rider,Titan,TAWARMUP,,Warmup for Ta Radiomeetry,Warmup needed for Radiometry period following,,,,,, 2004-300T10:30:09,000T01:40:00,26-Oct-04,ISS,Prime,Titan,REGMAP,Regional mapping,NRM (NAC Regional Map),regional map,,,,,, 2004-300T10:30:09,000T03:12:00,26-Oct-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,,Ride-along with ISS.,,,,,, 2004-300T10:30:09,000T03:12:00,26-Oct-04,VIMS,SPASS Rider,Titan,HIGHRES,High resolution observartion,Dark_Side VIMS_4868,Ridealong with ISS High Res. 12X12 all the way.,,,,,, 2004-300T11:58:16,000T07:03:46,26-Oct-04,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,TA Flyby,"TA is the first close encounter at Titan at 1200 km during the Cassini mission and thus the first encounter after the Voyager-1 encounter in November 1980. It will thus be of extreme scientific interest to the mission, the science community and for PR purposes. If the various approaches to obtain an improved neutral atmosphere model of Titan during this encounter possibly find a denser atmosphere, it may turn out to be among the closest encounters of the whole mission. The trajectory is on the downstream or wake side and therefore very suitable for studies of the tail formation processes. It thus has to be of highest priority i.e. grade 1 priority which assumes +- four hours (total duration eight hours) of high resolution data at 1976 bps (32 vps) total around closest approach.",,,,,, 2004-300T12:10:09,000T01:31:00,26-Oct-04,ISS,Prime,Titan,HIRESNAC,High resolution map,HRI (High Resolution Imaging),"high-resolution imaging, 50-200 m/px, special targets, emission angles < 45 prefer IR-polarizer (phase 45-110)",,,,,, 2004-300T13:30:09,000T01:21:00,26-Oct-04,CAPS,SPASS Rider,Titan,TAINBND,,MAPS 00ATI Campaign,Part of 00ATI MAPS Campaign. Inbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2004-300T13:30:09,000T01:32:30,26-Oct-04,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2004-300T13:42:09,000T00:21:00,26-Oct-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,,"Ride-along with VIMS landing site obs, actually during RCS/RWA transition.",,,,,, 2004-300T13:42:09,000T00:21:00,26-Oct-04,ISS,SPASS Rider,Titan,RADRCS,,RCS/RWA Transition Imaging,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2004-300T13:42:09,000T00:21:49,26-Oct-04,VIMS,SPASS Rider,Titan,TRANS,,Hi_Res_Trans VIMS_4868,"During the transition from RW to thrusters, take two 64 square cubes if possible.",,,,,, 2004-300T13:44:36,000T00:45:33,26-Oct-04,MIMI,SPASS Rider,Titan,TAINBND,,MAPS 00ATI(TA) Campaign,"Part of 00ATI(TA) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-300T14:02:09,000T00:02:00,26-Oct-04,ISS,Prime,Titan,WAYPTTURN,Waypoint turn,Return To Waypoint Following Transition,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2004-300T14:11:09,000T00:34:00,26-Oct-04,RADAR,Prime,Titan,TAINSCAT,,Inbound Scatterometry of Ta,Inbound Scatterometry during Ta flyby,,,,,, 2004-300T14:30:09,000T02:00:00,26-Oct-04,MIMI,SPASS Rider,Titan,TACLOSE,,MAPS 00ATI(TA) Campaign,"Part of 00ATI(TA) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-300T14:30:09,000T00:47:00,26-Oct-04,INMS,Non-SPASS,Titan,TACLOSE,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-300T14:45:09,000T00:33:00,26-Oct-04,VIMS,Prime,Titan,HIRES,High resolution image,Hi_Res_Regional VIMS_4868,"High resolution, low phase angle mapping. Line of 64X64 cubes probabaly best.",,,,,, 2004-300T14:45:09,000T00:32:00,26-Oct-04,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,,Ridealong with VIMS,,,,,, 2004-300T14:45:09,000T00:32:00,26-Oct-04,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"wind/cloud motions, 3-12 km/px, 3 images/timestep in CB1 filter to increase SNR, 12-bit lossless",,,,,, 2004-300T14:51:09,000T01:18:00,26-Oct-04,CAPS,SPASS Rider,Titan,TACLOSE,,MAPS 00ATI Campaign,Part of 00ATI MAPS Campaign. Observations of Titan's interaction with Saturn's magnetosphere,,,,,, 2004-300T15:02:39,000T00:21:30,26-Oct-04,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2004-300T15:17:09,000T00:13:00,26-Oct-04,INMS,SPASS Rider,Titan,TARAMPNT,,MAPS TOST Campaign,Ta is an engineering pass,,,,,, 2004-300T15:18:09,000T00:12:00,26-Oct-04,RADAR,Prime,Titan,TAPT4INMS,,TA Ride Along SAR,Ride along SAR of Titan with INMS.,,,,,, 2004-300T15:24:09,000T00:33:30,26-Oct-04,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2004-300T15:30:09,000T00:06:00,26-Oct-04,RADAR,Prime,Titan,TAHIGHSAR,,High Resolution SAR Imaging of Titan,High resolution SAR imaging of Titan during closest approach period,,,,,, 2004-300T15:30:09,000T01:00:00,26-Oct-04,INMS,Non-SPASS,Titan,TACLOSE,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-300T15:36:09,000T00:10:00,26-Oct-04,RADAR,Prime,Titan,TALOWSAR,,Low Resolution SAR Imaging of Ta,Low resolution SAR imaging during the post-closest approach time period,,,,,, 2004-300T15:46:09,000T00:14:00,26-Oct-04,RADAR,Prime,Titan,TAOUTALT,,Outbound Altimetry on Ta,Altimetry taken during the outbound trajectory of Ta,,,,,, 2004-300T15:57:39,000T01:32:30,26-Oct-04,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2004-300T16:00:09,000T00:45:00,26-Oct-04,RADAR,Prime,Titan,TAOUTSCAT,,Outbound Scatterometry of Ta,Outbound Scatterometry during Ta flyby,,,,,, 2004-300T16:09:09,000T01:21:00,26-Oct-04,CAPS,SPASS Rider,Titan,TAOUTBND,,MAPS 00ATI Campaign,Part of 00ATI MAPS Campaign. Outbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2004-300T16:30:09,000T01:14:13,26-Oct-04,MIMI,SPASS Rider,Titan,TAOUTBND,,MAPS 00ATI(TA) Campaign,"Part of 00ATI(TA) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-300T16:30:09,000T11:00:00,26-Oct-04,INMS,Non-SPASS,Titan,TAOUTBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-300T17:09:09,000T03:21:00,26-Oct-04,RADAR,Prime,Titan,TAOUTRAD,,Outbound Radiometry of Ta,Outbound Radiometry following the Ta flyby,,,,,, 2004-300T17:30:09,000T15:59:37,26-Oct-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-300T17:30:09,000T12:29:37,26-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-300T17:44:47,000T11:05:12,26-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-300T19:02:02,000T14:13:58,26-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps).,,,,,, 2004-300T20:30:09,000T03:15:00,26-Oct-04,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2004-300T20:30:09,000T03:15:00,26-Oct-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,,Ride-along with UVIS.,,,,,, 2004-300T20:30:09,000T03:15:00,26-Oct-04,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,WPH (WAC Photometry),"particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2004-300T20:30:09,000T03:15:00,26-Oct-04,VIMS,SPASS Rider,Titan,DARKSIDE,Dark side imaging,Dark_Side VIMS_4868,Dark side observations of TItan.,,,,,, 2004-301T00:16:00,000T09:00:00,27-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-301T03:30:09,000T13:44:51,27-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-301T04:50:01,000T04:40:00,27-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-301T06:00:00,000T03:30:00,27-Oct-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-301T09:16:00,001T23:59:00,27-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-301T09:30:00,003T12:20:00,27-Oct-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-301T09:30:00,002T05:30:00,27-Oct-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-301T09:30:01,000T14:29:59,27-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-301T10:40:00,000T00:30:00,27-Oct-04,ISS,Prime,rings(general),DIFFRNGLP,Diffuse ring observation,DIFFUSE RING SEARCH,"5 WACS at left ansa, covering F region thru E region, for diffuse rings at low phase and elevation angles.",,,,,, 2004-301T11:10:00,000T06:05:00,27-Oct-04,CIRS,Prime,rings(general),SUBMU07LP,Ring radial scan,CIRS_00ARI_SubmU07LP,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-301T11:10:00,000T06:05:00,27-Oct-04,CIRS,SPASS Rider,rings(general),SUBML07LP,Ring radial scan,CIRS_00ARI_SUBML07LP_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-301T11:10:00,000T06:05:00,27-Oct-04,UVIS,SPASS Rider,rings(general),SUBMU07LP,Ring radial scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-301T17:15:00,000T02:15:00,27-Oct-04,VIMS,Prime,rings(general),COMPLODRK,Low phase dark side ring radial scan,"radial scan, low phase, dark face","Cube Size (X,Z) = 64*12 hires, tau_IR=160 & 640 msec, Time per SC pointing (mins) = 11, Number of SC pointings = 10, Time of observation (hours) = 2.25, Desc = Obtain a complete hi-res radial scan of the dark face of the A, B and C rings, at low phase angle, on right ansa. Orient X-axis along scan direction (radial).",,,,,, 2004-301T17:15:00,000T02:15:00,27-Oct-04,CIRS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,CIRS_00ARI_COMPLODRK_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-301T17:15:00,000T02:15:00,27-Oct-04,CIRS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,CIRS_00ARI_COMPLODRK,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-301T17:15:00,000T02:15:00,27-Oct-04,ISS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,RING RADIAL SCAN IN WACS,VIMS RADIAL SCAN RIDE ALONG: 3 WAC FTPRINTS /ANSA X 6 COLORS X 2 ANSAE,,,,,, 2004-301T17:15:00,000T02:15:00,27-Oct-04,UVIS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-301T17:15:00,000T02:15:00,27-Oct-04,INMS,Non-SPASS,Saturn,INMAGCOMP,Inner magnetospheric composition,Field Aligned Flows ridealong,Inner Magnetospheric Composition Ridealong for field aligned flows.,,,,,, 2004-301T19:30:00,000T04:00:00,27-Oct-04,ISS,Prime,RingC,ANSAMOVIE,Ring ansa movie,ANSA MOVIE OF C RING GAPS,HI RES PING-PONG MOVIE OF MAXWELL GAP and COLOMBO GAP: ONE IMAGE ON EACH FEATURE ON RIGHT ANSA EVERY 6 MINUTES,,,,,, 2004-301T19:30:00,000T04:00:00,27-Oct-04,CIRS,SPASS Rider,RingC,ANSAMOVIE,Ring ansa movie,CIRS_00ARC_ANSAMOVIE,Ride with ISS,,,,,, 2004-301T19:30:00,000T05:24:00,27-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-302T00:00:00,000T15:10:00,28-Oct-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-302T00:00:00,000T06:00:00,28-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-302T00:30:00,000T05:30:00,28-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-302T00:54:00,000T05:36:00,28-Oct-04,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"MAPS Mag Survery, INMS switches to InnerMag inside 8 Rs.",,,,,, 2004-302T03:35:00,000T14:00:00,28-Oct-04,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. Need to do this inside 6 RS on at least half of the periapses inside of 6RS. No pointing requirement",,,,,, 2004-302T06:30:00,000T00:45:00,28-Oct-04,ISS,Prime,Tethys,GLOCOL,Global coverage mapping,TETHYS global color mapping,"1;Turn -Y to Tethys, offset (0,30,0). Use 7DELTA_BODY to position NAC FOV to one side of Tethys; Do 5x1 mosaic 3 NAC color + 3 NAC polarizer (GRN), range 255000km, Dwell longest in center panel for BOTSIMs",,,,,, 2004-302T06:30:00,000T00:45:00,28-Oct-04,CIRS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys Ridealong - ISS,"Ride with ISS. Phase=49, Sub-S/C=(22, 270), LT=13.3, AD=4.2 mrad.",,,,,, 2004-302T06:30:00,000T05:25:00,28-Oct-04,INMS,SPASS Rider,Saturn,INMAGCOMP,Inner magnetospheric composition,Corotation Ridealong,Inner Magnetospheric Composition Ridealong for field aligned flows.,,,,,, 2004-302T06:30:00,000T00:45:00,28-Oct-04,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-302T06:30:00,000T00:45:00,28-Oct-04,VIMS,SPASS Rider,Tethys,COMP,Sit and stare to derive composition,Comp VIMS_4868,"Ridealong observation. First opportunity to do low resolution compositional mapping of Tethys. POINTING ERROR ~ 10 mrad in x-direction. ISS to redesign to a 1x5 NAC mosaic, one long dwell for vims to do 64x12 during the long one, then 12x12 or whatever fites in the other. original: Ten 12X12 images, with 2-3 integration times interspersed. Some phase angle coverage.",,,,,, 2004-302T07:15:00,000T01:45:00,28-Oct-04,CIRS,Prime,RingC,SHADCIN,Ring shadow scan,CIRS_00ARC_SHADCIN,"Longitudinal scan of ring in the early mission (highest temperature contrasts), in and around shadow, Low Phase, lit face, dawn side -Y to ring, +Z perpendicular to rings (if not possible, +Z parallel to pole)",,,,,, 2004-302T07:15:00,000T01:45:00,28-Oct-04,CIRS,SPASS Rider,RingA,SHADCIN,Ring shadow scan,CIRS_00ARA_SHADCIN_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-302T07:15:00,000T01:45:00,28-Oct-04,UVIS,SPASS Rider,RingC,SHADCIN,Ring shadow scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-302T07:15:00,000T01:45:00,28-Oct-04,VIMS,SPASS Rider,RingC,SHADCIN,Ring shadow scan,C ring shadow scans,"Cube Size (X,Z) = 64*12, tau_IR = 160 & 640 msec, Time per SC pointing (mins) = 10, Number of SC pointings = 6/hr, Rider on CIRS azimuthal scans across planet shadow entry on C ring.",,,,,, 2004-302T09:00:00,000T03:00:00,28-Oct-04,CIRS,Prime,RingC,SHADA,Ring shadow scan,CIRS_00ARC_SHADA,"Longitudinal scan of ring in the early mission (highest temperature contrasts), in and around shadow, Low Phase, lit face, dawn side -Y to ring, +Z perpendicular to rings (if not possible, +Z parallel to pole)",,,,,, 2004-302T09:00:00,000T03:00:00,28-Oct-04,CIRS,SPASS Rider,RingA,SHADA,Ring shadow scan,CIRS_00ARA_SHADA_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-302T09:00:00,000T03:00:00,28-Oct-04,VIMS,SPASS Rider,RingA,SHADA,Ring shadow scan,A ring shadow scans,"Cube Size (X,Z) = 64*12, tau_IR = 640 msec, Time per SC pointing (mins) = 10, Number of SC pointings = 6/hr, Rider on CIRS azimuthal scans across planet shadow on A ring.",,,,,, 2004-302T09:35:00,000T00:15:00,28-Oct-04,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2004-302T10:35:00,000T00:05:00,28-Oct-04,RPWS,Non-SPASS,Saturn,HRSED,Highest resolution saturn kilometric radiation observation,Highest Resolution SED Observations,"Obtain the highest resolution observations of Saturn Electrostatic Discharges (SED) by using the RPWS HF-WBR mode at ~180 kbps within 6 RS for a total of 60 minutes within the first 12 periapses inside of 6 RS. Results will help to verify the source as lightning, or provide evidence that they could be of some other origin (e.g. rings). No attitude requirement.",,,,,, 2004-302T11:55:00,000T07:50:00,28-Oct-04,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"MAPS magnetospheric survey, INMS switches to OuterMag outbound.",,,,,, 2004-302T12:00:00,000T02:00:00,28-Oct-04,CIRS,Prime,RingC,SHADCOUT,Ring shadow scan,CIRS_00ARC_SHADCOUT,"Longitudinal scan of ring in the early mission (highest temperature contrasts), in and around shadow, Low Phase, lit face, dawn side -Y to ring, +Z perpendicular to rings (if not possible, +Z parallel to pole)",,,,,, 2004-302T12:00:00,000T02:00:00,28-Oct-04,CIRS,SPASS Rider,RingC,SHADCOUT,Ring shadow scan,CIRS_00ARC_SHADCOUT_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-302T12:00:00,000T02:00:00,28-Oct-04,UVIS,SPASS Rider,RingC,SHADCOUT,Ring shadow scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-302T12:00:00,000T02:00:00,28-Oct-04,VIMS,SPASS Rider,RingC,SHADCOUT,Ring shadow scan,C ring shadow scans,"Cube Size (X,Z) = 64*12, tau_IR = 640 msec, Time per SC pointing (mins) = 10, Number of SC pointings = 6/hr, Rider on CIRS azimuthal scans across planet shadow exit on C ring.",,,,,, 2004-302T14:00:00,000T02:15:00,28-Oct-04,VIMS,Prime,rings(general),COMPHIDRK,High phase dark side ring radial scan,"radial scan, high phase, dark face","Cube Size (X,Z) = 64*12 lores, tau_IR=160 & 640 msec, Time per SC pointing (mins) = 11, Number of SC pointings = 9 (?), Time of observation (hours) = 2.25, Desc = Obtain a complete hi-res radial scan of the dark face of the A, B and C rings, at high phase angle, on left ansa. Orient X-axis along scan direction (radial). Add extra cubes at each end to allow for 24 mrad pointing errors.",,,,,, 2004-302T14:00:00,000T02:15:00,28-Oct-04,CIRS,SPASS Rider,rings(general),COMPHIDRK,High phase dark side ring radial scan,CIRS_00ARI_COMPHIDRK_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-302T14:00:00,000T02:15:00,28-Oct-04,CIRS,SPASS Rider,rings(general),COMPHIDRK,High phase dark side ring radial scan,CIRS_00ARI_COMPHIDRK,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-302T14:00:00,000T02:15:00,28-Oct-04,ISS,SPASS Rider,rings(general),COMPHIDRK,High phase dark side ring radial scan,RING MOSAIC IN WACS,VIMS RIDE ALONG?: 5 2X1 WAC FTPRINTS X 6 COLORS,,,,,, 2004-302T14:00:00,000T02:15:00,28-Oct-04,UVIS,SPASS Rider,rings(general),COMPHIDRK,High phase dark side ring radial scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-302T15:10:00,000T03:55:00,28-Oct-04,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-302T16:15:00,000T02:45:00,28-Oct-04,ISS,Prime,rings(general),DIFFRNGHP,Diffuse ring observation,DIFFUSE RING SEARCH,"2x7 MOS, 5 COLORS, Left ANSAE OUT PAST E RING",,,,,, 2004-302T16:15:00,000T02:45:00,28-Oct-04,CIRS,SPASS Rider,rings(general),DIFF01,,CIRS_00ARI_DIFF01,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-302T17:45:00,000T01:15:00,28-Oct-04,CDA,Non-SPASS,RingE,ERING,E ring observation,Ering 7Rs,"within Ering, 7 to 8 Rs, pointing=CDA to Kepler RAM or windshield-wiper mode or roll;rate=524",,,,,, 2004-302T19:00:00,000T02:05:00,28-Oct-04,CDA,Prime,RingE,RPC,Ring plane crossing,Ring Plane Crossing @ 8 Rs,"Ring Plane Crossing @ 302T20:15?, pointing=CDA to Kepler RAM or windshield-wiper mode or roll;rate=524",,,,,, 2004-302T19:00:00,000T02:16:32,28-Oct-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-302T19:05:00,000T14:10:00,28-Oct-04,MIMI,SPASS Rider,DustRAM direction,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS MAGDYN Campaign,"Part of MAGDYN MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-302T19:17:00,000T02:00:00,28-Oct-04,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2004-302T19:45:00,000T13:30:00,28-Oct-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-302T21:05:00,000T01:40:00,28-Oct-04,CDA,Non-SPASS,RingE,ERING,E ring observation,Ering 8Rs,"within Ering, 8 Rs, pointing=CDA to Kepler RAM or windshield-wiper mode or roll;rate=524",,,,,, 2004-302T21:15:00,000T02:30:00,28-Oct-04,ISS,Prime,RingF,HIPHLFMOV,High phase F ring movie,Hi phase ansa F ring movie at high res,"Ansa movie of the F RING at HIGH RES, HIGH PHASE, LIT FACE.",,,,,, 2004-302T21:15:00,000T02:30:00,28-Oct-04,CIRS,SPASS Rider,rings(general),DIFF02,,CIRS_00ARI_DIFF02,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-302T21:15:00,000T02:30:00,28-Oct-04,VIMS,SPASS Rider,RingF,HIPHLFMOV,High phase F ring movie,ISS_00ARF_HIPHLFMOV Ride Along,"Stare at F Ring ansa. VIMS unc. data vol = 98 Mb, compressed = 49 Mbits. Instrument params: size = 32x32 centered on NAC, IRint = 320 msec. VIS on. Countinuous cube generation for entire 2.3 hour duration of observation.",,,,,, 2004-302T22:45:00,017T09:04:00,28-Oct-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,Survey measurements of dust in ram direction or S/C roll,,,,,, 2004-302T23:00:00,000T00:29:49,28-Oct-04,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2004-303T00:15:00,000T09:00:00,29-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-303T09:15:00,000T14:56:00,29-Oct-04,MIMI,SPASS Rider,DustRAM direction,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS MAGDYN Campaign,"Part of MAGDYN MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-303T09:15:00,001T00:15:00,29-Oct-04,INMS,Non-SPASS,Saturn,PSTOTM005,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-303T09:15:00,001T00:45:00,29-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-303T09:45:00,000T02:30:00,29-Oct-04,VIMS,Prime,rings(general),COMPHILI,High phase sunlit ring radial scan,"radial scan, high phase, sunlit face","Cube Size (X,Z) = 64*6 hires, tau_IR=160/640msec, Time per SC pointing (mins) = 5 to coordinate wiuth ISS_NAC scan. Number of SC pointings = 14(?). Time of observation (hours) = 2.5, Desc = Obtain a complete hi-res radial scan of the sunlit face of the A, B and C rings, at high phase angle, on right ansa. Orient X-axis along scan direction (radial). First 15 min intended for CIRS deep-space cal, if possible.",,,,,, 2004-303T09:45:00,000T02:30:00,29-Oct-04,CIRS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,CIRS_00ARI_COMPHILIT_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-303T09:45:00,000T02:30:00,29-Oct-04,CIRS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,CIRS_00ARI_COMPHILIT,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-303T09:45:00,000T02:30:00,29-Oct-04,ISS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,RING RADIAL SCAN,25 NACS (CLR) AND 3 WACS (3 COLORS EA) IN A RIDE ALONG RAD SCAN ON LF/HI PH ON EACH ANSA,,,,,, 2004-303T09:45:00,000T02:30:00,29-Oct-04,UVIS,SPASS Rider,rings(general),COMPHILI,High phase sunlit ring radial scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-303T12:15:00,000T04:45:00,29-Oct-04,CIRS,Prime,rings(general),SUBML06HP,Ring radial scan,CIRS_00ARI_SubmL06HP,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-303T12:15:00,000T04:45:00,29-Oct-04,CIRS,SPASS Rider,rings(general),SUBML06HP,Ring radial scan,CIRS_00ARI_SUBML06HP_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-303T12:15:00,000T04:45:00,29-Oct-04,UVIS,SPASS Rider,rings(general),SUBML06HP,Ring radial scan,,UV spectral mapping of Saturn's rings.,,,,,, 2004-303T15:00:00,001T06:50:00,29-Oct-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-303T17:00:00,000T07:00:00,29-Oct-04,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,latitude-phase coverage: 3x1 mosaic on each ansa,"Orbits = 00A-00B, Cube Size (X,Z) = 64*64, 160/640 msec, Time per SC pointing (mins) = 60, Number of SC pointings = 6, Time of observation (hours) = 6.0, Volume (Mbits) = 104 Desc = Obtain 3x1 mosaic on each ring ansa on sunlit face. Distance 20 R_S.",,,,,, 2004-303T17:00:00,000T07:00:00,29-Oct-04,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_007RI_LATPHASE_SI,Rider on Latphase,,,,,, 2004-303T17:00:00,000T07:00:00,29-Oct-04,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_00ALATPHASE,"Stare at West ansa, low phase, lit face -Y to ring, +Z parallel to equator",,,,,, 2004-303T17:00:00,000T07:00:00,29-Oct-04,ISS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,Rev A ring photometry,TWT RINGS; rider,,,,,, 2004-303T17:00:00,000T07:00:00,29-Oct-04,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,,UV spectral mapping of Saturn's rings.,,,,,, 2004-304T00:11:00,000T21:39:00,30-Oct-04,MIMI,SPASS Rider,DustRAM direction,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS MAGDYN Campaign,"Part of MAGDYN MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-304T00:30:00,000T09:00:00,30-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-304T01:00:00,000T02:16:32,30-Oct-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-304T01:30:00,000T03:00:00,30-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-304T09:30:00,002T07:05:00,30-Oct-04,INMS,Non-SPASS,Saturn,PSTOTM5BU,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-304T10:00:00,000T07:00:00,30-Oct-04,CIRS,Prime,RingA,COMPA,Sit and stare to derive composition,CIRS_00ARA_COMPA,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-304T10:00:00,000T07:00:00,30-Oct-04,CIRS,SPASS Rider,RingA,COMPA,Sit and stare to derive composition,CIRS_00ARA_COMPA_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-304T10:00:00,000T07:00:00,30-Oct-04,UVIS,SPASS Rider,RingA,COMPA,Sit and stare to derive composition,,UV spectral mapping of Saturn's rings.,,,,,, 2004-304T10:00:00,000T05:00:00,30-Oct-04,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required. Includes 2 hours for IFC cal and range checks.",,,,,, 2004-304T15:00:00,000T06:50:00,30-Oct-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-304T17:00:00,000T11:15:00,30-Oct-04,CIRS,Prime,Saturn,FIRMAP,Far infrared map,CIRS_00ASA_FIRMAP01,"Far-IR hemisphere mapping. Scan in the N/S direction at 25 microrad/s. POINTING: -y to Saturn, +x to pole",,,,,, 2004-304T17:00:00,000T11:15:00,30-Oct-04,CIRS,SPASS Rider,Saturn,FIRMAP,Far infrared map,CIRS_00ASA_FIRMAP_SI,Saturn FIRMAP SI,,,,,, 2004-304T17:00:00,000T11:15:00,30-Oct-04,UVIS,SPASS Rider,Saturn,FIRMAP,Far infrared map,EUVFUV FIRMAP Rider,UVIS EUV and FUV riding along with CIRS FIRMAP observation,,,,,, 2004-304T17:00:00,000T11:15:00,30-Oct-04,VIMS,SPASS Rider,Saturn,CYLMAP,Saturn cylindrical map,Saturn Cylindricalk Map: CIRS Ridealong,Saturn Cylindrical Map. Ridealong with CIRS observation,,,,,, 2004-304T21:50:00,001T18:45:00,30-Oct-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-304T21:50:00,001T18:45:00,30-Oct-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-304T21:50:00,001T18:45:00,30-Oct-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-304T21:50:01,001T18:44:59,30-Oct-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-305T04:15:00,000T02:45:00,31-Oct-04,CIRS,Prime,RingC,COMPC,Sit and stare to derive composition,CIRS_00ARC_COMPC,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-305T04:15:00,000T02:45:00,31-Oct-04,CIRS,SPASS Rider,RingC,COMPC,Sit and stare to derive composition,CIRS_00ARC_COMPC_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-305T04:15:00,000T02:45:00,31-Oct-04,UVIS,SPASS Rider,RingC,COMPC,Sit and stare to derive composition,,UV spectral mapping of Saturn's rings.,,,,,, 2004-305T07:30:00,000T09:00:00,31-Oct-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-305T08:00:00,000T06:00:00,31-Oct-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-305T18:30:00,000T05:15:00,31-Oct-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_22,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0628 mrad/sec about the Z-axis toward -MOS Orb for 10000s. 3) Drift at indicated rate about the Z-axis toward +MOS Orb for 8000s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 313.98mrad",,,,,, 2004-305T18:30:00,000T05:15:00,31-Oct-04,CIRS,SPASS Rider,rings(general),SYSCAN,Saturnian system scan,CIRS_00ARI_SYSCAN,Scan of Saturn system for deep space calibration and to map scattered Saturn-light.,,,,,, 2004-305T18:30:00,000T05:15:00,31-Oct-04,VIMS,SPASS Rider,rings(general),SYSCAN,Saturnian system scan,UVIS_00ASA_MOS02APO022 Ride Along,"Slow scan across E ring region by UVIS. Look for magnetospheric & torus IR emissions, etc. VIMS unc. data vol = 250 Mb, compressed = 125 Mbits. Instrument params: size = 64x64 IRint = 640 msec. VISint = 40 sec. Countinuous cube generation for entire 11 hour duration of observation. 48 min per cube. ~15 cubes.",,,,,, 2004-306T01:45:00,000T09:00:00,1-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-306T03:00:00,000T06:00:00,1-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-306T12:15:00,000T06:00:00,1-Nov-04,UVIS,Prime,Saturn,MOS02APOA,Apoapsis mosaic,MOSAIC_APO_02_22,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0628 mrad/sec about the Z-axis toward -MOS Orb for 10000s. 3) Drift at indicated rate about the Z-axis toward +MOS Orb for 10000s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 313.98mrad",,,,,, 2004-306T16:35:00,001T23:27:00,1-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-306T16:35:00,013T15:14:00,1-Nov-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-306T16:35:00,001T23:27:00,1-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-306T16:35:00,001T23:27:00,1-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-306T16:35:01,001T23:26:59,1-Nov-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-306T18:15:00,000T05:02:00,1-Nov-04,UVIS,Prime,rings(general),IMPACT,,,Use UVIS HSP and FUV to detect flashes from meter-sized interplanetary impactors on rings to constrain flux of important impact population for ring origin/evolution.,,,,,, 2004-306T18:15:00,000T05:02:00,1-Nov-04,CIRS,SPASS Rider,rings(general),IMPACT,,CIRS_00ARI_IMPACT,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2004-306T18:15:00,000T05:02:00,1-Nov-04,ISS,SPASS Rider,rings(general),IMPACT,,URIMPACT spoke and F ring images day 306,"One WAC at each ansa beginning, middle, and end; pointing by UVIS; occasionally insert a second exposure",,,,,, 2004-306T19:17:00,000T04:00:00,1-Nov-04,VIMS,SPASS Rider,rings(general),IMPACT,,VIMS_00ARI_IMPACT001_UVIS,48 min per cube. ~15 cubes.,,,,,, 2004-306T23:17:00,000T00:30:00,1-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 181 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-EN-JA-HE-CP (602, 610, 612, 614, 615)]",,,,,, 2004-306T23:47:00,000T06:00:00,1-Nov-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_23,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0518 mrad/sec about the Z-axis for 10000 to -MOS Orb. 3) Drift at indicated rate about the Z-axis toward +MOS Orb for 7500s. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 259.01mrad.",,,,,, 2004-307T07:02:00,000T09:00:00,2-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-307T10:00:00,000T03:00:00,2-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-307T17:02:00,000T01:00:00,2-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,Retargetted Observations of S/2004 S1 and S/2004 S,"Through SCR 734 we changed this to a retargetable observation during SSUP. We are targeting RA/DECs: (7.086/8.884), (5.860/8.278), and (4.977/7.586)",,,,,, 2004-307T18:02:00,000T12:00:00,2-Nov-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_24,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0472 mrad/sec about the Z-axis for 10000 to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 10000 to +MOS Orb. 4) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 5) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 6) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 236.14mrad.",,,,,, 2004-308T07:02:00,000T09:00:00,3-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-308T10:00:00,000T03:00:00,3-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-308T16:02:00,001T16:30:00,3-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-308T16:02:00,001T16:30:00,3-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-308T16:02:00,001T16:30:00,3-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-308T16:02:01,011T15:46:59,3-Nov-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-308T17:02:00,000T01:00:00,3-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,Retargetted Observations of S/2004 S1 and S/2004 S,Through SCR 734 we changed this to a retargetable observation during SSUP. We are targeting RA/DECs: (10.518/8.534) and (5.124/7.640),,,,,, 2004-308T18:02:00,000T12:00:00,3-Nov-04,UVIS,Prime,Saturn,MOS02APOA,Apoapsis mosaic,MOSAIC_APO_02_24a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0427 mrad/sec about the Z-axis for 10000s to -MOS Orb. 3) Drift at indicated rate about the Z-Axis for 10000s to +MOS Orb. 4) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 5) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 6) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb(+/-Range): 213.54mrad.",,,,,, 2004-309T07:02:00,000T09:00:00,4-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-309T10:00:00,000T03:00:00,4-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-309T17:02:00,000T05:30:00,4-Nov-04,UVIS,Prime,Saturn,MOS02APOB,Apoapsis mosaic,MOSAIC_APO_02_24b,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0393 mrad/sec about the Z-axis for 10000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 9000s to +MOS Orb. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 196.66mrad.",,,,,, 2004-309T23:32:00,000T09:00:00,4-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-310T08:32:00,002T23:46:00,5-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-310T08:32:00,002T23:46:00,5-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-310T08:32:00,002T23:46:00,5-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-310T09:32:00,000T01:00:00,5-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 184 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [PM-EP-CP-JA-PA-TL-HE-AT-EN-DI (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2004-310T10:32:00,000T18:30:00,5-Nov-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_25,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0367 mrad/sec about the Z-axis for 10000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 4) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 5) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 6) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 7) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 8) Drift at indicated rate about the Z-axis for 5000s to Saturn Center. 9) Reset pointing for Saturn center and stare for remaining observation time. MOS Orb (+//Range): 183.61mrad.",,,,,, 2004-310T11:30:00,000T09:10:00,5-Nov-04,CAPS,SPASS Rider,InstrumentCalibration,CALIBRATE,Calibration,CAPS Calibration,"CAPS periodic gain test and calibration. The specified rate and data volume are the delta above the MAGBOUND rate (4500 bps), and the rate is the average over the entire request (current plans are to conduct the test in two different rates.)",,,,,, 2004-311T05:02:00,000T00:46:00,6-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 185 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [AT-EP-EN-PM-JA-PA-MI-CP-DI-HE (601, 602, 604, 610, 611, 612, 614, 615, 616, 617)]",,,,,, 2004-311T06:48:00,000T09:00:00,6-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-311T10:00:00,000T03:00:00,6-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-311T16:48:00,000T03:00:00,6-Nov-04,RADAR,SPASS Rider,Other,SOUTHWARM,Instrument warmup,"Distant Titan Latitude Study, Southern Latitudes",Warmup for calibration and science data collection.,,,,,, 2004-311T19:48:00,000T02:30:00,6-Nov-04,RADAR,Prime,Titan,SOUTH7CAL,Distant Titan radiometery and calibration,"Distant Titan Latitude Study, Southern Latitudes",Obtain distant Titan radiometer science and calibration data. One of a set that provides coverage of Titan southern latitude variation along with some obtainable associated longitude variation.,,,,,, 2004-311T22:18:00,000T00:30:00,6-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 188 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 0 targets: [ ()]",,,,,, 2004-311T22:48:00,000T06:30:00,6-Nov-04,CIRS,Prime,rings(general),FMONITOR,F ring monitor,Ring FP3/FP4 integrations,Integration on the main rings with FP3 and FP4,,,,,, 2004-311T22:48:00,000T06:30:00,6-Nov-04,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring imaging on each ansa,"Two WAC exposures at left ansa, one at right ansa during CIRS observations",,,,,, 2004-311T22:48:00,000T06:30:00,6-Nov-04,UVIS,SPASS Rider,rings(general),FMONITOR,F ring monitor,FUV and EUV ring spectroscopy,,,,,,, 2004-311T22:48:00,000T06:30:00,6-Nov-04,VIMS,SPASS Rider,rings(general),FMONITOR,F ring monitor,Ring images during CIRS FP3 ring integrations,8 64x64 images timed to coincide with WAC images. IR exposure time = 80 ms; Frame duration = 6.4 min. VIS on.,,,,,, 2004-312T05:18:00,000T00:30:00,7-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 189 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 0 targets: [ ()]",,,,,, 2004-312T06:48:00,000T09:00:00,7-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-312T07:00:00,000T06:00:00,7-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-312T16:48:00,000T05:30:00,7-Nov-04,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,"(1) Turn VIMS solar_port to sun. (2) Do cross-shaped pattern of 7(X)*5(Z) cubes, each 64*32, tau_IR = 40 & 320 ms, tau_VIS = 50 ms; 4 cubes at each position; offset between frames = 10 pixels in X and 5 pixels in Z. (3) Acquire 4 cubes at solarport boresight in hi-rres mode and same two integ times. (4) Turn to blank sky & take 4 64*64 background cubes at same two integ. times. (5) Return to Waypoint.",,,,,, 2004-312T16:48:00,000T05:30:00,7-Nov-04,UVIS,SPASS Rider,Sun,SOLARPORT,Solar port observation,SOLAR PORT RIDER,RIDER TO VIMS SOLARPORT OBSERVATION,,,,,, 2004-312T23:18:00,000T09:00:00,7-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-313T00:00:00,000T03:00:00,8-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-313T08:18:00,002T23:57:00,8-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-313T08:18:00,002T07:15:00,8-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-313T08:18:00,002T23:57:00,8-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-313T09:18:00,000T20:30:00,8-Nov-04,CIRS,Prime,Saturn,COMPSITA,Sit and stare at one location to derive composition,CIRS_00ASA_COMPSITA12,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-313T09:18:00,000T20:30:00,8-Nov-04,CIRS,SPASS Rider,Saturn,COMPSITA,Sit and stare at one location to derive composition,Support image,"Support imaging for compsit, ~1 frame per hr",,,,,, 2004-313T09:18:00,000T20:30:00,8-Nov-04,UVIS,SPASS Rider,Saturn,COMPSITA,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2004-313T09:18:00,000T20:30:00,8-Nov-04,VIMS,SPASS Rider,Saturn,COMPOSITA,,"Saturn Far Global Mosaic, Go-East Template #33","Rider to CIRS composition observation Data volume: 12 observations * 2 exposures * 64*64*352*12 = 420 mbits Data vol. edited down to ~70% of original request, per requirements of the MAG TWT data vol. budget. D. Cruikshank 8/1/02",,,,,, 2004-314T06:48:00,000T09:00:00,9-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-314T07:00:00,000T03:00:00,9-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-314T16:48:00,000T12:30:00,9-Nov-04,CIRS,Prime,Saturn,COMPSITB,Sit and stare at one location to derive composition,CIRS_00ASA_COMPSITB12,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-314T16:48:00,000T12:30:00,9-Nov-04,CIRS,SPASS Rider,Saturn,COMPSITB,Sit and stare at one location to derive composition,Support image,"Support imaging for compsit, ~1 frame per hr",,,,,, 2004-314T16:48:00,000T12:30:00,9-Nov-04,UVIS,SPASS Rider,Saturn,COMPSITB,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2004-314T16:48:00,000T12:30:00,9-Nov-04,VIMS,SPASS Rider,Saturn,COMPOSITA,,,"Rider to CIRS composition observation Data volume: 7 observations * 2 exposures * 64*64*352*12 = 244 mbits Data vol. edited down to 70% or original request, per requirements of MAG TWT data vol. budget. D. Cruikshank 8/1/02",,,,,, 2004-315T06:33:00,000T09:00:00,10-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-315T07:00:00,000T03:00:00,10-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-315T15:33:00,000T16:42:00,10-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-315T16:33:00,000T05:42:00,10-Nov-04,UVIS,Prime,Saturn,MOS02APOC,Apoapsis mosaic,MOSAIC_APO_02_26c,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb 2) Drift at a rate of 0.0294 mrad/sec about the Z-axis for 10000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 9000s to +MOS Orb. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 146.85mrad.",,,,,, 2004-315T23:15:00,000T09:00:00,10-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-316T03:00:00,000T03:00:00,11-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-316T08:15:00,003T07:04:00,11-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-316T08:15:00,003T07:04:00,11-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-316T08:15:00,003T07:04:00,11-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-316T09:15:00,000T01:00:00,11-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,Retargetted Observations of S/2004 S1 and S/2004 S,"Through SCR 734 we changed this to a retargetable observation during SSUP. We are targeting RA/DECs: (20.737/6.745), (20.796/7.161), and (20.596/7.596)",,,,,, 2004-316T10:15:00,000T18:18:00,11-Nov-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_27,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0285 mrad/sec about the Z-axis for 10000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 4) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 5) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 6) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 7) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 8) Drift at indicated rate about the Z-axis for 5000s to Saturn Center. 9) Reset pointing for Saturn center and stare for remaining observation time. MOS Orb (+/-Range): 142.73mrad.",,,,,, 2004-317T04:33:00,000T01:00:00,12-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,Retargetted Observations of S/2004 S1 and S/2004 S,Through SCR 734 we changed this to a retargetable observation during SSUP. We are targeting RA/DECs: (21.691/7.348) and (26.534/7.157),,,,,, 2004-317T06:33:00,000T09:00:00,12-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-317T10:00:00,000T03:00:00,12-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-317T16:33:00,000T01:00:00,12-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 206 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [PA-PM-EN-JA-AT-CP-DI-HE-TL-EP (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2004-317T17:33:00,000T12:00:00,12-Nov-04,UVIS,Prime,Saturn,MOS02APOA,Apoapsis mosaic,MOSAIC_APO_02_27a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0278 mrad/sec about the Z-axis for 10000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 4) Drift at indicated rate about the Z-axis for 10000s to -MOS Orb. 5) Drift at indicated rate about the Z-axis for 10000s to +MOS Orb. 6) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 139.27mrad.",,,,,, 2004-318T06:33:00,000T09:00:00,13-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-318T16:33:00,000T00:46:00,13-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 209 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [JA-PM-DI-EN-EP-MI-CP-HE-TE-TL (601, 602, 603, 604, 610, 611, 612, 613, 614, 616)]",,,,,, 2004-318T17:19:00,000T12:00:00,13-Nov-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_28,"Mosaic of Saturn magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ plane. 2) Drift at a rate of 0.0976 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 5) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 6) Slew -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 7) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 390.56mrad.",,,,,, 2004-319T06:19:00,000T09:00:00,14-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-319T10:00:00,000T03:00:00,14-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-319T15:19:00,000T16:30:00,14-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-319T15:19:00,000T16:30:00,14-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-319T15:19:00,000T16:30:00,14-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-319T16:19:00,000T00:30:00,14-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 212 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-EP-EN-HE-DI (602, 604, 611, 612, 615)]",,,,,, 2004-319T16:49:00,000T05:00:00,14-Nov-04,UVIS,Prime,Saturn,MOS02APOA,Apoapsis mosaic,MOSAIC_APO_02_28a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of 0.0956 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis toward -MOS Orb for 2000s. 5) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 382.62mrad.",,,,,, 2004-319T22:49:00,000T09:00:00,14-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-320T01:00:00,000T03:00:00,15-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-320T07:49:00,007T00:11:00,15-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-320T07:49:00,006T00:46:56,15-Nov-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-320T07:49:00,006T00:51:00,15-Nov-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,Survey measurements of dust in ram direction or S/C roll,,,,,, 2004-320T07:49:00,000T01:22:00,15-Nov-04,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,STARTUP,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2004-320T07:49:00,002T23:56:00,15-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-320T07:49:00,002T23:56:00,15-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-320T08:49:00,000T20:00:00,15-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-320T08:49:00,000T20:00:00,15-Nov-04,CIRS,SPASS Rider,rings(general),SPKMOVPER,Ring spoke movie,CIRS_00ARI_SPKMOVPER001_ISS,ride with ISS,,,,,, 2004-320T08:49:00,000T20:00:00,15-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #1: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #1. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 14 image sets in 20 hours. Volume (downlinked) = 352*12*64*32*14*3*1.05/2 = 191 mbits downlinked Call it 200 mbits.",,,,,, 2004-320T09:11:00,005T22:49:00,15-Nov-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-321T06:19:00,000T09:00:00,16-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-321T07:05:00,000T03:00:00,16-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-321T16:19:00,000T00:45:00,16-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 218 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [AT-PM-CP-PA-EP-JA-DI-HE-EN-MI (601, 602, 604, 610, 611, 612, 614, 615, 616, 617)]",,,,,, 2004-321T16:22:00,000T04:33:04,16-Nov-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-321T17:04:00,000T12:00:00,16-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-321T17:04:00,000T12:00:00,16-Nov-04,CIRS,SPASS Rider,rings(general),SPKMOVPER,Ring spoke movie,CIRS_00ARI_SPKMOVPER002_ISS,ride with ISS,,,,,, 2004-321T17:04:00,000T12:00:00,16-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #2: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #2. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 9 image sets in 12 hours. Volume (downlinked) = 352*12*64*32*9*3*1.05/2 = 122 mbits downlinked Call it 130 mbits.",,,,,, 2004-322T06:04:00,000T09:00:00,17-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-322T06:49:00,000T03:00:00,17-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-322T16:04:00,000T05:41:00,17-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-322T16:04:00,000T05:41:00,17-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #3: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #3. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 9 image sets in 12 hours. Volume (downlinked) = 352*12*64*32*9*3*1.05/2 = 122 mbits downlinked Call it 130 mbits.",,,,,, 2004-322T22:45:00,000T09:00:00,17-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-322T23:30:00,000T03:00:00,17-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-323T07:45:00,001T07:19:00,18-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-323T07:45:00,001T07:19:00,18-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-323T08:45:00,000T01:00:00,18-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 221 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [AT-TL-HE-DI-PA-EN-JA-EP-PM-CP (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2004-323T09:45:00,000T01:00:00,18-Nov-04,ISS,Prime,rings(general),RNGPHOTMC,,RING PHOTOMETRY OF RING ANSA,3X3 NACS IN 5 COLORS ON RIGHT ANSA;,,,,,, 2004-323T10:45:00,000T18:19:00,18-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-323T10:45:00,000T18:19:00,18-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #4: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #4. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 9 image sets in 12 hours. Volume (downlinked) = 352*12*64*32*9*3*1.05/2 = 122 mbits downlinked Call it 130 mbits.",,,,,, 2004-324T06:04:00,000T09:00:00,19-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-324T06:49:00,000T03:00:00,19-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-324T15:04:00,003T13:50:00,19-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-324T15:04:00,001T16:56:00,19-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-324T16:04:00,000T01:00:00,19-Nov-04,ISS,Prime,rings(general),RNGPHOTMC,,RING PHOTOMETRY OF RING ANSA,3X3 NACS IN 4 COLORS ON RIGHT ANSA;,,,,,, 2004-324T17:04:00,000T12:00:00,19-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-324T17:04:00,000T12:00:00,19-Nov-04,CIRS,SPASS Rider,rings(general),SPKMOVPER,Ring spoke movie,CIRS_00ARI_SPKMOVPER005_ISS,ride with ISS,,,,,, 2004-324T17:04:00,000T12:00:00,19-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #5: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #5. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 9 image sets in 12 hours. Volume (downlinked) = 352*12*64*32*9*3*1.05/2 = 122 mbits downlinked Call it 130 mbits.",,,,,, 2004-325T06:04:00,000T09:00:00,20-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-325T06:49:00,000T03:00:00,20-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-325T07:04:00,000T02:16:32,20-Nov-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-325T16:04:00,000T06:00:00,20-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-325T16:04:00,000T06:00:00,20-Nov-04,CIRS,SPASS Rider,rings(general),SPKMOVPER,Ring spoke movie,CIRS_00ARI_SPKMOVPER006_ISS,ride with ISS,,,,,, 2004-325T16:04:00,000T06:00:00,20-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #6: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #6. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 5 image sets in 6 hours. Volume (downlinked) = 352*12*64*32*5*3*1.05/2 = 68 mbits downlinked Call it 70 mbits.",,,,,, 2004-325T23:00:00,000T09:00:00,20-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-326T08:00:00,000T00:41:00,21-Nov-04,INMS,Non-SPASS,Saturn,PSTOTM006,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-326T08:00:00,000T00:56:00,21-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-326T08:35:56,001T20:11:04,21-Nov-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-326T08:37:00,001T20:23:00,21-Nov-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-326T08:41:00,000T23:19:00,21-Nov-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-326T08:56:00,000T14:04:00,21-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-326T09:00:00,000T01:00:00,21-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 001 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [PM-PA-EP-TL-JA-AT-EN-HY-DI-HE (602, 604, 607, 610, 611, 612, 613, 615, 616, 617)]",,,,,, 2004-326T09:00:00,000T09:06:08,21-Nov-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-326T10:00:00,000T12:00:00,21-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-326T10:00:00,000T12:00:00,21-Nov-04,CIRS,SPASS Rider,rings(general),SPKMOVPER,Ring spoke movie,CIRS_00BRI_SPKMOVPER001_ISS,ride with ISS,,,,,, 2004-326T10:00:00,000T12:00:00,21-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #7: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #7 (First one in Rev 00B).. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 9 image sets in 12 hours. Volume (downlinked) = 352*12*64*32*9*3*1.05/2 = 123 mbits downlinked Call it 130 mbits.",,,,,, 2004-326T23:00:00,000T01:00:00,21-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-326T23:00:00,000T09:00:00,21-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-327T00:00:00,000T08:00:00,22-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-327T08:00:00,000T20:54:00,22-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-327T08:00:00,000T20:44:00,22-Nov-04,INMS,Non-SPASS,Saturn,PSTOTM6BU,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-327T08:00:00,000T20:49:00,22-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-327T09:00:00,000T15:20:00,22-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-327T09:00:00,000T15:20:00,22-Nov-04,CIRS,SPASS Rider,rings(general),SPKMOVPER,Ring spoke movie,CIRS_00BRI_SPKMOVPER002_ISS,ride with ISS,,,,,, 2004-327T09:00:00,000T15:20:00,22-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #8: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #8 (Second one in Rev 00B).. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 11 image sets in ~16 hours. Volume (downlinked) = 352*12*64*32*11*3*1.05/2 = 150 mbits downlinked Call it 170 mbits.",,,,,, 2004-328T03:30:00,000T01:20:00,23-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-328T04:41:00,000T00:14:00,23-Nov-04,CAPS,SPASS Rider,SpacecraftActivity,SLEEPMUTE,Huygens probe support,Sleep/Mute for Probe Chkout & MTU test,sleep instrument at -19 minutes and mute biu at -6 minutes,,,,,, 2004-328T04:43:00,000T00:20:00,23-Nov-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder,"Put CIRS to sleep/mute for probe activity. Sleep at -17 minutes, mute at -6 min",,,,,, 2004-328T04:44:00,000T00:10:00,23-Nov-04,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-328T04:45:00,000T00:09:50,23-Nov-04,ISS,Non-SPASS,InstrumentCalibration,PCOFINON,Huygens probe support,ISS sleep/mute for PCO,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2004-328T04:47:00,000T09:24:00,23-Nov-04,MIMI,SPASS Rider,Other,MUTEPRCO,Mute instrument for Probe Checkout,Sleep and Mute for Probe C/O & MTU Test,MIMI_Mute_for_Probe_MTU,,,,,, 2004-328T04:49:00,000T09:31:00,23-Nov-04,RPWS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,RPWS Sleep and Mute for Probe activity,"RPWS sleep/mute for Probe activity, followed by unmute/sleep.",,,,,, 2004-328T04:51:00,000T00:03:00,23-Nov-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (Final PCO),UVIS to go to sleep/mute for final PCO (MGTWT request),,,,,, 2004-328T04:52:00,000T00:02:00,23-Nov-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE for Final PCO,VIMS to SLEEP/ MUTE for Final PCO,,,,,, 2004-328T04:54:00,000T09:17:00,23-Nov-04,INMS,Non-SPASS,Saturn,MUTE,Instrument to sleep mode,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-328T04:54:00,000T09:17:00,23-Nov-04,MAG,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,"Mute,Unmute for final PCO and MTU test","Mute instrument during probe activity, unmute at end. Note: assume do not have to go into sleep.",,,,,, 2004-328T05:00:00,000T09:05:00,23-Nov-04,CDA,Non-SPASS,DustRAM direction,PROBEMUTE,Huygens Probe support,Mute CDA for probe activities,mute time for probe activity,,,,,, 2004-328T05:00:00,000T09:05:00,23-Nov-04,PROBE,Non-SPASS,Earth,PCOFINAL,Huygens probe support,Final Probe Check-Out,"Final Probe Checkout. X-band downlink required. The following Orbiter instruments will be ON, in sleep mode, and muted prior to PSA ON: CDA, CAPS, ISS, MIMI, RPWS, UVIS, and VIMS; MAG on and muted; other orbiter instruments OFF.",,,,,, 2004-328T14:11:00,001T15:24:00,23-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-328T14:11:00,000T02:17:00,23-Nov-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUNMUT,Huygens probe support,WakeUp/UnMute at Probe Chkout & MTU test,unmute biu at +6 and wake up at +7,,,,,, 2004-328T14:11:00,000T00:07:00,23-Nov-04,MIMI,SPASS Rider,Other,UNMUTEPR,RSS HGA boresight test,Unmute and Active for Probe C/O & MTU Test,"Unmute at start, go ""active"" 7 minutes later",,,,,, 2004-328T14:11:00,000T00:04:00,23-Nov-04,INMS,Non-SPASS,Saturn,UNMUTE,Huygens probe support,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-328T14:11:00,000T00:07:00,23-Nov-04,ISS,Non-SPASS,InstrumentCalibration,PCOFINOFF,Huygens probe support,ISS wake/unmute after PCO,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2004-328T14:11:00,004T15:13:00,23-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-328T14:11:00,000T00:11:00,23-Nov-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after final PCO,Unmute/go to active after final PCO (MAGTWT request),,,,,, 2004-328T14:11:15,000T00:20:00,23-Nov-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,Sleep/unmute placeholder,"UNMUTE. Put CIRS to sleep/mute to stop mirror scan. Due to large forces during release, may require mirror latching.",,,,,, 2004-328T14:13:00,011T15:29:00,23-Nov-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-328T14:15:00,004T15:15:00,23-Nov-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-328T14:18:00,010T00:42:00,23-Nov-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-328T14:20:00,001T15:15:00,23-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-328T14:23:00,000T00:02:00,23-Nov-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode after Final PCO,VIMS to ACTIVE after Final PCO,,,,,, 2004-328T16:50:00,000T12:00:00,23-Nov-04,ISS,Prime,rings(general),SPKMOVPER,Ring spoke movie,SPOKE PERIODICITY MOVIE,"SPOKE MOVIE, ONE WAC EVRY ~ 30 MINUTES.",,,,,, 2004-328T16:50:00,000T12:00:00,23-Nov-04,VIMS,SPASS Rider,Saturn,SPKMOVIE,Ring spoke movie,Saturn Spoke Movie #9: ISS ridealong,"Saturn far global imagery, rideing along with ISS spoke movie #9 (Third - and last - one in Rev 00B).. Images acquired close to apoapsis. Assume Saturn is smaller than 16 mrads across, and use double-sampling. Image once every 1.5 hours, using three exposures. 9 image sets in 12 hours. Volume (downlinked) = 352*12*64*32*9*3*1.05/2 = 123 mbits downlinked Call it 130 mbits.",,,,,, 2004-329T05:50:00,000T09:00:00,24-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-329T06:50:00,000T06:00:00,24-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-329T06:50:00,000T02:16:32,24-Nov-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-329T15:50:00,000T00:45:00,24-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 011 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [PA-JA-TL-HE-AT-EP-EN-DI-CP-MI (601, 602, 604, 610, 611, 612, 613, 614, 615, 617)]",,,,,, 2004-329T16:35:00,000T12:00:00,24-Nov-04,UVIS,Prime,Saturn,MOS02APOA,Apoapsis mosaic,MOSAIC_APO_02_31a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ Plane. 2) Drift at a rate of 0.0926 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 5) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 6) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 7) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 370.49mrad.",,,,,, 2004-330T05:35:00,002T23:49:00,25-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-330T05:35:00,001T02:00:00,25-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-330T05:35:00,000T09:00:00,25-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-330T06:20:00,000T03:00:00,25-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-330T15:35:00,000T06:00:00,25-Nov-04,UVIS,Prime,Saturn,MOS02APOB,Apoapsis mosaic,MOSAIC_APO_02_31b,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ plane. 2) Drift at a rate of 0.0933 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 4000s toward -MOS Orb. 7) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 373.5mrad.",,,,,, 2004-330T22:35:00,000T09:00:00,25-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-331T07:35:00,003T21:45:00,26-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-331T08:35:00,000T01:00:00,26-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 014 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [DI-CP-HE-TE-TL-RH-EN-PA-JA-PM (602, 603, 604, 605, 610, 612, 613, 614, 616, 617)]",,,,,, 2004-331T09:35:00,000T18:00:00,26-Nov-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_32,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1)Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ Plane. 2) Drift at a rate of 0.0944 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 5) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 6) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 7)Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 8) Rotate +64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 9) Rotate +64mrad in the YZ plane. Drift at indicated rate about the Z-axis for 4000s to Saturn Center. 10) Reset pointing for Saturn Center and stare for remaining observation time. MOS Orb (+/-Range): 377.58mrad.",,,,,, 2004-332T03:35:00,000T01:00:00,27-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 017 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [HE-CP-JA-PM-DI-EN-EP-TL-AT-PA (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2004-332T05:35:00,000T09:00:00,27-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-332T06:20:00,000T03:00:00,27-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-332T15:35:00,000T00:45:00,27-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 020 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [PA-EP-CP-EN-HE-DI-AT-PM-JA-TL (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2004-332T16:20:00,000T12:00:00,27-Nov-04,UVIS,Prime,Saturn,MOS02APOA,Apoapsis mosaic,MOSAIC_APO_02_32a,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ Plane. 2) Drift at a rate of 0.033 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 5) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 6) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 7) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 133.31mrad.",,,,,, 2004-333T05:24:00,002T03:56:00,28-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-333T05:24:00,005T09:36:00,28-Nov-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-333T05:30:00,007T00:14:00,28-Nov-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-333T07:18:00,000T07:02:00,28-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-333T09:00:00,000T03:00:00,28-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-333T15:20:00,000T01:00:00,28-Nov-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 023 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [HE-PA-EN-CP-JA-TL-DI-PM-AT-EP (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2004-333T15:20:00,000T02:16:32,28-Nov-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-333T16:20:00,000T12:00:00,28-Nov-04,UVIS,Prime,Saturn,MOS02APOB,Apoapsis mosaic,MOSAIC_APO_02_32b,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel to the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ Plane. 2) Drift at a rate of 0.034 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 5) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 6) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to -MOS Orb. 7) Slew back to SAturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range): 135.61mrad.",,,,,, 2004-334T05:20:00,000T09:00:00,29-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-334T19:20:00,000T01:00:00,29-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-334T20:20:00,000T11:30:00,29-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-334T22:00:00,000T04:00:00,29-Nov-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-335T05:20:00,003T10:16:00,30-Nov-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-335T07:50:00,000T01:30:00,30-Nov-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-335T09:20:00,003T05:40:00,30-Nov-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-335T10:20:00,000T06:50:00,30-Nov-04,CIRS,Prime,rings(general),FMONITOR,F ring monitor,Ring FP3/FP4 integrations,Integration on the main rings with FP3 and FP4,,,,,, 2004-335T10:20:00,000T06:50:00,30-Nov-04,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring imaging on each ansa,"Two WAC exposures at left ansa, one at right ansa during CIRS observations",,,,,, 2004-335T10:20:00,000T06:00:00,30-Nov-04,UVIS,SPASS Rider,rings(general),FMONITOR,F ring monitor,FUV and EUV ring spectroscopy,,,,,,, 2004-335T10:20:00,000T06:00:00,30-Nov-04,VIMS,SPASS Rider,rings(general),FMONITOR,F ring monitor,Ring images during CIRS FP3 ring integrations,8 64x64 images timed to coincide with WAC images. IR exposure time = 80 ms; Frame duration = 6.4 min. VIS on.,,,,,, 2004-335T16:20:00,000T03:00:00,30-Nov-04,RADAR,SPASS Rider,Other,WARM4RCAL,RADAR warmup,"Radiometric Calibration Using Microwave Sources, S",Warmup for calibration and science data collection.,,,,,, 2004-335T19:20:00,000T07:00:00,30-Nov-04,RADAR,Prime,Other,SRCRADCAL,RADAR microwave source radiometric calibration,"Radiometric Calibration Using Microwave Sources, S","Scan the Sun, Saturn, and microwave sources while collecting radiometry data.",,,,,, 2004-336T03:50:00,000T12:00:00,1-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-336T04:50:00,000T06:00:00,1-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-336T16:50:00,000T00:30:00,1-Dec-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 031 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-PM-DI-PA-AT (604, 611, 615, 616, 617)]",,,,,, 2004-336T17:20:00,000T07:00:00,1-Dec-04,UVIS,Prime,Saturn,MOS02APO,Apoapsis mosaic,MOSAIC_APO_02_34,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +128mrad in the YZ Plane. 2) Drift at a rate of 0.037 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 8000s to +MOS Orb. 4) Rotate -64mrad in the YZ Plane. Drift at indicated rate about the Z-axis for 7200s to -MOS Orb. 6) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS Orb (+/-Range: 146.23mrad.",,,,,, 2004-337T00:20:00,000T02:00:00,2-Dec-04,UVIS,Prime,Sun,SOL,Solar calibration,USUNCAL01,INSTANCE OF USUNCAL01. Solar Calibration,,,,,, 2004-337T03:36:00,000T12:00:00,2-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-337T04:36:00,000T06:00:00,2-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-337T04:36:00,000T04:33:04,2-Dec-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-337T16:36:00,000T00:30:00,2-Dec-04,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 035 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EP-EN-DI-JA (602, 604, 610, 611, 617)]",,,,,, 2004-337T17:06:00,000T09:30:00,2-Dec-04,VIMS,Prime,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global #1,Saturn FarGlobal Observation 1*1 should barely encompass the full disk. One observation per hour. Each observation has two exposures. Volume = 2*64*64*352*12*9.5 = 330 mbits,,,,,, 2004-338T03:36:00,000T12:00:00,3-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-338T04:36:00,000T06:00:00,3-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-338T15:00:00,001T14:54:00,3-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-338T15:00:00,001T14:54:00,3-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-338T15:00:01,001T14:46:59,3-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-338T15:36:00,000T16:15:00,3-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-338T16:36:00,000T02:15:00,3-Dec-04,CIRS,Prime,Saturn,COMPSITA,Sit and stare at one location to derive composition,CIRS_00BSA_COMPSITA11,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-338T16:36:00,000T02:15:00,3-Dec-04,VIMS,SPASS Rider,Saturn,COMPRA,Composition map,Saturn CIRS Ride-along Composition Map #1,Saturn CIRS Ride-along Composition Map Sit and stare at Saturn. Take three images (each with a different exposure) every 1.5 hours. Use Nyquist (double) sampling This observation opportunity yields three sets (9 image cubes) Data volume: 352*12*64*64*3*3*1.05/2 = 163.5/2 = 82 mbits downlinked Call it 50 mbits downlinked...,,,,,, 2004-338T19:51:00,000T12:00:00,3-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-338T20:36:00,000T06:00:00,3-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-339T07:51:00,000T21:58:00,4-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-339T08:51:00,000T12:50:00,4-Dec-04,CIRS,Prime,Saturn,COMPSITA,Sit and stare at one location to derive composition,CIRS_00BSA_COMPSITa12,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-340T05:41:00,000T00:14:00,5-Dec-04,CAPS,SPASS Rider,SpacecraftActivity,SLEEPMUTE,Huygens probe support,Sleep/Mute for Battery Depassivation,sleep instrument at -19 minutes and mute biu at -6 minutes,,,,,, 2004-340T05:42:00,000T02:26:00,5-Dec-04,CDA,Non-SPASS,DustRAM direction,PROBEMUTE,Huygens Probe support,ProbeMute,mute time for probe activity,,,,,, 2004-340T05:43:00,000T00:20:00,5-Dec-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,Sleep/mute placeholder,"Put CIRS to sleep/mute to stop mirror scan. Due to large forces during release, may require mirror latching.",,,,,, 2004-340T05:44:00,000T00:10:00,5-Dec-04,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-340T05:45:00,000T00:09:50,5-Dec-04,ISS,Non-SPASS,InstrumentCalibration,PCOBATON,Huygens probe support,ISS sleep/mute for Probe activity,ISS sleep/mute for Probe Battery activity,,,,,, 2004-340T05:45:00,000T00:09:50,5-Dec-04,ISS,Non-SPASS,InstrumentCalibration,PCODEPON,Huygens probe support,ISS sleep/mute for Probe activity,ISS sleep/mute for Probe depassivation activity,,,,,, 2004-340T05:47:00,000T02:19:00,5-Dec-04,MIMI,SPASS Rider,Other,MUTEBATT,Mute instrument for Probe Checkout,Sleep and Mute for Probe Battery Status,Sleep and Mute for Probe Battery Status,,,,,, 2004-340T05:49:00,000T02:26:00,5-Dec-04,RPWS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,RPWS Sleep and Mute for Probe activity,"RPWS sleep/mute for Probe activity, followed by unmute/sleep.",,,,,, 2004-340T05:51:00,000T00:03:00,5-Dec-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (Depassivation),UVIS to go to sleep/mute for probe depassivation (MGTWT request),,,,,, 2004-340T05:52:00,000T00:02:00,5-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS to SLEEP / MUTE for Probe Depass,VIMS to SLEEP/ MUTE for Probe Depass,,,,,, 2004-340T05:54:00,000T02:12:00,5-Dec-04,INMS,Non-SPASS,Saturn,MUTE,Instrument to sleep mode,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-340T05:54:00,000T02:12:00,5-Dec-04,MAG,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,"Mute,Unmute for Probe Battery Activity","Mute instrument during probe activity, unmute at end. Note: assume do not have to go into sleep.",,,,,, 2004-340T06:00:00,000T02:00:00,5-Dec-04,PROBE,Non-SPASS,Earth,DEPASSIV2,Huygens probe support,PROBE BATTERY DEPASSIVATION -2,Prepare Probe batteries for primary mission. X-band downlink required. Orbiter instruments off/sleep/mute as for probe checkouts.,,,,,, 2004-340T08:06:00,004T23:45:00,5-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-340T08:06:00,000T02:17:00,5-Dec-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUNMUT,Huygens probe support,WakeUp/UnMute at Probe Depassivation,unmute biu at +6 minutes and wake up at +7 minutes,,,,,, 2004-340T08:06:00,000T00:07:00,5-Dec-04,MIMI,SPASS Rider,Other,UNMUTEBAT,Huygens probe support,Unmute and active after Probe Battery Status,"Unmute at start, go ""active"" 7 minutes later",,,,,, 2004-340T08:06:00,000T00:04:00,5-Dec-04,INMS,Non-SPASS,Saturn,UNMUTE,Huygens probe support,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-340T08:06:00,000T00:07:00,5-Dec-04,ISS,Non-SPASS,InstrumentCalibration,PCODEPOFF,Huygens probe support,ISS wake/unmute Probe activity,ISS wake/unmute Probe depassivation activity,,,,,, 2004-340T08:06:00,004T23:45:00,5-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-340T08:06:00,000T00:11:00,5-Dec-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after depassivation,Unmute/go to active after depassivation (MAGTWT request),,,,,, 2004-340T08:06:15,000T00:20:00,5-Dec-04,CIRS,Non-SPASS,Other,PROUNMUTE,Huygens Probe support,Sleep/unmute placeholder,"UNMUTE. Put CIRS to sleep/mute to stop mirror scan. Due to large forces during release, may require mirror latching.",,,,,, 2004-340T08:08:00,000T01:52:00,5-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-340T08:10:00,004T21:56:00,5-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-340T08:13:00,004T23:38:00,5-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-340T08:15:00,000T06:51:00,5-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-340T08:18:00,000T00:02:00,5-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS to Active Mode after Probe Depass,VIMS to ACTIVE after Probe Depass,,,,,, 2004-340T10:00:00,000T04:59:00,5-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-340T14:57:00,000T00:07:00,5-Dec-04,ISS,Non-SPASS,InstrumentCalibration,PCOBATOFF,Huygens probe support,ISS wake/unmute after Probe activity,ISS wake/unmute ISS after probe battery activity,,,,,, 2004-340T14:59:00,001T13:43:00,5-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-340T15:06:00,000T00:35:00,5-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-340T15:41:00,002T12:55:00,5-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-340T16:41:00,000T11:10:00,5-Dec-04,ISS,Prime,Saturn,3X3MOVIEA,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2004-341T04:51:00,000T09:00:00,6-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-341T05:36:00,000T06:00:00,6-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-341T14:51:00,000T09:10:00,6-Dec-04,ISS,Prime,Saturn,3X3MOVIEA,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2004-341T14:51:00,000T09:06:08,6-Dec-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-342T04:42:01,000T08:33:59,7-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-342T13:16:00,002T18:36:00,7-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-342T15:41:00,000T05:55:00,7-Dec-04,CIRS,Prime,Saturn,COMPSITB,Sit and stare at one location to derive composition,CIRS_00BSA_COMPSITB11,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole INclude Iapetus from ~2004-340T22:00-23:00",,,,,, 2004-342T15:41:00,000T05:55:00,7-Dec-04,VIMS,SPASS Rider,Saturn,COMPRA,Composition map,Saturn CIRS Ride-along Composition Map #2,Saturn CIRS Ride-along Composition Map Sit and stare at Saturn. Take three images (each with a different exposure) every 1.5 hours. Use Nyquist (double) sampling This observation opportunity yields 9 sets (27 image cubes) Data volume: 352*12*64*32*9*3*1.05/2 = 122.6 = 123 mbits Call it 150 mbits downlinked...,,,,,, 2004-342T18:00:00,000T08:45:00,7-Dec-04,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS PIM (Ka-TWTA Maintenance),RSS PIM. Pointing=Not Applicable. DSN Tracking=None.,,,,,, 2004-342T22:36:00,000T06:00:00,7-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-342T23:36:00,000T04:00:00,7-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-343T04:36:00,001T00:00:00,8-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-343T05:36:00,000T16:00:00,8-Dec-04,CIRS,Prime,Saturn,COMPSITC,Sit and stare at one location to derive composition,CIRS_00BSA_COMPSITC11,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2004-343T05:36:00,000T16:00:00,8-Dec-04,VIMS,SPASS Rider,Saturn,COMPRA,Composition map,Saturn CIRS Ride-along Composition Map #3,Saturn CIRS Ride-along Composition Map Sit and stare at Saturn. Take three images (each with a different exposure) every 1.5 hours. Use Nyquist (double) sampling This observation opportunity yields 9 sets (27 image cubes) Data volume: 352*12*64*64*9*3*1.05/2 = 490.5/2 = 250 mbits downlinked Call it 150 mbits downlinked...,,,,,, 2004-343T22:36:00,000T06:00:00,8-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-343T23:21:00,000T05:15:00,8-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-343T23:36:00,000T09:06:08,8-Dec-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-344T04:36:00,000T16:30:00,9-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-344T05:36:00,000T03:00:00,9-Dec-04,ISS,Prime,rings(general),SPKFORM,Ring spoke movie,SPOKE FORMATION CAMPAIGN,SPK FORMATION SEQUENCE: NAC ON MORNING SIDE OF SHADOW AND TRACKING AT KEPLERIAN RATE,,,,,, 2004-344T08:36:00,000T11:30:00,9-Dec-04,VIMS,Prime,Saturn,FARGLO,Saturn far encounter global mosaic,Saturn Far Global #4,"Saturn FarGlobal Observation 2*2 should encompass the full disk. One observation per hour. Each observation has one exposure. Volume = 4*64*64*352*12*9 *1.05= 633 mbits, or 317 mbits downlinked or",,,,,, 2004-344T08:36:00,000T04:33:04,9-Dec-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-344T21:06:00,000T01:00:00,9-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-344T21:06:00,000T09:00:00,9-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-344T22:06:00,000T08:00:00,9-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-345T06:06:00,000T23:59:00,10-Dec-04,INMS,Non-SPASS,Saturn,PSTOTM007,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-345T06:06:00,000T04:54:00,10-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-345T07:51:00,000T03:09:00,10-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,CAPS magnetospheric boundary campaign,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2004-345T07:51:00,000T03:09:00,10-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-345T07:51:00,001T20:30:00,10-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-345T07:52:00,004T00:08:00,10-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-345T08:03:00,000T12:07:00,10-Dec-04,ISS,Prime,Titan,MOVIEC,Surface/winds/cloud movie,Titan Surface/winds/clouds,15 images of Titan every hour for 12 hours. Surface/winds/clouds,,,,,, 2004-345T08:03:00,000T12:07:00,10-Dec-04,VIMS,SPASS Rider,Titan,MOVIES,Surface/winds/cloud movie,Movies VIMS_4868,Ridealong with ISS movie,,,,,, 2004-345T11:00:00,002T22:38:13,10-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-345T11:00:00,001T17:21:00,10-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-345T11:00:00,001T17:21:00,10-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2004-345T11:00:00,001T17:21:00,10-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-345T21:05:00,000T09:30:00,10-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-345T22:35:00,000T06:00:00,10-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-346T06:05:00,001T17:33:13,11-Dec-04,INMS,Non-SPASS,Saturn,PSTOTM7BU,Magetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-346T08:03:00,000T15:57:00,11-Dec-04,ISS,Prime,Titan,MOVIED,Surface/winds/cloud movie,Titan Surface/winds/clouds,Surface/winds/clouds 15 images of Titan every hour for 15 hours,,,,,, 2004-346T08:03:00,000T15:57:00,11-Dec-04,CIRS,SPASS Rider,Titan,COMPMAP,Composition map,CIRS_00BTI_COMPMAP03,"To obtain measurements of nitriles, hydrocarbons, and an oxygen compound, CO2, as a function of latitude and emission angle (at equator) on Titan. POINTING: -y to Titan, z to pole",,,,,, 2004-346T08:03:00,000T15:57:00,11-Dec-04,VIMS,SPASS Rider,Titan,MOVIES,Surface/winds/cloud movie,Movies VIMS_4868,"Ridealong with ISS Titan movie, continued.",,,,,, 2004-347T00:00:00,000T01:30:00,12-Dec-04,ISS,Prime,rings(general),RADCOLOR,Radial color scan,RING RADIAL COLOR SCAN,"RADIAL COLOR SCAN, 15 COLORS, NAC",,,,,, 2004-347T04:21:00,000T01:56:00,12-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-347T04:21:00,001T05:17:13,12-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-347T04:21:00,001T05:17:13,12-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-347T04:36:00,000T09:00:00,12-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-347T06:06:00,000T06:00:00,12-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-347T06:17:00,000T07:19:00,12-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-347T07:17:00,000T02:16:32,12-Dec-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps survey rate.,,,,,, 2004-347T07:17:00,000T06:19:00,12-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-347T13:36:00,000T20:02:13,12-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-347T15:13:13,000T08:25:00,12-Dec-04,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2004-347T15:13:13,000T08:25:00,12-Dec-04,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (8 integrations total = 16 frames, 0.5 Mb/frame)",,,,,, 2004-347T15:13:13,000T08:25:00,12-Dec-04,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,"NMA/RCI (NAC Monitoring of Surface and Atmosphere,","monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2004-347T15:13:13,000T12:25:00,12-Dec-04,VIMS,SPASS Rider,Titan,MIDIR,Mid infrared thermal map,Mid-IR VIMS_4868,Ridealong with CIRS Titan Mid-IR nadir map and Far-IR nadir composition.,,,,,, 2004-347T23:38:13,000T04:00:00,12-Dec-04,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2004-347T23:38:13,000T04:00:00,12-Dec-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2004-347T23:38:13,000T04:00:00,12-Dec-04,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,"NGM/RCI (NAC Global Map, Ridealong Context Imaging",global map,,,,,, 2004-347T23:38:13,000T11:00:00,12-Dec-04,INMS,Non-SPASS,Titan,TBINBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-348T03:38:13,000T04:00:00,13-Dec-04,UVIS,Prime,Titan,EUFUV,,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2004-348T03:38:13,000T04:00:00,13-Dec-04,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. Ride with UVIS.",,,,,, 2004-348T03:38:13,000T04:00:00,13-Dec-04,ISS,SPASS Rider,Titan,EUFUV,,"WPH/NGM/RCI (WAC Photometry, NAC Global Mapping, R","particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2004-348T03:38:13,000T04:00:00,13-Dec-04,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,EUV/FUV VIMS_4868,Ridealong with UVIS observation. 64 probably best,,,,,, 2004-348T07:38:13,000T02:00:00,13-Dec-04,ISS,Prime,Titan,REGMAP,Regional mapping,NRM (NAC Regional Map),regional map,,,,,, 2004-348T07:38:13,000T04:02:00,13-Dec-04,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. Ride with ISS.",,,,,, 2004-348T07:38:13,000T04:02:00,13-Dec-04,VIMS,SPASS Rider,Titan,HIRES,High resolution image,Hi Res VIMS_4868,"Ridealong with ISS high resolution map (12X12 images). Also, ridealong with subsequent transition to thrusters (use 40-ms exposures there because of thruster-related smearing).",,,,,, 2004-348T09:38:13,000T01:30:00,13-Dec-04,ISS,Prime,Titan,HIRESNAC,High resolution map,HRI (High Resolution Imaging),"high-resolution imaging, 50-200 m/px, special targets, emission angles < 45 prefer IR-polarizer (phase 45-110)",,,,,, 2004-348T09:38:13,000T01:00:00,13-Dec-04,CAPS,SPASS Rider,Titan,TBINBND,,MAPS 00BTI Campaign,Part of 00BTI MAPS Campaign. Inbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2004-348T09:38:13,000T01:00:00,13-Dec-04,MIMI,SPASS Rider,Titan,TBINBND,,MAPS 00BTI(TB) Campaign,"Part of 00BTI(TB) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-348T09:38:13,000T04:00:00,13-Dec-04,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,TB Flyby,"TB is the first wake encounter with particular emphasis on the wake-Alfven-wing transition region. The flyby altitude of 2346 km is not optimum, however. Hence in spite of the relatively new and unique data in the early mission we assign only priority two to this flyby.",,,,,, 2004-348T09:38:13,000T01:30:00,13-Dec-04,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2004-348T10:38:13,000T02:00:00,13-Dec-04,CAPS,SPASS Rider,Titan,TBCLOSE,,MAPS 00BTI Campaign,Part of 00BTI MAPS Campaign. Observations of Titan's interaction with Saturn's magnetosphere,,,,,, 2004-348T10:38:13,000T02:00:00,13-Dec-04,MIMI,SPASS Rider,Titan,TBCLOSE,,MAPS 00BTI(TB) Campaign,"Part of 00BTI(TB) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-348T10:38:13,000T02:00:00,13-Dec-04,INMS,Non-SPASS,Titan,TBCLOSE,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-348T11:08:13,000T00:21:00,13-Dec-04,ISS,SPASS Rider,SpacecraftActivity,ORSRCS,,HRI (High Resolution Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2004-348T11:08:13,000T00:21:00,13-Dec-04,VIMS,SPASS Rider,Titan,RCSTRANS,,RWA_RCS_Transition,A single sit and stare 64X64 image during the RWA to RCS transition,,,,,, 2004-348T11:08:13,000T01:00:00,13-Dec-04,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2004-348T11:29:13,000T00:36:00,13-Dec-04,UVIS,Prime,Star,TWOSTOCCS,Stellar occultation,Titan Occults Alpha Vir and Lambda SCO,First Alpha Vir occultation then Lambda Sco occultation. UVIS FUV Occultation slit boresite on star for the entire time. Note: ISS observation which precedes this should leave NAC pointed to Alpha Vir so there should be no turn time at the start.,,,,,, 2004-348T12:05:13,000T00:23:00,13-Dec-04,UVIS,SPASS Rider,Star,TWOSTOCCS,Stellar occultation,Titan Occults Alpha Vir and Lambda SCO,First Alpha Vir occultation then Lambda Sco occultation. Rider observation during the transition from RCS to RWA while observing Lambda Sco.,,,,,, 2004-348T12:08:13,000T01:30:00,13-Dec-04,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2004-348T12:28:13,000T01:40:00,13-Dec-04,VIMS,Prime,Titan,DARKSIDE,Dark side imaging,Dark_Side VIMS_4868,Dark side observations of TItan. 64X64 cubes. Slow scan on limb to accommodate CIRS,,,,,, 2004-348T12:28:13,000T01:40:00,13-Dec-04,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,,Vertical aerosol sounding of Titan's stratosphere. Slow radial scans.,,,,,, 2004-348T12:28:13,000T01:40:00,13-Dec-04,ISS,SPASS Rider,Titan,DARKSIDE,Dark side imaging,"WNI/RCI (WAC Nightside Imaging, Ridealong Context",search for and monitor lightning/aurora,,,,,, 2004-348T12:38:13,000T01:00:00,13-Dec-04,CAPS,SPASS Rider,Titan,TBOUTBND,,MAPS 00BTI Campaign,Part of 00BTI MAPS Campaign. Outbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2004-348T12:38:13,000T01:00:00,13-Dec-04,MIMI,SPASS Rider,Titan,TBOUTBND,,MAPS 00BTI(TB) Campaign,"Part of 00BTI(TB) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2004-348T12:38:13,000T11:00:00,13-Dec-04,INMS,Non-SPASS,Titan,TBOUTBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2004-348T13:38:13,000T18:14:31,13-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-348T13:38:13,000T18:13:47,13-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-348T13:38:13,000T18:14:31,13-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-348T13:38:13,000T12:31:31,13-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-348T14:08:13,000T02:30:00,13-Dec-04,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2004-348T14:08:13,000T02:30:00,13-Dec-04,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk.",,,,,, 2004-348T14:08:13,000T02:30:00,13-Dec-04,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong context Imaging),"particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2004-348T16:38:13,000T02:00:00,13-Dec-04,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions.,,,,,, 2004-348T16:38:13,000T02:00:00,13-Dec-04,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2004-348T16:38:13,000T02:00:00,13-Dec-04,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,"WPH/NGM/RCI (WAC Photometry, NAC Global Mapping, R","particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2004-348T16:38:13,000T02:00:00,13-Dec-04,VIMS,SPASS Rider,Titan,MIDIR,Mid infrared thermal map,Dark_Side VIMS_4868,Ridealong with CIRS mid-IR limb map.,,,,,, 2004-348T18:38:13,000T03:30:00,13-Dec-04,VIMS,Prime,Titan,DARKSIDE,Dark side imaging,Dark_Side VIMS_4868,Dark side observations of TItan. 64X64 cubes. Nadir integrations. CIRS wants FIR FOV on Titan.,,,,,, 2004-348T18:38:13,000T03:30:00,13-Dec-04,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2004-348T18:38:13,000T03:30:00,13-Dec-04,ISS,SPASS Rider,Titan,DARKSIDE,Dark side imaging,"NNI/RCI (NAC Nightside Imaging, Ridealong Context",search for and monitor lightning/aurora,,,,,, 2004-348T22:52:00,000T09:00:00,13-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-348T23:38:13,000T08:14:31,13-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-349T00:22:00,000T06:00:00,14-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-349T02:09:00,000T05:43:00,14-Dec-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-349T07:52:00,001T16:08:00,14-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-349T07:52:00,001T07:30:00,14-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-349T07:52:00,001T16:08:00,14-Dec-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-349T07:52:00,000T22:30:00,14-Dec-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-349T07:52:01,000T21:33:00,14-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-349T07:52:44,000T11:15:17,14-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-349T08:00:00,000T13:00:00,14-Dec-04,CDA,Non-SPASS,DustRAM direction,RNGMAR,,Ring margin,"Ring margin dust measurements, 13 to 9 Rs",,,,,, 2004-349T09:00:00,000T07:52:00,14-Dec-04,VIMS,Prime,Saturn,CYLMAP,Saturn cylindrical map,Saturn Cylindrical Map #2,Saturn Cylindrical Map 2*6 mosaic done every two hours (5 times). Each observation has one exposure. Volume = 2*6*5*64*64*352*12 = 1040 mbits,,,,,, 2004-349T09:00:00,000T07:52:00,14-Dec-04,CIRS,SPASS Rider,Saturn,COMPFT,,CIRS_00BSA_COMPFT01,"At a range of 6 Rs, build a raster by scanning North/South over a region 12 [24] milliradians on a side at 13 [26] microrad/s VIMS RIDER",,,,,, 2004-349T09:00:00,000T07:52:00,14-Dec-04,ISS,SPASS Rider,Saturn,CYLMAP,Saturn cylindrical map,Saturn CYLMAP rider,Saturn rider to VIMS observation,,,,,, 2004-349T09:00:00,000T07:52:00,14-Dec-04,UVIS,SPASS Rider,Saturn,CYLMAP,Saturn cylindrical map,UVIS Rider to VIMS CYLMAP,UVIS Rider to VIMS CYLMAP,,,,,, 2004-349T09:00:00,000T02:25:04,14-Dec-04,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 34 B cycles duration. Data is in addition to 2000 bps survey rate.,,,,,, 2004-349T16:52:00,000T01:00:00,14-Dec-04,ISS,Prime,Dione,GLOCOL,Global coverage mapping,Dione regional mapping and global color mapping,Turn -Y to Dione; Do 1x1 mosaic NAC multi color + 9 NAC polarizer + 4 WAC polarizer filters; do WAC rgb; do 2x2 mosaic in NAC clear (two shutters per footprint); turn to WP.,,,,,, 2004-349T16:52:00,000T01:00:00,14-Dec-04,CIRS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,ISS ridealong,"Sub-S/C=(22, 223), LT=11:30, phase=46, AD=8+ mrad. CIRS at 15.5 cm-1 resolution; blink, shutter closed during central 5 min..",,,,,, 2004-349T16:52:00,000T01:00:00,14-Dec-04,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-349T16:52:00,000T01:00:00,14-Dec-04,VIMS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,Dione ride with ISS,"24x12i2-v3 double/triple res 160 ms , 640 ms pairs, do one set every 5 minutes (12/hour). 1.5 mbits per set, compressed. 18 mbits total compressed",,,,,, 2004-349T17:52:00,000T04:00:00,14-Dec-04,CIRS,Prime,rings(general),TEMPU05LP,Thermal map,CIRS_00BRI_TempU05LP,"Afternoon radial scan of main rings to obtain thermal measurement of rings. -Y to rings, Z perp to rings",,,,,, 2004-349T17:52:00,000T04:00:00,14-Dec-04,CIRS,SPASS Rider,rings(general),TEMPU05LP,Thermal map,CIRS_00BRI_TEMPU05LP_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-349T19:08:01,000T09:13:59,14-Dec-04,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"MAPS magnetospheric survey, INMS switches to inner Mag inside 8 Rs.",,,,,, 2004-349T21:00:00,000T09:00:00,14-Dec-04,CDA,Non-SPASS,RingE,ERING,E ring observation,Ering before priapsis,within Ering,,,,,, 2004-349T21:52:00,000T03:00:00,14-Dec-04,CIRS,Prime,Saturn,LIMBMAP,Limb map,CIRS_00BSA_LIMBMAP07,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, latitude coverage. POINTING: -y to Saturn, z to limb",,,,,, 2004-349T21:52:00,000T03:00:00,14-Dec-04,CIRS,SPASS Rider,Saturn,LIMBMAP,Limb map,CIRS_00BSA_LIMBMAP07 SI,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, latitude coverage. POINTING: -y to Saturn, z to limb",,,,,, 2004-349T21:52:00,000T04:30:00,14-Dec-04,RADAR,SPASS Rider,Other,WARM4MI,RADAR warmup,Scatterometry/Radiometry of Mimas.,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2004-349T21:52:00,000T03:00:00,14-Dec-04,UVIS,SPASS Rider,Saturn,LIMBMAP,Limb map,CIRS Rider,UVIS EUV and FUV riding along with CIRS LIMBMAP observation,,,,,, 2004-349T21:52:00,000T03:00:00,14-Dec-04,VIMS,SPASS Rider,Saturn,LIMBMAP,Limb map,Saturn CIRS ride-along limbmap observation,Saturn limb map Ridealong with CIRS. Design TBD,,,,,, 2004-349T23:14:18,000T14:00:00,14-Dec-04,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. Need to do this inside 6 RS on at least half of the periapses inside of 6RS. No pointing requirement",,,,,, 2004-350T00:52:00,000T00:48:00,15-Dec-04,ISS,Prime,Dione,REGMAP,Regional mapping,Dione regional mapping,"Turn -Y to Dione; do 5-NAC-frames mosaic (three shutters per footprint) (IR1, GRN, Clr filters) + 3 WAC rgb; turn to Dione center.",,,,,, 2004-350T00:52:00,000T00:48:00,15-Dec-04,CIRS,SPASS Rider,Dione,REGMAP,Regional mapping,ISS ridealong,"Sub-S/C=(33, 349), LT=06:00, phase=102+ , AD=13 mrad. CIRS at 15.5 cm-1 resolution; blink, shutter closed during central 5 min..",,,,,, 2004-350T00:52:00,000T00:48:00,15-Dec-04,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-350T00:52:00,000T00:48:00,15-Dec-04,VIMS,SPASS Rider,Dione,REGMAP,Regional mapping,Dione ride with ISS,"24x12i2-v3 double/triple res 160 ms , 640 ms pairs, do one set every 5 minutes (repeat 9). 1.5 mbits per set, compressed. 13.5 mbits total compressed",,,,,, 2004-350T01:40:00,000T00:42:00,15-Dec-04,CIRS,Prime,Dione,FP1DRKMAP,CIRS FP1 dark side map,FP1 map of predawn dark side,"FP1 map of predawn darkside in search of thermal anomalies and for thermal inertia investigation. One WAC SI at midpoint of observation. Two 8x8 FP1 mosaics, 15.5 cm-1 resolution. Sub-S/C=(28,007), LT=0600, phase=111, AD=12.4 mrad. Timing chosen to optimize darkside coverage vs spatial resolution. Note: offset of FP1 from -Y makes only VIMS, ISS capable of riding along.",,,,,, 2004-350T01:40:00,000T00:42:00,15-Dec-04,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-350T01:40:00,000T00:42:00,15-Dec-04,VIMS,SPASS Rider,Dione,FP1DRKMAP,CIRS FP1 dark side map,Dione ride with CIRS,"24x12i2-v3 double/triple res 160 ms , 640 ms pairs, do one set every 5 minutes (repeat 8). 1.5 mbits per set, compressed. 12 mbits total compressed",,,,,, 2004-350T02:22:00,000T02:00:00,15-Dec-04,RADAR,Prime,Dione,SCATTRADL,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Dione/Mimas,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2004-350T04:22:00,000T01:00:00,15-Dec-04,INMS,Prime,Saturn,INMAGSCN,Inner magnetosphere scan,Rev B Periapse,Part of Saturn TWT periapse. Inner magnetosphere ion composition observation.,,,,,, 2004-350T05:22:00,000T11:28:01,15-Dec-04,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"MAPS magnetospheric survey,INMS switches to outer Mag outside 8 Rs.",,,,,, 2004-350T05:25:00,000T08:57:00,15-Dec-04,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2004-350T06:00:00,000T04:14:00,15-Dec-04,CDA,Non-SPASS,RingE,ERING,E ring observation,Ering after periapsis to RPX,within Ering,,,,,, 2004-350T07:30:00,000T00:15:00,15-Dec-04,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2004-350T07:50:00,000T00:05:00,15-Dec-04,RPWS,Non-SPASS,Saturn,HRSED,Highest resolution saturn kilometric radiation observation,Highest Resolution SED Observations,"Obtain the highest resolution observations of Saturn Electrostatic Discharges (SED) by using the RPWS HF-WBR mode at ~180 kbps within 6 RS for a total of 60 minutes within the first 12 periapses inside of 6 RS. Results will help to verify the source as lightning, or provide evidence that they could be of some other origin (e.g. rings). No attitude requirement.",,,,,, 2004-350T09:15:00,000T05:15:00,15-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-350T10:14:00,000T02:00:00,15-Dec-04,CDA,SPASS Rider,RingE,RPX,Ring plane crossing,RPX at 5.8 Rs,"E-Ring Plane Crossing at 5.8 Rs; to accommodate the downlink here, we agree to have -z2Earth. CDA have to have to define an appropriate 2ndary axis to hold its prime request here. The relevant downlink request is: SP_00BEA_G70METNON350_Prime.",,,,,, 2004-350T10:33:00,000T02:00:00,15-Dec-04,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2004-350T12:14:00,000T04:46:00,15-Dec-04,CDA,Non-SPASS,RingE,ERING,E ring observation,Ering after RPX,within Ering,,,,,, 2004-350T14:22:00,000T09:38:00,15-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-350T15:22:00,000T08:38:00,15-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-350T16:22:00,000T03:08:00,15-Dec-04,UVIS,Prime,rings(general),IMPACT,,,"Use UVIS HSP and FUV to detect flashes from meter-sized interplanetary impactors on rings to constrain flux of important impact population for ring origin/evolution. HSP/FUV FOV in shadow: 1.5 hrs (absorbing turn times); WAC to B ring, R ansa: 30 minutes (allows 3 WACs and 2 VIMS exposures); repeat once.",,,,,, 2004-350T16:22:00,000T03:08:00,15-Dec-04,CIRS,SPASS Rider,rings(general),IMPACT,,CIRS_00B_RI_IMPACT_UVIS,ride with VIMS,,,,,, 2004-350T16:22:00,000T03:08:00,15-Dec-04,ISS,SPASS Rider,rings(general),IMPACT,,"IMPACT spoke imaging on R ansa, combined with exte","3 WACs in B ring R ansa in middle and end of observation. Phase angle 150 degrees, get some wavelength coverage",,,,,, 2004-350T16:22:00,000T03:08:00,15-Dec-04,VIMS,SPASS Rider,rings(general),IMPACT,,B ring mapping during UVIS impact observations,B ring spoke studies rinding on UVIS IMPACT,,,,,, 2004-350T16:50:01,000T07:09:59,15-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-350T17:00:00,000T07:00:00,15-Dec-04,CDA,Non-SPASS,DustRAM direction,RNGMAR,,Ring margin,Ring margin dust measurements,,,,,, 2004-350T19:30:00,000T04:00:00,15-Dec-04,CIRS,Prime,rings(general),TEMPL06MP,Thermal map,CIRS_00BRI_TempU05LP,"Afternoon radial scan of main rings to obtain thermal measurement of rings. -Y to rings, Z perp to rings",,,,,, 2004-350T19:30:00,000T04:00:00,15-Dec-04,CIRS,SPASS Rider,rings(general),TEMPL06MP,Thermal map,CIRS_00BRI_TEMPL06MP_SI,"Stare at West ansa, low phase, lit face -Y to ring, +Z perpendicular to ring radius",,,,,, 2004-350T19:30:00,000T04:00:00,15-Dec-04,VIMS,SPASS Rider,rings(general),TEMPL06MP,Thermal map,VIMS scan during CIRS temperature scan,Rider on CIRS temperature scan. Probably small cubes at 80 & 320 msec IR exposures. VIS on. Remaining details TBD.,,,,,, 2004-351T00:00:00,000T13:22:00,16-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-351T00:00:00,000T13:22:00,16-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-351T00:00:00,000T13:22:00,16-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-351T00:00:00,000T13:22:00,16-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-351T00:00:00,000T10:20:00,16-Dec-04,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-351T00:00:00,000T04:22:00,16-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-351T00:00:01,000T04:21:59,16-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-351T03:00:00,000T06:00:00,16-Dec-04,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2004-351T04:22:00,000T09:00:00,16-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-351T04:22:00,000T09:00:00,16-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-351T10:20:00,000T03:02:00,16-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-351T13:22:00,000T10:38:00,16-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-351T13:22:00,012T16:38:00,16-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-351T13:22:00,000T01:22:00,16-Dec-04,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,STARTUP,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2004-351T13:22:00,004T16:02:00,16-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-351T13:22:00,000T10:38:00,16-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-351T13:22:00,000T10:38:00,16-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-351T14:44:00,000T16:01:00,16-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-352T00:00:00,004T05:30:00,17-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-352T00:00:00,000T09:10:00,17-Dec-04,CAPS,SPASS Rider,InstrumentCalibration,CALIBRATE,Calibration,CAPS Calibration,"CAPS periodic gain test and calibration. The specified rate and data volume are the delta above the CAPS survey rate (1000 bps), and the rate is the average over the entire request (current plans are to conduct the test in two different rates.)",,,,,, 2004-352T00:00:00,004T05:19:00,17-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-352T00:00:01,000T17:30:00,17-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-352T04:22:00,000T09:00:00,17-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-352T06:45:00,001T00:00:00,17-Dec-04,INMS,Non-SPASS,Saturn,PTOTM008,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-352T17:30:01,003T11:46:59,17-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-353T04:22:00,000T09:00:00,18-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-353T06:45:00,002T22:29:00,18-Dec-04,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-353T13:23:00,000T03:37:00,18-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-354T04:07:00,000T09:00:00,19-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-354T13:07:00,000T03:53:00,19-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-355T04:07:00,000T09:00:00,20-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-355T13:07:00,000T03:53:00,20-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-356T05:11:00,000T00:15:00,21-Dec-04,CAPS,SPASS Rider,SpacecraftActivity,SLEEPMUTE,Huygens probe support,Sleep/Mute for Probe activity,"sleep instrument. Mute if that is required, if not, just sleep.",,,,,, 2004-356T05:12:00,000T03:08:00,21-Dec-04,CDA,Non-SPASS,DustRAM direction,PROBEMUTE,Huygens Probe support,Mute CDA for probe activities,CDA mute/sleep for probe avtivity followed by unmute/on,,,,,, 2004-356T05:13:00,000T00:11:00,21-Dec-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,,"Put CIRS to sleep/mute to stop mirror scan. Due to large forces during release, may require mirror latching.",,,,,, 2004-356T05:14:00,000T00:10:00,21-Dec-04,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,Probe Pre-Sep preparation,Sleep mode and muted for probe pre-seperation.,,,,,, 2004-356T05:15:00,000T00:04:00,21-Dec-04,ISS,Non-SPASS,Other,SLEEP,Instrument to sleep mode,Put ISS to sleep for probe separation,placeholder activity put into CIMS to remind ISS to go into sleep for probe separation at request of SPVT leads,,,,,, 2004-356T05:17:00,000T03:19:00,21-Dec-04,MIMI,SPASS Rider,Other,MUTEPRMTU,Mute instrument for Probe Checkout,Sleep and Mute for Probe MTU Loading,MIMI_Mute_for_Probe_MTU,,,,,, 2004-356T05:19:00,000T03:26:00,21-Dec-04,RPWS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,RPWS Sleep and Mute for Probe activity,"RPWS sleep/mute for Probe activity, followed by unmute/sleep.",,,,,, 2004-356T05:21:00,000T00:01:00,21-Dec-04,UVIS,Non-SPASS,Saturn,SLEEPMUTE,Huygens probe support,UVIS TO SLEEP/MUTE (pre probe release - MTU ld),UVIS to go to sleep/mute pre probe release - MTU loading(SOC request 6/16/03),,,,,, 2004-356T05:22:00,000T00:05:00,21-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMS SLEEP/MUTE for Probe Preseparation Activity,VIMS to SLEEP amd MUTE for Probe Preseparation Activity,,,,,, 2004-356T05:24:00,000T03:12:00,21-Dec-04,INMS,Non-SPASS,Saturn,MUTE,Instrument to sleep mode,Muting Instrument for Probe Activities,MAPS magnetospheric survey.,,,,,, 2004-356T05:24:00,000T00:04:00,21-Dec-04,ISS,Non-SPASS,Other,MUTE,Instrument to sleep mode,Mute ISS for probe pre separation.,placeholder activity put into CIMS to remind ISS to mute for probe pre-separation at request of SPVT leads,,,,,, 2004-356T05:24:00,000T03:12:00,21-Dec-04,MAG,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,MAG Mute for Probe MTU Load,Mute MAG for probe activity. Assume can remain active as for previous Probe checkouts. Note: Snapshots would allow data collection in this period.,,,,,, 2004-356T05:30:00,000T03:00:00,21-Dec-04,PROBE,Non-SPASS,Earth,PRESEPARA,Huygens Probe support,Probe Pre-Separation Configuration,"Loading of Probe Mission Timer, selection of USO or TCXO, patch deletion if necessary. X-band downlink required. Sleep and muted:ISS, UVIS, VIMS, CAPS, CDA, MIMI, RPWS. MAG ON and muted. Off: CIRS, INMS all others.",,,,,, 2004-356T05:48:00,000T00:05:00,21-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,WAKEUP,Wakeup instrument from sleep mode,VIMS UNMUTE/ACTIVE after Probe Preseparation,VIMS to UNMUTE and ACTIVE after Probe Preseparation Activity,,,,,, 2004-356T08:36:00,003T10:50:00,21-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-356T08:36:00,000T00:15:00,21-Dec-04,CAPS,SPASS Rider,SpacecraftActivity,WAKEUNMUT,Huygens probe support,WakeUp/UnMute at Probe activity,wake up & unmute biu,,,,,, 2004-356T08:36:00,000T00:07:00,21-Dec-04,MIMI,SPASS Rider,Other,UNMUTEPR,RSS HGA boresight test,Sleep and Mute for Probe MTU Loading,MIMI_Mute_for_Probe_MTU,,,,,, 2004-356T08:36:00,000T00:05:00,21-Dec-04,CIRS,Non-SPASS,Other,PROBEWAKE,Huygens Probe support,wake/return to science mode,wake and return to science post-probe activity Extra heating may be required for mirror delatching.,,,,,, 2004-356T08:36:00,000T00:04:00,21-Dec-04,INMS,Non-SPASS,co-rotation,UNMUTE,Huygens probe support,Unmuting from probe activities,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-356T08:36:00,000T00:02:00,21-Dec-04,ISS,Non-SPASS,Other,UNMUTE,Huygens probe support,Unmute ISS after probe pre-separation,placeholder activity put into CIMS to remind ISS to unmute after probe pre-separation at request of SPVT leads,,,,,, 2004-356T08:36:00,003T10:40:00,21-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-356T08:40:00,001T12:50:00,21-Dec-04,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-356T08:41:00,000T00:02:00,21-Dec-04,ISS,Non-SPASS,Other,WAKE,,Wake ISS after probe pre-separation,placeholder activity put into CIMS to remind ISS to wake after probe pre-separation at request of SPVT leads,,,,,, 2004-356T08:43:00,003T10:47:00,21-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-356T08:45:00,003T19:37:00,21-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-356T08:47:00,000T00:02:00,21-Dec-04,UVIS,Non-SPASS,Saturn,UNMUTEWAK,Huygens probe support,UVIS to unmute and wake up after MTU loading,Unmute/go to active after MTU loading (SCO request 6/16/03),,,,,, 2004-356T13:07:00,000T03:53:00,21-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-357T04:07:00,000T09:00:00,22-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-357T13:07:00,000T03:38:00,22-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-357T21:30:00,000T09:00:00,22-Dec-04,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-358T03:52:00,000T09:00:00,23-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-358T06:30:00,001T00:00:00,23-Dec-04,INMS,Non-SPASS,co-rotation,PTOTM009,MAPS survey,MAPS,"Part of MB,high MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-358T12:53:00,000T03:52:00,23-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-359T03:52:00,000T09:00:00,24-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-359T06:30:00,000T13:30:00,24-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-359T12:53:00,000T05:24:00,24-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-359T19:11:00,000T00:15:00,24-Dec-04,CAPS,SPASS Rider,SpacecraftActivity,TCMCFG,,Mute for Probe Separation,mute biu & configure for probe separation,,,,,, 2004-359T19:13:00,000T00:11:00,24-Dec-04,CIRS,Non-SPASS,Other,PROBEMUTE,Huygens Probe support,,"Put CIRS to sleep/mute to stop mirror scan. Due to large forces during release, may require mirror latching.",,,,,, 2004-359T19:14:00,000T13:16:00,24-Dec-04,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,Probe Pre-Sep preparation,Sleep for probe separation.,,,,,, 2004-359T19:15:00,000T00:04:00,24-Dec-04,ISS,Non-SPASS,Other,SLEEP,Instrument to sleep mode,Put ISS to sleep for probe separation,placeholder activity put into CIMS to remind ISS to go into sleep for probe separation at request of SPVT leads,,,,,, 2004-359T19:16:00,000T13:16:00,24-Dec-04,MAG,Non-SPASS,InstrumentCalibration,PROBERLSE,Huygens Probe support,MAG Probe Release Monitoring,"Make magnetic field measurements before, during and after probe release. Will allow the change in spacecraft magnetic field to be assessed plus we may be able to detect the spin up and separation of the probe itself as supplementary data for the probe engineers. This requests starts acquisition of Snapshot data in the DPU and generates data at 1976bps during the release period.",,,,,, 2004-359T19:17:00,000T13:16:00,24-Dec-04,MIMI,SPASS Rider,Other,PRSEPSAFE,Huygens Probe support,Park LEMMS for Probe Separation,Park LEMMS at zero for Probe Separation,,,,,, 2004-359T19:21:00,000T00:01:00,24-Dec-04,UVIS,Non-SPASS,Saturn,PRBCFGSEP,Huygens Probe support,UVIS PRE PROBE RELEASE CONFIGURATION,Configure UVIS to LORES/FUV and OCCULTATION/EUV slit (as during launch),,,,,, 2004-359T19:22:00,000T00:02:00,24-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,VIMS to SLEEP for Probe Release,VIMS to SLEEP for Probe Release,,,,,, 2004-359T19:30:00,000T00:02:00,24-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,SLEEP,Instrument to sleep mode,VIMS to SLEEP for Probe Release,VIMS to SLEEP for Probe Release,,,,,, 2004-359T19:41:00,000T00:04:00,24-Dec-04,ISS,Non-SPASS,Other,WAKE,,Put ISS to wake after probe separation,placeholder activity put into CIMS to remind ISS to wake after probe separation at request of SPVT leads,,,,,, 2004-359T19:48:00,000T12:32:00,24-Dec-04,CDA,Non-SPASS,DustRAM direction,TCMCFG,,TCM configuration for probe release,TCM like mode for probe release,,,,,, 2004-359T20:00:00,000T00:00:00,24-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-360T04:22:00,005T14:01:00,25-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-360T08:26:00,001T14:54:00,25-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS -,unmute after Probe Separation & return to normal operation,,,,,, 2004-360T08:26:00,000T00:15:00,25-Dec-04,CAPS,SPASS Rider,SpacecraftActivity,STDCFG,,WakeUp/UnMute after Probe Separation,"unmute biu & recover from TBD ""safe"" state during probe separation",,,,,, 2004-360T08:29:00,000T00:02:00,25-Dec-04,CIRS,Non-SPASS,Other,PROBEWAKE,Huygens Probe support,wake/return to science mode,wake and return to science post-probe activity Extra heating may be required for mirror delatching.,,,,,, 2004-360T08:30:00,001T11:30:00,25-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-360T08:32:00,000T00:01:00,25-Dec-04,MAG,Non-SPASS,InstrumentCalibration,RELSEMRE,,MAG Probe Post Release Activities,Contains the activities for the post probe release reconfiguration mini-sequence MRE: starts readout of snapshot data stored during release period.,,,,,, 2004-360T08:32:00,005T09:51:00,25-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-360T08:33:00,000T06:00:00,25-Dec-04,MIMI,SPASS Rider,Other,PRSEPRSUM,,Resume after Probe Separation,"Resume after Probe Separation: resume LEMMS, raise INCA and CHEMS HV",,,,,, 2004-360T08:37:00,000T00:01:00,25-Dec-04,UVIS,Non-SPASS,Saturn,PRBPSTSEP,Huygens Probe support,UVIS POST PROBE RELEASE CONFIGURATION,Reconfigure UVIS after Probe Sep,,,,,, 2004-360T08:38:00,000T00:02:00,25-Dec-04,VIMS,Non-SPASS,SpacecraftActivity,ACTIVE,Huygens probe support,VIMS to ACTIVE after Probe Release,VIMS to ACTIVE after Probe Release,,,,,, 2004-360T14:20:00,005T04:03:00,25-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-360T18:37:00,000T09:00:00,25-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-361T03:37:00,000T09:00:00,26-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-361T19:54:00,000T03:12:00,26-Dec-04,MAG,Non-SPASS,Other,PROBEPSA,Huygens Probe support,MAG Snapshot for Probe Post-Sep PSA Checkout,Snapshot data during PSA checkout as telemetry mode does not pick up MAG data.,,,,,, 2004-361T20:00:00,000T03:00:00,26-Dec-04,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,Probe Post Separation Checkout,Sleep for probe separation.,,,,,, 2004-361T20:00:00,000T03:00:00,26-Dec-04,PROBE,Non-SPASS,Earth,PSACHECK,Huygens Probe support,PSA checkout following Probe separation,PSA functional check following Probe separation. Data does not have to be played back if realtime data is acquired successfully.,,,,,, 2004-361T23:00:00,003T19:23:00,26-Dec-04,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS -,unmute after Probe Separation & return to normal operation,,,,,, 2004-361T23:00:00,000T19:40:00,26-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-362T03:37:00,000T09:00:00,27-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-362T21:00:00,000T09:00:00,27-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-363T03:37:00,000T09:00:00,28-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-363T06:00:00,001T00:00:00,28-Dec-04,INMS,Non-SPASS,Saturn,PTOTM010,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-363T12:38:00,000T05:24:00,28-Dec-04,ISS,Prime,InstrumentCalibration,DARKCAL,Dark image calibration,"Dark images, NAC and WAC plus three cal lamp image",Ride along during system scans take 5 dark images,,,,,, 2004-364T03:38:00,000T09:00:00,29-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-364T06:00:00,000T18:00:00,29-Dec-04,CDA,Non-SPASS,DustRAM direction,DECON,Decontamination,target decontamination,decontaminate chemical analyser target,,,,,, 2004-364T06:00:00,001T16:30:00,29-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-365T00:00:00,001T06:45:00,30-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,survey,dust survey measurements,,,,,, 2004-365T03:23:00,000T09:00:00,30-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-365T18:23:00,000T12:54:00,30-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-365T18:23:00,000T07:07:00,30-Dec-04,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2004-365T18:23:00,000T07:07:00,30-Dec-04,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2004-365T18:23:00,000T07:07:00,30-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-365T18:23:01,000T07:06:59,30-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-365T22:30:00,000T03:00:00,30-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-366T01:30:00,000T05:47:00,31-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-366T01:30:00,001T04:00:00,31-Dec-04,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2004-366T01:30:00,000T05:47:00,31-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-366T01:30:01,000T05:47:53,31-Dec-04,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2004-366T01:45:00,000T02:44:00,31-Dec-04,RADAR,SPASS Rider,Other,WARM4IA,RADAR warmup,Scatterometry/Radiometry of Iapetus.,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2004-366T01:53:00,000T00:42:00,31-Dec-04,ISS,Prime,Iapetus,GLOBCOLA,Global coverage observation,Iapetus close flyby 00B/00C global color observati,Do 2x3 mosaic; first two ftprts multi color,,,,,, 2004-366T01:53:00,000T00:42:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,GLOBCOLA,Global coverage observation,FP3 phase coverage at 3 cm-1 resolution,"FP3 observation of Iapetus for moderate spectral resolution integration for composition, and for phase angle coverage. Phase=37, Local time=14.4, sub S/C=(-23, 070), AD=7.7 mrad. Duration 00:45. CIRS at 3 cm-1 resolution (11.5 sec/frame, 92RTI), blink. Shutter closed 00:05-00:10 and 00:35-00:40.",,,,,, 2004-366T01:53:00,000T00:42:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T02:35:00,000T00:57:00,31-Dec-04,CIRS,Prime,Iapetus,FP3MAP,CIRS FP3 map,FP3 phase coverage at 3 cm-1 resolution,"FP3 observation of Iapetus for map of subsolar point, and for phase angle coverage. Phase=51, Local time=14.4?, sub S/C=(-23, 070)?, AD=8.7 mrad. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Duration 01:00. Shutter closed 00:05-00:10 and 00:50-00:55. FP3 mosaic to cover the 95% pointing uncertainty shown in the CWIIT plot at slowest reasonable scan rate.",,,,,, 2004-366T02:35:00,000T00:57:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T03:32:00,000T00:57:00,31-Dec-04,VIMS,Prime,Iapetus,COMPA,Sit and stare to derive composition,Iapetus compositional mapping,"18x18 low res IR and Vis, at 640, 320, 160, 640, 320ms int. time for IR (and what is Vis equiv.), 1 set==10min; 36x18 hi res IR and Vis (effective FOV 18x18 for IR), 640 ,320 and 160ms, 4set==45min; 12x12 IR only low res, 2000ms (for area beyond 3microns)==4min.",,,,,, 2004-366T03:32:00,000T00:57:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,COMPA,Sit and stare to derive composition,"FP1,3,4 0.5 cm-1 resolution composition","FP3 observation of Iapetus for map of subsolar point, and for phase angle coverage. Phase=39, Local time=14.5, sub S/C=(-24, 069), AD=8.3 mrad. CIRS at 0.5 cm-1 resolution (50 sec/frame, 400RTI), blink, coadd. Duration 01:00; shutter closed 00:05-00:15 and 00:40-00:55.",,,,,, 2004-366T03:32:00,000T00:57:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T04:29:00,000T03:31:00,31-Dec-04,RADAR,Prime,Iapetus,SCATTRADL,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Iapetus.,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2004-366T07:17:00,001T21:15:00,31-Dec-04,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2004-366T07:17:00,001T21:21:00,31-Dec-04,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2004-366T07:17:00,001T21:21:00,31-Dec-04,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2004-366T07:17:55,000T22:12:05,31-Dec-04,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2004-366T07:18:00,005T04:34:00,31-Dec-04,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,dust survey measurements,,,,,, 2004-366T08:00:00,000T00:30:00,31-Dec-04,ISS,Prime,Iapetus,LIMBTOPOB,Limb topography and geodesy observation,Iapetus close flyby 00B/00C imaging,Do NAC 3x3 mosaic plus WAC 4-color context.,,,,,, 2004-366T08:00:00,000T00:30:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOB,Limb topography and geodesy observation,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=43, Local time=14.8, sub S/C=(-26, 066), AD=9.9 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:02-00:07 and 00:23-00:28.",,,,,, 2004-366T08:00:00,000T00:30:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T08:00:00,000T00:30:00,31-Dec-04,VIMS,SPASS Rider,Iapetus,LIMBTOPOB,Limb topography and geodesy observation,Iapetus,"12x12 low res, at 320ms (50 sec), one cube per ISS NAC footprint = 6 cubes; 42x21 hi res IR andVis, at 160, 320, 640 and 160ms==19min, while ISS dwells 20 min. to Iapetus center for WAC images.",,,,,, 2004-366T09:00:00,000T04:30:00,31-Dec-04,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2004-366T14:00:00,000T00:30:00,31-Dec-04,ISS,Prime,Iapetus,GLOBMAPC,Global coverage mapping,Iapetus close flyby 00B/00C global mapping,Do NAC 3x3+2 clear mosaic + WAC 4-color context,,,,,, 2004-366T14:00:00,000T00:30:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,GLOBMAPC,Global coverage mapping,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=54, Local time=15.5, sub S/C=(-30, 056), AD=13.3 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:02-00:07 and 00:23-00:28.",,,,,, 2004-366T14:00:00,000T00:30:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T14:00:00,000T00:30:00,31-Dec-04,VIMS,SPASS Rider,Iapetus,GLOBMAPC,Global coverage mapping,Iapetus global mapping,"12x12 low res IR and Vis at 320ms (50sec), one cube per ISS NAC footprint == 13 cubes; 32x32 low res IR and Vis at 320ms (5,5 min), while ISS dwells to Iapetus center for WAC images.",,,,,, 2004-366T14:30:00,000T04:00:00,31-Dec-04,CIRS,Prime,Iapetus,FP3DSKMAP,CIRS FP3 disk map,"FP3,1 disk maps at 15.5 cm-1 resolution","FP3,1 disk maps of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=79, Local time=15.6?, sub S/C=(-31, 054)?, AD=12.2 mrad. Duration 04:00. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Old instructions: 1) Two 14x15 mrad FP3 disk maps, with scans about Z at 11 urad/sec (03:40); shutter closed first and last 5 minutes of each. 2) Nyquist 9-scan FP1 map of disk (15.6 mradx15.6 mrad) (13 min). 3) Return to waypoint. New instructions: Cover the pointing uncertainties shown on the CWIIT plot with both FP1 and FP3. Increase the fraction of time on the FP1 map if necessary to cover the disk, including pointing uncertainties, with Nyquist sampling. Go to a single FP3 map if necessary, still covering the disk including pointing uncertainties.",,,,,, 2004-366T14:30:00,000T04:00:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T18:30:00,000T00:30:00,31-Dec-04,ISS,Prime,Iapetus,LIMBTOPOD,Limb topography and geodesy observation,Iapetus close flyby 00B/00C imaging,Do 2x3 NAC clear mosaic + WAC 4-color context,,,,,, 2004-366T18:30:00,000T00:30:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOD,Limb topography and geodesy observation,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=68, Local time=16.5, sub S/C=(-35, 040), AD=17.1 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:02-00:07 and 00:23-00:28.",,,,,, 2004-366T18:30:00,000T00:30:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T18:30:00,000T00:30:00,31-Dec-04,VIMS,SPASS Rider,Iapetus,LIMBTOPOD,Limb topography and geodesy observation,Iapetus,"12x12 low res, at 320ms (50 sec), one cube per ISS NAC footprint = 15 cubes; 32x32 hi res IR andVis, at 320ms (5.5min), while ISS dwells to Iapetus center for WAC images.",,,,,, 2004-366T19:00:00,000T02:00:00,31-Dec-04,VIMS,Prime,Iapetus,COMPD,Sit and stare to derive composition,Iapetus compositional mapping,"36x36 low res IR and Vis, at 640, 320 and 160ms, 2 sets ==49min; 36x36 hi res IR and Vis (effective FOV 18x36 for IR), at 640 and 160ms, repeat 4 times, total of 8 cubes ==71min.",,,,,, 2004-366T19:00:00,000T02:00:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,COMPD,Sit and stare to derive composition,"FP1,3,4 0.5 cm-1 resolution composition","FP3 observation of Iapetus for map of subsolar point, and for phase angle coverage. Phase=74, Local time=17.4, sub S/C=(-36, 033), AD=18.6 mrad. CIRS at 0.5 cm-1 resolution (50 sec/frame, 400RTI), blink, coadd. Duration 02:00; shutter closed 00:05-00:15, 00:53-01:07 and 01:40-01:55.",,,,,, 2004-366T19:00:00,000T02:00:00,31-Dec-04,ISS,SPASS Rider,Iapetus,COMPD,Sit and stare to derive composition,Iapetus close flyby 00B/00C local-color imaging,Do NAC color during VIMS prime period,,,,,, 2004-366T19:00:00,000T02:00:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T21:00:00,000T01:00:00,31-Dec-04,CIRS,Prime,Iapetus,FP13MAPS,CIRS FP1 / FP3 mapping,"FP1,3 disk maps at 15.5 cm-1 resolution","FP1,3 disk maps of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=101, Local time=17.8?, sub S/C=(-36, 024?), AD=12.6 mrad. Duration 01:00. Old Instructions: CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. 1) Square 21.5x21.5 mrad FP1 Nyquist (12 scan) disk map, (00:20); 2) 3-scan FP3 map of noon side of disk (9 mradx6 mrad) shutter closed first and last 5 minutes (38 min). New instructions: Cover the disk plus pointing uncertainties with both FP1 and FP3, reducing overlap between FP1 fovs if necessary (sub-Nyquist sampling) in order to complete the observation in the available time.",,,,,, 2004-366T21:00:00,000T01:00:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T22:00:00,000T00:30:00,31-Dec-04,ISS,Prime,Iapetus,LIMBTOPOE,Limb topography and geodesy observation,Iapetus close flyby 00B/00C imaging,Do NAC 2+2x4 clear mosaic (1 min dwell),,,,,, 2004-366T22:00:00,000T00:30:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,LIMBTOPOE,Limb topography and geodesy observation,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=85, Local time=18.1, sub S/C=(-37, 021), AD=20.3 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:02-00:07 and 00:23-00:28.",,,,,, 2004-366T22:00:00,000T00:30:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2004-366T22:00:00,000T00:30:00,31-Dec-04,VIMS,SPASS Rider,Iapetus,LIMBTOPOE,Limb topography and geodesy observation,Iapetus,"12x12 low res, at 320ms (50 sec), one cube per ISS NAC footprint = 15 cubes; 32x32 hi res IR andVis, at 320ms (5.5min), while ISS dwells to Iapetus center for WAC images.",,,,,, 2004-366T22:30:00,000T02:00:00,31-Dec-04,VIMS,Prime,Iapetus,COMPE,Sit and stare to derive composition,Iapetus compositional mapping,"24X48 low res IR and Vis, at 640, 320 and 160ms, 2 sets ==49min; 36x36 hi res IR and Vis, at 640 and 160ms, repeat 4 times, total of 8 cubes ==71min.",,,,,, 2004-366T22:30:00,000T02:00:00,31-Dec-04,CIRS,SPASS Rider,Iapetus,COMPE,Sit and stare to derive composition,"FP1,3,4 0.5 cm-1 resolution composition","FP3 VIMS rider on Iapetus for high spectral resolution and for phase angle coverage. Phase=93, Local time=18.9, sub S/C=(-36, 008), AD=21.3 mrad. CIRS at 0.5 cm-1 resolution (50 sec/frame, 400RTI), blink, coadd. Duration 02:00; shutter closed 00:05-00:15, 00:53-01:07 and 01:40-01:55.",,,,,, 2004-366T22:30:00,000T02:00:00,31-Dec-04,ISS,SPASS Rider,Iapetus,COMPE,Sit and stare to derive composition,Iapetus close flyby 00B/00C context imaging,Do WAC 4-color context observations at begin of VIMS prime period,,,,,, 2004-366T22:30:00,000T02:00:00,31-Dec-04,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T00:30:00,000T00:30:00,1-Jan-05,CIRS,Prime,Iapetus,FP13MAPS,CIRS FP1 / FP3 mapping,"FP1,3 disk maps at 15.5 cm-1 resolution","FP3 disk map of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=112, Local time=19.5?, sub S/C=(-34, 355)?, AD=12.0 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), Blink. Single FP3 scan along the long axis of the pointing uncertainty (see CWIIT plot), hoping to catch the lit crescent somewhere along the way.",,,,,, 2005-001T00:30:00,000T00:30:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T00:30:00,000T00:30:00,1-Jan-05,VIMS,SPASS Rider,Iapetus,CIRSRIDER,,Iapetus compositional mapping,"36x36 low res IR and Vis, at 160, 640 ms, 2 cubes",,,,,, 2005-001T01:00:00,000T01:00:00,1-Jan-05,ISS,Prime,Iapetus,GLOBMAPF,Global coverage mapping,Iapetus close flyby 00B/00C global mapping and gra,Do NAC 2+3+2 clear mosaic + WAC 4-color context; do NAC 1x3 graylight mosaic.,,,,,, 2005-001T01:00:00,000T00:30:00,1-Jan-05,CIRS,SPASS Rider,Iapetus,GLOBMAPF,Global coverage mapping,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=109, Local time=19.9, sub S/C=(-33, 351), AD=21.9 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:02-00:07 and 00:23-00:28.",,,,,, 2005-001T01:00:00,000T00:14:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T01:00:00,000T00:30:00,1-Jan-05,VIMS,SPASS Rider,Iapetus,GLOBMAPF,Global coverage mapping,Iapetus compositional mapping,"12x12 low res, at 320ms (50 sec), 9 cubes with one cube per ISS NAC footprint ==about 7,5 min 48x24 hi res IR and Vis, at 160, 320, 160ms, while ISS dwells 15 min to Iapetus center for WAC images.",,,,,, 2005-001T01:14:00,000T00:46:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T01:30:00,000T00:30:00,1-Jan-05,CIRS,SPASS Rider,Iapetus,GRAYLITEG,Graylight observstion,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=109, Local time=19.9, sub S/C=(-33, 351), AD=21.9 mrad. Duration 00:30. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:02-00:07 and 00:23-00:28. Same as previous.",,,,,, 2005-001T01:30:00,000T00:30:00,1-Jan-05,VIMS,SPASS Rider,Iapetus,GRAYLITEG,Graylight observstion,Iapetus compositional mapping,"12x12 low res IR and Vis (50sec), one cube per ISS NAC footprint, 7 cubes == 5.5min; 12x12 low res IR and Vis, at 320, 640 and 160ms (161sec), repeat 8 times, while ISS dwells to Iapetus center for WAC images ( 8 x 160sec), 24 cubes; total of 31 cubes.",,,,,, 2005-001T02:00:00,000T02:00:00,1-Jan-05,CIRS,Prime,Iapetus,FP13MAPS,CIRS FP1 / FP3 mapping,"FP1,3 disk maps at 15.5 cm-1 resolution","FP1,3 disk maps of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=117, Local time=20.0,? sub S/C=(-31, 334)?, AD=11.6 mrad. Duration 02:00. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), EVEN DETECTORS. 1) A single FP1 map of the disk, including pointing uncertainties shown on the CWIIT plot, (00:58); shutter closed 00:40-00:50 2) Single FP3 diametric scan along the full length of the pointing uncertainty direction (00:52); shutter closed 01:50-02:00.",,,,,, 2005-001T02:00:00,000T02:00:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T04:00:00,000T01:00:00,1-Jan-05,ISS,Prime,Iapetus,GRAYLITEH,Graylight observstion,Iapetus close flyby 00B/00C graylight imaging,Do NAC 3+3+24 mosaic + WAC 4-color context; do 1x4 NAC graylight mosaic.,,,,,, 2005-001T04:00:00,000T01:00:00,1-Jan-05,CIRS,SPASS Rider,Iapetus,GRAYLITEH,Graylight observstion,"FP1,3,4 ISS rider at 15.5 cm-1 resolution","FP1,3,4 rider observation of Iapetus for low spectral resolution spatial coverage, and for phase angle coverage. Phase=125, Local time=21.0, sub S/C=(-27, 334), AD=20.7 mrad. Duration 01:00. CIRS at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), blink. Shutter closed 00:10-00:15 and 00:45-00:50.",,,,,, 2005-001T04:00:00,000T01:00:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T05:30:00,000T06:00:00,1-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-001T05:30:00,000T06:00:00,1-Jan-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-001T05:30:00,000T06:00:00,1-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,dust survey-DataRate Change from Sponge,dust survey measurements,,,,,, 2005-001T05:30:00,000T06:00:00,1-Jan-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-001T05:30:00,000T06:00:00,1-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-001T06:30:00,000T05:00:00,1-Jan-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-001T06:30:00,000T05:00:00,1-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-001T11:30:00,000T17:08:00,1-Jan-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-001T11:30:00,000T17:08:00,1-Jan-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-001T12:00:00,000T01:30:00,1-Jan-05,CIRS,Prime,Iapetus,FP13MAPS,CIRS FP1 / FP3 mapping,"FP1,3 disk maps at 15.5 cm-1 resolution","FP1 disk map of Iapetus for moderate spectral resolution spatial coverage, and for phase angle coverage. At 2005-001T12:00 Phase=138, Local time=23.0?, sub S/C=(-11, 308)?, AD=8.7 mrad. Duration 01:30. CIRS at 3 cm-1 resolution (38 RTI), EVEN DETECTORS. 1) One FP1 Nyquist disk map, including the pointing uncertainties from the CWIIT plot; shutter closed 01:15-01:20.",,,,,, 2005-001T12:00:00,000T01:30:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T13:00:00,000T02:00:00,1-Jan-05,RADAR,SPASS Rider,Other,WARM4IA,RADAR warmup,Scatterometry/Radiometry of Iapetus.,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2005-001T13:30:00,000T01:00:00,1-Jan-05,ISS,Prime,Iapetus,DUSTSEAR,Dust observation,"Iapetus mapping, graylight, dust search",Do NAC 7 ftprt mosaic of crescent; do 1x5 NAC mosaic for graylight; do 1x5 NAC mosaic for dust search.,,,,,, 2005-001T13:30:00,000T01:00:00,1-Jan-05,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-001T15:00:00,000T08:45:00,1-Jan-05,RADAR,Prime,Iapetus,SCATTRADL,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Iapetus.,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2005-002T00:08:00,000T04:30:00,2-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-002T00:30:00,000T06:00:00,2-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-002T04:32:00,004T07:20:00,2-Jan-05,CAPS,Non-SPASS,Saturn,2XSURVEY,MAPS survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-002T04:38:00,000T03:52:00,2-Jan-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-002T04:38:00,004T07:00:00,2-Jan-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-002T04:38:00,004T07:15:00,2-Jan-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-002T04:38:00,000T07:15:00,2-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-002T04:38:01,004T07:00:59,2-Jan-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-002T08:30:00,001T12:30:00,2-Jan-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-002T12:08:00,000T06:00:00,2-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-002T18:08:00,000T09:00:00,2-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-003T02:00:00,000T03:00:00,3-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-003T03:08:00,000T09:00:00,3-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-003T12:08:00,000T06:00:00,3-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-003T18:08:00,000T09:00:00,3-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-003T21:00:00,000T09:00:00,3-Jan-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-004T03:08:00,000T09:00:00,4-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-004T06:00:00,001T00:00:00,4-Jan-05,INMS,Non-SPASS,Saturn,PTOTM010A,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-004T12:08:00,000T06:00:00,4-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-004T18:08:00,000T09:00:00,4-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-005T03:08:00,000T09:00:00,5-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-005T06:00:00,001T05:35:00,5-Jan-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-005T12:08:00,000T05:45:00,5-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-005T17:53:00,000T09:00:00,5-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-006T01:00:00,000T03:00:00,6-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-006T02:53:00,000T08:01:00,6-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-006T11:33:00,000T00:30:00,6-Jan-05,CAPS,SPASS Rider,Saturn,PWROFF,Huygens probe support,,CAPS Power off for Critical Sequence,,,,,, 2005-006T11:34:00,010T05:25:00,6-Jan-05,CDA,Non-SPASS,Earth,OFF,,CDA off for probe demo,see above,,,,,, 2005-006T11:35:00,000T00:05:30,6-Jan-05,CIRS,Non-SPASS,Other,CIRSOFF,,CIRS off,"Turn CIRS off for Probe Relay. prefer sleep, mute, WAIVER PENDING",,,,,, 2005-006T11:35:00,000T00:01:00,6-Jan-05,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,Sleep for PCS,MAPS magnetospheric survey.,,,,,, 2005-006T11:36:00,008T23:34:00,6-Jan-05,INMS,Non-SPASS,Saturn,POWEROFF,Instrument power OFF,Poweroff for Probe,Power off for Probe.,,,,,, 2005-006T11:37:00,000T00:04:00,6-Jan-05,ISS,Non-SPASS,Other,POWEROFF,Instrument power OFF,power off ISS to sleep for critical sequence,placeholder activity put into CIMS to remind ISS to power off for the critical sequence at request of SPVT leads,,,,,, 2005-006T11:38:00,009T00:32:00,6-Jan-05,MAG,Non-SPASS,Other,PROBESEQ,Huygens Probe support,MAG Activities During Probe Entry,MAG will be On but active/muted for this period to a) avoid switchoff of sensors and subsequent loss of offset information and b) allow internal storage of field data whilst muted during probe entry to provide supplementary science data for the probe mission. Will start snapshot data collection. End of snapshot data collection will be triggered by timetagged command. Snapshot period will be 14T00:00 to 12:00 - (approx descent start-3hrs to surface+40min). Will include mute commands for the critical period itself.,,,,,, 2005-006T11:39:00,008T23:21:00,6-Jan-05,MIMI,SPASS Rider,co-rotation,OFFPROBE,,Turn off for Probe activity,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-006T11:43:00,000T00:02:00,6-Jan-05,UVIS,SPASS Rider,InstrumentCalibration,TURNOFF,Instrument turn OFF,UVIS OFF before Probe Relay,UVIS powered off during Probe Relay (MAGTWT request),,,,,, 2005-006T11:44:00,000T00:03:00,6-Jan-05,VIMS,Non-SPASS,SpacecraftActivity,SLEEPMUTE,Huygens probe support,VIMSSleep/Mute for Probe Relay,VIMS Sleep/Mute for Porbe Relay.,,,,,, 2005-006T11:53:00,004T00:01:00,6-Jan-05,RPWS,Non-SPASS,Earth,OFF,,RPWS OFF,Perform RPWS OFF for Probr relay test,,,,,, 2005-014T09:06:38,000T00:00:00,14-Jan-05,PROBE,Non-SPASS,Titan,DESCENT,Huygens probe support,Huygens Probe Entry and Descent,"Probe Mission. Titan descent, data collection and relay to Orbiter. PRLY mode required. All orbiter instruments should be OFF for this operation.",,,,,, 2005-014T14:00:00,000T00:00:00,14-Jan-05,PROBE,Non-SPASS,Earth,PLAYBACK,,Huygens Probe first data playback,Probe Mission Data playback.,,,,,, 2005-015T11:00:00,000T06:00:00,15-Jan-05,MIMI,SPASS Rider,co-rotation,POWERON,Huygens Probe support,Turn on after Probe activity,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-015T11:10:00,002T01:20:00,15-Jan-05,INMS,Non-SPASS,Saturn,POWERON,Huygens Probe support,INMS Power On,"INMS Power On, post Probe Critical Sequence",,,,,, 2005-015T11:11:00,000T00:20:00,15-Jan-05,CIRS,Non-SPASS,Other,CIRSON,,CIRS wake-up sequence,Wake CIRS following Probe Relay. Instrument thermally stabilized by 24 hours,,,,,, 2005-015T11:11:00,000T00:04:00,15-Jan-05,ISS,Non-SPASS,Other,POWERON,Huygens Probe support,power on ISS after critical sequence,"placeholder activity put into CIMS to remind ISS to power on, wake, load IEBs and load patch after the critical sequence at request of SPVT leads",,,,,, 2005-015T12:10:00,000T05:07:00,15-Jan-05,MAG,Non-SPASS,Other,PROBEEND,Huygens Probe support,MAG Recovery After Probe Mission,"Recover MAG after probe mission. MAG is active/muted for probe mission, this request would unmute and trigger readout of snapshot data. Set MAG rate to 494bps for compatibility with other requests/sequences.",,,,,, 2005-015T12:15:00,000T00:05:00,15-Jan-05,UVIS,Non-SPASS,InstrumentCalibration,TURNON,Instrument turn ON,UVIS TURN ON AFTER PROBE RELAY,UVIS to power on after probe relay (MAGTWT request),,,,,, 2005-015T12:50:00,000T00:02:00,15-Jan-05,VIMS,Non-SPASS,SpacecraftActivity,ACTIVE,Huygens probe support,VIMS Power On After Probe Relay,VIMS active after Porbe Relay.,,,,,, 2005-015T17:17:00,000T10:30:00,15-Jan-05,CAPS,SPASS Rider,Other,PWRON,Huygens probe support,Power on,"CAPS Power on after Probe mission. Must be done in an S&ER telemetry mode, not RTE&SPB and must be part of a mini-sequence (see comments).",,,,,, 2005-015T17:17:00,002T16:43:00,15-Jan-05,CAPS,Non-SPASS,Other,SURVEY,Magnetospheric survey,Magnetospheric Survey,CAPS Power On after Critical Sequence for Probe; Continuous Low Rate Magnetospheric Survey,,,,,, 2005-015T17:17:00,000T00:01:00,15-Jan-05,CDA,Non-SPASS,Earth,ON,,CDA on after probe demo,null,,,,,, 2005-015T17:17:00,000T19:03:00,15-Jan-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-015T17:17:00,000T00:01:00,15-Jan-05,RPWS,Non-SPASS,Earth,ON,,RPWS ON,Turn RPWS ON,,,,,, 2005-015T17:17:00,001T17:35:00,15-Jan-05,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-015T17:18:00,000T13:22:00,15-Jan-05,CDA,Non-SPASS,DustRAM direction,ERING,E ring observation,dust in E ring,dust survey measurements beyond E-ring margin zone before periapsis,,,,,, 2005-015T17:47:00,000T00:33:00,15-Jan-05,CIRS,Prime,Enceladus,FP3STARE,CIRS FP3 stare,"FP3,4 stare","AD=0.9 mrad; phase=50; LT=14.8; Sub_S/C=(5, 68); duration=00:33. This observation begins just 30 min after CIRS turnon, so significant drift is expected. FPB to Enceladus, and stare throughout. CIRS at 38 RTI (4.75 sec frame); shutter closed 00:05-00:10 and 00:23-00:28; center detectors.",,,,,, 2005-015T17:47:00,000T00:33:00,15-Jan-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-015T17:47:00,000T00:33:00,15-Jan-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus distant longitude coverage,"12x12 hi/hi (3x640ms, 2x320ms, 2x160ms) repeat 3 times",,,,,, 2005-015T18:00:00,000T15:32:01,15-Jan-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-015T18:20:00,000T01:00:00,15-Jan-05,ISS,Prime,Enceladus,PHOTOM,Photometry,ENCELADUS Color Photometry/Polarization,3; Enceladus color/polarization NP09+N05 filters,,,,,, 2005-015T18:20:00,000T01:00:00,15-Jan-05,CIRS,SPASS Rider,Enceladus,PHOTOM,Photometry,"FP3,4 ISS rider","AD=1.0 mrad; phase=55; LT=15; Sub_S/C=(6, 73); duration=01:00. CIRS at 38 RTI (4.75 sec frame); shutter closed 00:10-00:15 and 00:45-00:50; center detectors.",,,,,, 2005-015T18:20:00,000T01:00:00,15-Jan-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-015T18:20:00,000T01:00:00,15-Jan-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus distant longitude coverage,"12x12 hi/hi (4x640ms, 3x320ms, 3x160ms) repeat 3 times",,,,,, 2005-015T19:20:00,000T02:30:00,15-Jan-05,ISS,Prime,Mimas,PHOTOM,Photometry,MIMAS Color Photometry/Polarization,"2; Mimas photometry/polarization, NP09+N05 Done twice",,,,,, 2005-015T19:20:00,000T02:30:00,15-Jan-05,CIRS,SPASS Rider,Mimas,PHOTOM,Photometry,"FP3,4 ISS rider","0.8.lt.AD.lt.1.1 mrad; 49.lt.phase.lt.67; LT=3.4; Sub_S/C=(5, 80); duration=02:30. CIRS at 125 RTI (2 cm-1 res., 15.6 sec frame); shutter closed 00:35-00:45 and 01:45-01:55; center detectors.",,,,,, 2005-015T19:20:00,000T02:30:00,15-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-015T19:20:00,000T02:30:00,15-Jan-05,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas distant longitude coverage,"12x12 hi/hi (4x640ms, 4x320ms, 4x160ms) repeat 4 times",,,,,, 2005-015T21:50:00,000T02:15:00,15-Jan-05,ISS,Prime,Enceladus,PHOTOM,Photometry,ENCELADUS Color Photometry/Polarization,2; Enceladus photometry/polarization. NP09+N05,,,,,, 2005-015T21:50:00,000T02:15:00,15-Jan-05,CIRS,SPASS Rider,Enceladus,PHOTOM,Photometry,"FP3,4 ISS rider","1.4.lt.AD.lt.1.7 mrad; 74.lt.phase.lt.90; LT=17; Sub_S/C=(9, 87); duration=02:15. CIRS at 38 RTI (4.75 sec frame); shutter closed 00:30-00:40 and 001:35-01:45; center detectors.",,,,,, 2005-015T21:50:00,000T02:15:00,15-Jan-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-015T21:50:00,000T02:15:00,15-Jan-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus distant longitude coverage,"12x12 hi/hi (4x640ms, 4x320ms, 4x160ms) repeat 4 times",,,,,, 2005-015T23:42:00,000T14:00:00,15-Jan-05,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. Need to do this inside 6 RS on at least half of the periapses inside of 6RS. No pointing requirement",,,,,, 2005-016T00:05:00,000T01:00:00,16-Jan-05,ISS,Prime,Rhea,REGGEODA,Regional geodesy,Rhea regional geodesy,Turn -Y to Rhea; do 1x1 mosaic in NAC clear filter at start and at end of dwell period (00:29 to 00:40 UTC); turn to WP.,,,,,, 2005-016T00:05:00,000T01:00:00,16-Jan-05,CIRS,SPASS Rider,Rhea,REGGEODA,Regional geodesy,"FP3,4 ISS rider","2.9.lt.AD.lt.3.1 mrad; phase=37; LT=10.5; Sub_S/C=(6, 321); duration=01:00. CIRS at 125 RTI (2 cm-1 res., 15.6 sec frame); shutter closed 00:10-00:15 and 00:45-00:50; blink detectors.",,,,,, 2005-016T00:05:00,000T01:00:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T00:05:00,000T01:00:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea distant longitude coverage,"20x20 hi/hi (2x640ms, 1x320ms, 2x160ms) repeat 2 times",,,,,, 2005-016T01:05:00,000T00:25:00,16-Jan-05,VIMS,Prime,Mimas,MIMAS,Mimas,Mimas distant longitude coverage,"12x12 hi/hi (4x640ms, 4x320ms, 4x160ms) repeat 2 times",,,,,, 2005-016T01:05:00,000T00:25:00,16-Jan-05,CIRS,SPASS Rider,Mimas,FP3FAZ0P5,CIRS FP3 phase coverage,FP3 phase coverage at 0.5 cm-1 resolution,"FP1 observation of Mimas for high spectral resolution integration for composition, and for phase angle coverage. Phase=87, Local time= , sub S/C=( 11, 128), AD= 2.0 mrad. Request FP3 sit and stare. CIRS to blink and coadd. Scan at 15.5, integration at 0.5 cm-1 resolution.",,,,,, 2005-016T01:05:00,000T00:25:00,16-Jan-05,ISS,SPASS Rider,Mimas,MIMAS,Mimas,MIMAS Color Photometry/Polarization,"Mimas photometry/polarization, NP09+N05",,,,,, 2005-016T01:05:00,000T00:25:00,16-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T01:30:00,000T01:00:00,16-Jan-05,UVIS,Prime,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Turn from waypoint to Enceladus center of brightness. Dwell 10 minutes. Scan from limb to limb at 4 microrad/sec. Dwell at center of brightness for any remaining time.,,,,,, 2005-016T01:30:00,000T01:00:00,16-Jan-05,CIRS,SPASS Rider,Enceladus,FP3HTSPOT,,FP3 search for endogenic activity.,"(C/A ~ 2005-016T06:46 @ 190K km => AD=2.7 mrad). AD~2.0 mrad, phase=105, (12, 91). Request very slow disk scan in X at <=7.5 urad/sec. CIRS to alternately blink and coadd; resolution 15.5 cm- 1.",,,,,, 2005-016T01:30:00,000T01:00:00,16-Jan-05,ISS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ENCELADUS Color Photometry/Polarization,2; Enceladus photometry/polarization. NP09+N05,,,,,, 2005-016T01:30:00,000T01:00:00,16-Jan-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus distant longitude coverage UVIS R/A,"16x16 hi/hi (3x640ms, 3x320ms, 1x160ms) repeat 3 times",,,,,, 2005-016T02:30:00,000T00:27:00,16-Jan-05,VIMS,Prime,Mimas,MIMAS,Mimas,Mimas distant longitude coverage,"16x16 hi/hi (3x640ms, 1x320ms, 2x160ms) repeat 2 times",,,,,, 2005-016T02:30:00,000T00:27:00,16-Jan-05,CIRS,SPASS Rider,Mimas,FP3SUBSOL,,FP3 map of subsolar region,"(C/A ~ 2005-016T06:08 @ 114K km => AD=3.4 mrad). Tsubsol~100K, AD=2.7 mrad, phase=95, (13, 139). Request FP3 scan in X at <=5 urad/sec across disk, then FP3 stare. CIRS to blink and coadd.",,,,,, 2005-016T02:30:00,000T00:27:00,16-Jan-05,ISS,SPASS Rider,Mimas,MIMAS,Mimas,MIMAS Color Photometry/Polarization,"Mimas photometry/polarization, NP09+N05",,,,,, 2005-016T02:30:00,000T00:27:00,16-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T03:20:00,000T09:00:00,16-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-016T05:42:00,000T00:15:00,16-Jan-05,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2005-016T06:40:00,000T04:20:00,16-Jan-05,CDA,Non-SPASS,DustRAM direction,ERING,E ring observation,dust in E ring betwe. periapsis and RPX,dust survey measurements after periapsis and before RPX,,,,,, 2005-016T06:42:00,000T00:05:00,16-Jan-05,RPWS,Non-SPASS,Saturn,HRSED,Highest resolution saturn kilometric radiation observation,Highest Resolution SED Observations,"Obtain the highest resolution observations of Saturn Electrostatic Discharges (SED) by using the RPWS HF-WBR mode at ~180 kbps within 6 RS for a total of 60 minutes within the first 12 periapses inside of 6 RS. Results will help to verify the source as lightning, or provide evidence that they could be of some other origin (e.g. rings). No attitude requirement.",,,,,, 2005-016T09:32:00,000T02:48:00,16-Jan-05,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2005-016T10:57:00,000T02:00:00,16-Jan-05,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2005-016T11:00:00,000T02:30:00,16-Jan-05,CDA,Non-SPASS,DustRAM direction,RPX,Ring plane crossing,dust during ring plane crossing,dust measurements during ring plane crossing,,,,,, 2005-016T12:20:00,001T00:10:00,16-Jan-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-016T12:40:10,000T01:19:50,16-Jan-05,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2005-016T12:59:00,000T00:57:00,16-Jan-05,VIMS,Prime,Mimas,MIMAS,Mimas,Mimas distant longitude coverage,"8x8 hi/hi (4x640ms, 4x320ms, 2x160ms) repeat 8 time",,,,,, 2005-016T12:59:00,000T00:57:00,16-Jan-05,CIRS,SPASS Rider,Mimas,MIMAS,Mimas,FP3 VIMS rider,"(C/A ~ 2005-016T06:08 @ 114K km => AD=3.4 mrad). Tsubsol~100K. Here: AD=1.5 mrad, phase=130, (0, 260). Request FP3 scan in X at <=5 urad/sec across disk, then FP3 stare. CIRS at 15.5 cm-1 resolution (38 RTI, 4.75 sec/frame); center detectors. Duration 01:00; shutter closed 00:05-00:10 and 00:45-00:50.",,,,,, 2005-016T12:59:00,000T00:57:00,16-Jan-05,ISS,SPASS Rider,Mimas,MIMAS,Mimas,MIMAS Color Photometry/Polarization,"Mimas photometry/polarization, NP09+N05",,,,,, 2005-016T12:59:00,000T00:57:00,16-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T13:30:00,000T09:30:00,16-Jan-05,CDA,Non-SPASS,DustRAM direction,ERING,E ring observation,dust in E ring after periapsis and RPC,dust survey measurements after periapsis and RPC,,,,,, 2005-016T13:56:00,000T01:04:00,16-Jan-05,UVIS,Prime,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Turn from waypoint to Enceladus center of brightness. Dwell 10 minutes. Scan from limb to limb at 4 microrad/sec. Dwell at center of brightness for remaining time.,,,,,, 2005-016T13:56:00,000T01:04:00,16-Jan-05,CIRS,SPASS Rider,Enceladus,FP3HTSPOT,,FP3 search for endogenic activity.,"(C/A ~ 2005-016T06:46 @ 190K km => AD=2.7 mrad). AD~2.5 mrad, phase=148, ( -4, 136). Request very slow disk scan in X at <=7.5 urad/sec. CIRS to alternately blink and coadd; resolution 15.5 cm- 1.",,,,,, 2005-016T13:56:00,000T01:04:00,16-Jan-05,ISS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ENCELADUS Color Photometry/Polarization,2; Enceladus photometry/polarization. NP09+N05,,,,,, 2005-016T13:56:00,000T01:04:00,16-Jan-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus distant longitude coverage UVIS R/A,"16x16 hi/hi (4x640ms, 4x320ms) repeat 2 times",,,,,, 2005-016T14:00:00,000T22:30:00,16-Jan-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-016T15:00:00,000T00:32:00,16-Jan-05,VIMS,Prime,Mimas,MIMAS,Mimas,Mimas distant longitude coverage,"6x6 hi/hi (4x640ms, 4x320ms, 2x160ms) repeat 8 times",,,,,, 2005-016T15:00:00,000T00:32:00,16-Jan-05,CIRS,SPASS Rider,Mimas,MIMAS,Mimas,FP3 VIMS rider,"(C/A ~ 2005-016T06:08 @ 114K km => AD=3.4 mrad). Tsubsol~100K. Here AD=1.1 mrad, phase=140, (-2, 275). Request FP3 scan in X at <=5 urad/sec across disk, then FP3 stare. CIRS at 15.5 cm-1 resolution (38 RTI, 4.75 sec/frame); blink. Duration 00:32; shutter closed 00:05-00:10, 00:24-00:29.",,,,,, 2005-016T15:00:00,000T00:32:00,16-Jan-05,ISS,SPASS Rider,Mimas,MIMAS,Mimas,MIMAS Color Photometry/Polarization,"Mimas photometry/polarization, NP09+N05",,,,,, 2005-016T15:00:00,000T00:32:00,16-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T15:32:00,000T00:37:00,16-Jan-05,CIRS,SPASS Rider,Rhea,WAYPTTURN,Waypoint turn,"FP1,3,4 SP turn rider for calibration","SP turn rider for calibration of Rhea observations. CIRS at 28 RTI (one-sided 15.5 cm-1 res., 3.5 sec frame); duration 00:37. Shutter closed 00:05-00:10 and 00:27-00:32; blink detectors.",,,,,, 2005-016T16:09:00,000T00:16:00,16-Jan-05,ISS,Prime,Rhea,REGGEODC,Regional geodesy,Rhea regional geodesy,Dwell at center of Rhea for whole request period.,,,,,, 2005-016T16:09:00,000T00:16:00,16-Jan-05,CIRS,SPASS Rider,Rhea,REGGEODC,Regional geodesy,"FP1,3 ISS rider","FP1,3,4 ISS rider on Rhea. Phase= 61, Local time= 7.8, sub S/C=( -12, 53), AD= 10.6 mrad. CIRS at one-sided 15.5 cm-1 spectral resolution (28 RTI, 3.5 sec/frame); first 3 min. shutter closed.",,,,,, 2005-016T16:09:00,000T00:16:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T16:09:00,000T00:16:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","6 x 12 low/low 320ms, 16reps, 1/min",,,,,, 2005-016T16:25:00,000T02:15:00,16-Jan-05,CIRS,Prime,Rhea,FP1DAYMAP,CIRS FP1 daytime map,FP1 dayside disk map,"FP1 disk maps, followed by FP3 disk scans of Rhea. Phase= 61, Local time= 0800, sub S/C=( -15, 63), AD= 10.5 mrad. Two FP1 disk maps, Nyquist sampled (~20 min). Then integrate FP1 5 mrad off sunlit limb of Rhea. Move FP1 to 2 mrad from sunlit limb and scan in +X across center of disk at 8 urad/sec until UVISB is off dark limb. Step up in Z 3 mrad; then scan in -X 13 mrad at 8 urad/sec. Step down 6 mrad in Z, and scan 13 mrad in +X at 8 urad/sec. CIRS at 15.5 cm-1 spectral resolution.",,,,,, 2005-016T16:25:00,000T02:15:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T16:25:00,000T02:15:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A",64x64 hi/hi (2x640ms. 1x320ms),,,,,, 2005-016T18:40:00,000T00:15:00,16-Jan-05,ISS,Prime,Rhea,REGGEODD,Regional geodesy,Rhea regional geodesy,Do 2x5 mosaic in NAC clear filter (short dwell times),,,,,, 2005-016T18:40:00,000T00:15:00,16-Jan-05,CIRS,SPASS Rider,Rhea,REGGEODD,Regional geodesy,"FP1,3, 4 ISS rider","FP1,3,4 ISS rider on Rhea. Phase= 75, Local time= 6.9, sub S/C=( -17, 78), AD= 10.4 mrad. CIRS at one-sided 15.5 cm-1 spectral resolution (28 RTI, 3.5 sec/frame); blink; first 3 min. shutter closed.",,,,,, 2005-016T18:40:00,000T00:15:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T18:40:00,000T00:15:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","6 x 12 low/low 320ms, 15reps, 1/min",,,,,, 2005-016T18:55:00,000T01:35:00,16-Jan-05,CIRS,Prime,Rhea,FP1FAZ0P5,CIRS FP1 phase coverage,FP1 phase coverage at 0.5 cm-1 resolution,"FP1 observation of Rhea for high spectral resolution integration for composition, and FP3 scans of noon limb. Phase= 77, Local time= 0700, sub S/C=( -19, 87), AD= 10.0 mrad. Duration 01:35. Place FP1 just inside noon limb and integrate at 0.5 cm-1 resolution for 60 min. Then scan FP3,4/UVIS_FUV 5.4 mrad onto noon limb at 3 urad/sec (CIRS at 15.5 cm-1 resolution) -- (update from 4.5 mrad at 2.5 urad/sec, because cannot turn at half-urad/sec rates).",,,,,, 2005-016T18:55:00,000T01:35:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T18:55:00,000T01:35:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","24x48 lo/hi (2x640ms, 2x320ms) repeat 2 times",,,,,, 2005-016T20:30:00,000T00:15:00,16-Jan-05,ISS,Prime,Rhea,REGGEODE,Regional geodesy,Rhea regional geodesy,Do 2x3 mosaic in NAC clear filter,,,,,, 2005-016T20:30:00,000T00:15:00,16-Jan-05,CIRS,SPASS Rider,Rhea,REGGEODE,Regional geodesy,"FP1,3, 4 ISS rider","FP1,3,4 ISS rider on Rhea. Phase= 83, Local time= 6.0, sub S/C=( -21, 97), AD= 9.5 mrad. CIRS at one-sided 15.5 cm-1 spectral resolution (28 RTI, 3.5 sec/frame); blink; first 3 min. shutter closed.",,,,,, 2005-016T20:30:00,000T00:15:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T20:30:00,000T00:15:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","6 x 12 low/low 320ms, 15reps, 1/min",,,,,, 2005-016T20:45:00,000T01:35:00,16-Jan-05,CIRS,Prime,Rhea,FP3DSKSCN,CIRS FP3 disk scan,FP3 disk map,"FP3 scans across disk of Rhea to cover noon limb, and for phase angle coverage. Phase= 87, Local time= 0600, sub S/C=( -22, 107), AD= 9.3 mrad. Stand FP3 on equator at center of disk and scan 6 mrad in X across noon limb at 2.2 urad/sec. Displace FP3 down across equator 3 mrad, and scan back in X at 2.2 urad/sec. CIRS at 15.5 cm-1 spectral resolution.",,,,,, 2005-016T20:45:00,000T01:35:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T20:45:00,000T01:35:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","20x40 lo/hi (2x640ms, 2x320ms) repeat 3 times",,,,,, 2005-016T22:20:00,000T00:15:00,16-Jan-05,ISS,Prime,Rhea,REGGEODF,Regional geodesy,Rhea regional geodesy,Do 2x2+1 mosaic in NAC clear filter,,,,,, 2005-016T22:20:00,000T00:15:00,16-Jan-05,CIRS,SPASS Rider,Rhea,REGGEODF,Regional geodesy,"FP1,3, 4 ISS rider","FP1,3,4 ISS rider on Rhea. Phase= 93, Local time= 5.2, sub S/C=(-23, 115), AD= 8.5 mrad. CIRS at one-sided 15.5 cm-1 spectral resolution (28 RTI, 3.5 sec/frame); blink; first 3 min. shutter closed.",,,,,, 2005-016T22:20:00,000T00:15:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T22:20:00,000T00:15:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","6 x 12 low/low 320ms, 15reps, 1/min",,,,,, 2005-016T22:35:00,000T01:45:00,16-Jan-05,CIRS,Prime,Rhea,FP3DSKSCN,CIRS FP3 disk scan,FP3 disk scan,"FP3 scans across disk of Rhea to cover noon limb, and for phase angle coverage. Phase= 97, Local time= 0600, sub S/C=( -23, 124), AD= 8 mrad. Stand FP3 on equator at center of disk and scan 6 mrad in X across noon limb at 2.2 urad/sec. Displace FP3 down across equator 3 mrad, and scan back in X at 2.2 urad/sec. CIRS at 15.5 cm-1 spectral resolution. ALTERNATELY blink, and COADD to save data volume.",,,,,, 2005-016T22:35:00,000T01:45:00,16-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-016T22:35:00,000T01:45:00,16-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","20x40 lo/hi (2x640ms, 2x320ms) repeat 3 times",,,,,, 2005-016T23:00:00,000T15:00:00,16-Jan-05,CDA,Non-SPASS,DustRAM direction,RNGMAR,,dust survey ring margin zone,dust survey measurements beyond E-ring margin zone,,,,,, 2005-017T00:20:00,000T00:15:00,17-Jan-05,ISS,Prime,Rhea,REGGEODG,Regional geodesy,Rhea regional geodesy,Do 2+3 mosaic in NAC clear filter,,,,,, 2005-017T00:20:00,000T00:15:00,17-Jan-05,CIRS,SPASS Rider,Rhea,REGGEODG,Regional geodesy,"FP1,3, 4 ISS rider","FP1,3,4 ISS rider on Rhea. Phase= 102, Local time= 4.2, sub S/C=(-23, 132), AD= 7.6 mrad. CIRS at one-sided 15.5 cm-1 spectral resolution (28 RTI, 3.5 sec/frame); blink; first 3 min. shutter closed.",,,,,, 2005-017T00:20:00,000T00:15:00,17-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T00:20:00,000T00:15:00,17-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","6 x 12 low/low 320ms, 15reps, 1/min",,,,,, 2005-017T00:35:00,000T02:33:00,17-Jan-05,CIRS,Prime,Rhea,FP3SCNINT,CIRS FP3 integration,"FP3 disk scan, integration","FP3 scans across disk of Rhea to cover noon limb, and for phase angle coverage, followed by integration at high spectral resolution. Phase~105, Local time~0400, sub S/C=( -23, 147), AD~7 mrad. Stand FP3 on equator at center of disk and scan 5 mrad in X across noon limb at 2.2 urad/sec. Displace FP3 down across equator 3 mrad, and scan back in X at 2.2 urad/sec. CIRS at 15.5 cm-1 spectral resolution. Then place FP3,4/UVISB on lighted hemisphere and stare; CIRS at 0.5 cm-1 spectral resolution.",,,,,, 2005-017T00:35:00,000T02:33:00,17-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T00:35:00,000T02:33:00,17-Jan-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,"Rhea distant longitude coverage, CIRS R/A","48x48 hi/hi (4x640ms, 4x320ms)",,,,,, 2005-017T03:30:00,000T09:00:00,17-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-017T10:52:00,000T23:08:00,17-Jan-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-017T12:30:00,000T12:36:00,17-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-017T12:30:00,000T21:30:00,17-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-017T12:30:00,000T21:30:00,17-Jan-05,INMS,Non-SPASS,Saturn,POWERON,Huygens Probe support,INMS Survey,"INMS Power On, post Probe Critical Sequence",,,,,, 2005-017T12:30:00,000T21:30:00,17-Jan-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-017T12:30:00,000T21:30:00,17-Jan-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SUR Campaign,"Part of SUR MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-017T12:30:00,000T12:40:00,17-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-017T13:00:00,000T01:00:00,17-Jan-05,ISS,Prime,Mimas,LONPHA,Spectrophotometry / phase coverage,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-017T13:00:00,000T01:00:00,17-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T14:00:00,000T01:00:00,17-Jan-05,ISS,Prime,Dione,094W105PH,Spectrophotometery,Dione spectrophotometry/ phase coverage,Turn -Y to Dione; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-017T14:00:00,000T01:00:00,17-Jan-05,CIRS,SPASS Rider,Dione,094W105PH,Spectrophotometery,"FP1,3, 4 ISS rider","FP3 ISS rider on Dione. Phase= 105, Local time=4.7, sub S/C=(-9, 92), AD= 1.2 mrad. CIRS at 15.5 cm-1 spectral resolution (38 RTI, 4.75 sec/frame); center detectors. Duration 01:00; shutter closed 00:05-00:10, 00:50-00:55. Coadd.",,,,,, 2005-017T14:00:00,000T01:00:00,17-Jan-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T14:00:00,014T13:35:00,17-Jan-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,dust survey measurements,,,,,, 2005-017T15:00:00,000T00:45:00,17-Jan-05,ISS,Prime,Tethys,LONPHA,Spectrophotometry / phase coverage,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-017T15:00:00,000T00:45:00,17-Jan-05,CIRS,SPASS Rider,Tethys,LONPHA,Spectrophotometry / phase coverage,FP3 ISS rider,"FP3 ISS rider on Tethys. Phase= 109, Local time=4.3, sub S/C=(-9, 80), AD= 1.0 mrad. CIRS at 15.5 cm-1 spectral resolution (38 RTI, 4.75 sec/frame); center detectors. Duration 00:45; shutter closed 00:05-00:10, 00:35-00:40. Coadd.",,,,,, 2005-017T15:00:00,000T00:45:00,17-Jan-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T15:45:00,000T00:45:00,17-Jan-05,ISS,Prime,Enceladus,LONPHA,Spectrophotometry / phase coverage,Enceladus spectrophotometry/ phase coverage,Turn -Y to Enceladus; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-017T15:45:00,000T00:45:00,17-Jan-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T16:30:00,000T00:50:00,17-Jan-05,ISS,Prime,Tethys,094W109PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-017T16:30:00,000T00:50:00,17-Jan-05,CIRS,SPASS Rider,Tethys,094W109PH,Spectrophotometery,FP3 ISS rider,"FP3 ISS rider on Tethys. Phase= 108, Local time=4.3, sub S/C=(-10, 92), AD= 1.1 mrad. CIRS at 15.5 cm-1 spectral resolution (38 RTI, 4.75 sec/frame); center detectors. Duration 00:50; shutter closed 00:05-00:10, 00:40-00:45. COADD.",,,,,, 2005-017T16:30:00,000T00:50:00,17-Jan-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T17:20:00,000T00:40:00,17-Jan-05,ISS,Prime,Mimas,LONPHA,Spectrophotometry / phase coverage,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-017T17:20:00,000T00:40:00,17-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T18:00:00,000T02:00:00,17-Jan-05,UVIS,Prime,Saturn,AURORA,Saturn aurora,Aurora observation,"Boxscan mosaic of the South Saturn Pole. 1. Slew about the Z-axis -2.302 deg from Saturn center (RA/DEC: 34.94/4.17deg) toward the South Saturn Pole (RA/DEC: 34.86/1.87deg). 2. Step 10 times about the Z-axis, using -1.425 mrad step increments, dwell for 600s during each step increment. 3. Slew back to Saturn center and reset pointing.",,,,,, 2005-017T20:00:00,000T00:45:00,17-Jan-05,ISS,Prime,Mimas,310W121PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-017T20:00:00,000T00:45:00,17-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T20:45:00,000T00:45:00,17-Jan-05,ISS,Prime,Mimas,LONPHA,Spectrophotometry / phase coverage,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-017T20:45:00,000T00:45:00,17-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T21:30:00,000T00:40:00,17-Jan-05,ISS,Prime,Enceladus,LONPHA,Spectrophotometry / phase coverage,Enceladus spectrophotometry/ phase coverage,Turn -Y to Enceladus; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-017T21:30:00,000T00:40:00,17-Jan-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T22:10:00,000T00:30:00,17-Jan-05,ISS,Prime,Tethys,LONPHA,Spectrophotometry / phase coverage,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-017T22:10:00,000T00:30:00,17-Jan-05,CIRS,SPASS Rider,Tethys,LONPHA,Spectrophotometry / phase coverage,FP3 ISS rider,"FP3 ISS rider on Tethys. Phase= 109, Local time=4.3, sub S/C=(-12, 135), AD= 1.1 mrad. CIRS at 15.5 cm-1 spectral resolution (38 RTI, 4.75 sec/frame); center detectors. Duration 00:30; shutter closed 00:05-00:10, 00:20-00:25. COADD.",,,,,, 2005-017T22:10:00,000T00:30:00,17-Jan-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-017T22:40:00,000T02:00:00,17-Jan-05,UVIS,Prime,rings(general),IMPACT,,,Use UVIS HSP and FUV to detect flashes from meter-sized interplanetary impactors on rings to constrain flux of important impact population for ring origin/evolution.,,,,,, 2005-017T22:40:00,000T02:00:00,17-Jan-05,ISS,SPASS Rider,rings(general),IMPACT,,URIMPACT spoke and F ring imaging on each ansa,"Two WACs at each ansa, beginning and end. pointing by UVIS.",,,,,, 2005-017T22:40:00,000T02:00:00,17-Jan-05,VIMS,SPASS Rider,rings(general),IMPACT,,F Ring during UVIS impact observations,F Ring observations during UVIS searches for ring impacts.,,,,,, 2005-018T01:10:00,000T08:50:00,18-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-018T01:30:00,000T06:00:00,18-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-018T02:10:00,000T07:50:00,18-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-018T02:11:00,000T05:11:28,18-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-018T10:00:00,003T00:38:00,18-Jan-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-018T10:00:00,004T00:38:00,18-Jan-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-018T10:00:00,013T17:35:00,18-Jan-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,dust survey,dust survey measurements,,,,,, 2005-018T10:00:00,004T00:38:00,18-Jan-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,INMS further out and running survey,Running Default Scinece at 50 bps,,,,,, 2005-018T10:00:00,004T00:38:00,18-Jan-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-018T10:00:00,003T00:38:00,18-Jan-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-018T13:00:00,000T00:30:00,18-Jan-05,ISS,Prime,Mimas,LONPHA,Spectrophotometry / phase coverage,Mimas spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-018T13:00:00,000T00:30:00,18-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-018T13:50:00,000T00:30:00,18-Jan-05,ISS,Prime,Tethys,LONPHA,Spectrophotometry / phase coverage,Tethys spectrophotometry/ phase coverage,Turn -Y to Enceladus; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-018T13:50:00,000T00:30:00,18-Jan-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-018T16:30:00,000T00:30:00,18-Jan-05,ISS,Prime,Enceladus,LONPHA,Spectrophotometry / phase coverage,Enceladus spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-018T16:30:00,000T00:30:00,18-Jan-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-018T17:00:00,000T03:00:00,18-Jan-05,UVIS,Prime,rings(general),IMPACT,,,Use UVIS HSP and FUV to detect flashes from meter-sized interplanetary impactors on rings to constrain flux of important impact population for ring origin/evolution.,,,,,, 2005-018T17:00:00,000T03:00:00,18-Jan-05,CIRS,SPASS Rider,rings(general),IMPACT,,rider to UVIS rings impact,rider to UVIS impact observation,,,,,, 2005-018T17:00:00,000T03:00:00,18-Jan-05,ISS,SPASS Rider,rings(general),IMPACT,,URIMPACT spoke and F ring imaging on each ansa,One WAC at each ansa beginning and end; pointing by UVIS,,,,,, 2005-018T17:00:00,000T03:00:00,18-Jan-05,VIMS,SPASS Rider,rings(general),IMPACT,,F Ring imagingduring UVIS impact observation,"F Ring integrations during UVIS impact observation. IR 640 msec exp, VIS on, dimensions TBD.",,,,,, 2005-018T20:00:00,000T01:00:00,18-Jan-05,ISS,Prime,Mimas,LONPHA,Spectrophotometry / phase coverage,Mimas spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-018T20:00:00,000T01:00:00,18-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-019T00:23:00,000T00:30:00,19-Jan-05,ISS,Prime,Tethys,LONPHA,Spectrophotometry / phase coverage,Tethys spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer,,,,,, 2005-019T00:23:00,000T00:30:00,19-Jan-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-019T01:43:00,000T00:40:00,19-Jan-05,ISS,Prime,Rhea,310W121PH,Spectrophotometery,Rhea spectrophotometry/ phase coverage,Turn -Y to Rhea; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-019T01:43:00,000T00:40:00,19-Jan-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-019T02:53:00,000T09:00:00,19-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-019T05:00:00,000T03:00:00,19-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-019T13:00:00,000T00:30:00,19-Jan-05,ISS,Prime,Mimas,LONPHA,Spectrophotometry / phase coverage,Mimas spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosiac 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-019T13:00:00,000T00:30:00,19-Jan-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-019T13:30:00,000T11:00:00,19-Jan-05,VIMS,Prime,Saturn,REGAURORA,Regional Auroral map,Saturn Regional Aurora AND F ring clumps,Saturn Regional Aurora Map and F ring clumps,,,,,, 2005-019T13:30:00,000T11:00:00,19-Jan-05,ISS,SPASS Rider,Saturn,REGAURORA,Regional Auroral map,Fclump ansa observations; pointing by VIMS,Approx 2 BOTSIMS at each ansa every 2 hours,,,,,, 2005-020T01:53:00,000T09:00:00,20-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-020T04:00:00,000T03:00:00,20-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-020T12:00:00,000T00:30:00,20-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 044 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-PM-EN-PA-HE (602, 612, 614, 616, 617)]",,,,,, 2005-020T12:30:00,000T08:00:00,20-Jan-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,F Ring monitoring,F-ring monitor,,,,,, 2005-020T12:30:00,000T08:00:00,20-Jan-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring ansa observations; design by CIRS,"Approx 2 WACs at each ansa every 2 hours, 7 additional exposures and polarizations",,,,,, 2005-021T01:38:00,000T09:00:00,21-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-021T05:00:00,000T03:00:00,21-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-021T10:38:00,010T17:11:00,21-Jan-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-021T10:38:00,000T15:00:00,21-Jan-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-021T11:45:00,000T00:30:00,21-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 047 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 2 targets: [S2004S5, S2004S2]",,,,,, 2005-021T12:15:00,000T04:00:00,21-Jan-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,F Ring monitoring,F-ring monitor,,,,,, 2005-021T12:15:00,000T04:00:00,21-Jan-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring ansa observations; design by CIRS,"1 WAC each ansa every 2 hours, 2 extra exposures",,,,,, 2005-021T16:15:00,000T07:30:00,21-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-021T23:45:00,000T00:30:00,21-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 048 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 2 targets: [S2004S5, S2004S3]",,,,,, 2005-022T01:38:00,000T09:00:00,22-Jan-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-022T01:38:00,000T09:00:00,22-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-022T02:00:00,000T06:00:00,22-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-022T10:38:00,000T07:30:00,22-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-022T10:38:00,000T01:47:00,22-Jan-05,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,INMS Startup at beginning of S08,"INMS Power On, post Probe Critical Sequence",,,,,, 2005-022T10:38:00,012T22:22:00,22-Jan-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-022T10:38:00,000T07:30:00,22-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-022T10:38:00,009T16:57:45,22-Jan-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-022T10:38:01,009T16:57:43,22-Jan-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/high Campaign,"Part of MB/high MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-022T11:30:00,000T04:33:04,22-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-022T11:45:00,000T00:30:00,22-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 050 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-TL-HY-PM-EP (607, 610, 611, 613, 616)]",,,,,, 2005-022T12:15:00,000T04:00:00,22-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-022T12:25:00,001T23:05:00,22-Jan-05,INMS,Non-SPASS,Saturn,SLPLOADVR,,Sleep Until Table Load Verified,INMS survey.,,,,,, 2005-022T16:15:00,000T00:30:00,22-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 051 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-EN-AT-PA-JA (602, 610, 615, 616, 617)]",,,,,, 2005-022T18:08:00,000T09:00:00,22-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-022T20:00:00,000T06:00:00,22-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-023T03:08:00,000T22:15:00,23-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-023T03:08:00,000T22:15:00,23-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-023T04:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2LGTSEA,Lightning search,NAC Southern Hemisphere Saturn lightning search,2x2 NAC mos using the HAL+1 other filter. Obs repeat every 4 hours.,,,,,, 2005-023T04:30:00,000T09:06:08,23-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-023T06:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"2X2 mos, repeat every 4:00:00.",,,,,, 2005-023T08:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2LGTSEA,Lightning search,NAC Southern Hemisphere Saturn lightning search,2x2 NAC mos using the HAL+1 other filter. Obs repeat every 4 hours.,,,,,, 2005-023T10:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"2X2 mos, repeat every 4:00:00.",,,,,, 2005-023T12:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2LGTSEA,Lightning search,NAC Southern Hemisphere Saturn lightning search,2x2 NAC mos using the HAL+1 other filter. Obs repeat every 4 hours.,,,,,, 2005-023T14:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"2X2 mos, repeat every 4:00:00.",,,,,, 2005-023T16:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2LGTSEA,Lightning search,NAC Southern Hemisphere Saturn lightning search,2x2 NAC mos using the HAL+1 other filter. Obs repeat every 4 hours.,,,,,, 2005-023T18:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"2X2 mos, repeat every 4:00:00.",,,,,, 2005-023T20:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2LGTSEA,Lightning search,NAC Southern Hemisphere Saturn lightning search,2x2 NAC mos using the HAL+1 other filter. Obs repeat every 4 hours.,,,,,, 2005-023T22:15:00,000T01:00:00,23-Jan-05,ISS,Prime,Saturn,2X2MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"2X2 mos, repeat every 4:00:00.",,,,,, 2005-024T01:23:00,000T09:00:00,24-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-024T01:23:00,000T09:00:00,24-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-024T02:00:00,000T06:00:00,24-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-024T02:23:00,000T07:00:00,24-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-024T02:30:00,000T02:16:32,24-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-024T10:23:00,000T11:45:00,24-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-024T10:23:00,000T11:45:00,24-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-024T11:30:00,000T00:30:00,24-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,S/2004 S5 Retargettable,NACs and BOTSIMS FOR S/2004 S5 Retargettable,,,,,, 2005-024T11:30:00,003T22:38:00,24-Jan-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-024T12:00:00,000T04:00:00,24-Jan-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,F Ring monitoring,F-ring monitor,,,,,, 2005-024T12:00:00,000T04:00:00,24-Jan-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring ansa observations; design by CIRS,"1 WAC each ansa every 2 hours, 2 extra exposures",,,,,, 2005-024T12:00:00,000T09:06:08,24-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-024T16:00:00,000T04:30:00,24-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-024T20:30:00,000T00:30:00,24-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 057 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-EN-PA-AT-EP (602, 611, 615, 616, 617)]",,,,,, 2005-024T22:00:00,000T14:00:00,24-Jan-05,RSS,SPASS Rider,Earth,PATTERN,HGA pattern calibration,HGA Pattern Calibration,"HGA Pattern Calibration; Pointing: XBAND to Earth + two rastor scan maneuvers (one smaller for X and Ka bands, one larger for X and S bands). Last 10 hours required to be tracked at both DSS-25 and DSS-15 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation,",,,,,, 2005-024T22:08:00,000T03:52:00,24-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-025T02:00:00,000T01:00:00,25-Jan-05,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + 2 crosshair maneuvers. One hour required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2005-025T02:00:00,000T23:23:00,25-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-025T02:00:00,000T23:23:00,25-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-025T02:00:00,000T08:23:00,25-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-025T03:00:00,000T05:00:00,25-Jan-05,RSS,Prime,Earth,PATTERN,HGA pattern calibration,HGA Pattern Calibration,"HGA Pattern Calibration; Pointing: XBAND to Earth + large raster scan maneuver (for X and S bands, Ka-band if possible). Five hours required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation,",,,,,, 2005-025T08:00:00,000T01:46:00,25-Jan-05,RSS,Prime,Earth,IVDTEST,RSS Boresite calibration,IVD Boresight Calibration,"HGA Boresight Calibration; Pointing=XBAND to Earth + 3 IVD ""rose"" maneuvers. About two hours required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2005-025T09:46:00,000T00:20:00,25-Jan-05,RSS,Prime,Earth,RSSIVDTS,RSS boresight calibration,RSSIVD Boresight Calibration,"HGA Boresight Calibration; Pointing=XBAND to Earth + RSSIVD ""rose"" maneuver. 20 minutes required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2005-025T10:06:00,000T00:16:00,25-Jan-05,RSS,Prime,Earth,RSSIVDTS,RSS boresight calibration,RSSIVD Boresight Calibration,"HGA Boresight Calibration; Pointing=XBAND to Earth + RSSIVD ""rose"" maneuver. 16 minutes required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2005-025T10:22:00,000T00:38:00,25-Jan-05,RSS,Prime,Earth,RSSIVDTS,RSS boresight calibration,RSSIVD Boresight Calibration,"HGA Boresight Calibration; Pointing=XBAND to Earth + RSSIVD ""rose"" maneuver. 38 minutes required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2005-025T11:00:00,000T01:00:00,25-Jan-05,RSS,Prime,Earth,BPTEST,RSS blind pointing test,Blind Pointing/Monopulse Test,HGA Boresight Calibration; Pointing=XBAND to Earth. About one hour required to be tracked at both DSS-25 and DSS-14 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2005-025T13:00:00,000T00:30:00,25-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 059 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-DI-CP-PM-PA (604, 611, 614, 616, 617)]",,,,,, 2005-025T13:30:00,000T10:00:00,25-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-025T23:30:00,000T00:30:00,25-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 060 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [HE-MI-AT-EP-PA (601, 611, 612, 615, 617)]",,,,,, 2005-026T01:23:00,000T09:00:00,26-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-026T01:23:00,000T09:00:00,26-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-026T02:00:00,000T06:00:00,26-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-026T02:23:00,000T07:00:00,26-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-026T02:30:00,000T02:16:32,26-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-026T10:23:00,000T15:00:00,26-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-026T10:23:00,000T15:00:00,26-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-026T11:30:00,000T00:30:00,26-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 062 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-DI-EN-JA-PA (602, 604, 610, 615, 617)]",,,,,, 2005-026T11:30:00,000T04:33:04,26-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-026T12:00:00,000T04:00:00,26-Jan-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,F Ring monitoring,F-ring monitor,,,,,, 2005-026T12:00:00,000T04:00:00,26-Jan-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring ansa observations; design by CIRS,"1 WAC each ansa every 2 hours, 2 extra exposures",,,,,, 2005-026T13:00:00,000T03:00:00,26-Jan-05,RADAR,SPASS Rider,Other,SOUTHWARM,Instrument warmup,"Distant Titan Latitude Study, Southern Latitudes",Warmup for calibration and science data collection.,,,,,, 2005-026T16:00:00,000T02:00:00,26-Jan-05,RADAR,Prime,Titan,SOUTH7CAL,Distant Titan radiometery and calibration,"Distant Titan Latitude Study, Southern Latitudes",Obtain distant Titan radiometer science and calibration data. One of a set that provides coverage of Titan southern latitude variation along with some obtainable associated longitude variation.,,,,,, 2005-026T18:00:00,000T05:30:00,26-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-026T23:30:00,000T00:30:00,26-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 063 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-PM-PA-EP-CP (611, 614, 615, 616, 617)]",,,,,, 2005-027T01:23:00,000T09:00:00,27-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-027T02:00:00,000T06:00:00,27-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-027T10:23:00,000T14:45:00,27-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-027T10:23:00,000T14:45:00,27-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-027T11:30:00,000T00:30:00,27-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 065 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [MI-AT-JA-HE-PM (601, 610, 612, 615, 616)]",,,,,, 2005-027T12:00:00,000T04:00:00,27-Jan-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,F Ring monitoring,F-ring monitor,,,,,, 2005-027T12:00:00,000T04:00:00,27-Jan-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring ansa observations; design by CIRS,"1 WAC each ansa every 2 hours, 2 extra exposures",,,,,, 2005-027T16:00:00,000T07:30:00,27-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-027T23:30:00,000T00:30:00,27-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 066 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-PA-PM-EN-DI (602, 604, 611, 616, 617)]",,,,,, 2005-028T01:08:00,000T09:00:00,28-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-028T10:08:00,000T15:00:00,28-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-028T10:08:00,001T00:00:00,28-Jan-05,INMS,Non-SPASS,co-rotation,PTOTM012,MAPS survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-028T10:08:00,000T15:00:00,28-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-028T11:30:00,000T00:30:00,28-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 068 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EN-EP-TL-JA-AT (602, 610, 611, 613, 615)]",,,,,, 2005-028T12:00:00,000T04:00:00,28-Jan-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,F Ring monitoring,F-ring monitor,,,,,, 2005-028T12:00:00,000T04:00:00,28-Jan-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring ansa observations; design by CIRS,"1 WAC each ansa every 2 hours, 2 extra exposures",,,,,, 2005-028T13:00:00,000T03:00:00,28-Jan-05,RADAR,SPASS Rider,Other,SOUTHWARM,Instrument warmup,"Distant Titan Latitude Study, Southern Latitudes",Warmup for calibration and science data collection.,,,,,, 2005-028T16:00:00,000T01:00:00,28-Jan-05,RADAR,Prime,Titan,SOUTH5CAL,Distant Titan radiometery and calibration,"Distant Titan Latitude Study, Southern Latitudes",Obtain distant Titan radiometer science and calibration data. One of a set that provides coverage of Titan southern latitude variation along with some obtainable associated longitude variation.,,,,,, 2005-028T17:00:00,000T06:30:00,28-Jan-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,Magnetospheric Boundary Campaign,"Part of MB,High MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-028T23:30:00,000T00:30:00,28-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 069 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [HE-EP-PA-PM-CP (611, 612, 614, 616, 617)]",,,,,, 2005-029T01:08:00,000T09:00:00,29-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-029T01:08:00,000T09:00:00,29-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-029T02:00:00,000T04:33:04,29-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-029T02:08:00,000T07:00:00,29-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-029T10:08:00,002T17:17:00,29-Jan-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-029T11:30:00,000T00:30:00,29-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 071 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-JA-PM-EN-DI (602, 604, 610, 616, 617)]",,,,,, 2005-029T12:00:00,000T02:00:00,29-Jan-05,UVIS,Prime,Star,ALPVIR,Alpha Virginis occultation,USTRCAL01,INSTANCE OF USTRCAL01. Stellar Calibration: alpha Virginis,,,,,, 2005-029T12:00:00,000T02:00:00,29-Jan-05,ISS,SPASS Rider,Star,ALPVIR,Alpha Virginis occultation,ISS Sensitivity monitor,Periodic standard star image to monitor ISS sensitivity,,,,,, 2005-029T14:00:00,000T02:00:00,29-Jan-05,RADAR,SPASS Rider,Other,ENGTEST,Engineering test,Engineering Test of Diagnostic Modes,Engineering test of diagnostic modes on the flight unit.,,,,,, 2005-029T16:00:00,000T00:30:00,29-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 072 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-DI-JA-PA-AT (604, 610, 611, 615, 617)]",,,,,, 2005-029T17:38:00,000T09:00:00,29-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-029T18:00:00,000T06:00:00,29-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-030T03:45:00,000T00:30:00,30-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 073 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-PA-DI-PM-EN (602, 604, 610, 616, 617)]",,,,,, 2005-030T04:15:00,000T06:00:00,30-Jan-05,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,"Turn to sun; Time: 30 min Solar Port: 7x1 and 5x1 Mosaics w/64x32 FOV ; 4? cubes per ptg. @ 40 & 320 ms IR, VIS always @ 50ms; Time: 4.5 hr; Solar Background Calibration: 4 cubes w/64x32 FOV; same int. Time: 30 min; Turn to waypoint: 30 min",,,,,, 2005-030T04:15:00,000T06:00:00,30-Jan-05,UVIS,SPASS Rider,Sun,SOLARPORT,Solar port observation,VIMS SOLAR PORT RIDER,VIMS RIDER,,,,,, 2005-030T10:15:00,000T01:30:00,30-Jan-05,VIMS,Prime,Star,ALPCMICAL,Alpha CMI calibration,Alpha CMi calibration,"Turn to star : 0-25 min Multiple cubes w/32x32 FOV IR @ 80/640 ms, VIS @ 20000 ms; Time: 40-90min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 0-25 min Not time critical. RWA REQUIRED.",,,,,, 2005-030T11:45:00,000T01:30:00,30-Jan-05,VIMS,Prime,Star,DELVIRCAL,Delta Vir calibration,Delta Vir calibration,"Turn to star : 0-25 min Multiple cubes w/32x32 FOV IR @ 80/640 ms, VIS @ 20000 ms; Time: 40-90min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 0-25 min Not time critical. RWA REQUIRED.",,,,,, 2005-030T13:15:00,000T01:30:00,30-Jan-05,VIMS,Prime,Star,RWLMICAL,RW LMi calibration,RW LMi calibration,"Turn to star : 0-25 min Multiple cubes w/32x32 FOV IR @ 80/640 ms, VIS @ 20000 ms; Time: 40-90min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 0-25 min Not time critical. RWA REQUIRED.",,,,,, 2005-030T14:45:00,000T01:30:00,30-Jan-05,VIMS,Prime,Star,ALPTRACAL,Alpha TrA calibration,Alpha TrA calibration,"Turn to star : 0-25 min Multiple cubes w/32x32 FOV IR @ 80/640 ms, VIS @ 20000 ms; Time: 40-90min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 0-25 min Not time critical. RWA REQUIRED.",,,,,, 2005-030T16:15:00,000T01:30:00,30-Jan-05,VIMS,Prime,Star,VXSGRCAL,Stellar calibration,VX Sgr calibration,"Turn to star : 0-25 min Multiple cubes w/32x32 FOV IR @ 80/640 ms, VIS @ 20000 ms; Time: 40-90min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 0-25 min Not time critical. RWA REQUIRED.",,,,,, 2005-030T17:45:00,000T01:30:00,30-Jan-05,VIMS,Prime,Star,RCASCAL,R Cas calibration,R Cas calibration,"Turn to star : 0-25 min Multiple cubes w/32x32 FOV IR @ 80/640 ms, VIS @ 20000 ms; Time: 40-90min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 0-25 min Not time critical. RWA REQUIRED.",,,,,, 2005-030T19:15:00,000T00:30:00,30-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 074 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-PM-AT-TL-EP (611, 613, 615, 616, 617)]",,,,,, 2005-030T20:53:00,000T04:00:00,30-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-031T00:00:00,000T06:00:00,31-Jan-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-031T00:53:00,000T10:00:00,31-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-031T10:53:00,000T12:59:00,31-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-031T10:53:00,000T12:59:00,31-Jan-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-031T12:00:00,000T00:30:00,31-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 077 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-EP-DI-CP-HE (604, 611, 612, 614, 615)]",,,,,, 2005-031T12:00:00,000T02:16:32,31-Jan-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-031T12:30:00,000T09:00:00,31-Jan-05,VIMS,Prime,Star,FOMALHAUT,Fomalhaut,Fomalhaut,"Turn to Fomalhaut; Time: 30 min

Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2005-031T12:30:00,000T09:00:00,31-Jan-05,ISS,SPASS Rider,Star,FOMALHAUT,Fomalhaut,ISS Sensitivity monitor,Periodic standard star image to monitor ISS sensitivity,,,,,, 2005-031T21:30:00,000T00:30:00,31-Jan-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 078 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EN-JA-AT-PM (602, 610, 615, 616, 617)]",,,,,, 2005-031T22:00:00,000T00:30:00,31-Jan-05,ISS,Prime,Other,OPNAVRET,Retargetable observation,S/2004 S5 Retargetable,NACs of S/2004 S5,,,,,, 2005-031T23:22:00,000T12:00:00,31-Jan-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-031T23:52:00,000T11:30:00,31-Jan-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-032T00:00:00,000T06:00:00,1-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-032T00:45:00,000T09:06:08,1-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-032T00:52:00,000T09:30:00,1-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-032T03:25:00,003T07:42:00,1-Feb-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-032T03:35:45,003T05:24:16,1-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-032T03:35:45,003T07:31:15,1-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-032T03:45:00,005T13:21:59,1-Feb-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,Dust survey,Dust survey,,,,,, 2005-032T03:49:00,003T07:18:00,1-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-032T11:22:00,000T12:00:00,1-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-032T11:22:00,000T12:00:00,1-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-032T12:22:00,000T02:35:00,1-Feb-05,VIMS,Prime,rings(general),APOMOSAIC,Apoapsis mosaic,APOAPSE_MOSAIC,"Orbits = 001-014, Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2-4, Time of observation (hours) = 1.0-2.0, Volume (Mbits) = 69-138 Mosaic of entire ring system near apoapse. Sunlit face.Various mosaic sizes (2x1 - 4x1)., Desc = 1x3",,,,,, 2005-032T12:22:00,000T02:35:00,1-Feb-05,ISS,SPASS Rider,rings(general),APOMOSAIC,Apoapsis mosaic,rider WACs; design by VIMS,1 WAC each ansa every 2 hours,,,,,, 2005-032T12:30:00,000T06:49:36,1-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-032T14:57:00,000T07:25:00,1-Feb-05,CIRS,Prime,Saturn,COMPSITA,Sit and stare at one location to derive composition,CIRS_003SA_COMPSITA14,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2005-032T23:22:00,000T12:00:00,1-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-033T00:00:00,000T06:00:00,2-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-033T11:22:00,000T12:00:00,2-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-033T11:22:00,000T12:00:00,2-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-033T12:22:00,000T10:00:00,2-Feb-05,CIRS,Prime,Saturn,COMPSITB,Sit and stare at one location to derive composition,CIRS_003SA_COMPSITB14,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2005-033T23:22:00,000T12:00:00,2-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-034T00:00:00,000T06:00:00,3-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-034T11:22:00,000T12:30:00,3-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-034T11:22:00,000T12:30:00,3-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-034T12:22:00,000T10:00:00,3-Feb-05,CIRS,Prime,Saturn,COMPSITC,Sit and stare at one location to derive composition,CIRS_003SA_COMPSITC14,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. Pointing: -Y to Saturn, Z to pole",,,,,, 2005-034T23:07:00,000T12:00:00,3-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-034T23:52:00,000T11:15:00,3-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-035T00:00:00,000T06:00:00,4-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-035T00:52:00,000T09:15:00,4-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-035T02:00:00,000T06:49:36,4-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-035T09:00:00,002T00:37:00,4-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-035T09:00:01,002T00:36:59,4-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-035T11:07:00,001T22:30:00,4-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-035T11:07:00,000T06:00:00,4-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-035T11:07:00,007T22:00:00,4-Feb-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-035T11:07:00,000T06:00:00,4-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-035T11:07:00,001T22:20:00,4-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-035T12:07:00,000T04:00:00,4-Feb-05,ISS,Prime,Saturn,3X3MOVIEA,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2005-035T12:30:00,000T04:33:04,4-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-035T17:07:00,000T09:00:00,4-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-035T17:07:00,000T09:00:00,4-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-035T18:00:00,000T04:33:04,4-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-035T18:07:00,000T07:00:00,4-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-035T18:37:00,000T06:00:00,4-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-036T02:07:00,000T22:30:00,5-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-036T02:07:00,000T22:30:00,5-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-036T03:00:00,000T04:33:04,5-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-036T03:07:00,000T20:00:00,5-Feb-05,ISS,Prime,Saturn,3X3MOVIEB,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2005-036T23:07:00,000T00:30:00,5-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 012 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-CP-DI-HE-JA (604, 610, 611, 612, 614)]",,,,,, 2005-037T00:37:00,000T09:00:00,6-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-037T00:37:00,000T09:00:00,6-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-037T01:37:00,000T07:00:00,6-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-037T02:00:00,000T02:16:32,6-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-037T02:07:00,000T06:00:00,6-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-037T09:37:00,001T14:45:00,6-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-037T09:37:00,000T07:30:00,6-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-037T09:37:00,001T14:45:00,6-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-037T09:37:00,000T07:30:00,6-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-037T09:37:00,001T14:45:00,6-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-037T09:37:01,001T14:44:59,6-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-037T10:30:00,000T04:33:04,6-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-037T10:37:00,000T05:30:00,6-Feb-05,ISS,Prime,Saturn,3X3MOVIEA,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2005-037T10:37:00,000T05:30:00,6-Feb-05,VIMS,SPASS Rider,Saturn,3X3MOVIEA,3 x 3 mosaic,Saturn ISS/VIMS Movie #1,"Saturn ISS/VIMS Movie #1of 3. 5.5 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 5.5 hours = 200 mbits.",,,,,, 2005-037T17:07:00,000T09:00:00,6-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-037T17:07:00,001T16:15:00,6-Feb-05,CDA,Non-SPASS,DustRAM direction,SURV00A,Dust survey,Dust survey,Dust survey,,,,,, 2005-037T17:07:00,000T09:00:00,6-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-037T18:07:00,000T07:00:00,6-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-037T19:00:00,000T06:49:36,6-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-038T02:07:00,000T22:15:00,7-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-038T02:07:00,000T22:15:00,7-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-038T03:00:00,000T04:33:04,7-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-038T03:07:00,000T19:45:00,7-Feb-05,ISS,Prime,Saturn,3X3MOVIEB,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2005-038T03:07:00,000T19:45:00,7-Feb-05,VIMS,SPASS Rider,Saturn,3X3MOVIEA,3 x 3 mosaic,Saturn ISS/VIMS Movie #2,"Saturn ISS/VIMS Movie #2of 3. 19.75 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 20 hours = 750 mbits. Modified 9/26/02 to 200 Mbits to fit SSR data volume.",,,,,, 2005-038T22:23:00,000T10:59:00,7-Feb-05,RSS,SPASS Rider,Titan,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operational Readiness Test (ORT). Pointing=XBAND to Earth. Last 9 hours required to be tracked at DSS-14, DSS-25, and DSS-26.",,,,,, 2005-038T22:52:00,000T00:30:00,7-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,S/2004 S5 Retargetable,NACs and BOTSIMS of S/2004 S5,,,,,, 2005-039T00:22:00,003T01:15:00,8-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-039T00:22:00,000T09:00:00,8-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-039T00:22:00,003T01:15:00,8-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-039T00:22:00,003T01:15:00,8-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-039T00:22:00,000T09:00:00,8-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-039T00:22:01,003T01:14:59,8-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-039T01:22:00,000T07:00:00,8-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-039T01:52:00,000T06:00:00,8-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-039T02:00:00,000T02:16:32,8-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-039T09:23:00,000T11:28:59,8-Feb-05,CDA,Non-SPASS,DustRAM direction,SURV00B,Dust survey,Dust survey,Dust survey,,,,,, 2005-039T10:22:00,000T05:30:00,8-Feb-05,ISS,Prime,Saturn,3X3MOVIEA,3 x 3 mosaic,NAC Southern Hemisphere Saturn movie,"3X3 mos in two filters, BOTSIMS, repeat every 1:45.",,,,,, 2005-039T10:22:00,000T05:30:00,8-Feb-05,VIMS,SPASS Rider,Saturn,3X3MOVIEA,3 x 3 mosaic,Saturn ISS/VIMS Movie #3,"Saturn ISS/VIMS Movie #2of 3. 5.5 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 6 hours = 220 mbits.",,,,,, 2005-039T12:52:00,000T08:00:00,8-Feb-05,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. Last 4 hours required to be tracked at DSS-25 in 1-way mode.,,,,,, 2005-039T16:52:00,000T10:30:00,8-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-039T18:22:00,000T06:00:00,8-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-039T20:52:00,000T20:00:00,8-Feb-05,CDA,Non-SPASS,Other,DECONTERM,Decontamination,Decontermination of CDA,"Decontermination of the chemical analyser target of CDA. 0.5h before heating go off sun, 10h heating and be off sun, 2 h after heating be off sun. Pointing: CDA Boresight not into Sun. Could be done with -z2E and CDA Boresight to ME (articulation of CDA = 0 degree). Rolling around -z2E is possible, a possible fix attitude for the 2ndary axis is +x2NEP. Possible OpMode: DFPW if no ME-Cover closing is necessay.",,,,,, 2005-040T16:53:00,001T09:53:59,9-Feb-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,Dust survey,Dust survey,,,,,, 2005-040T22:52:00,000T00:30:00,9-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 024 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EN-EP-AT-PM (602, 611, 615, 616, 617)]",,,,,, 2005-041T00:22:00,000T09:00:00,10-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-041T01:52:00,000T06:00:00,10-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-041T09:22:00,000T07:15:00,10-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-041T09:22:00,000T07:15:00,10-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-041T10:22:00,000T05:15:00,10-Feb-05,VIMS,Prime,Saturn,CH4FLR,,Saturn Methane Fluorescence,"Saturn methane fluorescence. 11 hours observing, once every three hours per hour. 1*2 mosiac, each taking 2 hours . Each mosaic uses 352*12*64*64*2/2*(1.05) = 18.2 mbits. For 12 hours = 73 mbits. Integration time: 1 second per pixel.",,,,,, 2005-041T11:00:00,000T02:16:32,10-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-041T14:38:00,000T10:59:00,10-Feb-05,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,RSS Operational Readiness Test (ORT). Pointing=XBAND to Earth. Last 9 hours required to be tracked at DSS-63 and DSS-55.,,,,,, 2005-041T16:37:00,000T09:00:00,10-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-041T16:37:00,000T09:00:00,10-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-041T17:37:00,000T07:00:00,10-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-041T18:00:00,000T02:16:32,10-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-041T18:07:00,000T06:00:00,10-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-042T01:37:00,001T15:00:00,11-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-042T01:37:00,000T22:30:00,11-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-042T01:37:00,000T22:30:00,11-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-042T01:37:00,000T22:30:00,11-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-042T01:37:00,001T15:00:00,11-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-042T01:37:01,001T14:59:59,11-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-042T02:37:00,000T10:00:00,11-Feb-05,VIMS,Prime,Saturn,GLOMOV,Saturn global movie,Saturn Global Movie #1,"Saturn Global Movie #1 of 4. 10 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 10 hours = 370 mbits. Modified 9/26/02: Volume decreased to 100 mbits to fit SSR",,,,,, 2005-042T02:47:00,003T06:20:00,11-Feb-05,CDA,Non-SPASS,DustRAM direction,SURV00A,Dust survey,Dust survey,Dust survey,,,,,, 2005-042T03:00:00,000T13:39:12,11-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-042T12:37:00,000T00:30:00,11-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 030 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-PM-EP-PA-JA (610, 611, 615, 616, 617)]",,,,,, 2005-042T13:07:00,000T10:00:00,11-Feb-05,VIMS,Prime,Saturn,GLOMOV,Saturn global movie,Saturn Global Movie #2,"Saturn Global Movie #2 of 4. 10 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 10 hours = 370 mbits. Modified 9/26/02: Volume decreased to 100 Mbits to fit SSR",,,,,, 2005-043T00:07:00,000T09:00:00,12-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-043T00:07:00,000T09:00:00,12-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-043T09:07:00,000T07:30:00,12-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-043T09:07:00,000T16:30:00,12-Feb-05,INMS,Non-SPASS,co-rotation,PTOTM013,MAPS survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-043T09:07:00,000T07:30:00,12-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-043T09:07:00,000T07:30:00,12-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-043T10:07:00,000T04:30:00,12-Feb-05,ISS,Prime,RingC,LPMRLFMOV,Ansa movie,C RING ANSA MOVIE TO DETECT SATS,C RING ANSA MOVIE for satellite detection.,,,,,, 2005-043T14:37:00,000T01:00:00,12-Feb-05,ISS,Prime,Titan,1X1PHOT30,Photopolarimetry,Titan NAC Photopol 30 Phase,Titan NAC Photopol 30 Phase,,,,,, 2005-043T16:37:00,001T16:30:00,12-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-043T16:37:00,000T09:00:00,12-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-043T16:37:00,001T16:30:00,12-Feb-05,MAG,Non-SPASS,Other,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS Magbound Campaign,Observe magnetospheric boundaries at a variety of radial distances.,,,,,, 2005-043T16:37:00,001T08:23:00,12-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-043T16:37:00,000T09:00:00,12-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-043T16:37:01,001T16:29:59,12-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-043T17:30:00,000T04:33:04,12-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-043T17:37:00,000T07:00:00,12-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-044T01:37:00,000T22:30:00,13-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-044T01:37:00,000T22:30:00,13-Feb-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-044T01:37:00,000T22:30:00,13-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-044T02:37:00,000T10:00:00,13-Feb-05,VIMS,Prime,Saturn,GLOMOV,Saturn global movie,Saturn Global Movie #3,"Saturn Global Movie #3 of 4. 10 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 10 hours = 370 mbits. Modified 9/26/02: Volume decreased to 320 Mbits to fit SSR",,,,,, 2005-044T03:00:00,000T09:06:08,13-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-044T12:37:00,000T00:30:00,13-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 036 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-PM-JA-EN-DI (602, 604, 610, 616, 617)]",,,,,, 2005-044T13:07:00,000T10:00:00,13-Feb-05,VIMS,Prime,Saturn,GLOMOV,Saturn global movie,Saturn Global Movie #4,"Saturn Global Movie #4 of 4. 10 Hours observing, once per hour. 2*2 mosiac, each taking 4*7 + 12 = 40 minutes. Each mosaic uses 352*12*64*64*4/2*(1.05) = 36.3 mbits. For 10 hours = 370 mbits. Modified 9/26/02: Data reduced to 320 Mbits toi accomodate SSR volume constraints.",,,,,, 2005-044T22:08:00,000T10:59:00,13-Feb-05,RSS,SPASS Rider,Titan,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operational Readiness Test (ORT). Pointing=XBAND to Earth. Last 9 hours required to be tracked at DSS-14, DSS-25, DSS-26; first 5 hours after thermal stabilization required to be tracked by DSS-55.",,,,,, 2005-045T00:07:00,000T09:00:00,14-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-045T00:07:00,000T09:00:00,14-Feb-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-045T00:07:00,000T09:00:00,14-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-045T01:00:00,000T09:07:00,14-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-045T01:07:00,000T07:00:00,14-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-045T02:00:00,000T02:16:32,14-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-045T09:07:00,000T05:27:56,14-Feb-05,CAPS,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-045T09:07:00,000T05:27:56,14-Feb-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-045T09:07:00,000T04:53:00,14-Feb-05,MAG,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances. (Alternate_MB_A),,,,,, 2005-045T09:07:00,000T05:27:56,14-Feb-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-045T09:07:01,000T16:50:52,14-Feb-05,MIMI,SPASS Rider,Titan,T3EXTINB,,MAPS TI/EE Campaign,"Part of TI/EE MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS. With -Y pointed toward Titan, when far from Titan (more than 30 minutes to either side of a targeted flyby), measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV). Also, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing.",,,,,, 2005-045T09:08:00,001T23:52:59,14-Feb-05,CDA,Non-SPASS,DustRAM direction,SURV00B,Dust survey,Dust survey,Dust survey,,,,,, 2005-045T09:57:53,000T09:00:00,14-Feb-05,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,CIRS_003TI_MIRTMAP19,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, x to pole (x-axis negotiable) 15 minute stare at start for UVIS rider.",,,,,, 2005-045T09:57:53,000T09:00:00,14-Feb-05,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2005-045T09:57:53,000T09:00:00,14-Feb-05,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-045T09:57:53,000T09:00:00,14-Feb-05,UVIS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,UVIS Rider to CIRS MIDIRTMAP,UVIS Rider to CIRS Mid IR Thermal Map,,,,,, 2005-045T09:57:53,000T14:00:00,14-Feb-05,VIMS,SPASS Rider,Titan,MAPMONITR,,VIMS_ride VIMS_4862,Titan Map and Monitor,,,,,, 2005-045T14:00:00,000T00:34:56,14-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-045T14:34:56,000T11:22:57,14-Feb-05,CAPS,SPASS Rider,Titan,T3EXTINB,,MAPS TI/EE Campaign,Part of TI/EE MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS,,,,,, 2005-045T14:34:56,000T04:54:50,14-Feb-05,INMS,Non-SPASS,Titan,TINTERACT,MAPS TI/EE Campaign,MAPS TI/EE Campaign,Part of TI/EE MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS,,,,,, 2005-045T14:34:56,000T12:22:57,14-Feb-05,MAG,Non-SPASS,Titan,TINTERACT,MAPS TI/EE Campaign,MAG MAPS TI_EE Campaign,Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS. (03TI (T3)),,,,,, 2005-045T14:34:56,000T14:22:57,14-Feb-05,RPWS,Non-SPASS,Titan,TINTERACT,MAPS TI/EE Campaign,MAPS TI/EE Campaign,Part of TI/EE MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS,,,,,, 2005-045T18:57:53,000T01:00:00,14-Feb-05,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,NMA (NAC Monitoring of Surface and Atmosphere),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2005-045T18:57:53,000T01:00:00,14-Feb-05,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_003TI_FIRNADIRCOMPINT_02,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5-2.0. POINTING: -y to Titan, x away from sun.",,,,,, 2005-045T18:57:53,000T01:00:00,14-Feb-05,UVIS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,UVIS Rider to ISS MONITORNA,Ride along with ISS MONITORNA,,,,,, 2005-045T19:29:46,000T10:28:07,14-Feb-05,INMS,Non-SPASS,Titan,T3INBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2005-045T19:57:53,000T04:00:00,14-Feb-05,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,CIRS_003TI_MIRLIMBINT_01,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: -y to Titan, z within 30 degrees of normal to limb.",,,,,, 2005-045T19:57:53,000T04:00:00,14-Feb-05,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2005-045T19:57:53,000T04:00:00,14-Feb-05,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-045T19:57:53,000T04:00:00,14-Feb-05,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2005-045T23:57:53,000T02:00:00,14-Feb-05,ISS,Prime,Titan,COMBINED,,"WMO/WPH/NGM (WAC Movie, WAC Photometry, Low Phase","1) wind/cloud motions, 3-12 km/px, 3 images/timestep in CB1 filter to increase SNR, 12-bit lossless particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.3)low-phase global map, 200-1000",,,,,, 2005-045T23:57:53,000T02:00:00,14-Feb-05,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_003TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2005-045T23:57:53,000T02:00:00,14-Feb-05,UVIS,SPASS Rider,Titan,COMBINED,,UVIS Rider to ISS COMBINED observation,Ride along with ISS COMBINED,,,,,, 2005-045T23:57:53,000T02:00:00,14-Feb-05,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Med_Res_Regional VIMS_4868,Titan Global Map,,,,,, 2005-046T01:57:53,000T03:00:00,15-Feb-05,CAPS,SPASS Rider,Titan,T3INBND,,MAPS 003TI Campaign,Part of 003TI MAPS Campaign. Inbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2005-046T01:57:53,000T03:00:00,15-Feb-05,MIMI,SPASS Rider,Titan,T3INBND,,MAPS 003TI Campaign,"Part of 003TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-046T02:12:53,000T04:07:00,15-Feb-05,RADAR,SPASS Rider,Titan,T3WARMUP,,Warmup for T3 flyby,,,,,,, 2005-046T02:57:53,000T08:00:00,15-Feb-05,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T3 Flyby,T3 is the first very close encounter (953 km) at Titan on the wake side of the satellite. It is therefore very significant because of potential measurements below the ionosphere in the tail-forming regions i.e. on the downstream side of the satellite. The physics of the plasma interaction has been particularly resistant to understanding in this area. At least as important as the latter goal is the very good possibility to discover an internal field of Titan. These is also some chance to be in the magnetosheath or even solar wind at the local Saturnian time LT = 10.38 of this encounter. Grade 1 priority. NOTE: - continuous data rate of 1976bps (32vps).,,,,,, 2005-046T04:57:53,000T01:08:00,15-Feb-05,CAPS,SPASS Rider,Titan,T3INBND,,MAPS 003TI Campaign,Part of 003TI MAPS Campaign. Inbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2005-046T04:57:53,000T01:08:00,15-Feb-05,MIMI,SPASS Rider,Titan,T3INBND,,MAPS 003TI Campaign,"Part of 003TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-046T04:57:53,000T01:00:00,15-Feb-05,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2005-046T05:27:53,000T00:31:00,15-Feb-05,ISS,Prime,Titan,HIGHRESNA,High resolution observartion,HRI (High Resolution Imaging),search for and monitor lightning/aurora,,,,,, 2005-046T05:48:53,000T00:10:00,15-Feb-05,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,High_res VIMS_4868,Titan High res map - ISS ridealong,,,,,, 2005-046T05:57:53,000T02:00:00,15-Feb-05,INMS,Non-SPASS,Titan,T3CLOSE,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2005-046T05:57:53,000T02:00:00,15-Feb-05,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2005-046T05:58:53,000T00:21:00,15-Feb-05,ISS,SPASS Rider,SpacecraftActivity,RADRCS,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-046T05:58:53,000T00:21:00,15-Feb-05,VIMS,SPASS Rider,Titan,TRANSRCS,,RWA_RCS_Trans VIMS_4868,Sneak in a couple of 40 msec images (64 square) during the RWA to RCS transition,,,,,, 2005-046T06:05:53,000T01:54:00,15-Feb-05,CAPS,SPASS Rider,Titan,T3CLOSE,,MAPS 003TI Campaign,Part of 003TI MAPS Campaign. Observations of Titan's interaction with Saturn's magnetosphere,,,,,, 2005-046T06:05:53,000T01:54:00,15-Feb-05,MIMI,SPASS Rider,Titan,T3CLOSE,,MAPS 003TI Campaign,"Part of 003TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-046T06:19:53,000T00:18:00,15-Feb-05,RADAR,Prime,Titan,T3INALT,,T3 Inbound Altimetry,Collect altimetry data while maintaining nadir pointing.,,,,,, 2005-046T06:37:53,000T00:13:00,15-Feb-05,RADAR,Prime,Titan,T3INLSAR,,T3 Inbound Low Resolution SAR,Low Resolution Synthetic Aperture RADAR (SAR) Imaging.,,,,,, 2005-046T06:50:53,000T00:14:00,15-Feb-05,RADAR,Prime,Titan,T3HISAR,,T3 High Resolution SAR,High Resolution Synthetic Aperture RADAR (SAR) Imaging.,,,,,, 2005-046T07:04:53,000T00:13:00,15-Feb-05,RADAR,Prime,Titan,T3OTLSAR,,T3 Outbound Low Res SAR,Low Resolution Synthetic Aperture RADAR (SAR) Imaging.,,,,,, 2005-046T07:17:53,000T00:12:00,15-Feb-05,RADAR,Prime,Titan,T3OUTALT,,Outbound Altimetry on T3,Altimetry taken during the outbound trajectory of T3,,,,,, 2005-046T07:29:53,000T00:38:00,15-Feb-05,RADAR,Prime,Titan,T3OUTSCAT,,Outbound Scatterometry of T3,Outbound Scatterometry during Ta flyby,,,,,, 2005-046T07:57:53,000T11:00:00,15-Feb-05,INMS,Non-SPASS,Titan,T3OUTBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine,,,,,, 2005-046T07:57:53,000T01:00:00,15-Feb-05,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2005-046T07:59:53,000T00:58:00,15-Feb-05,CAPS,SPASS Rider,Titan,T3OUTBND,,MAPS 003TI Campaign,Part of 003TI MAPS Campaign. Outbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2005-046T07:59:53,000T01:29:10,15-Feb-05,MIMI,SPASS Rider,Titan,T3OUTBND,,MAPS 003TI Campaign,"Part of 003TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-046T08:30:53,000T03:27:00,15-Feb-05,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2005-046T08:30:53,000T03:27:00,15-Feb-05,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_003TI_FIRNADIRMAP_02,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2005-046T08:30:53,000T03:27:00,15-Feb-05,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-046T08:30:53,000T14:47:00,15-Feb-05,VIMS,SPASS Rider,Titan,NIGHT,,VIMS_ride VIMS_4870,Titan Night,,,,,, 2005-046T08:57:53,001T00:05:39,15-Feb-05,CAPS,SPASS Rider,Titan,T3EXTOUT,,MAPS 003TI Campaign,Part of 003TI MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS,,,,,, 2005-046T08:57:53,001T00:05:39,15-Feb-05,RPWS,Non-SPASS,Titan,TINTERACT,MAPS TI/EE Campaign,MAPS TI/EE Campaign,Part of TI/EE MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS,,,,,, 2005-046T09:30:01,000T23:29:58,15-Feb-05,MIMI,SPASS Rider,Titan,T3EXTOUT,,MAPS 003TI Campaign,"Part of 003TI MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS. With -Y pointed toward Titan, when far from Titan (more than 30 minutes to either side of a targeted flyby), measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV). Also, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing.",,,,,, 2005-046T10:57:53,000T22:02:07,15-Feb-05,MAG,Non-SPASS,Titan,TINTERACT,MAPS TI/EE Campaign,MAG MAPS TI_EE Campaign,Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS. (03TI (T3)),,,,,, 2005-046T11:57:53,000T01:30:00,15-Feb-05,ISS,Prime,Titan,NIGHTWAC,ISS lightning / aurora observation,WNI (WAC Nightside Imaging),search for and monitor lightning/aurora,,,,,, 2005-046T11:57:53,000T03:00:00,15-Feb-05,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_003TI_FIRNADIRMAP_03,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2005-046T11:57:53,000T03:00:00,15-Feb-05,UVIS,SPASS Rider,Titan,NIGHTWAC,ISS lightning / aurora observation,UVIS Rider to ISS NIGHTWAC and more,Ride along with ISS NIGHTWAC and other observations,,,,,, 2005-046T13:27:53,000T01:30:00,15-Feb-05,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2005-046T14:57:53,000T04:00:00,15-Feb-05,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_003TI_FIRNADIRCOMPINT_01,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5-2.0. POINTING: -y to Titan, x away from sun.",,,,,, 2005-046T14:57:53,000T04:00:00,15-Feb-05,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2005-046T14:57:53,000T01:00:00,15-Feb-05,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,NNI (NAC Nightside Imaging),search for and monitor lightning/aurora,,,,,, 2005-046T14:57:53,000T04:00:00,15-Feb-05,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,UVIS Rider to CIRS Far Nadir Comp,UVIS Rider to CIRS Far-IR Nadir Comp,,,,,, 2005-046T18:57:53,000T04:20:00,15-Feb-05,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,CIRS_003TI_MIRTMAP20,"obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. POINTING: -y to Titan, x to pole (x-axis negotiable)",,,,,, 2005-046T18:57:53,000T04:20:00,15-Feb-05,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2005-046T18:57:53,000T04:20:00,15-Feb-05,UVIS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,UVIS Rider to CIRS MIDIRTMAP,UVIS Rider to CIRS Mid IR Thermal Map,,,,,, 2005-046T18:57:53,000T05:01:07,15-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-046T23:59:00,000T09:00:00,15-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-046T23:59:00,000T09:00:00,15-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-046T23:59:00,000T09:00:00,15-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-047T00:00:00,000T06:00:00,16-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-047T00:59:00,000T07:00:00,16-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-047T01:30:00,000T04:33:04,16-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-047T08:59:00,000T01:31:00,16-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-047T09:00:00,000T13:20:00,16-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-047T09:00:00,000T05:34:00,16-Feb-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-047T09:00:00,000T01:20:00,16-Feb-05,RPWS,Non-SPASS,Titan,TINTERACT,MAPS TI/EE Campaign,MAPS TI/EE Campaign,Part of TI/EE MAPS Campaign. Investigate large-scale and distant aspects of the Titan interaction by observing during entire period around an encounter from 10 to 25 RS,,,,,, 2005-047T09:01:00,000T10:29:29,16-Feb-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,Dust survey,Dust survey,,,,,, 2005-047T09:03:32,000T17:56:57,16-Feb-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-047T09:10:00,000T08:36:00,16-Feb-05,CAPS,SPASS Rider,InstrumentCalibration,CALIBRATE,Calibration,CAPS Calibration,"CAPS periodic gain test and calibration. The specified rate and data volume are the delta above the CAPS survey rate (1000 bps), and the rate is the average over the entire request (current plans are to conduct the test in two different rates.)",,,,,, 2005-047T09:20:00,000T04:35:00,16-Feb-05,CIRS,Prime,RingF,FMOVIEA,F ring movie,CIRS_003RF_FMOVIEA001,F Ring rotation movie during early phase of mission. Do 1 of 3 in revs 3-5. Alternate between rings ansas with ~50-minute period.,,,,,, 2005-047T09:20:00,000T04:35:00,16-Feb-05,VIMS,SPASS Rider,RingF,FMOVIEA,F ring movie,F Ring Movie A,"32x32 cubes centered on CIRS FP1. IR + VIS. Four cubes on each visit to an F Ring ansa, one pair (80 and 320 msec) before the dark sky turn and another pair after.",,,,,, 2005-047T10:20:00,001T18:50:00,16-Feb-05,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-047T10:30:00,000T03:18:00,16-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-047T13:48:00,000T11:05:17,16-Feb-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-047T13:55:00,000T00:40:00,16-Feb-05,ISS,Prime,Enceladus,GEOLOG,Geologic study,ENCELADUS Geology,"Geology study, N03+NP03 at 180 longitude",,,,,, 2005-047T13:55:00,000T00:40:00,16-Feb-05,CIRS,SPASS Rider,Enceladus,GEOLOG,Geologic study,Enceladus rider (FP3 integration),"FP3 observation of Enceladus to search for current thermal activity. Sub-S/C=(-1, 178), phase=27, AD=2.2 mrad. CIRS at 15.5 cm-1 res (4.75 sec/frame), blink, shutter closed for central 5 minutes.",,,,,, 2005-047T13:55:00,000T00:40:00,16-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-047T13:55:00,000T00:40:00,16-Feb-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus rider with iss,"36i2-36v3 160 ms, 640 ms 9 min per pair 12.8 mbits per pair 3 sets, total equals 38.4 mbits",,,,,, 2005-047T14:34:00,000T22:16:00,16-Feb-05,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2005-047T14:35:00,000T01:14:00,16-Feb-05,CIRS,Prime,RingF,FMOVIEA,F ring movie,CIRS_003RF_FMOVIEA002,F Ring rotation movie during early phase of mission. Do 1 of 3 in revs 3-5. Alternate between rings ansas with ~50-minute period.,,,,,, 2005-047T14:35:00,000T01:14:00,16-Feb-05,VIMS,SPASS Rider,RingF,FMOVIEA,F ring movie,F Ring Movie A,"32x32 cubes centered on CIRS FP1. IR + VIS. 2 cubes on each visit to an F Ring ansa, one (160 msec) before the dark sky turn and another one after.",,,,,, 2005-047T15:20:29,000T02:00:00,16-Feb-05,RSS,SPASS Rider,Enceladus,THERMAL,Thermal stabilization period,RSS Enceladus Gravity Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2005-047T15:49:00,000T00:40:00,16-Feb-05,ISS,Prime,Enceladus,GEOLOG,Geologic study,ENCELADUS Geology,"Geology study, N03+NP03 range 185944 at 217 longitude",,,,,, 2005-047T15:49:00,000T01:10:00,16-Feb-05,CIRS,SPASS Rider,Enceladus,GEOLOG,Geologic study,Enceladus rider (FP3 integration),"FP3 observation of Enceladus to search for current thermal activity. Sub-S/C=(-1, 229), phase=22, AD=3 mrad. CIRS at 15.5 cm-1 res (4.75 sec/frame), blink, shutter closed for first and last 5 minutes.",,,,,, 2005-047T15:49:00,000T00:40:00,16-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-047T15:49:00,000T00:40:00,16-Feb-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus rider with iss,"36i2-36v3 160 ms, 640 ms 9 min per pair 12.8 mbits per pair 3 sets, total equal 38.4 mbits",,,,,, 2005-047T16:29:00,000T00:30:00,16-Feb-05,ISS,Prime,Enceladus,GEOLOG,Geologic study,ENCELADUS Geology,"Geology study, N03+NP03",,,,,, 2005-047T16:29:00,000T00:30:00,16-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-047T16:29:00,000T00:30:00,16-Feb-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus rider with iss,"36i2-36v3 160 ms, 640 ms 9 min per pair 12.8 mbits per pair 2 sets, total equal 25.6 mbits",,,,,, 2005-047T17:40:29,000T04:40:00,16-Feb-05,CDA,Non-SPASS,RingE,ERING,E ring observation,E ring dust measurement,"study E ring dust distribution, poiting: Ride along with RSS, rate =4192 bps, volume= 31.4 Mbits, secondary: -x close to 204/2.5",,,,,, 2005-047T17:43:39,000T04:06:50,16-Feb-05,RSS,SPASS Note,Enceladus,GRAVITYN,RSS gravity field determination,RSS Enceladus Gravity Field Determination,Enceladus mass determination,,,,,, 2005-047T17:54:02,000T14:00:00,16-Feb-05,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. Need to do this inside 6 RS on at least half of the periapses inside of 6RS. No pointing requirement",,,,,, 2005-047T22:20:00,000T05:10:00,16-Feb-05,MAG,SPASS Rider,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,"This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space. NOTE: period 4 INTFLD request is backup to this request. For whichever of these 2 requests (3/4) MAG is not made prime instrument, we still wish to take high rate continuous data.",,,,,, 2005-047T22:20:29,000T01:16:00,16-Feb-05,CDA,Non-SPASS,RingE,ERING,E ring observation,Dust survey within dust hazard zone,"Dust survey within dust hazard zone, CDA defines secondary axis, rate: 150 bps, volume: 1. Mb",,,,,, 2005-047T22:41:00,000T02:00:00,16-Feb-05,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2005-047T23:36:29,000T03:34:00,16-Feb-05,CDA,Non-SPASS,RingE,ERING,E ring observation,Dust survey,"Dust survey ,rate: 524 bps, volume: 5.8 Mb",,,,,, 2005-048T00:00:29,000T01:30:00,17-Feb-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,"64i2-64v1 160ms, 640ms (28 min/cycle) 21 Mbits/set, 3 sets total=63 mbits",,,,,, 2005-048T00:15:29,000T01:15:00,17-Feb-05,CIRS,Prime,Enceladus,FP1FP3MAP,CIRS FP1 integration / FP3 map,"Enceladus FP1 and FP3 maps, high spectral resoluti","NOTE: SHORTENED BY 15 MIN., SO DESIGN MUST BE RECONSIDERED!!!! FP1, FP3 observation of Enceladus to search for current thermal activity and to obtain high spectral resolution data. (0, 296), Sub-S/C,(1, 310), phase=23, 5.8,AD,10.6 mrad....A) Two 7 mrad FPB scans in X (over and back), the second displaced in Z by 3 mrad from the first, with pattern centered on disk (15 min); then 5 min with shutter closed; CIRS at 15.5 cm-1 res (4.75 sec/frame), blink...B) FP1 to disk center, spectral res 0.5 cm-1 (52 sec/frame) for 30 min...C) Similar to (A), but 3 X-scans (over, back, and over) to cover 9 mrad disk; shutter closed last 5 min.(28 min)..D) 7-scan Nyquist FP1 disk mosaic; 15.5 cm-1 resolution (4.75 sec/frame) (9 min). Return NAC to disk center for handoff to VIMS.",,,,,, 2005-048T00:15:29,000T01:15:00,17-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-048T00:53:17,000T11:06:43,17-Feb-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-048T00:55:00,000T00:15:00,17-Feb-05,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2005-048T01:14:00,000T00:05:00,17-Feb-05,RPWS,Non-SPASS,Saturn,HRSED,Highest resolution saturn kilometric radiation observation,Highest Resolution SED Observations,"Obtain the highest resolution observations of Saturn Electrostatic Discharges (SED) by using the RPWS HF-WBR mode at ~180 kbps within 6 RS for a total of 60 minutes within the first 12 periapses inside of 6 RS. Results will help to verify the source as lightning, or provide evidence that they could be of some other origin (e.g. rings). No attitude requirement.",,,,,, 2005-048T01:30:29,000T00:45:00,17-Feb-05,VIMS,Prime,Enceladus,ENCELADUS,Enceladus,Enceladus,"64x64i2-v3 160ms, 320ms, 80ms (28 min/cycle) 21 Mbits/frame compressed, 3 frames total=63 mbits 40 minute to complete. If not enough time, drop the 80 ms frame. point and stare at enceladus",,,,,, 2005-048T01:30:29,000T00:45:00,17-Feb-05,CIRS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,"Enceladus rider (FP1,FP3 high spectral resolution integration)","FP1, FP3 observation of Enceladus to search for current thermal activity and obtain high spectral resolution data. Sub-S/C=(1, 314), phase=25, 11AD>150 mrad; 130>phase>114.,,,,,, 2005-048T14:46:00,000T08:22:00,17-Feb-05,UVIS,SPASS Rider,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Rider opportunity,,,,,, 2005-048T15:00:00,000T06:00:00,17-Feb-05,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 8 kbps data (which gives uncollapsed ELS data). Data is in addition to 1000 bps from survey.,,,,,, 2005-048T23:43:00,000T09:00:00,17-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-049T05:10:00,000T03:33:00,18-Feb-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-049T08:43:00,000T00:30:00,18-Feb-05,ISS,Prime,Dione,320W119PH,Spectrophotometery,Dione spectrophotometry/ phase coverage,Turn -Y to Dione; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-049T08:43:00,007T23:23:00,18-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-049T08:43:00,000T00:30:00,18-Feb-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T08:43:00,007T23:23:00,18-Feb-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-049T08:43:00,000T23:53:00,18-Feb-05,INMS,Non-SPASS,Saturn,PTOTM014,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-049T08:43:00,000T23:53:00,18-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-049T08:43:00,002T00:17:00,18-Feb-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-049T10:20:00,000T00:30:00,18-Feb-05,ISS,Prime,Mimas,094W095PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-049T10:20:00,000T00:30:00,18-Feb-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T11:00:00,000T01:00:00,18-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 049 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 9 targets: [JA-AT-PM-HE-TE-EP-MI-RH-CP (601, 603, 605, 610, 611, 612, 614, 615, 616)]",,,,,, 2005-049T12:22:00,000T00:30:00,18-Feb-05,ISS,Prime,Tethys,022W098PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-049T12:22:00,000T00:30:00,18-Feb-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T14:10:00,000T00:25:00,18-Feb-05,ISS,Prime,Enceladus,094W091PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Turn -Y to Enceladus; do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-049T14:10:00,000T00:25:00,18-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T14:35:00,000T00:25:00,18-Feb-05,ISS,Prime,Mimas,166W100PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-049T14:35:00,000T00:25:00,18-Feb-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T15:00:00,000T01:00:00,18-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 050 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 7 targets: [EP-PM-CP-AT-JA-PA-DI (604, 610, 611, 614, 615, 616, 617)]",,,,,, 2005-049T16:30:00,000T00:25:00,18-Feb-05,ISS,Prime,Saturn,WINDS,Saturn wind observation,Saturn winds/cloud height 1x3 feature track,"Six 1x3 mosaics. 1,2,3 are near terminator. 4,5,6 view the same lats/lons as 1,2,3 but 75 minutes later. NAC in MT1/CB1, MT2/CB2, and BL1. One set of WAC in MT2, CB2, and BL1.",,,,,, 2005-049T16:55:00,000T00:25:00,18-Feb-05,ISS,Prime,Saturn,WINDS,Saturn wind observation,Saturn winds/cloud height 1x3 feature track,"Six 1x3 mosaics. 1,2,3 are near terminator. 4,5,6 view the same lats/lons as 1,2,3 but 75 minutes later. NAC in MT1/CB1, MT2/CB2, and BL1. One set of WAC in MT2, CB2, and BL1.",,,,,, 2005-049T17:20:00,000T00:25:00,18-Feb-05,ISS,Prime,Saturn,WINDS,Saturn wind observation,Saturn winds/cloud height 1x3 feature track,"Six 1x3 mosaics. 1,2,3 are near terminator. 4,5,6 view the same lats/lons as 1,2,3 but 75 minutes later. NAC in MT1/CB1, MT2/CB2, and BL1. One set of WAC in MT2, CB2, and BL1.",,,,,, 2005-049T17:45:00,000T00:25:00,18-Feb-05,ISS,Prime,Saturn,WINDS,Saturn wind observation,Saturn winds/cloud height 1x3 feature track,"Six 1x3 mosaics. 1,2,3 are near terminator. 4,5,6 view the same lats/lons as 1,2,3 but 75 minutes later. NAC in MT1/CB1, MT2/CB2, and BL1. One set of WAC in MT2, CB2, and BL1.",,,,,, 2005-049T18:10:00,000T00:25:00,18-Feb-05,ISS,Prime,Saturn,WINDS,Saturn wind observation,Saturn winds/cloud height 1x3 feature track,"Six 1x3 mosaics. 1,2,3 are near terminator. 4,5,6 view the same lats/lons as 1,2,3 but 75 minutes later. NAC in MT1/CB1, MT2/CB2, and BL1. One set of WAC in MT2, CB2, and BL1.",,,,,, 2005-049T18:35:00,000T00:12:00,18-Feb-05,ISS,Prime,Saturn,WINDS,Saturn wind observation,Saturn winds/cloud height 1x3 feature track,"Six 1x3 mosaics. 1,2,3 are near terminator. 4,5,6 view the same lats/lons as 1,2,3 but 75 minutes later. This picket only NAC in MT2/CB2, and BL1.",,,,,, 2005-049T18:47:00,000T00:28:00,18-Feb-05,ISS,Prime,Mimas,238W107PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-049T18:47:00,000T00:28:00,18-Feb-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T19:15:00,000T01:00:00,18-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 041 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 7 targets: [JA-EP-PM-AT-EN-CP-MI (601, 602, 610, 611, 614, 615, 616)]",,,,,, 2005-049T20:15:00,000T00:30:00,18-Feb-05,ISS,Prime,Enceladus,166W096PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Turn -Y to Enceladus; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-049T20:15:00,000T00:30:00,18-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T22:20:00,000T00:30:00,18-Feb-05,ISS,Prime,Rhea,238W116PH,Spectrophotometery,Rhea spectrophotometry/ phase coverage,Turn -Y to Rhea; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-049T22:20:00,000T00:30:00,18-Feb-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T22:50:00,000T00:23:00,18-Feb-05,ISS,Prime,Tethys,094W085PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-049T22:50:00,000T00:23:00,18-Feb-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T23:13:00,000T00:23:00,18-Feb-05,ISS,Prime,Mimas,310W104PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2005-049T23:13:00,000T00:23:00,18-Feb-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-049T23:36:00,000T09:00:00,18-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-050T08:36:00,000T15:08:00,19-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-050T08:36:00,000T11:24:00,19-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-050T08:36:00,000T15:08:00,19-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-050T08:36:00,000T15:08:00,19-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-050T09:01:00,000T00:10:00,19-Feb-05,ISS,Prime,Enceladus,310W101PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-050T09:01:00,000T00:10:00,19-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-050T09:32:00,000T00:30:00,19-Feb-05,ISS,Prime,Mimas,094W087PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-050T10:00:00,000T02:16:32,19-Feb-05,CAPS,Non-SPASS,Other,BURSK16K,16 kbps burst,Magnetospheric Survey,extra bits,,,,,, 2005-050T11:40:00,000T01:00:00,19-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 040 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 8 targets: [CP-HE-MI-EP-TE-EN-JA-PA (601, 602, 603, 610, 611, 612, 614, 617)]",,,,,, 2005-050T13:40:00,000T00:30:00,19-Feb-05,ISS,Prime,Mimas,166W090PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn -Y to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-050T13:40:00,000T00:30:00,19-Feb-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-050T14:10:00,000T01:10:00,19-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 042 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 9 targets: [PM-AT-PA-HE-CP-EP-TI-TE-JA (603, 606, 610, 611, 612, 614, 615, 616, 617)]",,,,,, 2005-050T15:20:00,000T00:30:00,19-Feb-05,ISS,Prime,Tethys,238W100PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-050T15:20:00,000T00:30:00,19-Feb-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-050T16:50:00,000T00:25:00,19-Feb-05,ISS,Prime,Enceladus,022W088PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Turn -Y to Enceladus; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-050T16:50:00,000T00:25:00,19-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-050T17:15:00,000T00:25:00,19-Feb-05,ISS,Prime,Dione,094W078PH,Spectrophotometery,Dione spectrophotometry/ phase coverage,Turn -Y to Dione; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-050T17:15:00,000T00:25:00,19-Feb-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-050T17:40:00,000T05:30:00,19-Feb-05,VIMS,Prime,RingG,G80PHASE,G ring observation,G Ring near phase 80,12x12; 1 sec exp; do any 1 of 9 at Priority 1; also any 1 of 9 at Priority 2,,,,,, 2005-050T17:40:00,000T05:30:00,19-Feb-05,ISS,SPASS Rider,RingG,G80PHASE,G ring observation,RIDE ALONG G RING OBSERVATIONS,RIDE ALONG G RING OBSERVATIONS,,,,,, 2005-050T20:00:00,007T04:36:00,19-Feb-05,INMS,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-050T23:44:00,000T08:52:00,19-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-050T23:44:00,000T08:52:00,19-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-051T02:36:00,000T03:00:00,20-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-051T08:36:00,000T14:45:00,20-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-051T08:36:00,000T01:00:00,20-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-051T09:00:00,005T23:06:00,20-Feb-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-051T09:36:00,000T02:04:00,20-Feb-05,VIMS,Prime,RingE,E80PHASE,E ring observation,E Ring near phase 80,"Orbits = 003-004, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 180, Time of observation (hours) = 20, Volume (Mbits) = 289, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturn's pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 9 at Priority 1; also any 1 of 9 at Priority 2; can be split",,,,,, 2005-051T09:36:00,000T02:04:00,20-Feb-05,CIRS,SPASS Rider,RingE,E80PHASE,E ring observation,VIMS E80 Phase,null,,,,,, 2005-051T09:36:00,000T03:20:00,20-Feb-05,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required.",,,,,, 2005-051T11:40:00,000T00:40:00,20-Feb-05,ISS,Prime,Tethys,022W083PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-051T11:40:00,000T00:40:00,20-Feb-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-051T12:20:00,000T01:00:00,20-Feb-05,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"MUTUAL EVENTS, TRANSIT OF Dione ACROSS Rhea","Transit of Dione across Rhea. 32 NACs, 180 ms exposure. One exposure every 34 seconds after imaging starts.",,,,,, 2005-051T12:56:00,000T10:25:00,20-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-051T13:20:00,000T01:45:00,20-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 045 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [EP-JA-PM-PA-AT-DI-EN-RH-CP-TE (602, 603, 604, 605, 610, 611, 614, 615, 616, 617)]",,,,,, 2005-051T15:05:00,000T01:00:00,20-Feb-05,ISS,Prime,Mimas,MUTUALEVE,Mutual event satellite transit observation,"MUTUAL EVENTS, TRANSIT OF Mimas ACROSS Pandora","37 NACs, 180 ms exposure. One image every 34 s after imaging starts. New ephemerides indicate that event will not occur.",,,,,, 2005-051T16:05:00,000T00:30:00,20-Feb-05,ISS,Prime,Dione,238W094PH,Spectrophotometery,Dione spectrophotometry/ phase coverage,Turn -Y to Dione; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-051T16:05:00,000T00:30:00,20-Feb-05,CIRS,SPASS Rider,Dione,238W094PH,Spectrophotometery,Dione rider,"Dione rider; request FP3(6) to target; 0.5 cm-1 resolution integration; AD=0.7 mrad at phase 94 degrees......... Time Range(km) Alt(km) SSCLat SSCLon. SSLat SSLon Vrad Vtan Phase AD(rad) SCET 234.625 1569153.777 1568593.777 0.250 229.248 -22.540 135.443 10.463 3.964 93.610 0.00071 2005 FEB 20, 15:00:00.00 234.667 1607881.684 1607321.684 0.242 235.190 -22.540 140.923 11.037 3.127 94.034 0.00070 2005 FEB 20, 16:00:00.00 234.708 1648511.691 1647951.691 0.235 241.012 -22.540 146.404 11.519 2.254 94.346 0.00068 2005 FEB 20, 17:00:00.00",,,,,, 2005-051T16:05:00,000T00:30:00,20-Feb-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-051T18:20:00,000T00:35:00,20-Feb-05,ISS,Prime,Enceladus,310W090PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Turn -Y to Enceladus; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-051T18:20:00,000T00:35:00,20-Feb-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,Ride along with other ORS instrument icy satellite observations,,,,,, 2005-051T18:55:00,000T03:26:00,20-Feb-05,VIMS,Prime,RingE,E80PHASE,E ring observation,E Ring near phase 80,"Orbits = 003-004, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 180, Time of observation (hours) = 20, Volume (Mbits) = 289, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturns pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 9 at Priority 1; also any 1 of 9 at Priority 2; can be split",,,,,, 2005-051T18:55:00,000T03:26:00,20-Feb-05,CIRS,SPASS Rider,RingE,E80PHASE,E ring observation,VIMS E80 Phase,null,,,,,, 2005-051T23:21:00,000T09:00:00,20-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-051T23:21:00,000T09:00:00,20-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-052T02:00:00,000T03:00:00,21-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-052T08:21:00,000T06:00:00,21-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-052T08:21:00,002T00:00:00,21-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-052T09:21:00,000T00:30:00,21-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,S/2004 S5,NACS and BOTSIMS of S/2004 S5 Retargettable,,,,,, 2005-052T09:51:00,000T03:30:00,21-Feb-05,VIMS,Prime,RingE,E80PHASE,E ring observation,E Ring near phase 80,"Orbits = 003-004, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 180, Time of observation (hours) = 20, Volume (Mbits) = 289, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturns pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 9 at Priority 1; also any 1 of 9 at Priority 2; can be split",,,,,, 2005-052T09:51:00,000T03:30:00,21-Feb-05,CIRS,SPASS Rider,RingE,E80PHASE,E ring observation,VIMS E80 Phase,RE phase rider,,,,,, 2005-052T14:21:00,000T12:00:00,21-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-052T14:21:00,000T12:00:00,21-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-052T17:21:00,000T06:00:00,21-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-053T02:21:00,000T21:00:00,22-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-053T02:21:00,000T21:00:00,22-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-053T03:21:00,000T19:30:00,22-Feb-05,CIRS,Prime,Saturn,MIRMAPA,Mid infrared map,CIRS_003SA_MIRMAPA01,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-053T23:21:00,000T09:00:00,22-Feb-05,CDA,Non-SPASS,DustRAM direction,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-053T23:21:00,000T09:00:00,22-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-054T08:21:00,002T23:45:00,23-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-054T10:21:00,000T01:15:00,23-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 053 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [EN-DI-TL-HE-CP-PM-AT-JA-EP-PA (602, 604, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2005-054T11:36:00,000T11:00:00,23-Feb-05,CIRS,Prime,Saturn,MIRMAPA,Mid infrared map,CIRS_003SA_MIRMAPA03,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-054T23:06:00,000T09:00:00,23-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-055T02:00:00,000T03:00:00,24-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-055T08:36:00,000T11:00:00,24-Feb-05,CIRS,Prime,Saturn,MIRMAPB,Mid infrared map,CIRS_003SA_MIRMAPB03,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-055T19:36:00,000T01:00:00,24-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 056 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 8 targets: [DI-CP-PM-EN-AT-HE-TE-EP (602, 603, 604, 611, 612, 614, 615, 616)]",,,,,, 2005-055T23:06:00,000T09:00:00,24-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-056T02:00:00,000T03:00:00,25-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-056T09:06:00,000T00:40:00,25-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-056T09:06:01,000T00:40:00,25-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-056T10:00:00,000T00:30:00,25-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,S/2004 S5 Retargettable,NACs and BOTSIMS of S/2004 S5 Retargettable,,,,,, 2005-056T11:14:00,000T00:40:00,25-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-056T11:14:01,000T00:40:00,25-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-056T11:54:00,000T01:28:00,25-Feb-05,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_03_SCATTERED_SUNLIGHT_TEST_PRIME,"To monitor the effect of ring particle impacts on the CIRS primary mirror performance requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; a continuous radial scan is required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scan will begin at waypoint (NAC to Saturn, +X to NSP), and will scan in Z to 12 degrees of Sun at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction to TBD degrees. From here, to 12 degrees of Sun back, repeated twice, Then back to waypoint. Waypoint is 111 degrees from sun.",,,,,, 2005-056T13:22:00,000T00:40:00,25-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-056T13:22:01,000T00:40:00,25-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-056T15:30:00,000T00:40:00,25-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-056T15:30:01,000T00:40:00,25-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-056T16:30:00,000T00:30:00,25-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 060 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-JA-PA-TL-DI (604, 610, 613, 614, 617)]",,,,,, 2005-056T17:38:00,000T00:40:00,25-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-056T17:38:01,000T00:40:00,25-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-056T19:46:00,000T00:40:00,25-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-056T19:46:01,000T00:40:00,25-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-056T21:00:00,000T00:30:00,25-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 061 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [MI-PA-PM-RH-HY (601, 605, 607, 616, 617)]",,,,,, 2005-056T23:06:00,000T09:00:00,25-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-057T00:36:00,000T06:00:00,26-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-057T08:06:00,000T16:30:00,26-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-057T08:06:00,000T16:30:00,26-Feb-05,CAPS,Non-SPASS,Saturn,2XSURVEY,MAPS survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-057T08:06:00,000T16:30:00,26-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2005-057T08:06:00,000T16:30:00,26-Feb-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-057T09:06:00,000T00:40:00,26-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-057T09:06:01,000T00:40:00,26-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-057T09:46:00,000T00:30:00,26-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 063 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-DI-HE-JA-EN (602, 604, 610, 612, 616)]",,,,,, 2005-057T11:14:00,000T00:40:00,26-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-057T11:14:01,000T00:40:00,26-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-057T13:22:00,000T00:40:00,26-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-057T13:22:01,000T00:40:00,26-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-057T14:06:00,000T00:30:00,26-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 064 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [AT-EP-CP-PA-TL (611, 613, 614, 615, 617)]",,,,,, 2005-057T15:36:00,000T09:00:00,26-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-057T17:06:00,000T06:00:00,26-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-058T00:36:00,000T06:17:11,27-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-058T00:36:00,000T06:12:00,27-Feb-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-058T00:36:00,000T01:22:00,27-Feb-05,INMS,Non-SPASS,Saturn,STARTUP,Sequence startup activity,STARTUP,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2005-058T00:36:00,000T22:14:00,27-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-058T00:36:00,000T06:17:11,27-Feb-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-058T00:41:55,000T05:37:34,27-Feb-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,Dust survey,Dust survey,,,,,, 2005-058T01:58:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEC,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T01:58:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEC,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T01:58:00,000T04:22:24,27-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-058T02:38:00,000T00:30:00,27-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 065 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [TL-AT-PA-PM-MI (601, 613, 615, 616, 617)]",,,,,, 2005-058T04:06:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEC,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T04:06:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEC,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T06:14:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEC,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T06:14:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEC,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T06:20:24,003T01:29:36,27-Feb-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-058T06:20:30,007T17:54:22,27-Feb-05,CDA,Non-SPASS,DustRAM direction,SURVEY,Magnetospheric survey,Dust survey,Dust survey,,,,,, 2005-058T06:20:30,009T17:19:30,27-Feb-05,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,Data rate,Dust survey,,,,,, 2005-058T06:48:00,007T00:47:00,27-Feb-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-058T06:53:11,007T16:21:49,27-Feb-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-058T06:53:11,001T00:00:00,27-Feb-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-058T07:00:00,003T00:00:00,27-Feb-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-058T08:22:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T08:22:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T09:30:00,000T00:30:00,27-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 001 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [HE-JA-PA-PM-TE (603, 610, 612, 616, 617)]",,,,,, 2005-058T10:30:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T10:30:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T12:38:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T12:38:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T14:46:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T14:46:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T16:54:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T16:54:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T19:02:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T19:02:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T20:30:00,000T00:30:00,27-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 002 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-JA-EP-PM-TL (610, 611, 613, 614, 616)]",,,,,, 2005-058T21:10:00,000T00:40:00,27-Feb-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-058T21:10:00,000T00:40:00,27-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-058T22:50:00,003T09:00:00,27-Feb-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-058T22:50:00,000T09:00:00,27-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-059T06:20:24,001T00:00:00,28-Feb-05,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2005-059T08:30:00,000T00:30:00,28-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 003 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [MI-AT-JA-PM-EP (601, 610, 611, 615, 616)]",,,,,, 2005-059T10:10:00,000T00:40:00,28-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-059T10:10:00,000T00:40:00,28-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-059T12:18:00,000T00:40:00,28-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-059T12:18:00,000T00:40:00,28-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-059T13:30:00,000T00:30:00,28-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 004 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-JA-EP-TL-CP (610, 611, 613, 614, 616)]",,,,,, 2005-059T14:26:00,000T00:40:00,28-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-059T14:26:00,000T00:40:00,28-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-059T16:34:00,000T00:40:00,28-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-059T16:34:00,000T00:40:00,28-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-059T18:42:00,000T00:40:00,28-Feb-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in three filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-059T18:42:00,000T00:40:00,28-Feb-05,VIMS,SPASS Rider,Saturn,1X6MOVIEB,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-059T20:00:00,000T00:30:00,28-Feb-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 005 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [HE-PA-AT-TE-JA (603, 610, 612, 615, 617)]",,,,,, 2005-059T22:50:00,000T09:00:00,28-Feb-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-059T23:35:00,000T06:00:00,28-Feb-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-060T06:20:24,002T18:12:53,1-Mar-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-060T09:50:00,000T01:30:00,1-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 017 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [TE-TL-MI-PA-HE-EP-CP-AT-EN-PM (601, 602, 603, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2005-060T11:20:00,000T11:00:00,1-Mar-05,CIRS,Prime,Saturn,MIRMAPA,Mid infrared map,CIRS_004SA_MIRMAPA39,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-060T22:50:00,000T09:00:00,1-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-061T07:50:00,001T00:00:00,2-Mar-05,INMS,Non-SPASS,Saturn,PTOTM015,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-061T08:20:00,000T11:00:00,2-Mar-05,CIRS,Prime,Saturn,MIRMAPB,Mid infrared map,CIRS_004SA_MIRMAPB39,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-061T19:20:00,000T01:30:00,2-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 011 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [TL-AT-EP-JA-EN-PM-TE-HE-MI-CP (601, 602, 603, 610, 611, 612, 613, 614, 615, 616)]",,,,,, 2005-061T22:50:00,000T09:00:00,2-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-062T01:00:00,000T00:30:00,3-Mar-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-062T07:50:00,002T23:45:00,3-Mar-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-062T07:50:00,004T23:44:00,3-Mar-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-062T08:50:00,000T05:15:00,3-Mar-05,VIMS,Prime,RingE,E45PHASE,E ring observation,E Ring near phase 45,"Orbits = 004-005, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 135, Time of observation (hours) = 15, Volume (Mbits) = 217, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturn's pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 4 at Priority 1; also any 1 of 4 at Priority 2",,,,,, 2005-062T08:50:00,000T05:15:00,3-Mar-05,CIRS,SPASS Rider,RingE,E45PHASE,E ring observation,VIMS E45 Phase,null,,,,,, 2005-062T14:05:00,000T00:30:00,3-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 013 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-TE-PM-PA-JA (603, 610, 614, 616, 617)]",,,,,, 2005-062T15:05:00,000T09:00:00,3-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-062T15:50:00,000T06:00:00,3-Mar-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-063T01:05:00,000T11:30:00,4-Mar-05,RPWS,Prime,Saturn,ANTCAL,Antenna calibration,RPWS Post-Probe Release Antenna Cal.,"Repeat of portion of Jupiter RPWS antenna calibration to check for change in antenna calibration after probe has been released. Require two eleven hour periods in the orbits just following probe release at apoapsis and again during orbits 21, 23, or 25 when apoapsis is larger. Attitude, rotate about an axis which is 30 degrees off the x-axis in the direction of -Y, in such a way that the RPWS antenna directions sweep through Saturn once per turn. FRs look okay to calibrate the Z-antenna.",,,,,, 2005-063T12:35:00,001T19:00:00,4-Mar-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-063T13:00:00,000T01:00:00,4-Mar-05,ISS,Prime,Rhea,166W047PH,Spectrophotometery,Rhea spectrophotometry/ phase coverage,Turn -Y to Rhea; Do 1x1 mosaic S19 filter set; turn to WP.,,,,,, 2005-063T13:00:00,000T01:00:00,4-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-063T14:00:00,000T05:35:00,4-Mar-05,VIMS,Prime,RingE,E45PHASE,E ring observation,E Ring near phase 45,"Orbits = 004-005, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 135, Time of observation (hours) = 15, Volume (Mbits) = 217, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturn's pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 4 at Priority 1; also any 1 of 4 at Priority 2",,,,,, 2005-063T14:00:00,000T05:35:00,4-Mar-05,CIRS,SPASS Rider,RingE,E45PHASE,E ring observation,VIMS E45 Phase,Re 45 deg phase rider,,,,,, 2005-063T14:00:00,000T05:35:00,4-Mar-05,ISS,SPASS Rider,RingE,E45PHASE,E ring observation,RIDE ALONG E RING OBSERVATIONS,RIDE ALONG E RING OBSERVATIONS,,,,,, 2005-063T19:35:00,000T00:30:00,4-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 016 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 3 targets: [TL-EP-PM (611, 613, 616)]",,,,,, 2005-063T22:35:00,000T09:00:00,4-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-064T08:35:00,000T00:55:00,5-Mar-05,ISS,Prime,Janus,MUTUALEVE,Mutual event satellite transit observation,"MUTUAL EVENTS, TRANSIT OF Janus ACROSS Encelad","Turn to satellite, take 1 NAC every ~ minute for duration of event while tracking satellite",,,,,, 2005-064T09:30:00,000T01:00:00,5-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 019 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 8 targets: [TE-CP-JA-PM-TL-EP-PA-HE (603, 610, 611, 612, 613, 614, 616, 617)]",,,,,, 2005-064T18:00:00,000T01:30:00,5-Mar-05,ISS,Prime,Janus,MUTUALEVE,Mutual event satellite transit observation,"MUTUAL EVENTS, TRANSIT OF Janus ACROSS Prometh","Turn to satellite, take 1 NAC every ~ minute for duration of event while tracking satellite",,,,,, 2005-064T19:30:00,000T01:30:00,5-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 020 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [CP-PA-AT-HE-MI-EP-JA-PM-EN-TL (601, 602, 610, 611, 612, 613, 614, 615, 616, 617)]",,,,,, 2005-064T22:35:00,000T09:00:00,5-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-065T07:35:00,002T00:00:00,6-Mar-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-065T07:35:00,000T23:45:00,6-Mar-05,INMS,Non-SPASS,Saturn,PTOTM016,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-065T07:35:00,001T23:59:00,6-Mar-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-065T08:50:00,000T00:58:00,6-Mar-05,ISS,Prime,Tethys,094W035PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn UVIS_FUV to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T08:50:00,000T00:58:00,6-Mar-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T09:48:00,000T00:30:00,6-Mar-05,ISS,Prime,Enceladus,238W049PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Turn UVIS_FUV to Enceladus; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T09:48:00,000T00:30:00,6-Mar-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T10:18:00,000T00:42:00,6-Mar-05,ISS,Prime,Mimas,022W040PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn UVIS_FUV to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T10:18:00,000T00:42:00,6-Mar-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T11:00:00,000T03:03:00,6-Mar-05,ISS,Prime,Saturn,WINDS1,Saturn wind observation,Saturn winds/cloud height 2x3 feature track,"A pair of 2x3 mosaics separated by 1h 20m. NAC in MT2/CB2 and MT1/CB1. Also a set of WACs in CB2, MT2, MT3.",,,,,, 2005-065T14:03:00,000T01:00:00,6-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 022 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 7 targets: [TL-PM-JA-EP-MI-TE-CP (601, 603, 610, 611, 613, 614, 616)]",,,,,, 2005-065T15:03:00,000T00:57:00,6-Mar-05,ISS,Prime,Mimas,094W036PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn UVIS_FUV to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T15:03:00,000T00:57:00,6-Mar-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T16:00:00,000T00:45:00,6-Mar-05,ISS,Prime,Enceladus,310W047PH,Spectrophotometery,Enceladus spectrophotometry/ phase coverage,Turn UVIS_FUV to Enceladus; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T16:00:00,000T00:45:00,6-Mar-05,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T17:15:00,000T00:20:00,6-Mar-05,ISS,Prime,Tethys,166W039PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn UVIS_FUV to Tethys; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T17:15:00,000T00:20:00,6-Mar-05,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T17:35:00,000T00:30:00,6-Mar-05,ISS,Prime,Dione,238W051PH,Spectrophotometery,Dione spectrophotometry/ phase coverage,Turn -Y to Dione; Do 1x1 mosaic S19 filter set; turn to WP.,,,,,, 2005-065T17:35:00,000T00:30:00,6-Mar-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T18:10:00,000T01:00:00,6-Mar-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 023 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 7 targets: [JA-PM-EN-PA-AT-CP-TE (602, 603, 610, 614, 615, 616, 617)]",,,,,, 2005-065T19:16:00,000T00:30:00,6-Mar-05,ISS,Prime,Mimas,166W039PH,Spectrophotometery,Mimas spectrophotometry/ phase coverage,Turn UVIS_FUV to Mimas; Do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters,,,,,, 2005-065T19:16:00,000T00:30:00,6-Mar-05,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-065T22:20:00,000T09:00:00,6-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-065T23:15:00,001T08:19:00,6-Mar-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-066T00:14:52,000T01:59:59,7-Mar-05,CDA,Non-SPASS,Hyperion,2400HYORX,Hyperion orbit crossing,Hyperion Orbit Xing 0.0070 deg from dust ram.",,,,,, 2005-068T01:30:47,000T01:21:07,9-Mar-05,CDA,Non-SPASS,DustRAM direction,0700DUST,Dust survey,E Ring dense - survey - 0.15 7.5m out of 45deg fov. Stays in fov rest of observation.",,,,,, 2005-068T08:05:00,000T03:03:01,9-Mar-05,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field. NOTE:- rate below assumes continuous 600bps survey will be added to make up the total rate (total rate required is 1976 bps).,,,,,, 2005-068T08:10:36,000T00:58:28,9-Mar-05,CDA,Non-SPASS,DustRAM direction,0400DUST,Dust survey,E Ring dense - survey - 0.1070 deg from dust ram.",,,,,, 2005-068T09:38:01,000T02:01:14,9-Mar-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS survey,MAPS magnetospeheric survey.,,,,,, 2005-068T09:38:01,000T01:00:29,9-Mar-05,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. Need to do this inside 6 RS on at least half of the periapses inside of 6RS. No pointing requirement",,,,,, 2005-068T09:45:39,000T01:08:32,9-Mar-05,CDA,Non-SPASS,DustRAM direction,0400DUST,Dust survey,E Ring dense - survey - 0.0470 deg from dust ram.",,,,,, 2005-088T12:58:30,000T06:31:30,29-Mar-05,CDA,Non-SPASS,DustRAM direction,DUSTSP,Dust survey,Dust survey during downlink,"Dust survey during downlink, rate=200, pointing: as defined by MAPS",,,,,, 2005-088T13:30:00,000T06:00:00,29-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-088T14:15:00,000T06:00:00,29-Mar-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-088T16:26:30,000T14:00:00,29-Mar-05,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. Need to do this inside 6 RS on at least half of the periapses inside of 6RS. No pointing requirement",,,,,, 2005-088T19:30:00,001T00:30:00,29-Mar-05,CDA,Non-SPASS,DustRAM direction,DUSTSER,Dust survey,Dust serendipity survey,"CDA dust survey, rate=100 pointing: no requirements",,,,,, 2005-088T20:00:00,000T03:00:00,29-Mar-05,CAPS,Prime,co-rotation,RNGSATPTG,Ring / Satellite,MAPS RS Campaign (Pointing),Part of RS MAPS Campaign. Request covers prime pointing only. Data volume is in RNGSAT request.,,,,,, 2005-088T20:10:00,000T07:05:00,29-Mar-05,MAG,SPASS Rider,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space. Port3 C kernal check shows field stays in -X 45deg fov for whole observation.,,,,,, 2005-088T23:00:00,000T09:00:00,29-Mar-05,CIRS,Prime,Saturn,LMBFRNG,F ring movie,CIRS_005SA_LMBFRNG002,"F Ring rotation movie (1st hr), Iapetus (30 min), epimetheus (30 min), LIMB MAP (6 hr), F Ring (1 hr). L ansa/limb.",,,,,, 2005-088T23:00:00,000T09:00:00,29-Mar-05,CIRS,SPASS Rider,Saturn,LMBFRNG,F ring movie,ISS_PHOT_1x1,"ISS WAC support imaging, 1 image per limb position (~9 positions = 4.5Mb, 0.5 Mb/frame)",,,,,, 2005-088T23:00:00,000T09:00:00,29-Mar-05,ISS,SPASS Rider,Saturn,LMBFRNG,F ring movie,"F RING, IA and EP observations RIDING with CIRS",F Ring rider observation. Also Iapetus spectrophotometry/ phase coverage of [Do 1x1 mosaic 3 NAC clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters] and Epimetheus obsvn,,,,,, 2005-088T23:00:00,000T09:00:00,29-Mar-05,VIMS,SPASS Rider,Saturn,LMBFRNG,F ring movie,Ring Movie A Limb,"32x32 cubes centered on CIRS FP1. IR + VIS. Continuous integration while on the F Ring ansa, using 320 msec integration.",,,,,, 2005-088T23:26:10,000T11:06:30,29-Mar-05,INMS,Non-SPASS,co-rotation,RNGSATIM,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-088T23:55:00,000T00:05:00,29-Mar-05,RPWS,Non-SPASS,Saturn,HRSED,Highest resolution saturn kilometric radiation observation,Highest Resolution SED Observations,"Obtain the highest resolution observations of Saturn Electrostatic Discharges (SED) by using the RPWS HF-WBR mode at ~180 kbps within 6 RS for a total of 60 minutes within the first 12 periapses inside of 6 RS. Results will help to verify the source as lightning, or provide evidence that they could be of some other origin (e.g. rings). No attitude requirement.",,,,,, 2005-089T00:30:00,000T00:30:00,30-Mar-05,VIMS,SPASS Rider,Epimetheus,EPIMETHEU,Epimetheus,Epimetheus,"24i2-v3 160 ms, 640 ms, 5.7 mb/cycle uncompressed, 4min/cycle repeat 5 times",,,,,, 2005-089T03:15:00,000T09:45:00,30-Mar-05,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,Observe Saturns inner magnetosphere and the interactions between icy satellites rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.,,,,,, 2005-089T08:00:00,000T03:00:00,30-Mar-05,VIMS,Prime,Saturn,THRCYLMAP,Saturn themal cylindrical map,Saturn Thermal Cylindrical Map,Saturn Thermal Cylindical Map,,,,,, 2005-089T08:00:00,000T03:00:00,30-Mar-05,UVIS,SPASS Rider,Saturn,THRCYLMAP,Saturn themal cylindrical map,UVIS Rider to VIMS THRCYLMAP,UVIS Rider to VIMS THRCYLMAP,,,,,, 2005-089T10:32:40,000T02:27:20,30-Mar-05,INMS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-089T10:57:59,000T02:02:01,30-Mar-05,MIMI,SPASS Rider,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-089T11:00:00,000T00:32:00,30-Mar-05,ISS,Prime,Rhea,REGMAPA,Regional map,Rhea regional mapping,Turn -Y to Rhea; do 3x3 mosaic in NAC clear.,,,,,, 2005-089T11:00:00,000T00:32:00,30-Mar-05,CIRS,SPASS Rider,Rhea,TRNFRMWPT,,Deep space during turn from waypoint,"Rider on ISS turn from Saturn rings to Rhea. Duration 00:32. CIRS: 38RTI, pairs 00:00 to 00:12; shutter closed 00:06 to 00:12. CIRS: 38 RTI, blink 001:12 to 00:32; shutter closed 00:18 to 00:24.",,,,,, 2005-089T11:00:00,000T00:32:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-089T11:00:00,000T00:32:00,30-Mar-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"160ms/pixel, as large a cube as will fit in the time.",,,,,, 2005-089T11:32:00,000T00:15:00,30-Mar-05,CIRS,Prime,Rhea,FP3SUBSOL,,FP3 map of subsolar region,"FP 3 map of Rhea subsolar region. AD=10.7 mrad, phase=52, LT=8.8, Sub S/C=(0, 79), Subsolar=(-22, 29). Duration 00:15. Handoff point: NAC to Rhea center, POS_Z to NSP Make 2-scan FP3 mosaic centered on subsolar point (adjust to provide lateral shift in space off bright limb); each scan 7 mrad at 16 microrad/sec. CIRS: 38 RTI, blink, shutter closed first (and last?) 2 min. Request one WAC image at turning point to second scan (ca. T11:39).",,,,,, 2005-089T11:32:00,000T00:15:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,"Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible but parallel to spin axis is prefered. Slew to center of illuminated disk. Stare for 1 min. Slew to bright limb, (slew perpendicular to long axis of slit) then turn slowly to other limb at 10 microrad/sec. Return to center of illuminated disk and stare for remainder of observation.",,,,,, 2005-089T11:32:00,000T00:15:00,30-Mar-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"160ms/pixel, as large a cube as will fit in the time.",,,,,, 2005-089T11:47:00,000T03:00:00,30-Mar-05,VIMS,Prime,Rhea,RHEA,Rhea,Rhea,"63x63i2v3 80ms, 640 ms (57 min/cycle) repeat 1 each hour, offset each hour so cirs can put fp1 then fp3 on rhea (note assume hirs vims still fits on bright protion of rhes Fill any extra time with 160ms/pxl cubes",,,,,, 2005-089T11:47:00,000T03:00:00,30-Mar-05,CIRS,SPASS Rider,Rhea,VIMSINT1,,1 cm-1 resolution rider on VIMS stare at Rhea,"Rider on VIMS long integration on Rhea. Duration 03:00. AD=10.6-10.1, phase=54-78, LT=8.7-6.9, Sub S/C=(0, 81)-(0, 118). CIRS: 224 RTI (1 cm-1 resolution), pairs; shutter closed 00:15 to 00:20, and 02:40 to 02:45. REQUEST VIMS PLACE FP1 ON RHEA OF HALF OF OBSERVATION CIRS: 38 RTI, blink 001:12 to 00:32; shutter closed 00:18 to 00:24.",,,,,, 2005-089T11:47:00,000T03:00:00,30-Mar-05,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea regional geodesy,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-089T11:47:00,000T03:00:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-089T13:00:00,001T05:05:16,30-Mar-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-089T13:00:00,000T06:22:00,30-Mar-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-089T13:00:00,001T03:05:16,30-Mar-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-089T13:00:00,000T06:22:00,30-Mar-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-089T13:00:00,000T06:22:00,30-Mar-05,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-089T14:47:00,000T00:10:00,30-Mar-05,ISS,Prime,Rhea,REGMAPE,Regional map,Rhea regional mapping,Do 3x3 mosaic in NAC clear.,,,,,, 2005-089T14:47:00,000T00:10:00,30-Mar-05,CIRS,SPASS Rider,Rhea,2X3MOSAIC,2 x 3 mosaic,Rider on ISS 2x3 mosaic of Rhea,"Rider on ISS 2x3 mosaic of Rhea (short dwells). Duration 00:10. AD=10.1, phase=76, LT=7.0, Sub S/C=(0, 116). CIRS: 38 RTI, blink.",,,,,, 2005-089T14:47:00,000T00:10:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-089T14:47:00,000T00:10:00,30-Mar-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"160ms/pixel, as large a cube as will fit in the time.",,,,,, 2005-089T14:57:00,000T00:33:00,30-Mar-05,CIRS,Prime,Rhea,FP13MAPS,CIRS FP1 / FP3 mapping,"FP1 disk scan, FP3 map of subsolar region","FP1 disk scan, FP3 map of Rhea subsolar region. AD=10.1-9.8 mrad, phase=78-82, LT=6.9-6.6, Sub S/C=(0, 118)-(0, 124), Subsolar=(-22, 41). Duration 00:33. Handoff point: NAC to Rhea center, POS_Z to NSP Make single FP1 diametric scan from dark to light side. Length 23 mrad; rate 24 microrad/sec (00:16). Then make 2-scan FP3 mosaic centered on lighted side (adjust to provide lateral shift in space off bright limb); each scan 7 mrad at 16 microrad/sec (00:15). Return to handoff point. CIRS: 38 RTI, pairs, shutter closed 00:14 to 00:16; 38 RTI, blink 00:16 to 00:33, shutter closed first (and last?) 2 min. Request one WAC image at beginning (14:57), another at turning point to second scan (ca. T15:20).",,,,,, 2005-089T14:57:00,000T00:33:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,"Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible but parallel to spin axis is prefered. Slew to center of illuminated disk. Stare for 1 min. Slew to bright limb, (slew perpendicular to long axis of slit), then turn slowly to other limb at 10 microrad/sec. Return to center of illuminated disk and stare for remainder of observation.",,,,,, 2005-089T14:57:00,000T00:33:00,30-Mar-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"160ms/pixel, as large a cube as will fit in the time.",,,,,, 2005-089T15:30:00,000T01:00:00,30-Mar-05,VIMS,Prime,Rhea,RHEA,Rhea,Rhea,"63x63i2v3 80ms, 640 ms (60 min/cycle) point and stare fill with 160ms if possible",,,,,, 2005-089T15:30:00,000T01:00:00,30-Mar-05,CIRS,SPASS Rider,Rhea,VIMSINT2,,1 cm-1 resolution rider on VIMS stare at Rhea,"Rider on VIMS long integration on Rhea. Duration 01:00. AD=9.8-9.3, phase=82-87, LT=6.6-6.1, SubS/C=(0, 124)-(0, 132). CIRS: 224 RTI (1 cm-1 resolution), pairs; shutter closed 00:10 to 00:13, and 00:47 to 00:50. REQUEST VIMS PLACE FP1 ON ILLUMINATED PORTION OF RHEA FOR HALF OF OBSERVATION CIRS: 38 RTI, blink 001:12 to 00:32; shutter closed 00:18 to 00:24.",,,,,, 2005-089T15:30:00,000T01:00:00,30-Mar-05,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea regional geodesy,Do WAC rgb and NAC clear filter at end of request.,,,,,, 2005-089T15:30:00,000T01:00:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-089T16:30:00,000T00:05:00,30-Mar-05,ISS,Prime,Rhea,REGGEODF,Regional geodesy,Rhea regional geodesy,Do 1+2 mosaic in NAC clear filter.,,,,,, 2005-089T16:30:00,000T00:05:00,30-Mar-05,CIRS,SPASS Rider,Rhea,MOSAIC2,Mosaic,Rider on ISS mosaic of Rhea,"Rider on ISS mosaic of Rhea (short dwells). Duration 00:05. AD=9.2, phase=87, LT=6.1, Sub S/C=(0, 132). CIRS: 38 RTI, blink.",,,,,, 2005-089T16:30:00,000T00:05:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-089T16:30:00,000T00:05:00,30-Mar-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"160ms/pixel, as large a cube as will fit in the time.",,,,,, 2005-089T16:35:00,000T01:25:00,30-Mar-05,CIRS,Prime,Rhea,FP13MAPS,CIRS FP1 / FP3 mapping,"FP1, FP3 maps of Rhea","FP1 disk map, FP3 disk map of Rhea. AD=9.1-8.2 mrad, phase=88-97, LT=6.1-5.5, Sub S/C=(0, 134)-(0, 148), Subsolar=(-22, 45)-(-22, 51). Duration 01:25. Handoff point: NAC to Rhea center, POS_Z to NSP; Return waypoint: NAC to L ansa F (0, 20, 0) offset), POS_X to NSP Make two Nyquist FP1 maps of 6 scans each (00:13). Then make 3-scan FP3 mosaic of disk; each scan 11 mrad at 12 microrad/sec (00:47). Return to waypoint (00:25???). CIRS: 38 RTI, blink, shutter closed first and last 10 min. Request one WAC image at beginning (16:35), another at turning point to second scan (ca. T17:20).",,,,,, 2005-089T16:35:00,000T01:25:00,30-Mar-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible but parallel to spin axis is prefered. Slew to center of illuminated disk. Stare for 1 min. Slew to bright limb (slew perpendicular to long axis of slit) then turn slowly to other limb at 10 microrad/sec. Return to center of illuminated disk and stare for remainder of observation.,,,,,, 2005-089T16:35:00,000T01:25:00,30-Mar-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"320ms/pixel, as large a cube as will fit in the time. (0r maybe 640 ms",,,,,, 2005-089T17:08:42,000T12:41:18,30-Mar-05,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,Ka-Downlink for Gravity,Additional downlink pass at Ka-band for Titan gravity science. This request includes 2 hours Ka-TWTA maintenance and 2 hours RFIS thermal stabilization.,,,,,, 2005-089T19:22:00,000T12:43:16,30-Mar-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-089T19:22:00,000T22:43:16,30-Mar-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-089T19:22:00,000T07:58:00,30-Mar-05,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-089T20:00:00,000T06:15:00,30-Mar-05,CDA,Non-SPASS,DustRAM direction,DUSTSP,Dust survey,CDA Dust survey during downlink,"Dust survey during downlink, rate=200, poiting: secondary: -x (RA: 217.6, DEC: 33.4)",,,,,, 2005-089T21:08:42,000T08:41:18,30-Mar-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-089T22:00:00,000T06:00:00,30-Mar-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-090T03:20:00,000T15:02:25,31-Mar-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-090T04:15:00,000T02:12:07,31-Mar-05,CDA,Non-SPASS,DustRAM direction,1500DUST,Dust survey,Ring Margin - survey - 0.14Reaction Wheels Required,,,,,, 2005-104T11:00:00,001T01:05:00,14-Apr-05,CAPS,SPASS Rider,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-104T11:00:00,000T07:50:00,14-Apr-05,MIMI,SPASS Rider,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-104T11:00:00,000T01:28:00,14-Apr-05,INMS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-104T11:00:00,000T08:00:00,14-Apr-05,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,Observe Saturns inner magnetosphere and the interactions between icy satellites rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.,,,,,, 2005-104T11:00:00,001T01:05:00,14-Apr-05,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2005-104T11:50:00,000T02:35:00,14-Apr-05,VIMS,Prime,Rhea,RHEA,Rhea,Rhea,"1x2 mosaic for ISS at beginning and end with minimum 15 second dwell, else point and stare centered on bight portion of disk. VIMS does 160 ms, 640ms pairs double res ir, triple res vis, FOV to frame object (keep frame size same for whole period. Frame size ~30x15 (may need large for vis coverage.",,,,,, 2005-104T11:50:00,000T02:35:00,14-Apr-05,CIRS,SPASS Rider,Rhea,CIRSRIDE1,,Rhea CIRS Ride With VIMS,"CIRS ridealong with VIMS. Cover afternoon/evening hemisphere. Desire FP1 integration (20 min), and FP3 map (20 min) interpolated within VIMS observations. (-13, 063); AD=6.1 mrad; 67 S.",,,,,, 2005-104T14:37:48,000T00:30:00,14-Apr-05,CDA,Non-SPASS,RingE,0707ERNGM,E ring margin,E-Ring Margin 7.0070 deg from dust ram.",,,,,, 2005-104T20:10:44,000T10:00:00,14-Apr-05,RPWS,Non-SPASS,Saturn,SEDMSEC,Saturn Electrical Discharge observation,High temporal observations of SED,Obtain millisecond temporal resolution observations of Saturn Electrostatic Discharges (SED) in order to characterize their temporal structure and to verify their source as lightning (or to refute this). No pointing requirement.,,,,,, 2005-104T20:25:00,000T04:00:00,14-Apr-05,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2005-104T20:29:46,000T00:10:03,14-Apr-05,CDA,Non-SPASS,RingE,0304ERNGX,Ring plane crossing,E Ring Xing 4.0070 deg from dust ram.",,,,,, 2005-122T22:08:43,000T10:00:00,2-May-05,RPWS,Non-SPASS,Saturn,SEDMSEC,Saturn Electrical Discharge observation,High temporal observations of SED,Obtain millisecond temporal resolution observations of Saturn Electrostatic Discharges (SED) in order to characterize their temporal structure and to verify their source as lightning (or to refute this). No pointing requirement.,,,,,, 2005-122T22:10:35,000T00:10:03,2-May-05,CDA,Non-SPASS,Enceladus,0400ENORX,Enceladus orbit crossing,Enceladus Orbit Xing 0.00Reaction Wheels Required",,,,,, 2005-132T02:42:00,002T00:08:00,12-May-05,CAPS,SPASS Rider,Saturn,MAGBNDORS,MAPS magnetosphere boundary campaign,MAPS ORS Boundary Campaign,MAPS magnetospheric survey,,,,,, 2005-132T02:42:00,002T00:07:59,12-May-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/B Campaign,"Part of MB/B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2005-132T02:42:00,002T00:08:00,12-May-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,B Campaign","Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-132T03:15:00,000T13:05:00,12-May-05,UVIS,Prime,Saturn,MOS07APO,Apoapsis mosaic,MOSAIC_APO_07_08,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, perpendicular to the orbital plane (FOV Twist: 91.57 deg). 1) Drift at a rate of 0.079413158 mrad/sec about the Z-axis from START RA/DEC (planet center) to -MOS orb for 8000s. Drift back to center, reset pointing for planet center. Total cycle time 16000 seconds. (2) Rotate 64 mr in the YZ plane from planet center. Repeat (1) for a cycle time of another 16000 seconds, and then drift at indicated rate to +MOS orb for 8000s. (3) Slew back to planet center and reset pointing. Stare at planet for remaining observation time. MOS orb (+/-range): 635.3052657 mrad",,,,,, 2005-132T03:22:50,001T23:27:10,12-May-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-132T03:23:49,001T23:26:01,12-May-05,CDA,Non-SPASS,DustRAM direction,0612DUST,Dust survey,Dust survey 12.06D rings) at 11 R_S. Obtain images to map opposition surge out to 0.5 deg phase angle at all ring radii. ISS, UVIS to ridealong.",,,,,, 2005-140T07:00:00,000T04:00:00,20-May-05,CIRS,SPASS Rider,rings(general),0PHASE,Zero phase observation,CIRS_ VIMS Rider,Ride along with VIMS observation,,,,,, 2005-140T07:00:00,000T04:00:00,20-May-05,ISS,SPASS Rider,rings(general),0PHASE,Zero phase observation,"Rev 8 ring zero-phase, left ansa, WAC","TWT RINGS; rider, corresponding to initial request ISS_010RI_W0PHLAN001",,,,,, 2005-140T07:00:00,000T04:00:00,20-May-05,UVIS,SPASS Rider,rings(general),0PHASE,Zero phase observation,,Hi spectral resolution UV map of rings at low phase.,,,,,, 2005-140T11:00:00,000T07:00:00,20-May-05,CIRS,Prime,rings(general),SUBML20LP,Ring radial scan,CIRS_008RI_SubmL20LP,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. CIRS_FP1 to rings, POS_X to NSP with Y-offset of +20 degrees.",,,,,, 2005-140T11:00:00,000T07:00:00,20-May-05,ISS,SPASS Rider,rings(general),SUBML20LP,Ring radial scan,RIDE ALONG WITH CIMS SUBMM RAD SCAN,RIDE ALONG WITH CIRS SUBML RADIAL SCAN; ABOUT 26 POINTINGS,,,,,, 2005-140T11:00:00,000T07:00:00,20-May-05,UVIS,SPASS Rider,rings(general),SUBML20LP,Ring radial scan,,Hi spectral resolution UV map of rings at low phase.,,,,,, 2005-140T18:00:00,000T02:06:00,20-May-05,ISS,Prime,Other,RETARGEMR,Retargetable observation,DETERMINING THE ORBITS OF NEWLY DISCOVERED SATELLI,"Turn to satellite, take 3x1 BOTSIM mosaic",,,,,, 2005-140T18:21:45,000T11:15:02,20-May-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-140T20:26:00,000T01:15:00,20-May-05,CIRS,Prime,Saturn,CWLEON,CW Leo occultation,CW Leo ingress occultation by Saturn,"Ingress latitude TBD; apparent drift rate ca. 17 km/sec. The apparent passage of CW Leo through the atmosphere of Saturn provides information on the composition and chemistry at high altitudes. One FP3 pixel is targeted on the star throughout the occultation. The FP3 array axis (Z) is aligned with the apparent drift direction across the planet. FK5 2000.0/2000.0 coordinates 09h 47m 57.3s, +13d 16m 44s = 146.989d, 13.279d.",,,,,, 2005-140T20:26:00,000T01:15:00,20-May-05,CIRS,SPASS Rider,Saturn,CWLEON,CW Leo occultation,CIRS_008SA_CWLEON_SI,"Support image for occultation. Single NAC losslessly compressed (3:1), within 10 minutes of observation start time",,,,,, 2005-140T20:26:00,000T01:15:00,20-May-05,VIMS,SPASS Rider,Saturn,CWLEON,CW Leo occultation,CW Leo Saturn occ.,"CW Leo Saturn occultation. tau_IR=80 msec, IR_only. Stellar_occ mode.",,,,,, 2005-140T21:02:16,000T00:30:00,20-May-05,CDA,Non-SPASS,DustRAM direction,0615SURIN,Dust survey,Dust survey inside 8 Rs 15.0070 deg from dust ram.",,,,,, 2005-141T02:35:00,000T07:35:00,21-May-05,MAG,SPASS Rider,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,"This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space. NOTE: period 9 INTFLD request is backup to this request. For whichever of these 2 requests (8/9) MAG is not made prime instrument, we still wish to take high rate continuous data.",,,,,, 2005-141T03:50:01,001T15:40:00,21-May-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-141T04:00:21,000T00:49:00,21-May-05,CDA,Prime,Enceladus,0400ENORX,Enceladus orbit crossing,Enceladus Orbit Xing 0.0070 deg from dust ram.",,,,,, 2005-159T07:10:00,000T07:35:00,8-Jun-05,MAG,SPASS Rider,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,"This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space. NOTE: request is backup to period 8 request. For whichever of these 2 requests (8/9) MAG is not made prime instrument, we still wish to take high rate continuous data.",,,,,, 2005-159T07:35:00,000T01:52:00,8-Jun-05,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2005-159T08:44:10,001T09:01:00,8-Jun-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-159T09:26:22,000T02:04:00,8-Jun-05,CDA,Prime,Enceladus,0400ENORX,Enceladus orbit crossing,Enceladus Orbit Xing 0.00D rings) at 11 R_S. Obtain images to map opposition surge out to 0.5 deg phase angle at all ring radii. ISS, UVIS to ridealong. scan across west (RIGHT) ansa.",,,,,, 2005-177T03:00:00,000T02:40:00,26-Jun-05,CIRS,SPASS Rider,rings(general),0PHASE,Zero phase observation,CIRS_ VIMS Rider,Ride along with VIMS observation,,,,,, 2005-177T03:00:00,000T02:40:00,26-Jun-05,ISS,SPASS Rider,rings(general),0PHASE,Zero phase observation,"Rev 10 low-phase ring mosaic, NAC + WAC","TWT RINGS; rider, corresponding to initial request ISS_007RI_WNLOPHAS001",,,,,, 2005-177T03:00:00,000T02:40:00,26-Jun-05,UVIS,SPASS Rider,rings(general),0PHASE,Zero phase observation,,Hi spectral resolution UV map of complete ring system at low phase angle in evening quadrant of rings.,,,,,, 2005-177T04:19:26,000T11:15:29,26-Jun-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-177T05:40:00,000T02:50:00,26-Jun-05,CIRS,Prime,Saturn,NADIROCC,Occultation,CIRS_010SA_NADIROCC01,"obtain CIRS spectra in the vicinity of RSS occultation points to obtain a new He determination. POINTING: -y to Saturn, z to pole",,,,,, 2005-177T06:55:00,000T09:33:00,26-Jun-05,RSS,SPASS Rider,Saturn,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band to improve Saturn's gravity field determination. This request includes 5 minutes Ka-band maintenance and 2 hours RFIS thermal stabilization.,,,,,, 2005-177T07:14:53,000T00:34:32,26-Jun-05,CDA,Non-SPASS,DustRAM direction,0615SURIN,Dust survey,Dust survey inside 8 Rs 15.0070 deg from dust ram.",,,,,, 2005-177T13:00:00,000T01:00:00,26-Jun-05,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-177T14:00:00,000T02:28:00,26-Jun-05,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-177T14:08:01,001T10:52:00,26-Jun-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-177T14:28:00,000T02:23:57,26-Jun-05,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 010RI PRE-OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band. This commences 2.5 hours prior to ring INGRESS on rev. 007.,,,,,, 2005-177T15:15:00,000T00:05:00,26-Jun-05,RPWS,Non-SPASS,Saturn,HRSED,Highest resolution saturn kilometric radiation observation,Highest Resolution SED Observations,"Obtain the highest resolution observations of Saturn Electrostatic Discharges (SED) by using the RPWS HF-WBR mode at ~180 kbps within 6 RS for a total of 60 minutes within the first 12 periapses inside of 6 RS. Results will help to verify the source as lightning, or provide evidence that they could be of some other origin (e.g. rings). No attitude requirement.",,,,,, 2005-177T15:34:55,000T11:15:00,26-Jun-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-177T15:34:55,000T00:17:56,26-Jun-05,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2005-177T15:42:35,000T00:00:01,26-Jun-05,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse per = 18.4 d, inc = 21.8 deg, r = 3.6 Rs, phase = 113 deg",,,,,, 2005-177T16:51:57,000T02:09:00,26-Jun-05,RSS,Prime,rings(general),OCC,Occultation,RSS Early Diametric Occ. Ring Ingress 010,"THIS REQUEST: The start time is 30 minutes before the outer edge of the F ring, in order to record a baseline prior to the ring ingress occultation. The observations end at the inner edge of the D ring, roughly corresponding with the beginning of the ionosphere. GENERAL DESCRIPTION: This is one of a set of diametric radio occultations by Saturn's rings and atmosphere. We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stabilization in RSS WARMUP mode. In the most general case, we will begin with a 30-min calibration period of free-space observation, and then observe continuously through the entire ingress ring occultation, during the free-space interval between the ring and atmospheric ingress, and we will track the position of the virtual Earth along Saturn's limb as the atmospheric occultation progresses. (For an ingress-only event, this observation will stop at the end of the atmosphere occultation. For an egress-only event, the observing sequence will begin with a two-hour thermal stabilization in RSS WARMUP mode prior to atmospheric egress.) After the ingress atmospheric occultation is over, the S/C may be switched to RSS WARMUP mode, if there is time and power for observations by other instruments while the S/C is in the Earth's shadow. Then the egress atmospheric event will commence with a limb track maneuver, followed by the egress atmosphere and ring occultations, and ending with another 30-minute free-space baseline calibration.",,,,,, 2005-177T19:00:57,000T00:36:00,26-Jun-05,RSS,Prime,Saturn,OCC,Occultation,RSS Early Diametric Occ. Atm. Ingress 010,"THIS REQUEST: Observations begin at the inner edge of the D ring, roughly corresponding with the beginning of the ionosphere, and continue for 20 minutes after the 2-bar level is reached. GENERAL: This is the first of a set of diametric radio occultations by Saturn's rings and atmosphere. We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stabilization in RSS WARMUP mode. In the most general case, we will begin with a 30-min calibration period of free-space observation, and then observe continuously through the entire ingress ring occultation, during the free-space interval between the ring and atmospheric ingress, and we will track the position of the virtual Earth along Saturn's limb as the atmospheric occultation progresses. (For an ingress-only event, this observation will stop at the end of the atmosphere occultation. For an egress-only event, the observing sequence will begin with a two-hour thermal stabilization in RSS WARMUP mode prior to atmospheric egress.) After the ingress atmospheric occultation is over, the S/C may be switched to RSS WARMUP mode, if there is time and power for observations by other instruments while the S/C is in the Earth's shadow. Then the egress atmospheric event will commence with a limb track maneuver, followed by the egress atmosphere and ring occultations, and ending with another 30-minute free-space baseline calibration.",,,,,, 2005-177T19:32:00,000T04:14:10,26-Jun-05,CDA,Non-SPASS,DustRAM direction,0418DUST,Dust survey,Dust survey inside 8 Rs 17.5570 deg from dust ram.",,,,,, 2005-195T19:25:22,000T01:00:00,14-Jul-05,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 011EN Campaign,Part of 011EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2005-195T19:25:22,000T01:00:00,14-Jul-05,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-195T19:25:22,000T00:50:20,14-Jul-05,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2005-195T19:26:22,000T00:08:00,14-Jul-05,ISS,Prime,Enceladus,MORPH,Morphology,NAC Shape/Morphology/Stereo,1;NAC (3x3xGRN) Shape/Morphology/Stereo,,,,,, 2005-195T19:26:22,000T00:08:00,14-Jul-05,CIRS,SPASS Rider,Enceladus,MORPH,Morphology,rider,Nfov= 0.00 Phase= 0.0 SCLON= 0.0 SCLAT= 0.0,,,,,, 2005-195T19:26:22,000T00:08:00,14-Jul-05,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus' surface plus limb drifts,,,,,, 2005-195T19:32:00,000T01:00:00,14-Jul-05,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-195T19:51:52,000T00:06:08,14-Jul-05,UVIS,Prime,Enceladus,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to gamma Ori. 12 min allowed for slew. Return to Enceladus center at 20:05 requires 15 min slew. Both slew durations assume turn is only about Z therefore s/c orientation must be set up prior to observation!!!,,,,,, 2005-195T19:51:52,000T00:06:08,14-Jul-05,CIRS,SPASS Rider,Enceladus,ICYEXO,Icy satellite exosphere,UVIS rider,"Nfov= 0.00 Phase= 0.0 SCLON= 0.0 SCLAT= 0.0 6970 deg from dust ram.",,,,,, 2005-195T20:25:22,000T19:32:35,14-Jul-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-195T20:26:30,000T00:52:52,14-Jul-05,CIRS,Prime,Enceladus,FP1NSSCAN,CIRS FP1 dark side scan,Winter pole and darkside map,"Ten minute FP1 integration at (89.5, 0.0) for polar night temperature determination. Nfov= 13.10 Phase=126.0 SCLON= 22.0 SCLAT= 51.0. Probably cannot start until ca. 20:41 because Enceladus cannot be tracked before that (at 20:42, AD=23.3 mrad, phase=130, sub-S/C=(50, 29)). Following this observation, a 20 minute Nyquist-sampled FP1 darkside disk mosaic (AD=21 mrad). Then return to waypoint.",,,,,, 2005-195T20:26:30,000T00:52:52,14-Jul-05,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus' surface plus limb drifts,,,,,, 2005-195T20:53:57,000T19:04:00,14-Jul-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-195T20:55:22,000T13:00:34,14-Jul-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-195T21:19:22,000T00:10:00,14-Jul-05,ISS,Prime,Enceladus,NCPOL,,NAC 3-Color Polarization,1;NAC 3-Color Polarization,,,,,, 2005-195T21:19:22,000T00:10:00,14-Jul-05,CIRS,SPASS Rider,Enceladus,NCPOL,,ISS rider,Nfov= 0.00 Phase= 0.0 SCLON= 0.0 SCLAT= 0.0,,,,,, 2005-195T21:19:22,000T00:10:00,14-Jul-05,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus' surface plus limb drifts,,,,,, 2005-195T21:19:22,000T00:10:00,14-Jul-05,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus targeted,"48i2-241 160ms integrations 3.2 min/cycle, 5.1 mbits cycle uncomp, repeat 6 times = 15.3 mbits compressed coordinate with cirs",,,,,, 2005-195T21:29:22,000T00:20:00,14-Jul-05,UVIS,Prime,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,"Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible. Precise targetting per agreement with VIMS, CIRS and ISS, 3-19-04.",,,,,, 2005-195T21:29:22,000T00:20:00,14-Jul-05,CIRS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,UVIS rider,Nfov= 0.00 Phase= 0.0 SCLON= 0.0 SCLAT= 0.0,,,,,, 2005-195T21:49:22,000T00:45:00,14-Jul-05,ISS,Prime,Epimetheus,STEREO,Stereo imaging,NAC GRN STEREO,"1;NAC GRN STEREO (twice - beginning and end), NAC 3 color, and NAC GRN Polarization.",,,,,, 2005-195T21:49:22,000T00:45:00,14-Jul-05,CIRS,SPASS Rider,Epimetheus,STEREO,Stereo imaging,ISS rider,Nfov= 0.00 Phase= 0.0 SCLON= 0.0 SCLAT= 0.0,,,,,, 2005-195T21:49:22,000T00:45:00,14-Jul-05,UVIS,SPASS Rider,Epimetheus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-195T21:49:22,000T00:45:00,14-Jul-05,VIMS,SPASS Rider,Epimetheus,EPIMETHE,Epimetheus,Epimetheus targeted,"12i2x36v3 160ms, 640ms. 4-minutes/cycle (2.9mbits/cycle comp) continuous for 45 min: 11 cycles,= 31.9mbits uncomp .",,,,,, 2005-195T22:10:01,000T00:00:01,14-Jul-05,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse per = 18.5 d, inc = 21.8 deg, r = 3.6 Rs, phase = 113 deg",,,,,, 2005-195T22:36:22,000T01:50:00,14-Jul-05,UVIS,Prime,Star,URSIGSGR,Stellar occultation,URSTAR,Instance of URSTAR: Ingress cut through B ring on north face. Not in shadow.,,,,,, 2005-195T22:36:22,000T01:50:00,14-Jul-05,CIRS,SPASS Rider,rings(general),URSIGSGR,Stellar occultation,CIRS_ UVIS Rider,Ride along with UVIS observation,,,,,, 2005-195T22:49:25,000T00:30:14,14-Jul-05,CDA,Non-SPASS,DustRAM direction,0315SURIN,Dust survey,Dust survey inside 8 Rs 15.00 AD~6.5 mrad, Phase= 66.0, LT~0600, SubS/C=(-60, 277). Pick up from ISS. .....A) offset FP1 1.0 mrad in -X from center; stare 15 min at 0.5 cm-1 resolution. Use detector pairs; shutter closed last 5 min. ......B) Offset FP3 in +X by 4.0 mrad from center; drift in -X 8.0 mrad at 15.7 microrad/sec, blinking at 15.5 cm-1 resolution; repeat twice more (3x8.5 min). Close shutter last 2 min of each scan......C) Offset FP3 2.0 mrad in -X from center and stare for 35 min, blinking at 0.5 cm-1 resolution. ...D) Perform three 5-scan FP1 Nyquist box mosaics (7.0 mrad x 7.0 mrad) of disk at 15.5 cm-1 resolution (3x4.9 min). Return to waypoint (9.4 min).",,,,,, 2005-213T14:20:00,000T01:40:00,1-Aug-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-213T16:00:00,000T00:40:00,1-Aug-05,UVIS,Prime,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,"Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Rotate from waypoint such that slit orientation is parallel to Dione spin axis. Target to Dione center with ISS_NAC, sit for one minute. Point one Dione diameter off west limb with FUV boresight. Slew slowly to just off east limb (~5 microrad/sec). Return to ISS_NAC to center, stare for remaining time.",,,,,, 2005-213T16:00:00,000T00:40:00,1-Aug-05,CIRS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,DIONE LONGITUDE COVERAGE,NP09,,,,,, 2005-213T16:00:00,000T00:40:00,1-Aug-05,ISS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione regional geodesy,Do 1x1 mosaic in NAC clear,,,,,, 2005-213T16:00:00,000T00:40:00,1-Aug-05,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,"24x24 hi/hi 3x640ms, 1x160ms 2x80ms",,,,,, 2005-213T16:40:00,000T00:40:00,1-Aug-05,VIMS,Prime,Rhea,RHEA,Rhea,Rhea,"Now: 32 x 32, low res vis, hi res IR 640ms,80ms, 1 sets (2 cubes) was: 36i2-54v3 160ms, 640 ms (10 min/cycle) repeat 4 times",,,,,, 2005-213T16:40:00,000T00:40:00,1-Aug-05,CIRS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,Rhea regional geodesy,Turn -Y to Rhea; FP3 RIDER.,,,,,, 2005-213T16:40:00,000T00:40:00,1-Aug-05,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea regional geodesy,Do 1x1 mosaic in NAC clear filter,,,,,, 2005-213T16:40:00,000T00:40:00,1-Aug-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-213T17:20:00,000T00:35:00,1-Aug-05,ISS,Prime,Dione,PHOTOM,Photometry,Dione spectrophotometry,Dione 9-color observation,,,,,, 2005-213T17:20:00,000T00:35:00,1-Aug-05,CIRS,SPASS Rider,Dione,PHOTOM,Photometry,Dione ISS rider,"FP3. SubS/C=(-43, 250), phase=40, AD=4.4 mrad.",,,,,, 2005-213T17:20:00,000T00:35:00,1-Aug-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-213T17:20:00,000T00:35:00,1-Aug-05,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,"28x28 hi/hi 3x640ms, 1x160ms 2x80ms was: 42i2-63v3 80,640 ms (13 minute/cycle) repeat 1",,,,,, 2005-213T17:55:00,000T00:45:00,1-Aug-05,UVIS,Prime,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,"Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Rotate from waypoint such that slit orientation parallel to Dione spin axis. Turn to Dione center with ISS_NAC, stare 1 min. Point just off west limb with FUV, latitude ~15 N. Slew slowly to just off east limb (~10-12 microrad/sec). Flyback to just off west limb, latitude ~-30S. Slew slowly to just off east limb (10-12 microrad/sec). Return to center, ISS_NAC boresight. Stare at least one minute. If this does not fit in allocated time, reposition slew may be used in mosaic instead of flyback. Higher slew rates, up to 15 microrad/sec are also acceptable.",,,,,, 2005-213T17:55:00,000T00:45:00,1-Aug-05,CIRS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,DIONE_FP3,RIDER,,,,,, 2005-213T17:55:00,000T00:45:00,1-Aug-05,ISS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione regional geodesy,Do 1x1 mosaic in NAC clear,,,,,, 2005-213T17:55:00,000T00:45:00,1-Aug-05,VIMS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione Targeted,"32x32 hi res vis, hi res ir 2x640ms, 320ms, 3x160ms, 2x80ms was:42i2-63v3 80,640 ms (13 minute/cycle) repeat 1",,,,,, 2005-213T17:59:56,000T11:15:20,1-Aug-05,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magneospheric survey.,,,,,, 2005-213T18:40:00,000T01:20:00,1-Aug-05,VIMS,Prime,Rhea,RHEA,Rhea,Rhea Targeted,"40x40 hi/hi 1x640ms, 2x160ms was:42i2-63v3 80,640 ms (13 minute/cycle) repeat 6 times",,,,,, 2005-213T18:40:00,000T01:20:00,1-Aug-05,CIRS,SPASS Rider,Rhea,RHEA,Rhea,RHEA LONGITUDE COVERAGE,NP09,,,,,, 2005-213T18:40:00,000T01:20:00,1-Aug-05,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea regional mapping,Do 1x2 mosaic in NAC clear and 3 colors.,,,,,, 2005-213T18:40:00,000T01:20:00,1-Aug-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-213T20:00:00,000T00:25:00,1-Aug-05,UVIS,Prime,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible. Target FUV to center ISS_NAC on body and capture south pole in FUV.,,,,,, 2005-213T20:00:00,000T00:25:00,1-Aug-05,CIRS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione rider with UVIS,FP3 blink at 15.5 cm-1 resolution.,,,,,, 2005-213T20:00:00,000T00:25:00,1-Aug-05,ISS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione regional geodesy,Do 1x1 mosaic in NAC clear (two shutters),,,,,, 2005-213T20:00:00,000T00:25:00,1-Aug-05,VIMS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione Targeted,"32x32 hi res vis, hi res ir 640ms,3x160ms, 80ms was:42i2-63v3 80,640 ms (13 minute/cycle) repeat 1",,,,,, 2005-213T20:25:00,000T00:40:00,1-Aug-05,VIMS,Prime,Rhea,RHEA,Rhea,Rhea,"24 x 48 hi res vis, hi res ir single 320ms, was: 36i2-54v3 160ms, 640 ms (10 min/cycle) repeat 7.5 times",,,,,, 2005-213T20:25:00,000T00:40:00,1-Aug-05,CIRS,SPASS Rider,Rhea,RHEA,Rhea,RHEA VIMS rider,"Vims rider on Rhea. SS/C=(-40, 330), phase=97, LT=0415, AD=7.4 mrad. FP3 blink at 15.5 cm-1 resolution.",,,,,, 2005-213T20:25:00,000T00:40:00,1-Aug-05,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea regional geodesy,Do 1x1 mosaic in NAC clear filter,,,,,, 2005-213T20:25:00,000T00:40:00,1-Aug-05,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-213T21:10:04,000T00:50:24,1-Aug-05,CDA,Non-SPASS,DustRAM direction,0615SURIN,Dust survey,Dust survey inside 8 Rs 15.0070 deg from dust ram.",,,,,, 2005-214T03:12:18,000T00:10:00,2-Aug-05,CDA,Non-SPASS,Enceladus,0400ENORX,Enceladus orbit crossing,Enceladus Orbit Xing 0.00Fomalhaut: multiple cubes w/12x12 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 2.0 hr; Volume: 10 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2005-219T05:36:00,000T00:30:00,7-Aug-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 030 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-219T07:36:00,000T09:00:00,7-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-219T08:22:00,000T11:15:00,7-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-219T08:22:00,000T11:15:00,7-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-219T08:22:00,000T11:15:00,7-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-219T16:32:00,008T05:05:00,7-Aug-05,CDA,Non-SPASS,DustRAM direction,DRATESP01,Data volume adjustment,CDA Datarate Sponge bit adjustment,null,,,,,, 2005-219T18:00:00,000T04:10:00,7-Aug-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-219T18:36:00,000T00:30:00,7-Aug-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 032 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-219T19:06:00,000T06:11:00,7-Aug-05,MIMI,Prime,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,"Magnetospheric Boundary Campaign, Co-rotation","Pointing for MAGBOUNDARY Campaign, Co-rotation attitude",,,,,, 2005-219T19:37:00,000T17:15:00,7-Aug-05,CAPS,SPASS Rider,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-219T19:37:00,000T17:15:00,7-Aug-05,INMS,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-219T19:37:00,000T17:15:00,7-Aug-05,MAG,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-220T01:17:00,000T11:00:00,8-Aug-05,CIRS,Prime,Saturn,MIRMAPA,Mid infrared map,CIRS_012SA_MIRMAPA02,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-220T12:52:00,000T09:15:00,8-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-220T12:52:00,000T09:15:00,8-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-220T12:52:00,000T09:15:00,8-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-220T12:52:00,000T09:15:00,8-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-220T14:00:00,000T06:00:00,8-Aug-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-220T22:07:00,000T14:45:00,8-Aug-05,CAPS,SPASS Rider,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-220T22:07:00,000T14:45:00,8-Aug-05,INMS,Non-SPASS,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-220T22:07:00,000T14:45:00,8-Aug-05,MAG,Non-SPASS,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-220T22:42:00,000T11:00:00,8-Aug-05,CIRS,Prime,Saturn,MIRMAPB,Mid infrared map,CIRS_012SA_MIRMAPB02,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2005-221T09:42:00,000T00:40:00,9-Aug-05,MIMI,Prime,SolarWind,MAGBNDSWD,MAPS solar wind campaign,"Magnetospheric Boundary Campaign, Solar Wind","Pointing for MAGBOUNDARY Campaign, Solar Wind Attitude",,,,,, 2005-221T10:22:00,000T00:30:00,9-Aug-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 037 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-221T12:52:00,000T09:15:00,9-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-221T12:52:00,000T09:15:00,9-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-221T12:52:00,000T09:15:00,9-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-221T12:52:00,000T09:15:00,9-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-221T22:07:00,000T10:00:00,9-Aug-05,CAPS,SPASS Rider,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-221T22:07:00,000T20:53:00,9-Aug-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/B Campaign,"Part of MB/B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2005-221T22:07:00,000T10:00:00,9-Aug-05,INMS,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-221T22:07:00,000T10:00:00,9-Aug-05,MAG,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-221T22:07:00,000T20:53:00,9-Aug-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,B Campaign","Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-221T23:07:00,000T07:39:00,9-Aug-05,MIMI,Prime,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,"Magnetospheric Boundary Campaign, Co-rotation","Pointing for MAGBOUNDARY Campaign, Co-rotation attitude",,,,,, 2005-222T07:21:00,000T09:00:00,10-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-222T08:07:00,000T10:53:00,10-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis",,,,,, 2005-222T08:07:00,000T08:14:00,10-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis.",,,,,, 2005-222T08:07:00,000T10:53:00,10-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_B_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-222T08:21:00,000T06:00:00,10-Aug-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,CIRS Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2005-222T16:21:00,000T15:43:01,10-Aug-05,INMS,Non-SPASS,Saturn,PTOTM027,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-222T19:00:00,000T13:31:16,10-Aug-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/B Campaign,"Part of MB/B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2005-222T19:00:00,000T13:33:00,10-Aug-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-222T19:00:00,001T03:07:00,10-Aug-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps). Note: Does NOT overlap XD campaign.,,,,,, 2005-222T19:00:00,000T13:30:13,10-Aug-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-222T20:00:00,000T00:40:00,10-Aug-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-222T20:00:00,000T00:40:00,10-Aug-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-222T20:00:00,000T02:16:32,10-Aug-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from survey.,,,,,, 2005-222T20:00:00,000T03:54:00,10-Aug-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-222T22:08:00,000T00:40:00,10-Aug-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-222T22:08:00,000T00:40:00,10-Aug-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-223T00:16:00,000T00:40:00,11-Aug-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-223T00:16:00,000T00:40:00,11-Aug-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-223T02:24:00,000T00:40:00,11-Aug-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-223T02:24:00,000T00:40:00,11-Aug-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-223T04:32:00,000T00:40:00,11-Aug-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-223T04:32:00,000T00:40:00,11-Aug-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-223T06:40:00,000T00:40:00,11-Aug-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-223T08:04:01,000T14:02:59,11-Aug-05,INMS,Non-SPASS,Saturn,PTOTM27BU,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-223T08:04:01,001T13:36:47,11-Aug-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-223T08:30:23,000T00:00:01,11-Aug-05,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse per = 18.2 d, inc = 21.9 deg, r = 40.7 Rs, phase = 68 deg",,,,,, 2005-223T08:31:16,000T13:35:44,11-Aug-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/B Campaign,"Part of MB/B MAPS Campaign. Observe variability of magnetospheric boundaries at several geometrically similar apoapsis. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2005-223T08:33:00,000T13:34:00,11-Aug-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-223T08:44:45,006T04:00:15,11-Aug-05,CDA,Non-SPASS,DustRAM direction,0713DUST,Dust survey,Dust survey 12.6070 deg from dust ram.",,,,,, 2005-232T09:14:25,000T00:10:03,20-Aug-05,CDA,Non-SPASS,Enceladus,0400ENORX,Enceladus orbit crossing,Enceladus Orbit Xing 0.00Pleiades: multiple cubes w/64x64 FOV IR @ 640 ms, VIS @ 40000 ms; Time: 7.0 hr 47 min; Volume: 86.5 Mbits; CompRatio: 2.0

Turn to waypoint: 30 min

Primary: -y to Pleiades; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2005-237T08:52:00,000T01:11:00,25-Aug-05,CAPS,Prime,co-rotation,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-237T10:03:00,000T00:30:00,25-Aug-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 030 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-237T10:53:00,000T11:15:00,25-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-237T10:53:00,000T09:15:00,25-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-237T10:53:00,000T11:15:00,25-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-237T11:08:00,000T09:00:00,25-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-237T20:08:00,000T23:51:00,25-Aug-05,INMS,Non-SPASS,Sun,PTOTM29,MAPS survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-237T22:08:00,000T02:25:00,25-Aug-05,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-237T22:08:00,000T10:45:00,25-Aug-05,CAPS,SPASS Rider,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-237T22:08:00,000T10:45:00,25-Aug-05,MAG,Non-SPASS,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-237T22:08:00,000T22:00:00,25-Aug-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-238T00:33:00,000T08:00:00,26-Aug-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,Ring FP3/FP4 during F Ring monitoring,6:40 integration on the main rings,,,,,, 2005-238T00:33:00,000T08:00:00,26-Aug-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring imaging on each ansa,One WAC each ansa repeated every 2 hours; 4 times,,,,,, 2005-238T00:33:00,000T08:00:00,26-Aug-05,UVIS,SPASS Rider,rings(general),FMONITOR,F ring monitor,,UV spectral mapping of Saturn's rings.,,,,,, 2005-238T00:33:00,000T08:00:00,26-Aug-05,VIMS,SPASS Rider,rings(general),FMONITOR,F ring monitor,Ring images during CIRS FP3 ring integrations,64x64 images riding with CIRS F ring study. Target TBD. IR exposure time = 640 ms; Frame duration = 48 min. VIS on.,,,,,, 2005-238T08:53:00,000T11:15:00,26-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-238T08:53:00,000T11:15:00,26-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-238T10:59:00,000T09:00:00,26-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-238T19:59:00,000T15:54:00,26-Aug-05,INMS,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-238T20:08:00,000T15:45:00,26-Aug-05,CAPS,SPASS Rider,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-238T20:08:00,000T15:45:00,26-Aug-05,MAG,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-238T20:08:00,001T01:00:00,26-Aug-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-238T20:33:00,000T06:00:00,26-Aug-05,CAPS,Prime,co-rotation,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-239T02:33:00,000T08:00:00,27-Aug-05,CIRS,Prime,rings(general),FMONITOR,F ring monitor,Ring FP3/FP4 during F Ring monitoring,6:40 integration on the main rings,,,,,, 2005-239T02:33:00,000T08:00:00,27-Aug-05,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring imaging on each ansa,One WAC each ansa repeated every 2 hours; 4 times,,,,,, 2005-239T02:33:00,000T08:00:00,27-Aug-05,UVIS,SPASS Rider,rings(general),FMONITOR,F ring monitor,,UV spectral mapping of Saturn's rings.,,,,,, 2005-239T02:33:00,000T08:00:00,27-Aug-05,VIMS,SPASS Rider,rings(general),FMONITOR,F ring monitor,Ring images during CIRS FP3 ring integrations,64x64 images riding with CIRS F ring study. Target TBD. IR exposure time = 640 ms; Frame duration = 48 min. VIS on.,,,,,, 2005-239T11:22:00,000T09:00:00,27-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-239T11:53:00,000T09:15:00,27-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-239T11:53:00,000T09:15:00,27-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-239T11:53:00,000T09:15:00,27-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-239T12:13:00,000T03:00:00,27-Aug-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-239T21:08:00,000T14:45:00,27-Aug-05,CAPS,SPASS Rider,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-239T21:08:00,000T14:30:16,27-Aug-05,INMS,Non-SPASS,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-239T21:08:00,000T14:45:00,27-Aug-05,MAG,Non-SPASS,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-239T21:08:00,000T15:38:08,27-Aug-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-239T22:28:00,000T00:30:00,27-Aug-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 037 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-239T22:58:00,000T04:30:00,27-Aug-05,VIMS,Prime,Star,FOMALHAUT,Fomalhaut,Fomalhaut calibration,"Turn to Fomalhaut; Time: 30 min

Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 3 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2005-240T03:28:00,000T01:15:00,28-Aug-05,VIMS,Prime,Star,BETPEGCAL,Beta Peg calibration,Beta Peg calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 60 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2005-240T04:43:00,000T01:15:00,28-Aug-05,VIMS,Prime,Star,TCEPCAL,T Cephei calibration,T Cephei calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 60 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2005-240T05:58:00,000T01:15:00,28-Aug-05,VIMS,Prime,Star,RLYRCAL,R Lyrae calibration,R Lyrae calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 60 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2005-240T07:13:00,000T00:45:00,28-Aug-05,VIMS,Prime,Star,ALPHERCAL,Alpha Her calibration,Alpha Her calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; Time: 15 min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 15 min Not time critical. RWA REQUIRED.,,,,,, 2005-240T07:58:00,000T01:25:00,28-Aug-05,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-240T09:23:00,000T00:30:00,28-Aug-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 038 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-240T09:47:00,000T11:25:00,28-Aug-05,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operational Readiness Test (ORT). Pointing=XBAND to Earth. Last 9.5 hours required to be tracked by DSS-14, DSS-25, DSS-26, and DSS-55. An RSS Boresight Calibration activity will also be done, from 14:52 to 15:52 (see request RSS_014EA_BORESIGHT001_PRIME), during which telemetry will be turned off.",,,,,, 2005-240T11:38:16,000T08:21:52,28-Aug-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-240T11:38:16,000T08:21:52,28-Aug-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-240T11:38:16,001T00:00:00,28-Aug-05,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2005-240T11:53:00,000T09:15:00,28-Aug-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-240T11:53:00,000T09:15:00,28-Aug-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-240T11:53:00,000T00:54:12,28-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2005-240T12:01:24,000T00:00:01,28-Aug-05,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse per = 16.0 d, inc = 15.8 deg, r = 37.8 Rs, phase = 75 deg",,,,,, 2005-240T12:47:12,000T08:20:48,28-Aug-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-240T12:50:00,002T08:52:59,28-Aug-05,CDA,Non-SPASS,DustRAM direction,1704DUST,Dust survey,Dust survey 3.86Arcturus: multiple sets of 10 cubes w/64x4 FOV IR @ 160 ms, VIS @ 10160 ms; Time: 8.0 hr; Volume: 125 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Arcturus; Secondary: +z to TBD",,,,,, 2005-245T08:08:00,000T00:30:00,2-Sep-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 014 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-245T09:30:08,000T09:22:00,2-Sep-05,INMS,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-245T10:38:00,000T09:22:00,2-Sep-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-245T10:38:00,000T09:22:00,2-Sep-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-245T10:38:00,000T09:22:00,2-Sep-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-245T11:00:00,000T09:00:00,2-Sep-05,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operational Readiness Test (ORT). Pointing=XBAND to Earth. Last 10.5 hours required to be tracked by DSS-14, DSS-25, DSS-26, DSS-63, and DSS-55.",,,,,, 2005-245T11:30:00,000T03:00:00,2-Sep-05,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,Deep Space Cal,Deep space observation for calibration,,,,,, 2005-245T13:00:00,000T01:28:00,2-Sep-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-245T18:52:08,001T01:37:52,2-Sep-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-245T20:00:00,000T03:25:00,2-Sep-05,CAPS,SPASS Rider,co-rotation,MAGBNDORS,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances. Ridealong with ORS",,,,,, 2005-245T20:00:00,000T00:35:00,2-Sep-05,CIRS,SPASS Rider,Enceladus,OPNAV,Optical navigation image,,Deep space obervations for calibration during OPNAV slews,,,,,, 2005-245T20:00:00,000T01:25:00,2-Sep-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). Data is in addition to magbound rate.,,,,,, 2005-245T20:00:00,001T23:30:00,2-Sep-05,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,add data rate,dust survey measurements,,,,,, 2005-245T20:00:00,001T00:10:00,2-Sep-05,MAG,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances. (Alternate_MB_A),,,,,, 2005-245T20:00:00,001T13:55:00,2-Sep-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-245T20:00:01,000T03:25:00,2-Sep-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-245T20:35:00,000T00:15:00,2-Sep-05,CIRS,SPASS Rider,Rhea,OPNAV,Optical navigation image,FP3_High_Res,"Rider OPNAV of Rhea; AD=0.83 mrad, Phase=70; LT=07; subS/C=(-5,313). Would like OPNAV image as Support Image.",,,,,, 2005-245T20:50:00,000T00:15:00,2-Sep-05,CIRS,SPASS Rider,Dione,OPNAV,Optical navigation image,FP3_High_Res,"Rider OPNAV of Dione; AD=0.94 mrad, Phase=51; LT=09; subS/C=(-8,165). Would like OPNAV image as Support Image.",,,,,, 2005-245T21:05:00,000T00:15:00,2-Sep-05,CIRS,SPASS Rider,Mimas,OPNAV,Optical navigation image,FP3_High_Res,"Rider OPNAV of Mimas; AD=0.31 mrad, Phase=56; LT=08; subS/C=(-6,187). Would like OPNAV image as Support Image.",,,,,, 2005-245T21:20:00,000T00:40:00,2-Sep-05,CIRS,SPASS Rider,Tethys,OPNAV,Optical navigation image,FP3_High_Res,"Rider OPNAV of Tethys; AD=0.59 mrad, Phase=60; LT=08; subS/C=(-5,333). Would like OPNAV image as Support Image.",,,,,, 2005-245T22:00:00,000T07:00:00,2-Sep-05,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,latitude-phase coverage: 3x1 mosaic on each ansa,"Orbits = 014-014, Cube Size (X,Z) = 64*64 hires, Time per SC pointing (mins) = 30, Number of SC pointings = 12, Time of observation (hours) = 6.0, Volume (Mbits) = 416, Desc = Obtain 6x1 mosaic on each ring ansa on sunlit face. Orient Z-axis parallel to Saturn's pole. Distance 20 R_S. * backup for R 6",,,,,, 2005-245T22:00:00,000T07:00:00,2-Sep-05,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_014RI_Latphase_SI,Rider on Latphase,,,,,, 2005-245T22:00:00,000T07:00:00,2-Sep-05,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_VIMS Rider,Ride along with ISS observation,,,,,, 2005-245T22:00:00,000T07:00:00,2-Sep-05,ISS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,Rev 14 VIMS rider,TWT RINGS Range 25.37 to 23.74 B -6.08 to -6.26 Phase (start) 52.22-57.13 Phase (end) 49.94-55.19,,,,,, 2005-245T22:00:00,000T07:00:00,2-Sep-05,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,UV Spectroscopy of Rings - Rider,UV solar reflectance spectroscopy of Saturn's rings. Rider to VIMS_LATPHASE.,,,,,, 2005-245T23:25:00,001T20:10:00,2-Sep-05,CAPS,Non-SPASS,Saturn,4KSURVEY,MAPS survey,MAPS Survey,MAPS magnetospheric survey. Note that pointing during this period will not be good. The extra bits here are really to get higher resolution data in the electrons (ELS).,,,,,, 2005-245T23:25:00,000T01:42:24,2-Sep-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 24 B cycles duration. Data is in addition to 4000 bps from magbound.,,,,,, 2005-245T23:25:00,002T00:45:00,2-Sep-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-246T01:30:00,000T03:30:00,3-Sep-05,RADAR,SPASS Rider,Other,WARMPO08R,RADAR warmup,Prioritized Ring Observation Number 8,Warmup for ring prioritized observation.,,,,,, 2005-246T05:00:00,000T06:00:00,3-Sep-05,RADAR,Prime,rings(general),PO8RINGS,Ring observation,Prioritized Ring Observation Number 8,Image rings via radiometry at low inclination and low resolution.,,,,,, 2005-246T20:10:00,000T03:50:00,3-Sep-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-246T20:30:00,000T00:30:00,3-Sep-05,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,Deep Space Cal,Deep space observation for calibration during turns,,,,,, 2005-246T20:30:00,000T08:40:00,3-Sep-05,INMS,Non-SPASS,Saturn,PTOTM31,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-246T21:00:00,000T07:00:00,3-Sep-05,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,latitude-phase coverage: 3x1 mosaic on each ansa,"Orbits = 014-014, Cube Size (X,Z) = 64*64 hires, Time per SC pointing (mins) = 30, Number of SC pointings = 12, Time of observation (hours) = 6.0, Volume (Mbits) = 416, Desc = Obtain 6x1 mosaic on each ring ansa on sunlit face. Orient Z-axis parallel to Saturn's pole. Distance 20 R_S. * backup for R 6",,,,,, 2005-246T21:00:00,000T07:00:00,3-Sep-05,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_014RI_Latphase_SI,Rider on Latphase,,,,,, 2005-246T21:00:00,000T07:00:00,3-Sep-05,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_VIMS Rider,Ride along with VIMS observation,,,,,, 2005-246T21:00:00,000T07:00:00,3-Sep-05,ISS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,Rev 14 VIMS rider (2nd occurrence),TWT RINGS Range 19.40 to 17.17 B -6.73 to -6.97 Phase (start) 43.15-49.53 Phase (end) 39.00-46.17,,,,,, 2005-246T21:00:00,000T07:00:00,3-Sep-05,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,UV Spectroscopy of Rings - Rider,UV solar reflectance spectroscopy of Saturn's rings. Rider to VIMS_LATPHASE.,,,,,, 2005-247T00:00:00,000T03:00:00,4-Sep-05,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required.",,,,,, 2005-247T03:00:00,000T21:10:00,4-Sep-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-247T04:00:00,000T06:00:00,4-Sep-05,CIRS,Prime,rings(general),TEMPL15LP,Thermal map,CIRS_014RI_TempL15LP,"Afternoon radial scan of main rings to obtain thermal measurement of rings. CIRS_FP1 to Saturn, POS_Z to POL_DIR",,,,,, 2005-247T04:00:00,000T06:00:00,4-Sep-05,CIRS,SPASS Rider,rings(general),TEMPL15LP,Thermal map,CIRS_014RI_TEMPL15_SI,Rider on Latphase,,,,,, 2005-247T04:00:00,000T06:00:00,4-Sep-05,UVIS,SPASS Rider,rings(general),TEMPL15LP,Thermal map,UV Spectroscopy of Rings - Rider,UV solar reflectance spectroscopy of Saturn's rings. Rider to CIRS_014RI_SUBML07LP001_PRIME,,,,,, 2005-247T05:10:00,000T14:20:00,4-Sep-05,INMS,Non-SPASS,Saturn,FULLSURV,MAPS magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-247T09:50:00,000T15:54:00,4-Sep-05,CDA,Non-SPASS,DustRAM direction,DOWNLK002,,Dust survey outside 8 Rs 7.0070 deg from dust ram.",,,,,, 2005-248T09:40:00,000T02:00:00,5-Sep-05,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 014RI PRE-OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band. This commences 2.5 hours prior to ring INGRESS.,,,,,, 2005-248T10:03:32,000T00:12:06,5-Sep-05,CDA,Non-SPASS,RingE,0304ERNGX,Ring plane crossing,E Ring Xing 4.0070 deg from dust ram.",,,,,, 2005-266T10:33:40,000T01:12:29,23-Sep-05,CDA,Non-SPASS,DustRAM direction,0700DUST,Dust survey,E Ring dense - survey - 0.17AD>20 mrad; (-2, 75)-(-2, 139); 75LT>0400.... Confusion here: I assume we are picking up from last UVIS observation (on Tethys) - the waypoint is Saturn, and I do not know the turn times.... A) FP1 Nyquist box mosaic of disk (31.2 mrad, 17 scans) = 34.4 min. CIRS at 15.5 cm-1 resolution (4.75 sec/frame); blink - shutter closed final 5 min.....B) Displace FP3 +7 mrad in Z, -12 mrad in X; drift in +X at 15.7 microradians/sec for 25 min (23.5 mrad). CIRS at 15.5 cm-1 resolution (4.75 sec/frame); blink..... C) FP1 Nyquist box mosaic of disk (23.4 mrad, 13 scans) = 22.0 min. CIRS at 15.5 cm-1 resolution (4.75 sec/frame); blink - shutter closed first 5 min. To waypoint at Saturn??? (I have left no time for waypoint turns....)",,,,,, 2005-267T03:30:00,000T00:57:00,24-Sep-05,ISS,SPASS Rider,Tethys,FP1FP3MAP,CIRS FP1 integration / FP3 map,TETHYS NAC COLOR AND STEREO,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-267T03:30:00,000T00:57:00,24-Sep-05,UVIS,SPASS Rider,Tethys,ICYMAP,Icy satellite surface map,ICYMAP,,,,,,, 2005-267T04:07:48,000T00:30:00,24-Sep-05,CDA,Non-SPASS,Dione,0600DIORX,Dione orbit crossing,Dione Orbit Xing 0.00Reaction Wheels Required",,,,,, 2005-268T15:10:46,000T02:09:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERIONV,Hyperion observation,Hyperion VIMS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T15:10:46,000T02:09:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-268T16:19:46,000T01:40:00,25-Sep-05,RSS,SPASS Rider,Hyperion,THERMAL,Thermal stabilization period,RSS Hyperion Mass Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band. Turn starts at -8 hours 25 minutes.,,,,,, 2005-268T16:38:26,000T00:37:34,25-Sep-05,CDA,Non-SPASS,DustRAM direction,2100DUST,Dust survey,Dust survey 0.17Reaction Wheels Required",,,,,, 2005-268T17:30:46,000T00:29:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERIONV,Hyperion observation,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T17:30:46,000T00:29:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-268T17:59:46,000T02:20:00,25-Sep-05,RSS,Prime,Hyperion,MASS,,RSS Hyperion Mass Determination,"We agreed within the SOST that RSS will track the spacecraft from -8 to -6 hours and from +2 to +4 hours. This is the request for the first segment. The HGA must be pointed toward Earth. We expect to have Ka-band downlink capabilities at all the complexes, so we will use at least X-X and X-Ka, and Ka-Ka if possible. We will get Doppler and ranging data. The use of Ka-band requires two hours of thermal stabilization, during which other instruments can control the pointing. The attitude of the spacecraft must be controled by the reaction wheels from the beginning of the first RSS segment to the end of the second RSS segment. The requirement for a quiet spacecraft is to be determined after analysis of the Quiet Test in late 2001.",,,,,, 2005-268T19:37:00,000T07:49:00,25-Sep-05,CDA,Non-SPASS,Hyperion,HYPDUST,Hyperion dust study,Dust envelope around Hyperion,Study dust envelope around Hyperion. pointing: CDA boresight to dust RAM power: 19 W (with articulation),,,,,, 2005-268T20:19:46,000T00:11:00,25-Sep-05,ISS,Prime,Hyperion,COLORF,Color image,HYPERION Color,NP09,,,,,, 2005-268T20:19:46,000T00:11:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERION,Hyperion,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T20:19:46,000T00:11:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T20:19:46,000T00:11:00,25-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,12x12 ISS r/a <~11 frames. Time with ISS frames,,,,,, 2005-268T20:30:46,000T00:50:00,25-Sep-05,VIMS,Prime,Hyperion,HYPERION,Hyperion,Hyperion,"vis and IR hi-res 16 x 16. 640 and 160 IR int time, 15 cyclics

Reaction Wheels Required",,,,,, 2005-268T20:30:46,000T00:50:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERIONV,Hyperion observation,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T20:30:46,000T00:50:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T21:20:46,000T00:01:45,25-Sep-05,ISS,Prime,Hyperion,ROTOBS,Satellite rotation observation,HYPERION Rotation Monitor,GRN+NP09,,,,,, 2005-268T21:20:46,000T00:11:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERION,Hyperion,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T21:20:46,000T00:11:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T21:22:31,000T00:09:15,25-Sep-05,ISS,Prime,Hyperion,COLORF,Color image,HYPERION Color,NP09,,,,,, 2005-268T21:31:46,000T00:23:00,25-Sep-05,VIMS,Prime,Hyperion,HYPERION,Hyperion,Hyperion,"vis and IR hi-res 16 x 16. 320 IR int time, 30 cyclics

Reaction Wheels Required",,,,,, 2005-268T21:31:46,000T00:23:00,25-Sep-05,ISS,SPASS Rider,Hyperion,HYPERION,Hyperion,HYPERION Color: VIMS rider,NP09,,,,,, 2005-268T21:31:46,000T00:23:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T21:54:46,000T00:06:00,25-Sep-05,ISS,Prime,Hyperion,COLORF,Color image,HYPERION Color,NP09,,,,,, 2005-268T21:54:46,000T00:06:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T21:54:46,000T00:06:00,25-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,12x12 hi res 320ms IR Time with ISS frames,,,,,, 2005-268T22:20:46,000T01:00:00,25-Sep-05,CIRS,Prime,Hyperion,FP3GLOBAL,CIRS FP3 global map,Global_FP3_map,"4.5.lt.AD.lt.5.6 mrad; (-35, 317); phase=51; LT~1520. From center of disk, displace FP3 5 mrad in +X, 1 mrad in +Z. Drift 10 mrad in -X at 7.8 microradians/sec (21.4 min). CIRS at 15.5 cm-1 resolution (4.75 sec/frame); blink, with shutter closed first 2 min. Drop FP3 2 mrad in -Z; drift 10 mrad in +X at 7.8 microradians/sec (21.4 min). FP3 to disk center (10 min). Return to waypoint.",,,,,, 2005-268T22:20:46,000T01:00:00,25-Sep-05,ISS,SPASS Rider,Hyperion,FP3GLOBAL,CIRS FP3 global map,CIRS Rider,NP09,,,,,, 2005-268T22:20:46,000T01:00:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T22:20:46,000T01:00:00,25-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,12 x12 hi res IR ISS r/a 40,,,,,, 2005-268T23:20:46,000T00:20:00,25-Sep-05,ISS,Prime,Hyperion,ROTOBS,Satellite rotation observation,HYPERION Rotation Monitor,"Multiple passes on NAC GRN, NAC COLOR, on NAC Polarization filters",,,,,, 2005-268T23:20:46,000T00:20:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERION,Hyperion,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T23:20:46,000T00:20:00,25-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-268T23:20:46,000T00:20:00,25-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,12x12 ISS r/a 15 frames. Time with ISS frames. 320ms,,,,,, 2005-268T23:40:46,000T00:59:00,25-Sep-05,UVIS,Prime,Hyperion,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map of Hyperion,UV albedo map of Hyperion's surface plus limb drifts. Two continuous slow slews to build north-south mosaic. Offset the scans by 3 mrad for CIRS in the z direction. The midline between the two scans should pass through the fattest part of the lit crescent.,,,,,, 2005-268T23:40:46,000T00:59:00,25-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERIONU,Hyperion observation,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-268T23:40:46,000T00:59:00,25-Sep-05,ISS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,HYPERION NAC UVIS Rider,NP09,,,,,, 2005-268T23:40:46,000T00:59:00,25-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,32x32 2 frames. hi res vis/IR. 640ms. then 1 frame at 80ms,,,,,, 2005-269T00:24:46,000T04:00:00,26-Sep-05,MAG,Non-SPASS,Hyperion,HYTAR,Hyperion targeted flyby,Hyperion targeted flyby,Monitor the interaction of Hyperion with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field. NOTE: - rate assumes continous 600bps survey will be added to make up the total rate (total data rate is 1976 bps),,,,,, 2005-269T00:39:46,000T00:30:00,26-Sep-05,ISS,Prime,Hyperion,MORPHO,Morphology,HYPERION Morphology,"GRN NAC, 2x2's; 1x2xN09, 3x4xGRN",,,,,, 2005-269T00:39:46,000T00:30:00,26-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERION,Hyperion,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-269T00:39:46,000T00:30:00,26-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-269T00:39:46,000T00:30:00,26-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,12x12 ISS r/a 25 frames. Time with ISS frames. 320ms 12 x 12 hi res IR,,,,,, 2005-269T01:09:46,000T00:20:00,26-Sep-05,CIRS,Prime,Hyperion,FP1GREEN,CIRS FP1 greenhouse search,Hyperion FP1 greenhouse search,"14AD>42 mrad; (43, 141); phase=119; LT~0300. Make FP1 Nyquist box mosaic (13.7 mrad x 13.7 mrad, 8 scans) of center of early morning hemisphere (10.1 min). Will use data from following UVIS scan for calibration. CIRS at 15.5 cm-1 resolution (4.75 sec/frame). NOTE: ""31 MIN TURN; START TRACKING AT HY+00:25"" Per: Date: Fri, 29 Apr 2005 12:40:16 -0700 To: sost@dcs04.jpl.nasa.gov From: Amanda Hendrix Subject: SOST: 015HY CCR",,,,,, 2005-269T02:18:46,000T01:00:00,26-Sep-05,ISS,SPASS Rider,Hyperion,FP1DSKOUT,CIRS FP1 outbound disk map,HYPERION Color,N05 color,,,,,, 2005-269T02:18:46,000T01:00:00,26-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-269T02:18:46,000T01:00:00,26-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,12 x12 hi res IR 50 reps,,,,,, 2005-269T02:34:46,000T01:35:30,26-Sep-05,RSS,SPASS Rider,Hyperion,THERMAL,Thermal stabilization period,RSS Hyperion Mass Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band. We need a unique sequence to have the reaction wheels in full motion. The turn starts at 1:50.,,,,,, 2005-269T02:39:46,000T01:00:00,26-Sep-05,INMS,Non-SPASS,Hyperion,ICYSATOB,Icy satellite imaging,SOST,Measurements of magnetospheric/exopspheric interaction and determination of surface composition.,,,,,, 2005-269T02:54:46,000T17:07:39,26-Sep-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-269T02:54:46,000T17:08:49,26-Sep-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-269T02:54:46,000T17:08:49,26-Sep-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-269T03:18:46,000T00:51:30,26-Sep-05,UVIS,Prime,Hyperion,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map of Hyperion,"UV albedo map of Hyperion's surface plus limb drifts. Continuous slew north-south mosaic with two scans, midline between the two scans passing through the fattest part of the illuminated crescent, offset by 3 mrad from each other for CIRS.",,,,,, 2005-269T03:18:46,000T00:51:30,26-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERIONU,Hyperion observation,Hyperion CIRS Rider,CIRS coverage of morning hemisphere.,,,,,, 2005-269T03:18:46,000T00:51:30,26-Sep-05,ISS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,HYPERION Color,N05 color,,,,,, 2005-269T03:18:46,000T00:51:30,26-Sep-05,VIMS,SPASS Rider,Hyperion,HYPERIONC,Hyperion observation,Hyperion,32x32 2 frames. hi res vis/IR. 640ms. then 1 frame at 80ms,,,,,, 2005-269T03:26:00,000T01:49:00,26-Sep-05,CDA,Non-SPASS,Hyperion,DUST,Dust survey,study of Hyperion dust environment,"Study dust in the vincinity of Hyperion. Ride along with RSS. Secondary axis: -x = (ra: 223.2, dec: 6.6). Power: 11 W. Data rate: 200 bps.",,,,,, 2005-269T03:39:46,000T10:53:49,26-Sep-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-269T04:10:16,000T01:45:00,26-Sep-05,RSS,Prime,Hyperion,MASS,,RSS Hyperion Mass Determination,"We agreed within the SOST that RSS will track the spacecraft from -8 to -6 hours and from +2 to +4 hours. This is the request for the second segment. The HGA must be pointed toward Earth. We expect to have Ka-band downlink capabilities at all the complexes, so we will use at least X-X and X-Ka, and Ka-Ka if possible. We will get Doppler and ranging data. The use of Ka-band requires two hours of thermal stabilization, during which other instruments can control the pointing. The attitude of the spacecraft must be controled by the reaction wheels from the beginning of the first RSS segment to the end of the second RSS segment. The requirement for a quiet spacecraft is to be determined after analysis of the Quiet Test in late 2001.",,,,,, 2005-269T04:24:46,000T14:55:14,26-Sep-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-269T05:15:01,000T14:04:54,26-Sep-05,CDA,Non-SPASS,DustRAM direction,GAP,,Dust survey,"Dust survey $ 452.34785 $ 458.95858 $ 24.777 to 41.172 Rs lat: -0.194 to -0.277 deg ring-alt: 5061. to 12009.km,pointing=CDA to Kepler RAM,rate=150,dataVolume=81.705",,,,,, 2005-269T05:55:16,000T03:01:46,26-Sep-05,RADAR,Prime,Hyperion,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Hyperion.,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2005-269T08:35:00,000T10:45:00,26-Sep-05,RSS,SPASS Rider,Hyperion,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band for Hyperion mass.,,,,,, 2005-269T08:57:02,000T01:25:51,26-Sep-05,VIMS,Prime,Hyperion,HYPERION,Hyperion,Hyperion,"vis and IR hi-res 16 x 16. 640ms and 160ms IR int time, 30 cyclics revisit the integration times and data vol (do we need a short time) -RNC 4/2/2002

Reaction Wheels Required",,,,,, 2005-269T08:57:02,000T01:25:51,26-Sep-05,CIRS,SPASS Rider,Hyperion,HYPERIONV,Hyperion observation,Hyperion CIRS Rider on VIMS,CIRS coverage of afternoon hemisphere.,,,,,, 2005-269T08:57:02,000T01:25:51,26-Sep-05,ISS,SPASS Rider,Hyperion,HYPERION,Hyperion,HYPERION Color,N05 color,,,,,, 2005-269T08:57:02,000T01:25:51,26-Sep-05,UVIS,SPASS Rider,Hyperion,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Hyperion, ORS Rider",UV albedo map of Hyperion's surface plus limb drifts,,,,,, 2005-269T14:33:34,002T04:37:26,26-Sep-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-269T19:20:00,001T00:05:00,26-Sep-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-269T19:20:00,006T03:40:20,26-Sep-05,CDA,Non-SPASS,DustRAM direction,2500DUST,Dust survey,Dust survey 0.19Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2005-271T10:11:00,000T09:15:00,28-Sep-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-271T11:00:00,000T06:00:00,28-Sep-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL,Deep space calibration,CIRS Deep Space Calibration,CIRS Deep Space Calibration,,,,,, 2005-271T19:11:00,000T21:15:00,28-Sep-05,INMS,Non-SPASS,co-rotation,PTOTM35,MAPS survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-271T19:26:00,000T12:00:00,28-Sep-05,CAPS,SPASS Rider,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-271T19:26:00,000T22:15:00,28-Sep-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-271T19:26:00,000T12:00:00,28-Sep-05,UVIS,SPASS Rider,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,UVIS MAPS Ride-Along,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-271T19:26:00,000T12:00:00,28-Sep-05,MAG,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-271T19:26:00,000T22:15:00,28-Sep-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-271T19:46:00,000T08:00:00,28-Sep-05,CIRS,Prime,rings(general),FP34INTEG,CIRS FP3 / FP4 integration,CIRS_015RI_F34INTEG_PRIME,FP3/4 integration on main rings,,,,,, 2005-271T19:46:00,000T08:00:00,28-Sep-05,CIRS,SPASS Rider,rings(general),FP34INTEG,CIRS FP3 / FP4 integration,CIRS_015RI_FP34INTEG001_SI,Support image for FP3/4 integration on main rings.,,,,,, 2005-272T03:46:00,000T04:14:00,29-Sep-05,CAPS,Prime,co-rotation,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T03:46:00,000T04:14:00,29-Sep-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-272T07:26:00,000T10:15:00,29-Sep-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T07:26:00,000T10:15:00,29-Sep-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-272T10:00:00,000T09:00:00,29-Sep-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-272T16:26:00,000T02:34:00,29-Sep-05,INMS,Non-SPASS,co-rotation,PTOTM35,MAPS survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T17:41:00,000T16:00:00,29-Sep-05,CAPS,SPASS Rider,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T17:41:00,003T05:52:00,29-Sep-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-272T17:41:00,000T16:00:00,29-Sep-05,MAG,Non-SPASS,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-272T17:41:00,001T01:45:00,29-Sep-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T19:00:00,000T14:41:00,29-Sep-05,UVIS,SPASS Rider,Sun,MAGBNDCOR,MAPS magnetosphere boundary campaign,UVIS MAPS Ride-Along,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-272T19:00:00,001T00:26:00,29-Sep-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T19:41:00,000T00:30:00,29-Sep-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 033 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-272T20:11:00,000T12:40:00,29-Sep-05,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-272T20:20:00,000T02:42:08,29-Sep-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-273T08:51:00,000T00:30:00,30-Sep-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 034 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-273T09:41:00,000T09:45:00,30-Sep-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-273T09:41:00,000T09:45:00,30-Sep-05,MAG,Non-SPASS,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-273T09:56:00,000T10:15:00,30-Sep-05,UVIS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,UVIS MAPS Ride-Along,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-273T19:26:00,005T23:16:00,30-Sep-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-273T19:26:00,000T21:45:00,30-Sep-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-273T19:26:00,002T04:07:00,30-Sep-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-273T19:26:00,002T03:50:08,30-Sep-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-273T20:26:00,000T00:40:00,30-Sep-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-273T20:26:00,000T00:40:00,30-Sep-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-273T21:06:00,000T00:30:00,30-Sep-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 036 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-273T22:34:00,000T00:40:00,30-Sep-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-273T22:34:00,000T00:40:00,30-Sep-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-274T00:42:00,000T00:40:00,1-Oct-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-274T00:42:00,000T00:40:00,1-Oct-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-274T02:50:00,000T00:40:00,1-Oct-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-274T02:50:00,000T00:40:00,1-Oct-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-274T03:30:00,000T00:30:00,1-Oct-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 037 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-274T04:58:00,000T00:40:00,1-Oct-05,ISS,Prime,Saturn,1X6MOVIEA,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-274T04:58:00,000T00:40:00,1-Oct-05,VIMS,SPASS Rider,Saturn,1X6MOVIEA,Saturn movie,ISS 1X6 Movie Ride Along,ISS Movie Ride Along,,,,,, 2005-274T08:11:00,000T09:00:00,1-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-274T09:15:00,000T06:00:00,1-Oct-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL,Deep space calibration,CIRS Deep Space Calibration,CIRS Deep Space Calibration,,,,,, 2005-274T17:11:00,001T02:49:00,1-Oct-05,INMS,Non-SPASS,Saturn,PTOTM36,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-274T17:46:00,000T00:40:00,1-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-274T18:26:00,000T00:30:00,1-Oct-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 038 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-274T19:54:00,000T00:40:00,1-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-274T22:02:00,000T00:40:00,1-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T00:10:00,000T00:40:00,2-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T00:50:00,000T00:30:00,2-Oct-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 039 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2005-275T02:18:00,000T00:40:00,2-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T04:26:00,000T00:40:00,2-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T06:34:00,000T00:40:00,2-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T08:42:00,000T00:40:00,2-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T11:00:00,000T09:00:00,2-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2005-275T11:45:00,000T06:00:00,2-Oct-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL,Deep space calibration,CIRS Deep Space Calibration,CIRS Deep Space Calibration,,,,,, 2005-275T12:00:00,000T00:34:08,2-Oct-05,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,Calibration/Gain curve of ELS sensor,Calibration/gain curve of ELS sensor. 8 B cycles duration in 16 kbps. Data is in addition to 1000 bps from SWSKR.,,,,,, 2005-275T20:00:00,000T03:07:00,2-Oct-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-275T21:30:00,000T00:40:00,2-Oct-05,ISS,Prime,Saturn,1X6MOVIEB,Saturn movie,NAC Southern Hemisphere Saturn movie,"1x6 mos in two filters plus one extra WAC, repeat every two hours, eight minutes.",,,,,, 2005-275T23:07:00,003T19:35:00,2-Oct-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-275T23:16:08,003T19:25:52,2-Oct-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-275T23:33:00,001T19:36:00,2-Oct-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-275T23:33:00,005T12:56:59,2-Oct-05,CDA,Non-SPASS,DustRAM direction,2500DUST,Dust survey,Dust survey 0.2870 deg from dust ram.",,,,,, 2005-284T15:27:02,000T00:15:00,11-Oct-05,CIRS,Prime,Dione,FP3DISCSC,CIRS FP3 disk map,Dione disk scan,"AD=15 mrad, phase=23, (-1, 165). Perform 4 mrad FP3,4 scan in X, centered on subsolar point, at 4 microrad/sec. CIRS at 15.5 cm-1 resolution.",,,,,, 2005-284T15:27:02,000T00:15:00,11-Oct-05,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,"40x40 lrlr 160ms, 320 ms (15 min)",,,,,, 2005-284T15:40:23,000T01:13:11,11-Oct-05,CDA,Non-SPASS,DustRAM direction,0700DUST,Dust survey,E Ring dense - survey - 0.1770 deg from dust ram.",,,,,, 2005-284T18:22:02,001T01:13:17,11-Oct-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-284T18:28:14,000T00:52:56,11-Oct-05,CDA,Non-SPASS,DustRAM direction,0600DUST,Dust survey,E Ring dense - survey - 0.11Pleiades: multiple cubes w/64x64 FOV IR @ 640 ms, VIS @ 40000 ms; Time: 7.0 hr 47 min; Volume: 86.5 Mbits; CompRatio: 2.0

Turn to waypoint: 30 min

Primary: -y to Pleiades; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2005-295T12:29:00,000T09:17:00,22-Oct-05,CDA,SPASS Rider,Other,DECON,Decontamination,Decontamination,"Pointing:CDA's boresight off-sun, no additional power resources (Watts) (covered by other requests)",,,,,, 2005-295T12:40:00,000T02:16:32,22-Oct-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-295T21:46:00,000T01:40:00,22-Oct-05,ISS,Prime,Star,MONITOR,,ISS Sensitivity monitor,Periodic standard star image to monitor ISS sensitivity. Scan along Z direction and 2X2 mosaoc,,,,,, 2005-295T23:26:00,000T02:00:00,22-Oct-05,UVIS,Prime,Star,ALPVIR,Alpha Virginis occultation,USTRCAL02,INSTANCE OF USTRCAL02. Stellar Calibration: alpha Virginis & HSP darck current measurement.,,,,,, 2005-296T01:26:00,000T06:58:00,23-Oct-05,VIMS,Prime,RingE,E60PHASE,E ring observation,E Ring near phase 60,"Orbits = 015-019, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 180, Time of observation (hours) = 20, Volume (Mbits) = 289, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturn's pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 5 at Priority 1; also any 1 of 5 at Priority 2; can be split",,,,,, 2005-296T01:26:00,000T06:58:00,23-Oct-05,CIRS,SPASS Rider,RingE,E60PHASE,E ring observation,,VIMS rider,,,,,, 2005-296T08:59:00,002T01:14:59,23-Oct-05,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addings due to SAP,datavol adjust,,,,,, 2005-296T08:59:00,000T08:55:00,23-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-296T10:00:00,000T06:00:00,23-Oct-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-296T18:00:00,000T02:16:32,23-Oct-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-296T18:29:00,000T13:55:00,23-Oct-05,VIMS,Prime,RingE,E60PHASE,E ring observation,E Ring near phase 60,"Orbits = 015-019, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 180, Time of observation (hours) = 20, Volume (Mbits) = 289, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturn's pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 5 at Priority 1; also any 1 of 5 at Priority 2; can be split",,,,,, 2005-296T18:29:00,000T13:55:00,23-Oct-05,CIRS,SPASS Rider,RingE,E60PHASE,E ring observation,,VIMS rider,,,,,, 2005-296T18:29:00,000T13:55:00,23-Oct-05,ISS,SPASS Rider,RingE,E60PHASE,E ring observation,RIDE ALONG E RING OBSERVATIONS,RIDE ALONG E RING OBSERVATIONS,,,,,, 2005-297T08:59:00,000T08:55:00,24-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-297T09:30:00,000T02:16:32,24-Oct-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-297T10:00:00,000T06:00:00,24-Oct-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-297T18:29:00,000T03:00:00,24-Oct-05,VIMS,Prime,RingE,E60PHASE,E ring observation,E Ring near phase 60,"Orbits = 015-019, Cube Size (X,Z) = 32*12, Time per SC pointing (mins) = 7, Number of SC pointings = 180, Time of observation (hours) = 20, Volume (Mbits) = 289, Desc = Stare at core of E ring from 30-40 R_S to build up spectra at different phase angles. Orient X-axis parallel to Saturn's pole to measure vertical ring profile. Observations at each phase angle need NOT be contiguous. 32x12; 1 sec exp; do any 1 of 5 at Priority 1; also any 1 of 5 at Priority 2; can be split",,,,,, 2005-297T18:29:00,000T03:00:00,24-Oct-05,CIRS,SPASS Rider,RingE,E60PHASE,E ring observation,,VIMS rider,,,,,, 2005-297T18:29:00,000T03:00:00,24-Oct-05,ISS,SPASS Rider,RingE,E60PHASE,E ring observation,RIDE ALONG E RING OBSERVATIONS,RIDE ALONG E RING OBSERVATIONS,,,,,, 2005-297T20:00:00,000T04:54:00,24-Oct-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2005-297T21:29:00,000T03:00:00,24-Oct-05,VIMS,Prime,RingG,G60PHASE,G ring observation,G Ring near phase 60,12x12; 1 sec exp; do any 1 of 5 at Priority 1; also any 1 of 5 at Priority 2,,,,,, 2005-297T21:29:00,000T03:00:00,24-Oct-05,ISS,SPASS Rider,RingG,G60PHASE,G ring observation,RIDE ALONG G RING OBSERVATIONS,RIDE ALONG G RING OBSERVATIONS,,,,,, 2005-298T01:04:00,000T09:10:00,25-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-298T01:35:00,000T02:16:32,25-Oct-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-298T10:14:00,000T14:25:00,25-Oct-05,CAPS,SPASS Rider,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-298T10:14:00,001T00:00:00,25-Oct-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-298T10:14:00,001T00:00:00,25-Oct-05,INMS,Non-SPASS,co-rotation,PTOTM040,MAPS survey,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-298T10:14:00,001T00:00:00,25-Oct-05,MAG,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances. (Alternate_MB_A),,,,,, 2005-298T10:14:00,001T00:00:00,25-Oct-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-298T12:14:00,000T06:25:00,25-Oct-05,MIMI,Prime,co-rotation,MAGBNDCOR,MAPS magnetosphere boundary campaign,"Magnetospheric Boundary Campaign, Co-rotation","Pointing for MAGBOUNDARY Campaign, Co-rotation attitude",,,,,, 2005-298T12:14:00,000T06:25:00,25-Oct-05,UVIS,SPASS Rider,co-rotation,MAGBNDPTG,MAPS magnetosphere boundary campaign,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-298T18:39:00,000T05:55:00,25-Oct-05,VIMS,Prime,RingG,G60PHASE,G ring observation,G Ring near phase 60,12x12; 1 sec exp; do any 1 of 5 at Priority 1; also any 1 of 5 at Priority 2,,,,,, 2005-299T00:39:00,000T09:35:00,26-Oct-05,CAPS,SPASS Rider,Other,MAGBNDDNL,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-299T01:14:00,000T09:00:00,26-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-299T10:14:00,000T01:42:24,26-Oct-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-299T10:14:00,001T08:15:00,26-Oct-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-299T10:14:00,000T21:15:00,26-Oct-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-299T10:14:00,001T08:15:00,26-Oct-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-299T10:14:00,001T08:15:00,26-Oct-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-299T10:14:00,001T08:15:00,26-Oct-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-299T10:44:00,000T03:40:00,26-Oct-05,VIMS,Prime,RingG,G60PHASE,G ring observation,G Ring near phase 60,12x12; 1 sec exp; do any 1 of 5 at Priority 1; also any 1 of 5 at Priority 2,,,,,, 2005-299T10:44:00,000T03:40:00,26-Oct-05,ISS,SPASS Rider,RingG,G60PHASE,G ring observation,RIDE ALONG G RING OBSERVATIONS,RIDE ALONG G RING OBSERVATIONS,,,,,, 2005-299T14:24:00,000T11:00:00,26-Oct-05,VIMS,Prime,Saturn,GLOBALMAP,Global coverage mapping,SaturnGlobal Track,Saturn Global Map,,,,,, 2005-300T01:24:00,000T07:00:00,27-Oct-05,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,CIRS_017TI_MidIRTempMAP08,"obtain information on the thermal structure of Titan's stratosphere. Slew cross disk at 4 microrad/s. POINTING: -y to Titan, x to pole (negotiable)",,,,,, 2005-300T01:24:00,000T07:00:00,27-Oct-05,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (8 integrations total = 16 frames, 0.5 Mb/frame)",,,,,, 2005-300T01:24:00,000T07:00:00,27-Oct-05,VIMS,SPASS Rider,Titan,MIDIRMAP,Mid infrared thermal map,VIMS_ride VIMS_4854,Ridealong with a CIRS Mid IR nadir Temp map. 64X64 different integration times.,,,,,, 2005-300T06:54:00,000T11:35:00,27-Oct-05,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band for Titan gravity science and for improving locally Cassini orbit.,,,,,, 2005-300T07:29:00,000T02:31:00,27-Oct-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-300T09:19:00,000T09:10:00,27-Oct-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-300T10:00:00,000T06:00:00,27-Oct-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-300T10:00:00,000T06:29:34,27-Oct-05,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2005-300T11:00:00,000T02:00:00,27-Oct-05,CDA,Non-SPASS,Hyperion,2400HYORX,Hyperion orbit crossing,Hyperion Orbit Xing 0.00 2--particle properties, vertical distributions about 6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested",,,,,, 2005-300T20:01:25,000T03:26:00,27-Oct-05,UVIS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,UVIS Rider to VIMS Medium Res Map,Ride along with VIMS MEDRES on Titan,,,,,, 2005-300T23:27:25,000T00:33:00,27-Oct-05,ISS,Prime,Titan,HIGHRESNA,High resolution observartion,High Resolution Imaging,"high-resolution imaging, 50-200 m/px, special targets, emission angles < 45 prefer IR-polarizer (phase 45-110)",,,,,, 2005-300T23:27:25,000T00:33:00,27-Oct-05,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_017TI_FIRNADIRMAP_04,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2005-300T23:27:25,000T00:33:00,27-Oct-05,UVIS,SPASS Rider,Titan,HIGHRESNA,High resolution observartion,UVIS Rider to ISS HIGHRESNA,Ride along with ISS HIRESNA,,,,,, 2005-300T23:27:25,000T00:33:00,27-Oct-05,VIMS,SPASS Rider,Titan,HIRES,High resolution image,VIMS_ride VIMS_4869,"Ridealong with ISS high resolution mapping. 12X12 mosaics, with 1 minute dwell time ideal.",,,,,, 2005-301T00:15:25,000T07:00:00,28-Oct-05,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T8 Flyby,"T 8 is the first close encounter, i.e. 1472 km at CA, upstream of Titan with penetration deep into the magnetic pile-up region of Titan's upstream interaction region. This is adjacent to the ionopause region, if one believes theoretical models, and therefore very diagnostic with regard to physical understanding. If some low shock-like feature occurs at least temporarily this flyby will have a very good chance to see it. Grade 1 priority. NOTE: - continuous data rate of 1976bps (32vps).",,,,,, 2005-301T00:30:25,000T02:02:00,28-Oct-05,RADAR,Prime,Titan,TI8P1RADI,,T8 Inbound Radiometry,Radiometry during the inbound leg of T8.,,,,,, 2005-301T02:15:25,000T01:00:00,28-Oct-05,CAPS,SPASS Rider,Titan,T8INBND,,MAPS 017TI(T8) Campaign,Part of 017TI(T8) MAPS Campaign. Inbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2005-301T02:15:25,000T01:00:00,28-Oct-05,MIMI,SPASS Rider,Titan,T8INBND,,MAPS 017TI(T8) Campaign,"Part of 017TI(T8) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-301T02:15:25,000T01:32:00,28-Oct-05,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2005-301T02:54:25,000T00:49:00,28-Oct-05,RADAR,Prime,Titan,TI8P2SCAT,,T8 Inbound Scatterometry,Collect inbound scatterometry data.,,,,,, 2005-301T03:15:25,000T02:00:00,28-Oct-05,CAPS,SPASS Rider,Titan,T8CLOSE,,MAPS 017TI(T8) Campaign,Part of 017TI(T8) MAPS Campaign. Observations of Titan's interaction with Saturn's magnetosphere,,,,,, 2005-301T03:15:25,000T02:00:00,28-Oct-05,MIMI,SPASS Rider,Titan,T8CLOSE,,MAPS 017TI(T8) Campaign,"Part of 017TI(T8) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-301T03:15:25,000T02:00:00,28-Oct-05,INMS,Non-SPASS,Titan,T8CLOSE,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine atmospheric and ionospheric composition and thermal structure.,,,,,, 2005-301T03:43:25,000T00:16:48,28-Oct-05,RADAR,Prime,Titan,TI8P3ALTI,,T8 Inbound Altimetry,Collect altimetry data while maintaining nadir pointing.,,,,,, 2005-301T03:47:25,000T00:54:00,28-Oct-05,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2005-301T04:00:13,000T00:12:12,28-Oct-05,RADAR,Prime,Titan,TI8P4LSAR,,T8 Low Resolution Synthetic Aperture RADAR SAR,Low Resolution Synthetic Aperture RADAR (SAR) Imaging.,,,,,, 2005-301T04:12:25,000T00:06:00,28-Oct-05,RADAR,Prime,Titan,TI8P5HSAR,,T8 High Resolution Synthetic Aperture RADAR SAR,High Resolution Synthetic Aperture RADAR (SAR) Imaging.,,,,,, 2005-301T04:18:25,000T00:12:00,28-Oct-05,RADAR,Prime,Titan,TI8P6LSAR,,T8 Low Resolution Synthetic Aperture RADAR SAR,Low Resolution Synthetic Aperture RADAR (SAR) Imaging.,,,,,, 2005-301T04:30:25,000T00:17:00,28-Oct-05,RADAR,Prime,Titan,TI8P7ALTO,,T8 Outbound Altimetry,Collect outbound altimetry data while maintaining nadir pointing.,,,,,, 2005-301T04:42:25,000T01:33:00,28-Oct-05,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2005-301T04:47:25,000T00:49:00,28-Oct-05,RADAR,Prime,Titan,TI8P8SCAT,,T8 Outbound Scatterometry,Collect oubound scatterometry data at 3 different polarization orientations.,,,,,, 2005-301T05:15:25,000T01:00:00,28-Oct-05,CAPS,SPASS Rider,Titan,T8OUTBND,,MAPS 017TI(T8) Campaign,Part of 017TI(T8) MAPS Campaign. Outbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2005-301T05:15:25,000T01:00:00,28-Oct-05,MIMI,SPASS Rider,Titan,T8OUTBND,,MAPS 017TI(T8) Campaign,"Part of 017TI(T8) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2005-301T05:15:25,000T11:00:00,28-Oct-05,INMS,Non-SPASS,Titan,T8OUTBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Observe magnetospheric/ionospheric interatction.,,,,,, 2005-301T06:00:25,000T03:25:00,28-Oct-05,RADAR,Prime,Titan,TI8P9RADO,,T8 Outbound Radiometry,Radiometry during the outbound leg of T8.,,,,,, 2005-301T06:15:25,000T18:33:35,28-Oct-05,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2005-301T06:15:25,001T03:50:51,28-Oct-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-301T06:15:25,000T12:40:26,28-Oct-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-301T07:15:25,001T02:33:35,28-Oct-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-301T09:55:25,000T03:20:00,28-Oct-05,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,CIRS_017TI_MIRLIMB_MAP_03,"Obtain vertical profiles of temperatures, HCN, and C2H2 in Titan's stratosphere. POINTING: -y to Titan, z within 30 degrees of normal to limb.",,,,,, 2005-301T09:55:25,000T03:20:00,28-Oct-05,CIRS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,ISS_PHOT_1x1,"ISS WAC support imaging, 18 images (18 frames, 0.5 Mb/frame)",,,,,, 2005-301T09:55:25,000T01:00:00,28-Oct-05,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,WAC Photometry,"particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2005-301T09:55:25,000T03:20:00,28-Oct-05,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2005-301T09:55:25,000T12:29:00,28-Oct-05,VIMS,SPASS Rider,Titan,LIMBNADIR,,VIMS_ride VIMS_4883,"Ridealong with CIRS, and then ISS. 64X64 cubes (CIRS is probably scanning slowly ~20 microrads per second or less.) As per TOST meeting 4/12/02, cut 1 hr. 41 minutes and 25 mbits.",,,,,, 2005-301T13:15:25,000T03:00:00,28-Oct-05,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_017TI_FIRNADIRCOMPINT_01,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5-2.0. POINTING: -y to Titan, x away from sun.",,,,,, 2005-301T13:15:25,000T03:00:00,28-Oct-05,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2005-301T13:15:25,000T03:00:00,28-Oct-05,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2005-301T13:15:25,000T03:00:00,28-Oct-05,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,UVIS Rider to CIRS Far Nadir Comp,UVIS Rider to CIRS Far-IR Nadir Comp,,,,,, 2005-301T14:02:11,000T02:00:00,28-Oct-05,CDA,Non-SPASS,rings(general),1600RINGM,Ring margin,Ring Margin 0.0070 deg from dust ram.",,,,,, 2005-302T13:15:40,000T01:38:24,29-Oct-05,CDA,Non-SPASS,DustRAM direction,0700DUST,Dust survey,E Ring dense - survey - 0.3370 deg from dust ram.",,,,,, 2005-331T00:37:39,001T06:47:21,27-Nov-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-331T00:53:39,000T00:50:00,27-Nov-05,CIRS,Prime,Rhea,FP3MAP,CIRS FP3 map,Rhea FP3 map,"(THIS SHOULD BE A NIGHTSIDE FP1 MAP, GIVEN THIS VIEWING OPPORTUNITY) FP3 map. Duration 00:50. AD=26-18 mrad, phase=161, sub S/C=(0, 12), Local time near midnight. Place FP3 five mrad off limb for calibration first 8 min (4 min shutter closed, then open); then an 9-scan map of equatorial region: 5 mrad/scan at 16 urad/sec. 15 cm-1, blink, shutter closed first, last 2 min.",,,,,, 2005-331T00:53:39,000T00:50:00,27-Nov-05,UVIS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Rhea, ORS Rider",UV albedo map of Rhea's surface plus limb drifts,,,,,, 2005-331T00:53:39,000T00:50:00,27-Nov-05,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,12 x 12 low res VIS and IR 320ms only total number of cubes 40,,,,,, 2005-331T00:53:39,000T01:40:00,27-Nov-05,CDA,Non-SPASS,DustRAM direction,0700DUST,Dust survey,E Ring dense - survey - 0.30Arcturus: multiple sets of 10 cubes w/64x4 FOV IR @ 160 ms, VIS @ 10160 ms; Time: 8.0 hr; Volume: 125 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Arcturus; Secondary: +z to TBD",,,,,, 2005-336T22:40:00,000T09:05:00,2-Dec-05,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addition due to SAP,sponge bit adjust,,,,,, 2005-336T22:40:00,000T09:05:00,2-Dec-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-336T22:40:00,000T09:05:00,2-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-336T22:40:01,000T09:04:59,2-Dec-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-336T23:40:00,000T05:32:48,2-Dec-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-337T00:15:00,000T06:00:00,3-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-337T02:00:00,000T01:22:00,3-Dec-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2005-337T07:45:00,000T09:29:00,3-Dec-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-337T07:45:00,000T22:29:00,3-Dec-05,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addition due to SAP,sponge bit adjust,,,,,, 2005-337T07:45:00,000T22:29:00,3-Dec-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-337T07:45:01,000T22:28:59,3-Dec-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-337T09:00:00,000T05:21:30,3-Dec-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2005-337T09:45:00,000T01:30:00,3-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 029 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 10 targets: [JA-MI-PA-TE-AT-EP-DI-EN-HE-CP (601, 602, 603, 604, 610, 611, 612, 614, 615, 617)]",,,,,, 2005-337T11:15:00,000T11:00:00,3-Dec-05,ISS,Prime,Phoebe,110PHO,Spectrophotometery,Phoebe Spectrophotometry,"Turn -Y to Phoebe, Do during one Phoebe rotation 6 1x1 mosaics, 10 filters",,,,,, 2005-337T11:15:00,000T11:00:00,3-Dec-05,UVIS,SPASS Rider,Phoebe,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-337T17:14:00,000T13:00:00,3-Dec-05,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4 kbps data,,,,,, 2005-337T22:15:00,000T07:30:00,3-Dec-05,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,Use standard solar port cal design from revs A or C. 6 hrs. - PDN,,,,,, 2005-338T06:14:00,003T01:21:00,4-Dec-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-338T06:14:00,000T09:05:00,4-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-338T06:14:01,003T01:21:00,4-Dec-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-338T07:14:00,000T05:32:48,4-Dec-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-338T09:19:00,000T03:00:00,4-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-338T10:00:00,000T01:22:00,4-Dec-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2005-338T16:00:00,000T01:27:00,4-Dec-05,UVIS,Prime,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2005-338T17:27:00,000T08:30:00,4-Dec-05,ISS,Prime,InstrumentCalibration,BITWEIGHT,Instrument calibration,ISS ADC Bitweight calibration,Dark current images with detector warm or cooling,,,,,, 2005-339T01:57:00,000T01:43:00,5-Dec-05,UVIS,Prime,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2005-339T03:40:00,000T01:20:00,5-Dec-05,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"MUTUAL EVENTS, TRANSIT OF Rhea ACROSS Dione","Turn to satellite, take 1 NAC every ~ minute for duration of event while tracking satellite",,,,,, 2005-339T05:00:00,000T00:30:00,5-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 033 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EN-TL-HE-MI-AT (601, 602, 612, 613, 615)]",,,,,, 2005-339T06:14:00,000T09:05:00,5-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-339T09:19:00,000T03:00:00,5-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-339T15:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T16:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T16:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T17:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T17:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T18:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T18:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T19:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T19:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T20:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T20:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T21:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T21:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T22:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T22:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T23:19:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-339T23:49:00,000T00:30:00,5-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T00:19:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T00:49:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T01:19:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCH,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T01:49:00,000T00:30:00,6-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 038 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [MI-EP-JA-PA-TE (601, 603, 610, 611, 617)]",,,,,, 2005-340T02:19:00,000T03:26:00,6-Dec-05,UVIS,Prime,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2005-340T06:15:00,000T09:05:00,6-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-340T09:20:00,000T03:00:00,6-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-340T15:50:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T16:20:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T16:50:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T17:20:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T17:50:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T18:20:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T18:50:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T19:20:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T19:50:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T20:20:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T20:50:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T21:20:00,000T00:30:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T21:50:00,000T00:15:00,6-Dec-05,ISS,Prime,Saturn,1X2PLRNCI,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-340T22:35:00,000T09:00:00,6-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-341T07:35:00,001T07:15:00,7-Dec-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2005-341T07:35:00,001T07:15:00,7-Dec-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-341T07:35:00,001T07:15:00,7-Dec-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-341T08:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T09:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T09:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T10:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T10:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T11:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T11:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T12:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T12:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T13:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T13:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T14:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T14:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T15:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T15:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T16:05:00,000T00:30:00,7-Dec-05,ISS,Prime,Saturn,1X2PLRNCJ,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-341T16:35:00,000T00:30:00,7-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 043 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [CP-DI-TE-TL-JA (603, 604, 610, 613, 614)]",,,,,, 2005-341T17:05:00,000T12:10:00,7-Dec-05,UVIS,Prime,Saturn,MOSAIC,Mosaic,UVIS MOSAIC,,,,,,, 2005-342T05:45:00,000T09:05:00,8-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-342T08:50:00,000T03:00:00,8-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-342T14:50:00,000T14:55:00,8-Dec-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-342T14:50:00,000T14:55:00,8-Dec-05,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addition due to SAP,sponge bit adjust,,,,,, 2005-342T14:50:00,000T14:55:00,8-Dec-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-342T14:50:00,000T14:55:00,8-Dec-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-342T14:50:00,002T00:00:00,8-Dec-05,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2005-342T15:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T15:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T16:00:00,000T04:31:25,8-Dec-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2005-342T16:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T16:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T17:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T17:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T18:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T18:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T19:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T19:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T20:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T20:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T21:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T21:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T22:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T22:50:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-342T23:20:00,000T00:30:00,8-Dec-05,ISS,Prime,Saturn,1X2PLRNCK,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T01:05:00,000T00:30:00,9-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 047 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [DI-EN-PM-AT-HY (602, 604, 607, 615, 616)]",,,,,, 2005-343T01:35:00,000T03:40:00,9-Dec-05,UVIS,Prime,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2005-343T05:45:00,001T09:05:00,9-Dec-05,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2005-343T05:45:00,001T09:05:00,9-Dec-05,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2005-343T05:45:00,000T09:05:00,9-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-343T06:45:00,000T05:32:48,9-Dec-05,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2005-343T08:50:00,000T03:00:00,9-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-343T10:00:00,000T01:22:00,9-Dec-05,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2005-343T15:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T15:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T16:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T16:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T17:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T17:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T18:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T18:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T19:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T19:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T20:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T20:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T21:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T21:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T22:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T22:50:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-343T23:20:00,000T00:30:00,9-Dec-05,ISS,Prime,Saturn,1X2PLRNCL,Polarimetry,NAC polarimetry Phase 90-135,NAC polarimetry Phase 90-135,,,,,, 2005-344T01:05:00,000T00:30:00,10-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 050 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-EN-HY-DI-EP (602, 604, 607, 611, 617)]",,,,,, 2005-344T01:35:00,000T03:40:00,10-Dec-05,UVIS,Prime,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2005-344T05:45:00,000T09:00:00,10-Dec-05,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2005-344T08:35:00,000T19:48:26,10-Dec-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-344T08:50:00,000T03:00:00,10-Dec-05,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2005-344T14:50:00,000T14:45:00,10-Dec-05,CAPS,SPASS Rider,Sun,MAGBNDSW,MAPS magnetosphere boundary campaign,CAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-344T14:50:00,000T13:41:07,10-Dec-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-344T14:50:00,002T00:00:00,10-Dec-05,MAG,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAG_MAPS_MB_A_Campaign,Observe_dawn-side_magnetospheric_boundaries_at_a_variety_of_radial_distances,,,,,, 2005-344T14:50:00,000T13:41:07,10-Dec-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-344T15:15:00,000T00:30:00,10-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 052 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-EP-MI-EN-AT (601, 602, 610, 611, 615)]",,,,,, 2005-344T15:45:00,000T11:20:00,10-Dec-05,MIMI,Prime,SolarWind,MAGBNDSWD,MAPS solar wind campaign,"Magnetospheric Boundary Campaign, Solar Wind","Pointing for MAGBOUNDARY Campaign, Solar Wind Attitude",,,,,, 2005-345T03:05:00,000T00:30:00,11-Dec-05,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 053 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PM-TE-PA-AT-EN (602, 603, 615, 616, 617)]",,,,,, 2005-345T04:23:26,000T10:11:34,11-Dec-05,INMS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-345T04:26:42,000T00:00:01,11-Dec-05,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse per = 27.4 d, inc = 0.4 deg, r = 53.6 Rs, phase = 89 deg",,,,,, 2005-345T04:31:07,001T10:18:53,11-Dec-05,MIMI,SPASS Rider,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2005-345T04:31:07,001T10:18:53,11-Dec-05,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2005-345T04:45:42,006T09:35:17,11-Dec-05,CDA,Non-SPASS,DustRAM direction,2500DUST,Dust survey,Dust survey 0.1670 deg from dust ram.",,,,,, 2005-358T10:17:58,000T00:49:59,24-Dec-05,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.00 25.2 Mb data volume.",,,,,, 2005-358T14:20:00,000T00:40:00,24-Dec-05,ISS,SPASS Rider,Dione,DIONE,Dione,Dione regional geodesy,Do 1x1 mosaic in NAC clear and 3-color plus WAC clear,,,,,, 2005-358T14:20:00,000T00:40:00,24-Dec-05,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2005-358T14:40:52,000T01:28:42,24-Dec-05,CDA,Non-SPASS,DustRAM direction,0600DUST,Dust survey,E Ring dense - survey - 0.1870 deg from dust ram.",,,,,, 2006-016T21:32:37,000T00:49:59,16-Jan-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.00AD>2.0 mrad; 146Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2006-033T20:38:00,000T04:00:00,2-Feb-06,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2006-033T20:38:00,000T04:00:00,2-Feb-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-033T20:38:00,000T04:00:00,2-Feb-06,UVIS,SPASS Rider,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2006-034T00:38:00,000T00:30:00,3-Feb-06,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 031 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [EP-DI-JA-PA-AT (604, 610, 611, 615, 617)]",,,,,, 2006-034T01:48:00,000T09:05:00,3-Feb-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2006-034T02:30:00,000T06:00:00,3-Feb-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,can't delete until removed from delivery Deep space obervations for calibration.,,,,,, 2006-034T10:38:00,002T10:13:45,3-Feb-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-034T10:53:00,000T14:55:00,3-Feb-06,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addition due to SAP,sponge bit adjust,,,,,, 2006-034T10:53:00,002T00:00:00,3-Feb-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey. Datarate is composed of continuous 494bps (8vps) plus bursts of 1976bps (32vps).,,,,,, 2006-034T11:23:00,000T00:30:00,3-Feb-06,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 032 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-CP-EP-JA-PM (610, 611, 614, 616, 617)]",,,,,, 2006-034T11:53:00,000T10:00:00,3-Feb-06,ISS,Prime,Saturn,3X5LIGHTH,3 x 5 mosaic lightning search,NAC Northern Hemisphere Saturn lightning search,"Each picket is 3x5 NAC mos using the HAL filter with 56 second exp times, picket duration 01:28:00. Repeat interval for the pickets is every 02:08:00. There are 5 pickets in this ob.",,,,,, 2006-034T11:53:00,000T10:00:00,3-Feb-06,CDA,SPASS Rider,Other,DECON,Decontamination,Decontamination,"CDA boresight off-sun, no Watts",,,,,, 2006-034T11:53:00,000T10:00:00,3-Feb-06,CIRS,SPASS Rider,Saturn,2X3LGTSEA,Lightning search,ISS Rider,ISS Rider,,,,,, 2006-034T11:53:00,000T10:00:00,3-Feb-06,VIMS,SPASS Rider,Saturn,2X3LGTSEA,Lightning search,Saturn Lightning during CIRS F Ring movie,Saturn Lightning during ISS mosaic.,,,,,, 2006-034T12:00:00,000T02:16:32,3-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-034T18:00:00,000T02:16:32,3-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-034T21:53:00,000T00:30:00,3-Feb-06,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 033 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [JA-AT-DI-EP-EN (602, 604, 610, 611, 615)]",,,,,, 2006-034T22:23:00,000T02:55:00,3-Feb-06,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2006-034T22:23:00,000T02:55:00,3-Feb-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL3,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-034T22:23:00,000T02:55:00,3-Feb-06,UVIS,SPASS Rider,InstrumentCalibration,IMPACT,,,Calibrate HSP and FUV instrument response on dark sky for statistical baseline comparison to IMPACT detection measurements.,,,,,, 2006-035T01:48:00,001T08:15:00,4-Feb-06,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addition due to SAP,sponge bit adjust,,,,,, 2006-035T01:48:00,000T09:05:00,4-Feb-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2006-035T02:48:00,000T03:00:00,4-Feb-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-035T03:00:00,000T02:16:32,4-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-035T11:23:00,000T01:00:00,4-Feb-06,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 034 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [TL-DI-AT-EP-JA (604, 610, 611, 613, 615)]",,,,,, 2006-035T12:00:00,000T02:16:32,4-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-035T12:00:00,000T05:14:00,4-Feb-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-035T12:23:00,000T10:00:00,4-Feb-06,ISS,Prime,Saturn,3X5LIGHTI,3 x 5 mosaic lightning search,NAC Northern Hemisphere Saturn lightning search,"Each picket is 3x5 NAC mos using the HAL filter with 56 second exp times, picket duration 01:28:00. Repeat interval for the pickets is every 02:08:00. There are 5 pickets in this ob.",,,,,, 2006-035T12:23:00,000T10:00:00,4-Feb-06,CIRS,SPASS Rider,Saturn,2X3LGTSEA,Lightning search,ISS Rider,ISS Rider,,,,,, 2006-035T12:23:00,000T10:00:00,4-Feb-06,VIMS,SPASS Rider,Saturn,2X3LGTSEA,Lightning search,Saturn Lightning during CIRS F Ring movie,Saturn Lightning during ISS mosaic.,,,,,, 2006-035T18:00:00,000T02:16:32,4-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-035T22:23:00,000T00:30:00,4-Feb-06,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 035 TH OBS","Images of small satellites for orbit determination purposes. One NAC (CL1,CL2) of each target. This observation has 5 targets: [PA-PM-CP-MI-HE (601, 612, 614, 616, 617)]",,,,,, 2006-035T22:53:00,000T01:55:00,4-Feb-06,CAPS,Prime,Other,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,A MAPS Campaign. Observe dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2006-036T01:48:00,000T09:05:00,5-Feb-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2006-036T02:48:00,000T03:00:00,5-Feb-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-036T03:00:00,000T02:16:32,5-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-036T03:00:00,000T01:13:00,5-Feb-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-036T10:03:00,000T00:50:00,5-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-036T10:03:00,000T17:20:00,5-Feb-06,CDA,Non-SPASS,Other,DATAVOL,Data volume adjustment,Datavol addition due to SAP,sponge bit adjust,,,,,, 2006-036T10:03:00,000T08:15:00,5-Feb-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-036T10:53:00,000T07:06:40,5-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-036T10:53:00,000T10:43:53,5-Feb-06,CAPS,Non-SPASS,Saturn,2KSURVEY,2 kbps survey mode,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-036T10:53:00,000T16:30:00,5-Feb-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_Survey_Measurements,Continuous_low_rate_magnetospheric_survey.,,,,,, 2006-036T10:53:00,000T10:43:53,5-Feb-06,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2006-036T11:23:00,000T06:24:00,5-Feb-06,ISS,Prime,Saturn,3X5LIGHTJ,3 x 5 mosaic lightning search,NAC Northern Hemisphere Saturn lightning search,"Each picket is 3x5 NAC mos using the HAL filter with 56 second exp times, picket duration 01:28:00. Repeat interval for the pickets is every 02:08:00. There are 3 pickets in this ob.",,,,,, 2006-036T11:23:00,000T06:24:00,5-Feb-06,CIRS,SPASS Rider,Saturn,2X3LGTSEA,Lightning search,ISS Rider,ISS Rider,,,,,, 2006-036T11:23:00,000T06:24:00,5-Feb-06,VIMS,SPASS Rider,Saturn,2X3LGTSEA,Lightning search,Saturn Lightning during CIRS F Ring movie,Saturn Lightning during ISS mosaic.,,,,,, 2006-036T18:18:00,000T03:18:53,5-Feb-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2006-036T19:03:00,000T08:02:08,5-Feb-06,CAPS,Non-SPASS,co-rotation,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-036T19:18:00,000T06:00:00,5-Feb-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-036T20:51:45,011T02:13:15,5-Feb-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-036T20:58:04,000T00:00:01,5-Feb-06,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse per = 39.2 d, inc = 0.4 deg, r = 68.2 Rs, phase = 107 deg",,,,,, 2006-036T21:00:00,000T03:15:00,5-Feb-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-036T21:36:53,000T05:46:07,5-Feb-06,CAPS,Non-SPASS,Saturn,2KSURVEY,2 kbps survey mode,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-036T21:36:53,000T05:46:08,5-Feb-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-036T21:36:53,000T05:46:07,5-Feb-06,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2006-036T21:36:53,000T05:46:07,5-Feb-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting H data at a low rate continuously. No special pointing is required.,,,,,, 2006-036T21:49:32,017T02:44:30,5-Feb-06,CDA,Non-SPASS,DustRAM direction,2500DUST,Dust survey,Dust survey 0.0370 deg from dust ram.",,,,,, 2006-056T01:05:00,000T17:39:59,25-Feb-06,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,adjust datavolume for E-Ring measurements,dust measurements,,,,,, 2006-056T01:05:00,000T00:47:50,25-Feb-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.0070 deg from dust ram.",,,,,, 2006-079T10:02:00,000T00:38:00,20-Mar-06,VIMS,Prime,Saturn,CYLMAP,Saturn cylindrical map,VIMS Cylindrical Map #3,"Cylindrical Map acquired near and at periapse. Short, 38-minute opportunity, followed by an Alp CMI occultation.",,,,,, 2006-079T10:02:00,000T00:38:00,20-Mar-06,UVIS,SPASS Rider,Saturn,CYLMAP,Saturn cylindrical map,Cyllindrical Map Rider,Ride along on VIMS cyllindrical map,,,,,, 2006-079T10:02:51,000T00:49:59,20-Mar-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.00S scan at 32 urad/sec. Should have time to get good space calibration for FP1 above north pole (terminate before clearing south pole if necessary -- will be obliquely crossing terminator there, anyway).",,,,,, 2006-080T05:00:00,000T01:45:00,21-Mar-06,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible. Crosses multiple CIRS and ISS observations.,,,,,, 2006-080T05:00:00,000T00:15:00,21-Mar-06,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"20x40 lo/lo 640ms, 160ms",,,,,, 2006-080T05:15:00,000T01:30:00,21-Mar-06,CIRS,Prime,Rhea,FP3CRESC,,Rhea FP3 map of crescent.,"FP1 observation of Rhea for high spectral resolution integration for composition, and for phase angle coverage. Phase=106.0, Local time= 4.9, sub S/C=( 1.1, 30.4), AD= 16.2 mrad. Map lit crescent with six 7-mrad FP3 scans at 8 urad/sec.",,,,,, 2006-080T05:15:00,000T01:30:00,21-Mar-06,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"20x40 lo/lo (2x640ms, 320ms, 160ms) repeat 3 times",,,,,, 2006-080T05:42:12,000T00:37:48,21-Mar-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.0070 deg from dust ram.",,,,,, 2006-118T14:02:37,000T00:49:59,28-Apr-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.00 RWA90).,,,,,, 2006-140T13:18:11,000T01:00:00,20-May-06,CAPS,SPASS Rider,Titan,T14OUTBND,,MAPS 024TI(T14) Campaign,Part of 024TI(T14) MAPS Campaign. Outbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2006-140T13:18:11,000T01:00:00,20-May-06,MIMI,SPASS Rider,Titan,T14OUTBND,,MAPS 024TI(T14) Campaign,"Part of 024TI(T14) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2006-140T13:18:11,000T11:00:00,20-May-06,INMS,Non-SPASS,Titan,T14OUTBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Observe magnetospheric/ionospheric interatction.,,,,,, 2006-140T13:45:11,000T00:48:00,20-May-06,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,CIRS_024TI_FIRLIMB_INTEG_02,"Vertical sounding stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically. POINTING: -y to Titan, -z within to limb. Substitutes: T12in/out.",,,,,, 2006-140T13:45:11,000T00:48:00,20-May-06,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2006-140T13:45:11,000T00:50:00,20-May-06,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2006-140T13:45:11,000T18:45:00,20-May-06,VIMS,SPASS Rider,Titan,LIMB,Limb observation,Comp_map_VIMS,"Limb integration followed by nadir temp map, with CIRS primary. 64 X 64 cubes at end, but during the first 8 hours, another mode may work better.",,,,,, 2006-140T14:18:11,004T06:06:55,20-May-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-140T14:18:11,000T22:20:55,20-May-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-140T14:18:11,000T14:46:55,20-May-06,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2006-140T14:33:11,000T02:45:00,20-May-06,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_024TI_FIRNADIRMAP_02,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps. Substitutes: T12out, T13in.",,,,,, 2006-140T14:33:11,000T02:45:00,20-May-06,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2006-140T14:33:11,000T02:45:00,20-May-06,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2006-140T16:18:11,001T03:37:48,20-May-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-140T17:18:11,000T05:00:00,20-May-06,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,CIRS_024TI_MIRLIMBINT_1,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: -y to Titan, z within 30 degrees of normal to limb. Substitute: T12out, T13in.",,,,,, 2006-140T17:18:11,000T05:00:00,20-May-06,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2006-140T17:18:11,000T04:00:00,20-May-06,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,WPH (WAC Photometry),"particle properties, vertical distributions ~6 km/px. 0.6 Mbit/frame with 2x2 summing. special S/C orientation requested.",,,,,, 2006-140T22:18:11,000T03:00:00,20-May-06,CDA,Prime,Other,ECCSCAN,Eccentricity scan,CDA Eccentricity Scan,"CDA eccentricity scan: An observation scenario which allows the separation of orbital elements to the greatest degree possible is required. Particle inclinations can be determined having a rolling S/C with a rotation axis parallel to the ring plane (equatorial orbits). However in order to determine particle eccentricities the CDA boresight must rotate in the ring plane. This observation mode requires a CDA prime observation and cannot easily be combined with ORS, RADAR or D/L observations.",,,,,, 2006-140T23:52:34,000T01:59:59,20-May-06,CDA,Non-SPASS,rings(general),1600RINGM,Ring margin,Ring Margin 0.0070 deg from dust ram.",,,,,, 2006-141T22:59:45,000T00:49:59,21-May-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.0070 deg from dust ram.",,,,,, 2006-181T03:02:23,000T00:49:59,30-Jun-06,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.0070 deg from dust ram.",,,,,, 2006-205T02:52:01,000T19:07:59,24-Jul-06,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MIMI Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2006-205T03:00:00,000T01:00:00,24-Jul-06,ISS,Prime,Dione,GLOCOL,Global coverage mapping,Dione global color mapping and regional mapping,Turn -Y to Dione; Do 1x1 mosaic 2 clear filter + 24 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; do scan for CIRS.,,,,,, 2006-205T03:00:00,000T01:00:00,24-Jul-06,CIRS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,Ride,"Ride on ISS. FP3/4 at 15.5 cm-1, blink. Of 01:00 duration, shutter closed 00:10-001:15 and 00:45-00:50.",,,,,, 2006-205T03:00:00,000T01:00:00,24-Jul-06,UVIS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2006-205T03:00:00,000T01:00:00,24-Jul-06,VIMS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,Dione,"36x18i2-v1, 160 ms and 640 ms (9.1 min/cycle). Repeat 2, 64x64i2-v3 (160, 320 ms (33 min/cycle) Data Volume 80Mbits After compression (2x) 40 Mbits",,,,,, 2006-205T03:00:00,000T05:11:05,24-Jul-06,CDA,Non-SPASS,DustRAM direction,0605DUST,Dust survey,E-Ring Margin - survey - 5.01Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2006-210T00:00:00,000T06:00:00,29-Jul-06,UVIS,SPASS Rider,Star,FOMALHAUT,Fomalhaut,Stellar Calibration on Fomalhaut,Ride-along on VIMS observation of Fomalhaut to get additional new calibration data,,,,,, 2006-210T04:45:00,000T11:05:00,29-Jul-06,RSS,SPASS Rider,Earth,SCE3,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #3,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2006-210T06:50:00,000T09:00:00,29-Jul-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-210T15:50:00,000T22:30:00,29-Jul-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-210T16:45:00,000T14:00:00,29-Jul-06,UVIS,SPASS Rider,Sun,SOLARPORT,Solar port observation,VIMS SOLAR PORT RIDER,VIMS RIDER,,,,,, 2006-210T22:15:00,000T01:25:00,29-Jul-06,VIMS,Prime,Star,30HERCAL,Stellar calibration,30 Her calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 70 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2006-210T22:15:00,000T08:30:00,29-Jul-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-210T23:30:00,000T00:34:08,29-Jul-06,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,Calibration/Gain curve of ELS sensor,Calibration/gain curve of ELS sensor. 8 B cycles duration in 16 kbps. Data is in addition to 1000 bps from SWSKR.,,,,,, 2006-210T23:40:00,000T01:25:00,29-Jul-06,VIMS,Prime,Star,CHICYGCAL,Chi Cygni calibration,Chi Cygni calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 70 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2006-211T01:05:00,000T01:25:00,30-Jul-06,VIMS,Prime,Star,MUCEPCAL,Mu Cepheii calibration,Mu Cepheii calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 70 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2006-211T02:30:00,000T01:25:00,30-Jul-06,VIMS,Prime,Star,RAQRCAL,,R Aquarii calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 70 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2006-211T03:55:00,000T01:25:00,30-Jul-06,VIMS,Prime,Star,PI1GRUCAL,pi_1 Gru calibration,pi_1 Gru calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 70 min; Volume: 26 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED.,,,,,, 2006-211T05:20:00,000T01:25:00,30-Jul-06,VIMS,Prime,Star,ETASGRCAL,ETA Sgr calibration,eta Sgr calibration,Turn to star : 15 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms; OCC mode tests. Time: 55 min; Volume: 26 Mbits; CompRatio: 2.0 Return to waypoint: 15 min Not time critical. RWA REQUIRED.,,,,,, 2006-211T06:45:00,000T07:00:00,30-Jul-06,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. This is one of two requests added to the S22 period. The start times are not critical but the period 198 to 201 is most suitable for these activities. This request uses a spare slot on day 211 which is just on edge of useful region. Duration 6 to 8 hours preferred to get a reasonable number of rolls. Overlaps MAGTAIL request so datarate set to zero. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equtorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2006-211T06:45:00,000T07:00:00,30-Jul-06,CAPS,Non-SPASS,Saturn,4KBURST,4 kbps burst,Burst of 4k data,Burst of 4k data,,,,,, 2006-211T06:45:00,000T07:00:00,30-Jul-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-211T12:15:00,000T11:05:00,30-Jul-06,RSS,SPASS Rider,Earth,SCE3,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #3,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2006-211T13:45:00,001T09:20:00,30-Jul-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-211T14:20:00,000T09:00:00,30-Jul-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-211T16:20:00,000T02:16:32,30-Jul-06,CAPS,Non-SPASS,Saturn,4KBURST,4 kbps burst,Burst of 4k data,Burst of 4k data,,,,,, 2006-211T23:20:00,000T02:00:00,30-Jul-06,INMS,Non-SPASS,Saturn,FULLSURV,MAPS magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-211T23:20:00,000T14:45:00,30-Jul-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-211T23:50:00,000T13:45:00,30-Jul-06,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_026SA_MIRMAP14,Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude,,,,,, 2006-211T23:50:00,000T13:45:00,30-Jul-06,UVIS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,EUVFUV MIRMAP Rider,UVIS EUV and FUV riding along with CIRS MIRMAP observation,,,,,, 2006-212T01:00:00,000T02:16:32,31-Jul-06,CAPS,Non-SPASS,Saturn,4KBURST,4 kbps burst,Burst of 4k data,Burst of 4k data,,,,,, 2006-212T01:20:00,000T11:30:00,31-Jul-06,ISS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Saturn BOTSIM imaging,Photometry/polarimetry,,,,,, 2006-212T01:20:00,001T21:45:00,31-Jul-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-212T12:00:00,000T11:05:00,31-Jul-06,RSS,SPASS Rider,Earth,SCE3,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #3,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2006-212T14:05:00,000T09:00:00,31-Jul-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-212T14:50:00,000T08:11:00,31-Jul-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-212T16:00:00,000T04:33:04,31-Jul-06,CAPS,Non-SPASS,Saturn,4KBURST,4 kbps burst,Burst of 4k data,Burst of 4k data,,,,,, 2006-212T23:05:00,000T15:00:00,31-Jul-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-212T23:05:01,000T14:59:59,31-Jul-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-212T23:35:00,000T04:30:00,31-Jul-06,ISS,Prime,Star,CHARGEXF,Instrument calibration,ISS CCD Charge Transfer Calibration,Point to M48. Rotate about -Y and image every 20-30 degrees.,,,,,, 2006-213T04:05:00,000T04:30:00,1-Aug-06,ISS,Prime,Star,CHARGEXF,Instrument calibration,ISS CCD Charge Transfer Calibration,Point to Pleiades. Rotate about -Y and image every 20-30 degrees.,,,,,, 2006-213T08:35:00,000T05:00:00,1-Aug-06,MIMI,Prime,Sun,TAILPLSFL,Magnetotail campaign,"Magnetotail Campaign, tailward flow","Pointing for MAGNETOTAIL Campaign, tailward flow attitude",,,,,, 2006-213T14:05:00,001T09:00:00,1-Aug-06,CAPS,Non-SPASS,Saturn,4KBURST,4 kbps burst,Burst of 4k data,Burst of 4k data,,,,,, 2006-213T14:05:00,001T09:00:00,1-Aug-06,CDA,Non-SPASS,Other,DRATESAP,Data volume adjustment,additional DV due to sponge bits,dust measurements,,,,,, 2006-213T14:05:00,001T09:00:00,1-Aug-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-213T14:05:00,000T09:00:00,1-Aug-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-213T14:05:01,001T08:59:59,1-Aug-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-213T23:05:00,000T02:00:00,1-Aug-06,INMS,Non-SPASS,Saturn,FULLSURV,MAPS magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-213T23:05:00,000T08:20:00,1-Aug-06,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2006-213T23:35:00,000T14:00:00,1-Aug-06,MIMI,Prime,Sun,TAILPLSFL,Magnetotail campaign,"Magnetotail Campaign, tailward flow","Pointing for MAGNETOTAIL Campaign, tailward flow attitude",,,,,, 2006-214T01:05:00,000T22:00:00,2-Aug-06,INMS,Non-SPASS,Saturn,PTOTM69,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-214T04:35:00,000T03:54:40,2-Aug-06,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2006-214T14:05:00,000T09:00:00,2-Aug-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-214T23:05:00,001T22:20:48,2-Aug-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-214T23:05:00,009T10:55:00,2-Aug-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-214T23:05:01,001T22:41:31,2-Aug-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-214T23:35:00,000T03:30:00,2-Aug-06,MIMI,Prime,Sun,TAILPLSFL,Magnetotail campaign,"Magnetotail Campaign, tailward flow","Pointing for MAGNETOTAIL Campaign, tailward flow attitude",,,,,, 2006-215T00:05:00,000T03:00:00,3-Aug-06,RADAR,SPASS Rider,Other,NORTHWARM,Distant Titan latitude study warmup,"Distant Titan Latitude Study, Northern Latitudes",Warmup for calibration and science data collection.,,,,,, 2006-215T03:05:00,000T02:30:00,3-Aug-06,RADAR,Prime,Titan,NORTH7CAL,Distant Titan latitude study,"Distant Titan Latitude Study, Northern Latitudes",Obtain distant Titan radiometer science and calibration data. One of a set that provides coverage of Titan northern latitude variation along with some obtainable associated longitude variation.,,,,,, 2006-215T05:35:00,000T08:00:00,3-Aug-06,MIMI,Prime,Sun,TAILPLSFL,Magnetotail campaign,"Magnetotail Campaign, tailward flow","Pointing for MAGNETOTAIL Campaign, tailward flow attitude",,,,,, 2006-215T12:00:00,000T11:05:00,3-Aug-06,RSS,SPASS Rider,Earth,SCE3,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #3,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2006-215T14:05:00,000T09:00:00,3-Aug-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-215T14:50:00,000T08:11:00,3-Aug-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-216T11:45:00,000T11:05:00,4-Aug-06,RSS,SPASS Rider,Earth,SCE3,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #3,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2006-216T13:50:00,000T09:00:00,4-Aug-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-216T14:35:00,000T08:11:00,4-Aug-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL2,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-216T21:19:56,000T00:00:01,4-Aug-06,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 24.0 d, inc = 14.9 deg, r = 49.0 Rs, phase = 172 deg",,,,,, 2006-216T21:25:12,000T00:00:01,4-Aug-06,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse per = 24.0 d, inc = 14.9 deg, r = 49.0 Rs, phase = 172 deg",,,,,, 2006-216T21:25:48,009T11:24:20,4-Aug-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-216T21:25:48,002T04:58:12,4-Aug-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-216T21:25:48,001T00:00:00,4-Aug-06,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2006-216T21:25:48,009T00:54:12,4-Aug-06,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2006-216T21:46:31,007T12:13:29,4-Aug-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-216T21:59:38,010T02:34:24,4-Aug-06,CDA,Non-SPASS,DustRAM direction,2100DUST,Dust survey,Dust survey 0.3070 deg from dust ram.",,,,,, 2006-229T01:30:00,000T01:55:00,17-Aug-06,CDA,Non-SPASS,DustRAM direction,0403DUST,Dust survey,E Ring dense - survey - 2.8570 deg from dust ram.",,,,,, 2006-252T19:37:59,000T00:42:01,9-Sep-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-252T20:20:00,000T02:30:00,9-Sep-06,MIMI,SPASS Rider,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2006-252T20:20:00,011T00:02:00,9-Sep-06,CDA,Non-SPASS,NotApplicable,DRATE,Data volume adjustment,Datavolume rider,DV Rider,,,,,, 2006-252T20:21:00,000T05:07:16,9-Sep-06,CDA,Non-SPASS,DustRAM direction,0408DUST,Dust survey,Dust survey inside 8 Rs 8.41 179 DEG. ***",,,,,, 2006-258T21:30:00,000T01:30:00,15-Sep-06,ISS,SPASS Rider,RingG,HIPHASE,High phase observation,,24 WAC filters during VIMS stare at highest phase region of G ring,,,,,, 2006-258T21:30:00,000T01:30:00,15-Sep-06,UVIS,SPASS Rider,RingG,HIPHASE,High phase observation,,UV spectral mapping of Saturn's rings.,,,,,, 2006-258T23:00:00,000T06:00:00,15-Sep-06,RSS,Prime,rings(general),OCC,Occultation,RSS Ring Ingress Occulation 028,"THIS REQUEST: Because this is a slow event, we include one hour of baseline prior to the F ring ingress time. GENERAL: We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stablization in RSS WARMUP mode. We will commence observations with a 60-minute baseline and calibration period, followed by the ring ingress, which ends at the D ring. After a two-hour thermal stabilization period, we commence observations of the ingress atmosphere occultation 60 minutes before the 1.3-bar level. Atmosphere ingress observations end 5 hours after the 1.3-bar level.",,,,,, 2006-259T05:00:00,000T07:00:00,16-Sep-06,RSS,Prime,Saturn,OCC,Occultation,RSS Saturn Atmosphere Ingress Occulation 028,"THIS REQUEST: Because this is a slow event, we include one hour of baseline prior to the atmosphere ingress time, and continue after the 1.3-bar level by an time correspondingly scaled up by the velocity compared with that of other occultations. GENERAL: We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stablization in RSS WARMUP mode. We will commence observations with a 60-minute baseline and calibration period, followed by the ring ingress, which ends at the D ring. After a two-hour thermal stabilization period, we commence observations of the ingress atmosphere occultation 60 minutes before the 1.3-bar level. Atmosphere ingress observations end 5 hours after the 1.3-bar level.",,,,,, 2006-259T12:00:00,000T08:00:00,16-Sep-06,RSS,Prime,Saturn,OCC,Occultation,RSS Saturn Atmosphere Ingress Occulation 028,"THIS REQUEST: Because this is a slow event, we include one hour of baseline prior to the atmosphere ingress time, and continue after the 1.3-bar level by an time correspondingly scaled up by the velocity compared with that of other occultations. GENERAL: We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stablization in RSS WARMUP mode. We will commence observations with a 60-minute baseline and calibration period, followed by the ring ingress, which ends at the D ring. After a two-hour thermal stabilization period, we commence observations of the ingress atmosphere occultation 60 minutes before the 1.3-bar level. Atmosphere ingress observations end 5 hours after the 1.3-bar level.",,,,,, 2006-259T20:00:00,000T06:30:00,16-Sep-06,RSS,Prime,Saturn,OCC,Occultation,RSS Atm. Flash and Egress Occultation 028,"To observe the Central Flash behind Saturn's atmosphere. This is followed by the RSS occultation EGRESS of Saturn's atmosphere and ionosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used.",,,,,, 2006-260T01:59:00,000T12:08:00,17-Sep-06,RSS,SPASS Rider,Saturn,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band for improving spacecraft ephemeris near Saturn and ring occultations. Time includes 5 minutes for Ka-TWTA maintenance and 2 hours for thermal stabilization.,,,,,, 2006-260T04:30:00,000T09:37:00,17-Sep-06,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously during downlink periods. No special pointing is required.,,,,,, 2006-260T14:00:01,000T03:08:57,17-Sep-06,MIMI,SPASS Rider,Other,MAGTAIL,MAPS magnetotail observation,MAPS MT/antiS Campaign,"Part of MT/antiS MAPS Campaign. MIMI setup for MAPS Magnetotail observations; observe plasma flows. Pointing: corotation and Saturn both in -X, Z half-plane; or rotate about -X to sun, or rotate about -Z to Earth. Observe the structure and dynamics of Saturns magnetotail at large distances downstream.",,,,,, 2006-260T14:07:00,000T03:10:00,17-Sep-06,CAPS,SPASS Rider,Other,MAGTAIL,MAPS magnetotail observation,MAPS,"Part of MT,antiS MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail in the anti-solar direction (Z GSE=0)",,,,,, 2006-260T14:07:00,000T03:01:58,17-Sep-06,INMS,Non-SPASS,Other,MAGTAIL,MAPS magnetotail observation,MAPS,"Part of MT,antiS MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail in the anti-solar direction",,,,,, 2006-260T14:07:00,003T06:15:00,17-Sep-06,MAG,Non-SPASS,Other,MAGTAIL,MAPS magnetotail observation,MAG_MAPS_MT_antiS_Campaign,Observe_the_structure_and_dynamics_of_Saturn's_magnetotail_in_the_anti-solar_direction. (0),,,,,, 2006-260T14:07:00,000T03:01:58,17-Sep-06,RPWS,Non-SPASS,Other,MAGTAIL,MAPS magnetotail observation,"MAPS MT,antiS Campaign","Part of MT,antiS MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail in the anti-solar direction",,,,,, 2006-260T14:45:00,000T13:45:00,17-Sep-06,MIMI,Prime,Saturn,TAILPADIS,Magnetotail campaign,"Magnetotail Campaign, pitch angle distribution","Pointing for MAGNETOTAIL Campaign, pitchangle distribution attitude",,,,,, 2006-260T15:15:00,000T06:00:00,17-Sep-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL1,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-260T17:08:58,003T03:13:02,17-Sep-06,MIMI,SPASS Rider,Other,MAGTAIL,MAPS magnetotail observation,MAPS MT/antiS Campaign,"Part of MT/antiS MAPS Campaign. MIMI setup for MAPS Magnetotail observations; observe plasma flows. Pointing: corotation and Saturn both in -X, Z half-plane; or rotate about -X to sun, or rotate about -Z to Earth. Observe the structure and dynamics of Saturns magnetotail at large distances downstream.",,,,,, 2006-260T17:08:58,001T04:57:02,17-Sep-06,INMS,Non-SPASS,Other,MAGTAIL,MAPS magnetotail observation,MAPS,"Part of MT,antiS MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail in the anti-solar direction",,,,,, 2006-260T17:08:58,003T03:13:02,17-Sep-06,RPWS,Non-SPASS,Other,MAGTAIL,MAPS magnetotail observation,"MAPS MT,antiS Campaign","Part of MT,antiS MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail in the anti-solar direction",,,,,, 2006-260T17:10:02,000T00:00:01,17-Sep-06,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 24.5 deg, r = 37.6 Rs, phase = 173 deg",,,,,, 2006-260T17:17:00,003T03:05:00,17-Sep-06,CAPS,SPASS Rider,Other,MAGTAIL,MAPS magnetotail observation,MAPS,"Part of MT,antiS MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail in the anti-solar direction (Z GSE=0)",,,,,, 2006-260T17:34:39,003T02:47:21,17-Sep-06,CDA,Non-SPASS,DustRAM direction,1902DUST,Dust survey,Dust survey 2.3370 deg from dust ram.",,,,,, 2006-268T22:00:00,000T01:10:00,25-Sep-06,VIMS,Prime,Star,DELVIROCC,Delta Vir occultation,delVir,"Orbits = 029-029, Cube Size (X,Z) = 64*64 IR-only, 8:1 spectral summing, tau_IR=80 ms Time per SC pointing (mins) = 6.0, Number of SC pointings = 10/hr, Time of observation (hours) = 1.0, Volume (Mbits) = 16/hr, Desc = Stellar_occ mode. ascent thru left ansa--A,B,C rings, Phase=41.8, Dist=0.27(10^6km)",,,,,, 2006-268T22:00:00,000T01:10:00,25-Sep-06,CIRS,SPASS Rider,rings(general),DELVIROCC,Delta Vir occultation,CIRS_029RI_DELVIROCC001_VIMS,ride with VIMS.,,,,,, 2006-268T22:00:00,000T01:10:00,25-Sep-06,UVIS,SPASS Rider,Star,DELVIROCC,Delta Vir occultation,URSTAR,RIDER,,,,,, 2006-268T22:00:00,000T01:10:00,25-Sep-06,VIMS,SPASS Rider,Star,DELVIROCC,Delta Vir occultation,Del Vir Stellar Occultation SI,ISS Support Imaging: Time is a place holder until PDT designs are done. VIMS will need two images one at the beginning of the observation and one at the end of the obasrvation.,,,,,, 2006-268T22:11:00,002T21:49:00,25-Sep-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-268T22:45:59,000T03:34:01,25-Sep-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-268T23:05:00,000T00:19:50,25-Sep-06,CDA,Non-SPASS,RingE,0407ERNGM,E ring margin,E-Ring Margin 7.00L>12, 1770 deg from dust ram.",,,,,, 2006-285T04:45:00,000T00:15:00,12-Oct-06,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,Deep Space Cal,Deep space observation for calibration during turns,,,,,, 2006-285T04:45:01,001T03:14:59,12-Oct-06,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MIMI Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed generally toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2006-285T05:00:00,000T01:35:00,12-Oct-06,CIRS,Prime,rings(general),TEMPU10MP,Thermal map,CIRS_030RI_TempUL10MP,"Afternoon radial scan of main rings to obtain thermal measurement of rings. -Y to rings, Z perp to rings",,,,,, 2006-285T05:00:00,000T01:35:00,12-Oct-06,CIRS,SPASS Rider,rings(general),TEMPU10MP,Thermal map,CIRS_029RI_TEMPU10MP_SI,,,,,,, 2006-285T05:00:00,000T01:35:00,12-Oct-06,UVIS,SPASS Rider,rings(general),TEMPU10MP,Thermal map,,UV spectral mapping of Saturn's rings.,,,,,, 2006-285T05:00:00,000T01:49:32,12-Oct-06,CDA,Non-SPASS,RingE,0710ERNGM,E ring margin,E-Ring Margin 10.0070 deg from dust ram.",,,,,, 2006-301T03:54:00,000T00:46:00,28-Oct-06,MIMI,SPASS Rider,co-rotation,IMVP5N,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=4.5-5, near 1200 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2006-301T04:30:00,000T01:30:00,28-Oct-06,INMS,Prime,Saturn,INMAGSCN,Inner magnetosphere scan,Rev 31 Periapse,Part of Rings TWT periapse. Inner magnetosphere ion composition observation.,,,,,, 2006-301T04:30:00,000T01:30:00,28-Oct-06,CIRS,SPASS Rider,InstrumentCalibration,INMAGSCN,Inner magnetosphere scan,CIRS_031IC_INMAGSCN001_INMS,rider,,,,,, 2006-301T04:30:00,000T04:30:35,28-Oct-06,CDA,Non-SPASS,DustRAM direction,0630SURIN,Dust survey,Dust survey inside 8 Rs 30.0070 deg from dust ram.",,,,,, 2006-313T03:00:00,000T02:00:00,9-Nov-06,VIMS,Prime,Tethys,TETHYS,Tethys,Tethys,"36i2-54v3 160ms, 640 ms (10 min/cycle) repeat 3 each hour",,,,,, 2006-313T03:00:00,000T02:00:00,9-Nov-06,CIRS,SPASS Rider,Tethys,TETHYS,Tethys,FP1 phase coverage at 0.5 cm-1 resolution,"Custom turn period.........Timing changed 02/18/03.........Geometry may need adjustment. VIMS rider on Tethys for high spectral resolution integration for composition, and for phase angle coverage. Phase= 46.0, Local time= 8.8, sub S/C=( -16.1, 294.4), AD= 5.3 mrad. Duration=02:00. CIRS: coadd detectors; 96 RTI, shutter closed 00:15 to 00:20 nad 01:40 to 01:45.",,,,,, 2006-313T03:00:00,000T02:00:00,9-Nov-06,ISS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys global color,Do multi-color imaging of Tethys,,,,,, 2006-313T03:00:00,000T02:00:00,9-Nov-06,UVIS,SPASS Rider,Tethys,TETHYS,Tethys,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2006-313T03:40:03,000T00:44:57,9-Nov-06,MIMI,SPASS Rider,co-rotation,IMVP5N,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=4.5-5, near 1200 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2006-313T04:25:00,000T16:35:00,9-Nov-06,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MIMI Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed generally toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2006-313T04:25:00,001T05:33:00,9-Nov-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-313T04:25:00,000T07:39:10,9-Nov-06,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-313T04:25:00,001T05:33:00,9-Nov-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-313T05:00:00,000T03:00:00,9-Nov-06,VIMS,Prime,rings(general),COMPLODRK,Low phase dark side ring radial scan,"radial scan, low phase, unlit side","Orbits = 031-034, Cube Size (X,Z) = 64*12 hires, tau_IR = 80 & 320 msec?, Time per SC pointing (mins) = 9, Number of SC pointings = 16, Time of observation (hours) = 2.5 , Volume (Mbits) = 52, Desc = Obtain a complete hi-res radial scan of the unlit face of the A, B and C rings, at low phase angle. Orient X-axis along scan direction (radial). At 6 R_S this will take 15 cubes and 2.3 hrs, which fits on revs 31-34. Do for east and west ansae. unlit face, low phase; west ansa",,,,,, 2006-313T05:00:00,000T03:00:00,9-Nov-06,CIRS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,CIRS_032RI_COMPLODRK_VIMS,ride with VIMS,,,,,, 2006-313T08:00:00,000T00:28:00,9-Nov-06,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,Deep Space Cal,Deep space observation for calibration during turns,,,,,, 2006-313T08:04:45,000T00:40:00,9-Nov-06,CDA,Non-SPASS,DustRAM direction,0630SURIN,Dust survey,Dust survey inside 8 Rs 30.0070 deg from dust ram.",,,,,, 2006-325T02:20:00,000T01:40:00,21-Nov-06,RADAR,Prime,Dione,SCATTRAD,RADAR Scatterometry / Radiometry,Simultaneous Scatterometry & Radiometry of Dione,Point -Z axis at target and execute raster scans centered on target. Acquire simultaneous scatterometry and radiometry of target.,,,,,, 2006-325T02:42:03,000T00:47:57,21-Nov-06,MIMI,SPASS Rider,co-rotation,IMVP5N,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=4.5-5, near 1200 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2006-325T03:30:00,000T17:30:00,21-Nov-06,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MIMI Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed generally toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2006-325T03:30:00,003T13:00:00,21-Nov-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-325T03:30:00,000T07:37:40,21-Nov-06,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-325T03:30:00,003T13:00:00,21-Nov-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-325T04:00:00,000T03:00:00,21-Nov-06,VIMS,Prime,rings(general),COMPLODRK,Low phase dark side ring radial scan,"radial scan, low phase, unlit side","Orbits = 031-034, Cube Size (X,Z) = 64*12 hires, tau_IR = 80 & 320 msec?, Time per SC pointing (mins) = 9, Number of SC pointings = 16, Time of observation (hours) = 2.5 , Volume (Mbits) = 52, Desc = Obtain a complete hi-res radial scan of the unlit face of the A, B and C rings, at low phase angle. Orient X-axis along scan direction (radial). At 6 R_S this will take 15 cubes and 2.3 hrs, which fits on revs 31-34. Do for east and west ansae. unlit face, low phase; west ansa",,,,,, 2006-325T04:00:00,000T03:00:00,21-Nov-06,CIRS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,CIRS_033RI_COMPLODRK_VIMS,ride with VIMS,,,,,, 2006-325T07:00:00,000T06:30:00,21-Nov-06,ISS,Prime,rings(general),LPHRDFMOV,Ansa movie,ANSA MOVIE SRCH FOR MOONLETS,Ansa movie of two narrow features in D ring,,,,,, 2006-325T07:10:00,000T00:40:00,21-Nov-06,CDA,Non-SPASS,DustRAM direction,0630SURIN,Dust survey,Dust survey inside 8 Rs 30.0070 deg from dust ram.",,,,,, 2006-337T01:20:02,000T00:44:58,3-Dec-06,MIMI,SPASS Rider,co-rotation,IMVP5N,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=4.5-5, near 1200 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2006-337T01:50:00,000T02:40:00,3-Dec-06,UVIS,Prime,Star,URALPVIR,Stellar occultation,URSTAR,Instance of URSTAR: grazing occultation through all rings.,,,,,, 2006-337T01:50:00,000T02:40:00,3-Dec-06,CIRS,SPASS Rider,Star,ALPVIR,Alpha Virginis occultation,CIRS_034RI_ALVIROCC_UVIS,ride with UVIS Stellar Occultation,,,,,, 2006-337T01:50:00,000T02:40:00,3-Dec-06,UVIS,SPASS Rider,Star,URALPVIR,Stellar occultation,Support Imaging,Adding precise timing for support imaging based on new trajectory. NAC and WAC images at the following times: 2006-337T02:43:58 2006-337T02:21:03 2006-337T02:11:11 2006-337T02:08:04 2006-337T03:30:02 2006-337T03:52:56 2006-337T04:02:48 2006-337T04:05:55,,,,,, 2006-337T01:50:00,000T04:35:01,3-Dec-06,CDA,Non-SPASS,DustRAM direction,0630SURIN,Dust survey,Dust survey inside 8 Rs 30.00 thrusters,,,,,, 2006-346T11:11:31,000T01:00:00,12-Dec-06,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2006-346T11:18:31,000T00:23:00,12-Dec-06,INMS,Prime,Titan,T21RMPNT,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2006-346T11:34:31,000T00:07:00,12-Dec-06,RADAR,SPASS Rider,Titan,T21RASAR,,T21 ride along SAR,Ride along SAR of Titan with INMS.,,,,,, 2006-346T11:41:31,000T00:07:00,12-Dec-06,RADAR,Prime,Titan,T21OTHSAR,,High Resolution SAR Imaging of Titan of T21,High resolution SAR imaging of Titan during closest approach period,,,,,, 2006-346T11:41:31,000T01:00:00,12-Dec-06,INMS,Non-SPASS,Titan,T21FULRT,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2006-346T11:48:31,000T00:08:00,12-Dec-06,RADAR,Prime,Titan,T21OTLSAR,,Low Resolution SAR Imaging of T21,Low resolution SAR imaging during the post-closest approach time period,,,,,, 2006-346T11:56:31,000T00:15:00,12-Dec-06,RADAR,Prime,Titan,T21OUTALT,,Outbound Altimetry on T21,Altimetry during the outbound trajectory of T21,,,,,, 2006-346T12:11:31,000T01:30:00,12-Dec-06,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2006-346T12:33:31,000T00:45:00,12-Dec-06,RADAR,Prime,Titan,T21OTSCAT,,T21 outbuond Scatterometry,Scatterometry of Titan. -Z scanned over Titan. Y axis controlled for different polarizations,,,,,, 2006-346T12:41:31,000T01:00:00,12-Dec-06,CAPS,SPASS Rider,Titan,T21OUTBND,,MAPS 035TI(T21) Campaign,Part of 035TI(T21) MAPS Campaign. Outbound approach observations and context for the interaction between Titan and Saturn's magnetosphere,,,,,, 2006-346T12:41:31,000T01:00:00,12-Dec-06,MIMI,SPASS Rider,Titan,T21OUTBND,,MAPS 035TI(T21) Campaign,"Part of 035TI(T21) MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2006-346T12:41:31,000T11:00:00,12-Dec-06,INMS,Non-SPASS,Titan,T21OUTBD,,MAPS TOST Campaign,Part of TOST MAPS Campaign. Observe magnetospheric/ionospheric interatction.,,,,,, 2006-346T13:18:31,000T02:23:00,12-Dec-06,RADAR,Prime,Titan,T21OUTRAD,,T21 outbound Radiometry,Radiometry of Titan. -Z scanned over Titan. Y axis controlled for different polarizations.,,,,,, 2006-346T13:41:31,002T14:39:39,12-Dec-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-346T13:41:31,000T10:24:43,12-Dec-06,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2006-346T15:11:31,000T00:30:00,12-Dec-06,CIRS,SPASS Rider,InstrumentCalibration,DSCALSHRT,Deep space calibration,,Deep space obervations for calibration.,,,,,, 2006-346T15:41:31,000T03:00:00,12-Dec-06,ISS,Prime,Titan,GLOBMAPNA,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2006-346T15:41:31,000T03:00:00,12-Dec-06,CIRS,SPASS Rider,Titan,GLOBMAPNA,Global coverage mapping,CIRS_035TI_FIRNADIRMAP_02,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps. Substitutes: T19out, T21out.",,,,,, 2006-346T15:41:31,000T03:00:00,12-Dec-06,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,ISS_Regional_Map VIMS_4868,Ridealong on regional map observation with ISS.,,,,,, 2006-346T15:41:31,000T04:00:00,12-Dec-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-346T18:41:31,000T02:00:00,12-Dec-06,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,CIRS_035TI_MIRLIMBINT_2,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: -y to Titan, z within 30 degrees of normal to limb. Substitute: T19out.",,,,,, 2006-346T18:41:31,000T02:00:00,12-Dec-06,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2006-346T18:41:31,000T02:00:00,12-Dec-06,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2006-346T18:41:31,000T02:00:00,12-Dec-06,VIMS,SPASS Rider,Titan,MIDIRLMB,,CIRS_mid_IR_Limb VIMS_4868,Ridealong on Mid-IR limb observation with CIRS.,,,,,, 2006-346T19:41:31,000T14:18:29,12-Dec-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-346T20:41:31,000T01:28:00,12-Dec-06,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,NMA (NAC Monitoring of Surface and Atmosphere),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2006-346T20:41:31,000T01:28:00,12-Dec-06,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,CIRS_035TI_FIRNADIRMAP_02,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps. Substitutes: T19out, T21out.",,,,,, 2006-346T20:41:31,000T01:00:00,12-Dec-06,VIMS,SPASS Rider,Titan,GLOBALMAP,Global coverage mapping,ISS_Global_Map VIMS_4868,Ridealong on global mapping observation with ISS.,,,,,, 2006-346T22:09:31,000T03:00:00,12-Dec-06,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_035TI_COMPMAP23,"To obtain measurements of nitriles, hydrocarbons, and an oxygen compound, CO2, as a function of latitude and emission angle (at equator) on Titan. POINTING: -y to Titan, z to pole",,,,,, 2006-346T22:09:31,000T03:00:00,12-Dec-06,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Titan NAC Movie,Titan NAC Photopol CIRS ridealong,,,,,, 2006-346T22:09:31,000T03:00:00,12-Dec-06,UVIS,SPASS Rider,Titan,COMPMAP,Composition map,UVIS Rider to CIRS COMPMAP,UVIS Rider to CIRS COMP Map,,,,,, 2006-346T23:37:25,000T08:10:35,12-Dec-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-347T00:00:01,000T07:47:59,13-Dec-06,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2006-347T02:21:00,000T08:00:00,13-Dec-06,CIRS,SPASS Rider,InstrumentCalibration,DSCAL06,Deep space calibration,CIRS Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2006-347T06:00:00,002T00:03:00,13-Dec-06,CDA,SPASS Rider,DustRAM direction,DATA,Data volume adjustment,DataVolume,,,,,,, 2006-347T07:48:00,000T00:58:29,13-Dec-06,CDA,Non-SPASS,DustRAM direction,1615DUSTB,Dust survey,Dust survey 14.78 retrograde dust with -y2Sat and AM=270",,,,,, 2006-349T10:10:00,000T02:00:00,15-Dec-06,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2006-349T13:00:00,000T01:39:32,15-Dec-06,CDA,Non-SPASS,DustRAM direction,0907SUOUT,Dust survey,Dust survey outside 8 Rs 7.00 retrograde dust with -y2Sat and AM=270",,,,,, 2006-349T13:25:04,001T19:45:56,15-Dec-06,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2006-349T13:25:04,007T01:08:56,15-Dec-06,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2006-349T13:25:04,000T01:37:56,15-Dec-06,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2006-349T13:25:04,003T02:34:56,15-Dec-06,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2006-349T14:40:32,000T01:48:03,15-Dec-06,CDA,Non-SPASS,DustRAM direction,1010DUST,Dust survey,Dust survey outside 8 Rs 9.5570 deg from dust ram.",,,,,, 2007-114T14:40:00,000T01:10:00,24-Apr-07,ISS,Prime,Enceladus,PLUMES,Observe Enceladus' plumes,Enceladus ORS South Polar Plume Observation,"Custom handoff from CDA_043RE_RPXING001_PRIME to Enceladus. Point and stare 30min at Enceladus, 15-min FP3 scan for CIRS. Custom handoff to ISS_043DI_REGMAPB001_PRIME",,,,,, 2007-114T14:40:00,000T01:10:00,24-Apr-07,CIRS,SPASS Rider,Enceladus,PLUMES,Observe Enceladus' plumes,Observation of Enceladus plumes,"Rider on Enceladus plume observation cut out of CDA and Dione observations. AD=2.9 mrad, phase=165-150, (5, 210) - (-15, 240). Duration 01:50. 15.5 cm-1, blink.",,,,,, 2007-114T14:40:00,000T01:10:00,24-Apr-07,UVIS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of satellite. Observations targeted to Enceladus will test connection of volatile changes to plume eruptions. This observation rides along on an ISS very high phase observation of the plume (165 deg).,,,,,, 2007-114T14:40:00,000T01:10:00,24-Apr-07,VIMS,SPASS Rider,Enceladus,PLUMES,Observe Enceladus' plumes,Enceladus Plume high phase,640ms/pixel framing for the plume region.,,,,,, 2007-114T14:49:57,000T00:25:03,24-Apr-07,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-114T15:00:00,000T00:50:00,24-Apr-07,CDA,Non-SPASS,Other,DRATEA,Data volume adjustment,adjust datavolume for E-Ring measurements,E-Ring dust measurements,,,,,, 2007-114T15:15:00,000T03:39:56,24-Apr-07,MIMI,SPASS Rider,co-rotation,IMVP65M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=6.5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2007-114T15:45:00,000T09:24:32,24-Apr-07,CDA,SPASS Rider,DustRAM direction,0603DUST,Dust survey,Dust survey inside 8 Rs 3.17Pleiades: multiple cubes w/64x64 FOV IR @ 640 ms, VIS @ 40000 ms; Time: 7.0 hr 47 min; Volume: 86.5 Mbits; CompRatio: 2.0

Turn to waypoint: 30 min

Primary: -y to Pleiades; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2007-120T15:45:00,000T04:30:00,30-Apr-07,VIMS,Prime,Star,ARCTURUS,Arcturus observation,Arcturus,"Turn to Arcturus; Time: 30 min

Arcturus: multiple sets of 10 cubes w/64x4 FOV IR @ 160 ms, VIS @ 10160 ms; Time: 8.0 hr; Volume: 125 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Arcturus; Secondary: +z to TBD",,,,,, 2007-120T20:45:00,000T09:00:00,30-Apr-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-121T05:45:00,001T03:48:00,1-May-07,INMS,Non-SPASS,Sun,PTOTM107B,MAPS survey,MAPS,"Part of MB,C MAPS Campaign. Observe afternoon magnetospheric boundaries at 35 RS apoapsis distance and a range of inclinations",,,,,, 2007-121T05:45:00,000T01:30:49,1-May-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2007-121T06:15:00,000T04:45:00,1-May-07,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2007-121T07:00:00,000T01:50:56,1-May-07,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-121T10:55:00,000T11:05:00,1-May-07,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rings/Saturn Occultation experiment on DOY 130.",,,,,, 2007-121T11:00:00,000T01:00:00,1-May-07,ISS,Prime,rings(general),WN50205,Ring photometry,Ring photometry,One WAC on left ansa in multi-colors plus NAC multi-color radial scan,,,,,, 2007-121T12:00:00,000T00:30:00,1-May-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 026 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-121T13:00:00,000T09:00:00,1-May-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-121T13:45:00,000T08:00:00,1-May-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-121T22:00:00,000T03:00:00,1-May-07,RADAR,SPASS Rider,Other,NORTHWARM,Distant Titan latitude study warmup,"Distant Titan Latitude Study, Northern Latitudes",Warmup for calibration and science data collection.,,,,,, 2007-121T23:30:00,000T01:30:00,1-May-07,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2007-122T01:00:00,000T01:00:00,2-May-07,RADAR,Prime,Titan,NORTH4CAL,Distant Titan latitude study,"Distant Titan Latitude Study, Northern Latitudes",Obtain distant Titan radiometer science and calibration data. One of a set that provides coverage of Titan northern latitude variation along with some obtainable associated longitude variation.,,,,,, 2007-122T02:00:00,000T03:00:00,2-May-07,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2007-122T05:00:00,000T15:00:00,2-May-07,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images. Distance to Saturn -s 2 million Km. Phase is 0-145,,,,,, 2007-122T09:33:00,000T00:22:58,2-May-07,INMS,Non-SPASS,Saturn,FRB,Memory read out,MAPS Survey,Memory read out request.,,,,,, 2007-122T09:55:58,000T13:38:10,2-May-07,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,C MAPS Campaign. Observe afternoon magnetospheric boundaries at 35 RS apoapsis distance and a range of inclinations",,,,,, 2007-122T20:30:00,000T09:00:00,2-May-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-122T21:15:00,000T08:00:00,2-May-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-122T23:25:47,000T00:00:01,2-May-07,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 15.9 d, inc = 39.1 deg, r = 36.2 Rs, phase = 67 deg",,,,,, 2007-122T23:34:08,001T22:25:52,2-May-07,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,C MAPS Campaign. Observe afternoon magnetospheric boundaries at 35 RS apoapsis distance and a range of inclinations",,,,,, 2007-122T23:34:08,001T22:25:52,2-May-07,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,C Campaign","Part of MB,C MAPS Campaign. Observe afternoon magnetospheric boundaries at 35 RS apoapsis distance and a range of inclinations",,,,,, 2007-122T23:40:04,001T22:19:56,2-May-07,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/C Campaign,"Part of MB/C MAPS Campaign. Observe afternoon magnetospheric boundaries at 35 RS apoapsis distance and a range of inclinations. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2007-122T23:41:00,001T22:19:00,2-May-07,CAPS,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS ""MB,C"" Campaign","Part of MB,C MAPS Campaign. Observe afternoon magnetospheric boundaries at 35 RS apoapsis distance and a range of inclinations",,,,,, 2007-122T23:54:47,001T22:05:13,2-May-07,CDA,Non-SPASS,DustRAM direction,1823DUST,Dust survey,Dust survey 23.3070 deg from dust ram.",,,,,, 2007-130T19:55:00,000T02:55:00,10-May-07,CAPS,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2007-130T19:55:00,000T02:55:00,10-May-07,INMS,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2007-130T19:55:00,000T02:55:00,10-May-07,MAG,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAG MAPS IM_VP Campaign,Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. (L~4.5-5 midnight (alt)),,,,,, 2007-130T19:55:00,000T02:55:00,10-May-07,RPWS,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2007-130T20:17:58,000T00:27:02,10-May-07,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-130T20:43:00,000T00:30:00,10-May-07,CIRS,Prime,Saturn,OCCLIMB,Occultation,CIRS_044SA_OCCLIMB01,"obtain stratospheric thermal structure at the RSS occultation points. POINTING: -y to Saturn, z to limb",,,,,, 2007-130T20:43:00,000T00:30:00,10-May-07,CIRS,SPASS Rider,Saturn,OCCLIMB,Occultation,CIRS_044SA_OCCLIMB SI,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, latitude coverage. POINTING: -y to Saturn, z to limb",,,,,, 2007-130T20:45:00,000T02:05:00,10-May-07,MIMI,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2007-130T21:00:01,015T23:34:59,10-May-07,CDA,SPASS Rider,DustRAM direction,RATEA,Data volume adjustment,Data RAte,,,,,,, 2007-130T21:00:01,000T05:18:39,10-May-07,CDA,Non-SPASS,DustRAM direction,0409DUST,Dust survey,Dust survey inside 8 Rs 8.7370 deg from dust ram.",,,,,, 2007-146T22:20:06,000T00:09:59,26-May-07,CDA,Non-SPASS,RingE,0304ERNGX,Ring plane crossing,E Ring Xing 4.0070 deg from dust ram.",,,,,, 2007-162T23:15:00,000T14:05:00,11-Jun-07,MIMI,SPASS Rider,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2007-163T00:10:00,000T00:40:00,12-Jun-07,INMS,Prime,Saturn,INMAGSCAN,Inner magnetosphere scan,INMS Inner Magnetospheric Scan,null,,,,,, 2007-163T00:10:00,000T00:40:00,12-Jun-07,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_046IC_DEEPSPACE_INMS,rider,,,,,, 2007-163T00:45:00,000T04:59:35,12-Jun-07,CDA,Non-SPASS,DustRAM direction,0307DUST,Dust survey,Dust survey inside 8 Rs 7.3970 deg from dust ram.",,,,,, 2007-178T17:51:31,000T00:15:00,27-Jun-07,ISS,Prime,Tethys,PHOTOM,Photometry,Tethys Photometry/Polarization,GEOLOGY STUDY: High-phase 1x3 mosaic. BOTSIMS (N04+W04) done three times.,,,,,, 2007-178T17:51:31,000T00:15:00,27-Jun-07,CIRS,SPASS Rider,Tethys,TETHYS,Tethys,Rider,"ISS rider. Phase=138, Local time= 21.1, sub S/C=(16, 169), AD= 15 mrad. Duration 00:15. CIRS: pairs, 15.5 cm-1, shutter closed first and last 2 min. FP1+FP3 only.",,,,,, 2007-178T17:51:31,000T00:18:00,27-Jun-07,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-178T17:51:31,000T00:15:00,27-Jun-07,VIMS,SPASS Rider,Tethys,PHOTOM,Photometry,Tethys,"24x12i2-v1 160 ms observation, assuming 1 minute dwell time by ISS, frame with ISS dwell, 15 cubes = 10.5 mbit Tethys is ~142 deg phase 30 pixels diam.",,,,,, 2007-178T18:06:31,000T00:37:00,27-Jun-07,CIRS,Prime,Tethys,FP1NITMAP,CIRS FP1 dark side map,FP1 darkside map,"FP1 dark side map of Tethys; duration 37 min. Phase=147, Local time= 21.5, sub S/C~(22, 164), AD=18-26 mrad. FP1+FP3 only. 15.5 or 6.6 cm-1 (TBD). Make FP1 map of full disk. If 15.5 cm-1, then time for full disk at nominal scan rate (420 urad/sec). If 6.6 cm-1, then probably cannot do full disk (290 urad/sec); if so, cut off region of lit crescent [Will want to start map at crescent side so that best spatial resolution will be obtained on the side with the dark limb at end of observation.]",,,,,, 2007-178T18:06:31,000T00:37:00,27-Jun-07,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-178T18:06:31,000T00:37:00,27-Jun-07,VIMS,SPASS Rider,Tethys,FP1AZOPS,,Tethys,"64x64i1-v1 640 ms observation 1 cube, Tethys is ~142 deg phase 45 pixels diam. 10.4 mbit compressed. CIRS may be raster scanning with FP1 so we may need to redesign this.",,,,,, 2007-178T18:32:28,000T00:30:00,27-Jun-07,CDA,Non-SPASS,RingE,0502ERNGX,Ring plane crossing,E Ring Xing 2.0070 deg from dust ram.",,,,,, 2007-201T09:37:40,000T00:49:59,20-Jul-07,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.00Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Fomalhaut; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2007-208T01:00:00,000T06:45:20,27-Jul-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-208T08:25:00,000T00:30:00,27-Jul-07,ISS,Prime,Rhea,310W020PH,Spectrophotometery,Rhea spectrophotometry/ phase coverage,Turn -Y to Rhea; do 1x1 mosaic 3 clear + 4 NAC color + 9 NAC polarizer + 4 WAC polarizer filters; turn to WP,,,,,, 2007-208T08:25:00,000T00:30:00,27-Jul-07,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-208T08:55:00,000T05:41:00,27-Jul-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_04,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn Spin Axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0354 mrad/sec about the Z-axis for 12000 to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 7000s toward +MOS Orb. 4) Slew back to Saturn Center and reset pointing. Stare for remaining observation time. MOS orb (+/-range): 212.62mrad",,,,,, 2007-208T08:55:00,000T05:41:00,27-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO004_UVIS,Calibration rider. Data Volume will be 81.84 Mb or less.,,,,,, 2007-208T15:06:00,000T09:00:00,27-Jul-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-208T16:00:00,000T08:00:00,27-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-209T00:06:04,000T07:44:51,28-Jul-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2007-209T00:36:00,000T00:22:58,28-Jul-07,INMS,Non-SPASS,Saturn,FRB,Memory read out,MAPS Survey,Memory read out request.,,,,,, 2007-209T00:58:58,004T23:37:02,28-Jul-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-209T01:36:00,000T05:45:00,28-Jul-07,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,Spectroscopic observation of Eta Carinae (RA=161.2619). Slew to star; settle; execute small box scan; return to waypoint.,,,,,, 2007-209T01:36:00,000T05:45:00,28-Jul-07,CIRS,SPASS Rider,Star,1STAROBS,Stellar spectroscopy,3 cm-1 characterization of two stars.,"ISS NAC support imaging, 2 images per observation: one at start +1 hour; the other at start +5 hours.",,,,,, 2007-209T01:36:00,000T05:45:00,28-Jul-07,ISS,SPASS Rider,Other,1STAROBS,Stellar spectroscopy,Support imaging for CIRS star calibration,TBD,,,,,, 2007-209T07:51:00,000T09:00:00,28-Jul-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-209T08:30:00,000T02:16:32,28-Jul-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-209T08:42:00,000T08:00:00,28-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-209T16:51:04,000T22:29:51,28-Jul-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2007-209T17:21:00,000T19:40:00,28-Jul-07,ISS,Prime,Saturn,STRMOVIEC,Saturn storm movie,NAC Southern Hemisphere Saturn strip movie,"1x6 BOTSIM mosaic in 6 filters of the 0-15S latitude band for two rotations; pickets of 1:20 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-209T17:21:00,000T19:40:00,28-Jul-07,CIRS,SPASS Rider,Saturn,STRMOVIEC,Saturn storm movie,CIRS movie rider,something,,,,,, 2007-209T17:21:00,000T19:40:00,28-Jul-07,UVIS,SPASS Rider,Saturn,STRMOVIEC,Saturn storm movie,,,,,,,, 2007-209T17:21:00,000T19:40:00,28-Jul-07,VIMS,SPASS Rider,Saturn,STRMOVIEC,Saturn storm movie,TBD,TBD,,,,,, 2007-210T13:01:00,000T01:50:00,29-Jul-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_06,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, parallel with the Saturn Spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .0306 mrad/sec about the Z-axis for 6000s to Saturn Center. 3) Reset pointing and stare for remaining observation time. MOS orb (+/-range): 183.79mrad",,,,,, 2007-210T13:01:00,000T01:50:00,29-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO006_UVIS,Calibration rider. Data Volume will be 26.4 Mb or less.,,,,,, 2007-210T15:21:00,000T09:00:00,29-Jul-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-210T16:10:00,000T08:00:00,29-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-211T01:51:00,000T00:30:00,30-Jul-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 038 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-211T02:21:00,000T09:10:00,30-Jul-07,CAPS,Prime,InstrumentCalibration,CALIBRATE,Calibration,CAPS Calibration,"CAPS periodic gain test and calibration. The specified rate and data volume are the delta above the CAPS survey rate (1000 bps), and the rate is the average over the entire request (current plans are to conduct the test in two different rates.)",,,,,, 2007-211T02:21:00,000T09:10:00,30-Jul-07,MAG,SPASS Rider,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Suitable periods for S32 are from day 206 to 223. The last requested rolls in S31 are on day 188. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equtorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2007-211T11:31:00,000T02:34:00,30-Jul-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_07,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .0292 mrad/sec about the Z-axis for 7500s toward +MOS Orb. 3) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/-range): 175.36mrad",,,,,, 2007-211T11:31:00,000T02:34:00,30-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO007_UVIS,Calibration rider. Data Volume will be 36.96 Mb or less.,,,,,, 2007-211T11:31:00,001T12:19:00,30-Jul-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-211T14:05:00,000T00:30:00,30-Jul-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 039 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-211T15:05:00,000T09:00:00,30-Jul-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-211T16:00:00,000T08:00:00,30-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-212T00:35:00,000T07:30:00,31-Jul-07,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,"Turn to sun; Time: 30 min Solar Port: 2 3x3 Mosaics w/64x64 FOV @ 20,80,320 ms IR, VIS always @ 50ms; Time: 13 hr; Volume: 374 Mbits; CompRatio: 3.0 Solar Background Calibration: 4 cubes w/64x64 FOV; Time: 30 min; Volume: 69.2 Mbits; CompRatio: 1.0 Turn to waypoint: 30 min",,,,,, 2007-212T08:05:00,000T05:45:00,31-Jul-07,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observation of VY Canis Majoris (RA=110.7466, Dec=-25.7688). Slew to star; settle; execute small box scan; return to waypoint.",,,,,, 2007-212T08:05:00,000T05:45:00,31-Jul-07,CIRS,SPASS Rider,Star,1STAROBS,Stellar spectroscopy,3 cm-1 characterization of two stars.,"ISS NAC support imaging, 2 images per observation: one at start +1 hour; the other at start +5 hours.",,,,,, 2007-212T13:50:00,000T00:30:00,31-Jul-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 040 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-212T14:50:00,000T09:00:00,31-Jul-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-212T15:40:00,000T08:00:00,31-Jul-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-212T23:50:00,001T00:00:00,31-Jul-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-212T23:50:04,000T14:59:51,31-Jul-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2007-213T01:20:00,000T03:30:00,1-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_09,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. 2) Drift at a rate of .1154 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 4000s to Saturn Center. 4) Reset pointing for Saturn center. MOS orb (+/-range): 461.84 mrad",,,,,, 2007-213T01:20:00,000T03:30:00,1-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO009_UVIS,Calibration rider. Data Volume will be 50.4 Mb or less.,,,,,, 2007-213T01:30:00,000T01:25:20,1-Aug-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-213T04:50:00,000T09:30:00,1-Aug-07,ISS,Prime,Saturn,APOMOVIEA,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for one rotation; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-213T04:50:00,000T09:30:00,1-Aug-07,CIRS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,CIRS movie rider,something,,,,,, 2007-213T04:50:00,000T09:30:00,1-Aug-07,UVIS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,DAYGLOW OBSERVATION,,,,,,, 2007-213T04:50:00,000T09:30:00,1-Aug-07,VIMS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,TBD,TBD,,,,,, 2007-213T05:00:00,000T09:36:00,1-Aug-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-213T14:50:00,000T09:00:00,1-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-213T15:30:00,000T03:46:08,1-Aug-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-213T15:40:00,000T08:00:00,1-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-213T23:50:00,008T23:30:00,1-Aug-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-213T23:50:04,000T07:44:51,1-Aug-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2007-214T00:20:00,000T01:00:00,2-Aug-07,ISS,Prime,Iapetus,MEETUSOON,,Iapetus: Final Saturn conjunction before close fly,"Turn -Y to Saturn north pole, to Rh/Te conjunction, to Saturn again, to Iapetus, to Saturn again for NAC north/south stripe; turn to WP",,,,,, 2007-214T00:20:00,000T01:00:00,2-Aug-07,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-214T00:36:00,000T00:22:58,2-Aug-07,INMS,Non-SPASS,Saturn,FRB,Memory read out,MAPS Survey,Memory read out request.,,,,,, 2007-214T00:58:58,003T22:36:02,2-Aug-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-214T01:20:00,000T00:40:00,2-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_10,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Drift at a rate of .1122 mrad/sec about the Z-axis for 2000s from Saturn Center toward -MOS Orb. 2) Slew back to Saturn Center and reset pointing. MOS orb (+/-range): 448.86mrad",,,,,, 2007-214T02:00:00,000T00:10:00,2-Aug-07,ISS,Prime,Saturn,APOMOVIEB,Apoapsis movie,WAC Saturn movie,1x2 WAC mosaic in 3 filters; picket of 0:10 duration.,,,,,, 2007-214T02:10:00,000T01:30:00,2-Aug-07,UVIS,Prime,Saturn,MOS48APOA,Apoapsis mosaic,MOSAIC_APO_48_10,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .1122 mrad/sec about the Z-axis for 4000s toward -MOS Orb. 3) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 449.0802364 mrad",,,,,, 2007-214T03:40:00,000T00:10:00,2-Aug-07,ISS,Prime,Saturn,APOMOVIEB,Apoapsis movie,WAC Saturn movie,1x2 WAC mosaic in 3 filters; picket of 0:10 duration.,,,,,, 2007-214T03:50:00,000T03:15:00,2-Aug-07,UVIS,Prime,Saturn,MOS48APOB,Apoapsis mosaic,MOSAIC_APO_48_10,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate +64mrad in the YZ plane. 2) Drift at a rate of .1122 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Rotate -64mrad in the YZ plane. Drift at indicated rate about the Z-axis for 4000s to Saturn Center. 4) Reset pointing for Saturn Center. MOS orb (+/-range): 448.86 mrad",,,,,, 2007-214T07:35:00,000T09:00:00,2-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-214T08:30:00,000T08:00:00,2-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-214T18:05:00,000T19:30:00,2-Aug-07,ISS,Prime,Saturn,APOMOVIEC,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for two rotations; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-214T18:05:00,000T19:30:00,2-Aug-07,CIRS,SPASS Rider,Saturn,APOMOVIEC,Apoapsis movie,CIRS movie rider,something,,,,,, 2007-214T18:05:00,000T19:30:00,2-Aug-07,UVIS,SPASS Rider,Saturn,APOMOVIEC,Apoapsis movie,DAYGLOW OBSERVATION,,,,,,, 2007-214T18:05:00,000T19:30:00,2-Aug-07,VIMS,SPASS Rider,Saturn,APOMOVIEC,Apoapsis movie,TBD,TBD,,,,,, 2007-215T13:35:00,000T01:00:00,3-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_11,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Drift at a rate of .1084 mrad/sec about the Z-axis for 3000s toward +MOS Orb. 2) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 433.44mrad",,,,,, 2007-215T15:05:00,000T09:00:00,3-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-215T16:00:00,000T08:00:00,3-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-216T00:35:00,000T04:15:00,4-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_12,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center +MOS Orb. Rotate -64mrad in the YZ plane. 2) Drift about the Z-axis at a rate of .1074 mrad/s for 8000s to -MOS Orb. 3) Drift at indicated rate for 6000s toward +MOS Orb. 4) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 429.66mrad",,,,,, 2007-216T00:35:00,000T04:15:00,4-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO012_UVIS,Calibration rider. Data Volume will be 61.2 Mb or less.,,,,,, 2007-216T04:50:00,000T09:30:00,4-Aug-07,ISS,Prime,Saturn,APOMOVIEA,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for one rotation; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-216T04:50:00,000T09:30:00,4-Aug-07,CIRS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,CIRS movie rider,something,,,,,, 2007-216T04:50:00,000T09:30:00,4-Aug-07,UVIS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,DAYGLOW OBSERVATION,,,,,,, 2007-216T04:50:00,000T09:30:00,4-Aug-07,VIMS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,TBD,TBD,,,,,, 2007-216T14:50:00,000T09:00:00,4-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-216T15:40:00,000T08:00:00,4-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-217T04:35:00,000T09:30:00,5-Aug-07,ISS,Prime,Saturn,APOMOVIEA,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for one rotation; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-217T04:35:00,000T09:30:00,5-Aug-07,CIRS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,CIRS movie rider,something,,,,,, 2007-217T04:35:00,000T09:30:00,5-Aug-07,UVIS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,DAYGLOW OBSERVATION,,,,,,, 2007-217T04:35:00,000T09:30:00,5-Aug-07,VIMS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,TBD,TBD,,,,,, 2007-217T14:35:00,000T09:00:00,5-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-217T23:35:00,001T00:00:00,5-Aug-07,INMS,Non-SPASS,Saturn,PTOTM123,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-217T23:35:04,000T14:59:51,5-Aug-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2007-218T00:05:00,000T04:30:00,6-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_14,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to +MOS Orb. Rotate -128mrad in the YZ plane. 2) Drift at a rate of .1043mrad/s about the Z-axis for 8000s to -MOS Orb. 3) Drift at indicated rate about the Z-axis for 6500s toward +MOS Orb. 4) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 417.30 mrad",,,,,, 2007-218T00:05:00,000T04:30:00,6-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO014_UVIS,Calibration rider. Data Volume will be 64.8 Mb or less.,,,,,, 2007-218T04:35:00,000T09:30:00,6-Aug-07,ISS,Prime,Saturn,APOMOVIEA,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for one rotation; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-218T05:00:00,000T02:16:32,6-Aug-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-218T14:35:00,000T09:00:00,6-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-218T23:35:00,000T00:33:00,6-Aug-07,INMS,Non-SPASS,Saturn,PTOTM123B,MAPS survey,MAPS Survey,Memory read out request.,,,,,, 2007-219T00:08:00,002T16:21:30,7-Aug-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-219T01:05:00,000T00:10:00,7-Aug-07,ISS,Prime,Saturn,APOMOVIEB,Apoapsis movie,WAC Saturn movie,1x2 WAC mosaic in 3 filters; picket of 0:10 duration.,,,,,, 2007-219T01:15:00,000T01:30:00,7-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_15,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn Spin Axis. 1) Slew about the Z-axis to +MOS Orb. Rotate +128mrad in the YZ plane. 2) Drift at a rate of .1033 mrad/sec about the Z-axis for 4000s toward -MOS Orb. 3) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 413.10mrad",,,,,, 2007-219T02:45:00,000T00:10:00,7-Aug-07,ISS,Prime,Saturn,APOMOVIEB,Apoapsis movie,WAC Saturn movie,1x2 WAC mosaic in 3 filters; picket of 0:10 duration.,,,,,, 2007-219T02:55:00,000T01:30:00,7-Aug-07,UVIS,Prime,Saturn,MOS48APOA,Apoapsis mosaic,MOSAIC_APO_48_15,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. Rotate +128mrad in the YZ plane. 2) Drift at a rate of .1033 mrad/sec about the Z-axis for 4000s toward +MOS Orb. 3) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 413.10 mrad",,,,,, 2007-219T02:55:00,000T01:30:00,7-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APOA,Apoapsis mosaic,CIRS_048IC_MOS48APOA015_UVIS,Calibration rider. Data Volume will be 21.6 Mb or less.,,,,,, 2007-219T04:25:00,000T00:10:00,7-Aug-07,ISS,Prime,Saturn,APOMOVIEB,Apoapsis movie,WAC Saturn movie,1x2 WAC mosaic in 3 filters; picket of 0:10 duration.,,,,,, 2007-219T04:35:00,000T02:00:00,7-Aug-07,UVIS,Prime,Saturn,MOS48APOB,Apoapsis mosaic,MOSAIC_APO_48_15,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn center to +MOS Orb. Rotate +128mrad in the YZ Plane. 2) Drift at a rate of .1033 mrad/sec about the Z-axis for 5800s toward -MOS Orb. 3) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 413.10mrad",,,,,, 2007-219T04:35:00,000T02:00:00,7-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APOB,Apoapsis mosaic,CIRS_048IC_MOS48APOB015_UVIS,Calibration rider. Data Volume will be 28.8 Mb or less.,,,,,, 2007-219T05:00:00,000T11:05:00,7-Aug-07,RSS,SPASS Rider,Earth,SCE4,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #4,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2007-219T07:05:00,000T09:00:00,7-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-219T08:00:00,000T08:00:00,7-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-219T16:35:00,000T19:30:00,7-Aug-07,ISS,Prime,Saturn,APOMOVIEC,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for two rotations; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-219T16:35:00,000T19:30:00,7-Aug-07,CIRS,SPASS Rider,Saturn,APOMOVIEC,Apoapsis movie,CIRS movie rider,something,,,,,, 2007-219T16:35:00,000T19:30:00,7-Aug-07,UVIS,SPASS Rider,Saturn,APOMOVIEC,Apoapsis movie,DAYGLOW OBSERVATION,,,,,,, 2007-219T16:35:00,000T19:30:00,7-Aug-07,VIMS,SPASS Rider,Saturn,APOMOVIEC,Apoapsis movie,TBD,TBD,,,,,, 2007-220T12:05:00,000T02:00:00,8-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_16,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn Center to -MOS Orb. 2) Drift at a rate of .1024mrad/sec about the Z-axis for 6000s toward +MOS Orb. 3) Slew back to Saturn center and reset pointing. MOS orb (+/-range): 409.68mrad",,,,,, 2007-220T12:05:00,000T02:00:00,8-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO016_UVIS,Calibration rider. Data Volume will be 28.8 Mb or less.,,,,,, 2007-220T12:30:00,000T11:05:00,8-Aug-07,RSS,SPASS Rider,Earth,SCE4,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #4,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2007-220T14:35:00,000T09:00:00,8-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-220T15:20:00,000T08:00:00,8-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-220T23:35:04,000T14:44:51,8-Aug-07,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2007-221T01:05:00,000T03:15:00,9-Aug-07,UVIS,Prime,Saturn,MOS48APO,Apoapsis mosaic,MOSAIC_APO_48_17,"Mosaic of Saturn inner magnetosphere. EUV and FUV low resolution slits on, aligned parallel with the Saturn spin axis. 1) Slew about the Z-axis from Saturn center to +MOS Orb. 2) Drift at a rate of .1018 mrad/sec about the Z-axis for 8000s to -MOS Orb. 3) Drift at indicated rate for 2000s toward +MOS Orb. 4) Slew back to Saturn center and reset pointing. Stare for remaining observation time. MOS orb (+/-range): 407.15 mrad",,,,,, 2007-221T01:05:00,000T03:15:00,9-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,MOS48APO,Apoapsis mosaic,CIRS_048IC_MOS48APO017_UVIS,Calibration rider. Data Volume will be 46.8 Mb or less.,,,,,, 2007-221T04:20:00,000T09:30:00,9-Aug-07,ISS,Prime,Saturn,APOMOVIEA,Apoapsis movie,NAC Southern Hemisphere Saturn movie,"4x4 BOTSIM mosaic in 2 filters of the Southern Hemisphere for one rotation; pickets of 1:10 duration, 6 repetitions with 1:40 spacing.",,,,,, 2007-221T04:20:00,000T09:30:00,9-Aug-07,CIRS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,CIRS movie rider,something,,,,,, 2007-221T04:20:00,000T09:30:00,9-Aug-07,UVIS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,DAYGLOW OBSERVATION,,,,,,, 2007-221T04:20:00,000T09:30:00,9-Aug-07,VIMS,SPASS Rider,Saturn,APOMOVIEA,Apoapsis movie,TBD,TBD,,,,,, 2007-221T04:30:00,000T02:16:32,9-Aug-07,CAPS,Non-SPASS,Saturn,BURST8K,8 kbps burst,Burst of 8kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data).,,,,,, 2007-221T12:15:00,000T11:05:00,9-Aug-07,RSS,SPASS Rider,Earth,SCE4,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #4,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2007-221T14:20:00,000T09:00:00,9-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-221T15:10:00,000T08:00:00,9-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-221T16:29:30,002T06:50:30,9-Aug-07,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2007-221T16:29:30,002T06:50:30,9-Aug-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-221T16:29:30,002T06:50:30,9-Aug-07,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-221T16:31:00,001T06:49:00,9-Aug-07,MIMI,Non-SPASS,co-rotation,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-221T16:45:42,002T06:34:18,9-Aug-07,CDA,Non-SPASS,DustRAM direction,2500DUST,Dust survey,Dust survey 0.22 11 Mbits/hour",,,,,, 2007-241T02:34:01,000T01:00:59,29-Aug-07,CDA,Non-SPASS,RingE,0800ERNGX,Ring plane crossing,E Ring Xing 0.0070 deg from dust ram.",,,,,, 2007-241T02:41:15,000T08:57:33,29-Aug-07,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-241T03:35:59,000T01:58:31,29-Aug-07,CDA,Non-SPASS,DustRAM direction,0700DUST,Dust survey,E Ring dense - survey - 0.07AD>11 mrad, phase~45, sub_S/C~(1,192), LT~9. Duration 01:10. CIRS 3 cm-1, blink, shutter closed first, last 5 min.",,,,,, 2007-242T05:58:55,000T01:07:00,30-Aug-07,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea close flyby,1x1 mosaic of Rhea center,,,,,, 2007-242T05:58:55,000T01:07:00,30-Aug-07,UVIS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map of Rhea and Limb Drifts,Map surface albedo of Rhea in UV. Limb drifts to determine atmospheric scattering. Carry out North-south scan(s) at 30 urad/sec slew rate.,,,,,, 2007-242T06:33:00,000T06:52:00,30-Aug-07,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-242T07:34:00,000T13:15:00,30-Aug-07,CDA,Non-SPASS,DustRAM direction,0800DUST,Dust survey,Ring Margin Survey,,,,,,, 2007-242T07:34:00,000T09:00:00,30-Aug-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-242T08:34:00,000T03:45:00,30-Aug-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-242T12:00:00,000T05:34:00,30-Aug-07,RSS,SPASS Rider,Earth,SCE4,Solar Corona Experiment,Solar Conjunction Experiment (SCE) #4,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2007-242T13:25:00,000T13:07:34,30-Aug-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-242T13:25:01,000T15:07:33,30-Aug-07,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-242T16:34:00,000T00:41:00,30-Aug-07,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-242T17:15:00,001T23:05:00,30-Aug-07,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-242T18:32:34,000T11:00:00,30-Aug-07,INMS,Non-SPASS,Titan,T35INBD,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2007-242T20:49:00,000T04:45:00,30-Aug-07,CDA,Non-SPASS,DustRAM direction,0800DUST,Dust survey,Ring Margin Survey,,,,,,, 2007-242T21:32:34,000T04:00:00,30-Aug-07,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2007-242T21:32:34,000T04:00:00,30-Aug-07,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2007-242T21:32:34,000T04:00:00,30-Aug-07,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),search for and monitor lightning/aurora,,,,,, 2007-242T21:32:34,000T04:00:00,30-Aug-07,VIMS,SPASS Rider,Titan,MIDIRLIMB,Mid infrared limb map,CIRS Mid IR limb,CIRS mid IR limb map and limb comp ridealong. Template R.,,,,,, 2007-243T01:32:34,000T03:00:00,31-Aug-07,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk.",,,,,, 2007-243T01:32:34,000T03:00:00,31-Aug-07,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2007-243T01:32:34,000T03:00:00,31-Aug-07,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),search for and monitor lightning/aurora,,,,,, 2007-243T01:32:34,000T03:00:00,31-Aug-07,VIMS,SPASS Rider,Titan,CIRSFP1,,CIRS FP!,CIRS FP1 slow scan ridelaong. Template T.,,,,,, 2007-243T01:34:00,014T09:50:46,31-Aug-07,CDA,Non-SPASS,DustRAM direction,1700DUST,Dust survey,Dust survey 0.08AD>11.7, phase=146, sub-S/C=(11, 64).",,,,,, 2007-252T22:25:00,000T01:30:00,9-Sep-07,CIRS,SPASS Rider,Iapetus,NITPOLRIZ,,4 WACs to support polarization pointing,"4 compressed WAC images (0.5 Mb each) for pointing verification. Frame at 2007-252T22:44, 2007-252T22:53, 2007-252T23:14, and 2007-252T23:23.",,,,,, 2007-252T22:25:00,000T01:30:00,9-Sep-07,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-252T22:25:00,000T01:30:00,9-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,TBD,Ride along with CIRS FP1,,,,,, 2007-252T23:55:00,000T02:50:00,9-Sep-07,RADAR,Prime,Iapetus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Iapetus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2007-253T02:45:00,000T01:35:00,10-Sep-07,VIMS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,"64i2-32v1 80ms, 640 ms (28 min/cycle) 1x2 mosaic each hour",,,,,, 2007-253T02:45:00,000T01:35:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,VIMS rider,"VIMS rider for high spectral resolution and phase coverage. Duration: 00:55. CIRS: 96 RTI (2.85 cm-1, 12 sec/frame), blink. Shutter closed 00:10 to 00:16, 00:44 to 00:50.",,,,,, 2007-253T02:45:00,000T01:35:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-253T03:55:00,000T04:50:00,10-Sep-07,RSS,SPASS Rider,Iapetus,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band for Iapetus gravity science and for improving locally Cassini orbit. The second pass is provided by already scheduled RSS tracking.,,,,,, 2007-253T04:20:00,000T01:06:00,10-Sep-07,ISS,Prime,Iapetus,SATUSHINE,,Iapetus global mapping and polar mapping in saturn,"Do 1x4 mosaic on bright crescent, 1x3 mosaic on southern leading side, 1x3 mosaic on northern leading side, 1 ftprt over ridge near 130W, 1 ftprt over landslide crater.",,,,,, 2007-253T04:20:00,000T01:06:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,GRAYNORTH,,ISS rider,"ISS rider. AD=17.6, phase=146, LT=21.8, (10, 65). Duration 00:30. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:05 to 00:08, 00:22 to 00:25.",,,,,, 2007-253T04:20:00,000T01:06:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-253T04:20:00,000T00:06:00,10-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus,"24i2-36v3 vis 160ms, 640 ir/pixel, continuous, ride along with ISS for 1/2 hours",,,,,, 2007-253T05:26:00,000T00:34:00,10-Sep-07,CIRS,SPASS Rider,Earth,WAYPTTURN,Waypoint turn,SP rider for deep space calibration,"SP rider for deep space calibration. Duration 00:20. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:06 to 00:10; then NODATA 00:10 to 00:20.",,,,,, 2007-253T06:00:00,000T02:45:00,10-Sep-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-253T08:44:53,000T02:20:47,10-Sep-07,RADAR,SPASS Rider,Other,WARMUP4IA,RADAR warmup,Warmup Radiometer before Iapetus,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2007-253T08:50:40,000T02:15:00,10-Sep-07,CIRS,Prime,Iapetus,FP1NITMAP,CIRS FP1 dark side map,Incoming dark side FP1 map,"Incoming darkside FP1 map. AD=37-50 mrad, phase=145, sub-s/c=(10, 67)= west central Cassini Regio, LT=21.7. CIRS 39 RTI (15.5 cm-1) Nyquist-sampled FP1 map of disk; construct to cover as much as possible (if any extra time, use it for integration at center of disk at BEGINNING of observation, OR for small FP3 map). FP1 (and time for SOME FP3; for FP3: center detectors, shutter closed first and last 3 min of FP3 period. May have up to 30 min with FP3 if no FP4 - which will exceed time left over after FP1 map).",,,,,, 2007-253T08:50:40,000T02:15:00,10-Sep-07,ISS,SPASS Rider,Iapetus,FP1NITMAP,CIRS FP1 dark side map,Iapetus I49 targeted flyby observation,CIRS scan,,,,,, 2007-253T08:50:40,000T02:15:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,"ICYMAP: Iapetus UV Map, Rider on ORS",UV albedo of Iapetus' surface,,,,,, 2007-253T08:50:40,000T02:15:00,10-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,TBD,Ride along with CIRS FP1,,,,,, 2007-253T11:05:40,000T01:25:00,10-Sep-07,RADAR,Prime,Iapetus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Iapetus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2007-253T11:39:16,000T02:00:00,10-Sep-07,MIMI,SPASS Rider,Iapetus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-253T12:15:40,000T04:00:00,10-Sep-07,MAG,Non-SPASS,Iapetus,IATAR,Iapetus targeted flyby,Iapetus targeted flyby,Monitor the interaction of Iapetus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field. NOTE:- rate below assumes continuous 600bps survey will be added to make up the total rate (total rate required is 1976 bps),,,,,, 2007-253T12:30:40,000T00:01:00,10-Sep-07,ISS,Prime,Iapetus,CASSREG,,Iapetus I49 targeted flyby imaging,Do BOTSIM over +2/130.,,,,,, 2007-253T12:30:40,000T00:25:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,ISSUVIS,ISS ride along activity on UVIS observation,ISS/UVIS rider,"ISS rider. AD=11-27, phase=141-131, LT=21.5-20.7, (8, 72)-(3, 83). Duration 01:13. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:05 to 00:10, 01:00 to 01:05.",,,,,, 2007-253T12:30:40,000T00:01:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,"ICYMAP: Iapetus UV Map, Rider on ORS",UV albedo of Iapetus' surface,,,,,, 2007-253T12:31:40,000T00:24:00,10-Sep-07,UVIS,Prime,Iapetus,ICYMAP,Icy satellite surface map,"ICYMAP: Iapetus UV Map, Rider on ORS",UV albedo of Iapetus' surface,,,,,, 2007-253T12:31:40,000T00:24:00,10-Sep-07,ISS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,Iapetus I49 targeted flyby imaging,Do BOTSIMs while UVIS is prime,,,,,, 2007-253T12:55:40,000T00:25:00,10-Sep-07,UVIS,Prime,Iapetus,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to star.,,,,,, 2007-253T12:55:40,000T00:25:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,ICYEXO,Icy satellite exosphere,UVIS rider,"UVIS rider. AD=30, phase=130-90 or so, LT=20-12 or so, (0, 90)-(-10, 140) or so. Duration 00:37. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:05 to 00:09, 00:28 to 00:32.",,,,,, 2007-253T12:55:40,000T00:25:00,10-Sep-07,ISS,SPASS Rider,Iapetus,ICYEXO,Icy satellite exosphere,Iapetus I49 targeted flyby imaging,Do a few NAC and WAC frames of south pole while UVIS tracks SigSgr,,,,,, 2007-253T12:55:40,000T00:25:00,10-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,TBD,Ride along with UVIS occultation,,,,,, 2007-253T13:15:40,000T00:30:00,10-Sep-07,CAPS,SPASS Rider,Iapetus,ENCOUNTER,MAPS Campaign,MAPS 049IA Campaign,Part of 049IA MAPS Campaign. Observe interaction between Iapetus and the solar wind,,,,,, 2007-253T13:15:40,000T02:00:00,10-Sep-07,INMS,Non-SPASS,Iapetus,I1CLOSE,Iapetus observation,Iapetus Observation,Iapetus Observation. Greg Fletcher is in the process of requesting full data rate for 1 hour before and after Iapetus closest approach.,,,,,, 2007-253T13:20:40,000T03:55:00,10-Sep-07,VIMS,Prime,Iapetus,ORSHIRES,High resolution observation,Iapetus,Best long+short exposure we can do along with other instruments. ISS works with vims on pointing design.,,,,,, 2007-253T13:20:40,000T03:55:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,ORSHIRES,High resolution observation,Iapetus rider with VIMS,"Long rider on Iapetus (through C/A!). 17756, 130>phase>C/A=59>30, (9,83)-(-4,156)-(-11,242). 15.5 cm-1, blink,.... but must request space every hour or so because phase angle changes substantially, and therefore the exposure of CIRS to sunlight.",,,,,, 2007-253T13:20:40,000T03:55:00,10-Sep-07,ISS,SPASS Rider,Iapetus,ORSHIRES,High resolution observation,Iapetus I49 targeted flyby imaging,Do various NAC mosaics plus WAC context,,,,,, 2007-253T13:20:40,000T03:55:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,"ICYMAP: Iapetus UV Map, Rider on ORS",UV albedo of Iapetus' surface,,,,,, 2007-253T13:39:18,003T22:03:49,10-Sep-07,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-253T13:45:40,000T01:00:00,10-Sep-07,CAPS,SPASS Rider,Iapetus,ENCOUNTER,MAPS Campaign,MAPS 049IA Campaign,Part of 049IA MAPS Campaign. Observe interaction between Iapetus and the solar wind,,,,,, 2007-253T13:45:40,000T01:00:00,10-Sep-07,CDA,Non-SPASS,Iapetus,IAPDUST,Iapetus dust study,Dust envelope around Iapetus,Study dust envelope around Iapetus. pointing: CDA boresight to dust RAM power: 19 W (with articulation) data volume: 2 Mbits data rate: 524 bps,,,,,, 2007-253T13:45:40,000T00:35:00,10-Sep-07,RPWS,Non-SPASS,Iapetus,IACA,Iapetus closest approach,Iapetus closest approach observations,"RPWS observations in the immediate vicinity of Iapetus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: Don't care",,,,,, 2007-253T14:20:40,000T00:25:00,10-Sep-07,RPWS,Non-SPASS,Iapetus,IACA,Iapetus closest approach,Iapetus closest approach observations,"RPWS observations in the immediate vicinity of Iapetus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: Don't care",,,,,, 2007-253T14:45:40,000T00:30:00,10-Sep-07,CAPS,SPASS Rider,Iapetus,ENCOUNTER,MAPS Campaign,MAPS 049IA Campaign,Part of 049IA MAPS Campaign. Observe interaction between Iapetus and the solar wind,,,,,, 2007-253T14:45:40,002T08:31:07,10-Sep-07,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-253T15:15:40,003T20:27:27,10-Sep-07,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2007-253T15:15:40,003T06:04:20,10-Sep-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-253T16:15:40,002T05:19:20,10-Sep-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-253T17:15:40,000T02:00:00,10-Sep-07,CIRS,Prime,Iapetus,FP1DAYMAP,CIRS FP1 daytime map,Outgoing dayside FP1 map,"PREVIOUS REMARKS: Shortened 20 minutes to 01:10; must redesign. 7/18/04. Outgoing dayside FP1 map. AD=52-36 mrad, phase=31, sub-s/c=(-12, 243)= Roncevaux Terra, LT=10.1. Duration=01:30 CIRS 38 RTI (15.67 cm-1, 4.75 sec./scan) Nyquist-sampled FP1 map of disk; construct to cover as much as possible (if any extra time, use it for integration at center of disk at END of observation). FP1 and FP3 only; for FP3: center detectors, shutter closed 00:10-00:15 and 01:20-01:25 NEW DESIGN REQUIREMENTS (3/19/07): First 30 min FP3, then FP1 map; last 30 min FP3 (time extended from 01:10 to 02:00). Include FP4, so use all focal planes.",,,,,, 2007-253T17:15:40,000T02:00:00,10-Sep-07,ISS,SPASS Rider,Iapetus,FP1DAYMAP,CIRS FP1 daytime map,Iapetus I49 targeted flyby observation,CIRS scan; ISS high-res. shutters,,,,,, 2007-253T17:15:40,000T02:00:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-253T17:15:40,000T02:00:00,10-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,TBD,Ride along with CIRS FP1 Surface resolution 12-17 km (nom pixel),,,,,, 2007-253T18:00:00,000T04:20:00,10-Sep-07,RSS,SPASS Rider,Iapetus,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band for Iapetus gravity science and for improving locally Cassini orbit. The second pass is provided by already scheduled RSS tracking.,,,,,, 2007-253T19:15:40,000T00:44:00,10-Sep-07,VIMS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus trailing side,"64i2-32v1 80ms, 640 ms (28 min/cycle) repeat 2 each hour

Reaction Wheels Required 1x2 mosaic desired for cirs.",,,,,, 2007-253T19:15:40,000T00:44:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,VIMS rider,"VIMS rider. AD=35, phase=32, LT=10.0, (-11, 245). Duration 00:35. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:05 to 00:08, 00:25 to 00:28. Note that this gets good space data, as it turns to Earth.",,,,,, 2007-253T19:15:40,000T00:44:00,10-Sep-07,ISS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus I49 targeted flyby imaging,1x1 mosaic of big basin; 1x1 multi-color of equat. transition zone,,,,,, 2007-253T19:15:40,000T00:44:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,"ICYMAP: Iapetus UV Map, Rider on ORS",UV albedo of Iapetus' surface,,,,,, 2007-253T20:05:00,000T02:25:00,10-Sep-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-253T22:20:00,000T00:20:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,WAYPTTURN,Waypoint turn,SP rider for deep space calibration,"SP rider for deep space calibration. Duration 00:20. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:00 to 00:05; with shutter open 00:05 to 00:20.",,,,,, 2007-253T22:20:00,000T04:40:00,10-Sep-07,RADAR,SPASS Rider,Other,WARMUP4IA,RADAR warmup,Warmup Radiometer before Iapetus,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2007-253T22:40:00,000T02:00:00,10-Sep-07,ISS,Prime,Iapetus,REGMAPTRL,,Iapetus I49 targeted flyby imaging,Do 15 NAC ftprts mosaic plus 2 saturnshine ftprts plus 1x4 multi-color mosaic,,,,,, 2007-253T22:40:00,000T02:00:00,10-Sep-07,CIRS,SPASS Rider,Iapetus,REGMAPTRL,,ISS rider,"ISS rider. AD=16, phase=33, LT=10, (-10, 247). Duration 00:40. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:05 to 00:08, 00:30 to 00:35.",,,,,, 2007-253T22:40:00,000T02:00:00,10-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-253T22:40:00,000T02:00:00,10-Sep-07,VIMS,SPASS Rider,Iapetus,REGMAPTRL,,Iapetus,"24i2-36v3 vis 80ms ir/pixel, 1 min/cycle, continuous, ride along with ISS for 2.5 hours during closest flyby",,,,,, 2007-254T00:40:00,000T01:40:00,11-Sep-07,CIRS,Prime,Iapetus,DAYPOLRIZ,,FP1 surface polarization measurement,"Search for FP1 polarization within 50 - 400 cm-1 range. Design: deep space, polarizer parallel to limb, polarizer perpendcular to limb, deep space. Phase= 33.8, Local time= 9.9, sub S/C=( -10.6, 248.3), AD= 11.8 mrad. Note that data multiplier is an odd one because we need only 2 Mb for support images.",,,,,, 2007-254T00:40:00,000T01:40:00,11-Sep-07,CIRS,SPASS Rider,Iapetus,DAYPOLRIZ,,4 WACs to support polarization pointing,"4 compressed WAC images (0.5 Mb each) for pointing verification. Frame at 2007-254T01:01, 2007-254T01:08, 2007-254T01:29, and 2007-254T01:36.",,,,,, 2007-254T00:40:00,000T01:40:00,11-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-254T02:20:00,000T00:40:00,11-Sep-07,ISS,Prime,Iapetus,REGCOLTRL,,Iapetus regional color observation,Do 1x1 mosaic over moat crater; do 1x1 mosaic (multi-color) over equat. transition terrain,,,,,, 2007-254T02:20:00,000T00:40:00,11-Sep-07,CIRS,SPASS Rider,Iapetus,REGCOLTRL,,ISS rider,"ISS rider. AD=13, phase=34, LT=9.9, (-10, 247). Duration 00:50. CIRS: blink, 38 RTI (15.7 cm-1, 4.75 sec/frame). Shutter closed 00:05 to 00:10, 00:40 to 00:45.",,,,,, 2007-254T02:20:00,000T00:40:00,11-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-254T02:20:00,000T00:40:00,11-Sep-07,VIMS,SPASS Rider,Iapetus,REGCOLTRL,,Iapetus,"24i2-36v3 vis 80ms ir/pixel, 1 min/cycle, continuous, ride along with ISS for 50 min",,,,,, 2007-254T03:00:00,000T02:10:00,11-Sep-07,RADAR,Prime,Iapetus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Iapetus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2007-254T05:30:00,000T14:55:00,11-Sep-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-254T06:15:00,000T05:25:00,11-Sep-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-254T20:45:00,000T02:15:00,11-Sep-07,VIMS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,"36i2-54v3 80ms, 640 ms (10 min/cycle) repeat 3 each hour",,,,,, 2007-254T20:45:00,000T02:15:00,11-Sep-07,ISS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus global color observation,Do NAC 1x1 multi-color imaging.,,,,,, 2007-254T20:45:00,000T02:15:00,11-Sep-07,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-254T23:00:00,000T04:00:00,11-Sep-07,CIRS,Prime,Iapetus,FP1FP3MAP,CIRS FP1 integration / FP3 map,"FP1 stare, FP3 map of Iapetus.","FP1 observation of Iapetus for high spectral resolution integration for composition, and for phase angle coverage. Phase= 34.0, Local time= 9.9, sub S/C=( -10.4, 252.5), AD= 4.9 mrad. Duration= 04:00 (accommodate other ORS?). Delete FP4 070629.",,,,,, 2007-254T23:00:00,000T04:00:00,11-Sep-07,RADAR,SPASS Rider,Other,WARMUP4IA,RADAR warmup,Warmup Radiometer before Iapetus,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2007-254T23:00:00,000T04:00:00,11-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-255T03:00:00,000T03:00:00,12-Sep-07,RADAR,Prime,Iapetus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Iapetus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2007-255T06:00:00,000T04:35:00,12-Sep-07,ISS,Prime,Saturn,STRMOVIEE,WAC Saturn movie,WAC Saturn movie,"1x2 WAC mosaic in 6 filters for half a rotation; pickets of 0:10 duration, 3 repetitions with 1:40 spacing.",,,,,, 2007-255T06:00:00,000T04:35:00,12-Sep-07,VIMS,SPASS Rider,Saturn,STRMOVIEE,WAC Saturn movie,Saturn,Saturn movie ride along with ISS,,,,,, 2007-255T07:05:00,000T04:00:00,12-Sep-07,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-255T10:35:00,000T00:30:00,12-Sep-07,ISS,Prime,Iapetus,LIMBTOPOI,Limb topography and geodesy observation,Iapetus limb topography and geodesy observation,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2007-255T12:35:00,000T09:00:00,12-Sep-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-255T13:35:00,000T08:00:00,12-Sep-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-255T21:35:00,009T00:01:00,12-Sep-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-255T21:35:00,001T14:08:07,12-Sep-07,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-255T22:05:00,000T05:30:00,12-Sep-07,CIRS,Prime,Iapetus,IAPETUS,Iapetus observation,ORS phase coverage.,"CIRS_049IA_IAPETUS004_PRIME 2007-255T22:20 (05:30) 2007-256T03:50. AD=2.8 mrad, phase=34, LT=9.9, (-10, 257)=just S of Roncevaux Terra. 1) Turn from waypoint (00:25); CIRS FP1 to Iapetus disk center for 01:11; 2) 5.8 mrad scan across disk with CIRS FP3 at 3 microrad/sec for 00:33. Repeat for 00:33; 3) ISS NAC centered on disk for 01:11; 4) CIRS FPB centered on disk for 01:11. 5) Return to waypoint (00:25); add or subtract time from (1) to make 05:30 duration.",,,,,, 2007-255T22:05:00,000T05:30:00,12-Sep-07,ISS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus limb topography and geodesy observation,Do 1x1 mosaic at start and end of request.,,,,,, 2007-255T22:05:00,000T05:30:00,12-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-255T22:05:00,000T05:30:00,12-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,TBD,ride with CIRS FP1,,,,,, 2007-256T00:00:00,000T00:34:08,13-Sep-07,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,Calibration/Gain curve of ELS sensor,Calibration/gain curve of ELS sensor. 8 B cycles duration in 16 kbps. Data is in addition to 1000 bps from SWSKR.,,,,,, 2007-256T03:35:00,000T03:15:00,13-Sep-07,VIMS,Prime,rings(general),APOMOSAIC,Apoapsis mosaic,APOAPSE_MOSAIC,"Orbits = 026-074, Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 24, Number of SC pointings = 4-30, Time of observation (hours) = 1.5-11, Volume (Mbits) = 69-519 Mosaic of entire ring system near apoapse. Unlit face. Various mosaic sizes (4x1 - 6x5)., Desc = Orbits = 049-049, Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 30, Number of SC pointings = 2-4, Time of observation (hours) = 1.0-2.0, Volume (Mbits) = 69-138, Desc = Mosaic of entire ring system near apoapse. Sunlit face.Various mosaic sizes (2x1 - 4x1). 1x3",,,,,, 2007-256T03:35:00,000T03:15:00,13-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-256T06:50:00,000T04:00:00,13-Sep-07,ISS,Prime,InstrumentCalibration,CALLAMP,ISS Wide angle camera calibration lamp exposure,ISS WAC CAL LAMP,ISS WAC Cal Lamp exposures,,,,,, 2007-256T06:50:00,000T04:00:00,13-Sep-07,CIRS,SPASS Rider,InstrumentCalibration,CALLAMP,ISS Wide angle camera calibration lamp exposure,CIRS_049IC_CALLAMP001_ISS,Calibration rider. Data Volume will be 57.6 Mb or less.,,,,,, 2007-256T12:20:00,000T09:00:00,13-Sep-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-256T21:20:00,001T00:01:00,13-Sep-07,INMS,Non-SPASS,Saturn,PTOTM128,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-256T21:50:00,000T03:00:00,13-Sep-07,CIRS,Prime,Iapetus,IAPETUS,Iapetus observation,ORS phase/longitude coverage,"CIRS_049IA_IAPETUS005_PRIME 2007-256T21:50 (03:00) 2007-257T00:50. AD=2.1 mrad, phase=34, LT=9.9, (-10, 261)=just S of Roncevaux Terra. (Note shortened duration) 1) Turn from waypoint (00:25); CIRS FP1 to Iapetus disk center for 00:34; 2) 5.0 mrad scan across disk with CIRS FP3 at 3 microrad/sec for 00:28; 3) ISS NAC centered on disk for 00:34; 4) CIRS FPB centered on disk for 00:34. 5) Return to waypoint (00:25); add or subtract time from (1) to make 03:00 duration.",,,,,, 2007-256T21:50:00,000T03:00:00,13-Sep-07,ISS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus limb topography and geodesy observation,Do 1x1 mosaic of Iapetus at start and end of request.,,,,,, 2007-256T21:50:00,000T03:00:00,13-Sep-07,UVIS,SPASS Rider,Iapetus,ICYMAP,Icy satellite surface map,ICYMAP: Iapetus UV Map,UV albedo of Iapetus' surface,,,,,, 2007-256T21:50:00,000T03:00:00,13-Sep-07,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,TBD,TBD,,,,,, 2007-257T00:50:00,000T11:00:00,14-Sep-07,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_049SA_COMPSIT09,"Measure oxygen compounds (H2O, CO2) in startosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole",,,,,, 2007-257T00:50:00,000T10:34:00,14-Sep-07,CDA,SPASS Rider,Other,DECON,Decontamination,Decontamination,"CDA boresight off-sun, no resources (Watts, bps) resources covered by other requests",,,,,, 2007-257T00:50:00,000T11:00:00,14-Sep-07,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,TBD,TBD,,,,,, 2007-257T11:37:51,000T00:00:01,14-Sep-07,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 32.0 d, inc = 6.1 deg, r = 59.7 Rs, phase = 42 deg",,,,,, 2007-257T11:43:07,006T12:16:53,14-Sep-07,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2007-257T11:43:07,008T09:07:53,14-Sep-07,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2007-257T11:43:07,008T09:07:53,14-Sep-07,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-257T11:54:47,008T08:56:13,14-Sep-07,CDA,Non-SPASS,DustRAM direction,1105DUST,Dust survey,Dust survey 4.75100 deg, size ~ 20 pixels ? If ISS stare, do bigger frames ideally alternate 160ms, 640ms frames",,,,,, 2007-273T00:00:00,000T03:00:00,30-Sep-07,RADAR,Prime,Dione,SCATTRAD,RADAR Scatterometry / Radiometry,Simultaneous Scatterometry & Radiometry of Dione,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2007-273T00:48:00,000T09:24:01,30-Sep-07,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-273T03:00:00,000T00:20:00,30-Sep-07,ISS,Prime,Dione,REGMAPE,Regional map,Dione regional mapping,Do 7-ftprt mosaic,,,,,, 2007-273T03:00:00,000T00:20:00,30-Sep-07,CIRS,SPASS Rider,Dione,ISSRIDER,ISS ride along activity,ISS rider on Dione,"FP1 observation of Tethys for high spectral resolution integration for composition, and for phase angle coverage. Phase= 90.7, Local time= 6.0, sub S/C=( 0.6, 120.9), AD= 20.4 mrad. Duration: 00:30. CIRS: 38 RTI (4.75 sec/frame), blink, FP1 and FP3 only. Shutter closed 00:05 to 00:10 and 00:50 to 00:55.",,,,,, 2007-273T03:00:00,000T00:20:00,30-Sep-07,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-273T03:00:00,000T00:20:00,30-Sep-07,VIMS,SPASS Rider,Dione,REGMAPE,Regional map,Dione,"Follow ISS, probably 12x24 double res IR phase ~ 90 deg, size ~ 30 pixels If ISS stare, do bigger frames ideally alternate 160ms, 640ms frames",,,,,, 2007-273T03:00:00,000T10:30:00,30-Sep-07,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,data volume,DV for ERing measurements,,,,,, 2007-273T03:20:00,000T00:30:00,30-Sep-07,CIRS,Prime,Dione,FP1AMATA,,new name,"Afternoon over Amata. Make a localized Nyquist FP3 mosaic to the south of Amata, at 3 cm-1 resolution using pairs of detectors. Interesting variability in wispy terrain. Pair with subsequent 050DI_FP1FAZ0P5029 data. AD=15.2-15.9 mrad, phase=84-79, (-9, 261), LT=17. Duration=00:30. Waypoint is Dione. Two 5 mrad scans of FP3 in X (turn about Z) at 6 urad/sec. The first centered on (-10, 285); the second (the return) moved north by one FP3 pixel (0.3 mrad). 00:28 Adjust scan length to fill alotted time. CIRS: Pairs, 3 cm-1 resolution (96 RTI, 12 sec/frame), shutter closed first and last 2 min.",,,,,, 2007-273T03:20:00,000T00:30:00,30-Sep-07,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-273T03:50:00,000T01:00:00,30-Sep-07,VIMS,Prime,Dione,DIONE,Dione,Dione,"42i2-63v3 80ms, 640 ms (13 min/cycle) 1x2 mosaic done 4 times, then 2x2 mosaics (1hr each) repeat 4 times (5.1 Mbit/cycle uncompressed)",,,,,, 2007-273T03:50:00,000T01:00:00,30-Sep-07,CIRS,SPASS Rider,Dione,VIMSRIDER,,VIMS rider on Dione,"FP1 observation of Tethys for high spectral resolution integration for composition, and for phase angle coverage. Phase= 90.7, Local time= 6.0, sub S/C=( 0.6, 120.9), AD= 20.4 mrad. Note that for objects of small apparent size, the 4 mrad +X offset of CIRS FP1 may make this observation incompatible with simultaneous UVIS and NAC observations; VIMS retains adequate overlap for simultaneous observations.",,,,,, 2007-273T03:50:00,000T01:00:00,30-Sep-07,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-273T04:00:03,000T04:53:54,30-Sep-07,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2007-273T04:50:00,000T01:30:00,30-Sep-07,ISS,Prime,Enceladus,PLUMES,Observe Enceladus' plumes,ENCELADUS High-Resolution Plumes Observation,Enceladus high-resolution plume observation at 155-deg. phase. Viewed perpendicular to tiger stripes.,,,,,, 2007-273T04:50:00,000T01:30:00,30-Sep-07,CIRS,SPASS Rider,Enceladus,PLUMES,Observe Enceladus' plumes,Rider on plume observation,.,,,,,, 2007-273T04:50:00,000T01:30:00,30-Sep-07,UVIS,SPASS Rider,Enceladus,PLUMES,Observe Enceladus' plumes,ICYLON: Longitude / Phase Space Coverage + Plumes,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-273T04:50:00,000T01:03:00,30-Sep-07,VIMS,SPASS Rider,Enceladus,PLUMES,Observe Enceladus' plumes,Dione,"Follow ISS, enceladus plume observation, 640ms exposures",,,,,, 2007-273T06:20:00,000T00:40:00,30-Sep-07,ISS,Prime,Dione,REGMAPF,Regional map,Dione regional mapping and regional color,Do 20 ftprts mosaic.,,,,,, 2007-273T06:20:00,000T00:40:00,30-Sep-07,CIRS,SPASS Rider,Dione,ISSRIDER,ISS ride along activity,ISS rider on Dione,"FP1 observation of Tethys for high spectral resolution integration for composition, and for phase angle coverage. Phase= 90.7, Local time= 6.0, sub S/C=( 0.6, 120.9), AD= 20.4 mrad. Note that for objects of small apparent size, the 4 mrad +X offset of CIRS FP1 may make this observation incompatible with simultaneous UVIS and NAC observations; VIMS retains adequate overlap for simultaneous observations.",,,,,, 2007-273T06:20:00,000T00:40:00,30-Sep-07,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-273T06:20:00,000T00:40:00,30-Sep-07,VIMS,SPASS Rider,Dione,REGMAPF,Regional map,Dione,"Follow ISS, probably 12x24 double res IR phase ~20 deg, size ~ 32 pixels If ISS stare, do bigger frames ideally alternate 160ms, 640ms frames",,,,,, 2007-273T07:00:00,000T00:45:00,30-Sep-07,VIMS,Prime,Dione,DIONE,Dione,Dione,"42i2-63v3 80ms, 640 ms (13 min/cycle) 1x2 mosaic done 4 times, then 2x2 mosaics (1hr each) repeat 4 times",,,,,, 2007-273T07:00:00,000T00:45:00,30-Sep-07,CIRS,SPASS Rider,Dione,VIMSRIDER,,VIMS rider on Dione,"FP1 observation of Tethys for high spectral resolution integration for composition, and for phase angle coverage. Phase= 90.7, Local time= 6.0, sub S/C=( 0.6, 120.9), AD= 20.4 mrad. Note that for objects of small apparent size, the 4 mrad +X offset of CIRS FP1 may make this observation incompatible with simultaneous UVIS and NAC observations; VIMS retains adequate overlap for simultaneous observations.",,,,,, 2007-273T07:00:00,000T00:45:00,30-Sep-07,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-273T07:15:52,000T14:25:44,30-Sep-07,CDA,Non-SPASS,DustRAM direction,0501DUST,Dust survey,E Ring dense - survey - 0.8070 deg from dust ram.",,,,,, 2007-297T03:45:00,000T00:29:00,24-Oct-07,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,,rider,,,,,, 2007-297T04:49:49,000T01:35:00,24-Oct-07,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS Atm. Ingress Occultation 051,"This is for the RSS occultation INGRESS of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2007-297T04:49:49,000T02:24:00,24-Oct-07,CDA,SPASS Rider,Saturn,MIDRSSOCC,,E Ring Xing 0.00Arcturus: multiple sets of 10 cubes w/64x4 FOV IR @ 160 ms, VIS @ 10160 ms; Time: 8.0 hr; Volume: 125 Mbits; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Arcturus; Secondary: +z to TBD",,,,,, 2007-302T22:50:00,000T04:30:00,29-Oct-07,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Suitable periods for S34 are from day 278 to 290, 302 to 315 (ends in S35). The last allocated roll prior to this is on day 264. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equtorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2007-303T03:20:00,000T00:30:00,30-Oct-07,ISS,Prime,Rhea,310W013PH,Spectrophotometery,Rhea spectrophotometry/ phase coverage,Turn -Y to Rhea; do 1x1 mosaic; turn to WP,,,,,, 2007-303T03:20:00,000T00:30:00,30-Oct-07,UVIS,SPASS Rider,Rhea,310W013PH,Spectrophotometery,,,,,,,, 2007-303T03:20:00,001T15:20:00,30-Oct-07,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2007-303T03:50:00,000T04:20:00,30-Oct-07,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images. Distance to Saturn -s 2 million Km. Phase is 0-145,,,,,, 2007-303T03:50:00,000T15:20:00,30-Oct-07,CDA,Non-SPASS,Other,DECONBCK,Decontamination,Decontamination - Backup,"CDA boresight off-sun, no resources (Watts, bps), resources covered by other request. Placeholder for RT-Decon Activity in case prime decon via S34M needs to be skipped. See also SCRs 106727 and 106755",,,,,, 2007-303T08:40:00,000T09:00:00,30-Oct-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-303T09:40:00,000T08:00:00,30-Oct-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-303T09:40:00,000T07:00:00,30-Oct-07,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-303T17:41:00,000T15:58:00,30-Oct-07,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-303T18:10:00,000T01:00:00,30-Oct-07,ISS,Prime,Dione,022W025PH,Spectrophotometery,Dione spectrophotometry/ phase coverage,Turn -Y to Dione; do 1x1 mosaic; turn to WP,,,,,, 2007-303T18:10:00,000T01:00:00,30-Oct-07,UVIS,SPASS Rider,Dione,022W025PH,Spectrophotometery,,,,,,,, 2007-303T19:10:00,000T01:40:00,30-Oct-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 044 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-303T20:50:00,000T00:30:00,30-Oct-07,ISS,Prime,Tethys,022W024PH,Spectrophotometery,Tethys spectrophotometry/ phase coverage,Turn -Y to Tethys; do 1x1 mosaic; turn to WP,,,,,, 2007-303T20:50:00,000T00:30:00,30-Oct-07,UVIS,SPASS Rider,Tethys,022W024PH,Spectrophotometery,,,,,,,, 2007-303T21:40:00,000T11:30:00,30-Oct-07,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_051SA_MIRMAP29,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2007-304T09:40:00,000T09:00:00,31-Oct-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-304T10:35:00,000T08:00:00,31-Oct-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-304T10:40:00,000T07:00:00,31-Oct-07,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-304T18:40:00,002T08:20:00,31-Oct-07,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-304T18:40:00,002T15:00:00,31-Oct-07,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,"Part of SW2 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observs the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2007-304T18:40:00,004T13:40:19,31-Oct-07,CDA,Non-SPASS,DustRAM direction,2500DUST,Dust survey,Dust survey 0.28Pleiades: multiple cubes w/64x64 FOV IR @ 640 ms, VIS @ 40000 ms; Time: 7.0 hr 47 min; Volume: 86.5 Mbits; CompRatio: 2.0

Turn to waypoint: 30 min

Primary: -y to Pleiades; Secondary: +z to TBD

Not time critical.

RWA REQUIRED.",,,,,, 2007-318T02:56:00,000T00:45:00,14-Nov-07,VIMS,Prime,Star,BETUMICAL,Stellar calibration,Stellar calibration,Turn to star : 25 min Multiple cubes w/12x12 FOV IR @ 40/160/640 ms. Time: 20 min; Volume: 10.5 Mbits; CompRatio: 2.0 Do not return to waypoint. Not time critical. RWA REQUIRED. Do 2 stars in 1 hr 30 min.,,,,,, 2007-318T03:41:00,000T00:45:00,14-Nov-07,VIMS,Prime,Star,2CENCAL,Stellar calibration,Stellar calibration,Turn to star : 15 min (from betUMi). Multiple cubes w/12x12 FOV IR @ 40/160/640 ms. Time: 20 min; Volume: 10.5 Mbits; CompRatio: 2.0 Return to waypoint: 10 min. Not time critical. RWA REQUIRED. Do 2 stars in 1 hr 30 min.,,,,,, 2007-318T04:26:00,000T03:30:00,14-Nov-07,ISS,Prime,RingG,GPHOT5DEG,G ring photometry,1x3 MOSAIC OF G RING PHOTOMETRY AT 5 DEG SSL,"A 1x3 MOSAIC ALONG THE G RING ANSA REGION AT LOW SSL ON THE UNLIT FACE, 6 COLOURS, PHOTOMETRY AT 5 DEG SSL. GREATER THAN 20 RS PHASE BETWEEN 50-90 SSL LESS THAN 5 DEG UNLIT FACE",,,,,, 2007-318T07:56:00,000T00:30:00,14-Nov-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 026 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-318T08:56:00,000T09:00:00,14-Nov-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-318T09:45:00,000T08:00:00,14-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-318T17:56:00,000T00:34:00,14-Nov-07,RADAR,SPASS Rider,Other,WARMPO08R,RADAR warmup,Prioritized Ring Observation Number 8,Warmup for ring prioritized observation.,,,,,, 2007-318T17:56:00,001T10:34:00,14-Nov-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-318T17:56:00,001T10:34:00,14-Nov-07,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2007-318T18:30:00,000T10:00:00,14-Nov-07,RADAR,Prime,rings(general),PO8RINGS,Ring observation,Prioritized Ring Observation Number 8,Image rings via radiometry at low inclination and low resolution.,,,,,, 2007-319T04:30:00,000T04:00:00,15-Nov-07,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,latitude-phase coverage: 3x1 mosaic on each ansa,"Orbits = 026-064, Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 60, Number of SC pointings = 4, Time of observation (hours) = 4.5, Desc = Obtain 3x1 mosaic on one ring ansa on unlit face, plus 1 ptg on other ansa,",,,,,, 2007-319T04:30:00,000T04:00:00,15-Nov-07,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,Ring rider,"rider. 38 RTI, blink.",,,,,, 2007-319T04:30:00,000T04:00:00,15-Nov-07,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,Rings Lat/Phase Rider,,,,,,, 2007-319T08:30:00,000T00:26:00,15-Nov-07,CIRS,SPASS Rider,Earth,DLTURN,Downlink turn,Rider for deep space calibration,"rider for deep space. 38 RTI, blink.",,,,,, 2007-319T08:56:00,000T09:00:00,15-Nov-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-319T09:41:00,000T08:00:00,15-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,CIRS_052IC_DSCAL07319_RIDER,Calibration rider. Data Volume will be 115.2 Mb or less.,,,,,, 2007-319T14:15:01,001T01:45:00,15-Nov-07,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2007-319T14:21:22,000T03:34:38,15-Nov-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-319T17:49:45,000T02:00:00,15-Nov-07,CDA,Non-SPASS,rings(general),1804RINGM,Ring margin,Ring Margin 4.0070 deg from dust ram.",,,,,, 2007-321T03:14:00,000T00:20:00,17-Nov-07,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Rider on ISS plume observation,,,,,, 2007-321T03:36:00,000T04:00:00,17-Nov-07,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2007-321T03:55:00,000T13:47:00,17-Nov-07,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-321T04:24:28,000T00:50:00,17-Nov-07,VIMS,SPASS Rider,Saturn,SOLOCC,Solar occultation,Solar Occultation,Solar Occultation by Saturn. Ride with UVIS.,,,,,, 2007-321T04:30:00,000T00:44:28,17-Nov-07,UVIS,Prime,Sun,USUNOCC,Solar occultation,USUN_S52I/E,This is an ingress occultation with 1000 sec lead time to estimated detection of extinction. 1) 10 min observation margin 2) EUV solar occultation port centered on sun at Ingress Activity Start Time: 2007-321T04:50:00. Record data during occulation. Ingress Activity End Time: 2007-321T05:25:00. 3) 5 min observation margin.,,,,,, 2007-321T04:50:00,000T01:01:47,17-Nov-07,CDA,Non-SPASS,DustRAM direction,0400DUST,Dust survey,E Ring dense - survey - 0.38 40 day gap to start of S35! Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equtorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2007-326T09:57:00,000T22:31:00,22-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,SWAUPOINT,Solar wind pointing,CIRS_052IC_SWAUPOINT001_MIMI,Calibration rider. Data Volume will be 324.24 Mb or less.,,,,,, 2007-326T09:57:00,001T07:31:00,22-Nov-07,INMS,Non-SPASS,Saturn,PTOTM134,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-326T14:30:00,000T00:34:08,22-Nov-07,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,Calibration/Gain curve of ELS sensor,Calibration/gain curve of ELS sensor. 8 B cycles duration in 16 kbps. Data is in addition to 1000 bps from SWSKR.,,,,,, 2007-327T08:28:00,004T22:57:04,23-Nov-07,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2007-327T08:28:00,001T23:31:27,23-Nov-07,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-327T08:28:00,000T09:00:00,23-Nov-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-327T17:28:00,001T14:31:27,23-Nov-07,INMS,Non-SPASS,Saturn,PTOTM134B,MAPS survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-327T18:58:00,000T13:15:00,23-Nov-07,MIMI,Prime,SolarWind,SWAUPOINT,Solar wind pointing,"MAPS Solar Wind Aurora campaign, SW pointing","Pointing for Solar Wind Aurora Campaign, Solar Wind attitude",,,,,, 2007-327T18:58:00,000T13:15:00,23-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,SWAUPOINT,Solar wind pointing,CIRS_052IC_SWAUPOINT002_MIMI,Calibration rider. Data Volume will be 190.8 Mb or less.,,,,,, 2007-328T06:08:00,000T11:05:00,24-Nov-07,RSS,SPASS Rider,Saturn,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Titan Gravity experiment on DOYs 338-339.",,,,,, 2007-328T08:13:00,000T09:00:00,24-Nov-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-328T09:00:00,000T08:00:00,24-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-328T17:13:00,000T00:51:00,24-Nov-07,MIMI,Prime,SolarWind,SWAUPOINT,Solar wind pointing,"MAPS Solar Wind Aurora campaign, SW pointing","Pointing for Iapetus (ISS, UVIS) plus Solar Wind Aurora Campaign, Solar Wind attitude (CAPS)",,,,,, 2007-328T17:13:00,000T00:51:00,24-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,SWAUPOINT,Solar wind pointing,CIRS_052IC_SWAUPOINT003_MIMI,Calibration rider. Data Volume will be 12.24 Mb or less.,,,,,, 2007-328T17:13:00,000T00:49:30,24-Nov-07,ISS,SPASS Rider,SolarWind,SWAUPOINT,Solar wind pointing,Iapetus limb topography and geodesy observation,Do 1x1 mosaic 6 NAC clear + 4 NAC color filters,,,,,, 2007-328T17:13:00,000T00:49:30,24-Nov-07,UVIS,SPASS Rider,Iapetus,LIMBTOPO,Limb topography and geodesy observation,,,,,,,, 2007-328T18:04:01,000T14:08:59,24-Nov-07,MIMI,Prime,SolarWind,SWAUPOINT,Solar wind pointing,"MAPS Solar Wind Aurora campaign, SW pointing","Pointing for Solar Wind Aurora Campaign, Solar Wind attitude",,,,,, 2007-328T18:04:01,000T14:08:59,24-Nov-07,CIRS,SPASS Rider,InstrumentCalibration,SWAUPOINT,Solar wind pointing,CIRS_052IC_SWAUPOINT004_MIMI,Calibration rider. Data Volume will be 203.756 Mb or less.,,,,,, 2007-329T07:54:29,000T00:00:01,25-Nov-07,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 12.0 deg, r = 38.0 Rs, phase = 25 deg",,,,,, 2007-329T07:59:16,002T23:25:48,25-Nov-07,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,"Part of SW2 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observs the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2007-329T07:59:27,000T00:00:50,25-Nov-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-329T07:59:27,000T09:13:33,25-Nov-07,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-329T08:00:00,003T08:58:00,25-Nov-07,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-329T08:00:17,002T01:42:43,25-Nov-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-329T08:13:00,000T09:00:00,25-Nov-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-329T08:14:31,006T09:52:06,25-Nov-07,CDA,Non-SPASS,DustRAM direction,1906DUST,Dust survey,Dust survey 5.8270 deg from dust ram.",,,,,, 2007-337T06:19:49,000T00:49:00,3-Dec-07,CDA,Prime,RingE,ERNX,E ring plane crossing,ring plane crossing,Study of the orbital elements of dust in the vincinity of inner rim of the E ring.,,,,,, 2007-337T06:19:49,000T00:49:00,3-Dec-07,CIRS,SPASS Rider,InstrumentCalibration,ERNX,E ring plane crossing,CIRS_053IC_ERNX001_CDA,Calibration rider. Data Volume will be 11.76 Mb or less.,,,,,, 2007-337T07:08:49,000T00:46:00,3-Dec-07,UVIS,Prime,Sun,USUNOCC,Solar occultation,USUN_S53E,This is an egress occultation with 1000 sec clear transmission time following atmosphere exit. 2) EUV solar occultation port centered on sun at Activity Start Time: 2007-337T07:35:00. Record data during occultation. Activity End Time: 2007-337T08:01:00.,,,,,, 2007-337T07:08:49,000T00:46:00,3-Dec-07,VIMS,SPASS Rider,Saturn,SOLOCC,Solar occultation,Solar Occultation,Solar Occultation,,,,,, 2007-337T07:08:49,000T06:33:36,3-Dec-07,CDA,Non-SPASS,DustRAM direction,0307DUST,Dust survey,E-Ring Margin - survey - 7.31,,,,,, 2007-337T20:05:00,001T02:01:50,3-Dec-07,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2007-337T20:05:00,000T04:02:00,3-Dec-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-337T20:05:00,000T13:09:00,3-Dec-07,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2007-337T20:05:01,000T04:01:59,3-Dec-07,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2007-338T00:07:00,000T11:59:50,4-Dec-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-338T00:07:01,000T09:06:59,4-Dec-07,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2007-338T00:24:00,000T08:50:00,4-Dec-07,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,Gravity downlink pass,Additional downlink pass at Ka-band for Titan gravity science. Time includes 5 minutes for Ka-TWTA maintenance and 2 hours for thermal stabilization.,,,,,, 2007-338T01:14:00,000T01:15:00,4-Dec-07,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_053RI_DEEPSPACE_NAV,rider,,,,,, 2007-338T03:14:00,000T06:00:00,4-Dec-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-338T03:14:00,000T06:00:00,4-Dec-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-338T07:49:54,000T02:00:00,4-Dec-07,CDA,Non-SPASS,rings(general),1402RINGM,Ring margin,Ring Margin 2.00 40 day gap to start of S35! Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equtorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2007-344T06:15:00,000T00:30:00,10-Dec-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 034 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-344T06:15:00,003T16:30:04,10-Dec-07,MAG,Non-SPASS,Other,SWAURORA,Solar wind campaign,SW Aurora Campaign,SW observations in conjunction with ISS auroral observations,,,,,, 2007-344T07:15:00,000T09:00:00,10-Dec-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-344T16:38:00,000T03:07:00,10-Dec-07,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,CAPS Control Pointing during Ring Sat Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2007-344T17:45:00,000T02:00:00,10-Dec-07,CIRS,SPASS Rider,InstrumentCalibration,SWAURPTG,MAPS aurora campaign,CIRS_053IC_SWAURPTG006_CAPS,Calibration rider. Data Volume will be 28.8 Mb or less.,,,,,, 2007-344T19:45:00,000T03:15:00,10-Dec-07,VIMS,Prime,rings(general),APOMOSAIC,Apoapsis mosaic,APOAPSE_MOSAIC,"Orbits = 026-074, Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 24, Number of SC pointings = 4-30, Time of observation (hours) = 1.5-11, Volume (Mbits) = 69-519 Mosaic of entire ring system near apoapse. Unlit face. Various mosaic sizes (4x1 - 6x5)., Desc = 1x5",,,,,, 2007-344T19:45:00,000T03:15:00,10-Dec-07,CIRS,SPASS Rider,rings(general),APOMOSAIC,Apoapsis mosaic,Ring FP3/FP4 during VIMS APOMOSAIC,FP3/4 integration on the main rings,,,,,, 2007-344T19:45:00,000T03:15:00,10-Dec-07,UVIS,SPASS Rider,rings(general),APOMOSAIC,Apoapsis mosaic,,,,,,,, 2007-344T21:40:00,000T11:05:00,10-Dec-07,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rings/Saturn Occultation experiment on DOY 353.",,,,,, 2007-344T23:00:00,000T00:22:00,10-Dec-07,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 037 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2007-344T23:45:00,000T09:00:00,10-Dec-07,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2007-345T00:30:00,000T08:00:00,11-Dec-07,CIRS,SPASS Rider,InstrumentCalibration,DSCAL07,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2007-345T05:34:35,000T00:00:01,11-Dec-07,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 26.0 deg, r = 37.5 Rs, phase = 30 deg",,,,,, 2007-345T05:35:09,002T04:34:51,11-Dec-07,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2007-345T05:35:18,000T03:09:43,11-Dec-07,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-345T05:36:44,002T17:08:20,11-Dec-07,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,"Part of SW2 MAPS Campaign. Image the magnetosphere and observe solar wind and pickup ions while ORS instruments make simultaneous observations of Saturns aurora, CAPS observs the solar wind, and RPWS observes SKR. -Y to Saturn (auroral region) and -X ~ to sun.",,,,,, 2007-345T05:38:00,002T23:52:04,11-Dec-07,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2007-345T05:50:33,003T10:09:26,11-Dec-07,CDA,Non-SPASS,DustRAM direction,1813DUST,Dust survey,Dust survey 13.41=00:15); single 7.2 mrad NAC disk scan at 16 urad/sec (00:09); FP1 stare (00:03); NAC stare (00:03); return to waypoint (>=00:15). If time remains, split it between FP1 and NAC stares. 15.5 cm-1, blink, shutter closed first and last 5 min.",,,,,, 2007-353T00:31:00,000T00:55:00,19-Dec-07,ISS,SPASS Rider,Rhea,ORSRHEA,,Rhea CIRS rider spectrophotometry,Turn -Y to Rhea; Do 1x1 mosaic 4 NAC color + 9 NAC polarizer,,,,,, 2007-353T00:31:00,000T00:55:00,19-Dec-07,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2007-353T00:31:00,000T00:55:00,19-Dec-07,VIMS,SPASS Rider,Rhea,FP1FAZ0P5,CIRS FP1 phase coverage,Rhea CIRS FP1,VIMS ride with CIRS FP1. specfiics TBD assume 55 min ar ~6 kbits/sec ~ 21 Mbits for a full FOV long+short integration,,,,,, 2007-353T00:35:00,000T09:10:00,19-Dec-07,MAG,SPASS Rider,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2007-353T01:27:59,000T01:06:14,19-Dec-07,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,E-Ring Measurements - DV,DV for ERing measurements,,,,,, 2007-353T02:14:40,000T01:03:30,19-Dec-07,RSS,Prime,rings(general),OCC,Occultation,RSS Late Inclined Ring Graze Occulation 054,"We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stablization in RSS WARMUP mode. We will commence observations with a 30-minute baseline and calibration period, observe the ring ingress occultation, and continue to the 1.3 bar level of the atmosphere. We immediately commence atmosphere ingress at the 1.3 bar level until 20 minutes past the 2-bar level. After a brief period of thermal stabilization, we continue with egress observations, starting 20 minutes before the 2-bar level and finishing 30 minutes past the 1.3 bar level.",,,,,, 2007-353T02:34:13,000T00:30:28,19-Dec-07,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,E-Ring Measurements - DV,DV for ERing measurements,,,,,, 2007-353T02:34:13,000T00:05:57,19-Dec-07,CDA,Non-SPASS,RingE,0307ERNGM,E ring margin,E-Ring Margin 7.0070 deg from dust ram.",,,,,, 2007-353T03:18:10,000T00:51:04,19-Dec-07,RSS,Prime,Saturn,OCC,Occultation,RSS Late Inclined Occulation 054,"We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stablization in RSS WARMUP mode. We will commence observations with a 30-minute baseline and calibration period, observe the ring ingress occultation, and continue to the 1.3 bar level of the atmosphere. We immediately commence atmosphere ingress at the 1.3 bar level until 20 minutes past the 2-bar level. After a brief period of thermal stabilization, we continue with egress observations, starting 20 minutes before the 2-bar level and finishing 30 minutes past the 1.3 bar level.",,,,,, 2007-353T03:56:04,000T08:21:56,19-Dec-07,MIMI,SPASS Rider,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2007-353T04:09:14,000T00:59:00,19-Dec-07,RSS,Prime,Saturn,OCC,Occultation,RSS Late Inclined Atmosphere Egress Occulation 054,"We will observe at Ka, X, and S bands. Observations will commence after a 2-hour period of thermal stablization in RSS WARMUP mode. We will commence observations with a 30-minute baseline and calibration period, observe the ring ingress occultation, and continue to the 1.3 bar level of the atmosphere. We immediately commence atmosphere ingress at the 1.3 bar level until 20 minutes past the 2-bar level. After a brief period of thermal stabilization, we continue with egress observations, starting 20 minutes before the 2-bar level and finishing 30 minutes past the 1.3 bar level.",,,,,, 2007-353T05:04:29,000T00:00:01,19-Dec-07,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.0 Rs, lat = -13 deg, phase = 150 deg",,,,,, 2007-353T05:10:00,000T01:30:00,19-Dec-07,INMS,Non-SPASS,Saturn,INMAGCOMP,Inner magnetospheric composition,INMS Inner Magnetospheric Composition,Acceptable time range - Start time 352T21:53:09 to end time 353T12:18:55,,,,,, 2007-353T05:25:00,000T01:11:00,19-Dec-07,CIRS,Prime,Saturn,OCCLIMB,Occultation,CIRS_054SA_OCCLIMB04,"obtain stratospheric thermal structure at the RSS occultation points. POINTING: -y to Saturn, z to limb 67 S latitude",,,,,, 2007-353T05:25:00,000T01:11:00,19-Dec-07,CIRS,SPASS Rider,Saturn,OCCLIMB,Occultation,CIRS_054SA_OCCLIMB SI,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, latitude coverage. POINTING: -y to Saturn, z to limb",,,,,, 2007-353T05:25:00,000T01:11:00,19-Dec-07,UVIS,SPASS Rider,Saturn,OCCLIMB,Occultation,OCCLIMB Rider,UVIS EUV and FUV riding along with CIRS NADIROCC observation,,,,,, 2007-353T05:25:00,000T01:11:00,19-Dec-07,VIMS,SPASS Rider,Saturn,OCCLIMB,Occultation,Saturn CIRS Occ Limb Ridealong,Saturn CIRS Occ Limb Ride-along.,,,,,, 2007-353T06:30:14,000T00:30:14,19-Dec-07,CDA,Non-SPASS,DustRAM direction,0323SURIN,Dust survey,Dust survey inside 8 Rs 22.5070 deg from dust ram.",,,,,, 2008-003T21:41:28,000T00:14:12,3-Jan-08,CDA,Non-SPASS,RingE,0402ERNGX,Ring plane crossing,E Ring Xing 2.0070 deg from dust ram.",,,,,, 2008-015T19:54:00,000T01:00:00,15-Jan-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-015T20:07:15,000T00:04:59,15-Jan-08,CDA,Non-SPASS,RingE,0302ERNGX,Ring plane crossing,E Ring Xing 2.006RS. EACH POINTING HAS 2 FILTERS X 2 EXPOSURES. ALTERNATE R AND L ANSAE IMMEDIATELY, TAKES ABOUT 23 MIN EACH ANSA, SO WITH TURNS GET EACH ANSA EVERY HOUR THUS 3 VISITS TO EACH ANSA TO GET A RANGE OF LONGITUDES. 6 SETS @ 4 POINTINGS @(2 FILTERS X 2 EXPOSURES) = 96 FRAMES",,,,,, 2008-017T23:30:00,000T04:20:00,17-Jan-08,CIRS,SPASS Rider,rings(general),DIFFRINGS,Diffuse ring observation,CIRS_056RI_DIFFRINGS001,null,,,,,, 2008-018T03:50:00,000T00:30:00,18-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 014 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-018T04:20:00,000T00:29:00,18-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_056IC_DEEPSPACE_SP,rider,,,,,, 2008-018T04:49:00,000T09:00:00,18-Jan-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-018T05:34:00,000T08:00:00,18-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-018T13:49:00,000T01:31:00,18-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_056IC_DEEPSPACE_NAV,rider,,,,,, 2008-018T15:20:00,000T00:30:00,18-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 015 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-018T15:50:00,000T03:00:00,18-Jan-08,ISS,Prime,RingG,GPHOT5DEG,G ring photometry,1x3 MOSAIC OF G RING PHOTOMETRY AT 5 DEG SSL,"A 1x3 MOSAIC ALONG THE G RING ANSA REGION AT LOW SSL ON THE UNLIT FACE, 6 COLOURS, PHOTOMETRY AT 5 DEG SSL. GREATER THAN 20 RS PHASE BETWEEN 0-20 SSL LESS THAN 5 DEG UNLIT FACE",,,,,, 2008-018T15:50:00,000T03:00:00,18-Jan-08,CIRS,SPASS Rider,RingG,GPHOT5DEG,G ring photometry,CIRS_056RG_GPHOT5DEG001,null,,,,,, 2008-018T18:50:00,000T06:30:00,18-Jan-08,CIRS,Prime,rings(general),SUBMU05LP,Ring radial scan,CIRS_056RI_SubmmU05LP,"Radial scan of main rings to obtain submillimeter measurement of rings at a variety of geometries. -Y to rings, Z perp to rings",,,,,, 2008-018T18:50:00,000T06:30:00,18-Jan-08,CIRS,SPASS Rider,rings(general),SUBMU05MP,Ring radial scan,CIRS_056RI_SUBMU05MP001_SI,,,,,,, 2008-018T18:50:00,000T06:30:00,18-Jan-08,UVIS,SPASS Rider,rings(general),SUBMUL05L,Ring radial scan,,,,,,,, 2008-018T18:50:00,000T06:30:00,18-Jan-08,VIMS,SPASS Rider,rings(general),SUBMU05LP,Ring radial scan,"radial scan, low phase, dark face","Cube Size (X,Z) = 64*12 hires, IRInt = 640 msec. Desc = Either 1 slow scan across an entire ring ansa, or 3 shorter scans across A,B, and C rings with interleaved dark skies. Low phase, dark side of rings, 7 hi-res cubes = 11.4 Mbit/hour",,,,,, 2008-018T23:10:08,002T21:58:52,18-Jan-08,CAPS,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS ""MB,D"" Campaign","Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-018T23:10:08,000T16:49:52,18-Jan-08,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/D Campaign,"Part of MB/D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2008-018T23:10:08,000T16:49:52,18-Jan-08,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-018T23:10:08,000T14:38:52,18-Jan-08,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MB D Campaign,Observer magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2008-018T23:10:08,000T14:38:52,18-Jan-08,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-019T01:20:00,000T00:30:00,19-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 016 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-019T01:50:00,000T02:30:00,19-Jan-08,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-019T01:50:00,000T02:30:00,19-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_056IC_MAGBNDPTG004_CAPS,Calibration rider. Data Volume will be 36 Mb or less.,,,,,, 2008-019T04:49:00,000T09:00:00,19-Jan-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-019T05:34:00,000T08:00:00,19-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-019T09:09:00,000T04:40:00,19-Jan-08,RSS,SPASS Rider,rings(general),OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rings Occultation experiment on DOY 027.",,,,,, 2008-019T13:49:00,000T06:41:00,19-Jan-08,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MB D Campaign,Observer magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2008-019T13:49:00,002T00:06:00,19-Jan-08,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-019T14:30:00,000T00:30:00,19-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 018 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-019T15:00:00,000T11:30:00,19-Jan-08,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-019T16:00:00,002T05:09:36,19-Jan-08,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-019T16:00:01,002T05:10:55,19-Jan-08,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/D Campaign,"Part of MB/D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2008-019T20:30:00,000T06:00:00,19-Jan-08,MAG,SPASS Rider,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Suitable periods for S36 are from START POSSIBLE CALROLL PERIOD 1 : 2007-344T00:00:00 END POSSIBLE CALROLL PERIOD: 1 : 2007-349T14:00:00 **************************************** START POSSIBLE CALROLL PERIOD 2 : 2007-351T14:00:00 END POSSIBLE CALROLL PERIOD: 2 : 2007-352T07:00:00 **************************************** START POSSIBLE CALROLL PERIOD 3 : 2007-356T00:00:00 END POSSIBLE CALROLL PERIOD: 3 : 2007-364T17:00:00 **************************************** START POSSIBLE CALROLL PERIOD 1 : 2008-002T01:00:00 END POSSIBLE CALROLL PERIOD: 1 : 2008-002T20:00:00 **************************************** START POSSIBLE CALROLL PERIOD 2 : 2008-004T23:00:00 END POSSIBLE CALROLL PERIOD: 2 : 2008-005T07:00:00 **************************************** START POSSIBLE CALROLL PERIOD 3 : 2008-007T05:00:00 END POSSIBLE CALROLL PERIOD: 3 : 2008-011T17:00:00 **************************************** START POSSIBLE CALROLL PERIOD 4 : 2008-014T05:00:00 END POSSIBLE CALROLL PERIOD: 4 : 2008-014T14:00:00 **************************************** START POSSIBLE CALROLL PERIOD 5 : 2008-016T21:00:00 END POSSIBLE CALROLL PERIOD: 5 : 2008-017T05:00:00 **************************************** START POSSIBLE CALROLL PERIOD 6 : 2008-019T04:00:00 END POSSIBLE CALROLL PERIOD: 6 : 2008-023T16:00:00 The last allocated roll prior to this is on day 344. The next feasible windows in S37 are d26,d28,d38,d40 - which mostly fall on downlinks! Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equtorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-020T02:30:00,000T00:30:00,20-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 019 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-020T02:30:00,002T11:05:00,20-Jan-08,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MB D Campaign,Observer magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2008-020T04:35:00,000T09:00:00,20-Jan-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-020T05:20:00,000T08:00:00,20-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-020T14:15:00,000T01:00:00,20-Jan-08,ISS,Prime,Titan,1X1PT60A,Photopolarimetry,Titan NAC Photopol 60 Phase,Titan NAC Photopol 60 Phase,,,,,, 2008-020T15:15:00,000T02:00:00,20-Jan-08,ISS,Prime,Star,MONITOR,,ISS Sensitivity monitor,Periodic standard star image to monitor ISS sensitivity,,,,,, 2008-020T17:15:00,000T07:00:00,20-Jan-08,CIRS,Prime,rings(general),FMONITOR,F ring monitor,Ring FP3/FP4 during F Ring monitoring,FP3/4 integration on the main rings,,,,,, 2008-020T17:15:00,000T07:00:00,20-Jan-08,ISS,SPASS Rider,rings(general),FMONITOR,F ring monitor,F ring imaging on each ansa,One WAC each ansa at beginning and every 2 hours or fraction afterwards.,,,,,, 2008-020T17:15:00,000T07:00:00,20-Jan-08,UVIS,SPASS Rider,rings(general),FMONITOR,F ring monitor,,,,,,,, 2008-021T00:15:00,000T03:45:00,21-Jan-08,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-021T04:35:00,000T09:00:00,21-Jan-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-021T05:35:00,000T08:00:00,21-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-021T13:55:00,000T07:14:39,21-Jan-08,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-021T14:05:00,000T10:00:00,21-Jan-08,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-021T14:05:00,000T07:00:00,21-Jan-08,ISS,SPASS Rider,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,ISS NAC dark current calibration,ISS NAC dark current calibration,,,,,, 2008-021T16:00:00,000T03:00:00,21-Jan-08,CDA,Non-SPASS,Other,FSWCO,Flight software checkout,CDA FSW CO 1,"Turn down instrument (HV, HRD off) CDA Reset Load CDA Enceladus Flyby FSW version 12.0 (spectra only) Perform first functional test. CDA Reset Load FSW 10.0 and configure for measurement",,,,,, 2008-021T21:09:00,000T16:26:00,21-Jan-08,CAPS,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-021T21:09:36,000T16:25:24,21-Jan-08,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-021T21:09:39,000T16:22:09,21-Jan-08,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-021T21:10:55,000T16:24:05,21-Jan-08,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/D Campaign,"Part of MB/D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2008-021T21:25:01,000T16:09:58,21-Jan-08,CDA,Non-SPASS,DustRAM direction,1221DUST,Dust survey,Dust survey 20.8870 deg from dust ram.",,,,,, 2008-027T18:22:00,000T01:00:00,27-Jan-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-027T18:27:56,000T00:04:59,27-Jan-08,CDA,Non-SPASS,RingE,0304ERNGX,Ring plane crossing,E Ring Xing 4.006RS. EACH POINTING HAS 2 FILTERS X 2 EXPOSURES. ALTERNATE R AND L ANSAE IMMEDIATELY, TAKES ABOUT 23 MIN EACH ANSA, SO WITH TURNS GET EACH ANSA EVERY HOUR THUS 3 VISITS TO EACH ANSA TO GET A RANGE OF LONGITUDES. 6 SETS @ 4 POINTINGS @(2 FILTERS X 2 EXPOSURES) = 96 FRAMES",,,,,, 2008-030T02:00:00,000T01:00:00,30-Jan-08,ISS,Prime,Titan,PHOTOOPS,Photo opportunity,Photo Opportunity of Titan and Saturn and the ring,"Image Titan while it emerges from behind Saturn's atmosphere, over the dark rings.",,,,,, 2008-030T03:00:00,000T00:35:00,30-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 014 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-030T03:35:00,000T00:30:00,30-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_057IC_DEEPSPACE_SP,rider,,,,,, 2008-030T04:05:00,000T09:00:00,30-Jan-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-030T04:50:00,000T08:00:00,30-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-030T08:25:00,000T04:40:00,30-Jan-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rings/Saturn Occultation experiment on DOY 039.",,,,,, 2008-030T13:05:00,000T01:25:00,30-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_057IC_DEEPSPACE_NAV,rider,,,,,, 2008-030T14:30:00,000T04:00:00,30-Jan-08,CIRS,Prime,rings(general),TEMPU05LP,Thermal map,CIRS_056RI_Tempu05lp,"Afternoon radial scan of main rings to obtain thermal measurement of rings. -Y to rings, Z perp to rings",,,,,, 2008-030T14:30:00,000T04:00:00,30-Jan-08,CIRS,SPASS Rider,rings(general),TEMPU05LP,Thermal map,CIRS_057RI_TEMPU05LP001_SI,,,,,,, 2008-030T18:30:00,000T04:00:00,30-Jan-08,VIMS,Prime,Star,FOMALHAUT,Fomalhaut,Fomalhaut,"Turn to Fomalhaut; Time: 30 min

Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0 Turn to waypoint: 30 min Primary: -y to Fomalhaut; Secondary: +z to TBD Not time critical. RWA REQUIRED.",,,,,, 2008-030T18:30:00,000T04:00:00,30-Jan-08,CIRS,SPASS Rider,Star,FOMALHAUT,Fomalhaut,Rider,UVIS rider,,,,,, 2008-030T21:20:00,000T15:30:00,30-Jan-08,CAPS,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-030T21:20:00,000T17:40:00,30-Jan-08,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/D Campaign,"Part of MB/D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2008-030T21:20:00,000T17:40:00,30-Jan-08,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-030T21:20:00,000T15:30:00,30-Jan-08,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MB D Campaign,Observer magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2008-030T22:30:00,000T04:50:00,30-Jan-08,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-031T03:50:00,000T09:00:00,31-Jan-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-031T04:35:00,000T08:00:00,31-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-031T12:50:00,002T07:01:00,31-Jan-08,CAPS,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-031T12:50:00,001T00:35:00,31-Jan-08,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MB D Campaign,Observer magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2008-031T12:50:00,002T07:05:08,31-Jan-08,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-031T13:20:00,000T01:40:00,31-Jan-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 019 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-031T15:00:00,000T11:45:00,31-Jan-08,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-031T15:00:00,000T11:45:00,31-Jan-08,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_057IC_MAGBNDPTG001_CAPS,Calibration rider. Data Volume will be 169.2 Mb or less.,,,,,, 2008-031T15:00:00,002T04:55:08,31-Jan-08,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-031T15:00:01,002T04:59:59,31-Jan-08,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/D Campaign,"Part of MB/D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2008-032T02:45:00,000T00:30:00,1-Feb-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 020 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-032T03:50:00,000T09:00:00,1-Feb-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-032T04:35:00,000T08:00:00,1-Feb-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,Deep Space Calibration,Deep space obervations for calibration.,,,,,, 2008-032T13:25:00,004T04:05:08,1-Feb-08,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MB D Campaign,Observer magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2008-032T13:30:00,000T00:30:00,1-Feb-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 021 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-032T14:00:00,000T12:45:00,1-Feb-08,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-032T14:00:00,000T12:45:00,1-Feb-08,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_057IC_MAGBNDPTG002_CAPS,Calibration rider. Data Volume will be 183.6 Mb or less.,,,,,, 2008-033T02:00:00,000T12:00:00,2-Feb-08,CDA,SPASS Rider,Other,DECON,Decontamination,Decontamination,"CDA boresight off-sun, no resources (Watts, bps), resources covered by other request",,,,,, 2008-033T02:45:00,000T00:30:00,2-Feb-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 022 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-033T03:45:00,000T03:05:00,2-Feb-08,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2008-033T03:51:00,000T09:00:00,2-Feb-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-033T05:50:00,000T01:00:00,2-Feb-08,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2008-033T06:50:00,000T06:00:00,2-Feb-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_057IC_DSCAL08033_RIDER,Calibration rider. Data Volume will be 28.8 Mb or less.,,,,,, 2008-033T08:10:00,000T04:45:00,2-Feb-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rings/Saturn Occultation experiment on DOY 039.",,,,,, 2008-033T13:21:00,000T00:30:00,2-Feb-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 024 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-033T13:51:00,000T05:30:00,2-Feb-08,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,CAPS Control Pointing during MAG BND Campaign,"Part of MB,C MAPS Campaign. Observe dusk-side magnetospheric boundaries at a variety of latitudes",,,,,, 2008-033T13:51:00,000T05:30:00,2-Feb-08,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_057IC_MAGBNDPTG003_CAPS,Calibration rider. Data Volume will be 79.2 Mb or less.,,,,,, 2008-033T19:21:00,000T07:00:00,2-Feb-08,VIMS,Prime,rings(general),APOMOSAIC,Apoapsis mosaic,APOAPSE_MOSAIC,"Orbits = 026-074, Cube Size (X,Z) = 64*64, Time per SC pointing (mins) = 24, Number of SC pointings = 4-30, Time of observation (hours) = 1.5-11, Volume (Mbits) = 69-519 Mosaic of entire ring system near apoapse. Unlit face. Various mosaic sizes (4x1 - 6x5)., Desc = 3x6",,,,,, 2008-033T19:21:00,000T07:00:00,2-Feb-08,UVIS,SPASS Rider,rings(general),APOMOSAIC,Apoapsis mosaic,,,,,,,, 2008-033T19:51:00,000T17:00:00,2-Feb-08,CAPS,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-033T19:55:08,002T21:28:33,2-Feb-08,INMS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS,"Part of MB,D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-033T19:55:08,002T21:35:00,2-Feb-08,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2008-033T20:00:00,002T21:30:08,2-Feb-08,MIMI,SPASS Rider,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/D Campaign,"Part of MB/D MAPS Campaign. Observer magnetospheric boundaries near noon on highly inclined orbits. Set up MIMI for magnetospheric boundaries campaign Pointing: -X to sun and/or corotation, internal B in X, Z plane; or spin about Z.",,,,,, 2008-033T20:07:35,000T00:00:01,2-Feb-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 11.9 d, inc = 46.5 deg, r = 30.1 Rs, phase = 31 deg",,,,,, 2008-033T20:10:08,005T00:58:39,2-Feb-08,CDA,Non-SPASS,DustRAM direction,1221DUST,Dust survey,Dust survey 20.9870 deg from dust ram.",,,,,, 2008-039T17:02:13,000T00:19:54,8-Feb-08,CDA,Non-SPASS,DustRAM direction,0302DUST,Dust survey,E Ring dense - survey - 2.1270 deg from dust ram.",,,,,, 2008-051T17:34:57,000T01:34:02,20-Feb-08,CDA,Non-SPASS,DustRAM direction,0306DUST,Dust survey,E-Ring Margin - survey - 5.7870 deg from dust ram.",,,,,, 2008-062T03:14:00,000T01:00:00,2-Mar-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-062T03:38:53,000T00:11:56,2-Mar-08,CDA,Non-SPASS,Enceladus,0400ENORX,Enceladus orbit crossing,Enceladus Orbit Xing 0.0070 deg from dust ram.",,,,,, 2008-072T18:35:34,000T01:00:00,12-Mar-08,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-072T18:36:12,000T01:00:00,12-Mar-08,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 061EN Campaign,Part of 061EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2008-072T18:36:12,000T01:00:00,12-Mar-08,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2008-072T18:44:42,000T00:26:30,12-Mar-08,CAPS,Prime,Enceladus,ENCLDSPTG,,CAPS control of pointing near Enceladus c/a,CAPS control of spacecraft pointing from -19 to +5 min. This request is in addition to the EN_ENCOUNTER request which covers the CAPS data volume,,,,,, 2008-072T18:44:42,000T00:26:30,12-Mar-08,CIRS,SPASS Rider,Enceladus,DRAGCIRS,ORS drag secondary axis,Drag CIRS FOVs across disk at closest approach.,"CIRS will take data during closest approach when S/C cannot track Enceladus, provided that the INMS orientation permits it. CIRS to operate all focal planes; 38 RTI (15.5 cm-1 resolution, 4.75 sec frame time). Blink.",,,,,, 2008-072T18:44:42,000T00:26:30,12-Mar-08,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus' surface plus limb drifts; will look for airglow in eclipse,,,,,, 2008-072T18:44:42,000T00:26:30,12-Mar-08,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus targeted,12x12i1v1 160 ms; Ride along with ISS framing,,,,,, 2008-072T19:01:12,000T00:10:00,12-Mar-08,INMS,SPASS Rider,Saturn,ENCRAMPNT,MAPS survey,MAPS Survey,"Enc Closest approach. CAPS prime, using ENC SC_RAM as pirme axis, and controlling 2nd for CAPS pointing.",,,,,, 2008-072T19:11:12,000T00:59:00,12-Mar-08,CIRS,Prime,Enceladus,FP3HOTSPT,CIRS FP3 hot spot mapping,FP3 map of hot spots in south polar region,"Change objective to FP3 thermal mapping of Cassini-discovered hot slots. Turn from pickup point to a known hot source region to take advantage of turn margin for integration (turn= T00:10:30 + 2 minute margin). Then FP3 map of active regions; then FP1 integration(?). - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Old plan: Turn to RA/Dec (ca. 9.9 min), then to Enceladus. At Enceladus, 39.gt.AD.gt.11 mrad; phase=64 (irrelevant), (-69, 332). CIRS 38 RTI. Rapid change in size requires tricky design. Nyquist FP1 map for 37 mrad target takes 46 min, but for 12 mrad target, takes only 8. Probably do in 2 or 3 ""rectangular"" submosaics to adjust to diminishing size.",,,,,, 2008-072T19:11:12,000T00:59:00,12-Mar-08,CIRS,SPASS Rider,Enceladus,FP3HOTSPT,CIRS FP3 hot spot mapping,Enceladus endogenic mapping SIs,Two NAC images to determine pointing during solar eclipse: first at start+00:10:45 (in dead time at end of turn to Enceladus); second at start +00:36:15 (during south polar stare). Tolerance for first image +/-5 seconds; for second image +/-2 minutes. Enceladus is in eclipse; shutter for Saturnshine (there may be very little).,,,,,, 2008-072T19:11:12,000T00:59:00,12-Mar-08,ISS,SPASS Rider,Enceladus,FP3HOTSPT,CIRS FP3 hot spot mapping,Enceladus -- Eclipse ingress imaging,POST-FLYBY Imaging: CIRS will point at Enceladus as it goes into eclipse. ISS will acquire several images (BOTSIMS) before ingress.,,,,,, 2008-072T19:11:12,000T00:59:00,12-Mar-08,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus' surface plus limb drifts; will look for airglow in eclipse,,,,,, 2008-072T19:11:12,000T00:59:00,12-Mar-08,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus targeted,"64x64i1v1 160ms, 64x32i2v1 320ms, 64x64i2v3 160ms",,,,,, 2008-072T19:11:12,000T00:55:00,12-Mar-08,INMS,Non-SPASS,Saturn,ENCOUTBND,MAPS survey,MAPS Survey,Enc Outbound observation,,,,,, 2008-072T19:35:34,000T00:04:26,12-Mar-08,MIMI,SPASS Rider,DustRAM direction,INCADUST,MIMI INCA dust observation,MAPS RS Campaign,"Part of RS MAPS Campaign. Spacecraft must be pointed such that the dust ram is not entering the INCA FOV. Required to satisfy FR76C3. This means INCA boresight (in S/C X, Y plane, 9.5 deg toward +X from -Y) >70 deg from dust ram.",,,,,, 2008-072T19:35:34,005T09:03:26,12-Mar-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2008-072T19:37:00,000T01:00:00,12-Mar-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-072T19:40:00,000T11:26:00,12-Mar-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-072T20:06:12,000T12:50:04,12-Mar-08,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2008-072T20:10:12,000T00:44:00,12-Mar-08,RADAR,Prime,Enceladus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Enceladus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2008-072T20:10:14,000T00:09:45,12-Mar-08,CDA,Non-SPASS,Other,DRATE,Data volume adjustment,E-Ring Measurements - DV,DV for ERing measurements,,,,,, 2008-072T20:19:59,000T00:10:46,12-Mar-08,CDA,Non-SPASS,DustRAM direction,0315SURIN,Dust survey,Dust survey inside 8 Rs 15.00 Arcturus: multiple sets of 10 cubes w/64x4 FOV IR @ 160 ms, VIS @ 10160 ms; Time: 2.75 hr; CompRatio: 3.0

Turn to waypoint: 30 min

Primary: -y to Arcturus; Secondary: +z to TBD",,,,,, 2008-076T12:21:00,000T02:45:00,16-Mar-08,CIRS,SPASS Rider,Star,ARCTURUS,Arcturus observation,,hidden,,,,,, 2008-076T15:06:00,000T00:30:00,16-Mar-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT DETERMINATION CAMPAIGN, 015 TH OBS","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-076T15:06:00,000T00:30:00,16-Mar-08,CIRS,SPASS Rider,Other,SATELLORB,Satellite orbit campaign,,rider,,,,,, 2008-076T15:36:00,000T01:30:00,16-Mar-08,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,,rider,,,,,, 2008-076T17:06:00,000T09:00:00,16-Mar-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-076T17:51:00,000T08:15:00,16-Mar-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_061IC_DSCAL08077_SP,rider,,,,,, 2008-077T02:06:00,000T22:29:00,17-Mar-08,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_061SA_MIRMAP043_PRIME,"Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2008-077T02:06:00,000T22:29:00,17-Mar-08,UVIS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,UVIS Rider to CIRS MIRMAP,,,,,,, 2008-078T00:35:00,000T09:00:00,18-Mar-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-078T01:35:00,000T08:00:00,18-Mar-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_061IC_DSCAL08078_SP,rider,,,,,, 2008-078T04:33:56,000T00:00:01,18-Mar-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 10.6 d, inc = 56.1 deg, r = 27.169 Rs, phase = 31 deg",,,,,, 2008-078T04:38:00,002T04:42:00,18-Mar-08,CDA,Non-SPASS,Other,DATAVOLUM,Data volume adjustment,DV Due to Sponge Bits,"Dust survey $ 1353.0929 $ 1356.1836 $ 20.361 to 27.204 Rs lat: 0.949 to 22.939 deg ring-alt: 20345. to 639671.km,pointing=CDA to Kepler RAM,rate=150,dataVolume=38.199",,,,,, 2008-078T04:39:00,004T20:55:56,18-Mar-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2008-078T04:39:40,004T00:20:20,18-Mar-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-078T04:40:00,000T04:55:00,18-Mar-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2008-078T04:40:56,003T04:12:04,18-Mar-08,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2008-078T04:54:18,003T11:39:43,18-Mar-08,CDA,Non-SPASS,DustRAM direction,1823DUST,Dust survey,Dust survey 23.0670 deg from dust ram.",,,,,, 2008-083T10:06:00,000T01:00:00,23-Mar-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-083T10:45:00,000T01:35:00,23-Mar-08,CIRS,Prime,Dione,FP1SECLN,CIRS elipse observation,CIRS_062DI_FP1SECLN001_PRIME,"FP3 observation of Dione solar eclipse entry. Phase= 13.0, Local time= 11.9, sub S/C=(-12.0, 357.0), AD=7.2 mrad. BEST Dione; spatially resolved. Duration 01:35. One NAC SI at 083T11:15. CIRS 38 RTI, blink, FP3 to (lat, lon)=(-18, 350). Shutter closed first half of turn from waypoint, and last half of return to waypoint.",,,,,, 2008-083T10:45:00,000T01:35:00,23-Mar-08,CIRS,SPASS Rider,Dione,FP1SECLN,CIRS elipse observation,CIRS_062DI_FP1SECLN_SI,,,,,,, 2008-083T10:45:00,000T01:35:00,23-Mar-08,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2008-083T10:53:40,000T01:30:00,23-Mar-08,INMS,Non-SPASS,Saturn,INMAGCOMP,Inner magnetospheric composition,INMS Inner Magnetospheric Composition,Acceptable time range - Start time 083T04:55:17 to end time 083T19:50:40,,,,,, 2008-083T11:10:00,000T03:55:04,23-Mar-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-083T11:46:45,000T00:12:05,23-Mar-08,CDA,Non-SPASS,DustRAM direction,0315SURIN,Dust survey,Dust survey inside 8 Rs 15.0070 deg from dust ram.",,,,,, 2008-092T17:59:00,000T01:00:00,1-Apr-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-092T18:55:00,000T06:39:00,1-Apr-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-092T18:59:00,000T01:01:00,1-Apr-08,RPWS,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-092T19:05:00,000T01:09:56,1-Apr-08,MIMI,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2008-092T19:05:14,000T01:29:59,1-Apr-08,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2008-092T19:23:00,000T00:27:00,1-Apr-08,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,,rider,,,,,, 2008-092T19:30:00,000T12:33:41,1-Apr-08,CDA,Non-SPASS,DustRAM direction,0409DUST,Dust survey,Dust survey inside 8 Rs 9.1770 deg from dust ram.",,,,,, 2008-102T08:03:00,000T01:00:00,11-Apr-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-102T08:51:00,000T06:39:00,11-Apr-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-102T09:03:00,000T01:17:00,11-Apr-08,RPWS,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-102T09:05:00,000T01:15:00,11-Apr-08,MIMI,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2008-102T09:10:10,000T01:30:00,11-Apr-08,INMS,Non-SPASS,Saturn,INMAGCOMP,Inner magnetospheric composition,INMS Inner Magnetospheric Composition,Acceptable time range - Start time 062T03:50:00 to end time 062T05:20:00,,,,,, 2008-102T09:19:00,000T13:29:00,11-Apr-08,CDA,Non-SPASS,DustRAM direction,0409DUST,Dust survey,Dust survey inside 8 Rs 9.2870 deg from dust ram.",,,,,, 2008-111T21:22:00,000T01:00:00,20-Apr-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-111T21:45:00,000T00:30:00,20-Apr-08,CIRS,SPASS Rider,rings(general),SOLAROCC,Solar occultation,,rider,,,,,, 2008-111T22:15:00,000T01:50:00,20-Apr-08,VIMS,Prime,RingB,SPOKEHIPH,High phase ring spoke observation,"Spoke formation--late, high phase",64x64; 80 msec; Observe spoke region in B ring at high phase angle. Do any 2 of 5 in revs 63-67,,,,,, 2008-111T22:15:00,000T01:50:00,20-Apr-08,CIRS,SPASS Rider,RingB,SPOKEHIPH,High phase ring spoke observation,,rider,,,,,, 2008-111T22:15:00,000T06:41:00,20-Apr-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-111T22:22:00,000T01:18:00,20-Apr-08,RPWS,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-111T22:25:00,000T01:15:00,20-Apr-08,MIMI,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2008-111T22:28:30,000T01:30:00,20-Apr-08,INMS,SPASS Rider,Saturn,INMAGCOMP,Inner magnetospheric composition,INMS Inner Magnetospheric Composition,Acceptable time range - Start time 062T03:50:00 to end time 062T05:20:00,,,,,, 2008-111T22:46:00,000T12:40:44,20-Apr-08,CDA,Non-SPASS,DustRAM direction,0409DUST,Dust survey,Dust survey inside 8 Rs 9.4770 deg from dust ram.",,,,,, 2008-121T10:28:00,000T01:00:00,30-Apr-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-121T10:50:00,000T00:30:00,30-Apr-08,CIRS,SPASS Rider,rings(general),SOLAROCC,Solar occultation,,rider,,,,,, 2008-121T11:20:00,000T02:30:00,30-Apr-08,ISS,Prime,rings(general),RETARGHPH,Retargetable observation,High res retargettable of clump or other ring,"Several features observable at high phase: clumps, other features. 3 NACs x 3 colors per observation; 1 obs/half hour",,,,,, 2008-121T11:20:00,000T02:30:00,30-Apr-08,CIRS,SPASS Rider,Other,RETARGHPH,Retargetable observation,,rider,,,,,, 2008-121T11:26:00,000T06:42:00,30-Apr-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-121T11:28:00,000T01:17:00,30-Apr-08,RPWS,Non-SPASS,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-121T11:30:00,000T01:15:00,30-Apr-08,MIMI,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2008-121T11:58:00,000T12:33:40,30-Apr-08,CDA,Non-SPASS,DustRAM direction,0407DUST,Dust survey,Dust survey inside 8 Rs 6.6670 deg from dust ram.",,,,,, 2008-130T23:43:00,000T01:00:00,9-May-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-130T23:44:52,000T01:30:00,9-May-08,INMS,Prime,Saturn,INMAGCOMP,Inner magnetospheric composition,INMS Inner Magnetospheric Composition,Acceptable time range - Start time 062T03:50:00 to end time 062T05:20:00,,,,,, 2008-131T00:00:00,000T02:00:00,10-May-08,CAPS,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-131T00:43:00,000T07:17:00,10-May-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,Auroral Campaign,Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-131T00:45:00,000T01:15:00,10-May-08,MIMI,SPASS Rider,co-rotation,IMVP5M,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=5, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2008-131T00:47:00,000T06:43:00,10-May-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-131T01:14:52,000T10:00:00,10-May-08,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2008-131T01:19:00,000T12:25:24,10-May-08,CDA,Non-SPASS,DustRAM direction,0501DUST,Dust survey,Dust survey inside 8 Rs 1.23AD>5.5; 81>phase>69, (-36, 56) to (-46, 47). 2-scan FP3 map at 8 urad/sec = 1.05*2*(6.5+2)*16/8 = 36 min. Center for NAC at end. 15.5 cm-1, blink, shutter closed first 3 and last 3 min.",,,,,, 2008-131T02:05:00,000T01:00:00,10-May-08,ISS,SPASS Rider,Tethys,TETHYS,Tethys,TETHYS,Tethys,,,,,, 2008-131T02:05:00,000T01:00:00,10-May-08,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2008-131T02:05:00,000T01:00:00,10-May-08,VIMS,SPASS Rider,Tethys,TETHYSC,Tethys,Tethys,"160ms, 640ms (13 min/cycle) if OK with cirs plan, sized for full tethys, repeat",,,,,, 2008-131T02:12:02,000T00:00:01,10-May-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.293 Rs, lat = -23 deg, phase = 150 deg",,,,,, 2008-131T03:05:00,000T03:15:00,10-May-08,ISS,Prime,rings(general),RDHRSSCHP,High resolution radial scan of ring system,High res radial scan of the main rings,HI RES RAD SCAN OF MAIN RINGS,,,,,, 2008-131T03:05:00,000T03:15:00,10-May-08,CIRS,SPASS Rider,rings(general),RDHRSSCHP,High resolution radial scan of ring system,CIRS_067RI_RDHRSSCHP001_ISS,rider,,,,,, 2008-131T03:05:00,000T03:15:00,10-May-08,VIMS,SPASS Rider,rings(general),RDHRSSCHP,High resolution radial scan of ring system,"radial scan, low phase, lit face","This is an ISS radial scan rider, design TBD. Assume 12*12, tau_IR = 320 msec OR 64*12 hires, tau_IR = 80 ms. Dwell time = 2-3 min. 20 frames per hour. LIt side, high phase. Data vol assumes 64x12 cubes.",,,,,, 2008-131T06:20:00,000T10:00:00,10-May-08,ISS,Prime,rings(general),AZSCAN,Azimuthal ring scan,Contiguous az scan of selected ring feature,AZIMUTHAL SCANS OF GAPS/RINGLETS/EDGES/WAVES/F RING AT LOW PHA,,,,,, 2008-131T06:20:00,000T10:00:00,10-May-08,CIRS,SPASS Rider,rings(general),AZSCAN,Azimuthal ring scan,CIRS_067RI_AZSCAN001_ISS,rider,,,,,, 2008-131T07:30:00,001T15:00:00,10-May-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-131T08:00:00,001T04:15:00,10-May-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-131T09:36:00,001T00:34:00,10-May-08,MIMI,SPASS Rider,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MAPS IM/DYN Campaign,"Part of IM/DYN MAPS Campaign. Image the dynamics of the inner magnetosphere in ENA with MIMI/INCA. With -Y pointed toward Saturn, corotation as close to the S/C -X, +/- Z plane as possible.",,,,,, 2008-131T11:14:52,001T10:47:06,10-May-08,INMS,Non-SPASS,Saturn,INMAGSURV,Observing neutral molecules in the inner magnetosphere,MAPS Survey,MAPS magnetospheric survey.,,,,,, 2008-131T13:44:24,000T00:51:58,10-May-08,CDA,Non-SPASS,DustRAM direction,0850SURVY,Dust survey,Dust survey 50.0070 deg from dust ram.",,,,,, 2008-138T22:33:00,000T01:00:00,17-May-08,CDA,SPASS Rider,RingE,RPX,Ring plane crossing,E Ring Xing 2.0070 deg from dust ram.",,,,,, 2008-146T21:45:00,000T01:00:00,25-May-08,CDA,SPASS Rider,RingE,RPX,Ring plane crossing,E Ring Xing 2.004, r<7.5",,,,,, 2008-231T18:40:00,000T10:45:00,18-Aug-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-231T18:40:00,000T10:36:35,18-Aug-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-231T22:30:00,000T02:00:00,18-Aug-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-232T00:25:00,000T12:15:00,19-Aug-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-232T00:30:00,003T08:35:00,19-Aug-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-232T02:25:00,000T02:23:13,19-Aug-08,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 081RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2008-232T03:49:00,000T00:40:00,19-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_081RI_DEEPSPACE232_SP,rider,,,,,, 2008-232T04:47:29,000T02:00:00,19-Aug-08,CDA,SPASS Rider,DustRAM direction,RPX0000,,CDA RPXing 2008-232T05:47:29 NTH,Nice to have - variation of angular distance to source (longitude),,,,,, 2008-232T04:48:13,000T01:01:00,19-Aug-08,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ring Occultation 081,"Early XM series of RSS ring occultations spanning a chord of the ring system. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 20 minute free-space baseline and calibration period, followed by the occultation and a subsequent 15 minute free-space baseline and calibration period.",,,,,, 2008-232T05:05:00,000T00:21:00,19-Aug-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0048274 Rs exit= 3.9676038 Range altitude= 39223.876 km ... 20438.900,,,,,, 2008-232T05:16:35,000T01:00:00,19-Aug-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-232T05:25:00,000T00:55:00,19-Aug-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-232T05:25:00,000T00:55:00,19-Aug-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-232T05:26:00,000T00:42:00,19-Aug-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9660120 Rs exit= 3.9235969 Range altitude= 19496.896 km ... -19185.208,,,,,, 2008-232T06:08:00,000T00:22:00,19-Aug-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9231292 Rs exit= 3.9196347 Range altitude= -20127.232 km ... -39846.323,,,,,, 2008-232T06:16:35,000T08:32:25,19-Aug-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-232T06:20:00,000T08:29:00,19-Aug-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-232T06:20:00,000T11:45:00,19-Aug-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-232T06:23:44,000T00:00:01,19-Aug-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.915 Rs, lat = -9 deg, phase = 158 deg",,,,,, 2008-232T06:30:00,003T16:12:00,19-Aug-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9197700 Rs exit= 4.0465075 Range altitude= -40781.481 km ... 40682.449,,,,,, 2008-232T06:49:00,000T01:11:00,19-Aug-08,ISS,Prime,Pallene,PALENCLOS,,Pallene close flyby,"observation during ~43,000 km flyby of Pallene. Unique opportunity in tour.",,,,,, 2008-232T06:49:00,000T01:11:00,19-Aug-08,VIMS,SPASS Rider,Other,PALLENE,,Pallene close approach,Hi res view,,,,,, 2008-232T08:00:00,000T01:15:00,19-Aug-08,VIMS,Prime,rings(general),HIRESHIPH,,"High res, High phase ring observation","4 at priority 1, 6 at priority 2",,,,,, 2008-232T08:00:00,000T01:15:00,19-Aug-08,CIRS,SPASS Rider,rings(general),HIRESHIPH,,CIRS_081RI_HIRESHIPH103_VIMS,rider,,,,,, 2008-232T09:15:00,000T03:54:00,19-Aug-08,CIRS,Prime,Rhea,SECLNX,,CIRS_081RH_SECLNX001_PRIME,"FP13 N, FP1 X; 3.9-2.7 mrad, ~30S, LT=12; stable pointing. Rings TWT. Start T09:15, end T13:09. Rhea eclipse. Entry at 2008-232T10:37:47; exit at 2008-232T12:29:31. Design:",,,,,, 2008-232T09:15:00,000T03:54:00,19-Aug-08,CIRS,SPASS Rider,Rhea,SECLNX,,CIRS_081RH SECLNX SI,3 WAC SI for for pointing verification of FP1 stare and eclipse observation (can use lossy compression). First at 2008-232T10:13 (within FP1 stare); Second at 2008-232T10:33 (5 min. before entry; entry at 2008-232T10:37:47); AD=3.4 mrad; Third at 2008-232T12:35 (5 min. past exit; exit at 2008-232T12:29:31); AD=2.8 mrad.,,,,,, 2008-232T09:15:00,000T03:54:00,19-Aug-08,ISS,SPASS Rider,Rhea,SECLNX,,Rhea eclipse observation,Rhea eclipse observation,,,,,, 2008-232T09:15:00,000T03:54:00,19-Aug-08,VIMS,SPASS Rider,Rhea,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-232T12:40:00,000T05:25:00,19-Aug-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-232T12:44:00,000T11:05:00,19-Aug-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-232T14:49:00,000T03:16:00,19-Aug-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-232T14:49:00,000T07:00:00,19-Aug-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-232T14:49:00,000T09:00:00,19-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-232T18:05:00,003T04:37:00,19-Aug-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-232T18:05:00,003T11:44:00,19-Aug-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-232T18:05:00,000T18:55:00,19-Aug-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-232T23:49:00,000T00:41:00,19-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_081RI_DEEPSPACE432_SP,rider,,,,,, 2008-233T00:30:00,000T13:24:00,20-Aug-08,VIMS,Prime,rings(general),FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2008-233T00:30:00,000T13:24:00,20-Aug-08,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,CIRS_081RI_FMOVIE106_VIMS,rider,,,,,, 2008-233T00:30:00,000T13:24:00,20-Aug-08,ISS,SPASS Rider,rings(general),FMOVIE,F ring movie,Medium Res F ring Movie,Medium Resolution F Ring Movie,,,,,, 2008-233T00:30:00,000T13:24:00,20-Aug-08,UVIS,SPASS Rider,rings(general),FMOVIE,F ring movie,,UV spectral mapping of Saturn's rings.,,,,,, 2008-233T12:29:00,000T11:05:00,20-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-233T13:00:00,002T09:42:00,20-Aug-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-233T13:54:00,000T00:40:00,20-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_081RI_DEEPSPACE233_RIDER,rider,,,,,, 2008-233T14:34:00,000T09:00:00,20-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-233T14:49:00,000T08:45:00,20-Aug-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-233T15:21:00,000T08:00:00,20-Aug-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-233T18:56:00,002T03:46:00,20-Aug-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-233T23:34:00,000T00:41:00,20-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_081RI_DEEPSPACE433_SP,rider,,,,,, 2008-234T00:15:00,000T11:00:00,21-Aug-08,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities (backup),,,,,, 2008-234T00:15:00,000T11:00:00,21-Aug-08,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_081RI_SPKMVLFLP001_ISS,rider,,,,,, 2008-234T00:15:00,000T11:00:00,21-Aug-08,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie,ISS rider,,,,,, 2008-234T11:15:00,000T01:39:00,21-Aug-08,ISS,Prime,Dione,098W003PH,,Dione lon/phase angle observation,"Turn UVIS_FUV to Dione; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-234T11:15:00,000T01:39:00,21-Aug-08,CIRS,SPASS Rider,Dione,098W003PH,,CIRS_081DI_098W003PH001_ISS,"Rider on ISS Dione. Duration T01:39. 0.91phase angle>5.7, (-10, 58) to (-9, 65). Center detectors, 3 cm-1.",,,,,, 2008-234T11:15:00,000T01:39:00,21-Aug-08,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-234T11:15:00,000T01:39:00,21-Aug-08,VIMS,SPASS Rider,Dione,098W003PH,,spectral cubes,Phase study,,,,,, 2008-234T12:29:00,000T11:05:00,21-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-234T14:34:00,000T09:00:00,21-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-234T15:21:00,000T08:00:00,21-Aug-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-235T00:10:00,000T02:00:00,22-Aug-08,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"low-phase, lit-face ring photometry","low-phase lit #1, B' = -5.5",,,,,, 2008-235T00:10:00,000T02:00:00,22-Aug-08,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_081RI_PHOTLIT001_ISS,rider,,,,,, 2008-235T02:10:00,000T00:30:00,22-Aug-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-235T02:40:00,000T02:00:00,22-Aug-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-235T02:40:00,000T02:00:00,22-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_081RI_DEEPSPACE235_CAPS,rider,,,,,, 2008-235T04:40:00,000T03:20:00,22-Aug-08,ISS,Prime,rings(general),GRINGARC,,G-ring arc observation,"G-ring arc observation, need 2 of 15 opportunities",,,,,, 2008-235T04:40:00,000T03:20:00,22-Aug-08,CIRS,SPASS Rider,rings(general),GRINGARC,,CIRS_081RI_GRINGARC001_ISS,rider,,,,,, 2008-235T04:40:00,000T03:20:00,22-Aug-08,VIMS,SPASS Rider,rings(general),GRINGARC,,G Ring arc observation,null,,,,,, 2008-235T08:00:00,000T02:00:00,22-Aug-08,ISS,Prime,Tethys,071W010PH,,Tethys lon/phase angle observation,"Turn UVIS_FUV to Tethys; then offset (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-235T08:00:00,000T02:00:00,22-Aug-08,CIRS,SPASS Rider,Tethys,071W010PH,,CIRS_081TE_071W010PH001_ISS,"Rider on ISS Tethys. Duration T02:00. 0.80phase angle>9.5, (0, 56) to (1, 70). Centers, 3.0 cm-1, shutter: ....",,,,,, 2008-235T08:00:00,000T02:00:00,22-Aug-08,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-235T08:00:00,000T02:00:00,22-Aug-08,VIMS,SPASS Rider,Tethys,071W010PH,,spectral cubes,Phase study,,,,,, 2008-235T09:05:00,000T02:00:00,22-Aug-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-235T10:00:00,000T02:00:00,22-Aug-08,ISS,Prime,Mimas,072W014PH,,Mimas lon/phase angle observation,Turn UVIS_FUV to Mimas; no CIRS rider,,,,,, 2008-235T10:00:00,000T02:00:00,22-Aug-08,CIRS,SPASS Rider,Mimas,072W014PH,,CIRS_081MI_072W014PH001_ISS,rider,,,,,, 2008-235T10:00:00,000T02:00:00,22-Aug-08,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-235T10:00:00,000T02:00:00,22-Aug-08,VIMS,SPASS Rider,Mimas,072W014PH,,spectral cubes,Phase study,,,,,, 2008-235T11:05:00,000T11:37:00,22-Aug-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-235T12:00:00,000T08:00:00,22-Aug-08,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2008-235T12:00:00,000T08:00:00,22-Aug-08,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_081RI_EGPHASE101_VIMS,rider,,,,,, 2008-235T12:00:00,000T08:00:00,22-Aug-08,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2008-235T20:00:00,000T00:49:00,22-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_081RI_DEEPSPACE435_SP,rider,,,,,, 2008-235T20:49:00,000T09:00:00,22-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-235T21:34:00,000T08:00:00,22-Aug-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-235T22:41:00,000T00:00:01,22-Aug-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.4 d, inc = 74.5 deg, r = 20.271 Rs, phase = 23 deg",,,,,, 2008-235T22:42:00,003T04:48:00,22-Aug-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-235T22:42:00,000T07:07:00,22-Aug-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9197700 Rs exit= 4.0465075 Range altitude= -40781.481 km ... 40682.449,,,,,, 2008-235T22:42:00,000T07:07:00,22-Aug-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-235T22:42:00,001T13:18:00,22-Aug-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-235T22:42:00,002T03:51:00,22-Aug-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-236T05:49:00,003T08:02:00,23-Aug-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9197700 Rs exit= 4.0465075 Range altitude= -40781.481 km ... 40682.449,,,,,, 2008-236T05:49:00,002T00:00:00,23-Aug-08,INMS,Non-SPASS,Saturn,SLEEP,Instrument to sleep mode,Survey,Sleep for duration of missing post-OTM requests,,,,,, 2008-236T05:49:00,002T21:41:00,23-Aug-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-236T06:29:00,000T12:00:00,23-Aug-08,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning N. hemisphere, may be split in half by downlink 1 of 3 acceptable (Rev 83 and Rev 84 have identical requests)",,,,,, 2008-236T18:29:00,000T01:05:00,23-Aug-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-236T20:49:00,000T09:00:00,23-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-237T07:19:00,000T10:00:00,24-Aug-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_082SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2008-237T12:00:00,001T15:30:00,24-Aug-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-237T17:19:00,000T02:50:00,24-Aug-08,ISS,Prime,rings(general),RETARMRLP,,Medium res retargetables,Medium Res Retarg of small ring region satellites. Need 25 of 54.,,,,,, 2008-237T18:44:00,000T11:05:00,24-Aug-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-237T20:49:00,000T09:00:00,24-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-237T21:04:00,000T08:45:00,24-Aug-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-238T02:33:00,003T01:16:00,25-Aug-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-238T05:49:00,001T09:18:00,25-Aug-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of inner mag",,,,,, 2008-238T06:29:00,000T07:21:00,25-Aug-08,UVIS,Prime,Saturn,NPOLECAM,,Saturn North Pole Campaign,UVIS/VIMS/ISS/CIRS North Pole Campaign end time set by VIMS GamCru Occ that follows,,,,,, 2008-238T06:29:00,000T07:21:00,25-Aug-08,CIRS,SPASS Rider,Saturn,NPOLECAM,,CIRS_082SA_NPOLECAM1_UVIS,N pole. campaign,,,,,, 2008-238T06:29:00,000T07:21:00,25-Aug-08,ISS,SPASS Rider,Saturn,NPOLECAM,,Polar 1x2 WAC movie in 8 filters,"WAC movie in CB3,MT3,CB2,MT2,VIO,RED,GRN,BL1: follow the template in the note",,,,,, 2008-238T06:29:00,000T07:46:00,25-Aug-08,VIMS,SPASS Rider,Saturn,NPOLEAUR,,North Pole aurora mosaic 1,"Joint observations with UVIS. VIMS will map out frames about 40% of the time. About every 4 hours, one frame of UV aurorae with 1 sec integration/pixel for 70 mins followed by a 2*2 mosaic for dynamics (takes another 40 minutes).",,,,,, 2008-238T13:50:00,000T04:40:00,25-Aug-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. MAG segment.",,,,,, 2008-238T13:50:00,000T04:40:00,25-Aug-08,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_082RI_GAMCRUOCC_VIMS,Ride along with VIMS stellar occultation,,,,,, 2008-238T13:50:00,000T04:40:00,25-Aug-08,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,,,,,,,, 2008-238T18:30:00,000T14:30:00,25-Aug-08,UVIS,Prime,Saturn,NPOLECAM,,Saturn North Pole Campaign,UVIS/VIMS/ISS/CIRS North Pole Campaign,,,,,, 2008-238T18:30:00,000T14:30:00,25-Aug-08,CIRS,SPASS Rider,Saturn,NPOLECAM,,CIRS_082SA_NPOLECAM002_UVIS,N pole. campaign,,,,,, 2008-238T18:30:00,000T14:30:00,25-Aug-08,ISS,SPASS Rider,Saturn,NPOLECAM,,"Polar movie till 239T03:00:00, aurora for the rest","dayside-WAC movie in CB3, MT2,CB2,MT2,BL: follow the template in the note (DAY ISS) aurora: follow (NIGHT ISS)in the template in the note.",,,,,, 2008-238T18:45:00,000T14:15:00,25-Aug-08,VIMS,SPASS Rider,Saturn,NPOLEAUR,,North Pole aurora mosaic 2,"Joint observations with UVIS. VIMS will map out frames about 40% of the time. About every 4 hours, one frame of UV aurorae with 1 sec integration/pixel for 70 mins followed by a 2*2 mosaic for dynamics (takes another 40 minutes).",,,,,, 2008-239T03:30:00,000T05:30:00,26-Aug-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-239T03:30:00,000T05:48:00,26-Aug-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-239T03:30:00,000T10:55:00,26-Aug-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-239T03:30:00,000T10:33:22,26-Aug-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-239T09:00:00,000T03:36:00,26-Aug-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-239T09:00:00,000T05:25:00,26-Aug-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-239T09:18:00,000T12:06:00,26-Aug-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-239T10:00:00,000T02:36:00,26-Aug-08,UVIS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,Saturn Aurora,"Part of CAPS campaign to observe the aurora while on active field lines. Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2008-239T11:11:00,000T02:25:00,26-Aug-08,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 082RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2008-239T13:29:00,000T11:05:00,26-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-239T13:34:29,000T01:39:31,26-Aug-08,CDA,SPASS Rider,DustRAM direction,RPX0010,,CDA RPXing 2008-239T14:34:29 NTH,Nice to have - variation of angular distance to source (longitude),,,,,, 2008-239T13:36:33,000T00:59:00,26-Aug-08,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ring Occultation 082,"Early XM series of RSS ring occultations spanning a chord of the ring system. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 20 minute free-space baseline and calibration period, followed by the occultation and a subsequent 15 minute free-space baseline and calibration period.",,,,,, 2008-239T13:51:00,000T00:22:00,26-Aug-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0444034 Rs exit= 4.0059169 Range altitude= 39751.985 km ... 20138.224,,,,,, 2008-239T14:03:22,000T01:00:00,26-Aug-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-239T14:13:00,000T00:42:00,26-Aug-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.0043600 Rs exit= 3.9628580 Range altitude= 19201.435 km ... -19263.253,,,,,, 2008-239T14:25:00,000T00:30:00,26-Aug-08,CAPS,SPASS Rider,Saturn,IMVP3,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2008-239T14:25:00,000T00:30:00,26-Aug-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-239T14:25:00,000T00:30:00,26-Aug-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-239T14:55:00,000T00:19:00,26-Aug-08,CDA,Prime,DustRAM direction,RPX0010,,CDA RPXing Prime Observation,"This is a prime observation to fill the gap between 239T14:55 and 239T15:14. This will be designed either by CDA or SP. This is due to private communication with Leo during MAGTWT. 02/11/08 CDA will stay at waypoint attitude, no PDT sasf is needed.",,,,,, 2008-239T14:55:00,000T06:30:00,26-Aug-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-239T14:55:00,000T00:22:00,26-Aug-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9623995 Rs exit= 3.9589456 Range altitude= -20199.986 km ... -39809.745,,,,,, 2008-239T14:55:00,000T12:00:00,26-Aug-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-239T15:03:22,000T02:30:38,26-Aug-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-239T15:07:00,000T00:53:00,26-Aug-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-239T15:10:39,000T00:00:01,26-Aug-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.956 Rs, lat = -9 deg, phase = 157 deg",,,,,, 2008-239T15:17:00,003T16:23:00,26-Aug-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9590757 Rs exit= 4.0382403 Range altitude= -40739.811 km ... 40519.964,,,,,, 2008-239T15:34:00,000T09:00:00,26-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-239T16:00:00,003T02:15:00,26-Aug-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-239T17:34:00,000T05:00:00,26-Aug-08,RPWS,SPASS Rider,Saturn,RCSWHIST,RPWS lightning search (RCS),non RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-239T21:24:00,000T05:31:00,26-Aug-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-239T21:25:00,000T05:30:00,26-Aug-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-239T22:34:00,000T04:21:00,26-Aug-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-240T01:14:00,000T11:35:00,27-Aug-08,UVIS,Prime,Saturn,SPOLECAM,Saturn south pole campaign,Saturn South Pole Campaign,UVIS/VIMS/ISS/CIRS South Pole Campaign,,,,,, 2008-240T01:14:00,000T11:35:00,27-Aug-08,CIRS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,CIRS_082SA_SPOLECAM1_UVIS,S pole. campaign,,,,,, 2008-240T01:14:00,000T11:35:00,27-Aug-08,ISS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,"Aurora till 240T3:00:00, then day side","aurora: follow (NIGHT ISS)in the template in the note. dayside-WAC movie in CB3, MT2,CB2,MT2,BL: follow the template in the note (DAY ISS)",,,,,, 2008-240T01:14:00,000T11:35:00,27-Aug-08,VIMS,SPASS Rider,Saturn,SPOLEAUR,,South Pole aurora mosaic 1,"Joint observations with UVIS. VIMS will map out frames about 40% of the time. About every 4 hours, one frame of UV aurorae with 1 sec integration/pixel for 70 mins followed by a 2*2 mosaic for dynamics (takes another 40 minutes).",,,,,, 2008-240T02:55:00,003T04:45:00,27-Aug-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-240T02:55:00,000T11:24:00,27-Aug-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-240T02:55:00,000T19:05:00,27-Aug-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-240T12:14:00,000T11:05:00,27-Aug-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-240T14:19:00,002T01:15:00,27-Aug-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-240T14:19:00,000T09:00:00,27-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-240T22:00:00,002T09:40:00,27-Aug-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-240T23:59:00,000T08:50:00,27-Aug-08,CIRS,Prime,rings(general),TEMPS20LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-240T23:59:00,000T08:50:00,27-Aug-08,UVIS,SPASS Rider,rings(general),TEMPS20LP,,,,,,,,, 2008-241T00:00:00,000T09:10:00,28-Aug-08,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,Standard calibration/gain,,,,,, 2008-241T01:00:00,000T05:00:00,28-Aug-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-241T03:49:00,002T03:51:00,28-Aug-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-241T08:49:00,000T02:50:00,28-Aug-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-241T08:49:00,000T02:50:00,28-Aug-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_082RI_FMONITOR003_ISS,rider,,,,,, 2008-241T11:39:00,000T02:00:00,28-Aug-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-241T12:14:00,000T11:05:00,28-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-241T14:19:00,000T09:00:00,28-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-241T23:59:00,000T05:05:00,28-Aug-08,ISS,Prime,Rhea,ZEROPHASE,Zero phase imaging,(Almost) zero phase,Turn -Y to Rhea; do 1x1 mosaic; turn to WP.,,,,,, 2008-241T23:59:00,000T05:05:00,28-Aug-08,CIRS,SPASS Rider,Rhea,ZEROPHASE,Zero phase imaging,CIRS_082RH_ZEROPHASE (mostly centers calibration),"Ride on ISS zero phase observation, mostly for calibration of pairs. AD~1, phase>0.3, (-5, 50). Duration 05:05. 15.5 cm-1, centers, shutter closed 00:20-00:40, 02:20-02:40, 04:20-04:40.",,,,,, 2008-241T23:59:00,000T05:05:00,28-Aug-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-241T23:59:00,000T05:05:00,28-Aug-08,VIMS,SPASS Rider,Rhea,055W001PH,,spectral cubes,Phase study,,,,,, 2008-242T04:29:00,000T11:05:00,29-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-242T06:34:00,000T09:00:00,29-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-242T08:00:00,000T05:00:00,29-Aug-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-242T15:34:00,002T00:00:00,29-Aug-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-242T16:14:00,000T02:01:00,29-Aug-08,ISS,Prime,Dione,GLOMAP,Saturn global map,Dione Global Color Mapping,Turn -Y to Dione; do 1x1 mosaic; turn to WP.,,,,,, 2008-242T16:14:00,000T02:00:00,29-Aug-08,CIRS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,CIRS_082DI_ICYLON (Mostly calibration for pairs),"Ride on UVIS observation, mostly for calibration of pairs. AD~0.8, phase=8, (1, 60). Duration 02:00. 15.5 cm-1, centers, shutter closed 00:20-00:40, 01:20-01:40.",,,,,, 2008-242T16:14:00,000T02:00:00,29-Aug-08,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-242T16:14:00,000T02:01:00,29-Aug-08,VIMS,SPASS Rider,Dione,DIONE,Dione,spectral cubes,Phase study,,,,,, 2008-242T18:15:00,000T08:10:00,29-Aug-08,ISS,Prime,Other,SATSEARCH,Satellite search,ORBIT 82 SATELLITE SEARCH,A satellite search observation staring off the ansa and taking pairs of WACs every ~5 mins for 14 hours. Looking for small satellites in the Mimas-Enceladus region. This observatiojn can be shortened/moved.,,,,,, 2008-242T18:15:00,000T02:00:00,29-Aug-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-242T20:15:00,000T11:25:00,29-Aug-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-243T02:25:00,000T03:00:00,30-Aug-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-243T04:29:00,000T11:05:00,30-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-243T05:25:00,000T00:29:00,30-Aug-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-243T06:34:00,000T01:06:00,30-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-243T07:39:11,000T00:00:01,30-Aug-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.4 d, inc = 74.5 deg, r = 20.267 Rs, phase = 23 deg",,,,,, 2008-243T07:40:00,003T04:45:00,30-Aug-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-243T07:40:00,003T15:07:00,30-Aug-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9590757 Rs exit= 4.0382403 Range altitude= -40739.811 km ... 40519.964,,,,,, 2008-243T07:40:00,003T04:05:00,30-Aug-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-243T07:40:00,001T14:20:00,30-Aug-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-243T07:40:00,002T03:50:00,30-Aug-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-243T15:34:00,000T00:40:00,30-Aug-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_083RI_DEEPSPACE243_SP,rider,,,,,, 2008-243T16:14:00,000T13:04:00,30-Aug-08,VIMS,Prime,rings(general),FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2008-243T16:14:00,000T13:04:00,30-Aug-08,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,CIRS_083RI_FMOVIE109_VIMS,rider,,,,,, 2008-243T16:14:00,000T13:04:00,30-Aug-08,ISS,SPASS Rider,rings(general),FMOVIE,F ring movie,Medium Res F ring Movie,Medium Resolution F Ring Movie,,,,,, 2008-244T04:29:00,000T11:05:00,31-Aug-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-244T06:34:00,000T09:00:00,31-Aug-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-244T08:00:00,000T06:30:00,31-Aug-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-244T15:34:00,001T20:51:00,31-Aug-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-244T17:04:00,000T07:46:00,31-Aug-08,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,"Titan compoistion, mid southern latitudes (27 deg)",,,,,, 2008-244T22:00:00,001T14:25:00,31-Aug-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-245T00:50:00,000T01:00:00,1-Sep-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-245T00:50:00,000T01:00:00,1-Sep-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_083RI_FMONITOR002_ISS,rider,,,,,, 2008-245T01:50:00,000T01:29:00,1-Sep-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_083RI_DEEPSPACE245_NAV,rider,,,,,, 2008-245T04:14:00,000T11:05:00,1-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period. Also, Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev84 Rings Occultation experiment on DOY 254.",,,,,, 2008-245T06:34:00,000T08:45:00,1-Sep-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-245T11:30:00,003T01:14:00,1-Sep-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-246T04:14:00,000T11:05:00,2-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period. Also, Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev84 Rings Occultation experiment on DOY 254.",,,,,, 2008-246T11:45:00,000T02:00:00,2-Sep-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-246T12:25:00,000T23:25:00,2-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-246T12:25:00,000T05:47:00,2-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-246T12:25:00,000T10:50:00,2-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-246T12:25:00,000T10:35:00,2-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-246T13:45:00,003T13:15:00,2-Sep-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-246T15:59:00,000T07:01:00,2-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-246T18:12:00,000T12:08:00,2-Sep-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-246T22:47:00,000T00:21:00,2-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0361418 Rs exit= 3.9993776 Range altitude= 39588.320 km ... 20887.484,,,,,, 2008-246T22:59:09,000T01:00:00,2-Sep-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-246T23:00:00,000T01:00:00,2-Sep-08,CDA,SPASS Rider,DustRAM direction,RPX0020,,CDA RPXing 2008-246T23:30:29 MH,Must Have - variation of angular distance to source (longitude) The last 18 minutes of this observation does not ride along any obs. Either the SP request this request is riding along has to be extended or CDA has to do the prime design for the last 18 minutes..Mou (01/23/08),,,,,, 2008-246T23:08:00,000T00:43:00,2-Sep-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9978037 Rs exit= 3.9552163 Range altitude= 19949.710 km ... -19499.966,,,,,, 2008-246T23:15:00,000T00:40:00,2-Sep-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-246T23:51:00,000T00:21:00,2-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9547718 Rs exit= 3.9515213 Range altitude= -20437.790 km ... -39138.074,,,,,, 2008-246T23:55:00,000T11:55:00,2-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-247T00:00:00,000T07:19:00,3-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-247T00:00:00,000T11:50:00,3-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-247T00:06:12,000T00:00:01,3-Sep-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.949 Rs, lat = -9 deg, phase = 157 deg",,,,,, 2008-247T00:12:00,003T16:21:00,3-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9516412 Rs exit= 4.0363552 Range altitude= -40069.545 km ... 40824.669,,,,,, 2008-247T04:14:00,000T11:05:00,3-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period. Also, Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev84 Rings Occultation experiment on DOY 254.",,,,,, 2008-247T06:20:00,000T05:30:00,3-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-247T11:50:00,003T04:44:00,3-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-247T11:50:00,004T03:14:00,3-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-247T11:50:00,000T19:10:00,3-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-248T04:14:00,000T11:05:00,4-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-248T07:00:00,002T09:34:00,4-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-248T08:15:00,000T11:45:00,4-Sep-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-248T12:44:00,002T03:49:00,4-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-249T04:14:00,000T11:05:00,5-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-250T03:00:00,000T02:00:00,6-Sep-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-250T03:59:00,000T11:05:00,6-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-250T05:00:00,000T11:34:00,6-Sep-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-250T16:32:46,000T00:00:01,6-Sep-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.4 d, inc = 74.5 deg, r = 20.266 Rs, phase = 23 deg",,,,,, 2008-250T16:33:00,003T15:07:00,6-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9516412 Rs exit= 4.0363552 Range altitude= -40069.545 km ... 40824.669,,,,,, 2008-250T16:33:00,002T03:50:00,6-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-250T16:34:00,003T04:41:00,6-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-250T16:34:00,003T01:26:00,6-Sep-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-250T16:34:00,001T13:56:00,6-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-251T01:20:00,000T02:00:00,7-Sep-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-251T03:20:00,000T01:14:00,7-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-251T03:59:00,000T11:05:00,7-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-251T06:04:00,000T09:00:00,7-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-251T15:04:00,002T00:00:00,7-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-251T16:40:00,000T11:09:00,7-Sep-08,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side",Do 15 unlit side at priority 2 (~every third orbit),,,,,, 2008-251T16:40:00,000T11:09:00,7-Sep-08,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_084RI_APOMOSU106_VIMS,rider,,,,,, 2008-252T03:49:00,000T01:00:00,8-Sep-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-252T03:49:00,000T01:00:00,8-Sep-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_084RI_FMONITOR002_ISS,rider,,,,,, 2008-252T03:59:00,000T11:05:00,8-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-252T04:49:00,000T01:14:00,8-Sep-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_084RI_DEEPSPACE252_NAV,rider,,,,,, 2008-252T06:04:00,000T09:00:00,8-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-252T06:30:00,001T14:45:00,8-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-252T15:45:00,000T02:00:00,8-Sep-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-252T17:45:00,000T00:40:00,8-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-252T18:25:00,000T11:00:00,8-Sep-08,VIMS,Prime,Saturn,NPOLEAUR,,North Pole aurora mosaic 1,"2x2 North Polar mosaics (1 sec integration, 70 mins per frame),followed by 2*2 dynamics mosaic (10 mins per frame). Takes 5hr 20 min hours per loop. Do this twice.",,,,,, 2008-252T18:25:00,000T11:00:00,8-Sep-08,CIRS,SPASS Rider,Saturn,NPOLEAUR,,CIRS_084SA_NPOLEAUR001_VIMS,N pole. capaign,,,,,, 2008-252T20:23:00,003T01:14:00,8-Sep-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-253T03:59:00,000T11:05:00,9-Sep-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-253T06:04:00,000T09:00:00,9-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-253T07:04:00,000T07:00:00,9-Sep-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-253T15:04:00,000T06:11:00,9-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-253T15:44:00,000T05:47:00,9-Sep-08,VIMS,Prime,Saturn,NPOLEAUR,,North Pole aurora mosaic 3,"Begin with 2*2 dynamics mosaics, 8 min between frame centers; Then 2x2 North Polar mosaics (1 sec integration, 70 mins per frame). Then second 2*2 dynamics mosaic ( 8 mins between frame centers). Takes 5hr 44 min.",,,,,, 2008-253T18:00:00,000T02:00:00,9-Sep-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-253T20:00:00,003T16:00:00,9-Sep-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-253T21:15:00,000T05:05:00,9-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-253T21:15:00,000T05:49:00,9-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-253T21:15:00,000T10:55:00,9-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-253T21:15:00,000T10:45:00,9-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-253T21:31:00,000T04:44:00,9-Sep-08,CIRS,Prime,Tethys,SECLNX,,CIRS_084TE_SECLNX001_PRIME;,"FP1N, X;2.0-2.5; N hem; stable pointing; LT~13. Entry at 253T22:01:15; exit at 254T00:43:34 -- Note use of out-of-date start time (should be half hour earlier, at 21:01:15). Must watch choice of waypoint to see whether adequate initial turn time (Frank has the 05:47 before this observation).",,,,,, 2008-253T21:31:00,000T04:44:00,9-Sep-08,CIRS,SPASS Rider,Tethys,SECLNX,,CIRS_084TE SECLNX SI,"3 NAC SI for for pointing verification: 2 for eclipse observation, 1 for NAC stare; can use lossy compression; +/- 1 minute tolerance. First NAC at 2008-253T21:56 (5 min. before entry; entry at 2008-253T22:01:15); AD=2.0 mrad; Second NAC at 2008-253T23:07 (5 min. before turn to space for FP1 calibration); AD=2.3 mrad; --- expose for grey light; Third NAC at 2008-254T00:50 (7 min. past exit; exit at 2008-255T00:43:34); AD=2.4 mrad.",,,,,, 2008-253T21:31:00,000T04:44:00,9-Sep-08,ISS,SPASS Rider,Tethys,SECLNX,,TETHYS eclipse,TETHYS eclipse,,,,,, 2008-253T21:31:00,000T04:44:00,9-Sep-08,VIMS,SPASS Rider,Tethys,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-254T02:15:00,000T04:22:00,10-Sep-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T02:15:00,000T04:17:00,10-Sep-08,UVIS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,Saturn Aurora,"Part of CAPS campaign to observe the aurora while on active field lines. Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2008-254T02:20:00,000T04:17:00,10-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T03:04:00,000T12:10:00,10-Sep-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-254T05:07:00,000T02:25:00,10-Sep-08,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 084RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2008-254T06:37:00,000T01:33:00,10-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T07:23:29,000T01:37:31,10-Sep-08,CDA,SPASS Rider,DustRAM direction,RPX0030,,CDA RPXing 2008-254T08:23:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-254T07:32:27,000T00:55:00,10-Sep-08,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ring Occultation 084,"Early XM series of RSS ring occultations spanning a chord of the ring system. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 20 minute free-space baseline and calibration period, followed by the occultation and a subsequent 15 minute free-space baseline and calibration period.",,,,,, 2008-254T07:40:00,000T00:22:00,10-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0342535 Rs exit= 3.9958532 Range altitude= 39892.753 km ... 20247.656,,,,,, 2008-254T07:52:27,000T01:00:00,10-Sep-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-254T08:02:00,000T00:42:00,10-Sep-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9943021 Rs exit= 3.9531774 Range altitude= 19309.341 km ... -19219.102,,,,,, 2008-254T08:10:00,000T00:40:00,10-Sep-08,CAPS,SPASS Rider,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Part of MAPS Survey,,,,,, 2008-254T08:10:00,000T00:40:00,10-Sep-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-254T08:44:00,000T00:22:00,10-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9527314 Rs exit= 3.9495773 Range altitude= -20157.392 km ... -39799.498,,,,,, 2008-254T08:50:00,000T00:37:00,10-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T08:50:00,000T11:55:00,10-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-254T08:50:00,000T11:55:00,10-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-254T08:59:24,000T00:00:01,10-Sep-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.947 Rs, lat = -9 deg, phase = 157 deg",,,,,, 2008-254T09:06:00,001T05:43:00,10-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S44,Range enter= 3.9497233 Rs exit= 4.0346349 Range altitude= -40731.080 km ... 40683.727,,,,,, 2008-254T09:27:00,000T04:30:00,10-Sep-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T09:27:00,000T04:30:00,10-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T09:27:00,000T04:30:00,10-Sep-08,UVIS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,Saturn Aurora,"Part of CAPS campaign to observe the aurora while on active field lines. Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2008-254T13:57:00,000T14:22:00,10-Sep-08,UVIS,Prime,Saturn,SPOLECAM,Saturn south pole campaign,Saturn South Pole Campaign,UVIS/VIMS/ISS/CIRS South Pole Campaign,,,,,, 2008-254T13:57:00,000T06:48:00,10-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-254T13:57:00,000T14:22:00,10-Sep-08,CIRS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,CIRS_084SA_SPOLECAM1_UVIS,S pole. capaign,,,,,, 2008-254T13:57:00,000T14:22:00,10-Sep-08,ISS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,"Aurora till 254T15:00:00, then day side","aurora: follow (NIGHT ISS)in the template in the note. dayside-WAC movie in CB3, MT2,CB2,MT2,BL: follow the template in the note (DAY ISS)",,,,,, 2008-254T13:57:00,000T14:22:00,10-Sep-08,VIMS,SPASS Rider,Saturn,SPOLEAUR,,South Pole aurora mosaic 1,"Joint observations with UVIS. VIMS will map out frames about 40% of the time. About every 4 hours, one frame of UV aurorae with 1 sec integration/pixel for 70 mins followed by a 2*2 mosaic for dynamics (takes another 40 minutes).",,,,,, 2008-254T15:14:00,000T05:31:00,10-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-254T20:45:00,003T01:34:00,10-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-254T20:45:00,000T23:30:00,10-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-254T20:45:00,000T19:15:00,10-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-255T03:44:00,000T11:05:00,11-Sep-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-255T05:49:00,000T09:00:00,11-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-255T14:49:00,001T00:00:00,11-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S44,Range enter= 3.9497233 Rs exit= 4.0346349 Range altitude= -40731.080 km ... 40683.727,,,,,, 2008-255T15:29:00,000T04:46:00,11-Sep-08,VIMS,Prime,Saturn,SPOLEAUR,,South Pole aurora mosaic 3,"2x2 North Polar mosaic (1 sec integration, 70 mins per frame). Takes 4 hr 40 min.",,,,,, 2008-255T15:29:00,000T04:46:00,11-Sep-08,UVIS,SPASS Rider,Saturn,SPOLEAUR,,Saturn Aurora,Rider on VIMS SPOLEAUR observations,,,,,, 2008-255T16:00:00,002T06:19:00,11-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-255T20:15:00,000T05:00:00,11-Sep-08,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-255T21:37:00,002T00:42:00,11-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-256T01:15:00,000T03:04:00,12-Sep-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_084SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere (87 S)",,,,,, 2008-256T01:15:00,000T13:04:00,12-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-256T03:44:00,000T11:05:00,12-Sep-08,RSS,SPASS Rider,Earth,SCE5,,Solar Conjunction Experiment (SCE) #5,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2008-256T05:49:00,000T09:00:00,12-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-256T14:19:00,001T08:00:00,12-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-256T14:49:00,001T07:30:00,12-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S44,Range enter= 3.9497233 Rs exit= 4.0346349 Range altitude= -40731.080 km ... 40683.727,,,,,, 2008-256T15:29:00,000T05:16:00,12-Sep-08,CIRS,Prime,rings(general),SUBMS10LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-256T20:45:00,000T04:00:00,12-Sep-08,ISS,Prime,Enceladus,PLMLP,Low phas plume imaging,low phase Observation,low phase observation,,,,,, 2008-256T20:45:00,000T04:00:00,12-Sep-08,CIRS,SPASS Rider,Enceladus,PLMLP,Low phas plume imaging,CIRS_084EN_PLMLP001_ISS,rider,,,,,, 2008-256T20:45:00,000T04:00:00,12-Sep-08,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2008-256T20:45:00,000T04:00:00,12-Sep-08,VIMS,SPASS Rider,Enceladus,PLMLP,Low phas plume imaging,spectral cubes,Enceladus Plume,,,,,, 2008-257T00:45:00,000T00:30:00,13-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-257T01:15:00,000T06:30:00,13-Sep-08,UVIS,Prime,Rhea,ICYSTARE,,ICYSTARE: long satellite stare,Long integration to look for trace volatiles,,,,,, 2008-257T01:15:00,000T06:30:00,13-Sep-08,CIRS,SPASS Rider,Rhea,ICYSTARE,,CIRS_084RH_ICYSTARE001_UVIS,"Rider on long UVIS Rhea integration at low phase angle. Duration 06:30. 2.4>AD>2.1, 214, r<7.5",,,,,, 2008-261T06:05:00,000T10:55:00,17-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-261T06:05:00,000T10:37:00,17-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-261T08:00:00,000T06:20:00,17-Sep-08,UVIS,Prime,Star,URALPARA,Alpha Ara occultation,URSTAR,,,,,,, 2008-261T08:00:00,000T06:20:00,17-Sep-08,CIRS,SPASS Rider,rings(general),URALPARA,Alpha Ara occultation,CIRS_085RI_URALPARA001_UVIS,rider,,,,,, 2008-261T08:00:00,000T06:20:00,17-Sep-08,UVIS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Support Imaging,NAC support images at the following times: 2008-261t08:49:0 2008-261t08:58:20.0 2008-261t09:31:31.5 2008-261t13:34:50.0 2008-261t13:25:02.0 2008-261t12:50:47.0,,,,,, 2008-261T10:30:00,000T02:50:00,17-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-261T11:54:00,000T12:09:00,17-Sep-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-261T13:20:00,000T03:40:00,17-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-261T14:20:00,000T01:40:00,17-Sep-08,ISS,Prime,Enceladus,PLMMP,,intermediate phase Observation,intermediate phase observation,,,,,, 2008-261T14:20:00,000T01:40:00,17-Sep-08,CIRS,SPASS Rider,Enceladus,PLMMP,,CIRS_085EN_PLMMP001_ISS,rider,,,,,, 2008-261T14:20:00,000T01:40:00,17-Sep-08,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2008-261T14:20:00,000T01:40:00,17-Sep-08,VIMS,SPASS Rider,Enceladus,PLMMP,,spectral cubes,Enceladus Plume,,,,,, 2008-261T16:00:00,000T01:45:00,17-Sep-08,VIMS,Prime,rings(general),SOLAROCC,Solar occultation,Ring solar occ,"2 at priority 1, and 2 at priority 2. B chord.",,,,,, 2008-261T16:00:00,000T01:45:00,17-Sep-08,CIRS,SPASS Rider,rings(general),SOLOCCS,,CIRS_085RI_SOLOCCS106_VIMS,rider,,,,,, 2008-261T16:00:00,000T01:45:00,17-Sep-08,UVIS,SPASS Rider,rings(general),SOLOCCS,,UV Ring solar occultation,,,,,,, 2008-261T16:13:29,000T02:00:00,17-Sep-08,CDA,SPASS Rider,DustRAM direction,RPX0040,,CDA RPXing 2008-261T17:13:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-261T16:30:00,000T00:22:00,17-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0325436 Rs exit= 3.9943716 Range altitude= 39751.607 km ... 20102.429,,,,,, 2008-261T16:42:00,000T01:00:00,17-Sep-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-261T16:50:00,000T02:00:00,17-Sep-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-261T16:52:00,000T00:42:00,17-Sep-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9928318 Rs exit= 3.9521943 Range altitude= 19163.931 km ... -19370.779,,,,,, 2008-261T17:00:00,000T00:40:00,17-Sep-08,CAPS,SPASS Rider,Saturn,IMVP3,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2008-261T17:00:00,000T00:40:00,17-Sep-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-261T17:34:00,000T00:22:00,17-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9517607 Rs exit= 3.9488712 Range altitude= -20309.189 km ... -39953.416,,,,,, 2008-261T17:40:00,000T03:20:00,17-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-261T17:40:00,000T11:50:00,17-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-261T17:42:00,000T11:48:00,17-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-261T17:45:00,000T02:55:00,17-Sep-08,ISS,Prime,rings(general),AZSCANLIT,,AZSCAN lit,non-contig. azscan A Ring Group,,,,,, 2008-261T17:45:00,000T02:55:00,17-Sep-08,CIRS,SPASS Rider,rings(general),AZSCANLIT,,CIRS_085RI_AZSCANLIT001_ISS,rider,,,,,, 2008-261T17:49:05,000T00:00:01,17-Sep-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.946 Rs, lat = -8 deg, phase = 157 deg",,,,,, 2008-261T17:56:00,003T16:18:00,17-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9490300 Rs exit= 4.0314140 Range altitude= -40885.080 km ... 40234.663,,,,,, 2008-261T18:50:00,003T02:59:00,17-Sep-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-261T20:40:00,000T06:30:00,17-Sep-08,CIRS,Prime,Enceladus,SECLNX,,CIRS_085EN_SECLNX001_PRIME;,"FP1 NX; AD=2.5-1.2, phase=76-60, (-64, 44)-(-63, 31); S polar look for FP1 effect of endogenic source; and FP3 integration or slow scan of south polar region near eclipse end for total endogenic energy. Stable pointing. Rings TWT. Start 261T20:40, N261T21:39:45, X262T00:09:00, end 262T03:10. FP1+FP3",,,,,, 2008-261T20:40:00,000T06:30:00,17-Sep-08,CIRS,SPASS Rider,Enceladus,SECLNX,,CIRS_085EN SECLNX SI,Five NAC images: 1) NAC at 2008-261T21:35 (pre-entry; sunlight); 2) NAC at 2008-261T22:45 (eclipsed; grey light or stars); 3) NAC at 2008-261T23:10 (post-exit; sunlight); 4) NAC at 2008-262T00:50 (sunlight); 5) NAC at 2008-262T02:30 (daylight).,,,,,, 2008-261T20:40:00,000T06:30:00,17-Sep-08,ISS,SPASS Rider,Enceladus,SECLNX,,ENCELADUS,ENCELADUS,,,,,, 2008-261T20:40:00,000T06:30:00,17-Sep-08,VIMS,SPASS Rider,Enceladus,SECLNX,,spectral cubes,eclipse,,,,,, 2008-261T21:00:00,000T02:15:00,17-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-261T23:15:00,000T06:15:00,17-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-262T00:03:00,000T05:27:00,18-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-262T03:10:00,000T01:00:00,18-Sep-08,VIMS,Prime,rings(general),SHADSCANL,,Ring SHADSCAN lit side,Do 2 at priority 1,,,,,, 2008-262T03:10:00,000T01:00:00,18-Sep-08,CIRS,SPASS Rider,rings(general),SHADSCANL,,CIRS_085RI_SHADSCANL107_VIMS,rider,,,,,, 2008-262T03:29:00,000T11:05:00,18-Sep-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-262T05:30:00,003T04:44:00,18-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-262T05:30:00,003T16:19:00,18-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-262T05:30:00,000T18:30:00,18-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-262T05:34:00,000T09:00:00,18-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-262T06:19:00,000T04:00:00,18-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-262T15:05:00,000T05:35:00,18-Sep-08,CIRS,Prime,rings(general),VCASLSLP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-262T15:05:00,000T05:35:00,18-Sep-08,CIRS,SPASS Rider,rings(general),VCASLSLP,,CIRS_085RI_VCASLSLP001_SI,,,,,,, 2008-262T15:05:00,000T05:35:00,18-Sep-08,UVIS,SPASS Rider,rings(general),VCASLSLP,,,,,,,,, 2008-262T20:40:00,000T09:00:00,18-Sep-08,VIMS,Prime,rings(general),RSCNCOCC,,Ring stellar occ - RS Cnc,"RS_Cnc occultation, outer C ring, R0=2.348, Rf=2.342, Rmin=1.346",,,,,, 2008-262T20:40:00,000T09:00:00,18-Sep-08,CIRS,SPASS Rider,rings(general),RSCNCOCC,,CIRS_085RI_RSCNCOCC201_VIMS,rider,,,,,, 2008-262T20:40:00,000T09:00:00,18-Sep-08,UVIS,SPASS Rider,rings(general),RSCNCOCC,,,,,,,,, 2008-263T00:00:00,002T10:14:00,19-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-263T06:09:00,000T08:25:00,19-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-263T06:24:00,000T08:10:00,19-Sep-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-263T06:28:00,000T08:06:00,19-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-263T06:54:00,000T04:00:00,19-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-263T14:34:00,001T19:40:00,19-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-263T15:05:00,000T04:10:00,19-Sep-08,CIRS,Prime,rings(general),TMAPS10LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-263T15:05:00,000T04:10:00,19-Sep-08,CIRS,SPASS Rider,rings(general),TMAPS10LP,,CIRS_085RI_TMAPS10LP001_SI,,,,,,, 2008-263T15:05:00,000T04:10:00,19-Sep-08,UVIS,SPASS Rider,rings(general),TMAPS10LP,,,,,,,,, 2008-263T18:00:00,000T04:33:04,19-Sep-08,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2008-263T19:15:00,000T10:20:00,19-Sep-08,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2008-263T19:15:00,000T10:20:00,19-Sep-08,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_085RI_SPKMVLFLP001_ISS,rider,,,,,, 2008-263T19:15:00,000T10:20:00,19-Sep-08,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie - litside,null,,,,,, 2008-264T05:35:00,000T00:30:00,20-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-264T06:05:00,000T02:00:00,20-Sep-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-264T08:05:00,000T01:15:00,20-Sep-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 72.9, range 1.56 Mkm",,,,,, 2008-264T08:05:00,000T01:15:00,20-Sep-08,CIRS,SPASS Rider,Titan,MR2CLD,,CIRS_085TI_MR2CLD263_ISS,rider,,,,,, 2008-264T08:05:00,000T01:15:00,20-Sep-08,UVIS,SPASS Rider,Titan,MR2CLD,,MR2CLD Rider for Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2008-264T09:20:00,000T02:00:00,20-Sep-08,ISS,Prime,Rhea,050W005PH,,Rhea lon/phase angle observation,"Turn UVIS_FUV to Rhea; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-264T09:20:00,000T02:00:00,20-Sep-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-264T09:20:00,000T02:00:00,20-Sep-08,VIMS,SPASS Rider,Rhea,050W005PH,,spectral cubes,Phase study,,,,,, 2008-264T11:20:00,000T01:28:00,20-Sep-08,CIRS,SPASS Rider,Skeletonrequest,OPNAV,Optical navigation image,CIRS_085SK_OPNAV641_NAV,rider,,,,,, 2008-264T12:49:00,000T09:00:00,20-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-264T13:34:00,000T08:00:00,20-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-264T21:49:00,000T05:11:00,20-Sep-08,INMS,Non-SPASS,Saturn,SURVPOTMA,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-264T22:25:00,000T02:00:00,20-Sep-08,ISS,Prime,Mimas,085W013PH,,Mimas lon/phase angle observation,"Turn UVIS_FUV to Mimas; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-264T22:25:00,000T02:00:00,20-Sep-08,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-264T22:25:00,000T02:00:00,20-Sep-08,VIMS,SPASS Rider,Mimas,085W013PH,,spectral cubes,Phase study,,,,,, 2008-265T00:25:00,000T00:30:00,21-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-265T00:55:00,000T01:15:00,21-Sep-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 62.4, range 1.81 Mkm",,,,,, 2008-265T00:55:00,000T01:15:00,21-Sep-08,CIRS,SPASS Rider,Titan,MR2CLD,,CIRS_085TI_MR2CLD264_ISS,rider,,,,,, 2008-265T00:55:00,000T01:15:00,21-Sep-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-265T02:10:00,000T09:09:00,21-Sep-08,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2008-265T02:10:00,000T09:09:00,21-Sep-08,CIRS,SPASS Rider,rings(general),EGPHASE,,VIMS rider,VIMS rider,,,,,, 2008-265T02:10:00,000T09:09:00,21-Sep-08,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2008-265T03:00:00,000T07:14:00,21-Sep-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-265T10:13:39,000T00:00:01,21-Sep-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.4 d, inc = 74.5 deg, r = 20.264 Rs, phase = 23 deg",,,,,, 2008-265T10:14:00,003T04:41:00,21-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-265T10:14:00,003T15:06:00,21-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9490300 Rs exit= 4.0314140 Range altitude= -40885.080 km ... 40234.663,,,,,, 2008-265T10:14:00,000T11:35:00,21-Sep-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-265T10:14:00,001T14:16:00,21-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-265T10:14:00,002T03:50:00,21-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-265T12:49:00,000T09:00:00,21-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-265T13:34:00,000T08:00:00,21-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-265T21:49:00,003T03:46:00,21-Sep-08,INMS,Non-SPASS,Saturn,SURVBOTMA,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-265T21:49:00,002T17:06:00,21-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-265T22:25:00,000T03:00:00,21-Sep-08,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2008-266T01:25:00,000T01:00:00,22-Sep-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-266T01:25:00,000T01:00:00,22-Sep-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_086RI_FMONITOR001_ISS,rider,,,,,, 2008-266T02:25:00,000T01:15:00,22-Sep-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 51.4, range 2.04 Mkm",,,,,, 2008-266T02:25:00,000T01:15:00,22-Sep-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-266T03:40:00,000T01:05:00,22-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-266T05:19:00,000T09:00:00,22-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-266T06:04:00,000T04:00:00,22-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-266T14:55:00,000T11:50:00,22-Sep-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_086SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2008-267T00:30:00,001T14:25:00,23-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-267T02:45:00,000T02:00:00,23-Sep-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-267T05:19:00,000T09:00:00,23-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-267T06:04:00,000T08:00:00,23-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-267T14:04:00,003T01:14:00,23-Sep-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-267T15:34:00,000T09:56:00,23-Sep-08,CIRS,Prime,rings(general),VTMPN60LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-267T15:34:00,000T09:56:00,23-Sep-08,CIRS,SPASS Rider,rings(general),VTMPN60LP,,CIRS_086RI_VTMPN60LP001_SI,,,,,,, 2008-267T15:34:00,000T09:56:00,23-Sep-08,UVIS,SPASS Rider,rings(general),VTMPN60LP,,,,,,,,, 2008-268T01:30:00,000T04:35:00,24-Sep-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. MAG segment.",,,,,, 2008-268T01:30:00,000T04:35:00,24-Sep-08,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_086RI_GAMCRUOCC004_VIMS,rider,,,,,, 2008-268T01:30:00,000T04:35:00,24-Sep-08,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,,,,,,,, 2008-268T02:59:00,000T11:05:00,24-Sep-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-268T06:34:00,000T07:30:00,24-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-268T07:19:00,000T04:00:00,24-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-268T14:35:00,000T02:10:00,24-Sep-08,VIMS,Prime,rings(general),SHADSCANU,,Ring SHADSCAN unlit side,Do 2 at priority 1,,,,,, 2008-268T14:35:00,000T02:10:00,24-Sep-08,CIRS,SPASS Rider,rings(general),SHADSCANU,,CIRS_086RI_SHADSCANU108_VIMS,rider,,,,,, 2008-268T14:55:00,000T04:20:00,24-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-268T14:55:00,000T05:47:00,24-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-268T14:55:00,000T10:50:00,24-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-268T14:55:00,000T10:37:00,24-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-268T16:45:00,000T06:30:00,24-Sep-08,UVIS,Prime,Star,URALPARA,Alpha Ara occultation,URSTAR,,,,,,, 2008-268T16:45:00,000T06:30:00,24-Sep-08,CIRS,SPASS Rider,rings(general),URALPARA,Alpha Ara occultation,CIRS_086RI_URALPARA001_UVIS,rider,,,,,, 2008-268T16:45:00,000T06:30:00,24-Sep-08,UVIS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Support Imaging,NAC support images at the following times: 2008-268t17:39:0 2008-268t17:48:42.0 2008-268t18:21:45.0 2008-268t22:24:0 2008-268t22:15:27.0 2008-268t21:41:20.0,,,,,, 2008-268T19:15:00,000T03:00:00,24-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-268T20:42:00,000T12:10:00,24-Sep-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-268T22:15:00,000T03:30:00,24-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-268T23:15:00,000T04:15:00,24-Sep-08,CIRS,Prime,Tethys,SECLN,,CIRS_086TE_SECLN001_PRIME;,"LIEN: FP13N, target (25, 325); 9.0-10.0-6.7; straddles C/A, N hem; LT~14. N269T00:31:08, C/A 269T01:24, X269T03:15:29 (iDigit). Start 6.2, 65, (60, 335) LT~12.5 -- C/A 9.7, 50, (17, 313) LT~15 -- End 6.4, 63, (-30, 314) LT~16.5.",,,,,, 2008-268T23:15:00,000T04:15:00,24-Sep-08,CIRS,SPASS Rider,Tethys,SECLN,,CIRS_085TE SECLN SI,Four WAC images: 1) WAC at 2008-269T00:26 (pre-entry; sunlight); 2) WAC at 2008-269T01:26 (eclipsed; grey light or stars); 3) WAC at 2008-269T01:45 (eclipsed; grey light or stars); 4) WAC at 2008-269T03:05 (eclipsed; grey light or stars).,,,,,, 2008-268T23:15:00,000T04:15:00,24-Sep-08,ISS,SPASS Rider,Tethys,SECLN,,Tethys eclipse CIRS RIDER,Tethys eclipse CIRS RIDER,,,,,, 2008-268T23:15:00,000T04:15:00,24-Sep-08,VIMS,SPASS Rider,Tethys,SECLN,,spectral cubes,eclipse,,,,,, 2008-269T01:02:29,000T02:00:00,25-Sep-08,CDA,SPASS Rider,DustRAM direction,RPX0050,,CDA RPXing 2008-269T02:02:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-269T01:20:00,000T00:21:00,25-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0293405 Rs exit= 3.9931035 Range altitude= 39302.013 km ... 20581.323,,,,,, 2008-269T01:32:00,000T01:00:00,25-Sep-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-269T01:35:00,000T02:00:00,25-Sep-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-269T01:41:00,000T00:43:00,25-Sep-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9915572 Rs exit= 3.9502287 Range altitude= 19642.573 km ... -19845.477,,,,,, 2008-269T01:45:00,000T00:45:00,25-Sep-08,CAPS,SPASS Rider,Saturn,IMVP3,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2008-269T01:45:00,000T00:45:00,25-Sep-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-269T02:24:00,000T00:21:00,25-Sep-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9498162 Rs exit= 3.9472239 Range altitude= -20784.137 km ... -39500.181,,,,,, 2008-269T02:30:00,000T03:15:00,25-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-269T02:30:00,000T11:50:00,25-Sep-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-269T02:32:00,000T11:48:00,25-Sep-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-269T02:38:27,000T00:00:01,25-Sep-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.944 Rs, lat = -8 deg, phase = 157 deg",,,,,, 2008-269T02:45:00,003T16:18:00,25-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9473775 Rs exit= 4.0326784 Range altitude= -40432.390 km ... 40498.642,,,,,, 2008-269T03:30:00,000T04:30:00,25-Sep-08,ISS,Prime,rings(general),RADSCAN,,Ring Half Radial Scan,"Ring Radial Scan, need 2 out of 5",,,,,, 2008-269T03:30:00,000T04:30:00,25-Sep-08,CIRS,SPASS Rider,rings(general),RADSCAN,,CIRS_086RI_RADSCAN001_ISS,rider,,,,,, 2008-269T03:30:00,000T04:30:00,25-Sep-08,VIMS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,Ring COMPHILIT,Do 4 at priority 1.,,,,,, 2008-269T03:35:00,003T02:05:00,25-Sep-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-269T05:45:00,000T02:15:00,25-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-269T08:00:00,000T04:00:00,25-Sep-08,CIRS,Prime,rings(general),VTMPS70MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-269T08:00:00,000T06:20:00,25-Sep-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-269T08:00:00,000T04:00:00,25-Sep-08,CIRS,SPASS Rider,rings(general),VTMPS70MP,,CIRS_086RI_VTMPS70MP001_SI,,,,,,, 2008-269T08:00:00,000T04:00:00,25-Sep-08,UVIS,SPASS Rider,rings(general),VTMPS70MP,,,,,,,,, 2008-269T08:00:00,000T04:00:00,25-Sep-08,VIMS,SPASS Rider,rings(general),VTMPS70MP,,,null,,,,,, 2008-269T08:52:00,000T05:28:00,25-Sep-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-269T10:29:00,000T11:05:00,25-Sep-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-269T12:34:00,000T09:00:00,25-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-269T13:19:00,000T08:00:00,25-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-269T14:20:00,003T04:43:00,25-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-269T14:20:00,003T07:00:00,25-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-269T14:20:00,000T18:40:00,25-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-269T22:05:00,000T01:15:00,25-Sep-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 13.3, range 1.67 Mkm",,,,,, 2008-269T22:05:00,000T01:15:00,25-Sep-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-269T23:20:00,000T08:45:00,25-Sep-08,CIRS,Prime,rings(general),SUBMS45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-269T23:20:00,000T08:45:00,25-Sep-08,CIRS,SPASS Rider,rings(general),SUBMS45LP,,CIRS_086RI_SUBMS45LP001_SI,,,,,,, 2008-269T23:20:00,000T08:45:00,25-Sep-08,UVIS,SPASS Rider,rings(general),SUBMS45LP,,,,,,,,, 2008-269T23:20:00,000T08:45:00,25-Sep-08,VIMS,SPASS Rider,rings(general),SUBMS45LP,,,null,,,,,, 2008-270T00:00:00,000T00:34:08,26-Sep-08,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2008-270T08:05:00,000T00:30:00,26-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-270T08:35:00,000T03:25:00,26-Sep-08,ISS,Prime,Rhea,GEOLOG,Geologic study,Rhea mapping,Turn -Y to Rhea; do 1x1 mosaic; turn to WP,,,,,, 2008-270T08:35:00,000T03:25:00,26-Sep-08,CIRS,SPASS Rider,Rhea,GEOLOG,Geologic study,CIRS_086RH_GEOLOG002_ISS,rider,,,,,, 2008-270T08:35:00,000T03:25:00,26-Sep-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-270T08:35:00,000T03:25:00,26-Sep-08,VIMS,SPASS Rider,Rhea,GEOLOG,Geologic study,mapping cubes,Lat-Long Vgr class,,,,,, 2008-270T09:00:00,002T10:03:00,26-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-270T12:34:00,000T09:00:00,26-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-270T12:49:00,000T08:45:00,26-Sep-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-270T13:19:00,000T04:00:00,26-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-270T15:18:00,002T03:45:00,26-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-270T22:05:00,000T10:25:00,26-Sep-08,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities (backup),,,,,, 2008-270T22:05:00,000T10:25:00,26-Sep-08,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_086RI_SPKMVLFLP002_ISS,rider,,,,,, 2008-270T22:05:00,000T10:25:00,26-Sep-08,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie - litside,null,,,,,, 2008-271T08:30:00,000T00:30:00,27-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-271T09:00:00,000T03:20:00,27-Sep-08,VIMS,Prime,rings(general),RLEOOCC,R Leo occultation,Ring stellar occ - R Leo,Outer A ring; do 3 at priority 2,,,,,, 2008-271T09:00:00,000T03:20:00,27-Sep-08,CIRS,SPASS Rider,rings(general),RLEOOCC,R Leo occultation,CIRS_086RI_RLEOOCC301_VIMS,rider,,,,,, 2008-271T09:00:00,000T03:20:00,27-Sep-08,UVIS,SPASS Rider,rings(general),RLEOOCC,R Leo occultation,,,,,,,, 2008-271T13:00:00,000T08:35:00,27-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-271T13:45:00,000T07:50:00,27-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-271T22:15:00,000T01:00:00,27-Sep-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-271T22:15:00,000T01:00:00,27-Sep-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_086RI_FMONITOR003_ISS,rider,,,,,, 2008-271T23:15:00,000T06:55:00,27-Sep-08,ISS,Prime,rings(general),FNTLPLE,,Phase Curve and color measurements of faint rings,"Low res, low elev., high-phase of E ring, need 3 of 20 opportunities",,,,,, 2008-271T23:15:00,000T06:55:00,27-Sep-08,CIRS,SPASS Rider,rings(general),FNTLPLE,,CIRS_086RI_FNTLPLE001_ISS,rider,,,,,, 2008-271T23:15:00,000T06:55:00,27-Sep-08,VIMS,SPASS Rider,rings(general),FNTLPLE,,faint ring observation,null,,,,,, 2008-272T05:40:00,000T02:00:00,28-Sep-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-272T06:10:00,000T02:00:00,28-Sep-08,ISS,Prime,Mimas,ICYLON,Icy satellite longitudinal coverage,Mimas request,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-272T06:10:00,000T02:00:00,28-Sep-08,CIRS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,CIRS_086MI_ICYLON001_ISS,rider,,,,,, 2008-272T06:10:00,000T02:00:00,28-Sep-08,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-272T06:10:00,000T02:00:00,28-Sep-08,VIMS,SPASS Rider,Mimas,086W014PH,,spectral cubes,Phase study,,,,,, 2008-272T07:40:00,000T11:23:00,28-Sep-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-272T08:10:00,000T02:00:00,28-Sep-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-272T10:10:00,000T00:40:00,28-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-272T12:20:00,000T09:00:00,28-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-272T13:05:00,000T08:00:00,28-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS Deep Space Calibration,null,,,,,, 2008-272T19:03:00,003T04:42:00,28-Sep-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-272T19:03:00,003T15:06:00,28-Sep-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9473775 Rs exit= 4.0326784 Range altitude= -40432.390 km ... 40498.642,,,,,, 2008-272T19:03:00,000T02:17:00,28-Sep-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-272T19:03:00,000T02:17:00,28-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-272T19:03:00,000T02:17:00,28-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-272T19:03:03,000T00:00:01,28-Sep-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.4 d, inc = 74.5 deg, r = 20.264 Rs, phase = 23 deg",,,,,, 2008-272T21:20:00,000T09:10:00,28-Sep-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-272T21:20:00,003T02:25:00,28-Sep-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-272T21:20:00,001T12:10:00,28-Sep-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-272T21:20:00,001T16:30:00,28-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-272T22:00:00,000T06:10:00,28-Sep-08,ISS,Prime,Star,CHARGEXF,Instrument calibration,ISS CCD Charge Transfer Calibration,"Two targets: M48 for NAC, Pleiades for WAC. For each rotate around the Y axis 180 degrees in 20 degree steps and image in three filters at each point. Initial secondary will be Pos Z or Neg Z to sun.",,,,,, 2008-273T04:50:00,000T09:00:00,29-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-273T05:50:00,000T04:00:00,29-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08273_SP,rider,,,,,, 2008-273T06:30:00,000T02:00:00,29-Sep-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-273T08:30:00,003T04:49:00,29-Sep-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-273T14:30:00,000T02:00:00,29-Sep-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-273T16:30:00,000T11:40:00,29-Sep-08,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side",Do 15 unlit side at priority 2 (~every third orbit),,,,,, 2008-273T16:30:00,000T11:40:00,29-Sep-08,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_087RI_APOMOSU109_VIMS,rider,,,,,, 2008-274T04:50:00,000T09:00:00,30-Sep-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-274T05:50:00,000T08:00:00,30-Sep-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08274_SP,rider,,,,,, 2008-274T09:30:00,000T19:20:00,30-Sep-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-274T13:50:00,000T08:59:00,30-Sep-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-274T14:30:00,000T00:30:00,30-Sep-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-274T14:30:00,000T00:30:00,30-Sep-08,CIRS,SPASS Rider,Other,SATELLORB,Satellite orbit campaign,CIRS_087OT_SATELLORB003_SP,rider,,,,,, 2008-274T15:00:00,000T01:15:00,30-Sep-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 69.9, range 1.25 Mkm",,,,,, 2008-274T15:00:00,000T01:15:00,30-Sep-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-274T16:15:00,000T11:55:00,30-Sep-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-274T16:15:00,000T11:55:00,30-Sep-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_087RF_FMOVIE003_ISS,rider,,,,,, 2008-274T16:15:00,000T11:55:00,30-Sep-08,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,ISS rider,,,,,, 2008-274T22:49:00,003T01:19:00,30-Sep-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-275T04:50:00,000T18:55:00,1-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-275T04:50:00,000T09:00:00,1-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-275T05:50:00,000T08:00:00,1-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08275_SP,rider,,,,,, 2008-275T15:03:00,000T02:10:00,1-Oct-08,UVIS,Prime,Star,ALPCRU,,Saturn Occults Alp Cru,UVIS FUV Occultation slit boresite on star for 40 minutes,,,,,, 2008-275T15:03:00,000T02:10:00,1-Oct-08,ISS,SPASS Rider,Star,ALPCRU,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2008-275T17:13:00,000T07:59:00,1-Oct-08,CIRS,Prime,rings(general),VENCUNLP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-275T17:13:00,000T07:59:00,1-Oct-08,VIMS,SPASS Rider,rings(general),VENCUNLP,,,null,,,,,, 2008-275T23:45:00,000T04:34:00,1-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-275T23:45:00,000T04:34:00,1-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-275T23:45:00,000T10:50:00,1-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-275T23:45:00,000T04:34:00,1-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-276T01:12:00,000T02:27:00,2-Oct-08,ISS,Prime,RingF,FMOVIE,F ring movie,SHORT HI RES F RING MOVIE,Short hi res F ring stare on day of periapse. Designed to fit into gaps left by other obs. Point to ring radius/longitude and stare for ~2 hrs as material passes through field of view to get ~40 degs of co-rotating longitude,,,,,, 2008-276T01:12:00,000T02:00:00,2-Oct-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_087RF_FMOVIE001_ISS,rider,,,,,, 2008-276T04:19:00,000T00:51:00,2-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T04:19:00,000T01:12:00,2-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-276T04:19:00,000T01:00:00,2-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-276T04:19:00,000T09:00:00,2-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-276T05:04:00,000T08:00:00,2-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08276_SP,rider,,,,,, 2008-276T05:10:00,000T02:25:00,2-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T05:19:00,000T05:02:00,2-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-276T05:31:00,000T12:10:00,2-Oct-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-276T06:18:00,000T04:45:00,2-Oct-08,RPWS,SPASS Rider,Saturn,WHISTLER,RPWS lightning search,non RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-276T07:35:00,000T03:00:00,2-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T09:52:29,000T02:00:00,2-Oct-08,CDA,SPASS Rider,DustRAM direction,RPX0060,,CDA RPXing 2008-276T10:52:29 NTH,Nice to have - variation of angular distance to source (longitude),,,,,, 2008-276T10:09:00,000T00:21:00,2-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0306059 Rs exit= 3.9943903 Range altitude= 39566.277 km ... 20853.145,,,,,, 2008-276T10:21:00,000T01:00:00,2-Oct-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-276T10:30:00,000T00:43:00,2-Oct-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9928450 Rs exit= 3.9515159 Range altitude= 19914.865 km ... -19555.885,,,,,, 2008-276T10:35:00,000T00:45:00,2-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-276T10:35:00,000T00:45:00,2-Oct-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-276T10:35:00,000T00:45:00,2-Oct-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-276T11:13:00,000T00:21:00,2-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9511024 Rs exit= 3.9484792 Range altitude= -20494.195 km ... -39203.942,,,,,, 2008-276T11:20:00,000T02:39:00,2-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T11:20:00,000T11:50:00,2-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-276T11:20:00,000T11:50:00,2-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-276T11:27:42,000T00:00:01,2-Oct-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.945 Rs, lat = -8 deg, phase = 157 deg",,,,,, 2008-276T11:34:00,003T16:01:00,2-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9486307 Rs exit= 4.0318411 Range altitude= -40135.871 km ... 40022.287,,,,,, 2008-276T13:19:00,000T05:11:00,2-Oct-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-276T13:32:00,000T02:43:00,2-Oct-08,UVIS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,Saturn Aurora,"Part of CAPS campaign to observe the aurora while on active field lines. Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2008-276T13:44:00,000T02:31:00,2-Oct-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T13:59:00,000T02:16:00,2-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T16:15:00,000T03:16:00,2-Oct-08,CIRS,Prime,Tethys,FP1SECLX,,CIRS_087TE_FP1SECLX001_PRIME;,"FP3 N, FP1 X; 5.7-3.3; S hem; LT~12; stable, but rapid range change; one of the best. FP1 and FP3 only. Exit at 16:31:29; AD=3.3, phase=54, (-59, 3). Request WAC SI at 16:40 and 19:00.",,,,,, 2008-276T16:15:00,000T06:55:00,2-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-276T16:15:00,000T03:16:00,2-Oct-08,CIRS,SPASS Rider,Tethys,FP1SECLX,,CIRS_087TE_FP1SECLX_SI,Two WAC images for pointing verification of Tethys eclipse.,,,,,, 2008-276T16:15:00,000T03:16:00,2-Oct-08,UVIS,SPASS Rider,Tethys,ICYECL,,ICYECL: observe satellite in eclipse,,,,,,, 2008-276T16:15:00,000T03:16:00,2-Oct-08,VIMS,SPASS Rider,Tethys,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-276T17:41:00,000T05:29:00,2-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-276T18:30:00,000T02:00:00,2-Oct-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,,,,,,, 2008-276T19:31:00,000T05:49:00,2-Oct-08,UVIS,Prime,Saturn,SPOLECAM,Saturn south pole campaign,South Pole Campaign,Joint UVIS/VIMS/ISS/CIRS campaign to study the auroras Repeated slews for UVIS Occasional stares for VIMS/ISS,,,,,, 2008-276T19:31:00,000T05:49:00,2-Oct-08,CIRS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,CIRS_087SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2008-276T19:31:00,000T05:49:00,2-Oct-08,ISS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,Aurora,aurora: follow (NIGHT ISS)in the template in the note.,,,,,, 2008-276T19:31:00,000T05:49:00,2-Oct-08,VIMS,SPASS Rider,Saturn,SPOLECAM,Saturn south pole campaign,South Pole UVIS ridealong,Ridealong with UVIS on observations of the south pole of Saturn,,,,,, 2008-276T20:30:00,000T17:05:00,2-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-276T23:10:00,003T04:25:00,2-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-276T23:10:00,005T00:05:00,2-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-276T23:10:00,000T19:50:00,2-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-277T01:20:00,000T02:35:00,3-Oct-08,CIRS,Prime,rings(general),VTMPS60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-277T01:20:00,000T02:35:00,3-Oct-08,VIMS,SPASS Rider,rings(general),VTMPS60MP,,,null,,,,,, 2008-277T04:35:00,000T09:00:00,3-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-277T05:35:00,000T08:00:00,3-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08277_SP,rider,,,,,, 2008-277T13:35:00,001T17:30:00,3-Oct-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-277T14:15:00,000T08:52:00,3-Oct-08,VIMS,Prime,rings(general),RSCNCOCC,,Ring stellar occ - RS Cnc,"RS_Cnc occultation, outer C ring, R0=2.343, Rf=2.348, Rmin=1.371",,,,,, 2008-277T14:15:00,000T08:52:00,3-Oct-08,CIRS,SPASS Rider,rings(general),RSCNCOCC,,CIRS_087RI_RSCNCOCC203_VIMS,rider,,,,,, 2008-277T19:00:00,002T08:35:00,3-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-277T23:07:00,000T02:18:00,3-Oct-08,ISS,Prime,rings(general),RETARMRLP,,Medium res retargetables,Medium Res Retarg of small ring region satellites. Need 25 of 54.,,,,,, 2008-277T23:07:00,000T02:18:00,3-Oct-08,CIRS,SPASS Rider,rings(general),RETARMRLP,,CIRS_087RI_RETARMRLP002_ISS,rider,,,,,, 2008-278T00:08:00,002T03:27:00,4-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-278T01:25:00,000T00:30:00,4-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-278T01:25:00,000T00:30:00,4-Oct-08,CIRS,SPASS Rider,Other,SATELLORB,Satellite orbit campaign,CIRS_087OT_SATELLORB008_ISS,rider,,,,,, 2008-278T01:55:00,000T02:00:00,4-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-278T04:30:00,000T09:05:00,4-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev89 Rings Occultation experiment on DOY 291.",,,,,, 2008-278T04:35:00,000T09:00:00,4-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-278T05:35:00,000T08:00:00,4-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08278_SP,rider,,,,,, 2008-278T14:15:00,000T04:00:00,4-Oct-08,CIRS,Prime,rings(general),TMAPS10LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-278T14:15:00,000T04:00:00,4-Oct-08,VIMS,SPASS Rider,rings(general),TMAPS10LP,,,null,,,,,, 2008-278T18:15:00,000T02:57:00,4-Oct-08,VIMS,Prime,rings(general),RLEOOCC,R Leo occultation,Ring stellar occ - R Leo,Outer A ring; do at full spectral resolution!,,,,,, 2008-278T18:15:00,000T02:57:00,4-Oct-08,CIRS,SPASS Rider,rings(general),RLEOOCC,R Leo occultation,CIRS_087RI_RLEOOCC302_VIMS,rider,,,,,, 2008-278T21:12:00,000T02:00:00,4-Oct-08,ISS,Prime,Mimas,100W015PH,,Mimas lon/phase observation,"Turn UVIS_FUV to satellite; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-278T21:12:00,000T02:00:00,4-Oct-08,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-278T21:12:00,000T02:00:00,4-Oct-08,VIMS,SPASS Rider,Mimas,100W015PH,,spectral cubes,Phase study,,,,,, 2008-278T23:12:00,000T00:30:00,4-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-278T23:42:00,000T01:15:00,4-Oct-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 90.0, range 1.04 Mkm",,,,,, 2008-278T23:42:00,000T01:15:00,4-Oct-08,CIRS,SPASS Rider,Titan,MR2CLD,,CIRS_087TI_MR2CLD279_ISS,rider,,,,,, 2008-278T23:42:00,000T01:15:00,4-Oct-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-279T00:57:00,000T02:58:00,5-Oct-08,ISS,Prime,Rhea,126W001PH,,Rhea lon/phase angle observation,"Turn UVIS_FUV to Rhea; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-279T00:57:00,000T02:58:00,5-Oct-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-279T00:57:00,000T02:58:00,5-Oct-08,VIMS,SPASS Rider,Rhea,126W001PH,,spectral cubes,Phase study,,,,,, 2008-279T04:35:00,000T06:30:00,5-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-279T05:35:00,000T05:30:00,5-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_087IC_DSCAL08279_SP,rider,,,,,, 2008-279T07:05:00,000T04:00:00,5-Oct-08,INMS,SPASS Rider,Titan,TTNTORUS,Titan torus observation,Titan Torus region full rate ridealong,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-279T11:05:00,000T16:30:00,5-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-279T11:45:00,000T02:30:00,5-Oct-08,ISS,Prime,Rhea,RHEARPXLP,Rhea ring search,Image Rhea's equatorial plane at low phase,Image Rhea's equatorial plane at low phase,,,,,, 2008-279T11:45:00,000T02:30:00,5-Oct-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-279T11:45:00,000T02:30:00,5-Oct-08,VIMS,SPASS Rider,Rhea,RHEARPXLP,Rhea ring search,Rhea RPXLP,Do 4 at priority 1.,,,,,, 2008-279T12:00:00,000T02:16:32,5-Oct-08,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2008-279T14:15:00,000T09:20:00,5-Oct-08,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2008-279T14:15:00,000T09:20:00,5-Oct-08,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_087RI_EGPHASE106_VIMS,rider,,,,,, 2008-279T14:15:00,000T09:20:00,5-Oct-08,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2008-279T23:35:00,000T02:00:00,5-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-280T01:35:00,000T09:00:00,6-Oct-08,CIRS,Prime,rings(general),COMP,Sit and stare to derive composition,CIRS_087RI_COMP279_PRIME;,null,,,,,, 2008-280T01:35:00,000T09:00:00,6-Oct-08,CIRS,SPASS Rider,rings(general),COMP,Sit and stare to derive composition,CIRS_087RI_COMP279_SI,,,,,,, 2008-280T01:35:00,000T09:00:00,6-Oct-08,UVIS,SPASS Rider,rings(general),COMP279,,,,,,,,, 2008-280T03:35:00,003T06:24:28,6-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-280T03:35:00,003T14:50:00,6-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9486307 Rs exit= 4.0318411 Range altitude= -40135.871 km ... 40022.287,,,,,, 2008-280T03:35:00,000T17:30:00,6-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-280T03:35:00,001T14:25:00,6-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-280T03:35:00,002T03:25:00,6-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-280T03:35:03,000T00:00:01,6-Oct-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.3 d, inc = 74.5 deg, r = 20.212 Rs, phase = 23 deg",,,,,, 2008-280T12:05:00,000T09:00:00,6-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-280T13:05:00,000T08:00:00,6-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_088IC_DSCAL08280_SP,rider,,,,,, 2008-280T21:05:00,000T23:45:00,6-Oct-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-280T21:40:00,000T09:30:00,6-Oct-08,ISS,Prime,RingF,FRSTRCHAN,F ring streamer movie,F RING STREAMER/CHANNEL,"Movie of streamer-channel feature raised in F ring by Prometheus apoapse passage. Need as close to 1 Prom orbital period as possible. Sometimes can be day before or day after. Want 12. 6 of 49 as priority 1, 6 of 49 as priority 2.",,,,,, 2008-280T21:40:00,000T09:30:00,6-Oct-08,CIRS,SPASS Rider,RingF,FRSTRCHAN,F ring streamer movie,CIRS_088RF_FRSTRCHAN001_ISS,rider,,,,,, 2008-281T07:10:00,000T04:05:00,7-Oct-08,CIRS,Prime,rings(general),TMAPN20LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-281T07:10:00,000T04:05:00,7-Oct-08,CIRS,SPASS Rider,rings(general),TMAPN20LP,,CIRS_088RI_TMAPN20LP001_SI,,,,,,, 2008-281T07:10:00,000T04:05:00,7-Oct-08,UVIS,SPASS Rider,rings(general),TMAPN20LP,,,,,,,,, 2008-281T07:10:00,000T04:05:00,7-Oct-08,VIMS,SPASS Rider,rings(general),TMAPN20LP,,,null,,,,,, 2008-281T11:50:00,000T09:00:00,7-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-281T12:50:00,000T08:00:00,7-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_088IC_DSCAL08281_SP,rider,,,,,, 2008-281T18:00:00,001T14:00:00,7-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-281T20:50:00,001T00:00:00,7-Oct-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-281T21:30:00,000T00:30:00,7-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-281T22:00:00,000T01:15:00,7-Oct-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 58.7, range 1.78 Mkm",,,,,, 2008-281T22:00:00,000T01:15:00,7-Oct-08,CIRS,SPASS Rider,Titan,MR2CLD,,CIRS_088TI_MR2CLD281_ISS,rider,,,,,, 2008-281T22:00:00,000T01:15:00,7-Oct-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-281T23:15:00,000T06:45:00,7-Oct-08,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-282T06:00:00,000T05:15:00,8-Oct-08,CIRS,Prime,rings(general),TMAPN45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-282T06:00:00,000T05:15:00,8-Oct-08,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_088RI_TMAPN45LP001_SI,,,,,,, 2008-282T06:00:00,000T05:15:00,8-Oct-08,UVIS,SPASS Rider,rings(general),TMAPN45LP,,,,,,,,, 2008-282T06:00:00,000T05:15:00,8-Oct-08,VIMS,SPASS Rider,rings(general),TMAPN45LP,,,null,,,,,, 2008-282T06:00:00,000T14:50:00,8-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-282T07:00:00,002T04:50:00,8-Oct-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-282T11:45:00,000T09:05:00,8-Oct-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-282T11:50:00,000T09:00:00,8-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-282T12:50:00,000T08:00:00,8-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_088IC_DSCAL08282_SP,rider,,,,,, 2008-282T17:30:00,000T03:20:00,8-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev89 Rings Occultation experiment on DOY 291.",,,,,, 2008-282T20:50:00,000T10:16:43,8-Oct-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-282T20:50:00,000T11:10:00,8-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-282T21:35:00,000T01:15:00,8-Oct-08,ISS,Prime,Titan,TITAN,Titan observation,,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-282T21:35:00,000T01:15:00,8-Oct-08,CIRS,SPASS Rider,Titan,TITAN,Titan observation,CIRS_088TI_TITAN001_ISS,rider,,,,,, 2008-282T21:35:00,000T01:15:00,8-Oct-08,UVIS,SPASS Rider,Titan,TITAN,Titan observation,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-282T21:35:00,000T01:15:00,8-Oct-08,VIMS,SPASS Rider,Titan,TITAN,Titan observation,,null,,,,,, 2008-282T22:50:00,000T03:25:00,8-Oct-08,UVIS,Prime,Saturn,AURORAE,Saturn aurora / lightning search,Saturn Aurora,Auroral Observations led by UVIS Repeated scans across pole to build up auroral images with spectral information,,,,,, 2008-282T22:50:00,000T03:25:00,8-Oct-08,ISS,SPASS Rider,Saturn,AURORAE,Saturn aurora / lightning search,Auroral stare at ~7 Rs.,Auroral stare.,,,,,, 2008-282T22:50:00,000T03:25:00,8-Oct-08,VIMS,SPASS Rider,Saturn,AURORAE,Saturn aurora / lightning search,spectral cubes,Saturn,,,,,, 2008-283T02:15:00,000T02:45:00,9-Oct-08,ISS,Prime,Enceladus,PLMHINCL,,High inclination plume observation,High inclination plume observation.,,,,,, 2008-283T02:15:00,000T02:45:00,9-Oct-08,CIRS,SPASS Rider,Enceladus,PLMHINCL,,CIRS_088EN_PLMHINCL001_ISS,rider,,,,,, 2008-283T02:15:00,000T02:45:00,9-Oct-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-283T02:15:00,000T02:45:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,PLMHINC,,spectral cubes,enceladus,,,,,, 2008-283T05:00:00,000T01:30:00,9-Oct-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-283T05:00:00,000T01:30:00,9-Oct-08,CIRS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,CIRS_088EN_ICYATM001_UVIS,rider,,,,,, 2008-283T05:00:00,000T01:30:00,9-Oct-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-283T05:00:00,000T01:30:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,spectral cubes,enceladus,,,,,, 2008-283T05:00:00,000T13:28:40,9-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-283T07:06:43,000T11:00:57,9-Oct-08,INMS,Non-SPASS,Enceladus,ENCEL5,,Enceladus observation,Enceladus observation,,,,,, 2008-283T08:00:00,000T05:46:00,9-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-283T08:00:00,000T10:50:00,9-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-283T09:30:00,000T01:00:43,9-Oct-08,RADAR,SPASS Rider,Other,WARMUP4EN,RADAR warmup,Warmup with data before Enceladus,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2008-283T09:59:28,000T08:37:16,9-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-283T10:30:40,000T03:36:00,9-Oct-08,RADAR,Prime,Enceladus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Enceladus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2008-283T13:46:00,000T12:11:00,9-Oct-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-283T14:06:40,000T03:00:00,9-Oct-08,CIRS,Prime,Enceladus,ENCEL,Enceladus,CIRS_088EN_ENCEL001_PRIME;,null,,,,,, 2008-283T14:06:40,000T03:00:00,9-Oct-08,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_088EN ENCEL SI,Four WAC images: 1) WAC at 2008-283T14:21 (sunlight); 2) WAC at 2008-283T15:16 (sunlight); 3) WAC at 2008-283T16:11 (sunlight); 4) WAC at 2008-283T17:01 (sunlight).,,,,,, 2008-283T14:06:40,000T03:00:00,9-Oct-08,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2008-283T14:06:40,000T03:00:00,9-Oct-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-283T14:06:40,000T03:00:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,spectral cubes,enceladus,,,,,, 2008-283T17:06:40,000T01:00:00,9-Oct-08,UVIS,Prime,Enceladus,ICYLIMB,,ICYLIMB: Icy satellite high resolution limb scan,Slow scan onto limb of icy satellite to look for volatiles: Start the scan as many mrads off the illuminated limb as the observation duration will allow. Slew slowly to center of Enceladus using 9 - 10 microrad/sec turn rate.,,,,,, 2008-283T17:06:40,000T01:00:00,9-Oct-08,ISS,SPASS Rider,Enceladus,ICYLIMB,,Enceladus,Enceladus,,,,,, 2008-283T17:06:40,000T01:00:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,LIMBSCAN,Limb scan,spectral cubes,enceladus,,,,,, 2008-283T17:06:40,000T04:00:00,9-Oct-08,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetspheric plasma and determine whether it generates an internal magnetic field. Rate set to zero as overlaps an INTFLD request.,,,,,, 2008-283T18:06:40,000T02:00:00,9-Oct-08,CDA,SPASS Rider,DustRAM direction,ENCEL,Enceladus,CDA RPXing 2008-283T19:07:29 MMH SOST CCR,"Enceladus flyby 25 km, 17 km/s, vertical C/A at least +/- 10 min. plus turn time (SOST agreement, 12. Nov 2007)",,,,,, 2008-283T18:07:40,000T01:14:00,9-Oct-08,INMS,Prime,Enceladus,ENCEL5,,Enceladus observation,Prime Enceladus observation,,,,,, 2008-283T18:25:00,000T00:21:00,9-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0297893 Rs exit= 3.9939825 Range altitude= 39090.005 km ... 20377.104,,,,,, 2008-283T18:28:40,000T01:16:00,9-Oct-08,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2008-283T18:36:40,000T01:00:00,9-Oct-08,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 088EN Campaign,Part of 088EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magn,,,,,, 2008-283T18:46:00,000T00:42:00,9-Oct-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9924575 Rs exit= 3.9524241 Range altitude= 19438.766 km ... -19090.375,,,,,, 2008-283T18:50:00,000T00:45:00,9-Oct-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-283T19:21:40,000T00:28:00,9-Oct-08,ISS,Prime,Enceladus,ENCELCA,,Enceladus C/A Flyby Imaging,"3-panel NAC mosaic, 2min dwells, 1 WAC for context.",,,,,, 2008-283T19:21:40,000T00:28:00,9-Oct-08,CIRS,SPASS Rider,Enceladus,ENCELCA,,CIRS_088EN_ENCELCA001_ISS,rider,,,,,, 2008-283T19:21:40,000T00:28:00,9-Oct-08,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus' surface plus limb drifts,,,,,, 2008-283T19:21:40,000T00:28:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,ENCELA,,spectral cubes,enceladus,,,,,, 2008-283T19:21:40,000T11:45:00,9-Oct-08,INMS,Non-SPASS,Enceladus,ENCEL5,,Enceladus observation,Enceladus observation,,,,,, 2008-283T19:28:00,000T00:22:00,9-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9520048 Rs exit= 3.9494051 Range altitude= -20028.665 km ... -39671.029,,,,,, 2008-283T19:35:00,000T11:50:00,9-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-283T19:36:44,000T09:39:10,9-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-283T19:43:10,000T00:00:01,9-Oct-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.946 Rs, lat = -8 deg, phase = 157 deg",,,,,, 2008-283T19:44:40,000T13:52:00,9-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-283T19:49:40,000T00:46:00,9-Oct-08,CIRS,Prime,Enceladus,SECLNX,,CIRS_088EN_SECLNX001_PRIME;,"(E5) FP3 Polar thermal output integration; 11-3, high S lat.; begins C/A+00:46. SOST. N283T19:52:09, X283T22:23:05.",,,,,, 2008-283T19:49:40,000T04:17:00,9-Oct-08,CIRS,SPASS Rider,Enceladus,SECLNX,,CIRS_088EN SECLNX SI,Four WAC images: Times and exposures TBD.,,,,,, 2008-283T19:49:40,000T00:46:00,9-Oct-08,ISS,SPASS Rider,Enceladus,SECLNX,,Enceladus,SPT in eclipse to detect non-thermal emission,,,,,, 2008-283T19:49:40,000T00:46:00,9-Oct-08,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, Eclipse entr",Monitor eclipse entry,,,,,, 2008-283T19:49:40,000T00:46:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-283T19:50:00,003T15:51:00,9-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9495771 Rs exit= 4.0246841 Range altitude= -40602.636 km ... 40583.443,,,,,, 2008-283T20:35:40,000T00:22:00,9-Oct-08,CIRS,SPASS Rider,Enceladus,SECLNX,,CIRS_088EN_SECLNX001_AACS;,"(E5) FP3 Polar thermal output integration; 11-3, high S lat.; begins C/A+00:46. SOST. N283T19:52:09, X283T22:23:05.",,,,,, 2008-283T20:35:40,000T00:22:00,9-Oct-08,ISS,SPASS Rider,SpacecraftActivity,DFPWBIAS,,Enceladus,SPT in eclipse to detect non-thermal emission,,,,,, 2008-283T20:35:40,000T00:22:00,9-Oct-08,UVIS,SPASS Rider,Enceladus,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2008-283T20:35:40,000T00:22:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-283T20:57:40,000T03:09:00,9-Oct-08,CIRS,Prime,Enceladus,SECLNX,,CIRS_088EN_SECLNX002_PRIME;,"(E5) FP3 Polar thermal output integration; 11-3, high S lat.; begins C/A+00:46. SOST. N283T19:52:09, X283T22:23:05.",,,,,, 2008-283T20:57:40,000T03:09:00,9-Oct-08,ISS,SPASS Rider,Enceladus,SECLNX,,Enceladus,SPT in eclipse to detect non-thermal emission,,,,,, 2008-283T20:57:40,000T03:09:00,9-Oct-08,UVIS,SPASS Rider,Enceladus,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2008-283T20:57:40,000T03:09:00,9-Oct-08,VIMS,SPASS Rider,Enceladus,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-284T00:06:40,000T02:00:00,10-Oct-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-284T00:06:40,000T02:00:00,10-Oct-08,CIRS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,CIRS_088EN_ICYATM002_UVIS,rider,,,,,, 2008-284T00:06:40,000T02:00:00,10-Oct-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-284T00:06:40,000T02:00:00,10-Oct-08,VIMS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,spectral cubes,enceladus,,,,,, 2008-284T01:57:00,000T05:28:00,10-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-284T02:06:40,000T04:23:00,10-Oct-08,UVIS,Prime,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-284T02:06:40,000T04:23:00,10-Oct-08,CIRS,SPASS Rider,Tethys,SECLNX,,CIRS_088TE_SECLNX001_UVIS;,"FP1 N, FP1 X;2.4-2.1; S hem; very stale; LT~11. N284T03:01:11, X284T05:47:25.",,,,,, 2008-284T02:06:40,000T04:23:00,10-Oct-08,ISS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,Tethys observation,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-284T02:06:40,000T04:23:00,10-Oct-08,VIMS,SPASS Rider,Tethys,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-284T05:15:54,003T06:25:06,10-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-284T07:06:43,000T03:53:17,10-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-284T07:25:00,000T13:25:00,10-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-284T07:25:00,000T19:35:00,10-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-284T11:00:00,000T02:00:00,10-Oct-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-284T11:45:00,000T09:05:00,10-Oct-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-284T11:50:00,000T09:00:00,10-Oct-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-284T11:50:00,000T09:00:00,10-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-284T12:50:00,000T08:00:00,10-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_088IC_DSCAL08284_SP,rider,,,,,, 2008-284T13:00:00,000T07:50:00,10-Oct-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-284T14:00:00,000T02:16:32,10-Oct-08,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2008-284T17:00:00,000T03:50:00,10-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev89 Rings Occultation experiment on DOY 291.",,,,,, 2008-284T20:50:00,002T06:01:00,10-Oct-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment boundary survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-284T20:50:00,005T19:05:00,10-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-284T20:50:00,000T11:35:00,10-Oct-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-284T21:40:00,000T04:00:00,10-Oct-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-284T21:40:00,000T04:00:00,10-Oct-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-285T00:00:00,000T09:10:00,11-Oct-08,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,Standard calibration/gain,,,,,, 2008-285T01:40:00,000T04:00:00,11-Oct-08,CIRS,Prime,rings(general),TMAPS30LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-285T01:40:00,000T04:00:00,11-Oct-08,CIRS,SPASS Rider,rings(general),TMAPS30LP,,CIRS_088RI_TMAPS30LP001_SI,,,,,,, 2008-285T01:40:00,000T04:00:00,11-Oct-08,UVIS,SPASS Rider,rings(general),TMAPS30LP,,,,,,,,, 2008-285T01:40:00,000T04:00:00,11-Oct-08,VIMS,SPASS Rider,rings(general),TMAPS30LP,,,null,,,,,, 2008-285T03:00:00,002T08:41:00,11-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-285T05:40:00,000T05:20:00,11-Oct-08,ISS,Prime,rings(general),LPMRLFOCD,,Outer Cassini Division ansa movie,Outer Cassini Division ansa movie. This is a backup to 2 other priority 1 movies.,,,,,, 2008-285T05:40:00,000T05:20:00,11-Oct-08,CIRS,SPASS Rider,rings(general),LPMRLFOCD,,CIRS_088RI_LPMRLFOCD001_ISS,rider,,,,,, 2008-285T05:40:00,000T05:20:00,11-Oct-08,VIMS,SPASS Rider,rings(general),LPMRLFOCD,,,null,,,,,, 2008-285T08:25:00,002T03:16:00,11-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-285T11:35:00,000T09:00:00,11-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rings Occultation experiment on DOY 291 (Rev89).",,,,,, 2008-285T11:35:00,000T09:00:00,11-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-285T12:35:00,000T08:00:00,11-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_088IC_DSCAL08285_SP,rider,,,,,, 2008-285T21:10:00,000T01:15:00,11-Oct-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 10.4, range 2.22 Mkm",,,,,, 2008-285T21:10:00,000T01:15:00,11-Oct-08,CIRS,SPASS Rider,Titan,MR3CLD,,CIRS_088TI_MR3CLD285_ISS,rider,,,,,, 2008-285T21:10:00,000T01:15:00,11-Oct-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-285T22:25:00,000T12:15:00,11-Oct-08,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2008-285T22:25:00,000T12:15:00,11-Oct-08,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_088RI_SPKMVLFLP001_ISS,rider,,,,,, 2008-285T22:25:00,000T12:15:00,11-Oct-08,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie - litside,null,,,,,, 2008-286T10:40:00,000T00:30:00,12-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-286T11:10:00,000T02:00:00,12-Oct-08,ISS,Prime,Tethys,093W008PH,,Tethys lon/phase angle observation,"Turn UVIS_FUV to Tethys; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-286T11:10:00,000T02:00:00,12-Oct-08,CIRS,SPASS Rider,Tethys,093W008PH,,CIRS_088TE_093W008PH001_ISS,rider,,,,,, 2008-286T11:10:00,000T02:00:00,12-Oct-08,VIMS,SPASS Rider,Tethys,093W008PH,,spectral cubes,Phase study,,,,,, 2008-286T13:10:00,000T01:15:00,12-Oct-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-286T13:10:00,000T01:15:00,12-Oct-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_088RI_FMONITOR003_ISS,rider,,,,,, 2008-286T14:25:00,000T01:00:00,12-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-286T14:25:00,000T01:00:00,12-Oct-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_088RI_SATELLORB012_ISS,rider,,,,,, 2008-286T15:25:00,000T01:50:00,12-Oct-08,ISS,Prime,Dione,081W005PH,,Dione lon/phase angle observation,"Turn UVIS_FUV to Dione; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-286T15:25:00,000T01:50:00,12-Oct-08,CIRS,SPASS Rider,Dione,081W005PH,,CIRS_088DI_081W005PH001_ISS,rider,,,,,, 2008-286T15:25:00,000T01:50:00,12-Oct-08,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-286T15:25:00,000T01:50:00,12-Oct-08,VIMS,SPASS Rider,Dione,081W005PH,,spectral cubes,Phase study,,,,,, 2008-286T17:51:00,000T09:00:00,12-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-286T18:51:00,000T08:00:00,12-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_088IC_DSCAL08286_SP,rider,,,,,, 2008-287T02:51:00,000T03:09:00,13-Oct-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-287T03:30:00,000T02:00:00,13-Oct-08,ISS,Prime,Rhea,044W009PH,,Rhea lon/phase angle observation,"Turn UVIS_FUV to Rhea; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-287T03:30:00,000T02:00:00,13-Oct-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-287T03:30:00,000T02:00:00,13-Oct-08,VIMS,SPASS Rider,Rhea,044W009PH,,spectral cubes,Phase study,,,,,, 2008-287T05:30:00,000T02:00:00,13-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-287T06:00:00,000T02:00:00,13-Oct-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-287T07:30:00,000T01:15:00,13-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-287T07:30:00,000T01:15:00,13-Oct-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_088RI_SATELLORB013_ISS,rider,,,,,, 2008-287T08:00:00,000T03:41:00,13-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-287T08:45:00,000T02:15:00,13-Oct-08,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Ymir spectrophotometry,Observation of outer moon Ymir,,,,,, 2008-287T08:45:00,000T02:15:00,13-Oct-08,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,,,,,,,, 2008-287T11:36:00,000T09:00:00,13-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-287T11:41:00,003T04:14:00,13-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-287T11:41:00,003T14:38:00,13-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9495771 Rs exit= 4.0246841 Range altitude= -40602.636 km ... 40583.443,,,,,, 2008-287T11:41:00,000T08:55:00,13-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-287T11:41:00,001T14:19:00,13-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-287T11:41:00,002T03:15:00,13-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-287T11:41:31,000T00:00:01,13-Oct-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.3 d, inc = 74.5 deg, r = 20.184 Rs, phase = 23 deg",,,,,, 2008-287T12:36:00,000T08:00:00,13-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08287_SP,rider,,,,,, 2008-287T20:36:00,001T03:24:00,13-Oct-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-287T21:10:00,000T00:30:00,13-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-287T21:40:00,000T02:00:00,13-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-287T23:40:00,000T09:55:00,13-Oct-08,CIRS,Prime,rings(general),TMAPN20LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-287T23:40:00,000T09:55:00,13-Oct-08,CIRS,SPASS Rider,rings(general),TMAPN20LP,,CIRS_089RI_TMAPN20LP001_SI,,,,,,, 2008-287T23:40:00,000T09:55:00,13-Oct-08,UVIS,SPASS Rider,rings(general),TMAPN20LP,,,,,,,,, 2008-287T23:40:00,000T09:55:00,13-Oct-08,VIMS,SPASS Rider,rings(general),TMAPN20LP,,,null,,,,,, 2008-288T09:35:00,000T00:31:00,14-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-288T11:36:00,000T09:00:00,14-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-288T12:36:00,000T08:00:00,14-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08288_SP,rider,,,,,, 2008-288T21:10:00,000T01:15:00,14-Oct-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 38.5, range 1.75 Mkm",,,,,, 2008-288T21:10:00,000T01:15:00,14-Oct-08,CIRS,SPASS Rider,Titan,MR2CLD,,CIRS_089TI_MR2CLD288_ISS,rider,,,,,, 2008-288T21:10:00,000T01:15:00,14-Oct-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-288T22:25:00,000T12:25:00,14-Oct-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-288T22:25:00,000T12:25:00,14-Oct-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_089RF_FMOVIE003_ISS,rider,,,,,, 2008-288T22:25:00,000T12:25:00,14-Oct-08,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2008-289T00:00:00,001T20:00:00,15-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-289T02:00:00,001T13:55:00,15-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-289T11:21:00,000T09:00:00,15-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-289T11:36:00,000T08:45:00,15-Oct-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-289T12:21:00,000T08:00:00,15-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08289_SP,rider,,,,,, 2008-289T14:56:00,003T05:25:00,15-Oct-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-289T20:55:00,000T05:50:00,15-Oct-08,CIRS,Prime,rings(general),VTMPN60LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-289T20:55:00,000T05:50:00,15-Oct-08,CIRS,SPASS Rider,rings(general),VTMPN60LP,,CIRS_089RI_VTMPN60LP001_SI,,,,,,, 2008-289T20:55:00,000T05:50:00,15-Oct-08,UVIS,SPASS Rider,rings(general),VTMPN60LP,,,,,,,,, 2008-289T20:55:00,000T05:50:00,15-Oct-08,VIMS,SPASS Rider,rings(general),VTMPN60LP,,,null,,,,,, 2008-290T02:45:00,000T04:40:00,16-Oct-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. Priority 1.",,,,,, 2008-290T02:45:00,000T04:40:00,16-Oct-08,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_089RI_GAMCRUOCC006_VIMS,rider,,,,,, 2008-290T02:45:00,000T04:40:00,16-Oct-08,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,,,,,,,, 2008-290T07:25:00,000T00:55:00,16-Oct-08,ISS,Prime,Other,RETARG,Retargetable observation,,ISS retargetable for yet-undiscovered moons or ring features,,,,,, 2008-290T08:20:00,000T04:55:00,16-Oct-08,UVIS,Prime,Star,URBETCEN,Stellar occultation,URSTAR,,,,,,, 2008-290T08:20:00,000T04:55:00,16-Oct-08,CIRS,SPASS Rider,rings(general),URBETCEN,Stellar occultation,CIRS_089RI_URBETCEN001_UVIS,rider,,,,,, 2008-290T08:20:00,000T04:55:00,16-Oct-08,UVIS,SPASS Rider,Star,URBETCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2008-290t09:06:30.0 2008-290t09:18:46.0 2008-290t09:57:10.0,,,,,, 2008-290T13:15:00,000T03:00:00,16-Oct-08,VIMS,Prime,rings(general),SHADSCANU,,Ring SHADSCAN unlit side,Do 2 at priority 1,,,,,, 2008-290T13:15:00,000T03:00:00,16-Oct-08,CIRS,SPASS Rider,rings(general),SHADSCANU,,CIRS_089RI_SHADSCANU111_VIMS,rider,,,,,, 2008-290T15:55:00,000T04:30:00,16-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-290T15:55:00,000T05:44:00,16-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-290T15:55:00,000T10:50:00,16-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-290T15:55:00,000T10:36:00,16-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-290T16:15:00,000T06:30:00,16-Oct-08,CIRS,Prime,rings(general),TDIFN45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-290T16:15:00,000T06:30:00,16-Oct-08,CIRS,SPASS Rider,rings(general),TDIFN45HP,,CIRS_089RI_TDIFN45HP001_SI,,,,,,, 2008-290T16:15:00,000T06:30:00,16-Oct-08,UVIS,SPASS Rider,rings(general),TDIFN45HP,,,,,,,,, 2008-290T20:00:00,000T02:00:00,16-Oct-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,,,,,,, 2008-290T20:25:00,000T02:55:00,16-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-290T21:39:00,000T12:13:00,16-Oct-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-290T22:00:00,000T14:10:00,16-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-290T23:20:00,000T03:25:00,16-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-290T23:25:00,000T03:00:00,16-Oct-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-291T00:00:00,000T02:25:00,17-Oct-08,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 089RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2008-291T02:02:29,000T02:00:00,17-Oct-08,CDA,SPASS Rider,DustRAM direction,RPX0080,,CDA RPXing 2008-291T03:02:29 NTH,Nice to have - variation of angular distance to source (longitude),,,,,, 2008-291T02:19:00,000T00:06:00,17-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0226213 Rs exit= 3.9866113 Range altitude= 39650.380 km ... 20920.367,,,,,, 2008-291T02:25:00,000T00:45:00,17-Oct-08,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ring Occultation 089,"Early XM series of RSS ring occultations spanning a chord of the ring system. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 20 minute free-space baseline and calibration period, followed by the occultation and a subsequent 15 minute free-space baseline and calibration period.",,,,,, 2008-291T02:25:00,000T00:45:00,17-Oct-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9850771 Rs exit= 3.9443173 Range altitude= 19981.102 km ... -19531.865,,,,,, 2008-291T02:31:00,000T01:00:00,17-Oct-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-291T02:45:00,000T00:45:00,17-Oct-08,CAPS,SPASS Rider,Saturn,IMVP3,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2008-291T02:45:00,000T00:45:00,17-Oct-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-291T03:10:00,000T00:34:00,17-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9439197 Rs exit= 3.9416369 Range altitude= -20471.182 km ... -39200.768,,,,,, 2008-291T03:10:00,000T09:00:00,17-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-291T03:30:00,000T03:05:00,17-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-291T03:30:00,000T11:50:00,17-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-291T03:31:00,000T07:54:00,17-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-291T03:37:42,000T00:00:01,17-Oct-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.939 Rs, lat = -8 deg, phase = 156 deg",,,,,, 2008-291T03:44:00,001T16:37:00,17-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S45,Range enter= 3.9418065 Rs exit= 4.0341951 Range altitude= -40133.671 km ... 40409.674,,,,,, 2008-291T04:10:00,000T07:00:00,17-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08291_SP,rider,,,,,, 2008-291T06:35:00,000T02:20:00,17-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-291T08:55:00,000T06:25:00,17-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-291T09:52:00,000T05:28:00,17-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-291T11:25:00,000T05:00:00,17-Oct-08,RPWS,SPASS Rider,Saturn,RCSWHIST,RPWS lightning search (RCS),non RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-291T12:10:00,000T05:15:00,17-Oct-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-291T12:10:00,000T05:15:00,17-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-291T15:20:00,001T05:01:00,17-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-291T15:20:00,001T05:01:00,17-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG_MAPS_SURVEY,Continuous low-rate magnetospheric survey,,,,,, 2008-291T15:20:00,000T20:00:00,17-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-291T17:25:00,001T02:56:00,17-Oct-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-291T18:00:00,000T07:00:00,17-Oct-08,CIRS,Prime,rings(general),SUBMS45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-291T18:00:00,000T07:00:00,17-Oct-08,CIRS,SPASS Rider,rings(general),SUBMS45LP,,CIRS_089RI_SUBMS45LP001_SI,,,,,,, 2008-291T18:00:00,000T07:00:00,17-Oct-08,UVIS,SPASS Rider,rings(general),SUBMS45LP,,,,,,,,, 2008-291T18:00:00,000T07:00:00,17-Oct-08,VIMS,SPASS Rider,rings(general),SUBMS45LP,,,null,,,,,, 2008-292T01:00:00,000T00:30:00,18-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-292T01:30:00,000T08:36:00,18-Oct-08,CIRS,Prime,rings(general),VCASLSLP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-292T01:30:00,000T08:36:00,18-Oct-08,CIRS,SPASS Rider,rings(general),VCASLSLP,,CIRS_089RI_VCASLSLP001_SI,,,,,,, 2008-292T01:30:00,000T08:36:00,18-Oct-08,UVIS,SPASS Rider,rings(general),VCASLSLP,,,,,,,,, 2008-292T01:30:00,000T08:36:00,18-Oct-08,VIMS,SPASS Rider,rings(general),VCASLSLP,,,null,,,,,, 2008-292T11:20:00,000T09:01:00,18-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-292T11:21:00,000T09:00:00,18-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-292T11:36:00,000T08:45:00,18-Oct-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-292T12:21:00,000T08:00:00,18-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08292_SP,rider,,,,,, 2008-292T20:21:00,001T22:47:00,18-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-292T20:21:00,001T22:46:00,18-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S S45,Range enter= 3.9418065 Rs exit= 4.0341951 Range altitude= -40133.671 km ... 40409.674,,,,,, 2008-292T20:21:00,000T00:43:00,18-Oct-08,INMS,Non-SPASS,Saturn,SURVEYSEQ,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-292T20:21:00,003T17:25:00,18-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-292T20:21:00,001T22:47:00,18-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-292T20:21:00,001T22:46:00,18-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-292T20:26:00,000T00:02:00,18-Oct-08,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S45 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2008-292T21:04:00,000T00:05:00,18-Oct-08,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-292T21:09:00,000T00:33:00,18-Oct-08,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-292T21:20:00,000T09:41:00,18-Oct-08,VIMS,Prime,rings(general),APOMOSL,,"Apoapse mosaic, lit side",Do 9 lit side at priority 2 (~every third orbit),,,,,, 2008-292T21:20:00,000T09:41:00,18-Oct-08,CIRS,SPASS Rider,rings(general),APOMOSL,,CIRS_089RI_APOMOSL107_VIMS,rider,,,,,, 2008-292T21:20:00,000T09:41:00,18-Oct-08,ISS,SPASS Rider,rings(general),APOMOSL,,Apoapse mosaic,Riding along on apoapse mosaic to search for spokes,,,,,, 2008-292T21:20:00,000T09:41:00,18-Oct-08,UVIS,SPASS Rider,rings(general),APOMOSL,,URSTAR,,,,,,, 2008-292T21:42:00,000T00:22:59,18-Oct-08,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-292T22:04:59,001T12:00:01,18-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-293T07:01:00,000T03:25:00,19-Oct-08,CIRS,Prime,rings(general),CWLEOOCC,CW Leo occultation,CIRS_089RI_CWLEOOCC293_PRIME;,null,,,,,, 2008-293T07:01:00,000T03:25:00,19-Oct-08,CIRS,SPASS Rider,rings(general),CWLEOOCC,CW Leo occultation,CIRS_089RI_CWLEOOCC293_SI,,,,,,, 2008-293T07:01:00,000T03:25:00,19-Oct-08,UVIS,SPASS Rider,Star,CWLEOOCC,CW Leo occultation,URSTAR,,,,,,, 2008-293T07:01:00,000T03:25:00,19-Oct-08,VIMS,SPASS Rider,rings(general),CWLEOOCC,CW Leo occultation,CW Leo occ.,"CW Leo Ring occultation. tau_IR=80 msec, IR_only. Stellar_occ mode. no spectral summing. CIRS rider.",,,,,, 2008-293T10:26:00,000T00:40:00,19-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_089RI_DEEPSPACE293_SP,rider,,,,,, 2008-293T11:06:00,000T09:00:00,19-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-293T12:06:00,000T08:00:00,19-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08293_SP,rider,,,,,, 2008-293T20:46:00,000T01:54:00,19-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-293T20:46:00,000T01:54:00,19-Oct-08,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_089RI_SURVEYPTG004_CAPS,rider,,,,,, 2008-293T22:40:00,000T02:00:00,19-Oct-08,ISS,Prime,Mimas,100W014PH,,Mimas lon/phase angle observation,"Turn UVIS_FUV to Mimas; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-293T22:40:00,000T02:00:00,19-Oct-08,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-293T22:40:00,000T02:00:00,19-Oct-08,VIMS,SPASS Rider,Mimas,100W014PH,,spectral cubes,Phase study,,,,,, 2008-294T00:40:00,000T02:00:00,20-Oct-08,ISS,Prime,Tethys,091W009PH,,Tethys lon/phase angle observation,"Turn UVIS_FUV to Tethys; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-294T00:40:00,000T02:00:00,20-Oct-08,CIRS,SPASS Rider,Tethys,091W009PH,,CIRS_089TE_091W009PH001_ISS,"Tethys rider; duration 02:00. AD=0.95, Phase=9, (-1, ~95). FP1 and FP3, 15.5cm-1, centers, shutter closed 00:30 to 00:45; THEN ALL FOCAL PLANES OFF, 401 RTI FOR 00:45 TO 01:45; then FP1 and FP3, 15.5cm-1, centers once again.",,,,,, 2008-294T00:40:00,000T02:00:00,20-Oct-08,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-294T00:40:00,000T02:00:00,20-Oct-08,VIMS,SPASS Rider,Tethys,091W009PH,,spectral cubes,Phase study,,,,,, 2008-294T02:40:00,000T03:00:00,20-Oct-08,ISS,Prime,rings(general),GRINGARC,,G-ring arc observation,"G-ring arc observation, need 2 of 15 opportunites",,,,,, 2008-294T02:40:00,000T03:00:00,20-Oct-08,CIRS,SPASS Rider,rings(general),GRINGARC,,CIRS_089RI_GRINGARC001_ISS,rider,,,,,, 2008-294T02:40:00,000T03:00:00,20-Oct-08,VIMS,SPASS Rider,rings(general),GRINGARC,,G Ring arc observation,null,,,,,, 2008-294T05:40:00,000T00:58:00,20-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 08","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-294T05:40:00,000T00:58:00,20-Oct-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_089RI_SATELLORB012_ISS,rider,,,,,, 2008-294T06:38:00,000T00:42:00,20-Oct-08,ISS,Prime,Mimas,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Mimas across Prometheus","Images of mutual event, transit of Mimas across Prometheus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2008-294T07:20:00,000T03:06:00,20-Oct-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-294T10:05:00,000T02:00:00,20-Oct-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-294T10:26:00,000T04:49:00,20-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-294T10:26:00,000T04:49:00,20-Oct-08,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_090RI_SURVEYPTG001_CAPS,rider,,,,,, 2008-294T12:05:00,000T07:03:00,20-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-294T15:15:00,000T01:15:00,20-Oct-08,ISS,Prime,Titan,MR1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86.9 range 1 Mkm",,,,,, 2008-294T15:15:00,000T01:15:00,20-Oct-08,CIRS,SPASS Rider,Titan,MR1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-294T15:15:00,000T01:15:00,20-Oct-08,UVIS,SPASS Rider,Titan,MR1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-294T16:30:00,000T00:30:00,20-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-294T17:36:00,000T09:00:00,20-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-294T18:36:00,000T08:00:00,20-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_089IC_DSCAL08294_SP,rider,,,,,, 2008-294T19:07:00,003T14:15:00,20-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9418065 Rs exit= 4.0341951 Range altitude= -40133.671 km ... 40409.674,,,,,, 2008-294T19:07:00,002T02:44:00,20-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-294T19:07:00,000T00:59:00,20-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-294T19:07:46,000T00:00:01,20-Oct-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.3 d, inc = 74.5 deg, r = 20.103 Rs, phase = 24 deg",,,,,, 2008-294T19:08:00,001T17:28:00,20-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-294T19:08:00,002T21:22:00,20-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-294T19:08:00,001T13:52:00,20-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-295T03:10:00,000T07:20:00,21-Oct-08,ISS,Prime,rings(general),RADMRLPDF,,Color Radial Scan,"High res radial scans. Need 1, want 2 out of 7",,,,,, 2008-295T03:10:00,000T07:20:00,21-Oct-08,CIRS,SPASS Rider,rings(general),RADMRLPDF,,CIRS_090RI_RADMRLPDF001_ISS,rider,,,,,, 2008-295T03:10:00,000T07:20:00,21-Oct-08,VIMS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,"radial scan, low phase, unlit side","Cube Size (X,Z) = 64*12 hires, tau_IR = 160 & 640 msec?, low phase angle. Rider on ISS_090RI_RADMRLPDF001_PRIME.",,,,,, 2008-295T10:30:00,000T00:36:00,21-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE295_SP,rider,,,,,, 2008-295T11:06:00,000T09:00:00,21-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-295T12:06:00,000T08:00:00,21-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_090IC_DSCAL08295_SP,rider,,,,,, 2008-295T20:46:00,000T00:30:00,21-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-295T20:46:00,000T00:30:00,21-Oct-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_090RI_SATELLORB003_ISS,rider,,,,,, 2008-295T21:16:00,000T01:50:00,21-Oct-08,UVIS,Prime,Dione,ICYSTARE,,ICYSTARE: long satellite stare,,,,,,, 2008-295T23:06:00,000T01:00:00,21-Oct-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-295T23:06:00,000T01:00:00,21-Oct-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_090RI_FMONITOR002_ISS,rider,,,,,, 2008-296T00:06:00,000T02:00:00,22-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-296T00:06:00,000T02:00:00,22-Oct-08,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_090RI_SURVEYPTG002_CAPS,rider,,,,,, 2008-296T02:06:00,000T01:29:00,22-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE296_NAV,rider,,,,,, 2008-296T03:31:00,000T09:05:00,22-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev91 Enceladus and Saturn gravity observations on DOY 305-306.",,,,,, 2008-296T03:36:00,000T09:00:00,22-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-296T04:36:00,000T08:00:00,22-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_090IC_DSCAL08296_SP,rider,,,,,, 2008-296T09:00:00,001T13:55:00,22-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-296T12:36:00,001T07:15:00,22-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-296T13:16:00,000T00:30:00,22-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-296T13:16:00,000T00:30:00,22-Oct-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_090RI_SATELLORB007_ISS,rider,,,,,, 2008-296T13:46:00,000T06:45:00,22-Oct-08,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-296T20:31:00,000T09:30:00,22-Oct-08,CIRS,Prime,rings(general),VTMPN60LP,,CIRS_090RI_VTMPN60LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-296T20:31:00,000T09:30:00,22-Oct-08,CIRS,SPASS Rider,rings(general),VTMPN60LP,,CIRS_090RI_VTMPN60LP001_SI,,,,,,, 2008-296T20:31:00,001T02:24:00,22-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-296T21:51:00,003T01:37:00,22-Oct-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-297T06:01:00,000T04:10:00,23-Oct-08,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2008-297T10:11:00,000T00:40:00,23-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE297_SP,rider,,,,,, 2008-297T10:46:00,000T09:05:00,23-Oct-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-297T10:46:00,000T09:05:00,23-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T46 Titan Bistatic and Occultation on DOY 308.",,,,,, 2008-297T10:51:00,000T09:00:00,23-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-297T11:51:00,000T08:00:00,23-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_090IC_DSCAL08297_SP,rider,,,,,, 2008-297T16:30:00,000T02:00:00,23-Oct-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-297T18:30:00,003T22:15:00,23-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-297T19:51:00,000T03:04:00,23-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-297T20:31:00,000T04:23:00,23-Oct-08,ISS,Prime,RingF,FRINGHRDF,,High Resolution F Ring Scan,Complete high resolution (0-10Rs) longitudinal scan of the F ring. Dark face. Need at least 3 during XM. 2 of 27 as priority 1 and 1 as priority 2.,,,,,, 2008-297T20:31:00,000T04:23:00,23-Oct-08,VIMS,SPASS Rider,RingF,FRINGHRDF,,F movie,"64*12, 640 msec",,,,,, 2008-297T22:55:00,000T10:55:00,23-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-297T22:55:00,000T05:48:00,23-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-297T22:55:00,000T10:55:00,23-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-297T22:55:00,000T10:39:00,23-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGNIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-298T00:54:00,000T06:19:00,24-Oct-08,UVIS,Prime,Star,URALPARA,Alpha Ara occultation,URSTAR,,,,,,, 2008-298T00:54:00,000T06:19:00,24-Oct-08,CIRS,SPASS Rider,rings(general),URALPARA,Alpha Ara occultation,CIRS_090RI_URALPARA_UVIS,rider,,,,,, 2008-298T00:54:00,000T06:19:00,24-Oct-08,UVIS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Support Imaging,NAC support images at the following times: 2008-298t01:41:30:0 2008-298t01:51:10:0 2008-298t02:23:46.0 2008-298t06:29:50.0 2008-298t06:20:10.0 2008-298t05:46:35.3,,,,,, 2008-298T04:43:00,000T12:11:00,24-Oct-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-298T07:13:00,000T01:44:00,24-Oct-08,ISS,Prime,Mimas,GEOLOG,Geologic study,Mimas geology,Mimas geology,,,,,, 2008-298T07:13:00,000T01:44:00,24-Oct-08,CIRS,SPASS Rider,Mimas,GEOLOG,Geologic study,CIRS_090MI_GEOLOG001_ISS,rider,,,,,, 2008-298T07:13:00,000T01:44:00,24-Oct-08,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-298T07:13:00,000T01:44:00,24-Oct-08,VIMS,SPASS Rider,Mimas,GEOLOG,Geologic study,mapping cubes,Lat-Long Vgr class,,,,,, 2008-298T08:50:00,000T00:30:00,24-Oct-08,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2008-298T08:57:00,000T01:37:00,24-Oct-08,VIMS,Prime,rings(general),SOLOCCS,,Ring solar occ,"2 at priority 1, and 2 at priority 2.",,,,,, 2008-298T08:57:00,000T01:37:00,24-Oct-08,UVIS,SPASS Rider,rings(general),SOLOCCS,,UV Ring solar occultation,,,,,,, 2008-298T09:05:29,000T02:00:00,24-Oct-08,CDA,SPASS Rider,DustRAM direction,RPX0090,,CDA RPXing 2008-298T10:05:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-298T09:22:00,000T00:21:00,24-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.0321523 Rs exit= 3.9965068 Range altitude= 39478.431 km ... 20785.641,,,,,, 2008-298T09:34:00,000T01:00:00,24-Oct-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-298T09:43:00,000T00:43:00,24-Oct-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9949889 Rs exit= 3.9547371 Range altitude= 19848.272 km ... -19583.613,,,,,, 2008-298T09:50:00,000T00:40:00,24-Oct-08,CAPS,SPASS Rider,Saturn,IMVP3,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2008-298T09:50:00,000T00:40:00,24-Oct-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-298T09:50:00,000T00:40:00,24-Oct-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-298T10:26:00,000T00:21:00,24-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9543472 Rs exit= 3.9521724 Range altitude= -20520.993 km ... -39212.235,,,,,, 2008-298T10:30:00,000T11:55:00,24-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-298T10:30:00,000T11:55:00,24-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-298T10:34:00,000T05:00:00,24-Oct-08,ISS,Prime,rings(general),AZSCANLIT,,AZSCAN lit,AZSCAN lit columbo ringlet,,,,,, 2008-298T10:34:00,000T11:51:00,24-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-298T10:40:04,000T00:00:01,24-Oct-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.948 Rs, lat = -8 deg, phase = 156 deg",,,,,, 2008-298T10:47:00,003T15:28:00,24-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9523451 Rs exit= 4.0335230 Range altitude= -40143.246 km ... 40058.481,,,,,, 2008-298T16:54:00,000T05:31:00,24-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-298T19:04:00,000T08:00:00,24-Oct-08,CIRS,Prime,rings(general),VTMPS60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-298T19:04:00,000T08:00:00,24-Oct-08,UVIS,SPASS Rider,rings(general),TMPS60MP,,,,,,,,, 2008-298T22:25:00,003T03:50:00,24-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-298T22:25:00,006T07:40:00,24-Oct-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-298T22:25:00,000T19:35:00,24-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-299T03:04:00,000T07:08:00,25-Oct-08,CIRS,Prime,rings(general),TMAPS45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-299T03:04:00,000T07:08:00,25-Oct-08,UVIS,SPASS Rider,rings(general),TMAPS45LP,,,,,,,,, 2008-299T03:04:00,000T07:08:00,25-Oct-08,VIMS,SPASS Rider,rings(general),TMAPS45LP,,,null,,,,,, 2008-299T10:47:00,000T09:05:00,25-Oct-08,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2008-299T10:52:00,000T09:00:00,25-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T46 Rev91 Titan Bistaitc and Occultation experiments 308.",,,,,, 2008-299T10:52:00,000T09:00:00,25-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-299T16:01:00,000T03:51:00,25-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T46 Rev91 Titan Bistatic and Occultation on DOY 308.",,,,,, 2008-299T18:00:00,002T08:15:00,25-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-299T19:52:00,000T00:40:00,25-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE299_SP,rider,,,,,, 2008-299T20:32:00,000T05:35:00,25-Oct-08,ISS,Prime,rings(general),LPMRLFMAX,,Maxwell ansa movie,Maxwell ansa movie,,,,,, 2008-299T20:32:00,000T05:35:00,25-Oct-08,CIRS,SPASS Rider,rings(general),LPMRLFMAX,,CIRS_090RI_LPMRLFMAX001_ISS,rider,,,,,, 2008-299T20:32:00,000T05:35:00,25-Oct-08,VIMS,SPASS Rider,rings(general),LPMRLFMAX,,,null,,,,,, 2008-299T23:28:00,002T02:47:00,25-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-300T00:00:00,000T00:34:08,26-Oct-08,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2008-300T02:07:00,000T01:14:00,26-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE700_NAV,rider,,,,,, 2008-300T03:22:00,000T09:00:00,26-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-300T04:22:00,000T08:00:00,26-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_090IC_DSCAL08300_SP,rider,,,,,, 2008-300T12:22:00,000T00:40:00,26-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE400_SP,rider,,,,,, 2008-300T13:02:00,000T00:43:00,26-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-300T13:02:00,000T00:43:00,26-Oct-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_090RI_SATELLORB009_ISS,rider,,,,,, 2008-300T13:45:00,000T09:00:00,26-Oct-08,CIRS,Prime,rings(general),SUBMS10LP,,CIRS_090RI_SUBMS10LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-300T13:45:00,000T09:00:00,26-Oct-08,CIRS,SPASS Rider,rings(general),SUBMS10LP,,CIRS_090RI_SUBMS10LP001_SI,,,,,,, 2008-300T13:45:00,000T09:00:00,26-Oct-08,ISS,SPASS Rider,rings(general),SUBMS10LP,,,Spoke periodicity movie. riding along on CIRS SUBM obs.,,,,,, 2008-300T13:45:00,000T09:00:00,26-Oct-08,UVIS,SPASS Rider,rings(general),SUBMS10LP,,,,,,,,, 2008-300T13:45:00,000T09:00:00,26-Oct-08,VIMS,SPASS Rider,rings(general),SUBMS10LP,,,null,,,,,, 2008-300T22:45:00,000T03:57:00,26-Oct-08,ISS,Prime,Rhea,065W001PH,,Rhea almost zero phase,"Turn UVIS_FUV to Rhea; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-300T22:45:00,000T03:57:00,26-Oct-08,CIRS,SPASS Rider,Rhea,065W001PH,,CIRS_090RH_065W001PH001_ISS,"Rhea rider. Duration 03:57. AD=1.15 mrad, phase=1, (-5, 65). FP1 and FP3, 15.5 cm-1, centers; shutter closed 01:00 to 01:40.",,,,,, 2008-300T22:45:00,000T03:57:00,26-Oct-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-300T22:45:00,000T03:57:00,26-Oct-08,VIMS,SPASS Rider,Rhea,065W001PH,,spectral cubes,Phase study,,,,,, 2008-301T02:42:00,000T00:40:00,27-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE301_SP,rider,,,,,, 2008-301T03:17:00,000T09:05:00,27-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T46 Titan Bistatic and Occultation on DOY 308.",,,,,, 2008-301T03:22:00,000T09:00:00,27-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-301T04:22:00,000T08:00:00,27-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_090IC_DSCAL08301_SP,rider,,,,,, 2008-301T13:02:00,000T02:00:00,27-Oct-08,ISS,Prime,Tethys,081W010PH,,Tethys lon/phase angle observation,"Turn UVIS_FUV to Tethys; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-301T13:02:00,000T02:00:00,27-Oct-08,CIRS,SPASS Rider,Tethys,081W010PH,,CIRS_090TE_081W010PH001_ISS,"Tethys rider. Duration 02:00. AD=0.9 mrad, phase=10, (1, ~87). FP1 and FP3, 15.5 cm-1, centers; shutter closed 00:20 to 00:45; THEN ALL FP OFF, 401 RTI 00:45 TO 01:45; then FP1 and FP3, 15.5 cm-1, centers, shutter open again to end.",,,,,, 2008-301T13:02:00,000T02:00:00,27-Oct-08,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-301T13:02:00,000T02:00:00,27-Oct-08,VIMS,SPASS Rider,Tethys,081W010PH,,spectral cubes,Phase study,,,,,, 2008-301T15:02:00,000T08:00:00,27-Oct-08,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2008-301T15:02:00,000T08:00:00,27-Oct-08,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_090RI_EGPHASE109_VIMS,rider,,,,,, 2008-301T15:02:00,000T08:00:00,27-Oct-08,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2008-301T16:45:00,000T02:00:00,27-Oct-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-301T18:45:00,000T07:30:00,27-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-301T23:02:00,000T01:15:00,27-Oct-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 13.8 range 2.4 Mkm",,,,,, 2008-301T23:02:00,000T01:15:00,27-Oct-08,CIRS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-301T23:02:00,000T01:15:00,27-Oct-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-302T00:17:00,000T02:00:00,28-Oct-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-302T00:17:00,000T02:00:00,28-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_090RI_DEEPSPACE302_CAPS,rider,,,,,, 2008-302T02:15:00,003T03:50:00,28-Oct-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-302T02:15:00,003T14:19:51,28-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9523451 Rs exit= 4.0335230 Range altitude= -40143.246 km ... 40058.481,,,,,, 2008-302T02:15:00,001T17:22:00,28-Oct-08,INMS,Non-SPASS,Saturn,SURVEYREV,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-302T02:15:00,001T14:15:00,28-Oct-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-302T02:15:00,002T02:47:00,28-Oct-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-302T02:15:10,000T00:00:01,28-Oct-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.3 d, inc = 74.5 deg, r = 20.109 Rs, phase = 24 deg",,,,,, 2008-302T02:17:00,000T07:10:00,28-Oct-08,ISS,Prime,Other,SATSEARCH,Satellite search,ORBIT 82 SATELLITE SEARCH,A satellite search observation staring off the ansa and taking pairs of WACs every ~5 mins for 14 hours. Looking for small satellites in the Mimas-Enceladus region. This observatiojn can be shortened/moved.,,,,,, 2008-302T02:17:00,000T07:10:00,28-Oct-08,CIRS,SPASS Rider,rings(general),SATSEARCH,Satellite search,CIRS_091RI_SATSEARCH001_ISS,rider,,,,,, 2008-302T06:37:00,000T08:00:00,28-Oct-08,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. Last 4 hours required to be tracked at DSS-25 and DSS-14 in 1-way mode.,,,,,, 2008-302T09:27:00,000T00:30:00,28-Oct-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-302T10:32:00,000T09:05:00,28-Oct-08,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T46 Rev91 Titan Bistatic and Occultation experiment on DOY 308.",,,,,, 2008-302T10:37:00,000T09:00:00,28-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-302T11:37:00,000T08:00:00,28-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_091IC_DSCAL08302_SP,rider,,,,,, 2008-302T19:37:00,000T00:40:00,28-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_091RI_DEEPSPACE702_SP,rider,,,,,, 2008-302T20:17:00,000T13:40:00,28-Oct-08,ISS,Prime,RingF,FRSTRCHAN,F ring streamer movie,F RING STREAMER/CHANNEL,"Movie of streamer-channel feature raised in F ring by Prometheus apoapse passage. Need as close to 1 Prom orbital period as possible. Sometimes can be day before or day after. Want 12. 6 of 49 as priority 1, 6 of 49 as priority 2.",,,,,, 2008-302T20:17:00,000T13:40:00,28-Oct-08,CIRS,SPASS Rider,RingF,FRSTRCHAN,F ring streamer movie,CIRS_091RF_FRSTRCHAN001_ISS,rider,,,,,, 2008-303T09:57:00,000T00:40:00,29-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_091RI_DEEPSPACE303_SP,rider,,,,,, 2008-303T10:37:00,000T09:00:00,29-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-303T11:37:00,000T08:00:00,29-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_091IC_DSCAL08303_SP,rider,,,,,, 2008-303T16:30:00,001T13:35:00,29-Oct-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-303T19:37:00,000T00:40:00,29-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_091RI_DEEPSPACE703_SP,rider,,,,,, 2008-303T19:37:00,001T00:00:00,29-Oct-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-303T20:17:00,000T12:50:00,29-Oct-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-303T20:17:00,000T12:50:00,29-Oct-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_091RF_FMOVIE003_ISS,rider,,,,,, 2008-303T20:17:00,000T12:50:00,29-Oct-08,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2008-304T05:02:00,003T01:38:00,30-Oct-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-304T09:07:00,000T01:29:00,30-Oct-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_091RI_DEEPSPACE304_NAV,rider,,,,,, 2008-304T10:37:00,000T09:00:00,30-Oct-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-304T11:37:00,000T08:00:00,30-Oct-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_091IC_DSCAL08304_SP,rider,,,,,, 2008-304T19:37:00,000T07:08:00,30-Oct-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-304T20:22:00,000T04:18:00,30-Oct-08,UVIS,Prime,Saturn,AURORAE,Saturn aurora / lightning search,Saturn Aurora,Auroral Observations led by UVIS Repeated scans across pole to build up auroral images with spectral information,,,,,, 2008-304T20:22:00,000T03:03:00,30-Oct-08,CIRS,SPASS Rider,Saturn,AURORAE,Saturn aurora / lightning search,CIRS_091SA_AURORAE001_UVIS,rider,,,,,, 2008-304T20:22:00,000T03:03:00,30-Oct-08,VIMS,SPASS Rider,Enceladus,AURORAE,Saturn aurora / lightning search,Enceladus,null,,,,,, 2008-304T21:37:00,000T03:03:00,30-Oct-08,ISS,SPASS Rider,Saturn,AURORAE,Saturn aurora / lightning search,Auroral WAC 1X2 movie + lightning search at ~7 Rs.,"Auroral WAC movie. 3 time steps in a 1x2 mosaic in clear, HAL and IR2 filters. Space pickets one hour apart. 18 im. /hour",,,,,, 2008-305T00:40:00,000T03:40:00,31-Oct-08,ISS,Prime,Enceladus,PLMHINCL,,High inc plume observation,High inclination WAC imaging of tendrils,,,,,, 2008-305T00:40:00,000T03:40:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,PLMHINCL,,CIRS_091EN_PLMHINCL001_ISS,FP1+FP3 only.,,,,,, 2008-305T00:40:00,000T03:40:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2008-305T00:40:00,000T03:40:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,PLMHINCL,,Enceladus,null,,,,,, 2008-305T02:45:00,000T02:00:00,31-Oct-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,MAPS Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-305T03:00:00,000T02:05:00,31-Oct-08,RSS,SPASS Rider,Enceladus,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2008-305T04:45:00,000T11:29:51,31-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-305T05:05:00,000T02:30:00,31-Oct-08,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus' Gravity Field Experiment,"Experiment to determine Enceladus's mass, and infer constraints on its internal structure.",,,,,, 2008-305T06:05:00,000T10:39:51,31-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-305T06:05:00,000T05:48:00,31-Oct-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-305T06:05:00,000T10:55:00,31-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-305T06:05:00,000T10:39:51,31-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-305T08:35:51,000T03:39:00,31-Oct-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-305T08:35:51,000T03:39:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,CIRS_091EN_ICYATM001_UVIS,FP1+FP3 only.,,,,,, 2008-305T08:35:51,000T03:39:00,31-Oct-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-305T08:35:51,000T03:39:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,null,,,,,, 2008-305T11:53:00,000T12:11:00,31-Oct-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-305T12:14:51,000T01:00:00,31-Oct-08,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus,null,,,,,, 2008-305T12:14:51,000T01:00:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_091EN_ENCEL001_VIMS,FP1+FP3 only.,,,,,, 2008-305T12:14:51,000T01:00:00,31-Oct-08,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2008-305T12:14:51,000T01:00:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo of icy satellite,,,,,, 2008-305T13:14:51,000T02:50:00,31-Oct-08,CIRS,Prime,Enceladus,FP3STARE,CIRS FP3 stare,CIRS_091EN_FP3STARE001_PRIME;,FP3 stare at north pole at high spectral resolution,,,,,, 2008-305T13:14:51,000T02:50:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,FP3STARE,CIRS FP3 stare,CIRS_091EN FP3STARE SI,Four WAC support images: 1) WAC at 2008-305T13:25 (sunlight); 2) WAC at 2008-305T14:15 (sunlight); 3) WAC at 2008-305T15:00 (sunlight); 4) WAC at 2008-305T15:55 (sunlight).,,,,,, 2008-305T13:14:51,000T02:50:00,31-Oct-08,ISS,SPASS Rider,Enceladus,FP3STARE,CIRS FP3 stare,Enceladus,Enceladus,,,,,, 2008-305T13:14:51,000T02:50:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo of icy satellite,,,,,, 2008-305T13:14:51,000T02:50:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,FP3STARE,CIRS FP3 stare,Enceladus,null,,,,,, 2008-305T15:14:51,000T04:00:00,31-Oct-08,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetspheric plasma and determine whether it generates an internal magnetic field. Rate set to zero as overlaps an INTFLD request.,,,,,, 2008-305T16:04:51,000T00:30:00,31-Oct-08,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus,null,,,,,, 2008-305T16:04:51,000T00:30:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_091EN_ENCEL002_VIMS,rider,,,,,, 2008-305T16:04:51,000T00:30:00,31-Oct-08,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2008-305T16:04:51,000T00:30:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo of icy satellite,,,,,, 2008-305T16:14:51,000T00:40:00,31-Oct-08,INMS,Non-SPASS,Enceladus,ENCEL6,,Enceladus encounter,,,,,,, 2008-305T16:15:29,000T02:00:00,31-Oct-08,CDA,SPASS Rider,DustRAM direction,ENCEL,Enceladus,CDA RPXing 2008-305T17:15:29 MH,Enceladus flyby 2000 km,,,,,, 2008-305T16:34:51,000T01:10:00,31-Oct-08,ISS,Prime,Enceladus,ENCELCA,,Enceladus flyby C/A imaging,Enceladus flyby closest approach imaging.,,,,,, 2008-305T16:34:51,000T01:10:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ENCELCA,,CIRS_091EN_ENCELCA001_ISS,rider,,,,,, 2008-305T16:34:51,000T01:10:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2008-305T16:34:51,000T01:10:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,ENCELA,,Enceladus,null,,,,,, 2008-305T16:34:51,000T00:35:00,31-Oct-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.9946389 Rs exit= 3.9550168 Range altitude= 19496.172 km ... -19931.918,,,,,, 2008-305T16:44:51,000T01:00:00,31-Oct-08,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 091EN Campaign,Part of 091EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magn,,,,,, 2008-305T16:44:54,000T01:00:00,31-Oct-08,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2008-305T16:54:51,000T00:40:00,31-Oct-08,INMS,Non-SPASS,Enceladus,ENCEL6,,Enceladus encounter,,,,,,, 2008-305T17:00:00,000T00:40:00,31-Oct-08,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-305T17:09:51,000T00:48:09,31-Oct-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9546418 Rs exit= 3.9527618 Range altitude= -20869.104 km ... -39555.722,,,,,, 2008-305T17:34:51,000T00:40:00,31-Oct-08,INMS,Non-SPASS,Enceladus,ENCEL6,,Enceladus encounter,,,,,,, 2008-305T17:40:00,000T11:55:00,31-Oct-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-305T17:44:51,000T00:20:00,31-Oct-08,UVIS,Prime,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering. Start scan with CIRS FP3 centered at TBD (ISS handoff location) and continue scan in direction such that CIRS FP3 goes through -75 / 200 W. Use TBD microrad/sec scan rate.,,,,,, 2008-305T17:44:51,000T11:50:06,31-Oct-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-305T17:44:51,000T00:20:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ICYSCAN,,CIRS_091EN_ICYSCAN001_UVIS,rider,,,,,, 2008-305T17:44:51,000T00:20:00,31-Oct-08,ISS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,Enceladus,Enceladus,,,,,, 2008-305T17:44:51,000T00:20:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,ICYSCAN,,Enceladus,null,,,,,, 2008-305T17:44:51,000T11:50:06,31-Oct-08,RPWS,Non-SPASS,Saturn,AURXNGSIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-305T17:50:20,000T00:00:01,31-Oct-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.948 Rs, lat = -8 deg, phase = 156 deg",,,,,, 2008-305T17:58:00,004T05:31:00,31-Oct-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.9529490 Rs exit= 4.4381755 Range altitude= -40486.467 km ... 40847.171,,,,,, 2008-305T18:04:51,000T03:10:00,31-Oct-08,CIRS,Prime,Enceladus,SECLNX,,CIRS_091EN_SECLNX001_PRIME;,"(E6) FP3 Polar thermal output integration; 9-3, high S lat.; begins C/A+00:51. SOST. N305T18:04:31, X305T20:37:00.",,,,,, 2008-305T18:04:51,000T03:10:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,SECLNX,,CIRS_091EN SECLNX SI,".....PLACEHOLDER (ZERO DATA VOLUME)........ 4 SI for for pointing verification: 2 NAC for FP3 eclipse entry, and 2 WAC for eclipse exit (can use lossy compression). First (NAC) at 2008-321T14:43 (5 min. before entry; entry at 2008-321T14:47:53); AD=2.8 mrad; Second (NAC) at 2008-321T17:23 (20 min. before exit; exit at 2008-321T17:42:50; expose for grey light or for star); AD=3.5 mrad; Third (WAC) at 2008-321T17:38 (5 min. before exit); AD=3.5 mrad; Fourth (WAC) just before return to waypoint (observation ends at 2008-321T18:23); AD~3.6 mrad.",,,,,, 2008-305T18:04:51,000T03:10:00,31-Oct-08,ISS,SPASS Rider,Enceladus,SECLNX,,Enceladus,SPT in eclipse to detect non-thermal emission,,,,,, 2008-305T18:04:51,000T00:20:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2008-305T18:04:51,000T03:10:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,SECLNX,,Enceladus,null,,,,,, 2008-305T18:14:51,002T01:07:06,31-Oct-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-305T18:24:51,000T00:40:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2008-305T19:04:51,000T02:10:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2008-305T21:14:51,000T01:00:00,31-Oct-08,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus,null,,,,,, 2008-305T21:14:51,000T01:00:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_091EN_ENCEL003_VIMS,rider,,,,,, 2008-305T21:14:51,000T01:00:00,31-Oct-08,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2008-305T21:14:51,000T01:00:00,31-Oct-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo of icy satellite,,,,,, 2008-305T22:14:51,000T02:00:00,31-Oct-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-305T22:14:51,000T02:00:00,31-Oct-08,CIRS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,CIRS_091EN_ICYATM002_UVIS,rider,,,,,, 2008-305T22:14:51,000T02:00:00,31-Oct-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-305T22:14:51,000T02:00:00,31-Oct-08,VIMS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,null,,,,,, 2008-306T00:04:00,000T05:31:00,1-Nov-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-306T01:15:00,000T00:45:00,1-Nov-08,RSS,Prime,Enceladus,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2008-306T02:00:00,000T03:30:00,1-Nov-08,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus' Gravity Field Experiment,"Experiment to determine Enceladus's mass, and infer constraints on its internal structure.",,,,,, 2008-306T05:35:00,002T10:00:13,1-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-306T05:35:00,001T13:47:00,1-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-306T05:35:00,000T19:00:00,1-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-306T06:15:00,000T03:22:00,1-Nov-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-306T06:15:00,000T03:22:00,1-Nov-08,CIRS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,CIRS_091EN_ICYATM003_UVIS,rider,,,,,, 2008-306T06:15:00,000T03:22:00,1-Nov-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-306T06:15:00,000T03:22:00,1-Nov-08,VIMS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,null,,,,,, 2008-306T10:17:00,000T09:05:00,1-Nov-08,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' mass,Downlink pass at Ka-band for Enceladus' mass determination and for improving locally Cassini orbit.,,,,,, 2008-306T10:22:00,000T09:00:00,1-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-306T11:22:00,000T08:00:00,1-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_091IC_DSCAL08306_SP,rider,,,,,, 2008-306T20:07:00,000T00:30:00,1-Nov-08,ISS,Prime,Rhea,GEOLOG,Geologic study,Rhea mapping,Turn -Y to Rhea; do 1x1 mosaic; turn to WP.,,,,,, 2008-306T20:07:00,000T00:30:00,1-Nov-08,CIRS,SPASS Rider,Rhea,GEOLOG,Geologic study,CIRS_091RH_GEOLOG001_ISS,rider,,,,,, 2008-306T20:07:00,000T00:30:00,1-Nov-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-306T20:07:00,000T00:30:00,1-Nov-08,VIMS,SPASS Rider,Rhea,GEOLOG,Geologic study,Rhea,null,,,,,, 2008-306T20:37:00,000T13:00:00,1-Nov-08,VIMS,Prime,rings(general),APOMOSL,,"Apoapse mosaic, lit side",Do 9 lit side at priority 2 (~every third orbit),,,,,, 2008-306T20:37:00,000T13:00:00,1-Nov-08,CIRS,SPASS Rider,rings(general),APOMOSL,,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2008-306T20:37:00,000T13:00:00,1-Nov-08,ISS,SPASS Rider,rings(general),APOMOSL,,Apoapse mosaic,Riding along on apoapse mosaic to search for spokes,,,,,, 2008-306T20:37:00,000T13:00:00,1-Nov-08,UVIS,SPASS Rider,rings(general),APOMOS,Apoapsis mosaic,,,,,,,, 2008-307T00:35:00,001T15:00:23,2-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-307T06:40:00,000T12:42:00,2-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-307T10:17:00,000T09:05:00,2-Nov-08,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat and occultation,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2008-307T10:22:00,000T09:00:00,2-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-307T10:37:00,000T05:54:00,2-Nov-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-307T11:22:00,000T08:00:00,2-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_091IC_DSCAL08307_SP,rider,,,,,, 2008-307T19:22:00,000T21:13:23,2-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-307T19:22:00,000T18:13:23,2-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-307T19:22:00,000T20:13:23,2-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-307T20:17:33,000T06:17:50,2-Nov-08,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2008-307T20:17:33,000T06:17:50,2-Nov-08,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (8 integrations total = 16 frames, 0.5 Mb/frame)",,,,,, 2008-307T20:17:33,000T08:17:50,2-Nov-08,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp Map,VIMS_Rings. Ridealong with CIRS obs.,,,,,, 2008-308T02:35:23,000T06:00:00,3-Nov-08,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-308T02:35:23,000T06:00:00,3-Nov-08,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2008-308T04:35:23,000T04:00:00,3-Nov-08,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR nadir comp map,VIMS_Rings. Ridealong with CIRS obs.,,,,,, 2008-308T08:35:23,000T04:00:00,3-Nov-08,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2008-308T08:35:23,000T04:00:00,3-Nov-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-308T08:35:23,000T04:00:00,3-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,ISS Global Map,Global mapping. Ridealong with ISS,,,,,, 2008-308T12:35:23,000T01:30:00,3-Nov-08,ISS,Prime,Titan,REGMAP,Regional mapping,NAC Regional Map,regional map,,,,,, 2008-308T12:35:23,000T01:30:00,3-Nov-08,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-308T12:35:23,000T01:30:00,3-Nov-08,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,ISS Regional Map,Regional mapping. Ridealong with ISS,,,,,, 2008-308T13:35:23,000T08:00:00,3-Nov-08,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,MAPS_Titan_Flyby,"T046 is a flank-in flyby with a minimum altitude of 1200 km. This geometry is adequate for studies of the draping of the external magnetic field around Titan on the nightside hemisphere. T046 takes place in Saturn's near-noon sector (10.5 hours SLT), where Titan could be found in the magnetosheath if the solar wind pressure is high. We assign grade one priority.",,,,,, 2008-308T14:06:23,000T02:01:00,3-Nov-08,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2008-308T14:06:23,000T02:01:00,3-Nov-08,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2008-308T14:06:23,000T01:39:00,3-Nov-08,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong context imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-308T14:06:23,000T01:39:00,3-Nov-08,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS Far-IR Nadir Map,Ridealong with CIRS Far-IR mapping,,,,,, 2008-308T14:10:23,000T02:05:00,3-Nov-08,RSS,SPASS Rider,Titan,THERMAL,Thermal stabilization period,RSS Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2008-308T15:35:23,000T01:00:00,3-Nov-08,CAPS,SPASS Rider,Titan,T46INBND,,Inbound 091TI (T45),Inbound leg of a Titan encoun,,,,,, 2008-308T15:35:23,000T01:00:00,3-Nov-08,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-308T15:35:23,000T01:30:00,3-Nov-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-308T16:09:23,000T01:12:00,3-Nov-08,RSS,Prime,Titan,BISTATIN,RSS Bistatic ingress observation,RSS Bistatic Obs of Titan T46 (ingress),"Bistatic scattering measurments at three radio wavelengths to determine the physical properties of Titan's surface, including reflectivity, dielectric constant, and roughness.",,,,,, 2008-308T16:35:23,000T02:00:00,3-Nov-08,CAPS,SPASS Rider,Titan,T46CLOSE,,Closest approach 091TI (T45),Closest approach of a Titan encoun,,,,,, 2008-308T16:35:23,000T02:00:00,3-Nov-08,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-308T16:35:23,000T00:40:00,3-Nov-08,INMS,Non-SPASS,Titan,TITAN46,,Titan observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-308T17:05:23,000T01:00:00,3-Nov-08,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2008-308T17:15:23,000T00:40:00,3-Nov-08,INMS,Non-SPASS,Titan,TITAN46,,Titan observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-308T17:21:23,000T00:33:00,3-Nov-08,RSS,Prime,Titan,OCC,Occultation,RSS OCC of Titan T46,RSS ingress/egress occultation of Titan's atmosphere and ionosphere,,,,,, 2008-308T17:54:23,000T00:56:54,3-Nov-08,RSS,Prime,Titan,BISTATOUT,RSS Bistatic egress observation,RSS Bistatic Obs of Titan T46(egress),"Bistatic scattering measurments at three radio wavelengths to determine the physical properties of Titan's surface, including reflectivity, dielectric constant, and roughness.",,,,,, 2008-308T17:55:23,000T00:40:00,3-Nov-08,INMS,Non-SPASS,Titan,TITAN46,,Titan observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-308T18:05:23,000T01:30:00,3-Nov-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-308T18:35:23,000T01:00:00,3-Nov-08,CAPS,SPASS Rider,Titan,T46OUTBND,,Outbound 091TI (T45),Outbound leg of a Titan encoun,,,,,, 2008-308T18:35:23,000T23:00:00,3-Nov-08,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-308T18:35:23,000T01:39:36,3-Nov-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-308T19:03:23,000T00:24:00,3-Nov-08,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2008-308T19:26:23,000T07:09:00,3-Nov-08,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2008-308T19:26:23,000T07:08:00,3-Nov-08,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong context imaging),regional map,,,,,, 2008-308T19:27:23,000T07:08:00,3-Nov-08,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk.",,,,,, 2008-308T19:27:23,000T07:08:00,3-Nov-08,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,UVIS ERVFUV Map,Ridealong with UVIS EUVFUV Map,,,,,, 2008-308T19:35:13,001T03:54:47,3-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-308T19:35:23,000T23:32:36,3-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-308T20:15:00,000T02:00:00,3-Nov-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-308T21:35:23,000T21:32:37,3-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-308T22:15:00,000T20:53:00,3-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-309T02:35:23,000T01:00:00,4-Nov-08,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-309T02:35:23,000T01:00:00,4-Nov-08,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-309T02:35:23,000T01:00:00,4-Nov-08,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Photometry Obs.,Ridealong with ISS photmetry obs.,,,,,, 2008-309T03:35:23,000T04:38:00,4-Nov-08,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-309T03:35:23,000T04:38:00,4-Nov-08,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (35integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2008-309T03:35:23,000T03:00:00,4-Nov-08,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir comp. map,Ridealong with CIRS obs. Far-IR nadir comp. map,,,,,, 2008-309T06:35:23,000T01:00:00,4-Nov-08,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,"ISS Monitor, NAC",Ridealong with ISS monitoring NAC obs.,,,,,, 2008-309T07:35:23,000T01:48:10,4-Nov-08,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp Map,Ridealong with CIRS Temp Map,,,,,, 2008-309T08:13:23,000T01:00:00,4-Nov-08,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-309T08:13:33,000T01:00:00,4-Nov-08,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Night NAC,"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2008-309T10:03:00,000T09:05:00,4-Nov-08,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat and occultation,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2008-309T10:08:00,000T09:00:00,4-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-309T11:08:00,000T08:00:00,4-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_091IC_DSCAL08309_SP,rider,,,,,, 2008-309T12:00:00,000T02:00:00,4-Nov-08,CAPS,Non-SPASS,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-309T17:35:23,000T05:54:37,4-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-309T19:08:00,000T01:14:00,4-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_091RI_DEEPSPACE309_NAV,rider,,,,,, 2008-309T19:08:00,000T04:22:00,4-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-309T19:08:00,003T15:47:00,4-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-309T19:08:00,000T04:21:00,4-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-309T20:23:00,000T03:00:00,4-Nov-08,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2008-309T20:23:00,000T03:00:00,4-Nov-08,CIRS,SPASS Rider,rings(general),ALPVIR,Alpha Virginis occultation,CIRS_091RI_ALPVIR001_UVIS,rider,,,,,, 2008-309T23:23:00,000T00:37:00,4-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-309T23:23:00,000T00:37:00,4-Nov-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_091RI_SATELLORB001_ISS,rider,,,,,, 2008-309T23:29:00,003T21:05:00,4-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 3.9529490 Rs exit= 4.4381755 Range altitude= -40486.467 km ... 40847.171,,,,,, 2008-309T23:29:00,002T10:31:00,4-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-309T23:29:51,000T00:00:01,4-Nov-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 7.9 d, inc = 70.6 deg, r = 21.149 Rs, phase = 26 deg",,,,,, 2008-309T23:30:00,003T11:25:00,4-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-309T23:30:00,003T10:45:00,4-Nov-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-309T23:30:00,001T06:30:00,4-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-310T00:00:00,000T09:00:00,5-Nov-08,CIRS,Prime,rings(general),TMAPN20LP,,CIRS_092RI_TMAPN20LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-310T00:00:00,000T09:00:00,5-Nov-08,CIRS,SPASS Rider,rings(general),TMAPN20LP,,CIRS_092RI_TMAPN20LP001_SI,,,,,,, 2008-310T00:00:00,000T09:00:00,5-Nov-08,UVIS,SPASS Rider,rings(general),TMAPN20LP,,URSTAR,,,,,,, 2008-310T00:00:00,001T00:00:00,5-Nov-08,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2008-310T09:00:00,000T00:28:00,5-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-310T09:00:00,000T00:28:00,5-Nov-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_092RI_SATELLORB002_ISS,rider,,,,,, 2008-310T09:28:00,000T00:40:00,5-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE310_SP,rider,,,,,, 2008-310T10:08:00,000T09:00:00,5-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-310T11:08:00,000T08:00:00,5-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_092IC_DSCAL08310_SP,rider,,,,,, 2008-310T19:08:00,000T00:40:00,5-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE710_SP,rider,,,,,, 2008-310T19:48:00,000T06:10:00,5-Nov-08,CIRS,Prime,rings(general),TMAPN30LP,,CIRS_092RI_TMAPN30LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-310T19:48:00,000T06:10:00,5-Nov-08,CIRS,SPASS Rider,rings(general),TMAPN30LP,,CIRS_092RI_TMAPN30LP001_SI,,,,,,, 2008-310T19:48:00,000T06:10:00,5-Nov-08,UVIS,SPASS Rider,rings(general),TMAPN30LP,,URSTAR,,,,,,, 2008-311T01:58:00,000T00:40:00,6-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE311_SP,rider,,,,,, 2008-311T02:33:00,000T09:05:00,6-Nov-08,RSS,SPASS Rider,Saturn,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev92 and Rev93 Saturn Gravity experiments on DOY 313 and DOY 322.",,,,,, 2008-311T02:38:00,000T09:00:00,6-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-311T03:38:00,000T08:00:00,6-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_092IC_DSCAL08311_SP,rider,,,,,, 2008-311T06:00:00,002T04:55:00,6-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-311T12:00:00,000T03:33:00,6-Nov-08,RADAR,SPASS Rider,Other,WU4NMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2008-311T12:18:00,000T01:15:00,6-Nov-08,ISS,Prime,Titan,MR1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 89.4 range 1.2 Mkm",,,,,, 2008-311T12:18:00,000T01:15:00,6-Nov-08,CIRS,SPASS Rider,Titan,MR1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-311T12:18:00,000T01:15:00,6-Nov-08,UVIS,SPASS Rider,Titan,MR1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-311T13:33:00,000T02:00:00,6-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-311T13:33:00,000T02:00:00,6-Nov-08,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_092RI_SURVEYPTG002_CAPS,rider,,,,,, 2008-311T15:33:00,000T01:57:00,6-Nov-08,RADAR,Prime,Titan,NMIDLCAL,,"Distant Titan Radiometry, South Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2008-311T17:30:00,000T00:30:00,6-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-311T17:30:00,000T00:30:00,6-Nov-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_092RI_SATELLORB006_ISS,rider,,,,,, 2008-311T18:00:00,000T09:00:00,6-Nov-08,CIRS,Prime,rings(general),TMAPN45LP,,CIRS_092RI_TMAPN45LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-311T18:00:00,000T09:00:00,6-Nov-08,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_092RI_TMAPN45LP001_SI,,,,,,, 2008-311T18:00:00,000T09:00:00,6-Nov-08,UVIS,SPASS Rider,rings(general),TMAPN45LP,,URSTAR,,,,,,, 2008-312T00:00:00,000T00:34:08,7-Nov-08,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2008-312T03:00:00,000T03:00:00,7-Nov-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-312T03:00:00,000T03:00:00,7-Nov-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_092RF_FMOVIE003_ISS,rider,,,,,, 2008-312T06:00:00,000T02:00:00,7-Nov-08,ISS,Prime,rings(general),RETARMRLP,,Medium res retargetables,Medium Res Retarg of small ring region satellites. Need 25 of 54.,,,,,, 2008-312T06:00:00,000T02:00:00,7-Nov-08,CIRS,SPASS Rider,rings(general),RETARMRLP,,CIRS_092RI_RETARMRLP001_ISS,rider,,,,,, 2008-312T08:00:00,000T00:38:00,7-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-312T08:00:00,000T00:38:00,7-Nov-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_092RI_SATELLORB007_ISS,rider,,,,,, 2008-312T08:38:00,000T01:29:00,7-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE312_NAV,rider,,,,,, 2008-312T10:00:00,003T00:55:00,7-Nov-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-312T10:03:00,000T07:47:00,7-Nov-08,RSS,SPASS Rider,Saturn,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev92 and Rev93 Saturn Gravity experiments on DOY 313 and DOY 322.",,,,,, 2008-312T10:08:00,000T07:42:00,7-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-312T11:08:00,000T06:42:00,7-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_092IC_DSCAL08312_SP,rider,,,,,, 2008-312T18:30:00,000T06:00:00,7-Nov-08,UVIS,Prime,Star,URALP1CRU,,URSTAR,,,,,,, 2008-312T18:30:00,000T06:00:00,7-Nov-08,CIRS,SPASS Rider,rings(general),URALP1CRU,,CIRS_092RI_URALP1CRU_UVIS,rider,,,,,, 2008-312T18:30:00,000T06:00:00,7-Nov-08,UVIS,SPASS Rider,Star,URALP1CRU,,Support Imaging,NAC support images at the following times: 2008-312t19:31:40.0 2008-312t19:48:29:5 2008-312T20:42:51.7,,,,,, 2008-313T00:30:00,000T05:27:00,8-Nov-08,ISS,Prime,RingF,FRINGHRDF,,High Resolution F Ring Scan,Complete high resolution (0-10Rs) longitudinal scan of the F ring. Dark face. Need at least 3 during XM. 2 of 27 as priority 1 and 1 as priority 2.,,,,,, 2008-313T00:30:00,000T05:27:00,8-Nov-08,VIMS,SPASS Rider,RingF,FRINGHRDF,,F movie,"64*12, 640 msec",,,,,, 2008-313T05:57:00,000T04:41:00,8-Nov-08,UVIS,Prime,Star,URBETCEN,Stellar occultation,URSTAR,,,,,,, 2008-313T05:57:00,000T04:41:00,8-Nov-08,CIRS,SPASS Rider,rings(general),URBETCEN,Stellar occultation,CIRS_092RI_URBETACEN_UVIS,rider,,,,,, 2008-313T05:57:00,000T04:41:00,8-Nov-08,UVIS,SPASS Rider,Star,URBETCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2008-313T09:50:00.0 2008-313T09:37:39.0 2008-313T08:56:02.0,,,,,, 2008-313T10:15:00,000T02:00:00,8-Nov-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-313T10:38:00,000T02:05:00,8-Nov-08,VIMS,Prime,rings(general),SHADSCANU,,Ring SHADSCAN unlit side,Do 2 at priority 1,,,,,, 2008-313T10:38:00,000T02:05:00,8-Nov-08,CIRS,SPASS Rider,rings(general),SHADSCANU,,CIRS_092RI_SHADSCANU_VIMS,rider,,,,,, 2008-313T10:55:00,000T14:28:00,8-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-313T10:55:00,000T10:18:00,8-Nov-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-313T10:55:00,000T23:20:00,8-Nov-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-313T10:55:00,000T06:28:00,8-Nov-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-313T12:15:00,000T13:08:00,8-Nov-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-313T12:43:00,000T03:00:00,8-Nov-08,CIRS,Prime,rings(general),TDIFN45HP,,,,,,,,, 2008-313T12:43:00,000T03:00:00,8-Nov-08,CIRS,SPASS Rider,rings(general),TDIFN45HP,,CIRS_092RI_TDIFN45HP001_SI,,,,,,, 2008-313T16:23:00,000T09:00:00,8-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-313T17:23:00,000T07:00:00,8-Nov-08,RPWS,SPASS Rider,Saturn,RCSWHIST,RPWS lightning search (RCS),non RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-313T20:20:29,000T02:00:00,8-Nov-08,CDA,SPASS Rider,DustRAM direction,RPX0110,,CDA RPXing 2008-313T21:20:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-313T20:25:00,000T02:30:00,8-Nov-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-313T20:34:00,000T00:23:00,8-Nov-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.4355522 Rs exit= 4.3827618 Range altitude= 39981.104 km ... 20865.428,,,,,, 2008-313T20:50:00,000T01:00:00,8-Nov-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-313T20:57:00,000T00:46:00,8-Nov-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.3805906 Rs exit= 4.3044642 Range altitude= 19994.256 km ... -19264.102,,,,,, 2008-313T21:13:00,000T07:00:00,8-Nov-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-313T21:43:00,000T00:23:00,8-Nov-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.3032656 Rs exit= 4.2824938 Range altitude= -20135.339 km ... -39250.097,,,,,, 2008-313T22:06:00,004T00:23:00,8-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 4.2818061 Rs exit= 4.4367255 Range altitude= -40115.918 km ... 40399.712,,,,,, 2008-313T22:36:06,000T00:00:01,8-Nov-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.269 Rs, lat = -15 deg, phase = 154 deg",,,,,, 2008-314T00:23:00,000T10:09:00,9-Nov-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-314T01:23:00,000T02:27:00,9-Nov-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-314T01:23:00,000T05:07:00,9-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-314T01:23:00,000T17:30:00,9-Nov-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-314T04:13:00,000T06:02:00,9-Nov-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-314T04:30:00,000T04:43:00,9-Nov-08,ISS,Prime,rings(general),AZSCANLIT,,AZSCAN lit,AZSCAN maxwell ringlet,,,,,, 2008-314T06:30:00,000T03:45:00,9-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-314T09:53:00,000T09:00:00,9-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-314T10:15:00,003T12:15:00,9-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-314T10:15:00,000T17:58:00,9-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-314T10:15:00,000T16:45:00,9-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-314T10:53:00,000T08:00:00,9-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_092IC_DSCAL08314_SP,rider,,,,,, 2008-314T18:53:00,001T22:37:00,9-Nov-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-314T19:33:00,000T01:15:00,9-Nov-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 56 range 1.8 Mkm",,,,,, 2008-314T19:33:00,000T01:15:00,9-Nov-08,CIRS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-314T19:33:00,000T01:15:00,9-Nov-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-314T20:48:00,000T02:00:00,9-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-314T20:48:00,000T02:00:00,9-Nov-08,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_092RI_SURVEYPTG003_CAPS,rider,,,,,, 2008-314T22:48:00,000T01:12:00,9-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-314T22:48:00,000T01:12:00,9-Nov-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_092RI_SATELLORB008_ISS,rider,,,,,, 2008-315T00:00:00,000T04:13:00,10-Nov-08,VIMS,Prime,rings(general),RSCNCOCC,,Ring stellar occ - RS Cnc,"B ring, region IV",,,,,, 2008-315T00:00:00,000T04:13:00,10-Nov-08,CIRS,SPASS Rider,rings(general),RSCNCOCC,,CIRS_092RI_RSCNCOCC301_VIMS,rider,,,,,, 2008-315T00:00:00,000T04:13:00,10-Nov-08,UVIS,SPASS Rider,rings(general),RSCNCOCC,,URSTAR,,,,,,, 2008-315T03:00:00,002T19:30:00,10-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-315T04:13:00,000T05:00:00,10-Nov-08,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-315T09:13:00,000T00:40:00,10-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE315_SP,rider,,,,,, 2008-315T09:13:00,002T00:47:00,10-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-315T09:53:00,000T09:00:00,10-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-315T10:08:00,000T08:45:00,10-Nov-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-315T10:53:00,000T08:00:00,10-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_092IC_DSCAL08315_SP,rider,,,,,, 2008-315T10:55:00,002T11:34:00,10-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-315T18:53:00,000T00:40:00,10-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE715_SP,rider,,,,,, 2008-315T19:33:00,000T00:27:00,10-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-315T20:00:00,000T08:44:00,10-Nov-08,CIRS,Prime,rings(general),TMAPS10LP,,CIRS_092RI_TMAPS10LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-315T20:00:00,000T08:44:00,10-Nov-08,CIRS,SPASS Rider,rings(general),TMAPS10LP,,CIRS_092RI_TMAPS10LP001_SI,,,,,,, 2008-315T20:00:00,000T08:44:00,10-Nov-08,UVIS,SPASS Rider,rings(general),TMAPS10LP,,URSTAR,,,,,,, 2008-316T04:44:00,000T00:30:00,11-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-316T05:14:00,000T02:00:00,11-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-316T07:14:00,000T01:24:00,11-Nov-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-316T07:14:00,000T01:24:00,11-Nov-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_092RI_FMONITOR003_ISS,rider,,,,,, 2008-316T08:38:00,000T01:14:00,11-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE316_NAV,rider,,,,,, 2008-316T09:53:00,000T09:00:00,11-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-316T10:53:00,000T08:00:00,11-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_092IC_DSCAL08316_SP,rider,,,,,, 2008-316T17:30:00,000T02:00:00,11-Nov-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-316T18:53:00,000T00:40:00,11-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE716_SP,rider,,,,,, 2008-316T19:30:00,001T03:00:00,11-Nov-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-316T19:33:00,000T11:12:00,11-Nov-08,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2008-316T19:33:00,000T11:12:00,11-Nov-08,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_092RI_EGPHASE110_VIMS,rider,,,,,, 2008-316T19:33:00,000T11:12:00,11-Nov-08,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2008-316T19:33:00,000T11:12:00,11-Nov-08,UVIS,SPASS Rider,rings(general),EGPHASE,,URSTAR,,,,,,, 2008-317T06:45:00,000T08:00:00,12-Nov-08,CIRS,Prime,rings(general),TMAPN10LP,,CIRS_092RI_TMAPN10LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-317T06:45:00,000T08:00:00,12-Nov-08,CIRS,SPASS Rider,rings(general),TMAPN10LP,,CIRS_092RI_TMAPN10LP001_SI,,,,,,, 2008-317T06:45:00,000T08:00:00,12-Nov-08,UVIS,SPASS Rider,rings(general),TMAPN10LP,,URSTAR,,,,,,, 2008-317T10:00:00,000T05:00:00,12-Nov-08,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE 25Rs AND SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. IF OpMode not ORS, unique sequence will be required.",,,,,, 2008-317T14:45:00,000T00:44:00,12-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-317T14:45:00,000T00:44:00,12-Nov-08,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_092RI_SATELLORB011_ISS,rider,,,,,, 2008-317T15:00:00,000T07:29:00,12-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-317T15:29:00,000T00:40:00,12-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_092RI_DEEPSPACE317_SP,rider,,,,,, 2008-317T16:09:00,000T09:00:00,12-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-317T22:29:00,003T21:54:00,12-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 4.2818061 Rs exit= 4.4367255 Range altitude= -40115.918 km ... 40399.712,,,,,, 2008-317T22:29:00,000T02:40:00,12-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-317T22:29:00,002T11:31:00,12-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-317T22:29:11,000T00:00:01,12-Nov-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 8.0 d, inc = 70.5 deg, r = 21.284 Rs, phase = 26 deg",,,,,, 2008-317T22:30:00,003T12:15:00,12-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-317T22:30:00,000T02:39:00,12-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-317T22:30:00,001T07:30:00,12-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-318T01:09:00,001T00:00:00,13-Nov-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-318T01:09:00,002T10:00:00,13-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-318T01:49:00,000T01:15:00,13-Nov-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 56 range 1.8 Mkm",,,,,, 2008-318T03:04:00,000T02:00:00,13-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-318T05:04:00,000T00:30:00,13-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-318T05:34:00,000T09:55:00,13-Nov-08,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side",Do 15 unlit side at priority 2 (~every third orbit),,,,,, 2008-318T05:34:00,000T09:55:00,13-Nov-08,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_093RI_APOMOSU115_VIMS,rider,,,,,, 2008-318T12:00:00,000T01:08:16,13-Nov-08,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2008-318T16:09:00,000T09:00:00,13-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-318T17:09:00,000T08:00:00,13-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_093IC_DSCAL08318_SP,rider,,,,,, 2008-319T01:09:00,002T10:00:00,14-Nov-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post Backup OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-319T01:49:00,000T03:11:00,14-Nov-08,UVIS,Prime,Mimas,ICYSTARE,,ICYSTARE: long satellite stare,,,,,,, 2008-319T05:00:00,000T10:00:00,14-Nov-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_093SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2008-319T06:00:00,001T05:00:00,14-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-319T15:00:00,000T09:39:00,14-Nov-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-319T15:00:00,000T09:39:00,14-Nov-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_093RF_FMOVIE003_ISS,rider,,,,,, 2008-320T02:09:00,000T09:00:00,15-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-320T03:09:00,000T08:00:00,15-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_093IC_DSCAL08320_SP,rider,,,,,, 2008-320T06:00:00,000T01:00:00,15-Nov-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-320T10:00:00,003T00:45:00,15-Nov-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-320T11:00:00,001T16:03:00,15-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-320T11:09:00,000T23:36:00,15-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-320T12:00:00,000T04:33:04,15-Nov-08,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2008-320T12:00:00,000T03:51:00,15-Nov-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-320T12:44:00,000T02:01:00,15-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-320T14:45:00,000T04:57:00,15-Nov-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. MAG segment.",,,,,, 2008-320T19:42:00,000T05:47:00,15-Nov-08,VIMS,Prime,Saturn,NPOLEAUR,,North Pole aurora mosaic 2,3x3 North Polar mosaic. 1 sec integration/pixel. Each frame takes approx 70 min.,,,,,, 2008-320T19:42:00,000T05:47:00,15-Nov-08,ISS,SPASS Rider,Saturn,NPOLEAUR,,"Polar movie with the WAC in CB3,MT2,CB2,MT2, BL1","4 pickets spaced 1h 30m. 2x1 WAC in CB3/MT3 (left frame only), CB2/MT2, and BL1.",,,,,, 2008-320T19:42:00,000T05:47:00,15-Nov-08,UVIS,SPASS Rider,Saturn,NPOLEAUR,,Saturn Aurora,Rider on VIMS NPOLEAUR observations,,,,,, 2008-321T02:09:00,000T09:00:00,16-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-321T03:09:00,000T08:00:00,16-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_093IC_DSCAL08321_SP,rider,,,,,, 2008-321T03:09:00,000T07:00:00,16-Nov-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-321T10:45:00,000T05:55:00,16-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-321T10:45:00,000T10:16:00,16-Nov-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-321T10:45:00,000T23:15:00,16-Nov-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-321T11:09:00,001T07:15:00,16-Nov-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-321T11:49:00,000T01:58:00,16-Nov-08,ISS,Prime,RingF,FMOVIE,F ring movie,SHORT HI RES F RING MOVIE,Short hi res F ring stare on day of periapse. Designed to fit into gaps left by other obs. Point to ring radius/longitude and stare for ~2 hrs as material passes through field of view to get ~40 degs of co-rotating longitude,,,,,, 2008-321T13:47:00,000T04:36:00,16-Nov-08,CIRS,Prime,Dione,SECLNX,,CIRS_093DI_SECLNX001_PRIME;,"FP3 N, FP1 X; 2.9-4.0; N hem., LT~14; moderate range decrease. MAG TWT. N321T14:47:53, X321T17:42:50. Entry: FP3 to (15, 330); exit: FP1 to (316, 25). Center detectors, 15.5 cm-1, shutter first and last 3 min. Observe Dione in eclipse by Saturn. Look for spatial variability at low latitudes.",,,,,, 2008-321T13:47:00,000T04:36:00,16-Nov-08,CIRS,SPASS Rider,Dione,SECLNX,,CIRS_093DI SECLNX SI,"4 SI for for pointing verification: 2 NAC for FP3 eclipse entry, and 2 WAC for eclipse exit (can use lossy compression). First (NAC) at 2008-321T14:43 (5 min. before entry; entry at 2008-321T14:47:53); AD=2.8 mrad; Second (NAC) at 2008-321T17:23 (20 min. before exit; exit at 2008-321T17:42:50; expose for grey light or for star); AD=3.5 mrad; Third (WAC) at 2008-321T17:38 (5 min. before exit); AD=3.5 mrad; Fourth (WAC) just before return to waypoint (observation ends at 2008-321T18:23); AD~3.6 mrad.",,,,,, 2008-321T13:47:00,000T04:36:00,16-Nov-08,UVIS,SPASS Rider,Dione,ICYECL,,ICYECL: observe satellite in eclipse,,,,,,, 2008-321T13:47:00,000T04:36:00,16-Nov-08,VIMS,SPASS Rider,Dione,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-321T16:40:00,000T08:40:00,16-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-321T16:48:00,000T02:05:00,16-Nov-08,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2008-321T18:53:00,000T07:30:00,16-Nov-08,RSS,SPASS Rider,Saturn,GRAVITY,RSS gravity science experiment,RSS Saturn's Gravity Field Experiment,Experiment to determine Saturn's gravity field and infer constraints on its internal structure.,,,,,, 2008-321T20:10:00,000T02:30:00,16-Nov-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-321T20:23:00,000T00:16:29,16-Nov-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.4341097 Rs exit= 4.3815052 Range altitude= 39533.056 km ... 20405.171,,,,,, 2008-321T20:38:00,000T01:00:00,16-Nov-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-321T20:39:29,000T01:00:00,16-Nov-08,CDA,Prime,Other,RATE320,,Data rate,Range enter= 4.3793434 Rs exit= 4.3037261 Range altitude= 19533.480 km ... -19744.579,,,,,, 2008-321T21:01:00,000T07:01:00,16-Nov-08,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2008-321T21:39:29,000T00:15:31,16-Nov-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.3025406 Rs exit= 4.2820774 Range altitude= -20616.169 km ... -39737.695,,,,,, 2008-321T21:55:00,003T12:22:00,16-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 4.2814045 Rs exit= 5.3163934 Range altitude= -40603.778 km ... 40176.583,,,,,, 2008-321T22:22:21,000T00:00:01,16-Nov-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.269 Rs, lat = -15 deg, phase = 154 deg",,,,,, 2008-321T23:00:00,000T00:30:00,16-Nov-08,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2008-322T01:20:00,000T08:40:00,17-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-322T02:48:00,000T03:07:00,17-Nov-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-322T03:03:00,000T02:52:00,17-Nov-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-322T04:02:00,000T05:58:00,17-Nov-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-322T05:55:00,000T02:49:00,17-Nov-08,CIRS,Prime,rings(general),TDIFS45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-322T05:55:00,000T02:49:00,17-Nov-08,CIRS,SPASS Rider,rings(general),TDIFS45HP,,CIRS_093RI_TDIFS45HP001_SI,,,,,,, 2008-322T05:55:00,000T20:05:00,17-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-322T09:24:00,000T09:00:00,17-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-322T10:00:00,002T03:56:18,17-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-322T10:00:00,001T08:24:00,17-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-322T10:24:00,000T04:00:00,17-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_093IC_DSCAL08322_SP,rider,,,,,, 2008-322T18:24:00,000T02:36:00,17-Nov-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post Backup OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-322T19:04:00,000T08:40:00,17-Nov-08,CIRS,Prime,rings(general),SUBMS30LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-322T19:04:00,000T08:40:00,17-Nov-08,CIRS,SPASS Rider,rings(general),SUBMS30LP,,CIRS_093RI_SUBMS30LP001_SI,,,,,,, 2008-322T21:00:00,000T02:00:00,17-Nov-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,,,,,,, 2008-322T23:00:00,000T19:24:00,17-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-323T02:00:00,000T14:00:00,18-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-323T03:44:00,000T05:00:00,18-Nov-08,VIMS,Prime,Saturn,SPOLEAUR,,South Pole aurora mosaic 3,3x3 North Polar mosaic. 1 sec integration/pixel. Each frame takes approx 70 min.,,,,,, 2008-323T03:44:00,000T05:00:00,18-Nov-08,ISS,SPASS Rider,Saturn,SPOLEAUR,,"Polar movie with the WAC in CB3,MT2,CB2,MT2, BL1","4 pickets spaced 1h 30m. 2x1 WAC in CB3/MT3 (left frame only), CB2/MT2, and BL1.",,,,,, 2008-323T03:44:00,000T05:00:00,18-Nov-08,UVIS,SPASS Rider,Saturn,SPOLEAUR,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2008-323T09:24:00,000T09:00:00,18-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-323T10:24:00,000T04:00:00,18-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_093IC_DSCAL08323_SP,rider,,,,,, 2008-323T10:45:00,001T23:32:00,18-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-323T16:00:00,000T23:00:00,18-Nov-08,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-323T18:24:00,000T20:32:28,18-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-323T18:24:00,000T17:32:28,18-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-323T19:19:00,000T07:37:28,18-Nov-08,VIMS,Prime,Titan,CLOUDMAP,Cloud map,cloud monitoring,Stare at Titan to monitor clouds,,,,,, 2008-323T19:19:00,000T07:37:28,18-Nov-08,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong context imaging),regional map,,,,,, 2008-323T19:19:33,000T07:36:55,18-Nov-08,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Ride along with VIMS.,,,,,, 2008-324T02:56:28,000T04:00:00,19-Nov-08,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Stare at Titan to monitor clouds,,,,,, 2008-324T02:56:28,000T04:00:00,19-Nov-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2008-324T02:56:28,000T04:00:00,19-Nov-08,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T06:56:28,000T01:00:00,19-Nov-08,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2008-324T06:56:28,000T01:00:00,19-Nov-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2008-324T06:56:28,000T01:00:00,19-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with ISS ride-along,,,,,, 2008-324T07:56:28,000T03:00:00,19-Nov-08,VIMS,Prime,Titan,MEDRES,Medium resolution global mapping,Map of Titan,1 Global map with long and short exp. 2 x 2 mosaic of Titan,,,,,, 2008-324T07:56:28,000T03:00:00,19-Nov-08,CIRS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,,Ride along with VIMS.,,,,,, 2008-324T07:56:28,000T03:00:00,19-Nov-08,ISS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T10:56:28,000T03:00:00,19-Nov-08,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping of Titan,"Regional mosaic SouthEast of Xanadu with specific pointing. -Y at different places around (-40,90)",,,,,, 2008-324T10:56:28,000T03:50:00,19-Nov-08,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with VIMS.,,,,,, 2008-324T10:56:28,000T03:00:00,19-Nov-08,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T11:56:28,000T08:00:00,19-Nov-08,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,MAPS_Titan_Flyby,"T047 is a flank-out flyby with a minimum altitude of 1000 km. The geometry of this flyby makes it complementary to T046 in the study of the draping of the external magnetic field around Titan by covering the dayside hemisphere. T047 takes place in Saturn's near-noon sector (10.5 hours SLT), where Titan could be found in the magnetosheath if the solar wind pressure is high. We assign grade one priority.",,,,,, 2008-324T13:56:00,000T01:30:00,19-Nov-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-324T13:56:28,000T01:02:00,19-Nov-08,VIMS,Prime,Titan,HIRES,High resolution image,Regional mapping of Titan,"Regional mosaic SouthEast of Xanadu with specific pointing. -Y at different places around (-40,90)",,,,,, 2008-324T13:56:28,000T01:15:00,19-Nov-08,CAPS,SPASS Rider,Titan,T47INBND,,Inbound 093TI (T47),Inbound leg of a Titan encoun,,,,,, 2008-324T13:56:28,000T01:02:00,19-Nov-08,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T14:46:28,000T00:45:00,19-Nov-08,CIRS,SPASS Rider,Titan,ETAUMA,ETA UMa occultation,,Ride along with UVIS.,,,,,, 2008-324T14:56:28,000T00:40:00,19-Nov-08,INMS,Non-SPASS,Titan,TITAN47,,Titan observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-324T14:58:28,000T00:11:00,19-Nov-08,UVIS,Prime,Star,ETAUMATI,,Titan Occults Eta UMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2008-324T14:58:28,000T00:11:00,19-Nov-08,VIMS,SPASS Rider,Titan,LIMBMAP,Limb map,Map of Titan,Map of Titan's limb prior to C/A with UVIS ride-along,,,,,, 2008-324T15:00:00,000T02:00:00,19-Nov-08,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-324T15:09:28,000T00:01:00,19-Nov-08,UVIS,SPASS Rider,SpacecraftActivity,ORSRCS,,Titan Occults Eta UMa (ENGR Prime minute),UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2008-324T15:09:28,000T00:22:00,19-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Observations during RWA to RCS Transition,,,,,, 2008-324T15:10:28,000T00:21:00,19-Nov-08,UVIS,Prime,Star,ETAUMATI,,Titan Occults Eta UMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2008-324T15:11:28,000T01:30:00,19-Nov-08,CAPS,SPASS Rider,Titan,T47CLOSE,,Closest approach 093TI (T47),Closest approach of a Titan encoun,,,,,, 2008-324T15:26:00,000T01:00:00,19-Nov-08,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2008-324T15:31:28,000T00:49:00,19-Nov-08,VIMS,Prime,Titan,HIRES,High resolution image,Titan landing site,"Noodle scan followed by (64.64) cube of Landing site (-10.4,192.4W) followed by noodle scan (T20-like observations). For the pointing, it means that the primary (-Y) must be such that it points to the landing site when it starts acquiring the cube and then don't move during the noodle acquisition",,,,,, 2008-324T15:31:28,000T00:49:00,19-Nov-08,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with VIMS.,,,,,, 2008-324T15:36:28,000T00:40:00,19-Nov-08,INMS,Non-SPASS,Titan,TITAN47,,Titan observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-324T15:41:28,000T00:39:00,19-Nov-08,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T16:16:28,000T00:40:00,19-Nov-08,INMS,Non-SPASS,Titan,TITAN47,,Titan observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-324T16:20:28,000T00:16:00,19-Nov-08,UVIS,Prime,Star,BETCMATI,,Titan Occults Beta Cma,Egress occultation,,,,,, 2008-324T16:20:28,000T00:38:00,19-Nov-08,CIRS,SPASS Rider,Titan,BETACMA,,,Ride along with UVIS.,,,,,, 2008-324T16:20:28,000T00:38:00,19-Nov-08,VIMS,SPASS Rider,Titan,LIMBMAP,Limb map,Map of Titan,Map of Titan's limb after C/A with UVIS ride-along,,,,,, 2008-324T16:26:00,000T01:30:00,19-Nov-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-324T16:36:28,000T00:22:00,19-Nov-08,UVIS,SPASS Rider,SpacecraftActivity,BETCMATI,,"Titan Occults Beta Cma, ENGR prime part",Egress occultation,,,,,, 2008-324T16:41:28,000T01:15:00,19-Nov-08,CAPS,SPASS Rider,Titan,T47OUTBND,,Outbound 093TI (T47),Outbound leg of a Titan encoun,,,,,, 2008-324T16:56:28,000T02:23:32,19-Nov-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-324T16:58:28,000T01:13:00,19-Nov-08,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2008-324T16:58:28,000T01:13:00,19-Nov-08,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2008-324T16:58:28,000T01:13:00,19-Nov-08,UVIS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,UVIS Rider to CIRS FIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2008-324T16:58:28,000T00:58:00,19-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with CIRS ride-along,,,,,, 2008-324T17:00:00,000T01:00:00,19-Nov-08,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-324T17:56:18,000T16:20:42,19-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-324T17:56:28,000T03:00:00,19-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with CIRS ride-along,,,,,, 2008-324T18:00:00,000T16:17:00,19-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-324T18:11:28,000T02:45:00,19-Nov-08,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2008-324T18:11:28,000T02:45:00,19-Nov-08,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2008-324T18:11:28,000T02:45:00,19-Nov-08,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T19:20:00,000T02:00:00,19-Nov-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-324T19:56:28,001T03:28:32,19-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-324T20:56:28,000T04:00:00,19-Nov-08,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,"Obtain vertical profiles of temperatures at composition in Titan's stratosphere, by integrating on the limb for ~4 hrs at two altitudes with Z perp to limb.",,,,,, 2008-324T20:56:28,000T04:00:00,19-Nov-08,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2008-324T20:56:28,000T04:00:00,19-Nov-08,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong context imaging),regional map,,,,,, 2008-324T20:56:28,000T04:00:00,19-Nov-08,UVIS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,UVIS Rider to CIRS MIRLMBMAP,UVIS Rider to CIRS Mid IR Limb observation,,,,,, 2008-324T20:56:28,000T04:00:00,19-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with CIRS ride-along,,,,,, 2008-324T21:20:00,000T12:57:00,19-Nov-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-325T00:56:28,000T01:00:00,20-Nov-08,ISS,Prime,Titan,PHOTOMWAC,Photometry map,PHW (WAC Photometry),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2008-325T00:56:28,000T01:00:00,20-Nov-08,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS.,,,,,, 2008-325T00:56:28,000T01:00:00,20-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with ISS ride-along,,,,,, 2008-325T01:56:28,000T03:00:00,20-Nov-08,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-325T01:56:28,000T03:00:00,20-Nov-08,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2008-325T01:56:28,000T03:00:00,20-Nov-08,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong context imaging),regional map,,,,,, 2008-325T01:56:28,000T03:00:00,20-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with CIRS ride-along,,,,,, 2008-325T04:56:28,000T01:00:00,20-Nov-08,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NTN(Nightside NAC),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-325T04:56:28,000T01:00:00,20-Nov-08,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with ISS.,,,,,, 2008-325T04:56:28,000T01:00:00,20-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with ISS ride-along,,,,,, 2008-325T05:56:28,000T02:00:00,20-Nov-08,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2008-325T05:56:28,000T02:00:00,20-Nov-08,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2008-325T05:56:28,000T02:00:00,20-Nov-08,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong context imaging),regional map,,,,,, 2008-325T05:56:28,000T02:00:00,20-Nov-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Map of Titan with CIRS ride-along,,,,,, 2008-325T09:25:00,000T09:00:00,20-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-325T10:14:24,000T00:00:01,20-Nov-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 8.0 d, inc = 72.3 deg, r = 20.296 Rs, phase = 25 deg",,,,,, 2008-325T10:17:00,003T12:08:00,20-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-325T10:17:00,003T21:34:59,20-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 4.2814045 Rs exit= 5.3163934 Range altitude= -40603.778 km ... 40176.583,,,,,, 2008-325T10:17:00,000T01:58:00,20-Nov-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-325T10:17:00,001T08:43:00,20-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-325T10:17:00,001T07:43:00,20-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-325T10:17:00,000T08:08:00,20-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-325T10:25:00,000T08:00:00,20-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08325_SP,rider,,,,,, 2008-325T12:15:00,000T02:00:00,20-Nov-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-325T14:15:00,000T09:10:00,20-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-325T18:25:00,000T05:00:00,20-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-325T19:25:00,000T04:00:00,20-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08725_SP,rider,,,,,, 2008-325T23:25:00,003T01:00:00,20-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-325T23:25:00,002T23:00:00,20-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-326T00:05:00,000T08:25:00,21-Nov-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_094SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2008-326T09:10:00,000T09:00:00,21-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-326T10:10:00,000T08:00:00,21-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08326_SP,rider,,,,,, 2008-326T18:10:00,000T23:50:00,21-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-326T18:50:00,000T00:30:00,21-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-326T19:00:00,000T23:10:00,21-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-326T19:20:00,000T02:00:00,21-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-326T21:20:00,000T11:10:00,21-Nov-08,ISS,Prime,RingF,FMOVIE,F ring movie,SHORT HI RES F RING MOVIE,Short hi res F ring stare on day of periapse. Designed to fit into gaps left by other obs. Point to ring radius/longitude and stare for ~2 hrs as material passes through field of view to get ~40 degs of co-rotating longitude,,,,,, 2008-326T21:20:00,000T11:10:00,21-Nov-08,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2008-327T09:10:00,000T09:00:00,22-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-327T09:25:00,000T05:54:00,22-Nov-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-327T10:10:00,000T04:00:00,22-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08327_SP,rider,,,,,, 2008-327T18:00:00,000T21:25:00,22-Nov-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-327T18:10:00,000T21:15:00,22-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-327T19:40:00,000T04:00:00,22-Nov-08,ISS,Prime,rings(general),PHOTDARK,,"high-latitude, dark-face ring photometry","high latitude unlit #2: B ~ 55, phase ~ 60, B = -4.0",,,,,, 2008-327T19:40:00,000T04:00:00,22-Nov-08,CIRS,SPASS Rider,rings(general),PHOTDARK,,CIRS_094RI_PHOTDARK001_ISS,rider,,,,,, 2008-327T19:40:00,000T04:00:00,22-Nov-08,VIMS,SPASS Rider,rings(general),PHOTDARK,,PhotDark mosaic,Main ring photometry,,,,,, 2008-327T23:40:00,000T04:44:00,22-Nov-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. Priority 1. tau=20 msec",,,,,, 2008-327T23:40:00,000T04:44:00,22-Nov-08,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_094RI_GAMCRUOCC009_VIMS,rider,,,,,, 2008-327T23:40:00,000T04:44:00,22-Nov-08,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,URSTAR,,,,,,, 2008-328T04:24:00,000T01:35:00,23-Nov-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-328T04:24:00,000T01:35:00,23-Nov-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_094RF_FMOVIE001_ISS,rider,,,,,, 2008-328T05:59:00,000T08:46:00,23-Nov-08,VIMS,Prime,rings(general),EPSMUSOCC,,Ring stellar occ - epsMus,"B ring, region III; do 2 at priority 1. tau=40 ms",,,,,, 2008-328T05:59:00,000T08:46:00,23-Nov-08,CIRS,SPASS Rider,rings(general),EPSMUSOCC,,CIRS_094RI_EPSMUSOCC201_VIMS,rider,,,,,, 2008-328T05:59:00,000T08:46:00,23-Nov-08,UVIS,SPASS Rider,rings(general),EPSMUSOCC,,URSTAR,,,,,,, 2008-328T15:25:00,000T07:00:00,23-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-328T15:25:00,002T10:15:00,23-Nov-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-328T15:25:00,000T09:00:00,23-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-328T16:25:00,000T04:00:00,23-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08328_SP,rider,,,,,, 2008-328T22:25:00,000T23:00:00,23-Nov-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-328T22:25:00,000T23:00:00,23-Nov-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-328T22:25:00,000T23:00:00,23-Nov-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-328T22:25:00,000T18:00:00,23-Nov-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-329T00:25:00,000T08:05:00,24-Nov-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-329T01:05:00,000T02:00:00,24-Nov-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-329T03:05:00,000T04:25:00,24-Nov-08,CIRS,Prime,rings(general),TDIFN20HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-329T03:05:00,000T04:25:00,24-Nov-08,UVIS,SPASS Rider,rings(general),TDIFN20HP,,URSTAR,,,,,,, 2008-329T07:20:00,000T03:20:00,24-Nov-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-329T07:30:00,000T02:00:00,24-Nov-08,ISS,Prime,Helene,HELENCLOS,,Helene close flyby,observation during flyby of Helene.,,,,,, 2008-329T07:30:00,000T02:00:00,24-Nov-08,UVIS,SPASS Rider,Helene,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-329T07:30:00,000T02:00:00,24-Nov-08,VIMS,SPASS Rider,Helene,HELENCLOS,,Helene C/A,null,,,,,, 2008-329T07:43:29,000T02:00:00,24-Nov-08,CDA,SPASS Rider,DustRAM direction,RPX0130,,CDA RPXing 2008-329T08:43:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-329T07:51:59,000T00:25:00,24-Nov-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.3147839 Rs exit= 5.2799142 Range altitude= 39393.956 km ... 20568.922,,,,,, 2008-329T08:12:00,000T01:00:00,24-Nov-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-329T08:16:59,000T00:51:00,24-Nov-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 5.2786197 Rs exit= 5.2304957 Range altitude= 19783.142 km ... -19543.501,,,,,, 2008-329T08:30:00,000T02:00:00,24-Nov-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-329T09:07:59,000T00:26:00,24-Nov-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.2298703 Rs exit= 5.2185995 Range altitude= -20329.284 km ... -39935.923,,,,,, 2008-329T09:30:00,000T02:00:00,24-Nov-08,ISS,Prime,Tethys,GEOLOG,Geologic study,Tethys lon/phase angle observation,Tethys,,,,,, 2008-329T09:30:00,000T02:00:00,24-Nov-08,CIRS,SPASS Rider,Tethys,GEOLOG,Geologic study,CIRS_094TE_GEOLOG001_ISS,rider,,,,,, 2008-329T09:30:00,000T02:00:00,24-Nov-08,UVIS,SPASS Rider,Tethys,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2008-329T09:30:00,000T02:00:00,24-Nov-08,VIMS,SPASS Rider,Tethys,GEOLOG,Geologic study,mapping cubes,Lat-Long Vgr class,,,,,, 2008-329T09:33:59,002T08:21:01,24-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S46,Range enter= 5.2183240 Rs exit= 5.3162577 Range altitude= -40718.264 km ... 40211.656,,,,,, 2008-329T09:51:14,000T00:00:01,24-Nov-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.213 Rs, lat = -10 deg, phase = 155 deg",,,,,, 2008-329T10:30:00,000T13:55:00,24-Nov-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-329T11:30:00,000T03:15:00,24-Nov-08,CIRS,Prime,rings(general),TDIFS45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-329T11:30:00,000T03:15:00,24-Nov-08,UVIS,SPASS Rider,rings(general),TDIFS45HP,,URSTAR,,,,,,, 2008-329T15:25:00,000T09:00:00,24-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-329T16:25:00,000T04:00:00,24-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08329_SP,rider,,,,,, 2008-329T16:25:00,000T07:00:00,24-Nov-08,RPWS,SPASS Rider,Saturn,RCSWHIST,RPWS lightning search (RCS),non RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-329T21:25:00,001T20:30:00,24-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-329T21:25:00,001T20:30:00,24-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-329T21:25:00,001T03:35:00,24-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-329T23:40:00,000T09:10:00,24-Nov-08,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,Standard calibration/gain,,,,,, 2008-330T00:25:00,001T17:30:00,25-Nov-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post Backup OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-330T01:05:00,000T07:10:00,25-Nov-08,CIRS,Prime,rings(general),TMAPS45LP,,CIRS_094RI_TMAPS45LP001_PRIME;,null,,,,,, 2008-330T01:05:00,000T07:10:00,25-Nov-08,CIRS,SPASS Rider,rings(general),TMAPS45LP,,CIRS_094RI_TMAPS45LP001_SI,,,,,,, 2008-330T01:05:00,000T07:10:00,25-Nov-08,ISS,SPASS Rider,rings(general),TMAPS45LP,,,Spoke periodicity movie. riding along on CIRS TMAP obs.,,,,,, 2008-330T01:05:00,000T07:10:00,25-Nov-08,UVIS,SPASS Rider,rings(general),TMAPS45,,URSTAR,,,,,,, 2008-330T08:55:00,000T09:00:00,25-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-330T09:55:00,000T08:00:00,25-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08330_SP,rider,,,,,, 2008-330T18:35:00,000T01:15:00,25-Nov-08,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 54 range 1.9 Mkm",,,,,, 2008-330T18:35:00,000T01:15:00,25-Nov-08,CIRS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-330T18:35:00,000T01:15:00,25-Nov-08,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-330T19:50:00,000T02:00:00,25-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-330T19:50:00,000T02:00:00,25-Nov-08,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_094RI_SURVEYPTG004_CAPS,rider,,,,,, 2008-330T21:50:00,000T10:25:00,25-Nov-08,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2008-330T21:50:00,000T10:25:00,25-Nov-08,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_094RI_SPKMVLFLP001_ISS,rider,,,,,, 2008-330T21:50:00,000T10:35:00,25-Nov-08,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie - litside,null,,,,,, 2008-331T01:00:00,000T16:55:00,26-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-331T01:40:00,000T16:15:00,26-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-331T08:15:00,000T00:40:00,26-Nov-08,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_094RI_DEEPSPACE331_SP,rider,,,,,, 2008-331T08:55:00,000T09:00:00,26-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-331T09:55:00,000T08:00:00,26-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08331_SP,rider,,,,,, 2008-331T17:55:00,001T15:36:00,26-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-331T17:55:00,001T15:36:00,26-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S S46,Range enter= 5.2183240 Rs exit= 5.3162577 Range altitude= -40718.264 km ... 40211.656,,,,,, 2008-331T17:55:00,000T00:43:00,26-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEQ,,MAPS TOST Campaign,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-331T17:55:00,001T00:00:00,26-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-331T17:55:00,001T15:36:00,26-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-331T17:55:00,001T06:15:00,26-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-331T18:00:00,000T00:02:00,26-Nov-08,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S46 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2008-331T18:38:00,000T00:05:00,26-Nov-08,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-331T18:43:00,000T00:33:00,26-Nov-08,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-331T19:16:00,000T00:22:59,26-Nov-08,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-331T19:38:59,000T22:16:01,26-Nov-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,RINGS_94B,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-331T21:30:00,000T04:05:00,26-Nov-08,ISS,Prime,rings(general),RADMRLPLF,,Color Radial Scan,"Color radial scan, need 1 want 2 out of 5",,,,,, 2008-331T21:30:00,000T04:05:00,26-Nov-08,UVIS,SPASS Rider,rings(general),RADMRLPLF,,URSPEC,,,,,,, 2008-331T21:30:00,000T04:05:00,26-Nov-08,VIMS,SPASS Rider,rings(general),RADMRLPLF,,Color radial scan,Radial scan of rings,,,,,, 2008-332T01:35:00,000T08:30:00,27-Nov-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_094SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2008-332T10:05:00,000T02:00:00,27-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-332T12:05:00,000T00:30:00,27-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-332T12:35:00,000T01:55:00,27-Nov-08,UVIS,Prime,Star,URTHEHYA,URSTAR observation,URSTAR,,,,,,, 2008-332T12:35:00,000T01:55:00,27-Nov-08,UVIS,SPASS Rider,Star,URTHEHYA,URSTAR observation,Support Imaging,NAC support images at the following times: 2008-332T13:15:40.0 2008-332T13:16:24.5 2008-332T13:18:51.0 2008-332T13:41:23.5 2008-332T13:40:41.0 2008-332T13:38:12.9,,,,,, 2008-332T15:10:00,000T09:00:00,27-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-332T16:10:00,000T08:00:00,27-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_094IC_DSCAL08332_SP,rider,,,,,, 2008-332T17:55:00,000T06:15:00,27-Nov-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-332T17:55:00,004T03:45:00,27-Nov-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-333T00:10:00,000T09:21:00,28-Nov-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-333T00:10:00,000T09:21:00,28-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-333T00:50:00,000T01:15:00,28-Nov-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 19.0, range 2.46 Mkm",,,,,, 2008-333T00:50:00,000T01:15:00,28-Nov-08,CIRS,SPASS Rider,Titan,MR3CLD,,CIRS_094TI_MR3CLD333_ISS,rider,,,,,, 2008-333T02:05:00,000T00:30:00,28-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-333T02:35:00,000T05:41:00,28-Nov-08,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2008-333T02:35:00,000T05:41:00,28-Nov-08,CIRS,SPASS Rider,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2008-333T08:56:00,000T09:00:00,28-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-333T09:29:06,000T00:00:01,28-Nov-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 8.0 d, inc = 72.3 deg, r = 20.294 Rs, phase = 25 deg",,,,,, 2008-333T09:31:00,003T12:09:00,28-Nov-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-333T09:31:00,002T08:10:00,28-Nov-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 5.2183240 Rs exit= 5.3162577 Range altitude= -40718.264 km ... 40211.656,,,,,, 2008-333T09:31:00,000T08:25:00,28-Nov-08,INMS,Non-SPASS,Saturn,SURVEYREV,,SATURN_94_95,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-333T09:31:00,001T08:29:00,28-Nov-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-333T09:31:00,002T07:49:00,28-Nov-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-333T09:31:00,000T08:25:00,28-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-333T09:56:00,000T08:00:00,28-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08333_SP,rider,,,,,, 2008-333T17:56:00,000T04:34:00,28-Nov-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-333T18:36:00,000T12:55:00,28-Nov-08,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning N. hemisphere, may be split in half by downlink 1 of 2 acceptable (Rev 97 has identical request)",,,,,, 2008-333T22:30:00,000T02:00:00,28-Nov-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-334T00:30:00,002T23:26:00,29-Nov-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-334T07:31:00,000T00:30:00,29-Nov-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-334T08:41:00,000T09:00:00,29-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-334T09:41:00,000T08:00:00,29-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08334_SP,rider,,,,,, 2008-334T18:00:00,001T20:56:00,29-Nov-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-334T18:21:00,000T02:00:00,29-Nov-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-334T20:21:00,000T11:40:00,29-Nov-08,UVIS,Prime,Saturn,NPOLEAUR,,Saturn Aurora,Rider on VIMS NPOLEAUR observations,,,,,, 2008-334T20:21:00,000T11:40:00,29-Nov-08,ISS,SPASS Rider,Saturn,NPOLEAUR,,"Polar movie with the WAC in MT2,CB2,MT2, BL1","7 pickets spaced 1h 30m. 2x1 WAC in MT3, CB2, MT2, and BL1.",,,,,, 2008-334T20:21:00,000T11:40:00,29-Nov-08,VIMS,SPASS Rider,Saturn,NPOLEAUR,,North Pole aurora mosaic 1,Aurora ridealong with UVIS,,,,,, 2008-335T08:41:00,000T09:00:00,30-Nov-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-335T08:56:00,000T06:34:00,30-Nov-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-335T09:41:00,000T08:00:00,30-Nov-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08335_SP,rider,,,,,, 2008-335T09:41:00,000T07:00:00,30-Nov-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-335T17:20:00,003T07:40:00,30-Nov-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-335T17:41:00,001T06:19:00,30-Nov-08,CDA,Non-SPASS,Other,RATE010A,,Data rate Enter:SApo,Range enter= 5.2183240 Rs exit= 5.3162577 Range altitude= -40718.264 km ... 40211.656,,,,,, 2008-335T19:11:00,000T13:05:00,30-Nov-08,VIMS,Prime,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,North Pole dynamics mosaic 1,"3x3 North Polar mosaic. Imaging on 10-min centers, with 7 mins for observing and 3 minutes for repositioning",,,,,, 2008-335T19:11:00,000T13:05:00,30-Nov-08,ISS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,"Polar movie with the WAC in MT2,CB2,MT2, BL1","9 pickets spaced 1h 30m. 2x1 WAC in MT3, CB2, MT2, and BL1.",,,,,, 2008-335T19:11:00,000T13:05:00,30-Nov-08,UVIS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Saturn Aurora,Rider on VIMS NPOLEDYN observations,,,,,, 2008-336T05:16:00,000T03:00:00,1-Dec-08,RADAR,SPASS Rider,Other,WU4NRPOL,,Warmup for Saturn North Pole Map,Warmup for north pole map.,,,,,, 2008-336T08:16:00,000T06:00:00,1-Dec-08,RADAR,Prime,Saturn,NORTHPOL,,Saturn North Pole Map,map north pole; coordinated with VIMS.,,,,,, 2008-336T14:56:00,000T06:44:00,1-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-336T14:56:00,000T09:00:00,1-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-336T15:56:00,000T04:00:00,1-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08336_SP,rider,,,,,, 2008-336T21:40:00,000T00:45:00,1-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-336T21:40:00,000T23:00:00,1-Dec-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-336T21:40:00,000T23:00:00,1-Dec-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-336T21:40:00,000T18:16:00,1-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-336T22:25:00,000T05:35:00,1-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-336T23:56:00,000T08:04:00,1-Dec-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-337T00:00:00,000T07:06:59,2-Dec-08,CDA,Non-SPASS,Other,RATE010B,,Data rate Enter:SApo,Range enter= 5.2183240 Rs exit= 5.3162577 Range altitude= -40718.264 km ... 40211.656,,,,,, 2008-337T00:36:00,000T03:24:00,2-Dec-08,CAPS,Prime,Saturn,AURXNGPTG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Prime pointing during AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-337T04:00:00,000T02:30:00,2-Dec-08,ISS,Prime,Enceladus,GEOLOG,Geologic study,Enceladus observation,Enceladus observation,,,,,, 2008-337T04:00:00,000T07:30:00,2-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-337T04:00:00,000T02:30:00,2-Dec-08,CIRS,SPASS Rider,Enceladus,GEOLOG,Geologic study,CIRS_095EN_GEOLOG001_ISS,rider,,,,,, 2008-337T04:00:00,000T02:30:00,2-Dec-08,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-337T04:00:00,000T02:30:00,2-Dec-08,VIMS,SPASS Rider,Enceladus,GEOLOG,Geologic study,mapping cubes,Lat-Long Vgr class,,,,,, 2008-337T06:30:00,000T03:00:00,2-Dec-08,CDA,Prime,DustRAM direction,RPX0140,,CDA RPXing 2008-337T07:58:29 MMH,"must must have, vertical crossing",,,,,, 2008-337T06:35:00,000T03:20:00,2-Dec-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-337T06:50:00,000T02:00:00,2-Dec-08,VIMS,SPASS Rider,Calypso,ROTCOLR,,Calypso,multiple 16/640 ms.,,,,,, 2008-337T07:06:59,000T00:25:00,2-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.3146481 Rs exit= 5.2797768 Range altitude= 39429.041 km ... 20604.267,,,,,, 2008-337T07:27:00,000T01:00:00,2-Dec-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-337T07:31:59,000T00:51:00,2-Dec-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 5.2784823 Rs exit= 5.2303606 Range altitude= 19818.497 km ... -19507.861,,,,,, 2008-337T08:00:00,000T02:00:00,2-Dec-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-337T08:22:59,000T00:26:00,2-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.2297353 Rs exit= 5.2184690 Range altitude= -20293.645 km ... -39900.368,,,,,, 2008-337T08:48:59,000T02:11:01,2-Dec-08,CDA,Non-SPASS,Other,RATE010A,,Data rate End:SApo,Range enter= 5.2181937 Rs exit= 5.7969554 Range altitude= -40682.716 km ... 40468.733,,,,,, 2008-337T09:06:50,000T00:00:01,2-Dec-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.213 Rs, lat = -10 deg, phase = 155 deg",,,,,, 2008-337T09:30:00,000T04:46:00,2-Dec-08,ISS,Prime,Saturn,AURMOV,Saturn aurora movie,Auroral WAC 2X2 movie + lightning search,"Auroral WAC movie. pickets in a 1x2 mosaic in clear, HAL and IR2 filters. Space pickets one hour apart.",,,,,, 2008-337T09:30:00,000T04:46:00,2-Dec-08,UVIS,SPASS Rider,Saturn,AURMOV,Saturn aurora movie,Saturn Aurora,Rider on ISS AURMOV observations,,,,,, 2008-337T10:00:00,000T13:56:00,2-Dec-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-337T11:00:00,000T21:26:00,2-Dec-08,CDA,Non-SPASS,Other,RATE010B,,Data rate End:SApo,Range enter= 5.2181937 Rs exit= 5.7969554 Range altitude= -40682.716 km ... 40468.733,,,,,, 2008-337T11:30:00,000T05:00:00,2-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-337T14:56:00,000T09:00:00,2-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-337T15:56:00,000T08:00:00,2-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08337_SP,rider,,,,,, 2008-337T15:56:00,000T07:00:00,2-Dec-08,RPWS,SPASS Rider,Saturn,RCSWHIST,RPWS lightning search (RCS),non RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-337T16:30:00,000T04:10:00,2-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-337T20:40:00,002T15:45:35,2-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-337T20:40:00,001T07:21:00,2-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-337T20:40:00,001T03:20:00,2-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-337T23:56:00,000T03:00:00,2-Dec-08,RADAR,SPASS Rider,Other,WU4SOPOL,,Warmup for Saturn South Pole Map,Warmup for south pole map.,,,,,, 2008-337T23:56:00,001T17:30:00,2-Dec-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-338T00:36:00,000T02:20:00,3-Dec-08,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics mosaic 1,"3x3 South Polar mosaic. Frames taken on 10 minute centers, 7 minutes for observing and 3 minutes for repositioning",,,,,, 2008-338T00:36:00,000T02:20:00,3-Dec-08,ISS,SPASS Rider,Saturn,SPOLEDYN,,"Polar movie with the WAC in MT2,CB2,MT2, BL1","2 pickets spaced 1h 30m. 2x1 WAC in MT3, CB2, MT2, and BL1.",,,,,, 2008-338T00:36:00,000T02:20:00,3-Dec-08,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2008-338T02:56:00,000T04:50:00,3-Dec-08,RADAR,Prime,Saturn,SOUTHPOL,,Saturn South Pole Map,map south pole; coordinated with VIMS.,,,,,, 2008-338T08:26:00,002T09:55:00,3-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 5.2181937 Rs exit= 5.7969554 Range altitude= -40682.716 km ... 40468.733,,,,,, 2008-338T08:26:00,000T09:00:00,3-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-338T09:26:00,000T08:00:00,3-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08338_SP,rider,,,,,, 2008-338T18:06:00,000T08:40:00,3-Dec-08,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics mosaic 2,"3x3 South Polar mosaic. Frames taken on 10 minute centers, 7 minutes for observing and 3 minutes for repositioning",,,,,, 2008-338T18:06:00,000T08:40:00,3-Dec-08,CIRS,SPASS Rider,Saturn,SPOLEDYN,,CIRS_095SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2008-338T18:06:00,000T08:40:00,3-Dec-08,ISS,SPASS Rider,Saturn,SPOLEDYN,,"Polar movie with the WAC in MT2,CB2,MT2, BL1","4 pickets spaced 1h 30m. 2x1 WAC in MT3, CB2, MT2, and BL1.",,,,,, 2008-338T18:06:00,000T08:40:00,3-Dec-08,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2008-339T00:00:00,001T12:25:00,4-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-339T01:00:00,000T16:26:00,4-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-339T02:46:00,000T01:15:00,4-Dec-08,ISS,Prime,Titan,MR1CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 81.1, range 0.71 Mkm",,,,,, 2008-339T02:46:00,000T01:15:00,4-Dec-08,CIRS,SPASS Rider,Titan,MR1CLDF,,CIRS_095TI_MR1CLDF338_ISS,rider,,,,,, 2008-339T04:01:00,000T06:45:00,4-Dec-08,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-339T10:46:00,000T06:40:00,4-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-339T11:26:00,000T06:00:00,4-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-339T12:11:00,000T05:15:00,4-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_095IC_DSCAL08339_SP,rider,,,,,, 2008-339T17:26:00,000T19:59:45,4-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-339T17:26:00,000T16:59:45,4-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-339T17:26:00,001T00:55:00,4-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-339T18:21:33,000T07:04:12,4-Dec-08,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Map of Titan,Global mapping of Titan,,,,,, 2008-339T18:21:33,000T07:04:12,4-Dec-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2008-339T18:25:45,000T07:00:00,4-Dec-08,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong context imaging),regional map,,,,,, 2008-340T01:25:45,000T04:00:00,5-Dec-08,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-340T01:25:45,000T04:00:00,5-Dec-08,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2008-340T01:25:45,000T04:00:00,5-Dec-08,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong context imaging),regional map,,,,,, 2008-340T01:25:45,000T04:00:00,5-Dec-08,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2008-340T01:25:45,000T04:00:00,5-Dec-08,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far IR Nadir comp.,VIMS ridealong with CIRS,,,,,, 2008-340T05:10:45,000T08:25:00,5-Dec-08,RADAR,SPASS Rider,Titan,T48WARMUP,,Warmup for T48,Warmup for T48.,,,,,, 2008-340T05:25:45,000T04:00:00,5-Dec-08,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2008-340T05:25:45,000T04:00:00,5-Dec-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2008-340T05:25:45,000T04:00:00,5-Dec-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global and cloud mapping,VIMS ridealong with ISS for global and cloud mapping. One cube every 30 min.,,,,,, 2008-340T09:25:45,000T02:00:00,5-Dec-08,ISS,Prime,Titan,REGMAP,Regional mapping,NAC Regional Map,regional map,,,,,, 2008-340T09:25:45,000T02:00:00,5-Dec-08,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS.,,,,,, 2008-340T09:25:45,000T02:00:00,5-Dec-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Cloud and global mapping,VIMS ridealong with ISS for global and cloud mapping. One cube every 20 min.,,,,,, 2008-340T10:25:45,000T08:00:00,5-Dec-08,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,MAPS_Titan_Flyby,"T048 is very similar to T047, with a minimum altitude of 1000 km. Therefore, we will be able to look for temporal effects in response to changes in the upstream conditions (i.e. the flyby occurring at a different SKR phase). T048 also takes place in Saturn's near-noon sector (10.5 hours SLT), where Titan could be found in the magnetosheath if the solar wind pressure is high. We assign grade one priority.",,,,,, 2008-340T11:25:45,000T01:00:00,5-Dec-08,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2008-340T11:25:45,000T01:00:00,5-Dec-08,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2008-340T11:25:45,000T01:00:00,5-Dec-08,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong context imaging),regional map,,,,,, 2008-340T11:25:45,000T01:00:00,5-Dec-08,UVIS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,UVIS Rider to CIRS FIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2008-340T11:25:45,000T01:00:00,5-Dec-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,VIMS ridealong with CIRS,,,,,, 2008-340T12:25:00,000T01:00:00,5-Dec-08,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-340T12:25:00,000T01:30:00,5-Dec-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-340T12:25:45,000T00:48:00,5-Dec-08,ISS,Prime,Titan,HIGHRES,High resolution observartion,NHR (NAC High Resolution),regional map,,,,,, 2008-340T12:25:45,000T01:00:00,5-Dec-08,CAPS,SPASS Rider,Titan,T48INBND,,Inbound 095TI (T48),Inbound leg of a Titan encoun,,,,,, 2008-340T12:25:45,000T01:10:00,5-Dec-08,CIRS,SPASS Rider,Titan,HIGHRES,High resolution observartion,,Ride along with ISS.,,,,,, 2008-340T12:25:45,000T00:48:00,5-Dec-08,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping,VIMS ridealong with ISS. VIMS acquires 8 cubes with 6-min dwell times within the observing period.,,,,,, 2008-340T13:07:45,000T02:36:00,5-Dec-08,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2008-340T13:14:45,000T00:21:00,5-Dec-08,ISS,Prime,Titan,TRNSITION,,(TNI) Transition NAC Imaging,viewing during RCS/RWA transition,,,,,, 2008-340T13:25:00,000T02:00:00,5-Dec-08,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-340T13:25:45,000T02:00:00,5-Dec-08,CAPS,SPASS Rider,Titan,T48CLOSE,,Closest approach 095TI (T48),Closest approach of a Titan encoun,,,,,, 2008-340T13:25:45,000T00:54:00,5-Dec-08,INMS,Non-SPASS,Titan,TITAN48,,Titan Flyby,Titan observation,,,,,, 2008-340T13:35:45,000T00:20:00,5-Dec-08,RADAR,Prime,Titan,T48IHISAR,,T48 Inbound HiSAR,,,,,,, 2008-340T13:55:45,000T00:12:00,5-Dec-08,RADAR,Prime,Titan,T48INALT,,T48 Inbound Altimetry,,,,,,, 2008-340T14:07:45,000T00:13:00,5-Dec-08,RADAR,Prime,Titan,T48INSAR,,T48 Inbound SAR for Tui Regio,,,,,,, 2008-340T14:19:45,000T00:21:00,5-Dec-08,INMS,Non-SPASS,Titan,TITAN48,,Titan Flyby,Prime Titan observation,,,,,, 2008-340T14:20:45,000T00:27:00,5-Dec-08,RADAR,Prime,Titan,T48RASAR,,T48 Ride-along SAR with INMS,,,,,,, 2008-340T14:40:45,000T00:45:00,5-Dec-08,INMS,Non-SPASS,Titan,TITAN48,,Titan Flyby,Titan observation,,,,,, 2008-340T14:47:45,000T00:33:00,5-Dec-08,CIRS,SPASS Rider,Star,EPSCMATI,,,Ride along with SP/UVIS/ENGR,,,,,, 2008-340T14:47:45,000T00:21:04,5-Dec-08,UVIS,SPASS Rider,SpacecraftActivity,DFPWBIAS,,Rider during RCS -> RWA transition (eps cma occ.),UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates. Duration includes half hour turns on each end.,,,,,, 2008-340T14:55:00,000T01:30:00,5-Dec-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-340T15:08:49,000T00:11:56,5-Dec-08,UVIS,Prime,Star,EPSCMATI,,Titan Occults Eps CMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates. Duration includes half hour turns on each end.,,,,,, 2008-340T15:08:49,000T00:11:56,5-Dec-08,VIMS,SPASS Rider,Titan,LMBMAP,,Limb map during stellar occultation,VIMS ridealong with UVIS during stellar occulation. Note: time occurs during RCS/RWA turn.,,,,,, 2008-340T15:20:45,000T01:20:00,5-Dec-08,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2008-340T15:20:45,000T01:20:00,5-Dec-08,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2008-340T15:25:00,000T01:00:00,5-Dec-08,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-340T15:25:45,000T01:00:00,5-Dec-08,CAPS,SPASS Rider,Titan,T48OUTBND,,Outbound 095TI (T48),Outbound leg of a Titan encoun,,,,,, 2008-340T15:25:45,000T01:15:00,5-Dec-08,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong context imaging),regional map,,,,,, 2008-340T15:25:45,000T01:15:00,5-Dec-08,UVIS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,UVIS Rider to CIRS FIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2008-340T15:25:45,000T01:15:00,5-Dec-08,VIMS,SPASS Rider,Titan,LMBMAP,,LIMB mapping,VIMS ridealong with CIRS during limb integration.,,,,,, 2008-340T15:25:45,000T02:56:15,5-Dec-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-340T16:25:00,000T01:57:00,5-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-340T16:25:35,000T01:56:25,5-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-340T16:40:45,000T06:45:00,5-Dec-08,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2008-340T16:40:45,000T06:45:00,5-Dec-08,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS EUV-FUV scan,,,,,, 2008-340T16:40:45,000T06:45:00,5-Dec-08,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong context imaging),regional map,,,,,, 2008-340T16:40:45,000T06:45:00,5-Dec-08,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Limb map of Titan,VIMS ridealong with UVIS,,,,,, 2008-340T18:19:47,000T00:00:01,5-Dec-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 8.0 d, inc = 73.1 deg, r = 19.778 Rs, phase = 24 deg",,,,,, 2008-340T18:21:00,003T22:37:59,5-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 5.2181937 Rs exit= 5.7969554 Range altitude= -40682.716 km ... 40468.733,,,,,, 2008-340T18:21:00,002T05:39:00,5-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-340T18:22:00,003T12:48:00,5-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-340T18:22:00,000T02:00:00,5-Dec-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-340T18:22:00,000T14:05:00,5-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-340T18:25:45,001T03:01:15,5-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-340T20:22:00,001T01:05:00,5-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-340T23:25:45,000T04:00:00,5-Dec-08,VIMS,Prime,Titan,CLOUDMAP,Cloud map,Map of Titan,Global mapping of Titan,,,,,, 2008-340T23:25:45,000T04:00:00,5-Dec-08,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride along with VIMS.,,,,,, 2008-340T23:25:45,000T04:00:00,5-Dec-08,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong context imaging),regional map,,,,,, 2008-341T03:25:45,000T01:00:00,6-Dec-08,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Night NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2008-341T03:25:45,000T01:00:00,6-Dec-08,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with ISS.,,,,,, 2008-341T03:25:45,000T01:00:00,6-Dec-08,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Cloud and global mapping. Stare at Titan.,VIMS ridealong with ISS for global mapping.,,,,,, 2008-341T04:25:45,000T03:06:48,6-Dec-08,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2008-341T04:25:45,000T03:06:48,6-Dec-08,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (7 integrations total = 14 frames, 0.5 Mb/frame)",,,,,, 2008-341T04:25:45,000T03:00:00,6-Dec-08,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong context imaging),regional map,,,,,, 2008-341T04:25:45,000T03:06:48,6-Dec-08,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp Map,VIMS ridealong with CIRS,,,,,, 2008-341T08:27:00,000T05:58:00,6-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-341T09:27:00,000T08:00:00,6-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08341_SP,rider,,,,,, 2008-341T14:25:00,000T20:35:00,6-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-341T17:27:00,000T04:00:00,6-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-341T18:27:00,000T03:00:00,6-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08741_SP,rider,,,,,, 2008-341T21:27:00,002T10:33:00,6-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-341T21:27:00,002T09:43:00,6-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-341T22:07:00,000T06:55:00,6-Dec-08,CIRS,Prime,rings(general),TMAPN20LP,,CIRS_096RI_TMAPN20LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-341T22:07:00,000T06:55:00,6-Dec-08,CIRS,SPASS Rider,rings(general),TMAPN20LP,,CIRS_096RI_TMAPN20LP001_SI,,,,,,, 2008-341T22:07:00,000T06:55:00,6-Dec-08,ISS,SPASS Rider,rings(general),TMAPN20LP,,Spoke Periodicity Monitoring,One WAC every 20 minutes to look for spokes,,,,,, 2008-341T22:07:00,000T06:55:00,6-Dec-08,UVIS,SPASS Rider,rings(general),TMAPN20LP,,,,,,,,, 2008-342T05:02:00,000T02:00:00,7-Dec-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-342T07:02:00,000T00:30:00,7-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-342T08:12:00,000T09:00:00,7-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-342T09:12:00,000T08:00:00,7-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08342_SP,rider,,,,,, 2008-342T11:00:00,001T20:10:00,7-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-342T17:52:00,000T05:20:00,7-Dec-08,CIRS,Prime,rings(general),TMAPN45LP,,CIRS_096RI_TMAPN45LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-342T17:52:00,000T05:20:00,7-Dec-08,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_096RI_TMAPN45LP001_SI,,,,,,, 2008-342T17:52:00,000T05:20:00,7-Dec-08,UVIS,SPASS Rider,rings(general),TMAPN45LP,,,,,,,,, 2008-342T17:52:00,000T05:20:00,7-Dec-08,VIMS,SPASS Rider,rings(general),TMAPN45LP,,VIMS rider on CIMS,VIMS ridealong with CIRS,,,,,, 2008-342T23:12:00,000T01:29:00,7-Dec-08,CIRS,SPASS Rider,rings(general),OPNAV,Optical navigation image,CIRS_096RI_OPNAV421_NAV,rider,,,,,, 2008-343T00:00:00,003T12:00:00,8-Dec-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-343T00:42:00,000T09:00:00,8-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-343T01:42:00,000T08:00:00,8-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08343_SP,rider,,,,,, 2008-343T10:08:00,000T04:28:00,8-Dec-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. Priority 1., tau=20 ms",,,,,, 2008-343T10:08:00,000T04:28:00,8-Dec-08,UVIS,SPASS Rider,Star,GAMCRUOCC,Gamma Cru occultation,URSTAR,,,,,,, 2008-343T14:36:00,000T01:33:00,8-Dec-08,ISS,Prime,rings(general),RETARMRMP,,Medium res retargetables,Medium Res Retarg of small ring region satellites.,,,,,, 2008-343T14:36:00,000T01:33:00,8-Dec-08,CIRS,SPASS Rider,rings(general),HRRETARG,,CIRS_096RI_HRRETARG001_ISS,rider,,,,,, 2008-343T16:09:00,000T05:00:00,8-Dec-08,UVIS,Prime,Star,URBETCEN,Stellar occultation,URSTAR,,,,,,, 2008-343T16:09:00,000T05:00:00,8-Dec-08,ISS,SPASS Rider,Star,URBETCEN,Stellar occultation,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2008-343T16:09:00,000T05:00:00,8-Dec-08,UVIS,SPASS Rider,Star,URBETCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2008-343T16:57:25.0 2008-343T17:09:22.5 2008-343T17:47:40.0,,,,,, 2008-343T21:09:00,000T07:22:00,8-Dec-08,ISS,Prime,RingF,FRINGHRDF,,High Resolution F Ring Scan,Complete high resolution (0-10Rs) longitudinal scan of the F ring. Dark face. Need at least 3 during XM. 2 of 27 as priority 1 and 1 as priority 2.,,,,,, 2008-343T21:09:00,000T07:22:00,8-Dec-08,CIRS,SPASS Rider,RingF,FRINGHRDF,,CIRS_096RF_FRINGHRDF001_ISS,rider,,,,,, 2008-344T04:31:00,000T06:08:00,9-Dec-08,UVIS,Prime,Star,URALPARA,Alpha Ara occultation,URSTAR,,,,,,, 2008-344T04:31:00,000T06:08:00,9-Dec-08,UVIS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Support Imaging,NAC support images at the following times: 2008-344T05:17:30 2008-344T05:31:07 2008-344T09:38:10 2008-344T09:52:37,,,,,, 2008-344T07:10:00,000T04:50:00,9-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-344T07:10:00,000T21:55:00,9-Dec-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-344T07:10:00,000T21:55:00,9-Dec-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-344T07:10:00,000T08:50:00,9-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-344T08:00:00,000T02:00:00,9-Dec-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,,,,,,, 2008-344T10:00:00,000T13:27:00,9-Dec-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-344T10:39:00,000T01:22:00,9-Dec-08,VIMS,Prime,rings(general),SPOKE,Ring spoke movie,Spoke observation,null,,,,,, 2008-344T10:39:00,000T01:22:00,9-Dec-08,CIRS,SPASS Rider,rings(general),SPOKE,Ring spoke movie,CIRS_096RI_SPOKE105_VIMS,rider,,,,,, 2008-344T10:39:00,000T01:22:00,9-Dec-08,ISS,SPASS Rider,rings(general),SPOKE,Ring spoke movie,spoke observation,"VIMS rider, searching for spokes",,,,,, 2008-344T10:39:00,000T01:22:00,9-Dec-08,UVIS,SPASS Rider,rings(general),SPOKE,Ring spoke movie,,,,,,,, 2008-344T12:00:00,000T11:30:00,9-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-344T12:01:00,000T01:54:00,9-Dec-08,CIRS,Prime,Tethys,SECLNX,,CIRS_096TE_SECLXN001_PRIME,"10 minute turn; Single 5 mrad FP3 scan from 1 mrad off bright limb at 4 urad/sec (21 min.); deep space reference 10 mrad off limb (10 min); FP1 stare at (50, 335) for eclipse entry; 10 minute return to waypoint. Entry at 2008-344t13:01:55. 15.5 cm-1, blink, shutter closed first and last 3 min. 4.1-4.7 mrad, 83-87 phase, (68, 280)-(47, 276), LT~17. 2 WAC support images.",,,,,, 2008-344T12:01:00,000T01:54:00,9-Dec-08,CIRS,SPASS Rider,Tethys,FP1SECLN,CIRS elipse observation,CIRS_096TE_FP1SECLN001_SI,"2 WAC support images: one at 344T12:55 (sunlight), one at 344T13:35 (grey light)",,,,,, 2008-344T12:01:00,000T01:54:00,9-Dec-08,ISS,SPASS Rider,Tethys,SECLNX,,Tethys eclipse,Tethys eclipse,,,,,, 2008-344T12:01:00,000T01:54:00,9-Dec-08,UVIS,SPASS Rider,Tethys,ICYECL,,ICYECL: observe satellite in eclipse,,,,,,, 2008-344T12:01:00,000T01:54:00,9-Dec-08,VIMS,SPASS Rider,Tethys,ECLIPSE,,spectral cubes,eclipse,,,,,, 2008-344T14:27:00,000T09:00:00,9-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-344T15:27:00,000T08:00:00,9-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08344_SP,rider,,,,,, 2008-344T16:00:00,000T01:32:00,9-Dec-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-344T16:53:29,000T02:00:00,9-Dec-08,CDA,SPASS Rider,DustRAM direction,RPX0150,,CDA RPXing 2008-344T17:53:29 MH,Must Have - variation of angular distance to source (longitude),,,,,, 2008-344T16:58:59,000T00:27:00,9-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.7962290 Rs exit= 5.7808875 Range altitude= 39726.913 km ... 20401.701,,,,,, 2008-344T17:25:59,000T00:54:00,9-Dec-08,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 5.7804345 Rs exit= 5.7710708 Range altitude= 19657.265 km ... -19829.128,,,,,, 2008-344T17:32:00,000T01:00:00,9-Dec-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-344T18:07:23,000T00:00:01,9-Dec-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.765 Rs, lat = -2 deg, phase = 155 deg",,,,,, 2008-344T18:19:59,000T00:27:00,9-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.7711713 Rs exit= 5.7773831 Range altitude= -20573.546 km ... -39897.889,,,,,, 2008-344T18:32:00,000T03:55:00,9-Dec-08,RPWS,Non-SPASS,co-rotation,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-344T18:46:59,003T23:01:01,9-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 5.7777602 Rs exit= 5.7964971 Range altitude= -40639.656 km ... 40126.995,,,,,, 2008-344T22:27:00,000T06:38:00,9-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-344T23:27:00,000T17:45:00,9-Dec-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-344T23:30:00,000T05:35:00,9-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-344T23:52:00,000T01:15:00,9-Dec-08,VIMS,Prime,rings(general),HIRESHIPH,,Ring HIRESHIPH,Do 4 at priority 1.,,,,,, 2008-344T23:52:00,000T01:15:00,9-Dec-08,CIRS,SPASS Rider,rings(general),HIRESHIPH,,CIRS_096RI_HIRESHIPH101_VIMS,rider,,,,,, 2008-344T23:52:00,000T01:15:00,9-Dec-08,UVIS,SPASS Rider,rings(general),HIRESHIPH,,,,,,,,, 2008-345T01:07:00,000T06:35:00,10-Dec-08,ISS,Prime,rings(general),AZSCANLIT,,AZSCAN lit,AZSCAN 1.470 Rs ringlet,,,,,, 2008-345T01:07:00,000T06:35:00,10-Dec-08,CIRS,SPASS Rider,rings(general),AZSCANLIT,,CIRS_096RI_AZSCANLIT001_ISS,rider,,,,,, 2008-345T05:05:00,003T12:44:00,10-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-345T05:05:00,003T11:53:00,10-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-345T05:05:00,000T12:07:00,10-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-345T08:12:00,000T09:00:00,10-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-345T09:12:00,000T08:00:00,10-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08345_SP,rider,,,,,, 2008-345T17:12:00,002T23:46:00,10-Dec-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-345T17:12:00,001T03:48:00,10-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-345T17:52:00,000T12:55:00,10-Dec-08,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2008-345T17:52:00,000T12:55:00,10-Dec-08,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_096RF_FMOVIE004_ISS,rider,,,,,, 2008-345T17:52:00,000T12:55:00,10-Dec-08,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2008-346T06:47:00,000T00:30:00,11-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-346T07:57:00,000T09:00:00,11-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-346T08:12:00,000T05:00:00,11-Dec-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-346T08:57:00,000T08:00:00,11-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08346_SP,rider,,,,,, 2008-346T10:00:00,000T02:16:32,11-Dec-08,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,MAPS Survey,MAPS magn,,,,,, 2008-346T12:00:00,001T04:57:00,11-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-346T17:37:00,000T05:10:00,11-Dec-08,ISS,Prime,rings(general),SPKFMLFLP,,Lit Face Low Phase Spoke Formation Movie,Spoke Movie to observe formation,,,,,, 2008-346T17:37:00,000T05:10:00,11-Dec-08,VIMS,SPASS Rider,rings(general),SPKFMLFLP,,VIMS rider on ISS,VIMS rider on ISS spoke observation,,,,,, 2008-346T21:00:00,000T19:57:00,11-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-346T22:47:00,000T00:30:00,11-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-346T23:17:00,000T08:00:00,11-Dec-08,VIMS,Prime,rings(general),APOMOSL,,"Apoapse mosaic, lit side",Do 9 lit side at priority 2 (~every third orbit),,,,,, 2008-346T23:17:00,000T08:00:00,11-Dec-08,CIRS,SPASS Rider,rings(general),APOMOSL,,CIRS_096RI_APOMOSL114_VIMS,rider,,,,,, 2008-346T23:17:00,000T08:00:00,11-Dec-08,UVIS,SPASS Rider,rings(general),APOMOSL,,,,,,,,, 2008-347T00:00:00,000T00:34:08,12-Dec-08,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2008-347T07:57:00,000T09:00:00,12-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-347T08:57:00,000T08:00:00,12-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08347_SP,rider,,,,,, 2008-347T16:57:00,001T00:52:00,12-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-347T16:57:00,001T00:51:00,12-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-347T17:37:00,000T01:15:00,12-Dec-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 22.1 range 2.45 Mkm",,,,,, 2008-347T17:37:00,000T01:15:00,12-Dec-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-347T18:52:00,000T08:00:00,12-Dec-08,CIRS,Prime,rings(general),SUBMS10LP,,CIRS_096RI_SUBMS10LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-347T18:52:00,000T08:00:00,12-Dec-08,CIRS,SPASS Rider,rings(general),SUBMS10LP,,CIRS_096RI_SUBMS10LP001_SI,,,,,,, 2008-347T18:52:00,000T08:00:00,12-Dec-08,ISS,SPASS Rider,rings(general),SUBMS10LP,,,Spoke periodicity movie. riding along on CIRS SUBM obs.,,,,,, 2008-347T18:52:00,000T08:00:00,12-Dec-08,UVIS,SPASS Rider,rings(general),SUBMS10LP,,,,,,,,, 2008-347T18:52:00,000T08:00:00,12-Dec-08,VIMS,SPASS Rider,rings(general),SUBMS10LP,,VIMS rider on CIRS,VIMS ridealong with CIRS,,,,,, 2008-348T02:52:00,000T00:30:00,13-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-348T03:22:00,000T02:00:00,13-Dec-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-348T03:22:00,000T02:00:00,13-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,SURVEYPTG,MAPS survey/Prime pointing,CIRS_096IC_SURVEYPTG004_CAPS,rider,,,,,, 2008-348T05:22:00,000T03:00:00,13-Dec-08,ISS,Prime,rings(general),FMONITOR,F ring monitor,F RING TEMPORAL MONITORING,Long term temporal monitoring of F ring. Observation in collaboration with Jeff Cuzzi. The time isn't critical so the obs can be put anywhere in the same ~14 hr period between downlinks.,,,,,, 2008-348T05:22:00,000T03:00:00,13-Dec-08,CIRS,SPASS Rider,rings(general),FMONITOR,F ring monitor,CIRS_096RI_FMONITOR002_ISS,rider,,,,,, 2008-348T05:22:00,000T03:00:00,13-Dec-08,VIMS,SPASS Rider,rings(general),FMONITOR,F ring monitor,FMONITOR,F ring observation,,,,,, 2008-348T08:22:00,000T00:30:00,13-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-348T08:52:00,000T04:06:00,13-Dec-08,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2008-348T08:52:00,000T04:06:00,13-Dec-08,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2008-348T14:13:00,000T09:00:00,13-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-348T15:13:00,000T08:00:00,13-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_096IC_DSCAL08348_SP,rider,,,,,, 2008-348T16:58:00,000T06:15:00,13-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-348T16:58:00,003T13:32:00,13-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-348T17:46:19,000T00:00:01,13-Dec-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 8.0 d, inc = 72.9 deg, r = 19.746 Rs, phase = 25 deg",,,,,, 2008-348T17:48:00,003T22:29:59,13-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 5.7777602 Rs exit= 5.7964971 Range altitude= -40639.656 km ... 40126.995,,,,,, 2008-348T17:48:00,002T05:52:00,13-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-348T17:49:00,003T12:41:00,13-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-348T17:49:00,001T16:41:00,13-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-348T23:13:00,000T17:45:00,13-Dec-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-348T23:53:00,000T07:25:00,13-Dec-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_097SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern or Northern hemisphere",,,,,, 2008-348T23:53:00,000T07:25:00,13-Dec-08,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Redealong,CIRS Compsit Ridealong. Watch Saturn rotate underneath,,,,,, 2008-349T07:58:00,000T09:00:00,14-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-349T08:58:00,000T08:00:00,14-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_097IC_DSCAL08349_SP,rider,,,,,, 2008-349T16:58:00,000T02:02:00,14-Dec-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-349T17:38:00,000T00:50:00,14-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-349T18:28:00,000T12:35:00,14-Dec-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_097SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2008-349T18:28:00,000T12:35:00,14-Dec-08,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong,CIRS Compsit Ridealong. Watch Saturn rotate underneath,,,,,, 2008-349T19:00:00,000T02:00:00,14-Dec-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-349T21:00:00,003T01:58:00,14-Dec-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-350T07:43:00,000T09:00:00,15-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-350T08:43:00,000T08:00:00,15-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_097IC_DSCAL08350_SP,rider,,,,,, 2008-350T10:30:00,000T22:18:00,15-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-350T17:23:00,000T01:15:00,15-Dec-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 22.2, range 2.03 Mkm",,,,,, 2008-350T17:23:00,000T01:15:00,15-Dec-08,CIRS,SPASS Rider,Titan,MR3CLD,,CIRS_097TI_MR3CLD350_ISS,rider,,,,,, 2008-350T17:23:00,000T01:15:00,15-Dec-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-350T18:38:00,000T02:00:00,15-Dec-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-350T20:38:00,000T02:30:00,15-Dec-08,CIRS,Prime,Saturn,REGMAP,Regional mapping,Saturn Regional Map,"Regional map - temp. mapping of N. pole, hexagon",,,,,, 2008-350T23:40:00,003T11:40:00,15-Dec-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-350T23:48:00,000T09:00:00,15-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-351T00:48:00,000T08:00:00,16-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_097IC_DSCAL08351_SP,rider,,,,,, 2008-351T08:48:00,000T21:42:00,16-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-351T09:28:00,000T04:27:00,16-Dec-08,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. SAT segment.",,,,,, 2008-351T13:55:00,000T04:42:00,16-Dec-08,VIMS,Prime,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,North Pole dynamics mosaic 1,"3x3 North Polar mosaics. Each frame takes 7 minutes to integrate, followed by 3-min repositions. Repeat for the duration of the observation slot.",,,,,, 2008-351T13:55:00,000T04:42:00,16-Dec-08,ISS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,"Polar movie with the WAC in MT2,CB2,MT2, BL1","4 2x1 mosaic at the dayside two corners of the 3x3 VIMS mosaics spaced 1h 30m. WAC in MT3, CB2, MT2, and BL1. COORDINATE WITH VIMS!!!",,,,,, 2008-351T13:55:00,000T04:42:00,16-Dec-08,UVIS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Saturn Aurora,Rider on VIMS NPOLEDYN observations,,,,,, 2008-351T18:37:00,000T01:32:00,16-Dec-08,UVIS,Prime,Star,ALPCRUSA,,Saturn Occults Alp Cru,TIMING INCLUDES 20 MINUTES FOR TURNS EACH END PLUS 20 MINUTES EXTRA MARGIN EACH END. UVIS FUV Occultation slit boresite on star for 40 minutes,,,,,, 2008-351T18:37:00,000T01:32:00,16-Dec-08,ISS,SPASS Rider,Star,ALPCRUSA,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2008-351T20:09:00,000T02:09:00,16-Dec-08,VIMS,Prime,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,North Pole dynamics mosaic 1,"3x3 North Polar mosaics. Each frame takes 7 minutes to integrate, followed by 3-min repositions. Repeat for the duration of the observation slot.",,,,,, 2008-351T20:09:00,000T02:09:00,16-Dec-08,ISS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,"Polar movie with the WAC in MT2,CB2,MT2, BL1","2 2x1 mosaic at the dayside two corners of the 3x3 VIMS mosaics spaced 1h 30m. WAC in MT3, CB2, MT2, and BL1. COORDINATE WITH VIMS!!!",,,,,, 2008-351T20:09:00,000T02:09:00,16-Dec-08,UVIS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Saturn Aurora,Rider on VIMS NPOLEDYN observations,,,,,, 2008-351T22:18:00,000T01:30:00,16-Dec-08,UVIS,Prime,Star,BETCENSA,,Saturn Occults Beta Cen,Timing includes 23 minutes for turns at both ends and 20 minutes margin at both ends. UVIS FUV Occultation slit boresite on star for 40 minutes,,,,,, 2008-351T22:18:00,000T01:30:00,16-Dec-08,ISS,SPASS Rider,Star,BETCENSA,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2008-351T23:48:00,000T02:42:00,16-Dec-08,VIMS,Prime,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,North Pole dynamics mosaic 1,"3x3 North Polar mosaics. Each frame takes 7 minutes to integrate, followed by 3-min repositions. Repeat for the duration of the observation slot.",,,,,, 2008-351T23:48:00,000T02:42:00,16-Dec-08,ISS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,"Polar movie with the WAC in MT2,CB2,MT2, BL1","2 2x1 mosaic at the dayside two corners of the 3x3 VIMS mosaics spaced 1h 30m. WAC in MT3, CB2, MT2, and BL1. COORDINATE WITH VIMS!!!",,,,,, 2008-351T23:48:00,000T02:42:00,16-Dec-08,RADAR,SPASS Rider,Other,WU4NRPOL,,Warmup for Saturn North Pole Map,Warmup for north pole map.,,,,,, 2008-351T23:48:00,000T02:42:00,16-Dec-08,UVIS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Saturn Aurora,Rider on VIMS NPOLEDYN observations,,,,,, 2008-352T02:30:00,000T07:00:00,17-Dec-08,RADAR,Prime,Saturn,NORTHPOL,,Saturn North Pole Map,map north pole; coordinated with VIMS.,,,,,, 2008-352T06:30:00,000T21:55:00,17-Dec-08,CAPS,SPASS Rider,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source region,,,,,, 2008-352T06:30:00,000T21:55:00,17-Dec-08,MAG,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAG MAPS AS Campaign,"Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions. AURXNG are L>4, r<7.5",,,,,, 2008-352T06:30:00,000T21:55:00,17-Dec-08,MIMI,Non-SPASS,Saturn,AURXNG,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-352T08:48:00,000T06:10:00,17-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-352T09:30:00,000T02:13:00,17-Dec-08,ISS,Prime,Rhea,020W151PH,,Rhea phase coverage,"Turn UVIS_FUV to Rhea; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-352T09:30:00,000T02:13:00,17-Dec-08,CIRS,SPASS Rider,Rhea,020W151PH,,CIRS_097RH_020W151PH001_ISS,rider,,,,,, 2008-352T09:30:00,000T02:13:00,17-Dec-08,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-352T09:30:00,000T02:13:00,17-Dec-08,VIMS,SPASS Rider,Rhea,020W151PH,,spectral cubes,Phase study,,,,,, 2008-352T11:43:00,000T00:45:00,17-Dec-08,ISS,Prime,Saturn,LIMBSCAN,Limb scan,Saturn Limb Scan,Rings behind Saturn nightside limb,,,,,, 2008-352T11:43:00,000T00:45:00,17-Dec-08,VIMS,SPASS Rider,Saturn,LIMBOBS,,High-res limbscans,"Hi Res Limbscans ridealong with ISS. Image about 6 places along the sunlit limb, avoiding the ring.",,,,,, 2008-352T14:58:00,000T08:00:00,17-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_097IC_DSCAL08352_SP,rider,,,,,, 2008-352T14:58:00,000T07:00:00,17-Dec-08,RPWS,SPASS Rider,Saturn,WHISTLER,RPWS lightning search,RWA wideband search for lightning whistlers,"Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement for the observation, but since we need to conserve fuel, we can only go to RCS control during a downlink period.",,,,,, 2008-352T15:20:00,000T04:00:00,17-Dec-08,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-352T16:11:29,000T02:00:00,17-Dec-08,CDA,SPASS Rider,DustRAM direction,RPX0160,,CDA RPXing 2008-352T17:11:29 MMH,"must must have, vertical crossing",,,,,, 2008-352T16:17:59,000T00:27:00,17-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.7957772 Rs exit= 5.7806007 Range altitude= 39385.282 km ... 20063.225,,,,,, 2008-352T16:31:00,000T01:00:00,17-Dec-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-352T17:25:26,000T00:00:01,17-Dec-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.765 Rs, lat = -2 deg, phase = 155 deg",,,,,, 2008-352T17:37:59,000T00:27:00,17-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.7711035 Rs exit= 5.7771897 Range altitude= -20158.709 km ... -39480.173,,,,,, 2008-352T18:04:59,002T22:24:01,17-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 5.7775618 Rs exit= 9.1071336 Range altitude= -40221.847 km ... 40461.726,,,,,, 2008-352T21:58:00,000T04:02:00,17-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-352T22:58:00,000T02:00:00,17-Dec-08,RADAR,SPASS Rider,Other,WU4SOPOL,,Warmup for Saturn South Pole Map,Warmup for south pole map.,,,,,, 2008-352T22:58:00,000T16:02:00,17-Dec-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-352T23:38:00,000T01:20:00,17-Dec-08,VIMS,Prime,Saturn,SPOLEHIRE,,South Pole hi-res mosaic,2*3 + 2 mosaic of the southpole,,,,,, 2008-353T00:58:00,000T07:00:00,18-Dec-08,RADAR,Prime,Saturn,SOUTHPOL,,Saturn South Pole Map,map south pole; coordinated with VIMS.,,,,,, 2008-353T04:25:00,002T12:04:00,18-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2008-353T04:25:00,002T12:04:00,18-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-353T04:25:00,000T19:33:00,18-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-353T07:58:00,000T14:50:00,18-Dec-08,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics mosaic 1,"3x3 South Polar mosaics, repeated as usual. Each frame takes approx 7 min.to integrate, followed by 3 mins of reposition slews. Repeat.",,,,,, 2008-353T07:58:00,000T14:50:00,18-Dec-08,ISS,SPASS Rider,Saturn,SPOLEDYN,,"Polar movie with the WAC in MT2,CB2,MT2, BL1","10 pickets spaced 1h 30m. 2x1 WAC in MT3, CB2.",,,,,, 2008-353T07:58:00,000T14:50:00,18-Dec-08,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2008-353T15:00:00,000T02:00:00,18-Dec-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-353T17:00:00,000T15:58:00,18-Dec-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-353T22:48:00,000T00:30:00,18-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-353T23:58:00,000T20:02:00,18-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-353T23:58:00,000T09:00:00,18-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-354T00:58:00,000T08:00:00,19-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_097IC_DSCAL08354_SP,rider,,,,,, 2008-354T08:58:00,001T07:31:00,19-Dec-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-354T09:30:00,000T15:00:00,19-Dec-08,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",,,,,,, 2008-354T09:38:00,000T01:15:00,19-Dec-08,ISS,Prime,Titan,MR1CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 74.6, range 0.95 Mkm",,,,,, 2008-354T09:38:00,000T01:15:00,19-Dec-08,CIRS,SPASS Rider,Titan,MR1CLDF,,CIRS_097TI_MR1CLDF354_ISS,rider,,,,,, 2008-354T09:38:00,000T01:15:00,19-Dec-08,UVIS,SPASS Rider,Titan,MR1CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-354T10:53:00,000T22:00:00,19-Dec-08,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning S. hemisphere, may be split in half by downlink",,,,,, 2008-354T11:20:00,002T01:44:00,19-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-354T20:00:00,000T17:00:00,19-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-355T08:33:00,000T07:56:00,20-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-355T10:18:00,000T06:11:00,20-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_097IC_DSCAL08355_SP,rider,,,,,, 2008-355T13:00:00,000T22:00:00,20-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-355T16:29:00,000T18:30:43,20-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-355T16:29:00,000T20:35:00,20-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 5.7775618 Rs exit= 9.1071336 Range altitude= -40221.847 km ... 40461.726,,,,,, 2008-355T16:29:00,000T19:30:52,20-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-355T16:29:00,000T16:30:52,20-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-355T17:24:32,000T06:35:20,20-Dec-08,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2008-355T17:24:32,000T06:35:20,20-Dec-08,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong context imaging),regional map,,,,,, 2008-355T17:24:32,000T06:35:20,20-Dec-08,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Mapping,VIMS ridealong with CIRS. Monitoring clouds,,,,,, 2008-355T23:59:52,000T04:00:00,20-Dec-08,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2008-355T23:59:52,000T04:00:00,20-Dec-08,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2008-355T23:59:52,000T04:00:00,20-Dec-08,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong context imaging),regional map,,,,,, 2008-355T23:59:52,000T04:00:00,20-Dec-08,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2008-355T23:59:52,000T04:00:00,20-Dec-08,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir Comp.,VIMS ridealong with CIRS. Clouds and global mapping,,,,,, 2008-356T03:59:52,000T04:00:00,21-Dec-08,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2008-356T03:59:52,000T04:00:00,21-Dec-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2008-356T03:59:52,000T04:00:00,21-Dec-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,VIMS ridealong with ISS. Plan 1 cube every 20 min.,,,,,, 2008-356T07:59:52,000T02:00:00,21-Dec-08,ISS,Prime,Titan,REGMAP,Regional mapping,NAC Regional Map,regional map,,,,,, 2008-356T07:59:52,000T02:00:00,21-Dec-08,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS.,,,,,, 2008-356T07:59:52,000T02:00:00,21-Dec-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global and cloud mapping,VIMS ridealong with ISS. Plan 1 cube every 10 min.,,,,,, 2008-356T08:59:52,000T08:00:00,21-Dec-08,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,MAPS_Titan_Flyby,"T049 is an upstream flank-out flyby with a minimum altitude of 1000 km. The geometry of this flyby is suitable to study the magnetic pileup region and the pressure balance between the magnetic pressure in the magnetic barrier and the thermal pressure in the ionosphere. T049 also takes place in Saturn's near-noon sector (10.5 hours SLT), where Titan could be found in the magnetosheath if the solar wind pressure is high. We assign grade one priority.",,,,,, 2008-356T09:59:52,000T01:00:00,21-Dec-08,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2008-356T09:59:52,000T01:00:00,21-Dec-08,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2008-356T09:59:52,000T01:00:00,21-Dec-08,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong context imaging),regional map,,,,,, 2008-356T09:59:52,000T02:36:00,21-Dec-08,RADAR,SPASS Rider,Titan,T49WARMUP,,Warmup for T49.,Warmup for T49,,,,,, 2008-356T09:59:52,000T01:00:00,21-Dec-08,UVIS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,UVIS Rider to CIRS FIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2008-356T09:59:52,000T01:00:00,21-Dec-08,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,VIMS ridealong with CIRS.,,,,,, 2008-356T10:59:52,000T01:14:00,21-Dec-08,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Mosaic,Regional mapping and 3 x 3 mosaic,,,,,, 2008-356T10:59:52,000T01:15:00,21-Dec-08,CAPS,SPASS Rider,Titan,T49INBND,,Inbound 097TI (T49),Inbound leg of a Titan encoun,,,,,, 2008-356T10:59:52,000T01:14:00,21-Dec-08,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2008-356T10:59:52,000T01:14:00,21-Dec-08,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong context imaging),regional map,,,,,, 2008-356T11:00:00,000T01:00:00,21-Dec-08,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-356T11:00:00,000T01:30:00,21-Dec-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-356T11:59:52,000T00:40:00,21-Dec-08,INMS,Non-SPASS,Titan,TITAN49,,Titan Flyby,Titan observation,,,,,, 2008-356T12:00:00,000T01:04:00,21-Dec-08,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-356T12:14:52,000T00:21:00,21-Dec-08,VIMS,Prime,Titan,TRANS,,ENGR reg. map.,2 VIMS cubes while RWA to RCS transition. Note this was scheduled in the prime spreadsheet. Pointing at Tui regio for a mapping at 5 km/pixel if possible,,,,,, 2008-356T12:14:52,000T01:30:00,21-Dec-08,CAPS,SPASS Rider,Titan,T49CLOSE,,Closest approach 097TI (T49),Closest approach of a Titan encoun,,,,,, 2008-356T12:30:00,000T00:34:00,21-Dec-08,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2008-356T12:35:52,000T00:15:00,21-Dec-08,RADAR,Prime,Titan,T49INSAR,,T49 Inbound SAR,,,,,,, 2008-356T12:39:52,000T00:40:00,21-Dec-08,INMS,Non-SPASS,Titan,TITAN49,,Titan Flyby,Titan observation,,,,,, 2008-356T12:50:52,000T00:05:00,21-Dec-08,RADAR,Prime,Titan,T49CAALT,,T49 Altimetry at C/A over Ontario,,,,,,, 2008-356T12:55:52,000T00:22:00,21-Dec-08,RADAR,Prime,Titan,T49OUTSAR,,T49 Outbound SAR,,,,,,, 2008-356T13:04:00,000T00:56:00,21-Dec-08,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-356T13:04:00,000T18:10:00,21-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 5.7775618 Rs exit= 9.1071336 Range altitude= -40221.847 km ... 40461.726,,,,,, 2008-356T13:04:00,001T09:10:00,21-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-356T13:04:00,000T00:26:00,21-Dec-08,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2008-356T13:04:11,000T00:00:01,21-Dec-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 9.4 d, inc = 74.7 deg, r = 19.715 Rs, phase = 25 deg",,,,,, 2008-356T13:17:52,000T00:12:00,21-Dec-08,RADAR,Prime,Titan,T49OUTALT,,T49 Outbound Altimetry,,,,,,, 2008-356T13:19:52,000T00:40:00,21-Dec-08,INMS,Non-SPASS,Titan,TITAN49,,Titan Flyby,Titan observation,,,,,, 2008-356T13:29:52,000T00:20:00,21-Dec-08,RADAR,Prime,Titan,T49OHISAR,,T49 outbound HiSAR,,,,,,, 2008-356T13:30:00,000T01:30:00,21-Dec-08,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2008-356T13:44:52,000T01:15:00,21-Dec-08,CAPS,SPASS Rider,Titan,T49OUTBND,,Outbound 097TI (T49),Outbound leg of a Titan encoun,,,,,, 2008-356T13:59:52,001T08:14:08,21-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-356T14:00:00,000T01:00:00,21-Dec-08,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2008-356T14:11:06,000T00:48:46,21-Dec-08,RADAR,Prime,Titan,T49OUTSCT,,T49 Outbound Scatterometry,,,,,,, 2008-356T14:59:52,000T03:30:00,21-Dec-08,RADAR,Prime,Titan,T49OUTRAD,,T49 Outbound Radiometry,,,,,,, 2008-356T14:59:52,001T07:15:08,21-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-356T15:00:00,001T13:15:00,21-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-356T16:59:52,001T05:14:08,21-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-356T18:29:52,000T03:30:00,21-Dec-08,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2008-356T18:29:52,000T03:30:00,21-Dec-08,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2008-356T18:29:52,000T03:30:00,21-Dec-08,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong context imaging),regional map,,,,,, 2008-356T18:29:52,000T03:30:00,21-Dec-08,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2008-356T18:29:52,000T03:30:00,21-Dec-08,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Mid-IR Limb Mapping,VIMS ridealong with CIRS. Cloud mapping,,,,,, 2008-356T21:59:52,000T04:00:00,21-Dec-08,VIMS,Prime,Titan,CLOUDMAP,Cloud map,Cloud Mapping,VIMS Prime for Cloud mapping.,,,,,, 2008-356T21:59:52,000T04:00:00,21-Dec-08,CIRS,SPASS Rider,Titan,DUMMY,,,Ride along with VIMS.,,,,,, 2008-356T21:59:52,000T04:00:00,21-Dec-08,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong context imaging),regional map,,,,,, 2008-357T01:59:52,000T00:30:00,22-Dec-08,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Night NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2008-357T01:59:52,000T00:30:00,22-Dec-08,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with VIMS.,,,,,, 2008-357T01:59:52,000T00:30:00,22-Dec-08,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare on night-side with NAC,VIMS ridealong with ISS. If dwell times of 6 min. then 5 cubes can be obtained during the hour,,,,,, 2008-357T01:59:52,000T00:30:00,22-Dec-08,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare on night-side with NAC,VIMS ridealong with ISS. If dwell times of 6 min. then 5 cubes can be obtained during the hour,,,,,, 2008-357T02:29:52,000T03:30:00,22-Dec-08,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2008-357T02:29:52,000T03:30:00,22-Dec-08,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2008-357T02:29:52,000T03:30:00,22-Dec-08,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong context imaging),regional map,,,,,, 2008-357T02:29:52,000T03:30:00,22-Dec-08,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp. Mapping,VIMS ridealong with CIRS. Map of Titan.,,,,,, 2008-357T05:59:52,000T00:30:00,22-Dec-08,ISS,Prime,Titan,LRMONITOR,Long range monitor,LRM (Long Range Monitor),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2008-357T05:59:52,000T00:30:00,22-Dec-08,CIRS,SPASS Rider,Titan,LRMONITOR,Long range monitor,,Ride along with VIMS.,,,,,, 2008-357T07:14:00,003T21:28:59,22-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 5.7775618 Rs exit= 9.1071336 Range altitude= -40221.847 km ... 40461.726,,,,,, 2008-357T07:14:00,000T09:00:00,22-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-357T08:14:00,000T08:00:00,22-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08357_SP,rider,,,,,, 2008-357T16:14:00,000T06:00:00,22-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-357T17:14:00,000T05:00:00,22-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08757_SP,rider,,,,,, 2008-357T22:14:00,002T00:30:00,22-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-357T22:14:00,001T03:01:00,22-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-357T22:14:00,001T06:46:00,22-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-357T22:15:00,001T03:00:00,22-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-357T22:54:00,000T07:40:00,22-Dec-08,CIRS,Prime,rings(general),TMAPN30LP,,CIRS_098RI_TMAPN30LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-357T22:54:00,000T07:40:00,22-Dec-08,CIRS,SPASS Rider,rings(general),TMAPN30LP,,CIRS_098RI_TMAPN30LP001_SI,,,,,,, 2008-357T22:54:00,000T07:40:00,22-Dec-08,ISS,SPASS Rider,rings(general),TMAPN30LP,,Spoke Periodicity Monitoring,One WAC every 20 minutes,,,,,, 2008-357T22:54:00,000T07:40:00,22-Dec-08,UVIS,SPASS Rider,rings(general),TMAPN30LP,,,,,,,,, 2008-358T04:15:00,000T21:00:00,23-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-358T07:14:00,000T09:00:00,23-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-358T07:29:00,000T05:54:00,23-Dec-08,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2008-358T08:14:00,000T08:00:00,23-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08358_SP,rider,,,,,, 2008-358T16:54:00,000T01:06:00,23-Dec-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-358T18:00:00,000T00:30:00,23-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-358T18:30:00,000T04:00:00,23-Dec-08,CIRS,Prime,rings(general),TMAPN45LP,,CIRS_098RI_TMAPN45LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-358T18:30:00,000T04:00:00,23-Dec-08,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_098RI_TMAPN45LP001_SI,,,,,,, 2008-358T18:30:00,000T04:00:00,23-Dec-08,UVIS,SPASS Rider,rings(general),TMAPN45LP,,,,,,,,, 2008-358T19:30:00,000T03:00:00,23-Dec-08,RADAR,SPASS Rider,Other,WU4NMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2008-358T22:30:00,000T01:30:00,23-Dec-08,RADAR,Prime,Titan,NMIDLCAL,,"Distant Titan Radiometry, North Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2008-359T00:00:00,000T04:21:00,24-Dec-08,UVIS,Prime,Star,URDELCEN,Stellar occultation,URSTAR,,,,,,, 2008-359T00:00:00,000T04:21:00,24-Dec-08,CIRS,SPASS Rider,rings(general),URDELCEN,Stellar occultation,CIRS_098RI_URDELCEN001_UVIS,rider,,,,,, 2008-359T00:00:00,000T04:21:00,24-Dec-08,ISS,SPASS Rider,Star,URDELCEN,Stellar occultation,Stellar Occultation by Rings NAC Rider,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-359T00:00:00,000T04:21:00,24-Dec-08,UVIS,SPASS Rider,Star,URDELCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2008-359T00:45:00.0 2008-359T00:57:18.0 2008-359T01:36:33.5,,,,,, 2008-359T01:15:00,000T04:00:00,24-Dec-08,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS campaign,,,,,, 2008-359T01:15:00,000T04:00:00,24-Dec-08,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2008-359T01:15:00,000T04:00:00,24-Dec-08,MIMI,Non-SPASS,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2008-359T01:15:00,000T04:00:00,24-Dec-08,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2008-359T04:21:00,000T02:00:00,24-Dec-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-359T05:00:00,004T00:00:00,24-Dec-08,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-359T05:15:00,001T20:20:00,24-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-359T05:15:00,001T20:20:00,24-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-359T05:15:00,001T20:20:00,24-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-359T06:21:00,000T01:04:00,24-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-359T07:25:00,000T05:15:00,24-Dec-08,UVIS,Prime,Star,URBETCRU,,URSTAR,,,,,,, 2008-359T07:25:00,000T05:15:00,24-Dec-08,CIRS,SPASS Rider,rings(general),URBETCRU,,CIRS_098RI_URBETCRU001_UVIS,rider,,,,,, 2008-359T07:25:00,000T05:15:00,24-Dec-08,ISS,SPASS Rider,Star,URBETCRU,,Stellar Occultation by Rings NAC Rider,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-359T07:25:00,000T05:15:00,24-Dec-08,UVIS,SPASS Rider,Star,URBETCRU,,Support Imaging,NAC support images at the following times: 2008-359T08:11:00.0 2008-359T08:24:46.0 2008-359T09:08:23.5,,,,,, 2008-359T12:40:00,000T00:24:00,24-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-359T13:44:00,000T09:00:00,24-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-359T14:44:00,000T08:00:00,24-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08359_SP,rider,,,,,, 2008-359T22:44:00,001T05:31:00,24-Dec-08,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-359T23:24:00,000T06:12:00,24-Dec-08,CIRS,Prime,rings(general),VTMPN60MP,,CIRS_098RI_VTMPN60MP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-359T23:24:00,000T06:12:00,24-Dec-08,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_098RI_VTMPN60MP001_SI,,,,,,, 2008-359T23:24:00,000T06:12:00,24-Dec-08,UVIS,SPASS Rider,rings(general),VTMPN60MP,,,,,,,,, 2008-360T00:00:00,000T00:34:08,25-Dec-08,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2008-360T05:36:00,000T07:00:00,25-Dec-08,UVIS,Prime,Star,URALPARA,Alpha Ara occultation,URSTAR,,,,,,, 2008-360T05:36:00,000T07:00:00,25-Dec-08,CIRS,SPASS Rider,rings(general),URALPARA,Alpha Ara occultation,CIRS_098RI_URALPARA001_UVIS,rider,,,,,, 2008-360T05:36:00,000T07:00:00,25-Dec-08,ISS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Stellar Occultation by Rings NAC Rider,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2008-360T05:36:00,000T07:00:00,25-Dec-08,UVIS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Support Imaging,NAC support images at the following times: 2008-360T06:26:00.0 2008-360T06:42:45.0 2008-360T07:47:50.0 2008-360T11:47:00.0 2008-360T11:31:21.0 2008-360T10:26:10.0,,,,,, 2008-360T12:36:00,000T08:00:00,25-Dec-08,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2008-360T12:36:00,000T08:00:00,25-Dec-08,CIRS,SPASS Rider,rings(general),SHRTMOV,,CIRS_098RI_SHRTMOV001_ISS,rider,,,,,, 2008-360T12:36:00,000T08:00:00,25-Dec-08,VIMS,SPASS Rider,rings(general),SHRTMOV,,VIMS rider on ISS SHRTMOV,VIMS Rider on ISS,,,,,, 2008-360T13:30:00,000T10:00:00,25-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-360T20:36:00,000T05:00:00,25-Dec-08,CIRS,Prime,rings(general),TDIFN20HP,,CIRS_098RI_TDIFN20HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-360T20:36:00,000T05:00:00,25-Dec-08,CIRS,SPASS Rider,rings(general),TDIFN20HP,,CIRS_098RI_TDIFN20HP001_SI,,,,,,, 2008-360T20:36:00,000T05:00:00,25-Dec-08,ISS,SPASS Rider,rings(general),TDIFN20HP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2008-360T20:36:00,000T05:00:00,25-Dec-08,UVIS,SPASS Rider,rings(general),TDIFN20HP,,,,,,,,, 2008-360T23:30:00,000T01:30:00,25-Dec-08,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Region Campaign,Part of RPWS campaign to obtain high resolution WBR data in the narrow band emission source region,,,,,, 2008-361T01:35:00,000T08:40:00,26-Dec-08,CAPS,SPASS Rider,Saturn,IMVP9,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2008-361T01:35:00,000T08:40:00,26-Dec-08,MAG,Non-SPASS,Saturn,IMVP9,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L ~9",,,,,, 2008-361T01:35:00,000T08:40:00,26-Dec-08,MIMI,Non-SPASS,Saturn,IMVP9,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2008-361T01:35:00,000T03:21:00,26-Dec-08,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-361T04:15:00,000T02:00:00,26-Dec-08,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2008-361T04:42:59,000T02:27:00,26-Dec-08,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.1070391 Rs exit= 9.1229757 Range altitude= 39918.076 km ... -39575.641,,,,,, 2008-361T04:56:00,000T02:00:00,26-Dec-08,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2008-361T04:57:29,000T02:00:00,26-Dec-08,CDA,SPASS Rider,DustRAM direction,RPX0170,,CDA RPXing 2008-361T05:57:29 NTH,"Nice to have - small/medium inclination - large ring extention, RPXing at > 8 Rs",,,,,, 2008-361T05:10:51,000T00:00:01,26-Dec-08,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 9.095 Rs, lat = 2 deg, phase = 154 deg",,,,,, 2008-361T06:15:00,001T02:14:00,26-Dec-08,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-361T06:56:00,000T03:19:00,26-Dec-08,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2008-361T06:57:00,000T03:00:00,26-Dec-08,ISS,Prime,Enceladus,PLMMRHP,,Medium res plume obs at high phase,LIEN. Medium resolution plume observation at high phase,,,,,, 2008-361T06:57:00,000T03:00:00,26-Dec-08,CIRS,SPASS Rider,Enceladus,PLMMRHP,,CIRS_098EN_PLMMRHP001_ISS,rider,,,,,, 2008-361T06:57:00,000T03:00:00,26-Dec-08,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2008-361T06:57:00,000T03:00:00,26-Dec-08,VIMS,SPASS Rider,Enceladus,PLMMRHP,,spectral cubes,Enceladus Plume,,,,,, 2008-361T07:09:59,004T17:01:01,26-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 9.1232878 Rs exit= 9.1118652 Range altitude= -40119.316 km ... 40456.992,,,,,, 2008-361T09:57:00,000T03:00:00,26-Dec-08,CIRS,Prime,rings(general),TDIFS20HP,,CIRS_098RI_TDIFS20HP001_PRIME,rider,,,,,, 2008-361T09:57:00,000T03:00:00,26-Dec-08,CIRS,SPASS Rider,rings(general),TDIFS20HP,,CIRS_098RI_TDIFS20HP001_SI,,,,,,, 2008-361T09:57:00,000T03:00:00,26-Dec-08,UVIS,SPASS Rider,rings(general),TDIFS20HP,,,,,,,,, 2008-361T10:15:00,004T13:57:00,26-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-361T10:15:00,002T05:45:00,26-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-361T10:15:00,003T01:45:00,26-Dec-08,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2008-361T11:00:00,000T01:00:00,26-Dec-08,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Region Campaign,Part of RPWS campaign to obtain high resolution WBR data in the narrow band emission source region,,,,,, 2008-361T12:00:00,000T20:29:00,26-Dec-08,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2008-361T12:57:00,000T03:30:00,26-Dec-08,VIMS,Prime,rings(general),COMPHILIT,High phase sunlit ring radial scan,Ring COMPHILIT,Do 4 at priority 1.,,,,,, 2008-361T12:57:00,000T03:30:00,26-Dec-08,CIRS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,CIRS_098RI_COMPHILIT120_VIMS,rider,,,,,, 2008-361T12:57:00,000T03:30:00,26-Dec-08,UVIS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,,,,,,,, 2008-361T16:27:00,000T05:32:00,26-Dec-08,CIRS,Prime,rings(general),VENCLSHP,,CIRS_098RI_VENCLSHP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2008-361T16:27:00,000T05:32:00,26-Dec-08,CIRS,SPASS Rider,rings(general),VENCLSHP,,CIRS_098RI_VENCLSHP001_SI,,,,,,, 2008-361T16:27:00,000T05:32:00,26-Dec-08,UVIS,SPASS Rider,rings(general),VENCLSHP,,,,,,,,, 2008-361T23:29:00,000T09:00:00,26-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-362T00:29:00,000T08:00:00,27-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08362_SP,rider,,,,,, 2008-362T08:29:00,001T07:31:00,27-Dec-08,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2008-362T09:09:00,000T21:11:00,27-Dec-08,CIRS,Prime,rings(general),SHADLMP,Saturn ring shadow observation,CIRS_098RI_SHADLMP001_PRIME;,null,,,,,, 2008-362T09:09:00,000T21:11:00,27-Dec-08,CIRS,SPASS Rider,rings(general),SHADLMP,Saturn ring shadow observation,CIRS_098RI_SHADLMP001_SI,,,,,,, 2008-363T05:00:00,000T11:00:00,28-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-363T07:00:00,000T09:00:00,28-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-363T08:00:00,000T08:00:00,28-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08363_SP,rider,,,,,, 2008-363T16:00:00,002T06:12:00,28-Dec-08,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-363T16:00:00,000T05:30:00,28-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-363T16:00:00,002T08:11:00,28-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-363T17:15:00,000T01:00:00,28-Dec-08,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2008-363T18:15:00,000T01:15:00,28-Dec-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2008-363T18:15:00,000T01:15:00,28-Dec-08,CIRS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-363T18:15:00,000T01:15:00,28-Dec-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-363T19:30:00,000T02:00:00,28-Dec-08,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2008-363T21:30:00,000T06:15:00,28-Dec-08,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2008-364T03:45:00,000T01:00:00,29-Dec-08,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2008-364T03:45:00,004T11:20:00,29-Dec-08,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2008-364T04:45:00,000T19:05:00,29-Dec-08,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning S. hemisphere, may be split in half by downlink",,,,,, 2008-364T12:00:00,001T12:12:00,29-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-365T00:15:00,000T09:00:00,30-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-365T01:15:00,000T08:00:00,30-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_098IC_DSCAL08365_SP,rider,,,,,, 2008-365T09:55:00,000T01:15:00,30-Dec-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2008-365T09:55:00,000T01:15:00,30-Dec-08,CIRS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-365T09:55:00,000T01:15:00,30-Dec-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-365T11:10:00,000T00:30:00,30-Dec-08,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2008-365T11:40:00,000T01:00:00,30-Dec-08,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2008-365T12:40:00,000T06:00:00,30-Dec-08,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_098SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2008-365T12:40:00,000T06:00:00,30-Dec-08,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2008-365T18:40:00,000T09:25:00,30-Dec-08,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2008-365T18:40:00,000T09:25:00,30-Dec-08,ISS,SPASS Rider,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2008-365T22:12:00,000T02:00:00,30-Dec-08,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2008-366T00:06:10,000T00:00:01,31-Dec-08,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 9.6 d, inc = 69.0 deg, r = 19.732 Rs, phase = 26 deg",,,,,, 2008-366T00:11:00,004T18:21:59,31-Dec-08,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 9.1232878 Rs exit= 9.1118652 Range altitude= -40119.316 km ... 40456.992,,,,,, 2008-366T00:11:00,002T18:49:00,31-Dec-08,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2008-366T00:12:00,002T14:53:00,31-Dec-08,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2008-366T00:12:00,004T17:48:00,31-Dec-08,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2008-366T00:12:00,001T17:48:00,31-Dec-08,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2008-366T04:05:00,000T02:00:00,31-Dec-08,ISS,Prime,Dione,088W008PH,,Dione lon/phase angle observation,"Turn UVIS_FUV to Dione; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2008-366T04:05:00,000T02:00:00,31-Dec-08,CIRS,SPASS Rider,Dione,088W008PH,,CIRS_099DI_088W008PH001_ISS,rider,,,,,, 2008-366T04:05:00,000T02:00:00,31-Dec-08,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2008-366T04:05:00,000T02:00:00,31-Dec-08,VIMS,SPASS Rider,Dione,088W008PH,,spectral cubes,Phase study,,,,,, 2008-366T06:45:00,000T08:00:00,31-Dec-08,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS Ka-TWTA Maintenance,Ka-TWTA maintenance; Pointing = n/a; No DSN tracking required.,,,,,, 2008-366T06:45:00,000T09:00:00,31-Dec-08,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2008-366T07:45:00,000T08:00:00,31-Dec-08,CIRS,SPASS Rider,InstrumentCalibration,DSCAL08,Deep space calibration,CIRS_099IC_DSCAL08366_SP,rider,,,,,, 2008-366T16:25:00,000T01:15:00,31-Dec-08,ISS,Prime,Titan,MR3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2008-366T16:25:00,000T01:15:00,31-Dec-08,CIRS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2008-366T16:25:00,000T01:15:00,31-Dec-08,UVIS,SPASS Rider,Titan,MR3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2008-366T17:40:00,000T08:00:00,31-Dec-08,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,Turn to sun; Time: 30 min Solar Port: same 5*7 cross design as on revs A and C; tau_IR = 40 & 320 msec; VIS always @ 50ms; Total time: 8hr; Volume: 240 Mbits; Solar Background Calibration: 4 cubes w/64x64 FOV; Time: 30 min; Turn to waypoint: 30 min,,,,,, 2008-366T17:40:00,000T08:00:00,31-Dec-08,UVIS,SPASS Rider,Sun,SOLARPORT,Solar port observation,VIMS SOLAR PORT RIDER,VIMS RIDER,,,,,, 2009-001T01:40:00,000T02:00:00,1-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-001T03:40:00,000T01:00:00,1-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-001T04:40:00,000T13:18:00,1-Jan-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning S. hemisphere, may be split in half by downlink 1 of 2 acceptable (Rev 101 has identical request)",,,,,, 2009-001T04:40:00,000T13:18:00,1-Jan-09,VIMS,SPASS Rider,Saturn,FIRMAP,Far infrared map,FIRMAP ridealong with CIRS,FIRMAP Ridealong with CIRS,,,,,, 2009-001T17:58:00,000T01:00:00,1-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-001T18:00:00,000T21:05:00,1-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-001T18:58:00,000T09:17:00,1-Jan-09,VIMS,Prime,Other,PLEIADES,Pleiades,Pleiades,"Turn to Pleiades; Time: 30 min Pleiades: multiple cubes w/64x64 FOV IR @ 640 ms, VIS @ 40000 ms; Time: 7.0 hr 47 min; Volume: 86.5 Mbits; CompRatio: 2.0 Turn to waypoint: 30 min Primary: -y to Pleiades; Secondary: +z to TBD Not time critical. RWA REQUIRED.",,,,,, 2009-002T04:15:00,000T01:00:00,2-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-002T06:45:00,000T09:00:00,2-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-002T07:45:00,000T08:00:00,2-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_099IC_DSCAL09002_SP,rider,,,,,, 2009-002T07:45:00,000T11:15:00,2-Jan-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-002T15:05:00,000T04:00:00,2-Jan-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS campaign,,,,,, 2009-002T15:05:00,000T04:00:00,2-Jan-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-002T15:05:00,000T04:00:00,2-Jan-09,MIMI,Non-SPASS,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-002T16:25:00,000T01:15:00,2-Jan-09,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2009-002T16:25:00,000T01:15:00,2-Jan-09,CIRS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-002T16:25:00,000T01:15:00,2-Jan-09,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-002T17:40:00,000T10:11:00,2-Jan-09,VIMS,Prime,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,North Pole dynamics mosaic 1,"3x3 North Polar mosaics. Each frame takes 7 min to integrate, followed by 3 min reposition slews. Repeat.",,,,,, 2009-002T17:40:00,000T10:11:00,2-Jan-09,ISS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Auroral WAC 1X2 movie + lightning search,"Auroral WAC rider on VIMS, CL1 if at the night side, CB2 if at the day side at the corners of VIMS mosaic. 4 images per 110 min cut by 3 images due to data volme",,,,,, 2009-002T17:40:00,000T10:11:00,2-Jan-09,UVIS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Saturn Aurora,Rider on VIMS NPOLEDYN observations,,,,,, 2009-002T19:00:00,004T00:00:00,2-Jan-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-002T19:05:00,001T20:20:00,2-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-002T19:05:00,001T20:20:00,2-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-002T19:05:00,001T20:20:00,2-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-003T03:51:00,000T01:30:00,3-Jan-09,UVIS,Prime,Star,BETCRU,,Saturn Occults Beta Cru,UVIS FUV Occultation slit boresite on star for 40 minutes,,,,,, 2009-003T05:21:00,000T17:00:00,3-Jan-09,VIMS,Prime,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,North Pole dynamics mosaic 3,"3x3 North Polar mosaics. Each frame takes 7 min to integrate, followed by 3 min reposition slews. Repeat.",,,,,, 2009-003T05:21:00,000T17:00:00,3-Jan-09,ISS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Auroral WAC 1X2 movie + lightning search,"Auroral WAC rider on VIMS, CL1 if at the night side, CB2 if at the day side at the corners of VIMS mosaic. 4 images per 110 min cut by 5 images due to data volme",,,,,, 2009-003T05:21:00,000T17:00:00,3-Jan-09,UVIS,SPASS Rider,Saturn,NPOLEDYN,Mosaic imaging of the North Pole to investigate cloud motion and atmospheric dynamics,Saturn Aurora,Rider on VIMS NPOLEDYN observations,,,,,, 2009-003T13:10:00,000T18:51:00,3-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-003T23:01:00,000T09:00:00,3-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-004T00:01:00,000T08:00:00,4-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_099IC_DSCAL09004_SP,rider,,,,,, 2009-004T08:01:00,000T07:24:00,4-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-004T08:26:00,000T03:51:00,4-Jan-09,UVIS,Prime,Saturn,AURORA,Saturn aurora,Saturn Aurora,"Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2009-004T08:26:00,000T03:51:00,4-Jan-09,ISS,SPASS Rider,Saturn,AURORA,Saturn aurora,Auroral WAC 2X2 movie + lightning search. North,"Auroral WAC movie. 3 time steps in a 1x2 mosaic in clear, HAL and IR2 filters. Space pickets one hour apart.",,,,,, 2009-004T08:26:00,000T03:51:00,4-Jan-09,VIMS,SPASS Rider,Saturn,AURORA,Saturn aurora,North Pole Aurora ridealong,Several Obs. At least one should be a 1-sec per-pixel integration image of the pole.,,,,,, 2009-004T12:17:00,000T03:08:00,4-Jan-09,ISS,Prime,Tethys,064W150PH,,Tethys lon/phase angle observation,"Turn UVIS_FUV to Tethys; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2009-004T12:17:00,000T03:08:00,4-Jan-09,CIRS,SPASS Rider,Tethys,064W150PH,,CIRS_099TE_064W150PH001_ISS,"All FP, blink, 15.5 cm-1; shutter closed 00:10-00:05, 01:45-01:55, 02:55-03:00.",,,,,, 2009-004T12:17:00,000T03:08:00,4-Jan-09,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-004T12:17:00,000T03:08:00,4-Jan-09,VIMS,SPASS Rider,Tethys,064W150PH,,spectral cubes,Phase study,,,,,, 2009-004T15:25:00,000T08:40:00,4-Jan-09,CAPS,Prime,Saturn,IMVP9PTG,,MAPS IMVP Campaign,Prime pointing during IMVP MAPS Campaign (Inner magn,,,,,, 2009-004T15:25:00,000T08:40:00,4-Jan-09,CAPS,SPASS Rider,Saturn,IMVP9,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2009-004T15:25:00,000T08:40:00,4-Jan-09,MAG,Non-SPASS,Saturn,IMVP9,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L ~9",,,,,, 2009-004T15:25:00,000T08:40:00,4-Jan-09,MIMI,Non-SPASS,Saturn,IMVP9,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2009-004T15:25:00,000T03:21:00,4-Jan-09,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-004T18:00:00,000T02:00:00,4-Jan-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-004T18:32:59,000T02:27:00,4-Jan-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.1117693 Rs exit= 9.1274759 Range altitude= 39913.536 km ... -39551.685,,,,,, 2009-004T18:46:00,000T02:00:00,4-Jan-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-004T18:47:29,000T02:00:00,4-Jan-09,CDA,SPASS Rider,DustRAM direction,RPX0180,,CDA RPXing 2009-004T19:47:29 NTH,"Nice to have - small/medium inclination - large ring extention, RPXing at > 8 Rs",,,,,, 2009-004T19:01:08,000T00:00:01,4-Jan-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 9.100 Rs, lat = 2 deg, phase = 154 deg",,,,,, 2009-004T20:00:00,004T15:59:00,4-Jan-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-004T20:46:00,000T05:04:00,4-Jan-09,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-004T20:59:59,003T18:16:01,4-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S47,Range enter= 9.1277862 Rs exit= 9.1101179 Range altitude= -40095.167 km ... 40518.247,,,,,, 2009-005T00:05:00,000T11:00:00,5-Jan-09,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics movie Part 1,"3x3 South Polar mosaics. . Each frame takes approx 7 min. to integrate, followed by 3 min reposition slews. repeat",,,,,, 2009-005T00:05:00,000T11:00:00,5-Jan-09,ISS,SPASS Rider,Saturn,SPOLEDYN,,"Auroral WAC 2X2 movie + lightning search, dayside","3x3 WAC mosaic in clear, HAL and IR2 filters on the night side, and CB2,MT2 on day side, ~3 im/footprint(10 min from VIMS) on average",,,,,, 2009-005T00:05:00,000T11:00:00,5-Jan-09,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2009-005T00:05:00,004T13:54:00,5-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-005T00:05:00,004T15:11:00,5-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-005T00:05:00,003T00:55:00,5-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-005T01:50:00,001T04:41:00,5-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-005T16:05:00,000T13:11:00,5-Jan-09,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics movie Part 2,"3x3 South Polar mosaics. . Each frame takes approx 7 min. to integrate, followed by 3 min reposition slews. repeat",,,,,, 2009-005T16:05:00,000T13:11:00,5-Jan-09,ISS,SPASS Rider,Saturn,SPOLEDYN,,Dayside WAC movie,"3x3 WAC mosaic in clear, HAL and IR2 filters on the night side, and CB2,MT2 on day side, ~3 im/footprint(10 min from VIMS) on average",,,,,, 2009-005T16:05:00,000T13:11:00,5-Jan-09,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2009-006T06:31:00,000T08:00:00,6-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-006T06:31:00,000T09:00:00,6-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-006T07:31:00,000T08:00:00,6-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_099IC_DSCAL09006_SP,rider,,,,,, 2009-006T16:11:00,000T01:15:00,6-Jan-09,ISS,Prime,Titan,MR2HAZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2009-006T16:11:00,000T01:15:00,6-Jan-09,CIRS,SPASS Rider,Titan,MR2HAZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-006T16:11:00,000T01:15:00,6-Jan-09,UVIS,SPASS Rider,Titan,MR2HAZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-006T17:26:00,000T01:00:00,6-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-006T18:26:00,000T11:10:00,6-Jan-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_099SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-006T18:26:00,000T11:10:00,6-Jan-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,South Pole Compsit ridealong with CIRS,Compsit Ridealong with CIRS,,,,,, 2009-006T18:27:00,000T11:10:00,6-Jan-09,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2009-006T19:00:00,001T19:16:00,6-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-007T06:16:00,000T09:00:00,7-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-007T06:31:00,000T04:29:00,7-Jan-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-007T07:16:00,000T08:00:00,7-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_099IC_DSCAL09007_SP,rider,,,,,, 2009-007T15:16:00,000T02:40:00,7-Jan-09,RADAR,SPASS Rider,Other,WU4SMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-007T15:56:00,000T02:00:00,7-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-007T17:56:00,000T01:30:00,7-Jan-09,RADAR,Prime,Titan,SMIDLCAL,,"Distant Titan Radiometry, South Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-007T19:26:00,000T01:00:00,7-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-007T20:26:00,000T08:00:00,7-Jan-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_099SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-007T20:26:00,000T08:00:00,7-Jan-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,South Pole Compsit ridealong with CIRS number 3 (s,Compsit Ridealong with CIRS,,,,,, 2009-008T01:00:00,001T12:59:00,8-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-008T04:26:00,000T01:10:00,8-Jan-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements based on shadow lengths, high res photo ops, low res photo ops, movies, etc. Need 50, want 70.",,,,,, 2009-008T06:16:00,000T09:00:00,8-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-008T07:16:00,000T08:00:00,8-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_099IC_DSCAL09008_SP,rider,,,,,, 2009-008T14:16:00,000T23:42:00,8-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-008T15:16:00,000T22:42:00,8-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S S47,Range enter= 9.1277862 Rs exit= 9.1101179 Range altitude= -40095.167 km ... 40518.247,,,,,, 2009-008T15:56:00,000T00:30:00,8-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 09","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-008T16:00:00,000T14:00:00,8-Jan-09,VIMS,Non-SPASS,SpacecraftActivity,DECONHIGH,Decontamination,Decontamination - High Power,IR Optics Decontamination at high power (88 Watts). Other instruments can observe during this request.,,,,,, 2009-008T16:26:00,000T01:00:00,8-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-008T17:26:00,000T11:10:00,8-Jan-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_099SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2009-008T20:00:00,000T09:10:00,8-Jan-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,Standard calibration/gain,,,,,, 2009-009T04:36:00,000T01:00:00,9-Jan-09,ISS,Prime,Saturn,1X2WP25,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 1X2 mosaic,,,,,, 2009-009T06:16:00,000T09:00:00,9-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-009T07:16:00,000T08:00:00,9-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_099IC_DSCAL09009_SP,rider,,,,,, 2009-009T10:00:00,000T00:10:00,9-Jan-09,RPWS,Non-SPASS,Saturn,HRSKR,High resolution saturn kilometric radiation observation,Highest Resolution SKR Observations,Obtain the highest resolution observations of Saturn Kilometric radiation(SKR) by using the RPWS HF-WBR mode at ~180 kbps,,,,,, 2009-009T11:59:00,000T02:00:00,9-Jan-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2009-009T13:52:43,000T00:00:01,9-Jan-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 9.6 d, inc = 69.0 deg, r = 19.727 Rs, phase = 27 deg",,,,,, 2009-009T13:58:00,000T01:18:00,9-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 9.1277862 Rs exit= 9.1101179 Range altitude= -40095.167 km ... 40518.247,,,,,, 2009-009T13:58:00,000T01:18:00,9-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-009T13:58:00,000T01:18:00,9-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-009T13:59:00,000T01:17:00,9-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-009T13:59:00,000T01:17:00,9-Jan-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-009T13:59:00,000T01:17:00,9-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-009T15:16:00,002T13:34:00,9-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-009T15:16:00,004T17:01:59,9-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 9.1277862 Rs exit= 9.1101179 Range altitude= -40095.167 km ... 40518.247,,,,,, 2009-009T15:16:00,000T00:43:00,9-Jan-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-009T15:16:00,002T13:34:00,9-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-009T15:16:00,001T16:44:00,9-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-009T15:16:00,002T16:15:00,9-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-009T15:21:00,000T00:02:00,9-Jan-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S47 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-009T15:55:00,000T01:15:00,9-Jan-09,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2009-009T15:55:00,000T01:15:00,9-Jan-09,CIRS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-009T15:55:00,000T01:15:00,9-Jan-09,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-009T15:59:00,000T00:05:00,9-Jan-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-009T16:04:00,000T00:33:00,9-Jan-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-009T16:37:00,000T00:22:59,9-Jan-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-009T16:59:59,001T07:00:01,9-Jan-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-009T17:10:00,000T09:36:00,9-Jan-09,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2009-009T17:10:00,000T09:36:00,9-Jan-09,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_100RI_EGPHASE114_VIMS,rider,,,,,, 2009-009T17:10:00,000T09:36:00,9-Jan-09,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2009-010T02:46:00,000T02:00:00,10-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-010T06:16:00,000T09:00:00,10-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-010T07:16:00,000T08:00:00,10-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09010_SP,rider,,,,,, 2009-010T15:50:00,000T05:40:00,10-Jan-09,ISS,Prime,rings(general),RADMRLPDF,,Color Radial Scan,"High res radial scans. Need 1, want 2 out of 7",,,,,, 2009-010T15:50:00,000T05:40:00,10-Jan-09,CIRS,SPASS Rider,rings(general),RADMRLPDF,,CIRS_100RI_RADMRLPDF001_ISS,rider,,,,,, 2009-010T15:50:00,000T05:40:00,10-Jan-09,VIMS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,"radial scan, low phase, unlit side","Cube Size (X,Z) = 64*12 hires, tau_IR = 320 msec, low phase angle.",,,,,, 2009-010T21:30:00,000T00:30:00,10-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-010T21:30:00,000T00:30:00,10-Jan-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_100RI_SATELLORB004_ISS,rider,,,,,, 2009-010T22:31:00,000T09:00:00,10-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-010T23:31:00,000T08:00:00,10-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09410_SP,rider,,,,,, 2009-011T00:00:00,000T02:00:00,11-Jan-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2009-011T02:00:00,002T17:15:00,11-Jan-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-011T08:00:00,000T20:50:00,11-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-011T08:05:00,000T00:30:00,11-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-011T08:35:00,000T02:00:00,11-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-011T10:35:00,000T11:25:00,11-Jan-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-011T10:35:00,000T11:25:00,11-Jan-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_100RF_FMOVIE003_ISS,rider,,,,,, 2009-011T10:35:00,000T11:25:00,11-Jan-09,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2009-011T22:31:00,000T09:00:00,11-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-011T23:31:00,000T08:00:00,11-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09011_SP,rider,,,,,, 2009-012T04:50:00,000T04:00:00,12-Jan-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS campaign,,,,,, 2009-012T04:50:00,000T04:00:00,12-Jan-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-012T04:50:00,000T04:00:00,12-Jan-09,MIMI,Non-SPASS,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-012T04:50:00,000T04:00:00,12-Jan-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-012T07:31:00,004T01:29:00,12-Jan-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-012T08:05:00,000T00:30:00,12-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-012T08:35:00,000T04:50:00,12-Jan-09,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. Priority 2. tau=20 ms.",,,,,, 2009-012T08:35:00,000T04:50:00,12-Jan-09,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_100RI_GAMCRUOCC015_VIMS,rider,,,,,, 2009-012T08:35:00,000T04:50:00,12-Jan-09,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,,,,,,,, 2009-012T08:50:00,001T20:20:00,12-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-012T08:50:00,001T20:20:00,12-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-012T08:50:00,001T20:20:00,12-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-012T13:25:00,000T08:15:00,12-Jan-09,UVIS,Prime,Star,URALP1CRU,,URSTAR,,,,,,, 2009-012T13:25:00,000T08:15:00,12-Jan-09,CIRS,SPASS Rider,rings(general),URALP1CRU,,CIRS_100RI_URALP1CRU001_UVIS,rider,,,,,, 2009-012T13:25:00,000T08:15:00,12-Jan-09,UVIS,SPASS Rider,Star,URALPCRU,,Support Imaging,NAC support images at the following times: 2009-012T14:14:00.0 2009-012T14:37:10.5 2009-012T16:19:40.5 2009-012T20:45:00.0 2009-012T20:22:00.0 2009-012T18:39:00.0,,,,,, 2009-012T20:00:00,001T02:00:00,12-Jan-09,CDA,SPASS Rider,Other,DECON,Decontamination,Decontamination,"CDA boresight off-sun, no resources (Watts, bps), resources covered by other request",,,,,, 2009-012T21:40:00,000T04:30:00,12-Jan-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-012T21:40:00,000T04:30:00,12-Jan-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_100RI_MNRNGSHAD004_ISS,rider,,,,,, 2009-013T02:10:00,000T09:30:00,13-Jan-09,VIMS,Prime,rings(general),ALPTRAOCC,Alpha TrA occultation,Ring stellar occ - alpTrA,"B ring, region 1; do one at priority 2, tau=80 ms",,,,,, 2009-013T02:10:00,000T09:30:00,13-Jan-09,CIRS,SPASS Rider,rings(general),ALPTRAOCC,Alpha TrA occultation,CIRS_100RI_ALPTRAOCC103_VIMS,rider,,,,,, 2009-013T02:10:00,000T09:30:00,13-Jan-09,UVIS,SPASS Rider,rings(general),ALPTRAOCC,Alpha TrA occultation,,,,,,,, 2009-013T03:00:00,001T01:35:00,13-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-013T12:17:00,000T09:00:00,13-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-013T13:17:00,000T08:00:00,13-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09013_SP,rider,,,,,, 2009-013T19:15:00,000T02:00:00,13-Jan-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-013T21:15:00,004T17:17:00,13-Jan-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-013T21:50:00,000T07:15:00,13-Jan-09,ISS,Prime,RingF,FRINGHRDF,,High Resolution F Ring Scan,Poorer opportunity. Complete high resolution (0-10Rs) longitudinal scan of the F ring. Dark face. Need at least 3 during XM. 2 of 27 as priority 1 and 1 as priority 2.,,,,,, 2009-013T21:50:00,000T07:15:00,13-Jan-09,CIRS,SPASS Rider,RingF,FRINGHRDF,,CIRS_100RF_FRINGHRDF001_ISS,rider,,,,,, 2009-013T21:50:00,000T07:15:00,13-Jan-09,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,null,,,,,, 2009-014T04:35:00,000T03:56:00,14-Jan-09,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-014T05:05:00,000T03:25:00,14-Jan-09,CAPS,Prime,Saturn,IMVP9PTG,,MAPS IMVP Campaign,Prime pointing during IMVP MAPS Campaign (Inner magn,,,,,, 2009-014T05:05:00,000T03:25:00,14-Jan-09,CAPS,SPASS Rider,Saturn,IMVP9,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2009-014T05:10:00,000T08:40:00,14-Jan-09,MAG,Non-SPASS,Saturn,IMVP9,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9",,,,,, 2009-014T05:10:00,000T08:40:00,14-Jan-09,MIMI,Non-SPASS,Saturn,IMVP9,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2009-014T08:17:59,000T02:27:00,14-Jan-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.1100240 Rs exit= 9.1260386 Range altitude= 39974.710 km ... -39502.901,,,,,, 2009-014T08:30:00,000T02:00:00,14-Jan-09,ISS,Prime,Rhea,RHEARPXHP,,Image Rhea's equatorial plane at high phase,Image Rhea's equatorial plane at high phase,,,,,, 2009-014T08:30:00,000T05:20:00,14-Jan-09,CAPS,SPASS Rider,Saturn,IMVP9,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2009-014T08:30:00,000T02:00:00,14-Jan-09,CIRS,SPASS Rider,Rhea,RHEARPXHP,,Rider in search for Rhea ring.,"Duration=02:00. AD=2.4-2.5, phase=155-150, (2, 57)-(-3, 60). 15.5, Centers; shutter first, last 3 minutes.",,,,,, 2009-014T08:30:00,000T02:00:00,14-Jan-09,VIMS,SPASS Rider,Rhea,RHEARPXHP,,Rhea RPXHP,Do 4 at priority 1.,,,,,, 2009-014T08:31:00,000T02:00:00,14-Jan-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-014T08:32:29,000T02:00:00,14-Jan-09,CDA,SPASS Rider,DustRAM direction,RPX0190,,CDA RPXing 2009-014T09:32:29 NTH,"Nice to have - small/medium inclination - large ring extention, RPXing at > 8 Rs",,,,,, 2009-014T08:45:11,000T00:00:01,14-Jan-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 9.098 Rs, lat = 2 deg, phase = 153 deg",,,,,, 2009-014T10:30:00,000T01:30:00,14-Jan-09,ISS,Prime,rings(general),LOINCSTR,,Strange Ringlet Observation at low Elevation,Strange Ringlet Observation at low Elevation. Need 15 out of 19.,,,,,, 2009-014T10:30:00,000T01:30:00,14-Jan-09,CIRS,SPASS Rider,rings(general),LOINCSTR,,CIRS_100RI_LOINCSTR001_ISS,rider,,,,,, 2009-014T10:31:00,000T05:04:00,14-Jan-09,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-014T10:44:59,004T16:58:01,14-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 9.1263511 Rs exit= 9.1113948 Range altitude= -40046.470 km ... 40041.457,,,,,, 2009-014T12:00:00,000T05:30:00,14-Jan-09,CIRS,Prime,rings(general),TDIFS20HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-014T12:00:00,000T05:30:00,14-Jan-09,CIRS,SPASS Rider,rings(general),TDIFS20HP,,CIRS_100RI_TDIFS20HP001_SI,,,,,,, 2009-014T12:00:00,000T05:30:00,14-Jan-09,UVIS,SPASS Rider,rings(general),TDIFS20HP,,,,,,,,, 2009-014T13:50:00,004T13:54:00,14-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-014T13:50:00,004T00:42:00,14-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-014T13:50:00,003T01:10:00,14-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-014T15:35:00,000T06:42:00,14-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-014T17:30:00,000T03:32:00,14-Jan-09,VIMS,Prime,rings(general),COMPHILIT,High phase sunlit ring radial scan,Ring COMPHILIT,Do 4 at priority 1.,,,,,, 2009-014T17:30:00,000T03:32:00,14-Jan-09,CIRS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,CIRS_100RI_COMPHILIT122_VIMS,rider,,,,,, 2009-014T17:30:00,000T03:32:00,14-Jan-09,UVIS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,,,,,,,, 2009-014T22:17:00,000T19:03:00,14-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-014T22:17:00,000T09:00:00,14-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-014T23:17:00,000T08:00:00,14-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09014_SP,rider,,,,,, 2009-015T07:50:00,000T02:00:00,15-Jan-09,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"intermediate phase, lit-face ring photometry","intermediate lit #4: B = -68, phase = 90, B' = -3.2",,,,,, 2009-015T07:50:00,000T02:00:00,15-Jan-09,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_100RI_PHOTLIT002_ISS,rider,,,,,, 2009-015T07:50:00,000T02:00:00,15-Jan-09,VIMS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,PhotLit mosaic,Main ring photometry,,,,,, 2009-015T09:50:00,000T04:55:00,15-Jan-09,UVIS,Prime,Star,URGAMCAS,Stellar occultation,URSTAR,,,,,,, 2009-015T09:50:00,000T04:55:00,15-Jan-09,CIRS,SPASS Rider,rings(general),URGAMCAS,Stellar occultation,CIRS_100RI_URGAMCAS001_UVIS,rider,,,,,, 2009-015T09:50:00,000T04:55:00,15-Jan-09,UVIS,SPASS Rider,Star,URGAMCAS,Stellar occultation,Support Imaging,NAC support images at the following times: 2009-015T13:53:00.0 2009-015T13:42:10.0 2009-015T13:06:33.5,,,,,, 2009-015T09:50:00,000T04:55:00,15-Jan-09,VIMS,SPASS Rider,rings(general),URGAMCAS,Stellar occultation,VIMS rider on UVIS star occ,radial scan of rings,,,,,, 2009-015T14:45:00,000T07:00:00,15-Jan-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-015T22:17:00,000T09:00:00,15-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-015T23:17:00,000T08:00:00,15-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09015_SP,rider,,,,,, 2009-016T07:50:00,000T01:15:00,16-Jan-09,ISS,Prime,Titan,MR2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2009-016T07:50:00,000T01:15:00,16-Jan-09,CIRS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-016T07:50:00,000T01:15:00,16-Jan-09,UVIS,SPASS Rider,Titan,MR2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-016T07:50:00,000T01:15:00,16-Jan-09,VIMS,SPASS Rider,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 25.7 range 1.6 Mkm",,,,,, 2009-016T09:00:00,002T05:32:00,16-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-016T09:05:00,000T01:45:00,16-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-016T09:05:00,000T01:45:00,16-Jan-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_100RI_SATELLORB009_ISS,rider,,,,,, 2009-016T10:50:00,000T02:00:00,16-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-016T12:50:00,000T01:45:00,16-Jan-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-016T12:50:00,000T01:45:00,16-Jan-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_100RI_MNRNGSHAD008_ISS,rider,,,,,, 2009-016T14:35:00,000T08:00:00,16-Jan-09,CIRS,Prime,rings(general),TMAPS45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-016T14:35:00,000T08:00:00,16-Jan-09,CIRS,SPASS Rider,rings(general),TMAPS45LP,,CIRS_100RI_TMAPS45LP001_SI,,,,,,, 2009-016T14:35:00,000T08:00:00,16-Jan-09,UVIS,SPASS Rider,rings(general),TMAPS45LP,,,,,,,,, 2009-016T14:35:00,000T08:00:00,16-Jan-09,VIMS,SPASS Rider,rings(general),TMAPS45LP,,VIMS rider on CIRS,CIRS scan of rings,,,,,, 2009-016T22:35:00,000T04:25:00,16-Jan-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE",Do 6 at priority 2,,,,,, 2009-016T22:35:00,000T04:25:00,16-Jan-09,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_100RI_LATPHASE103_VIMS,rider,,,,,, 2009-016T22:35:00,000T04:25:00,16-Jan-09,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,,,,,,,, 2009-017T03:00:00,000T02:15:00,17-Jan-09,ISS,Prime,rings(general),RETARMRLP,,Medium res retargetables,Medium Res Retarg of small ring region satellites. Need 25 of 54.,,,,,, 2009-017T03:00:00,000T02:15:00,17-Jan-09,CIRS,SPASS Rider,rings(general),RETARMRLP,,CIRS_100RI_RETARMRLP002_ISS,rider,,,,,, 2009-017T05:47:00,000T09:00:00,17-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-017T06:47:00,000T08:00:00,17-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09017_SP,rider,,,,,, 2009-017T15:00:00,001T12:44:00,17-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-017T15:20:00,000T00:40:00,17-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-017T16:00:00,000T12:02:00,17-Jan-09,CIRS,Prime,rings(general),SUBMS20LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-017T16:00:00,000T12:02:00,17-Jan-09,CIRS,SPASS Rider,rings(general),SUBMS20LP,,CIRS_100RI_SUBMS20LP001_SI,,,,,,, 2009-017T16:00:00,000T12:02:00,17-Jan-09,ISS,SPASS Rider,rings(general),SUBMS20LP,,,Spoke periodicity movie. riding along on CIRS SUBM obs.,,,,,, 2009-017T16:00:00,000T12:02:00,17-Jan-09,UVIS,SPASS Rider,rings(general),SUBMS20LP,,,,,,,,, 2009-017T16:00:00,000T12:02:00,17-Jan-09,VIMS,SPASS Rider,rings(general),SUBMS20LP,,VIMS rider on CIRS,VIMS ridealong with CIRS,,,,,, 2009-018T05:32:00,000T09:00:00,18-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-018T06:02:00,000T11:05:36,18-Jan-09,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4kbps data,,,,,, 2009-018T06:02:00,000T08:00:00,18-Jan-09,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2009-018T06:32:00,000T08:00:00,18-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_100IC_DSCAL09018_SP,rider,,,,,, 2009-018T14:32:00,000T01:55:00,18-Jan-09,RADAR,SPASS Rider,Other,WU4SRCCAL,,Warm Up for Microwave Source Calibration,Warmup for calibration and science data collection.,,,,,, 2009-018T14:32:00,000T13:12:00,18-Jan-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-018T14:32:00,003T04:03:00,18-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-018T14:32:00,000T13:11:00,18-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-018T15:02:00,000T01:25:00,18-Jan-09,ISS,Prime,Titan,M30R2CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.3 range 1.6 Mkm",,,,,, 2009-018T15:02:00,000T01:25:00,18-Jan-09,CIRS,SPASS Rider,Titan,M30R2CLDF,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-018T15:02:00,000T01:25:00,18-Jan-09,UVIS,SPASS Rider,Titan,M30R2CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-018T16:27:00,000T07:00:00,18-Jan-09,RADAR,Prime,Other,SRCRADCAL,RADAR microwave source radiometric calibration,Radiometric Microwave Sources Calibration,"Scan the Sun, Saturn, and microwave sources while collecting radiometry data.",,,,,, 2009-018T16:27:00,000T05:30:00,18-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,SRCRADCAL,RADAR microwave source radiometric calibration,CIRS_100IC_SRCRADCAL001_RADAR,rider,,,,,, 2009-018T16:27:00,000T05:00:00,18-Jan-09,ISS,SPASS Rider,Other,SRCRADCAL,RADAR microwave source radiometric calibration,ISS WAC dark current calibration,ISS WAC dark current calibration,,,,,, 2009-018T22:00:00,000T07:23:44,18-Jan-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16kbps data,,,,,, 2009-018T23:27:00,000T03:25:00,18-Jan-09,VIMS,Prime,Saturn,SREGMAP,Regional mapping mosaics of the southern hemisphere,Southern Regional Map,"3*3 mosaic, on 10-minute centers",,,,,, 2009-018T23:27:00,000T03:25:00,18-Jan-09,ISS,SPASS Rider,Saturn,SREGMAP,Regional mapping mosaics of the southern hemisphere,WAC polarimetry rider,WAC polarimetry,,,,,, 2009-019T02:52:00,000T02:00:00,19-Jan-09,ISS,Prime,Dione,080W009PH,,Dione lon/phase angle observation,"Turn UVIS_FUV to Dione; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2009-019T02:52:00,000T02:00:00,19-Jan-09,CIRS,SPASS Rider,Dione,089W008PH,,CIRS_100DI_089W008PH001_ISS,rider,,,,,, 2009-019T02:52:00,000T02:00:00,19-Jan-09,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-019T02:52:00,000T02:00:00,19-Jan-09,VIMS,SPASS Rider,Dione,080W009PH,,spectral cubes,Phase study,,,,,, 2009-019T03:37:34,000T00:00:01,19-Jan-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 9.6 d, inc = 69.0 deg, r = 19.727 Rs, phase = 27 deg",,,,,, 2009-019T03:43:00,004T18:20:59,19-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 9.1263511 Rs exit= 9.1113948 Range altitude= -40046.470 km ... 40041.457,,,,,, 2009-019T03:43:00,002T18:47:00,19-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-019T03:44:00,002T14:51:00,19-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-019T03:44:00,000T01:59:00,19-Jan-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2009-019T03:44:00,001T18:16:00,19-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-019T05:32:00,000T09:00:00,19-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-019T05:43:00,004T15:17:00,19-Jan-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-019T06:02:00,000T08:23:28,19-Jan-09,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4kbps data,,,,,, 2009-019T06:02:00,000T08:00:00,19-Jan-09,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2009-019T06:32:00,000T08:00:00,19-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09019_SP,rider,,,,,, 2009-019T15:12:00,000T13:11:00,19-Jan-09,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2009-020T04:23:00,000T00:30:00,20-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-020T05:33:00,000T09:00:00,20-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-020T06:33:00,000T08:00:00,20-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09020_SP,rider,,,,,, 2009-020T15:13:00,000T13:40:00,20-Jan-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning N. hemisphere, may be split in half by downlink",,,,,, 2009-020T15:13:00,000T13:40:00,20-Jan-09,VIMS,SPASS Rider,Saturn,FIRMAP,Far infrared map,CIRS FIRMAP Ridealong,Ridealong with CIRS,,,,,, 2009-020T22:00:00,000T20:35:00,20-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-021T05:33:00,000T09:00:00,21-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-021T05:45:00,000T06:00:00,21-Jan-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-021T06:33:00,000T08:00:00,21-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09021_SP,rider,,,,,, 2009-021T15:13:00,000T07:12:00,21-Jan-09,UVIS,Prime,Saturn,AURORA,Saturn aurora,Saturn Aurora,"Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2009-021T15:13:00,000T07:12:00,21-Jan-09,CIRS,SPASS Rider,Saturn,AURORA,Saturn aurora,,null,,,,,, 2009-021T15:13:00,000T07:12:00,21-Jan-09,ISS,SPASS Rider,Saturn,AURORA,Saturn aurora,"Hi-res NAC mosaic of N Polar Hexagon in MT2,CB2,M","4 pickets spaced 1h 30m. 3x1 NAC in MT3, CB2, MT2, and BL1.",,,,,, 2009-021T15:13:00,000T07:12:00,21-Jan-09,VIMS,SPASS Rider,Saturn,AURORA,Saturn aurora,Aurora,Aurora. One frame is 70-minutes (1 sec integrations). Others are shorter. Ridealong with UVIS,,,,,, 2009-021T18:35:00,000T04:00:00,21-Jan-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS campaign,,,,,, 2009-021T18:35:00,000T04:00:00,21-Jan-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-021T18:35:00,000T04:00:00,21-Jan-09,MIMI,Non-SPASS,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-021T18:35:00,000T04:00:00,21-Jan-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-021T22:25:00,000T04:50:00,21-Jan-09,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. SAT segment.",,,,,, 2009-021T22:25:00,000T04:50:00,21-Jan-09,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_101_RI_GAMCRUOCC016_VIMS,rider,,,,,, 2009-021T22:30:00,003T23:15:00,21-Jan-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-021T22:35:00,001T20:20:00,21-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-021T22:35:00,001T20:20:00,21-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-021T22:35:00,001T19:45:00,21-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-022T03:15:00,000T00:42:00,22-Jan-09,VIMS,Prime,Saturn,REGDYN,,Dynamics mosaic 1,"2*2 mosiac, 10 minute centers",,,,,, 2009-022T03:57:00,000T01:22:00,22-Jan-09,UVIS,Prime,Star,BETCRU,,Saturn Occults Beta Cru,UVIS FUV Occultation slit boresite on star for 40 minutes,,,,,, 2009-022T03:57:00,000T01:22:00,22-Jan-09,CIRS,SPASS Rider,rings(general),BETCRU,,CIRS_101_RI_BETCRU001_UVIS,rider,,,,,, 2009-022T03:57:00,000T01:22:00,22-Jan-09,ISS,SPASS Rider,Star,BETCRU,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2009-022T05:19:00,000T01:44:00,22-Jan-09,VIMS,Prime,Saturn,REGDYN,,Dynamics mosaic 2,"3*3 mosiac, 10 minute centers",,,,,, 2009-022T07:03:00,000T01:30:00,22-Jan-09,UVIS,Prime,Star,BETCRU,,Saturn Occults Beta Cru,UVIS FUV Occultation slit boresite on star for 40 minutes,,,,,, 2009-022T07:03:00,000T01:30:00,22-Jan-09,CIRS,SPASS Rider,rings(general),BETCRU,,CIRS_101_RI_BETCRU002_UVIS,rider,,,,,, 2009-022T07:03:00,000T01:30:00,22-Jan-09,ISS,SPASS Rider,Star,BETCRU,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2009-022T08:33:00,000T12:00:00,22-Jan-09,VIMS,Prime,Saturn,REGDYN,,Dynamics mosaic 3,"3*3 mosiac, 10 minute centers . Repeat",,,,,, 2009-022T16:45:00,001T00:35:00,22-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-022T20:33:00,000T01:14:00,22-Jan-09,CIRS,SPASS Rider,rings(general),OPNAV,Optical navigation image,CIRS_101_RI_OPNAV221_NAV,rider,,,,,, 2009-022T21:48:00,000T09:00:00,22-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-022T22:18:00,000T08:23:28,22-Jan-09,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4kbps data,,,,,, 2009-022T22:18:00,000T08:00:00,22-Jan-09,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2009-022T22:48:00,000T08:00:00,22-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09022_SP,rider,,,,,, 2009-023T07:28:00,000T06:47:00,23-Jan-09,UVIS,Prime,Saturn,AURORA,Saturn aurora,Saturn Aurora,"Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2009-023T07:28:00,000T06:47:00,23-Jan-09,CIRS,SPASS Rider,Saturn,AURORA,Saturn aurora,,null,,,,,, 2009-023T07:28:00,000T06:47:00,23-Jan-09,ISS,SPASS Rider,Saturn,AURORA,Saturn aurora,Auroral WAC 2X2 movie + lightning search. North.,"Auroral WAC movie. 6 time steps in a 1x2 mosaic in clear, HAL and IR2 filters. Space pickets one hour apart.",,,,,, 2009-023T07:28:00,000T06:47:00,23-Jan-09,VIMS,SPASS Rider,Saturn,AURORA,Saturn aurora,Aurora,Aurora. One frame is 70-minutes (1 sec integrations). Others are shorter. Ridealong with UVIS,,,,,, 2009-023T14:15:00,000T04:05:00,23-Jan-09,ISS,Prime,Mimas,086W151PH,,Mimas lon/phase angle observation,"Turn UVIS_FUV to Mimas; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2009-023T14:15:00,000T04:05:00,23-Jan-09,CIRS,SPASS Rider,Mimas,086W151PH,,CIRS_101MI_086W151PH001_ISS,rider,,,,,, 2009-023T14:15:00,000T04:05:00,23-Jan-09,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-023T14:15:00,000T04:05:00,23-Jan-09,VIMS,SPASS Rider,Mimas,086W151PH,,spectral cubes,Phase study,,,,,, 2009-023T14:33:00,000T02:16:32,23-Jan-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16kbps data,,,,,, 2009-023T18:20:00,000T02:48:00,23-Jan-09,CAPS,Prime,Saturn,IMVP9PTG,,MAPS IMVP Campaign,Prime pointing during IMVP MAPS Campaign (Inner magn,,,,,, 2009-023T18:20:00,000T09:15:00,23-Jan-09,CAPS,SPASS Rider,Saturn,IMVP9,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2009-023T18:20:00,000T09:15:00,23-Jan-09,MIMI,Non-SPASS,Saturn,IMVP9,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2009-023T18:20:00,000T02:48:00,23-Jan-09,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-023T18:55:00,000T08:40:00,23-Jan-09,MAG,Non-SPASS,Saturn,IMVP9,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9",,,,,, 2009-023T21:00:00,000T02:00:00,23-Jan-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-023T21:48:00,000T09:00:00,23-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-023T22:03:59,000T02:27:00,23-Jan-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.1113059 Rs exit= 9.1280150 Range altitude= 39497.974 km ... -39967.552,,,,,, 2009-023T22:16:00,000T02:00:00,23-Jan-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-023T22:17:29,000T02:00:00,23-Jan-09,CDA,SPASS Rider,DustRAM direction,RPX0200,,CDA RPXing 2009-023T23:17:29 NTH,"Nice to have - small/medium inclination - large ring extention, RPXing at > 8 Rs",,,,,, 2009-023T22:29:13,000T00:00:01,23-Jan-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 9.100 Rs, lat = 2 deg, phase = 153 deg",,,,,, 2009-023T22:48:00,000T08:00:00,23-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09023_SP,rider,,,,,, 2009-023T23:00:00,000T07:48:00,23-Jan-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-024T00:30:59,004T16:38:01,24-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 9.1283321 Rs exit= 9.1070718 Range altitude= -40511.011 km ... 40403.450,,,,,, 2009-024T03:35:00,004T13:34:00,24-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-024T03:35:00,002T16:43:00,24-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-024T03:35:00,003T01:25:00,24-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-024T05:20:00,001T01:40:00,24-Jan-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-024T06:48:00,001T00:00:00,24-Jan-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-024T07:28:00,000T13:40:00,24-Jan-09,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics mosaic 1,"First, a 70-minute frame (1-sec per pixel integrations). Then 3*3 mosaic, on 10-minute centers per frame. Then repeat (both 70-minute and 3*3 mosaic) until end of the observation.",,,,,, 2009-024T07:28:00,000T13:40:00,24-Jan-09,ISS,SPASS Rider,Saturn,SPOLEDYN,,Auroral WAC 1X2 movie + lightning search,"Auroral WAC rider on VIMS, during the mosaic part of VIMS pointing make one clear filter WAC image. 70 min wait, then 1 image per 10 min for 90 min.",,,,,, 2009-024T07:28:00,000T13:40:00,24-Jan-09,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2009-024T21:48:00,000T09:00:00,24-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-024T22:48:00,000T08:00:00,24-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09024_SP,rider,,,,,, 2009-025T00:00:00,000T00:34:08,25-Jan-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2009-025T06:48:00,003T10:21:00,25-Jan-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-025T07:28:00,000T01:15:00,25-Jan-09,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 126 range 1.6 Mkm",,,,,, 2009-025T07:28:00,000T01:15:00,25-Jan-09,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-025T07:28:00,000T01:15:00,25-Jan-09,UVIS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-025T08:43:00,000T12:10:00,25-Jan-09,VIMS,Prime,Saturn,SPOLEDYN,,South Pole dynamics mosaic 2,"Polar mosaic. At beginning, 70-min frame centered at pole. Then 3x3 mosaics on 10-minute centers 3 times. Repeat",,,,,, 2009-025T08:43:00,000T12:10:00,25-Jan-09,ISS,SPASS Rider,Saturn,SPOLEDYN,,"Polar movie with the WAC in MT2,CB2,MT2, BL1","WAC in MT3, CB2, MT2, and BL1 following the VIMS pointing: 1 footprint (4 im) first 70 min, then 1 footprint(4 im) per 10 min at each part of VIMS mosaic. cycle~32 im/160 min.",,,,,, 2009-025T08:43:00,000T12:10:00,25-Jan-09,UVIS,SPASS Rider,Saturn,SPOLEDYN,,Saturn Aurora,Rider on VIMS SPOLEDYN observations,,,,,, 2009-025T21:33:00,000T09:00:00,25-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-025T21:45:00,002T19:24:00,25-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-025T22:33:00,000T08:00:00,25-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09025_SP,rider,,,,,, 2009-026T07:13:00,000T11:05:00,26-Jan-09,VIMS,SPASS Rider,Saturn,FIRMAP,Far infrared map,CIRS FIRMAP Ridealong,Ridealong with CIRS,,,,,, 2009-026T07:18:00,000T11:00:00,26-Jan-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning S. hemisphere + pole, may be split in half by downlink",,,,,, 2009-026T18:18:00,000T02:00:00,26-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-026T20:18:00,000T06:45:00,26-Jan-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-027T03:03:00,000T00:30:00,27-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-027T03:03:00,003T03:15:00,27-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-027T05:00:00,001T12:09:00,27-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-027T05:03:00,000T09:00:00,27-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-027T06:03:00,000T08:00:00,27-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09027_SP,rider,,,,,, 2009-027T14:43:00,000T13:10:00,27-Jan-09,UVIS,Prime,Saturn,AURORA,Saturn aurora,Saturn Aurora,"Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews.",,,,,, 2009-027T14:43:00,000T13:10:00,27-Jan-09,CIRS,SPASS Rider,Saturn,AURORA,Saturn aurora,,null,,,,,, 2009-027T14:43:00,000T13:10:00,27-Jan-09,ISS,SPASS Rider,Saturn,AURORA,Saturn aurora,Dayside WAC 2X2 5-filter movie. North.,"Dayside WAC movie. 8 time steps in a 2x2 mosaic in CB3,MT2,CB2,MT2,BL Space pickets 1.5 hours apart.",,,,,, 2009-027T14:43:00,000T13:10:00,27-Jan-09,VIMS,SPASS Rider,Saturn,AURORA,Saturn aurora,Aurora,"Aurora. Every 6.5 hours, One frame is 70-minutes (1 sec integrations). Others are shorter. Ridealong with UVIS",,,,,, 2009-028T03:53:00,000T00:30:00,28-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-028T05:03:00,000T09:00:00,28-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-028T06:03:00,000T08:00:00,28-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_101IC_DSCAL09028_SP,rider,,,,,, 2009-028T14:43:00,000T02:17:00,28-Jan-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-028T14:43:00,000T02:17:00,28-Jan-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2009-028T17:00:00,000T01:15:00,28-Jan-09,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 45.8 range 2.3 Mkm",,,,,, 2009-028T17:00:00,000T01:15:00,28-Jan-09,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-028T17:00:00,000T01:15:00,28-Jan-09,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-028T17:01:56,000T00:00:01,28-Jan-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 9.5 d, inc = 69.0 deg, r = 19.674 Rs, phase = 27 deg",,,,,, 2009-028T17:09:00,002T14:41:00,28-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-028T17:09:00,004T18:02:59,28-Jan-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 9.1283321 Rs exit= 9.1070718 Range altitude= -40511.011 km ... 40403.450,,,,,, 2009-028T17:09:00,000T02:00:00,28-Jan-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,"Ridealong, full rate inner mag composition measurement",,,,,, 2009-028T17:09:00,001T17:51:00,28-Jan-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-028T17:09:00,002T17:51:00,28-Jan-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-028T18:15:00,000T03:24:00,28-Jan-09,ISS,Prime,rings(general),GRINGARC,,G-ring arc observation,"G-ring arc observation, need 2 of 15 opportunities",,,,,, 2009-028T19:09:00,001T11:09:00,28-Jan-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-028T21:39:00,000T02:00:00,28-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-028T23:39:00,000T04:29:00,28-Jan-09,CIRS,Prime,rings(general),COMP,Sit and stare to derive composition,CIRS_102RI_COMP029_PRIME;,null,,,,,, 2009-028T23:39:00,000T04:29:00,28-Jan-09,CIRS,SPASS Rider,rings(general),COMP,Sit and stare to derive composition,CIRS_102RI_COMP029_SI,,,,,,, 2009-029T00:48:00,000T07:00:00,29-Jan-09,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. Last 3 hours required to be tracked at DSS-25 and DSS-14 in 1-way mode.,,,,,, 2009-029T03:48:00,000T05:00:00,29-Jan-09,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2009-029T04:48:00,000T09:00:00,29-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-029T05:48:00,000T08:00:00,29-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09029_SP,rider,,,,,, 2009-029T07:48:00,000T01:00:00,29-Jan-09,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2009-029T14:00:00,000T03:29:04,29-Jan-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16kbps data,,,,,, 2009-029T14:28:00,000T06:10:00,29-Jan-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_102SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-029T14:28:00,000T06:10:00,29-Jan-09,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2009-029T21:18:00,000T09:00:00,29-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-029T21:48:00,000T08:23:28,29-Jan-09,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4kbps data,,,,,, 2009-029T21:48:00,000T08:00:00,29-Jan-09,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2009-029T22:18:00,000T08:00:00,29-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09429_SP,rider,,,,,, 2009-030T06:18:00,000T00:40:00,30-Jan-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_102RI_DEEPSPACE030_SP,rider,,,,,, 2009-030T06:18:00,003T02:42:00,30-Jan-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-030T06:18:00,001T01:32:00,30-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-030T06:58:00,000T01:15:00,30-Jan-09,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 26.5 range 2.3 Mkm",,,,,, 2009-030T06:58:00,000T01:15:00,30-Jan-09,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-030T06:58:00,000T01:15:00,30-Jan-09,UVIS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-030T08:13:00,000T11:20:00,30-Jan-09,ISS,Prime,RingF,FRSTRCHAN,F ring streamer movie,F RING STREAMER/CHANNEL,"Movie of streamer-channel feature raised in F ring by Prometheus apoapse passage. Need as close to 1 Prom orbital period as possible. Sometimes can be day before or day after. Want 12. 6 of 49 as priority 1, 6 of 49 as priority 2.",,,,,, 2009-030T08:13:00,000T11:20:00,30-Jan-09,CIRS,SPASS Rider,rings(general),FRSTRCHAN,F ring streamer movie,CIRS_102RI_FRSTRCHAN001_ISS,rider,,,,,, 2009-030T08:20:00,000T06:24:00,30-Jan-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16kbps data,,,,,, 2009-030T11:00:00,000T20:50:00,30-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-030T19:33:00,000T00:30:00,30-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-030T19:33:00,000T00:30:00,30-Jan-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_102RI_SATELLORB007_ISS,rider,,,,,, 2009-030T21:18:00,000T09:00:00,30-Jan-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-030T21:48:00,000T08:23:28,30-Jan-09,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4kbps data,,,,,, 2009-030T21:48:00,000T08:00:00,30-Jan-09,RPWS,Non-SPASS,Saturn,HIRATE,High rate mode,"MAPS MB,A Campaign",null,,,,,, 2009-030T22:18:00,000T08:00:00,30-Jan-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09030_SP,rider,,,,,, 2009-031T06:58:00,000T02:45:00,31-Jan-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-031T06:58:00,000T02:45:00,31-Jan-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_102RI_DEEPSPACE031_CAPS,rider,,,,,, 2009-031T07:50:00,000T03:45:00,31-Jan-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS campaign,,,,,, 2009-031T07:50:00,000T03:45:00,31-Jan-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-031T07:50:00,000T03:45:00,31-Jan-09,MIMI,Non-SPASS,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-031T07:50:00,000T03:45:00,31-Jan-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-031T09:43:00,000T00:40:00,31-Jan-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-031T09:43:00,000T00:40:00,31-Jan-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_102RI_SATELLORB008_ISS,rider,,,,,, 2009-031T10:23:00,000T01:15:00,31-Jan-09,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 23.9 range 2 Mkm",,,,,, 2009-031T10:23:00,000T01:15:00,31-Jan-09,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-031T10:23:00,000T01:15:00,31-Jan-09,UVIS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-031T11:00:00,004T01:00:00,31-Jan-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-031T11:35:00,001T20:30:00,31-Jan-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-031T11:35:00,001T20:30:00,31-Jan-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-031T11:35:00,001T20:30:00,31-Jan-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-031T11:38:00,000T04:50:00,31-Jan-09,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"F-D Rings, do 9 of 17. Priority 2. tau=60 ms.",,,,,, 2009-031T11:38:00,000T04:50:00,31-Jan-09,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_102RI_GAMCRUOCC017_VIMS,rider,,,,,, 2009-031T11:38:00,000T04:50:00,31-Jan-09,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,URSTAR,,,,,,, 2009-031T16:28:00,000T02:02:00,31-Jan-09,ISS,Prime,Other,RETARG,Retargetable observation,ISS Retarg,ISS retargetable for yet-undiscovered moons or ring features,,,,,, 2009-031T16:28:00,000T02:02:00,31-Jan-09,CIRS,SPASS Rider,rings(general),RETARG,Retargetable observation,CIRS_102RI_RETARG001_ISS,rider,,,,,, 2009-031T18:30:00,000T04:30:00,31-Jan-09,UVIS,Prime,Star,URBETCEN,Stellar occultation,URSTAR,,,,,,, 2009-031T18:30:00,000T04:30:00,31-Jan-09,CIRS,SPASS Rider,rings(general),URBETCEN,Stellar occultation,CIRS_102RI_URBETCEN001_UVIS,rider,,,,,, 2009-031T18:30:00,000T04:30:00,31-Jan-09,UVIS,SPASS Rider,Star,URBETCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2009-031T19:17:35.0 2009-031T19:30:20.0 2009-031T20:09:00.0,,,,,, 2009-031T23:00:00,000T06:07:00,31-Jan-09,ISS,Prime,rings(general),PHOTDRKBK,,"high-latitude, dark-face ring photometry","high latitude unlit #3: B ~ 65, phase ~ 70, B = -2.9",,,,,, 2009-031T23:00:00,000T06:07:00,31-Jan-09,CIRS,SPASS Rider,rings(general),PHOTDRKBK,,CIRS_102RI_PHOTDRKBK001_ISS,rider,,,,,, 2009-031T23:00:00,000T06:07:00,31-Jan-09,VIMS,SPASS Rider,rings(general),PHOTDRKBK,,PhotDark mosaic,Main ring photometry,,,,,, 2009-032T05:07:00,000T09:15:00,1-Feb-09,VIMS,Prime,rings(general),ALPTRAOCC,Alpha TrA occultation,Ring stellar occ - alpTrA,"B ring, region 1; do one at priority 2",,,,,, 2009-032T05:07:00,000T09:15:00,1-Feb-09,CIRS,SPASS Rider,rings(general),ALPTRAOCC,Alpha TrA occultation,CIRS_102RI_ALPTRAOCC105_VIMS,rider,,,,,, 2009-032T05:07:00,000T09:15:00,1-Feb-09,UVIS,SPASS Rider,rings(general),ALPTRAOCC,Alpha TrA occultation,URSTAR,,,,,,, 2009-032T05:55:00,000T15:09:00,1-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-032T14:22:00,000T06:02:00,1-Feb-09,CIRS,Prime,rings(general),VENCUNMP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-032T14:22:00,000T06:02:00,1-Feb-09,CIRS,SPASS Rider,rings(general),VENCUNMP,,CIRS_102RI_VENCUNMP001_SI,,,,,,, 2009-032T14:22:00,000T06:02:00,1-Feb-09,UVIS,SPASS Rider,rings(general),VENCUNMP,,URSPEC,,,,,,, 2009-032T20:24:00,000T00:40:00,1-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_102RI_DEEPSPACE032_SP,rider,,,,,, 2009-032T21:04:00,000T09:21:00,1-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-032T21:04:00,000T09:00:00,1-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-032T22:04:00,000T08:00:00,1-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09032_SP,rider,,,,,, 2009-033T06:04:00,000T00:30:00,2-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,WAYPTTURN,Waypoint turn,CIRS_102IC_WAYPTTURN033_SP,For deep space prior to ISS observation. FP1+FP3.,,,,,, 2009-033T06:34:00,000T00:36:00,2-Feb-09,ISS,Prime,Rhea,GEOLOG,Geologic study,Rhea mapping,"1x2 NAC mosaic, then sit'n'stare.",,,,,, 2009-033T06:34:00,000T00:36:00,2-Feb-09,CIRS,SPASS Rider,Rhea,GEOLOG,Geologic study,CIRS_102RH_GEOLOG001_ISS,rider,,,,,, 2009-033T06:34:00,000T00:36:00,2-Feb-09,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude and phase coverage,Longitude and phase coverage,,,,,, 2009-033T06:34:00,000T00:36:00,2-Feb-09,VIMS,SPASS Rider,Rhea,GEOLOG,Geologic study,mapping cubes,Lat-Long Vgr class,,,,,, 2009-033T07:10:00,000T01:00:00,2-Feb-09,UVIS,Prime,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2009-033T07:10:00,000T01:00:00,2-Feb-09,CIRS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,CIRS_102RH_ICYMAP001_UVIS rider,rider. FP1+FP3 only.,,,,,, 2009-033T08:05:00,000T08:40:00,2-Feb-09,CAPS,SPASS Rider,Saturn,IMVP9,,MAPS IMVP Campaign,Part of IMVP MAPS Campaign (Inner magn,,,,,, 2009-033T08:05:00,000T08:40:00,2-Feb-09,MAG,Non-SPASS,Saturn,IMVP9,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9",,,,,, 2009-033T08:05:00,000T08:40:00,2-Feb-09,MIMI,Non-SPASS,Saturn,IMVP9,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2009-033T08:05:00,000T08:40:00,2-Feb-09,RPWS,Non-SPASS,co-rotation,IMVP9,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-033T08:10:00,000T02:30:00,2-Feb-09,ISS,Prime,Rhea,GEOLOG,Geologic study,Rhea mapping and color,"2x3 mosaic, then sit'n'stare over lit hemisphere, then 2x3 mosaic (~09:40 UTC), then sit'n'stare again.",,,,,, 2009-033T08:10:00,000T02:30:00,2-Feb-09,CIRS,SPASS Rider,Rhea,GEOLOG,Geologic study,CIRS_102RH_GEOLOG002_ISS rider,rider,,,,,, 2009-033T09:00:00,000T02:00:00,2-Feb-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2009-033T10:40:00,000T00:20:00,2-Feb-09,CIRS,Prime,Rhea,FP1MAP,CIRS FP1 map,CIRS_102RH_FP1MAP_PRIME disk map,"AD=15.5 mrad (closest approach), LT=18. FP1 only. Fast 9-scan FP1 map (13 min.); FP1 10 mrad to space (5 min.).",,,,,, 2009-033T11:00:00,000T00:30:00,2-Feb-09,ISS,Prime,Rhea,GEOLOG,Geologic study,Rhea mapping,2x3 mosaic.,,,,,, 2009-033T11:00:00,000T00:30:00,2-Feb-09,CIRS,SPASS Rider,Rhea,GEOLOG,Geologic study,CIRS_102RH_GEOLOG004_ISS rider,rider. FP1+FP3 only. Coverage down to -50 latitude; evening terminator.,,,,,, 2009-033T11:00:00,002T02:34:00,2-Feb-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-033T11:11:59,000T02:27:00,2-Feb-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.1069819 Rs exit= 9.1234789 Range altitude= 39860.048 km ... -39597.162,,,,,, 2009-033T11:25:00,000T02:00:00,2-Feb-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-033T11:26:29,000T02:00:00,2-Feb-09,CDA,SPASS Rider,DustRAM direction,RPX0210,,CDA RPXing 2009-033T12:26:29 NTH,"large ring extention, RPXing at > 8 Rs",,,,,, 2009-033T11:30:00,000T01:10:00,2-Feb-09,UVIS,Prime,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2009-033T11:30:00,000T01:10:00,2-Feb-09,CIRS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,CIRS_102RH_ICYMAP002_UVIS rider,rider. FP1+FP3 only. Near equatorial latitude; see to -60.,,,,,, 2009-033T11:36:29,000T00:00:01,2-Feb-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 9.095 Rs, lat = 2 deg, phase = 153 deg",,,,,, 2009-033T12:40:00,000T00:20:00,2-Feb-09,ISS,Prime,Rhea,GEOLOG,Geologic study,Rhea mapping,2x3 mosaic.,,,,,, 2009-033T12:40:00,000T00:20:00,2-Feb-09,CIRS,SPASS Rider,Rhea,GEOLOG,Geologic study,CIRS_102RH_GEOLOG005_ISS rider,"rider. FP1+FP3 only. Sightly south of equator, coverage down to pole; evening terminator.",,,,,, 2009-033T13:00:00,000T01:15:00,2-Feb-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 62.8 range 1.2 Mkm",,,,,, 2009-033T13:00:00,000T01:15:00,2-Feb-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"Rider to ISS Titan cloud monitor, but for calibration purposes. FP1+FP3 only. Data only during first and last 15 min.; no-data between. Shutter 00:10-00:15, 01:00-01:05. (""Space"" first and last 10 min., during turns). This reduces the rate multiplier to 0.22.",,,,,, 2009-033T13:00:00,000T01:15:00,2-Feb-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-033T13:38:59,005T12:57:00,2-Feb-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 9.1237941 Rs exit= 19.850398 Range altitude= -40140.586 km ... 285187.93,,,,,, 2009-033T14:15:00,000T02:25:00,2-Feb-09,CIRS,Prime,Rhea,FP13SECLN,,CIRS_102RH_FP13SECLN001_PRIME,"Rhea eclipse, FP13 N; entry at 2009-033T14:54:44. 9.3-6.4 mrad, phase=82, sub-S/C=(-24, 273)-(-37, 280), LT=18. Rings TWT insert. Start T14:15, end T16:40. Design: Intermediate speed FP1 map (13 min.); mini FP1 map around FP1 target point (AD 30% larger at entry than at end) (8 min); target FP1 to ~(-20, 340), take WAC SI (7 min.); FP3 map around FP3 target point (5 min.); FP3 to ~(-10, 335) for eclipse entry at entry-10 min; NAC SI at entry-5 min.; FP1 10 mrad to space (10 min) at entry+45 min.; then FP1 to ~(-20,340); WAC SI at end-7 min.; FP1 map (5 min.); end.",,,,,, 2009-033T14:15:00,000T02:25:00,2-Feb-09,CIRS,SPASS Rider,Rhea,FP13SECLN,,CIRS_102RH FP13SECLN SI,"2 WAC, 1 NAC SI for for pointing verification of FP1, FP3 eclipse observation (can use lossy compression). WAC at 2009-033T14:45 (10 min. before eclipse entry); NAC at 2009-033T14:50 (5 min. before eclipse entry); WAC by grey light at 2009-033T16:30 (5 min. before observation ends). Eclipse entry at 2009-033T14:54:44; AD=8.3 mrad; phase=81, sub-S/C=(-28, 275).",,,,,, 2009-033T14:15:00,000T02:25:00,2-Feb-09,UVIS,SPASS Rider,Rhea,ICYECL,,ICYECL: observe satellite in eclipse,,,,,,, 2009-033T14:15:00,000T02:25:00,2-Feb-09,VIMS,SPASS Rider,Rhea,ECLIPSE,,spectral cubes,eclipse,,,,,, 2009-033T16:40:00,000T00:20:00,2-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,WAYPTTURN,Waypoint turn,CIRS_102IC_WAYPTTURN433_SP,For deep space following eclipse observation. FP1+FP3.,,,,,, 2009-033T16:45:00,004T14:05:43,2-Feb-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-033T16:45:00,003T20:34:00,2-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-033T16:45:00,003T01:15:00,2-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-033T17:00:00,000T01:00:00,2-Feb-09,VIMS,Prime,rings(general),HIRESHIPH,,Ring HIRESHIPH,Do 4 at priority 1.,,,,,, 2009-033T17:00:00,000T01:00:00,2-Feb-09,CIRS,SPASS Rider,rings(general),HIRESHIPH,,CIRS_102RI_HIRESHIPH001_VIMS,rider,,,,,, 2009-033T17:00:00,000T01:00:00,2-Feb-09,UVIS,SPASS Rider,rings(general),HIRESHIPH,,URSPEC,,,,,,, 2009-033T18:00:00,000T02:00:00,2-Feb-09,ISS,Prime,RingF,FMOVIE,F ring movie,SHORT HI RES F RING MOVIE,Short hi res F ring stare on day of periapse. Designed to fit into gaps left by other obs. Point to ring radius/longitude and stare for ~2 hrs as material passes through field of view to get ~40 degs of co-rotating longitude,,,,,, 2009-033T18:00:00,000T02:00:00,2-Feb-09,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,CIRS_102RI_FMOVIE001_ISS,rider,,,,,, 2009-033T18:00:00,000T02:00:00,2-Feb-09,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,null,,,,,, 2009-033T18:25:00,001T01:45:00,2-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-033T20:00:00,000T07:04:00,2-Feb-09,ISS,Prime,rings(general),SPKTRKLF,,Spoke Tracking observation,Need 6 out of 8,,,,,, 2009-033T20:00:00,000T07:04:00,2-Feb-09,CIRS,SPASS Rider,rings(general),SPKTRKLF,,CIRS_102RI_SPKTRKLF001_ISS,rider,,,,,, 2009-034T04:34:00,000T09:00:00,3-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-034T05:34:00,000T08:00:00,3-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09034_SP,rider,,,,,, 2009-034T14:14:00,000T08:00:00,3-Feb-09,CIRS,Prime,rings(general),VTMPS60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-034T14:14:00,000T08:00:00,3-Feb-09,CIRS,SPASS Rider,rings(general),VTMPS60MP,,CIRS_102RI_VTMPS60MP001_SI,,,,,,, 2009-034T14:14:00,000T08:00:00,3-Feb-09,UVIS,SPASS Rider,rings(general),VTMPS60MP,,URSPEC,,,,,,, 2009-034T22:14:00,000T05:40:00,3-Feb-09,VIMS,Prime,Star,TXCAMOCC,,Ring stellar occ - TX Cam,"Ring occultation; ingress only, tau=40 ms",,,,,, 2009-034T22:14:00,000T05:40:00,3-Feb-09,CIRS,SPASS Rider,rings(general),TXCAMOCC,,CIRS_102RI_TXCAMOCC001_VIMS,rider,,,,,, 2009-034T22:14:00,000T05:40:00,3-Feb-09,UVIS,SPASS Rider,rings(general),TXCAMOCC,,URSPEC,,,,,,, 2009-035T03:54:00,000T00:40:00,4-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_102RI_DEEPSPACE035_SP,rider,,,,,, 2009-035T04:34:00,000T09:00:00,4-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-035T05:34:00,000T08:00:00,4-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09035_SP,rider,,,,,, 2009-035T12:00:00,002T01:19:00,4-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-035T13:34:00,000T23:45:00,4-Feb-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-035T14:14:00,000T01:15:00,4-Feb-09,ISS,Prime,Titan,M90R1CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 72.5 range 1.1 Mkm",,,,,, 2009-035T14:14:00,000T01:15:00,4-Feb-09,CIRS,SPASS Rider,Titan,M90R1CLDF,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-035T14:14:00,000T01:15:00,4-Feb-09,UVIS,SPASS Rider,Titan,M90R1CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-035T15:29:00,000T04:00:00,4-Feb-09,CIRS,Prime,rings(general),TMAPS45MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-035T15:29:00,000T04:00:00,4-Feb-09,CIRS,SPASS Rider,rings(general),TMAPS45MP,,CIRS_102RI_TMAPS45MP001_SI,,,,,,, 2009-035T15:29:00,000T04:00:00,4-Feb-09,UVIS,SPASS Rider,rings(general),TMAPS45MP,,URSPEC,,,,,,, 2009-035T19:29:00,000T01:01:00,4-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-035T19:29:00,000T01:01:00,4-Feb-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_102RI_SATELLORB010_ISS,rider,,,,,, 2009-035T20:30:00,000T04:25:00,4-Feb-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE",Do 6 at priority 2,,,,,, 2009-035T20:30:00,000T04:25:00,4-Feb-09,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,URSTAR,,,,,,, 2009-036T00:55:00,000T02:44:00,5-Feb-09,ISS,Prime,rings(general),RETARMRLP,,Medium res retargetables,Medium Res Retarg of small ring region satellites. Need 25 of 54.,,,,,, 2009-036T00:55:00,000T02:44:00,5-Feb-09,CIRS,SPASS Rider,rings(general),RETARMRLP,,CIRS_102RI_RETARMRLP002_ISS,rider,,,,,, 2009-036T03:39:00,000T00:40:00,5-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_102RI_DEEPSPACE036_SP,rider,,,,,, 2009-036T04:19:00,000T09:00:00,5-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-036T05:19:00,000T08:00:00,5-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09036_SP,rider,,,,,, 2009-036T13:19:00,001T00:00:00,5-Feb-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-036T13:59:00,000T00:30:00,5-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-036T13:59:00,000T00:30:00,5-Feb-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_102RI_SATELLORB012_ISS,rider,,,,,, 2009-036T14:29:00,000T02:00:00,5-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2009-036T16:29:00,000T09:20:00,5-Feb-09,ISS,Prime,rings(general),SPKFMLFLP,,Lit Face Low Phase Spoke Formation Movie,Spoke Movie to observe formation,,,,,, 2009-036T16:29:00,000T09:20:00,5-Feb-09,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,,spoke movie rider,,,,,, 2009-036T16:29:00,000T09:20:00,5-Feb-09,UVIS,SPASS Rider,rings(general),SPKFMLFLP,,URSPEC,,,,,,, 2009-036T18:00:00,000T14:50:00,5-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-037T01:49:00,000T01:15:00,6-Feb-09,ISS,Prime,Titan,M90R1CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 70.4 range 0.8 Mkm",,,,,, 2009-037T01:49:00,000T01:15:00,6-Feb-09,CIRS,SPASS Rider,Titan,M90R1CLDF,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-037T01:49:00,000T01:15:00,6-Feb-09,UVIS,SPASS Rider,Titan,M90R1CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-037T03:04:00,000T01:14:00,6-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_102RI_DEEPSPACE037_NAV,rider,,,,,, 2009-037T04:19:00,000T09:00:00,6-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-037T05:19:00,000T08:00:00,6-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_102IC_DSCAL09037_SP,rider,,,,,, 2009-037T08:50:00,000T23:00:00,6-Feb-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-037T13:19:00,000T18:31:51,6-Feb-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-037T13:19:00,000T15:31:51,6-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-037T13:19:00,001T13:17:00,6-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-037T14:14:31,000T05:36:20,6-Feb-09,VIMS,Prime,Titan,CLOUD,,Cloud and global mapping,"Stare at Titan for cloud and global mapping. Cubes of 32 x 32, 48 x 48 and 64 x 64 at various exposure times.",,,,,, 2009-037T14:14:31,000T05:36:20,6-Feb-09,CIRS,SPASS Rider,Titan,CLOUD,,,Ride along with VIMS.,,,,,, 2009-037T14:14:31,000T05:36:20,6-Feb-09,ISS,SPASS Rider,Titan,CLOUD,,RCI (Ridealong context imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-037T14:14:31,000T05:36:20,6-Feb-09,UVIS,SPASS Rider,Titan,DUMMYRIDE,,Rider to VIMS,Rider to VIMS,,,,,, 2009-037T19:50:51,000T03:30:00,6-Feb-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-037T19:50:51,000T03:30:00,6-Feb-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-037T19:50:51,000T03:30:00,6-Feb-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong context imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-037T19:50:51,000T03:30:00,6-Feb-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-037T19:50:51,000T03:30:00,6-Feb-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir Comp.,VIMS ridealong with CIRS for cloud mapping.,,,,,, 2009-037T23:05:51,000T04:15:00,6-Feb-09,RADAR,SPASS Rider,Titan,T50WARMUP,,Warmup for T50,,,,,,, 2009-037T23:20:51,000T04:00:00,6-Feb-09,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-037T23:20:51,000T04:00:00,6-Feb-09,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-037T23:20:51,000T04:00:00,6-Feb-09,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong context imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-037T23:20:51,000T04:00:00,6-Feb-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Mid-IR Limb Map,VIMS ridealong with CIRS for cloud and global mapping.,,,,,, 2009-038T03:20:51,000T03:30:00,7-Feb-09,RADAR,Prime,Titan,T50INRAD,,T50 Inbound Radiometry,,,,,,, 2009-038T04:50:51,000T08:00:00,7-Feb-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,MAPS_Titan_Flyby,"T050 is an upstream flank-in flyby with a minimum altitude of 1000 km. The geometry of this flyby is suitable to study the magnetic pileup region across the nightside hemisphere. T050 also takes place in Saturn's near-noon sector (10.5 hours SLT), where Titan could be found in the magnetosheath if the solar wind pressure is high. We assign grade one priority.",,,,,, 2009-038T06:50:51,000T00:48:00,7-Feb-09,RADAR,Prime,Titan,T50INSCAT,,T50 Inbound Scatterometry,,,,,,, 2009-038T06:50:51,000T01:15:00,7-Feb-09,CAPS,SPASS Rider,Titan,T50INBND,,Inbound 102TI (T50),Inbound leg of a Titan encoun,,,,,, 2009-038T06:50:51,000T01:30:00,7-Feb-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-038T07:39:51,000T00:41:00,7-Feb-09,RADAR,Prime,Titan,T50IHISAR,,T50 Inbound HiSAR,,,,,,, 2009-038T07:50:00,000T02:00:00,7-Feb-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-038T07:50:51,000T00:48:00,7-Feb-09,INMS,Non-SPASS,Titan,TITAN50,,Titan observation,Titan observation,,,,,, 2009-038T08:05:51,000T01:30:00,7-Feb-09,CAPS,SPASS Rider,Titan,T50CLOSE,,Closest approach 120TI (T50),Closest approach of a Titan encoun,,,,,, 2009-038T08:20:51,000T00:18:00,7-Feb-09,RADAR,Prime,Titan,T50INALT,,T50 Inbound Altimetry,,,,,,, 2009-038T08:20:51,000T01:00:00,7-Feb-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-038T08:38:51,000T00:24:00,7-Feb-09,RADAR,Prime,Titan,T50RASAR,,T50 Ride-along SAR with INMS at C/A,,,,,,, 2009-038T08:38:51,000T00:24:00,7-Feb-09,INMS,Non-SPASS,Titan,TITAN50,,Prime Titan Observation,Prime Titan observation,,,,,, 2009-038T09:02:51,000T00:18:00,7-Feb-09,RADAR,Prime,Titan,T50OUTALT,,T50 Outbound Altimetry,,,,,,, 2009-038T09:02:51,000T00:48:00,7-Feb-09,INMS,Non-SPASS,Titan,TITAN50,,Titan observation,Titan observation,,,,,, 2009-038T09:20:51,000T00:20:00,7-Feb-09,RADAR,Prime,Titan,T50OHISAR,,T50 outbound HiSAR,,,,,,, 2009-038T09:20:51,000T01:30:00,7-Feb-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-038T09:35:51,000T01:15:00,7-Feb-09,CAPS,SPASS Rider,Titan,T50OUTBND,,Outbound 120TI (T50),Outbound leg of a Titan encoun,,,,,, 2009-038T09:50:00,000T01:00:00,7-Feb-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-038T09:50:51,000T16:46:09,7-Feb-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-038T10:02:32,000T00:48:19,7-Feb-09,RADAR,Prime,Titan,T50OUTSCT,,T50 Outbound Scatterometry,,,,,,, 2009-038T10:50:00,000T15:47:00,7-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-038T10:50:43,000T15:46:17,7-Feb-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magn,,,,,, 2009-038T10:50:51,000T04:00:00,7-Feb-09,RADAR,Prime,Titan,T50OUTRAD,,T50 Outbound Radiometry,,,,,,, 2009-038T12:50:51,000T16:16:09,7-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-038T14:50:51,000T03:00:00,7-Feb-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-038T14:50:51,000T03:00:00,7-Feb-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS EUV-FUV scan,,,,,, 2009-038T14:50:51,000T03:00:00,7-Feb-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong context imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-038T14:50:51,000T03:00:00,7-Feb-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Limb Map of Titan,"VIMS ridealong with UVIS,",,,,,, 2009-038T17:50:51,000T01:00:00,7-Feb-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,PHW (WAC Photometry),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-038T17:50:51,000T01:00:00,7-Feb-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS,,,,,, 2009-038T17:50:51,000T01:00:00,7-Feb-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Global Map of Titan,VIMS ridealong with ISS. Obtain 10 cubes during one hour with 6 min. dwell times.,,,,,, 2009-038T18:50:51,000T03:00:00,7-Feb-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-038T18:50:51,000T03:00:00,7-Feb-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-038T18:50:51,000T03:00:00,7-Feb-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong context imaging),regional map,,,,,, 2009-038T18:50:51,000T03:00:00,7-Feb-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir Comp.,VIMS ridealong with CIRS for cloud and global mapping.,,,,,, 2009-038T21:50:51,000T00:30:00,7-Feb-09,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Night NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-038T21:50:51,000T00:13:00,7-Feb-09,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with ISS,,,,,, 2009-038T21:50:51,000T00:30:00,7-Feb-09,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare on nightside of Titan with NAC,"VIMS ridealong with ISS. If 6 min. dwell times, 5 cubes can be obtained during the 30 min.",,,,,, 2009-038T22:20:51,000T04:30:00,7-Feb-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-038T22:20:51,000T04:30:00,7-Feb-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (6 integrations total = 12 frames, 0.5 Mb/frame)",,,,,, 2009-038T22:20:51,000T04:30:00,7-Feb-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong context imaging),regional map,,,,,, 2009-038T22:20:51,000T04:30:00,7-Feb-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp Map/Cloud Mapping,VIMS ridealong with CIRS for cloud mapping.,,,,,, 2009-039T00:00:00,000T00:34:08,8-Feb-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration and gain,,,,,, 2009-039T02:29:27,000T00:00:01,8-Feb-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 11.9 d, inc = 65.3 deg, r = 19.828 Rs, phase = 26 deg",,,,,, 2009-039T02:36:00,001T22:21:00,8-Feb-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-039T02:36:00,005T13:22:00,8-Feb-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 19.848299 Rs exit= 13.694371 Range altitude= 285057.17 km ... 40352.240,,,,,, 2009-039T02:36:00,000T13:43:00,8-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-039T02:36:00,004T09:29:00,8-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-039T02:37:00,000T01:59:00,8-Feb-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-039T02:37:00,000T20:16:34,8-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-039T02:50:51,000T00:30:00,8-Feb-09,ISS,Prime,Titan,LRMONITOR,Long range monitor,LRM (Long Range Monitor),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-039T04:19:00,000T09:00:00,8-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-039T04:36:00,000T11:43:00,8-Feb-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-039T05:07:00,000T11:12:00,8-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-039T05:19:00,000T08:00:00,8-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09039_SP,rider,,,,,, 2009-039T13:19:00,000T03:00:00,8-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-039T14:19:00,000T02:00:00,8-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09439_SP,rider,,,,,, 2009-039T16:19:00,001T20:45:00,8-Feb-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-039T16:19:00,001T08:38:00,8-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-039T16:44:00,000T10:40:00,8-Feb-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_103SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-039T16:44:00,000T10:40:00,8-Feb-09,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2009-039T22:53:34,001T02:03:26,8-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-040T04:04:00,000T09:00:00,9-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-040T05:04:00,000T08:00:00,9-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09040_SP,rider,,,,,, 2009-040T13:44:00,000T00:30:00,9-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-040T14:14:00,000T02:00:00,9-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-040T16:14:00,000T11:10:00,9-Feb-09,ISS,Prime,RingF,FRSTRCHAN,F ring streamer movie,F RING STREAMER/CHANNEL,"Movie of streamer-channel feature raised in F ring by Prometheus apoapse passage. Need as close to 1 Prom orbital period as possible. Sometimes can be day before or day after. Want 12. 6 of 49 as priority 1, 6 of 49 as priority 2.",,,,,, 2009-040T16:14:00,000T11:10:00,9-Feb-09,CIRS,SPASS Rider,RingF,FRSTRCHAN,F ring streamer movie,CIRS_103RF_FRSTRCHAN001_ISS,rider,,,,,, 2009-041T00:57:00,000T23:30:00,10-Feb-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-041T00:57:00,000T23:30:00,10-Feb-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-041T00:57:00,000T23:30:00,10-Feb-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-041T00:57:00,000T23:30:00,10-Feb-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-041T04:04:00,000T09:00:00,10-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-041T05:04:00,000T08:00:00,10-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09041_SP,rider,,,,,, 2009-041T13:04:00,000T00:56:00,10-Feb-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-041T13:04:00,001T00:00:00,10-Feb-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-041T14:22:00,000T10:42:00,10-Feb-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. This can be an ansa stare, an azimuthal scan or other design. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-041T14:22:00,000T10:42:00,10-Feb-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_103RF_FMOVIE003_ISS,rider,,,,,, 2009-041T14:22:00,000T10:42:00,10-Feb-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,Do about 5 of 50.,,,,,, 2009-041T22:04:00,000T03:00:00,10-Feb-09,RADAR,SPASS Rider,Other,WU4NMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-041T22:05:20,000T00:00:01,10-Feb-09,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2009-042T00:27:00,006T12:08:00,11-Feb-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-042T00:27:00,003T08:58:00,11-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-042T00:27:00,001T22:33:26,11-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-042T00:57:00,000T23:03:00,11-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-042T01:04:00,000T01:30:00,11-Feb-09,RADAR,Prime,Titan,NMIDLCAL,,"Distant Titan Radiometry, North Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-042T04:04:00,000T09:00:00,11-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-042T05:04:00,000T08:00:00,11-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09042_SP,rider,,,,,, 2009-042T13:04:00,005T23:31:00,11-Feb-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM request to trigger nominal science mode,"Ridealong, survey of outer mag at high latitudes",,,,,, 2009-042T13:44:00,000T00:30:00,11-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-042T14:14:00,000T02:00:00,11-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-042T16:14:00,000T10:41:00,11-Feb-09,CIRS,Prime,rings(general),VTMPN60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-042T16:14:00,000T10:41:00,11-Feb-09,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_103RI_VTMPN60MP002_SI,,,,,,, 2009-043T00:00:00,000T04:05:00,12-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-043T02:55:00,000T00:30:00,12-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-043T04:05:00,000T09:00:00,12-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-043T04:05:00,000T09:00:00,12-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-043T05:05:00,000T08:00:00,12-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09043_SP,rider,,,,,, 2009-043T12:05:00,003T03:45:00,12-Feb-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-043T13:05:00,001T16:55:00,12-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-043T13:45:00,000T01:55:00,12-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-043T15:40:00,000T11:30:00,12-Feb-09,CIRS,Prime,rings(general),TDIFN45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-043T15:40:00,000T11:30:00,12-Feb-09,CIRS,SPASS Rider,rings(general),TDIFN45HP,,CIRS_103RI_TDIFN45HP001_SI,,,,,,, 2009-043T23:00:26,001T12:21:46,12-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-044T03:50:00,000T09:00:00,13-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-044T04:00:00,000T08:30:00,13-Feb-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-044T04:50:00,000T08:00:00,13-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09044_SP,rider,,,,,, 2009-044T13:13:00,000T08:17:00,13-Feb-09,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2009-044T15:58:00,000T03:18:00,13-Feb-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.693646 Rs exit= 13.634242 Range altitude= 39549.260 km ... -39206.827,,,,,, 2009-044T16:39:00,000T02:00:00,13-Feb-09,CDA,SPASS Rider,DustRAM direction,RPX0000,,CDA RPXing 2009-044T17:39:00 NtH,"RPXing at 13.661041 Rs, large ring extention, small/medium inclintn",,,,,, 2009-044T19:16:00,003T17:19:00,13-Feb-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S48,Range enter= 13.633756 Rs exit= 13.705159 Range altitude= -40009.815 km ... 40766.695,,,,,, 2009-044T21:30:00,000T11:55:00,13-Feb-09,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2009-044T21:30:00,000T11:55:00,13-Feb-09,CIRS,SPASS Rider,rings(general),SHRTMOV,,CIRS_103RI_SHRTMOV001_ISS,rider,,,,,, 2009-044T21:30:00,000T11:55:00,13-Feb-09,VIMS,SPASS Rider,rings(general),SHRTMOV,,Short movie,"B ring, lit face",,,,,, 2009-045T01:43:14,000T00:00:01,14-Feb-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 13.573 Rs, lat = -14 deg, phase = 154 deg",,,,,, 2009-045T06:00:00,001T18:00:00,14-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-045T09:25:00,000T10:15:00,14-Feb-09,CIRS,Prime,rings(general),TDIFS45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-045T09:25:00,000T10:15:00,14-Feb-09,CIRS,SPASS Rider,rings(general),TDIFS45HP,,CIRS_103RI_TDIFS45HP001_SI,,,,,,, 2009-045T09:25:00,000T05:00:00,14-Feb-09,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2009-045T11:22:12,003T01:12:48,14-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-045T14:25:00,002T22:10:00,14-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-045T20:20:00,000T09:00:00,14-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-045T21:20:00,000T08:00:00,14-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09045_SP,rider,,,,,, 2009-046T06:00:00,000T09:15:00,15-Feb-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-046T06:00:00,000T09:15:00,15-Feb-09,CIRS,SPASS Rider,Titan,CLOUD,,,Cloud monitor,,,,,, 2009-046T06:00:00,000T09:15:00,15-Feb-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,VIMS ridealong with ISS for cloud monitoring,,,,,, 2009-046T15:15:00,000T00:30:00,15-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-046T15:45:00,000T02:00:00,15-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-046T15:50:00,001T20:45:00,15-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-046T17:45:00,000T08:35:00,15-Feb-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_103SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2009-047T00:00:00,001T12:35:00,16-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGIN,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-047T03:35:00,000T09:00:00,16-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-047T04:35:00,000T08:00:00,16-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09047_SP,rider,,,,,, 2009-047T13:15:00,000T04:10:00,16-Feb-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE",Do 6 at priority 2,,,,,, 2009-047T13:15:00,000T04:10:00,16-Feb-09,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_103RI_LATPHASE106_VIMS,rider,,,,,, 2009-047T17:25:00,000T09:30:00,16-Feb-09,CIRS,Prime,rings(general),TMAPS45MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-047T17:25:00,000T09:30:00,16-Feb-09,CIRS,SPASS Rider,rings(general),TMAPS45MP,,CIRS_103RI_TMAPS45MP001_SI,,,,,,, 2009-047T17:25:00,000T09:30:00,16-Feb-09,VIMS,SPASS Rider,rings(general),TMAPS45MP,,,null,,,,,, 2009-048T03:35:00,000T09:00:00,17-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-048T03:45:00,000T08:30:00,17-Feb-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-048T04:35:00,000T08:00:00,17-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09048_SP,rider,,,,,, 2009-048T12:35:00,004T11:12:00,17-Feb-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-048T12:35:00,002T12:47:00,17-Feb-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S S48,Range enter= 13.633756 Rs exit= 13.705159 Range altitude= -40009.815 km ... 40766.695,,,,,, 2009-048T12:35:00,000T00:43:00,17-Feb-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-048T12:35:00,000T00:46:00,17-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-048T12:35:00,000T08:04:33,17-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-048T12:35:00,000T23:25:00,17-Feb-09,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-048T12:35:00,002T12:47:00,17-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-048T12:40:00,000T00:02:00,17-Feb-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S48 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-048T13:18:00,000T00:05:00,17-Feb-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-048T13:21:00,000T04:54:00,17-Feb-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-048T13:23:00,000T00:33:00,17-Feb-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-048T13:56:00,000T00:22:59,17-Feb-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-048T14:18:59,002T11:03:01,17-Feb-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-048T18:15:00,000T08:40:00,17-Feb-09,CIRS,Prime,rings(general),TMAPS30LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-048T18:15:00,000T08:40:00,17-Feb-09,CIRS,SPASS Rider,rings(general),TMAPS30LP,,CIRS_103RI_TMAPS30LP001_SI,,,,,,, 2009-048T18:15:00,000T08:40:00,17-Feb-09,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2009-048T18:15:00,000T08:40:00,17-Feb-09,VIMS,SPASS Rider,rings(general),TMAPS30LP,,,null,,,,,, 2009-048T18:15:00,004T05:32:00,17-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-048T20:39:33,002T04:42:27,17-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-049T00:00:00,001T00:00:00,18-Feb-09,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2009-049T03:35:00,000T09:00:00,18-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-049T04:35:00,000T08:00:00,18-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09049_SP,rider,,,,,, 2009-049T13:15:00,000T01:15:00,18-Feb-09,ISS,Prime,Titan,M30R2CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 9.8 range 1.9 Mkm",,,,,, 2009-049T13:15:00,000T01:15:00,18-Feb-09,CIRS,SPASS Rider,Titan,M30R2CLDF,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-049T13:15:00,000T01:15:00,18-Feb-09,UVIS,SPASS Rider,Titan,M30R2CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-049T14:30:00,000T11:35:00,18-Feb-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_103SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2009-049T14:30:00,000T11:35:00,18-Feb-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,COMPSIT ridealong with CIRS,COMPSIT Ridealong with CIRS,,,,,, 2009-049T15:00:00,000T09:10:00,18-Feb-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-050T02:05:00,000T01:29:00,19-Feb-09,CIRS,SPASS Rider,Skeletonrequest,OPNAV,Optical navigation image,CIRS_103SK_OPNAV501_NAV,rider,,,,,, 2009-050T03:35:00,000T09:00:00,19-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-050T04:35:00,000T08:00:00,19-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_103IC_DSCAL09050_SP,rider,,,,,, 2009-050T13:15:00,000T13:25:00,19-Feb-09,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2009-050T13:15:00,000T13:25:00,19-Feb-09,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_103RI_EGPHASE117_VIMS,rider,,,,,, 2009-050T13:15:00,000T13:25:00,19-Feb-09,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2009-051T01:01:50,000T00:00:01,20-Feb-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 11.9 d, inc = 65.3 deg, r = 19.825 Rs, phase = 26 deg",,,,,, 2009-051T01:22:00,005T13:10:00,20-Feb-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 13.633756 Rs exit= 13.705159 Range altitude= -40009.815 km ... 40766.695,,,,,, 2009-051T01:22:00,000T02:00:00,20-Feb-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-051T01:22:00,000T20:04:35,20-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-051T01:22:00,004T09:36:00,20-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-051T03:20:00,000T09:00:00,20-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-051T03:22:00,002T01:28:00,20-Feb-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-051T04:20:00,000T08:00:00,20-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09051_SP,rider,,,,,, 2009-051T13:00:00,000T03:30:00,20-Feb-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-051T13:00:00,000T03:30:00,20-Feb-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2009-051T15:00:00,000T03:00:00,20-Feb-09,RADAR,SPASS Rider,Other,WU4NEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-051T16:30:00,000T01:30:00,20-Feb-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Skathi observation,Observation of outer moon Skathi,,,,,, 2009-051T18:00:00,000T01:10:00,20-Feb-09,RADAR,Prime,Titan,NEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-051T19:50:00,000T09:00:00,20-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-051T20:50:00,000T08:00:00,20-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09451_SP,rider,,,,,, 2009-051T21:26:35,001T02:20:25,20-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-052T05:30:00,000T11:20:00,21-Feb-09,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side",Do 15 unlit side at priority 2 (~every third orbit),,,,,, 2009-052T05:30:00,000T11:20:00,21-Feb-09,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_104RI_APOMOSU126_VIMS,rider,,,,,, 2009-052T16:50:00,000T01:50:00,21-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-052T18:40:00,000T00:30:00,21-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-052T19:50:00,000T09:00:00,21-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-052T20:50:00,000T08:00:00,21-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09052_SP,rider,,,,,, 2009-052T23:47:00,000T23:35:00,21-Feb-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-052T23:47:00,001T01:25:40,21-Feb-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-052T23:47:00,000T05:03:00,21-Feb-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-052T23:47:00,000T23:35:00,21-Feb-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-053T04:50:00,000T01:14:00,22-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE053_NAV,rider,,,,,, 2009-053T04:50:00,005T07:10:00,22-Feb-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-053T04:50:00,000T18:32:00,22-Feb-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-053T06:05:00,000T00:35:00,22-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-053T06:05:00,000T00:35:00,22-Feb-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_104RI_SATELLORB008_ISS,rider,,,,,, 2009-053T06:40:00,000T07:35:00,22-Feb-09,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"Inner A ring; do 4 at priority 2, tau=20 ms",,,,,, 2009-053T06:40:00,000T07:35:00,22-Feb-09,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_104RI_GAMCRUOCC102_VIMS,rider,,,,,, 2009-053T06:40:00,000T07:35:00,22-Feb-09,UVIS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,URSTAR,,,,,,, 2009-053T14:15:00,000T13:10:00,22-Feb-09,UVIS,Prime,Star,URBETCEN,Stellar occultation,URSTAR,,,,,,, 2009-053T14:15:00,000T13:10:00,22-Feb-09,CIRS,SPASS Rider,rings(general),URBETCEN,Stellar occultation,CIRS_104RI_URBETCEN001_UVIS,rider,,,,,, 2009-053T14:15:00,000T13:10:00,22-Feb-09,UVIS,SPASS Rider,Star,URBETCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2009-053T15:58:00.0 2009-053T16:14:48.0 2009-053T17:07:50.0 2009-054T03:24:23.0 2009-054T02:31:21.0,,,,,, 2009-053T23:22:00,010T23:30:00,22-Feb-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-053T23:22:00,006T00:38:00,22-Feb-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-054T01:12:40,001T20:21:32,23-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-054T03:25:00,000T00:35:00,23-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE054_SP,rider,,,,,, 2009-054T04:00:00,000T08:25:00,23-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-054T05:00:00,000T07:25:00,23-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09054_SP,rider,,,,,, 2009-054T13:00:00,000T02:00:00,23-Feb-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-054T13:00:00,000T02:00:00,23-Feb-09,CIRS,SPASS Rider,rings(general),SURVEYTG,,CIRS_104RI_SURVEYTG003_CAPS,rider,,,,,, 2009-054T15:00:00,000T11:00:00,23-Feb-09,CIRS,Prime,rings(general),VTMPN60MP,,CIRS_104RI_VTMPN60MP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-054T15:00:00,000T11:00:00,23-Feb-09,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_104RI_VTMPN60MP001_SI,,,,,,, 2009-054T15:00:00,000T11:00:00,23-Feb-09,UVIS,SPASS Rider,rings(general),VTMPN60MP,,URSTAR,,,,,,, 2009-054T15:00:00,000T11:00:00,23-Feb-09,VIMS,SPASS Rider,rings(general),VTMPN60MP,,,null,,,,,, 2009-055T02:00:00,000T00:30:00,24-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-055T02:00:00,000T00:30:00,24-Feb-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_104RI_SATELLORB012_ISS,rider,,,,,, 2009-055T03:05:00,000T09:00:00,24-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-055T04:05:00,000T08:00:00,24-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09055_SP,rider,,,,,, 2009-055T10:58:00,003T03:30:00,24-Feb-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-055T12:45:00,000T01:15:00,24-Feb-09,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 156 range 1.8 Mkm",,,,,, 2009-055T12:45:00,000T01:15:00,24-Feb-09,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-055T12:45:00,000T01:15:00,24-Feb-09,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-055T14:00:00,000T06:00:00,24-Feb-09,CIRS,Prime,rings(general),TDIFN45HP,,CIRS_104RI_TDIFN45HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-055T14:00:00,000T06:00:00,24-Feb-09,CIRS,SPASS Rider,rings(general),TDIFN45HP,,CIRS_104RI_TDIFN45HP001_SI,,,,,,, 2009-055T14:00:00,000T06:00:00,24-Feb-09,ISS,SPASS Rider,rings(general),TDIFN45HP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-055T14:00:00,000T06:00:00,24-Feb-09,UVIS,SPASS Rider,rings(general),TDIFN45HP,,URSTAR,,,,,,, 2009-055T20:00:00,000T04:00:00,24-Feb-09,ISS,Prime,rings(general),PHOTDARK,,"high-phase, dark-face ring photometry","high phase unlit #1: B = 31, phase = 130, B' = -2.6",,,,,, 2009-055T20:00:00,000T04:00:00,24-Feb-09,CIRS,SPASS Rider,rings(general),PHOTDARK,,CIRS_104RI_PHOTDARK001_ISS,rider,,,,,, 2009-055T21:34:12,001T12:24:43,24-Feb-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-056T00:00:00,000T02:45:00,25-Feb-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. This can be an ansa stare, an azimuthal scan or other design. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-056T00:00:00,000T02:45:00,25-Feb-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_104RF_FMOVIE003_ISS,rider,,,,,, 2009-056T02:45:00,000T00:35:00,25-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE056_SP,rider,,,,,, 2009-056T03:20:00,000T09:00:00,25-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-056T04:20:00,000T08:00:00,25-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09455_SP,rider,,,,,, 2009-056T12:50:00,000T02:10:00,25-Feb-09,ISS,Prime,Dione,160W160PH,,Dione phase coverage,"Turn UVIS_FUV to Dione; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2009-056T12:50:00,000T02:10:00,25-Feb-09,CIRS,SPASS Rider,Dione,160W160PH,,Rider in Longitude-phase observation of Dione.,"Duration=02:10. AD~2.2, phase~165, ~(7,140). 15.5, Centers; shutter first, last 3 minutes.",,,,,, 2009-056T12:50:00,000T02:10:00,25-Feb-09,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-056T12:50:00,000T02:10:00,25-Feb-09,VIMS,SPASS Rider,Dione,160W160PH,,,high phase angles and trailing hemisphere coverage,,,,,, 2009-056T14:32:00,000T03:20:00,25-Feb-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.704438 Rs exit= 13.644882 Range altitude= 39964.213 km ... -39547.454,,,,,, 2009-056T15:00:00,000T02:00:00,25-Feb-09,CDA,Prime,DustRAM direction,RPX0010,,CDA RPXing 2009-056T16:13:00 NtH,"RPXing at 13.672008 Rs, large ring extention, small/medium inclintn",,,,,, 2009-056T15:00:00,000T02:00:00,25-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE156_CDA,rider,,,,,, 2009-056T17:00:00,000T08:00:00,25-Feb-09,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2009-056T17:00:00,000T08:00:00,25-Feb-09,CIRS,SPASS Rider,rings(general),SHRTMOV,,CIRS_104RI_SHRTMOV002_ISS,rider,,,,,, 2009-056T17:52:00,006T06:28:00,25-Feb-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 13.644401 Rs exit= 13.706460 Range altitude= -40349.948 km ... 40571.052,,,,,, 2009-057T00:16:12,000T00:00:01,26-Feb-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 13.584 Rs, lat = -14 deg, phase = 154 deg",,,,,, 2009-057T01:00:00,000T06:00:00,26-Feb-09,CIRS,Prime,rings(general),TDIFS20HP,,CIRS_104RI_TDIFS20HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-057T01:00:00,000T06:00:00,26-Feb-09,CIRS,SPASS Rider,rings(general),TDIFS20HP,,CIRS_104RI_TDIFS20HP001_SI,,,,,,, 2009-057T01:00:00,000T06:00:00,26-Feb-09,ISS,SPASS Rider,rings(general),TDIFS20HP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-057T01:00:00,000T06:00:00,26-Feb-09,UVIS,SPASS Rider,rings(general),TDIFS20HP,,URSTAR,,,,,,, 2009-057T07:00:00,000T00:50:00,26-Feb-09,VIMS,Prime,rings(general),HIRESHIPH,,Ring HIRESHIPH,Do 4 at priority 1.,,,,,, 2009-057T07:00:00,000T00:50:00,26-Feb-09,CIRS,SPASS Rider,rings(general),HIRESHIPH,,CIRS_104RI_HIRESHIPH001_VIMS,rider,,,,,, 2009-057T07:00:00,000T00:50:00,26-Feb-09,UVIS,SPASS Rider,rings(general),HIRESHIPH,,URSTAR,,,,,,, 2009-057T07:50:00,000T03:15:00,26-Feb-09,VIMS,Prime,rings(general),BETPEGOCC,,Ring stellar occ - betPeg,"betPeg occultation, 2 of 4, F-D rings, R0=2.348, Rf=1.129, Rmin=1.129, tau=40 ms",,,,,, 2009-057T07:50:00,000T03:15:00,26-Feb-09,CIRS,SPASS Rider,rings(general),BETPEGOCC,,CIRS_104RI_BETPEGOCC102_VIMS,rider,,,,,, 2009-057T07:50:00,000T03:15:00,26-Feb-09,UVIS,SPASS Rider,rings(general),BETPEGOCC,,URSTAR,,,,,,, 2009-057T09:58:55,003T09:24:52,26-Feb-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-057T11:05:00,000T07:55:00,26-Feb-09,CIRS,Prime,rings(general),VCASLSHP,,CIRS_104RI_VCASLSHP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-057T11:05:00,000T07:55:00,26-Feb-09,CIRS,SPASS Rider,rings(general),VCASLSHP,,CIRS_104RI_VCASLSHP001_SI,,,,,,, 2009-057T11:05:00,000T07:55:00,26-Feb-09,UVIS,SPASS Rider,rings(general),VCASLSHP,,URSTAR,,,,,,, 2009-057T19:00:00,000T00:35:00,26-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE057_SP,rider,,,,,, 2009-057T19:35:00,000T09:00:00,26-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-057T20:35:00,000T08:00:00,26-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09057_SP,rider,,,,,, 2009-058T04:35:00,000T00:35:00,27-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE058_SP,rider,,,,,, 2009-058T05:10:00,000T04:30:00,27-Feb-09,CIRS,Prime,rings(general),VTMPS60MP,,CIRS_104RI_VTMPS60MP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-058T05:10:00,000T04:30:00,27-Feb-09,CIRS,SPASS Rider,rings(general),VTMPS60MP,,CIRS_104RI_VTMPS60MP001_SI,,,,,,, 2009-058T05:10:00,000T04:30:00,27-Feb-09,ISS,SPASS Rider,rings(general),VTMPS60MP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-058T05:10:00,000T04:30:00,27-Feb-09,UVIS,SPASS Rider,rings(general),VTMPS60MP,,URSTAR,,,,,,, 2009-058T05:10:00,000T04:30:00,27-Feb-09,VIMS,SPASS Rider,rings(general),VTMPS60MP,,,null,,,,,, 2009-058T09:40:00,000T08:50:00,27-Feb-09,UVIS,Prime,Star,UREPSCAS,,URSTAR,,,,,,, 2009-058T09:40:00,000T08:50:00,27-Feb-09,CIRS,SPASS Rider,Star,UREPSCAS,,CIRS_104ST_UREPSCAS001_UVIS,rider,,,,,, 2009-058T09:40:00,000T08:50:00,27-Feb-09,UVIS,SPASS Rider,Star,UREPSCAS,,Support Imaging,NAC support images at the following times: 2009-058T10:47:00.0 2009-058T11:09:32.0 2009-058T12:39:25.0 2009-058T17:31:00.0 2009-058T17:09:00.0 2009-058T15:40:00.0,,,,,, 2009-058T09:40:00,000T08:50:00,27-Feb-09,VIMS,SPASS Rider,rings(general),UREPSCAS,,,slow radial ring scan,,,,,, 2009-058T12:00:00,004T12:20:00,27-Feb-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-058T14:28:00,004T09:52:00,27-Feb-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-058T18:30:00,000T06:50:00,27-Feb-09,CIRS,Prime,rings(general),VTMPS60MP,,CIRS_104RI_VTMPS60MP002_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-058T18:30:00,000T06:50:00,27-Feb-09,CIRS,SPASS Rider,rings(general),VTMPS60MP,,CIRS_104RI_VTMPS60MP002_SI,,,,,,, 2009-058T18:30:00,000T06:50:00,27-Feb-09,UVIS,SPASS Rider,rings(general),VTMPS60MP,,URSTAR,,,,,,, 2009-058T18:30:00,000T06:50:00,27-Feb-09,VIMS,SPASS Rider,rings(general),VTMPS60MP,,,null,,,,,, 2009-059T01:20:00,000T01:29:00,28-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE059_NAV,rider,,,,,, 2009-059T02:50:00,000T09:00:00,28-Feb-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-059T03:50:00,000T08:00:00,28-Feb-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09059_SP,rider,,,,,, 2009-059T11:50:00,000T00:40:00,28-Feb-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE059_SP,rider,,,,,, 2009-059T12:30:00,000T08:30:00,28-Feb-09,CIRS,Prime,rings(general),TMAPS45MP,,CIRS_104RI_TMAPS45MP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-059T12:30:00,000T08:30:00,28-Feb-09,CIRS,SPASS Rider,rings(general),TMAPS45MP,,CIRS_104RI_TMAPS45MP001_SI,,,,,,, 2009-059T12:30:00,000T08:30:00,28-Feb-09,UVIS,SPASS Rider,rings(general),TMAPS45MP,,URSTAR,,,,,,, 2009-059T12:30:00,000T08:30:00,28-Feb-09,VIMS,SPASS Rider,rings(general),TMAPS45MP,,,null,,,,,, 2009-059T21:00:00,000T01:10:00,28-Feb-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-059T21:00:00,000T01:10:00,28-Feb-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_104RI_SATELLORB016_ISS,rider,,,,,, 2009-059T22:10:00,000T04:00:00,28-Feb-09,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"intermediate phase, lit-face ring photometry","intermediate lit #6: B = -43, phase = 62, B' = -2.5",,,,,, 2009-059T22:10:00,000T04:00:00,28-Feb-09,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_104RI_PHOTLIT003_ISS,rider,,,,,, 2009-059T22:10:00,000T04:00:00,28-Feb-09,VIMS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,PhotLit mosaic,Main ring photometry,,,,,, 2009-060T00:00:00,004T22:52:00,1-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-060T02:10:00,000T00:40:00,1-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE060_SP,rider,,,,,, 2009-060T02:10:00,000T10:10:00,1-Mar-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-060T02:50:00,000T09:00:00,1-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-060T03:50:00,000T08:00:00,1-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09060_SP,rider,,,,,, 2009-060T11:50:00,000T00:30:00,1-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE460_SP,rider,,,,,, 2009-060T12:20:00,000T06:30:00,1-Mar-09,CIRS,Prime,rings(general),TMAPS30LP,,CIRS_104RI_TMAPS30LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-060T12:20:00,000T06:30:00,1-Mar-09,CIRS,SPASS Rider,rings(general),TMAPS30LP,,CIRS_104RI_TMAPS30LP001_SI,,,,,,, 2009-060T12:20:00,000T06:30:00,1-Mar-09,ISS,SPASS Rider,rings(general),TMAPS30LP,,,Spoke periodicity movie. riding along on CIRS TMAP obs.,,,,,, 2009-060T12:20:00,000T06:30:00,1-Mar-09,UVIS,SPASS Rider,rings(general),TMAPS30LP,,URSTAR,,,,,,, 2009-060T12:20:00,000T06:30:00,1-Mar-09,VIMS,SPASS Rider,rings(general),TMAPS30LP,,,null,,,,,, 2009-060T15:20:00,000T08:00:00,1-Mar-09,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 4 hours required to be tracked at DSS-25 in 1-way mode.,,,,,, 2009-060T19:20:00,000T09:00:00,1-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-060T19:23:47,002T04:56:13,1-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-060T20:20:00,000T08:00:00,1-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09460_SP,rider,,,,,, 2009-061T05:00:00,000T01:15:00,2-Mar-09,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 44.2 range 2.3 Mkm",,,,,, 2009-061T05:00:00,000T01:15:00,2-Mar-09,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-061T05:00:00,000T01:15:00,2-Mar-09,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-061T06:15:00,000T00:30:00,2-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 021 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-061T06:15:00,000T00:30:00,2-Mar-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_104RI_SATELLORB021_ISS,rider,,,,,, 2009-061T06:45:00,000T02:00:00,2-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-061T06:45:00,000T02:00:00,2-Mar-09,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_104RI_SURVEYPTG006_CAPS,rider,,,,,, 2009-061T08:45:00,000T09:00:00,2-Mar-09,ISS,Prime,rings(general),RADMRLPLF,,Color Radial Scan,"Color radial scan, need 1 want 2 out of 5",,,,,, 2009-061T08:45:00,000T09:00:00,2-Mar-09,CIRS,SPASS Rider,rings(general),RADMRLPLF,,CIRS_104RI_RADMRLPLF001_ISS,rider,,,,,, 2009-061T08:45:00,000T09:00:00,2-Mar-09,VIMS,SPASS Rider,rings(general),RADMRLPLF,,,null,,,,,, 2009-061T17:45:00,000T00:35:00,2-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_104RI_DEEPSPACE061_SP,rider,,,,,, 2009-061T18:20:00,000T08:25:00,2-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-061T19:20:00,000T07:25:00,2-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09061_SP,rider,,,,,, 2009-062T03:20:00,000T02:30:00,3-Mar-09,UVIS,Prime,Star,URTHEHYA,URSTAR observation,URSTAR,,,,,,, 2009-062T03:20:00,000T02:30:00,3-Mar-09,CIRS,SPASS Rider,rings(general),URTHEHYA,URSTAR observation,CIRS_104RI_URTHEHYA001_UVIS,rider,,,,,, 2009-062T03:20:00,000T02:30:00,3-Mar-09,UVIS,SPASS Rider,Star,URTHEHYA,URSTAR observation,Support Imaging,NAC support images at the following times: 2009-062T04:44:35.0 2009-062T04:46:44.8 2009-062T05:05:52.0 2009-062T05:03:42.5,,,,,, 2009-062T05:50:00,000T02:00:00,3-Mar-09,ISS,Prime,Rhea,RHEARPXLP,Rhea ring search,Image Rhea's equatorial plane at low phase,Image Rhea's equatorial plane at low phase,,,,,, 2009-062T05:50:00,000T02:00:00,3-Mar-09,UVIS,SPASS Rider,Rhea,RHEARPXLP,Rhea ring search,,,,,,,, 2009-062T05:50:00,000T02:00:00,3-Mar-09,VIMS,SPASS Rider,Rhea,RHEARPXLP,Rhea ring search,Rhea RPXLP,Do 4 at priority 1.,,,,,, 2009-062T07:50:00,000T08:00:00,3-Mar-09,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2009-062T07:50:00,000T08:00:00,3-Mar-09,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_104RI_EGPHASE118_VIMS,rider,,,,,, 2009-062T07:50:00,000T08:00:00,3-Mar-09,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2009-062T15:50:00,000T02:00:00,3-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-062T19:05:00,000T09:00:00,3-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-062T20:05:00,000T08:00:00,3-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_104IC_DSCAL09062_SP,rider,,,,,, 2009-062T23:46:32,000T00:00:01,3-Mar-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 12.0 d, inc = 65.3 deg, r = 19.840 Rs, phase = 26 deg",,,,,, 2009-063T00:20:00,005T13:08:00,4-Mar-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 13.644401 Rs exit= 13.706460 Range altitude= -40349.948 km ... 40571.052,,,,,, 2009-063T00:20:00,000T02:00:00,4-Mar-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-063T00:20:00,000T19:57:14,4-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-063T00:20:00,004T09:51:00,4-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-063T00:20:00,000T03:45:00,4-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-063T02:20:00,005T09:00:00,4-Mar-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-063T08:40:00,000T05:20:00,4-Mar-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. This can be an ansa stare, an azimuthal scan or other design. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-063T08:40:00,000T05:20:00,4-Mar-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_105RF_FMOVIE003_ISS,rider,,,,,, 2009-063T08:40:00,000T05:20:00,4-Mar-09,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,null,,,,,, 2009-063T14:00:00,000T04:30:00,4-Mar-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-063T14:00:00,000T04:30:00,4-Mar-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2009-063T19:05:00,000T09:00:00,4-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-063T20:05:00,000T08:00:00,4-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09063_SP,rider,,,,,, 2009-063T20:17:14,002T03:51:02,4-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-064T04:45:00,000T01:15:00,5-Mar-09,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 20.8 range 2.3 Mkm",,,,,, 2009-064T04:45:00,000T01:15:00,5-Mar-09,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-064T04:45:00,000T01:15:00,5-Mar-09,UVIS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-064T06:00:00,000T02:00:00,5-Mar-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Siarnaq rotation period,Observation of outer moon Siarnaq.,,,,,, 2009-064T06:00:00,000T02:00:00,5-Mar-09,CIRS,SPASS Rider,rings(general),OUTERSATS,Icy satellite observaton,CIRS_105RI_OUTERSATS001_ISS,rider,,,,,, 2009-064T08:00:00,000T08:00:00,5-Mar-09,CIRS,Prime,rings(general),TMAPN45LP,,CIRS_105RI_TMAPN45LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-064T08:00:00,000T08:00:00,5-Mar-09,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_105RI_TMAPN45LP001_SI,,,,,,, 2009-064T08:00:00,000T08:00:00,5-Mar-09,ISS,SPASS Rider,rings(general),TMAPN45LP,,,Spoke periodicity movie. riding along on CIRS TMAP obs.,,,,,, 2009-064T08:00:00,000T08:00:00,5-Mar-09,UVIS,SPASS Rider,rings(general),TMAPN45LP,,URSTAR,,,,,,, 2009-064T08:00:00,000T08:00:00,5-Mar-09,VIMS,SPASS Rider,rings(general),TMAPN45LP,,,null,,,,,, 2009-064T16:00:00,000T00:30:00,5-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-064T16:00:00,000T00:30:00,5-Mar-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_105RI_SATELLORB005_ISS,rider,,,,,, 2009-064T16:30:00,000T02:00:00,5-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-064T19:05:00,000T09:00:00,5-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-064T20:05:00,000T08:00:00,5-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09064_SP,rider,,,,,, 2009-064T22:52:00,000T23:50:00,5-Mar-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-064T22:52:00,000T01:08:00,5-Mar-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-064T22:52:00,000T23:50:00,5-Mar-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-065T00:00:00,000T22:42:00,6-Mar-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-065T04:40:00,000T02:00:00,6-Mar-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-065T04:40:00,000T02:00:00,6-Mar-09,CIRS,SPASS Rider,rings(general),HLCUSPPTG,,CIRS_105RI_HLCUSPPTG001_CAPS,rider,,,,,, 2009-065T06:40:00,000T07:05:00,6-Mar-09,CIRS,Prime,rings(general),SATREFL,,CIRS_105RI_SATREFL065_PRIME;,null,,,,,, 2009-065T06:40:00,000T07:05:00,6-Mar-09,CIRS,SPASS Rider,rings(general),SATREFL,,CIRS_105RI_SATREFL065_SI,,,,,,, 2009-065T06:40:00,000T07:05:00,6-Mar-09,UVIS,SPASS Rider,rings(general),SATREFL,,URSTAR,,,,,,, 2009-065T13:45:00,000T13:25:00,6-Mar-09,UVIS,Prime,Star,URBETCEN,Stellar occultation,URSTAR,,,,,,, 2009-065T13:45:00,000T13:25:00,6-Mar-09,CIRS,SPASS Rider,rings(general),URBETCEN,Stellar occultation,CIRS_105RI_URBETCEN001_UVIS,rider,,,,,, 2009-065T13:45:00,000T13:25:00,6-Mar-09,UVIS,SPASS Rider,Star,URBETCEN,Stellar occultation,Support Imaging,NAC support images at the following times: 2009-065T14:52:25.0 2009-065T15:08:11.0 2009-065T16:01:55.0 2009-066T02:34:00.0 2009-066T02:18:20.0 2009-066T01:25:18.5,,,,,, 2009-065T17:55:00,000T04:50:00,6-Mar-09,VIMS,SPASS Rider,rings(general),ALCENAOCC,,Ring occ - alCenA,alCenA ring occultation,,,,,, 2009-065T22:42:00,010T23:10:00,6-Mar-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-065T22:42:00,006T01:18:00,6-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-066T00:00:00,000T00:34:00,7-Mar-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-066T00:08:16,000T08:41:24,7-Mar-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-066T03:40:00,000T07:40:00,7-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-066T04:40:00,000T06:40:00,7-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09066_SP,rider,,,,,, 2009-066T08:49:40,001T11:39:55,7-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-066T12:50:00,000T01:15:00,7-Mar-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 73.5 range 1.9 Mkm",,,,,, 2009-066T12:50:00,000T01:15:00,7-Mar-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-066T12:50:00,000T01:15:00,7-Mar-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-066T14:05:00,000T01:25:00,7-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-066T14:05:00,000T01:25:00,7-Mar-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_105RI_SATELLORB011_ISS,rider,,,,,, 2009-066T15:30:00,000T10:10:00,7-Mar-09,UVIS,Prime,Star,URALPARA,Alpha Ara occultation,URSTAR,,,,,,, 2009-066T15:30:00,000T10:05:00,7-Mar-09,CIRS,SPASS Rider,rings(general),URALPARA,Alpha Ara occultation,CIRS_105RI_URALPARA001_UVIS,rider,,,,,, 2009-066T15:30:00,000T10:10:00,7-Mar-09,UVIS,SPASS Rider,Star,URALPARA,Alpha Ara occultation,Support Imaging,NAC support images at the following times: 2009-066T16:55:00.0 2009-066T17:12:20.0 2009-066T18:11:00.0 2009-067T01:16:00.0 2009-067t00:59:45.0 2009-067t00:01:00.0,,,,,, 2009-067T02:20:00,000T09:00:00,8-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-067T03:20:00,000T08:00:00,8-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09067_SP,rider,,,,,, 2009-067T10:11:00,003T03:29:00,8-Mar-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-067T12:00:00,000T00:30:00,8-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-067T12:00:00,000T00:30:00,8-Mar-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_105RI_SATELLORB012_ISS,rider,,,,,, 2009-067T12:30:00,000T04:00:00,8-Mar-09,CIRS,Prime,rings(general),TDIFN45HP,,CIRS_105RI_TDIFN45HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-067T12:30:00,000T04:00:00,8-Mar-09,CIRS,SPASS Rider,rings(general),TDIFN45HP,,CIRS_105RI_TDIFN45HP001_SI,,,,,,, 2009-067T12:30:00,000T04:00:00,8-Mar-09,ISS,SPASS Rider,rings(general),TDIFN45HP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-067T12:30:00,000T04:00:00,8-Mar-09,UVIS,SPASS Rider,rings(general),TDIFN45HP,,URSTAR,,,,,,, 2009-067T12:30:00,000T04:00:00,8-Mar-09,VIMS,SPASS Rider,rings(general),TDIFN45HP,,,null,,,,,, 2009-067T16:30:00,000T09:15:00,8-Mar-09,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2009-067T16:30:00,000T09:15:00,8-Mar-09,CIRS,SPASS Rider,rings(general),SHRTMOV,,CIRS_105RI_SHRTMOV001_ISS,rider,,,,,, 2009-067T20:29:35,001T12:24:24,8-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-068T01:45:00,000T00:35:00,9-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPCE,,CIRS_105RI_DEEPSPCE068_SP,rider,,,,,, 2009-068T02:20:00,000T09:00:00,9-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-068T03:20:00,000T08:00:00,9-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09068_SP,rider,,,,,, 2009-068T11:20:00,001T06:15:00,9-Mar-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey.,,,,,, 2009-068T12:00:00,000T02:00:00,9-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-068T13:28:00,000T03:20:00,9-Mar-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.705738 Rs exit= 13.646259 Range altitude= 39768.067 km ... -39792.359,,,,,, 2009-068T14:00:00,000T03:35:00,9-Mar-09,ISS,Prime,Rhea,RHEARPXHP,,Image Rhea's equatorial plane at high phase,Image Rhea's equatorial plane at high phase,,,,,, 2009-068T14:00:00,000T03:00:00,9-Mar-09,UVIS,SPASS Rider,Rhea,RHEARPXLP,Rhea ring search,,,,,,,, 2009-068T14:09:00,000T02:00:00,9-Mar-09,CDA,SPASS Rider,DustRAM direction,RPX0020,,CDA RPXing 2009-068T15:09:00 NtH,"RPXing at 13.673320 Rs, large ring extention, small/medium inclintn",,,,,, 2009-068T16:48:00,006T06:30:00,9-Mar-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 13.645780 Rs exit= 13.693648 Range altitude= -40595.334 km ... 40599.829,,,,,, 2009-068T17:00:00,000T08:00:00,9-Mar-09,CIRS,SPASS Rider,rings(general),SHRTMOV,,CIRS_105RI_SHRTMOV002_ISS,rider,,,,,, 2009-068T17:35:00,000T07:25:00,9-Mar-09,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2009-068T23:07:42,000T00:00:01,9-Mar-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 13.586 Rs, lat = -13 deg, phase = 153 deg",,,,,, 2009-069T01:00:00,000T06:00:00,10-Mar-09,CIRS,Prime,rings(general),TDIFS20HP,,CIRS_105RI_TDIFS20HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-069T01:00:00,000T06:00:00,10-Mar-09,CIRS,SPASS Rider,rings(general),TDIFS20HP,,CIRS_105RI_TDIFS20HP001_SI,,,,,,, 2009-069T01:00:00,000T06:00:00,10-Mar-09,ISS,SPASS Rider,rings(general),TDIFS20HP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-069T01:00:00,000T06:00:00,10-Mar-09,UVIS,SPASS Rider,rings(general),TDIFS20HP,,URSTAR,,,,,,, 2009-069T07:00:00,000T00:55:00,10-Mar-09,VIMS,Prime,rings(general),HIRESHIPH,,Ring HIRESHIPH,Do 4 at priority 1.,,,,,, 2009-069T07:00:00,000T00:55:00,10-Mar-09,CIRS,SPASS Rider,rings(general),HIRESHIPH,,CIRS_105RI_HIRESHIPH001_VIMS,rider,,,,,, 2009-069T07:00:00,000T00:55:00,10-Mar-09,UVIS,SPASS Rider,rings(general),HIRESHIPH,,URSTAR,,,,,,, 2009-069T07:55:00,000T00:40:00,10-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_105RI_DEEPSPACE069_SP,rider,,,,,, 2009-069T08:35:00,000T09:00:00,10-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-069T08:53:59,003T09:37:14,10-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-069T09:35:00,000T08:00:00,10-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09069_SP,rider,,,,,, 2009-069T17:35:00,005T05:43:00,10-Mar-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post Backup OTM Survey,MAPS magnetospheric survey.,,,,,, 2009-069T18:10:00,000T06:40:00,10-Mar-09,CIRS,Prime,Rhea,FP1SECLNX,CIRS elipse observation,CIRS_105RH_FP1SECLNX001_PRIME;,"RINGS TWT. FP1 entry, exit. 2.5>AD>2.3 mrad; S polar. ENTRY CONFLICT: DOWNLINK ENDS AT 17:35.",,,,,, 2009-069T18:10:00,000T06:40:00,10-Mar-09,CIRS,SPASS Rider,Rhea,FP1SECLNX,CIRS elipse observation,CIRS_105RH_FP1SECLNX001_SI,Three WAC images for pointing verification at times TBD.,,,,,, 2009-069T18:10:00,000T06:40:00,10-Mar-09,UVIS,SPASS Rider,Rhea,ICYECL,,ICYECL: observe satellite in eclipse,,,,,,, 2009-069T18:10:00,000T06:40:00,10-Mar-09,VIMS,SPASS Rider,Rhea,ECLIPSE,,,null,,,,,, 2009-070T02:05:00,000T09:00:00,11-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T51 Rev107 Titan Bistatic experiment on 2009/086 and the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-070T02:05:00,000T09:00:00,11-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-070T03:05:00,000T08:00:00,11-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09070_SP,rider,,,,,, 2009-070T11:45:00,000T13:40:00,11-Mar-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-070T11:45:00,000T13:40:00,11-Mar-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_105RF_FMOVIE002_ISS,rider,,,,,, 2009-070T11:45:00,000T13:40:00,11-Mar-09,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Ring movie,null,,,,,, 2009-070T13:40:00,004T09:38:00,11-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-071T01:25:00,000T00:40:00,12-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_105RI_DEEPSPACE071_SP,rider,,,,,, 2009-071T02:05:00,000T09:00:00,12-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-071T03:05:00,000T08:00:00,12-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09071_SP,rider,,,,,, 2009-071T11:45:00,000T09:10:00,12-Mar-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE","8*1 mosaic, 2 exposures each",,,,,, 2009-071T11:45:00,000T09:10:00,12-Mar-09,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_105RI_LATPHASE108_VIMS,rider,,,,,, 2009-071T11:45:00,000T09:10:00,12-Mar-09,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,URSTAR,,,,,,, 2009-071T20:55:00,000T01:00:00,12-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-071T20:55:00,000T01:00:00,12-Mar-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_105RI_SATELLORB015_ISS,rider,,,,,, 2009-071T20:55:00,000T03:00:00,12-Mar-09,RADAR,SPASS Rider,Other,WU4SMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-071T21:55:00,000T02:00:00,12-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-071T23:55:00,000T01:30:00,12-Mar-09,RADAR,Prime,Titan,SMIDLCAL,,"Distant Titan Radiometry, South Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-072T00:00:00,000T11:45:00,13-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-072T02:05:00,000T09:00:00,13-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T51 Rev107 Titan Bistatic experiment on 2009/086 and the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-072T02:05:00,000T09:00:00,13-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-072T03:05:00,000T08:00:00,13-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09072_SP,rider,,,,,, 2009-072T11:45:00,000T05:00:00,13-Mar-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-072T16:45:00,000T02:00:00,13-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-072T16:45:00,000T02:00:00,13-Mar-09,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_105RI_SURVEYPTG005_CAPS,rider,,,,,, 2009-072T16:45:00,004T05:07:00,13-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-072T18:31:13,002T04:46:47,13-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-072T18:45:00,000T06:25:00,13-Mar-09,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-072T18:45:00,000T06:25:00,13-Mar-09,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_105RI_SPKMVLFLP001_ISS,rider,,,,,, 2009-072T18:45:00,000T06:25:00,13-Mar-09,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie,null,,,,,, 2009-073T01:10:00,000T00:40:00,14-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_105RI_DEEPSPACE073_SP,rider,,,,,, 2009-073T01:50:00,000T09:00:00,14-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-073T02:50:00,000T08:00:00,14-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09073_SP,rider,,,,,, 2009-073T10:50:00,000T07:30:00,14-Mar-09,ISS,SPASS Rider,SpacecraftActivity,GYROBCALB,,ISS NAC dark current calibration,ISS NAC dark current calibration,,,,,, 2009-073T18:20:00,000T09:00:00,14-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-073T19:20:00,000T08:00:00,14-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09473_SP,rider,,,,,, 2009-074T04:00:00,000T12:20:00,15-Mar-09,VIMS,Prime,rings(general),EGPHASE,,E/G Ring phase observation,null,,,,,, 2009-074T04:00:00,000T12:20:00,15-Mar-09,CIRS,SPASS Rider,rings(general),EGPHASE,,CIRS_105RI_EGPHASE119_VIMS,rider,,,,,, 2009-074T04:00:00,000T12:20:00,15-Mar-09,ISS,SPASS Rider,rings(general),EGPHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., high-phase of G or E ring",,,,,, 2009-074T16:20:00,000T00:30:00,15-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 024 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-074T16:20:00,000T00:30:00,15-Mar-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_105RI_SATELLORB024_ISS,rider,,,,,, 2009-074T18:20:00,000T09:00:00,15-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-074T19:20:00,000T08:00:00,15-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_105IC_DSCAL09074_SP,rider,,,,,, 2009-074T22:48:15,000T00:00:01,15-Mar-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 12.0 d, inc = 65.3 deg, r = 19.888 Rs, phase = 27 deg",,,,,, 2009-074T23:18:00,005T13:38:00,15-Mar-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 13.645780 Rs exit= 13.693648 Range altitude= -40595.334 km ... 40599.829,,,,,, 2009-074T23:18:00,000T02:00:00,15-Mar-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-074T23:18:00,000T20:26:32,15-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-074T23:18:00,002T03:47:00,15-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-074T23:18:00,000T04:02:00,15-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-075T01:18:00,002T01:47:00,16-Mar-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-075T04:00:00,000T01:15:00,16-Mar-09,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 58.8 range 1.9 Mkm",,,,,, 2009-075T04:00:00,000T01:15:00,16-Mar-09,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-075T04:00:00,000T01:15:00,16-Mar-09,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-075T05:15:00,000T00:30:00,16-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-075T05:45:00,000T02:00:00,16-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-075T05:45:00,000T02:00:00,16-Mar-09,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_106RI_SURVEYPTG001_CAPS,rider,,,,,, 2009-075T07:45:00,000T10:00:00,16-Mar-09,CIRS,Prime,rings(general),TMAPN20LP,,CIRS_106RI_TMAPN20LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-075T07:45:00,000T10:00:00,16-Mar-09,CIRS,SPASS Rider,rings(general),TMAPN20LP,,CIRS_106RI_TMAPN20LP001_SI,,,,,,, 2009-075T07:45:00,000T10:00:00,16-Mar-09,UVIS,SPASS Rider,rings(general),TMAPN20LP,,URSTAR,,,,,,, 2009-075T07:45:00,000T10:00:00,16-Mar-09,VIMS,SPASS Rider,rings(general),TMAPN20LP,,,null,,,,,, 2009-075T18:20:00,000T09:00:00,16-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-075T18:20:00,000T09:00:00,16-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-075T19:20:00,000T08:00:00,16-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09075_SP,rider,,,,,, 2009-075T19:44:32,001T02:07:28,16-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-076T03:20:00,000T00:40:00,17-Mar-09,CIRS,SPASS Rider,rings(general),DEEPSPACE,Deep space calibration,CIRS_106RI_DEEPSPACE076_SP,rider,,,,,, 2009-076T04:00:00,000T13:25:00,17-Mar-09,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side","30 frame mosaic, tau_IR=320 msec.",,,,,, 2009-076T04:00:00,000T13:25:00,17-Mar-09,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_106RI_APOMOSU128_VIMS,rider,,,,,, 2009-076T04:00:00,000T13:25:00,17-Mar-09,UVIS,SPASS Rider,rings(general),APOMOSU,,URSTAR,,,,,,, 2009-076T18:05:00,000T09:00:00,17-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T51 Rev107 Titan Bistatic experiment on 2009/086 and the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-076T18:05:00,000T09:00:00,17-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-076T19:05:00,000T08:00:00,17-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09076_SP,rider,,,,,, 2009-076T21:52:00,000T05:13:00,17-Mar-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-076T21:52:00,000T23:55:00,17-Mar-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-076T21:52:00,000T05:13:00,17-Mar-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-076T21:52:00,000T23:55:00,17-Mar-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-077T03:05:00,000T18:42:00,18-Mar-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-077T03:05:00,006T07:15:00,18-Mar-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-077T03:05:00,000T18:42:00,18-Mar-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-077T03:05:00,001T22:30:00,18-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-077T03:45:00,000T01:15:00,18-Mar-09,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 41.5 range 1.9 Mkm",,,,,, 2009-077T03:45:00,000T01:15:00,18-Mar-09,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-077T03:45:00,000T01:15:00,18-Mar-09,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-077T05:00:00,000T00:53:00,18-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-077T05:53:00,000T07:47:00,18-Mar-09,VIMS,Prime,rings(general),GAMCRUOCC,Gamma Cru occultation,Ring stellar occ - gamCru,"Inner A ring; do 4 at priority 2, tau=40 ms.",,,,,, 2009-077T05:53:00,000T07:47:00,18-Mar-09,CIRS,SPASS Rider,rings(general),GAMCRUOCC,Gamma Cru occultation,CIRS_106RI_GAMCRUOCC104_VIMS,rider,,,,,, 2009-077T13:40:00,000T02:40:00,18-Mar-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-077T16:20:00,000T08:00:00,18-Mar-09,CIRS,Prime,rings(general),VTMPN60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-077T16:20:00,000T08:00:00,18-Mar-09,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_106RI_VTMPN60MP001_SI,,,,,,, 2009-077T21:47:00,007T12:18:00,18-Mar-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS Survey,,,,,, 2009-077T21:47:00,007T12:18:00,18-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-077T21:47:00,001T22:12:57,18-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-078T00:20:00,000T01:14:00,19-Mar-09,CIRS,SPASS Rider,Skeletonrequest,OPNAV,Optical navigation image,CIRS_106SK_OPNAV781_NAV,rider,,,,,, 2009-078T01:35:00,000T09:00:00,19-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T51 Rev107 Titan Bistatic experiment on 2009/086 and the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-078T01:35:00,000T09:00:00,19-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-078T02:35:00,000T08:00:00,19-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09078_SP,rider,,,,,, 2009-078T10:35:00,000T02:40:00,19-Mar-09,RADAR,SPASS Rider,Other,WU4NMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-078T11:15:00,000T02:00:00,19-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-078T13:15:00,000T01:40:00,19-Mar-09,RADAR,Prime,Titan,NMIDLCAL,,"Distant Titan Radiometry, North Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-078T14:55:00,000T10:00:00,19-Mar-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_106SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. North Pole",,,,,, 2009-078T14:55:00,000T10:00:00,19-Mar-09,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2009-079T01:35:00,000T09:00:00,20-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T51 Rev107 Titan Bistatic experiment on 2009/086 and the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-079T01:35:00,000T01:00:00,20-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-079T01:35:00,000T09:00:00,20-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-079T02:35:00,000T08:00:00,20-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09079_SP,rider,,,,,, 2009-079T02:35:00,000T06:16:00,20-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-079T03:00:00,000T04:33:04,20-Mar-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-079T08:51:00,000T01:44:00,20-Mar-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-079T10:35:00,003T01:48:00,20-Mar-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-079T11:15:00,000T03:00:00,20-Mar-09,ISS,Prime,rings(general),PHOTDARK,,"intermediate phase, dark-face ring photometry","intermediate unlit #8: B = 43, phase = 117, B' = -2.2",,,,,, 2009-079T11:15:00,000T03:00:00,20-Mar-09,CIRS,SPASS Rider,rings(general),PHOTDARK,,CIRS_106RI_PHOTDARK002_ISS,rider,,,,,, 2009-079T11:15:00,000T03:00:00,20-Mar-09,VIMS,SPASS Rider,rings(general),PHOTDARK,,PhotDark mosaic,Main ring photometry,,,,,, 2009-079T14:15:00,000T01:50:00,20-Mar-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-079T14:15:00,000T01:50:00,20-Mar-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_106RI_MNRNGSHAD001_ISS,rider,,,,,, 2009-079T16:05:00,000T03:55:00,20-Mar-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-079T16:05:00,000T03:55:00,20-Mar-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,VIMS ridealong with ISS for cloud monitoring,,,,,, 2009-079T19:59:57,001T12:20:23,20-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-079T20:00:00,000T04:40:00,20-Mar-09,CIRS,Prime,rings(general),TDIFN20HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-079T20:00:00,000T04:40:00,20-Mar-09,CIRS,SPASS Rider,rings(general),TDIFN20HP,,CIRS_106RI_TDIFN20HP001_SI,,,,,,, 2009-079T20:00:00,000T04:40:00,20-Mar-09,VIMS,SPASS Rider,rings(general),TDIFN20HP,,,null,,,,,, 2009-080T00:00:00,000T00:34:00,21-Mar-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-080T00:40:00,000T10:20:00,21-Mar-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-080T01:20:00,000T09:00:00,21-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-080T02:20:00,000T08:00:00,21-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09080_SP,rider,,,,,, 2009-080T11:00:00,000T02:37:00,21-Mar-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-080T12:56:00,000T03:20:00,21-Mar-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.692927 Rs exit= 13.633542 Range altitude= 39796.316 km ... -39816.557,,,,,, 2009-080T13:37:00,000T02:38:00,21-Mar-09,CDA,Prime,DustRAM direction,RPX0030,,CDA RPXing 2009-080T14:37:00 NtH,"RPXing at 13.660548 Rs, large ring extention, small/medium inclintn",,,,,, 2009-080T16:15:00,000T03:15:00,21-Mar-09,ISS,Prime,Enceladus,PLMPHSA,,Phase Function Observation,Campaign to study phase function of plume,,,,,, 2009-080T16:15:00,000T03:15:00,21-Mar-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-080T16:15:00,000T03:15:00,21-Mar-09,VIMS,SPASS Rider,Enceladus,PLMPHSA,,,null,,,,,, 2009-080T16:16:00,004T17:49:00,21-Mar-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S49,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-080T19:30:00,000T04:20:00,21-Mar-09,CIRS,Prime,rings(general),TDIFS20HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-080T19:30:00,000T04:20:00,21-Mar-09,CIRS,SPASS Rider,rings(general),TDIFS20HP,,CIRS_106RI_TDIFS20HP001_SI,,,,,,, 2009-080T19:30:00,000T04:20:00,21-Mar-09,VIMS,SPASS Rider,rings(general),TDIFS20HP,,,null,,,,,, 2009-080T22:33:47,000T00:00:01,21-Mar-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 13.574 Rs, lat = -13 deg, phase = 153 deg",,,,,, 2009-080T23:50:00,000T01:29:00,21-Mar-09,CIRS,SPASS Rider,Skeletonrequest,OPNAV,Optical navigation image,CIRS_106SK_OPNAV801_NAV,rider,,,,,, 2009-081T01:20:00,000T09:00:00,22-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-081T02:20:00,000T08:00:00,22-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09081_SP,rider,,,,,, 2009-081T08:20:20,003T09:32:21,22-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-081T11:00:00,000T01:15:00,22-Mar-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 76.9 range 1.1 Mkm",,,,,, 2009-081T11:00:00,000T01:15:00,22-Mar-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-081T11:00:00,000T01:15:00,22-Mar-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-081T12:15:00,000T07:44:00,22-Mar-09,CIRS,Prime,rings(general),TDIFS45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-081T12:15:00,000T07:44:00,22-Mar-09,CIRS,SPASS Rider,rings(general),TDIFS45HP,,CIRS_106RI_TDIFS45HP001_SI,,,,,,, 2009-081T12:15:00,000T07:44:00,22-Mar-09,VIMS,SPASS Rider,rings(general),TDIFS45HP,,,null,,,,,, 2009-081T19:59:00,000T04:41:00,22-Mar-09,VIMS,Prime,rings(general),RCASOCC,R Cas ring occultation,Ring stellar occ - R Cas,"R_Cas occultation, outer C ring, R0=2.349, Rmin=1.339",,,,,, 2009-081T19:59:00,000T04:41:00,22-Mar-09,CIRS,SPASS Rider,rings(general),RCASOCC,R Cas ring occultation,CIRS_106RI_RCASOCC104_VIMS,rider,,,,,, 2009-082T01:20:00,000T09:00:00,23-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-082T02:20:00,000T08:00:00,23-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09082_SP,rider,,,,,, 2009-082T11:00:00,000T13:10:00,23-Mar-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-082T11:00:00,000T13:10:00,23-Mar-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_106RF_FMOVIE002_ISS,rider,,,,,, 2009-082T11:00:00,000T13:10:00,23-Mar-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,,FMOVIE,,,,,, 2009-082T12:23:00,002T12:42:00,23-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-083T00:10:00,000T00:30:00,24-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-083T01:20:00,000T09:00:00,24-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-083T02:20:00,000T08:00:00,24-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09083_SP,rider,,,,,, 2009-083T10:20:00,000T23:45:00,24-Mar-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-083T11:00:00,000T01:15:00,24-Mar-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 77.8 range 1.1 Mkm",,,,,, 2009-083T11:00:00,000T01:15:00,24-Mar-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-083T11:00:00,000T01:15:00,24-Mar-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-083T12:15:00,000T02:00:00,24-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-083T14:15:00,000T10:10:00,24-Mar-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_106SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2009-084T01:05:00,000T09:00:00,25-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-084T02:05:00,000T08:00:00,25-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09084_SP,rider,,,,,, 2009-084T10:05:00,001T00:00:00,25-Mar-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-084T10:45:00,000T02:00:00,25-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-084T12:45:00,000T11:40:00,25-Mar-09,ISS,Prime,Other,SIARNAQ,,Siarnaq rotation light curve,Siarnaq rotation light curve,,,,,, 2009-084T17:52:41,000T16:12:19,25-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-085T01:05:00,000T09:00:00,26-Mar-09,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2009-085T01:05:00,000T09:00:00,26-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-085T01:05:00,000T09:00:00,26-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-085T02:05:00,000T08:00:00,26-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_106IC_DSCAL09085_SP,rider,,,,,, 2009-085T03:00:00,000T04:37:04,26-Mar-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-085T10:05:00,000T16:38:36,26-Mar-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-085T10:05:00,000T18:46:00,26-Mar-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S S49,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-085T10:05:00,000T00:43:00,26-Mar-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-085T10:05:00,000T14:38:36,26-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-085T10:05:00,000T16:38:37,26-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-085T10:05:00,000T18:46:00,26-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-085T10:10:00,000T00:02:00,26-Mar-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S49 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-085T10:48:00,000T00:05:00,26-Mar-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-085T10:53:00,000T00:33:00,26-Mar-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-085T11:00:31,000T03:43:05,26-Mar-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-085T11:00:31,000T03:43:05,26-Mar-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-085T11:00:31,000T03:43:05,26-Mar-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-085T11:00:31,000T03:43:05,26-Mar-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Cloud and global mapping,VIMS ridealong with CIRS.,,,,,, 2009-085T11:26:00,000T00:22:59,26-Mar-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-085T11:48:59,000T15:54:37,26-Mar-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-085T14:43:36,000T02:00:00,26-Mar-09,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,MNA (Monitor NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-085T14:43:36,000T02:00:00,26-Mar-09,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Cloud monitor,,,,,, 2009-085T14:43:36,000T02:00:00,26-Mar-09,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,Global and cloud mapping,VIMS ridealong with ISS. Plan 1 cube every 20 min.,,,,,, 2009-085T16:43:36,000T03:00:00,26-Mar-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-085T16:43:36,000T03:00:00,26-Mar-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-085T16:43:36,000T02:30:00,26-Mar-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-085T16:43:36,000T03:00:00,26-Mar-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-085T16:43:36,000T03:00:00,26-Mar-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan. Cloud mapping,VIMS ridealong with CIRS.,,,,,, 2009-085T19:43:36,000T04:00:00,26-Mar-09,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,GMA (Global Map),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-085T19:43:36,000T04:00:00,26-Mar-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Cloud monitor,,,,,, 2009-085T19:43:36,000T04:00:00,26-Mar-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global mapping,VIMS ridealong with ISS. Plan 1 cube every 15 min.,,,,,, 2009-085T23:43:36,000T03:00:00,26-Mar-09,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping,Regional Mapping of Titan.,,,,,, 2009-085T23:43:36,000T03:00:00,26-Mar-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Cloud monitor,,,,,, 2009-085T23:43:36,000T03:00:00,26-Mar-09,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-085T23:43:36,000T03:00:00,26-Mar-09,UVIS,SPASS Rider,Titan,REGMAP,Regional mapping,UVIS Rider to VIMS REGMAP,UVIS Rider to VIMS Titan REGMAP,,,,,, 2009-086T00:43:36,000T08:00:00,27-Mar-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,MAPS_Titan_Flyby,"T051 is another near-noon (10.5 h SLT), upstream flank-out flyby, with a minimum altitude of 1000 km, which is almost parallel to T050. Therefore, the measurements will be complementary to T050, providing a description of the draping and the pileup of the external magnetic field around Titan on the dayside hemisphere. As in the previous flybys, Titan could be found in the magnetosheath during T051. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-086T02:43:36,000T01:08:00,27-Mar-09,ISS,Prime,Titan,REGMAP,Regional mapping,RMA (Regional Map),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-086T02:43:36,000T01:20:00,27-Mar-09,CAPS,SPASS Rider,Titan,T51INBND,,Inbound 106TI (T51),Inbound 106TI (T51),,,,,, 2009-086T02:43:36,000T01:08:00,27-Mar-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Cloud monitor,,,,,, 2009-086T02:43:36,000T01:08:00,27-Mar-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping,VIMS ridealong with ISS. Obtain cubes per 6 min. dwell times for regional mapping.,,,,,, 2009-086T02:43:36,000T01:30:00,27-Mar-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-086T02:43:37,000T01:00:00,27-Mar-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-086T02:58:30,000T02:00:06,27-Mar-09,RSS,SPASS Rider,Titan,THERMAL,Thermal stabilization period,RSS Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-086T03:43:36,000T01:00:00,27-Mar-09,INMS,Non-SPASS,Titan,TITAN51,,Titan Flyby,Titan observation,,,,,, 2009-086T03:43:37,000T01:08:23,27-Mar-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-086T03:51:36,000T00:22:00,27-Mar-09,CIRS,SPASS Rider,Titan,TRANS,,,Cloud monitor,,,,,, 2009-086T03:52:36,000T01:06:00,27-Mar-09,VIMS,Prime,Titan,HIRES,High resolution image,Titan Mosaic,"High resolution cubes. Path over Ontario lake 12 minutes before closest approach (-70, 180W) with images at 1.5 km/pixel. High resolution image of Titan at (-30,230W). Noodle mode? No more turn to INMS (10/24/2008)",,,,,, 2009-086T03:52:36,000T00:51:00,27-Mar-09,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),Lacus Ontario,,,,,, 2009-086T04:03:36,000T01:20:00,27-Mar-09,CAPS,SPASS Rider,Titan,T51CLOSE,,Closest Approach 106TI (T51),Closest Approach 106TI (T51),,,,,, 2009-086T04:13:36,000T00:30:00,27-Mar-09,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Cloud monitor,,,,,, 2009-086T04:13:36,000T00:37:23,27-Mar-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-086T04:43:36,000T00:15:00,27-Mar-09,CIRS,SPASS Rider,Titan,TITAN51,,,Cloud monitor,,,,,, 2009-086T04:43:36,000T00:15:00,27-Mar-09,INMS,SPASS Rider,Titan,TITAN51,,Titan Flyby,Prime Titan observation,,,,,, 2009-086T04:51:00,007T20:38:00,27-Mar-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End:SApo,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-086T04:51:00,007T20:38:00,27-Mar-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-086T04:51:00,000T00:22:36,27-Mar-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-086T04:51:35,000T00:00:01,27-Mar-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.5 d, inc = 65.2 deg, r = 19.723 Rs, phase = 29 deg",,,,,, 2009-086T04:52:00,000T00:51:37,27-Mar-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-086T04:58:36,000T01:13:00,27-Mar-09,RSS,Prime,Titan,BISTATOUT,RSS Bistatic egress observation,RSS Bistatic Obs of Titan T51 (outbound),"Bistatic scattering measurments at three radio wavelengths to determine the physical properties of Titan's surface, including reflectivity, dielectric constant, and roughness.",,,,,, 2009-086T04:58:36,000T01:13:00,27-Mar-09,CIRS,SPASS Rider,Titan,BISTATOUT,RSS Bistatic egress observation,,Cloud monitor,,,,,, 2009-086T04:58:36,000T00:45:00,27-Mar-09,INMS,Non-SPASS,Titan,TITAN51,,Titan Flyby,Titan observation,,,,,, 2009-086T05:13:36,000T01:30:00,27-Mar-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-086T05:23:36,000T01:20:00,27-Mar-09,CAPS,SPASS Rider,Titan,T51OUTBND,,Outbound 106TI (T51),Outbound 106TI (T51),,,,,, 2009-086T05:43:36,001T10:21:23,27-Mar-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-086T05:43:37,000T01:00:00,27-Mar-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-086T06:11:36,000T00:21:07,27-Mar-09,CIRS,SPASS Rider,Saturn,DFPWBIAS,,,Cloud monitor,,,,,, 2009-086T06:32:43,000T03:10:53,27-Mar-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-086T06:35:36,000T03:08:00,27-Mar-09,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-086T06:35:36,000T03:08:00,27-Mar-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Global mapping,VIMS ridealong with CIRS.,,,,,, 2009-086T06:43:36,002T11:03:23,27-Mar-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-086T06:43:37,001T08:46:59,27-Mar-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-086T08:43:36,001T08:06:24,27-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-086T09:43:36,000T04:00:00,27-Mar-09,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-086T09:43:36,000T04:00:00,27-Mar-09,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-086T09:43:36,000T04:00:00,27-Mar-09,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),global map,,,,,, 2009-086T09:43:36,000T04:00:00,27-Mar-09,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-086T09:43:36,000T04:00:00,27-Mar-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Mid-IR Limb mapping,VIMS ridealong with CIRS.,,,,,, 2009-086T13:43:36,000T01:00:00,27-Mar-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-086T13:43:36,000T01:00:00,27-Mar-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Cloud monitor,,,,,, 2009-086T13:43:36,000T01:00:00,27-Mar-09,UVIS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Rider ro ISS PHOTOMWAC,Stare at Titan,,,,,, 2009-086T13:43:36,000T01:00:00,27-Mar-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan. Cloud mapping,VIMS ridealong with ISS.,,,,,, 2009-086T14:43:36,000T03:00:00,27-Mar-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-086T14:43:36,000T03:00:00,27-Mar-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-086T14:43:36,000T03:00:00,27-Mar-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-086T14:43:36,000T03:00:00,27-Mar-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-086T14:43:36,000T03:00:00,27-Mar-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir Comp.,VIMS ridealong with CIRS.,,,,,, 2009-086T17:43:36,000T00:30:00,27-Mar-09,ISS,Prime,Titan,NIGHTNA,,NNA (Nightside NAC Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-086T17:43:36,000T00:30:00,27-Mar-09,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Cloud monitor,,,,,, 2009-086T17:43:36,000T00:30:00,27-Mar-09,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare at nightside of Titan,VIMS ridealong with ISS.,,,,,, 2009-086T18:13:36,000T05:12:00,27-Mar-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-086T18:13:36,000T05:12:00,27-Mar-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-086T18:13:36,000T05:12:00,27-Mar-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-086T18:13:36,000T05:12:00,27-Mar-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR temp. mapping,VIMS ridealong with CIRS.,,,,,, 2009-086T23:25:36,000T00:30:00,27-Mar-09,ISS,Prime,Titan,NIGHTNA,,NNA (Nightside NAC Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-086T23:25:36,000T00:30:00,27-Mar-09,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Cloud monitor,,,,,, 2009-086T23:25:36,000T00:30:00,27-Mar-09,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare at nightside of Titan,VIMS ridealong with ISS.,,,,,, 2009-087T00:50:00,006T08:44:00,28-Mar-09,RPWS,Non-SPASS,co-rotation,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dusk-side magnetospheric boundaries at a variety of radial distances",,,,,, 2009-087T00:50:00,000T09:00:00,28-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-087T01:50:00,000T08:00:00,28-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09087_SP,rider,,,,,, 2009-087T05:33:15,000T00:00:01,28-Mar-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 19.667 Rs, lat = 21 deg, phase = 28 deg",,,,,, 2009-087T09:25:00,000T07:25:00,28-Mar-09,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2009-087T09:50:00,000T07:00:00,28-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-087T10:50:00,000T06:00:00,28-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09487_SP,rider,,,,,, 2009-087T15:30:36,001T02:16:24,28-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-087T16:05:00,001T00:00:00,28-Mar-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-087T16:50:00,001T00:57:00,28-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-087T17:30:00,000T10:00:00,28-Mar-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_107SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole northern hemisphere",,,,,, 2009-088T03:30:00,000T00:55:00,29-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-088T03:30:00,000T00:55:00,29-Mar-09,CIRS,SPASS Rider,Other,SATELLORB,Satellite orbit campaign,CIRS_107OT_SATELLORB005_ISS,rider,,,,,, 2009-088T04:25:00,000T02:00:00,29-Mar-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-088T07:05:00,000T09:00:00,29-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-088T08:05:00,000T08:00:00,29-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09088_SP,rider,,,,,, 2009-088T16:05:00,000T17:45:00,29-Mar-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-088T16:45:00,000T06:35:00,29-Mar-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-088T16:45:00,000T06:35:00,29-Mar-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_107RF_FMOVIE002_ISS,rider,,,,,, 2009-088T16:45:00,000T06:35:00,29-Mar-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,ISS rider,,,,,, 2009-088T17:47:00,000T22:10:00,29-Mar-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-088T17:47:00,000T22:10:00,29-Mar-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-088T17:47:00,000T22:10:00,29-Mar-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-088T17:47:00,000T22:10:00,29-Mar-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-088T23:20:00,000T01:29:00,29-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_107SK_OPNAV881_NAV,rider,,,,,, 2009-089T00:50:00,000T09:00:00,30-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-089T01:50:00,000T08:00:00,30-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09089_SP,rider,,,,,, 2009-089T09:50:00,000T08:40:00,30-Mar-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-089T10:30:00,000T02:00:00,30-Mar-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-089T12:30:00,000T01:29:00,30-Mar-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-089T12:30:00,000T01:29:00,30-Mar-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_107RI_MNRNGSHAD002_ISS,rider,,,,,, 2009-089T13:59:00,000T00:30:00,30-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-089T14:29:00,000T02:11:00,30-Mar-09,CIRS,Prime,rings(general),SATREFL,,CIRS_107RI_SATREFL089_PRIME;,null,,,,,, 2009-089T14:29:00,000T02:11:00,30-Mar-09,CIRS,SPASS Rider,rings(general),SATREFL,,CIRS_107RI_SATREFL089_SI,,,,,,, 2009-089T15:57:00,002T19:30:00,30-Mar-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-089T15:57:00,002T19:30:00,30-Mar-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-089T15:57:00,002T19:30:00,30-Mar-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-089T17:20:00,000T09:00:00,30-Mar-09,RSS,SPASS Rider,Titan,BISTATORT,RSS Bistatic operational readiness test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T52 Rev107-108 Titan Bistatic and occultation experiment on 2009/094.",,,,,, 2009-089T17:20:00,000T09:00:00,30-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-089T18:20:00,000T08:00:00,30-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09489_SP,rider,,,,,, 2009-089T18:30:00,000T02:00:00,30-Mar-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-089T20:30:00,001T13:05:00,30-Mar-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-090T03:00:00,000T03:35:00,31-Mar-09,ISS,Prime,InstrumentCalibration,POLCAL,,ISS Polarizer calibration,"NAC to Titan Like CHARGEX requests, rotate around the Y axis 120 degrees in 30 degree steps and image in three polarizers at each point. Initial secondary will be Pos Z or Neg Z to sun.",,,,,, 2009-090T03:00:00,000T03:35:00,31-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,POLCAL,,CIRS_107IC_POLCAL002,rider,,,,,, 2009-090T07:05:00,000T09:00:00,31-Mar-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-090T08:05:00,000T08:00:00,31-Mar-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09090_SP,rider,,,,,, 2009-090T16:45:00,000T06:40:00,31-Mar-09,CIRS,Prime,rings(general),VTMPN60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-090T16:45:00,000T06:40:00,31-Mar-09,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_107RI_VTMPN60MP002_SI,,,,,,, 2009-090T23:25:00,000T00:30:00,31-Mar-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-091T00:35:00,000T09:00:00,1-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-091T01:35:00,000T08:00:00,1-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09091_SP,rider,,,,,, 2009-091T09:35:00,000T16:30:00,1-Apr-09,INMS,Non-SPASS,Saturn,SURVPOTMA,,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-091T10:15:00,000T06:20:00,1-Apr-09,CIRS,Prime,rings(general),TMAPN45MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-091T10:15:00,000T06:20:00,1-Apr-09,CIRS,SPASS Rider,rings(general),TMAPN45MP,,CIRS_107RI_TMAPN45MP001_SI,,,,,,, 2009-091T17:05:00,000T09:00:00,1-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-091T18:05:00,000T08:00:00,1-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09491_SP,rider,,,,,, 2009-092T02:05:00,001T07:29:00,2-Apr-09,INMS,Non-SPASS,Saturn,SURVBOTMA,,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-092T02:45:00,000T03:25:00,2-Apr-09,CIRS,Prime,rings(general),TDIFN45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-092T02:45:00,000T03:25:00,2-Apr-09,CIRS,SPASS Rider,rings(general),TDIFN45HP,,CIRS_107RI_TDIFN45HP001_SI,,,,,,, 2009-092T06:10:00,000T03:00:00,2-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-092T09:50:00,000T06:00:00,2-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-092T10:50:00,000T05:00:00,2-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09092_SP,rider,,,,,, 2009-092T11:27:00,000T03:00:00,2-Apr-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-092T11:27:00,000T03:00:00,2-Apr-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-092T11:27:00,000T03:00:00,2-Apr-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-092T11:27:00,000T03:00:00,2-Apr-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-092T14:27:00,000T19:07:00,2-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-092T14:27:00,000T02:03:00,2-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-092T14:27:00,000T19:07:00,2-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-092T16:30:00,000T06:45:00,2-Apr-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-092T23:15:00,000T01:18:00,2-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_107SK_OPNAV921_NAV,rider,,,,,, 2009-092T23:15:00,000T10:19:00,2-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-093T00:34:00,000T09:00:00,3-Apr-09,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2009-093T00:34:00,000T09:00:00,3-Apr-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-093T00:34:00,000T09:00:00,3-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-093T01:34:00,000T08:00:00,3-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_107IC_DSCAL09093_SP,rider,,,,,, 2009-093T09:34:00,000T14:13:47,3-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-093T09:34:00,000T15:13:47,3-Apr-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-093T09:34:00,000T12:13:47,3-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-093T09:34:00,000T14:13:48,3-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-093T10:29:34,000T01:48:13,3-Apr-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-093T10:29:34,000T01:48:13,3-Apr-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-093T10:29:34,000T01:48:13,3-Apr-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-093T10:29:34,000T01:48:13,3-Apr-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp Map.,VIMS ridealong with CIRS.,,,,,, 2009-093T12:17:47,000T00:30:00,3-Apr-09,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Night NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-093T12:17:47,000T00:30:00,3-Apr-09,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride with ISS.,,,,,, 2009-093T12:17:47,000T00:30:00,3-Apr-09,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare at Titan's nightside,VIMS ridealong with ISS. Stare at Titan's nightside. 6 min dwell times allow 5 images.,,,,,, 2009-093T12:47:47,000T04:00:00,3-Apr-09,VIMS,Prime,Titan,CLOUDMAP,Cloud map,Cloud Mapping of Titan,Stare at Titan for cloud mapping. Plan 64 x 64 cubes of various exposures. Un-illuminated approach (phase ~105).,,,,,, 2009-093T12:47:47,000T04:00:00,3-Apr-09,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride with VIMS.,,,,,, 2009-093T12:47:47,000T04:00:00,3-Apr-09,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-093T16:47:47,000T02:40:00,3-Apr-09,VIMS,Prime,Titan,MEDRESDRK,Medium resolution global mapping,Global mapping,Global mapping of Titan. Plan 2 x 2 mosaic and cubes at various exposure times. Un-illuminated approach (phase ~105).,,,,,, 2009-093T16:47:47,000T02:40:00,3-Apr-09,CIRS,SPASS Rider,Titan,MEDRESDRK,Medium resolution global mapping,,Ride with VIMS.,,,,,, 2009-093T16:47:47,000T02:40:00,3-Apr-09,ISS,SPASS Rider,Titan,MEDRESDRK,Medium resolution global mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-093T16:47:47,000T02:40:00,3-Apr-09,RADAR,SPASS Rider,Titan,T52WARMUP,,Warmup for T52 Radiometry,,,,,,, 2009-093T19:27:47,000T02:00:00,3-Apr-09,RADAR,Prime,Titan,T52INRAD,,T52 Inbound Radiometry-part 1,,,,,,, 2009-093T21:28:47,000T00:59:00,3-Apr-09,RADAR,Prime,Titan,T52INRAD,,T52 Inbound Radiometry-part2,,,,,,, 2009-093T21:47:47,000T08:00:00,3-Apr-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T52 flyby,"T52 is a flank-out, post-dusk, high altitude (>4000 km) flyby that will be useful to characterize the background field in which Titan sits. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2009-093T22:27:47,000T02:00:00,3-Apr-09,UVIS,Prime,Star,ALPERITI,,Titan Occults Alpha Eri,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2009-093T22:27:47,000T02:00:00,3-Apr-09,RSS,SPASS Rider,Titan,THERMAL,Thermal stabilization period,RSS Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-093T22:28:47,000T01:59:00,3-Apr-09,CIRS,SPASS Rider,Titan,ALPERITI,,,Ride with VIMS.,,,,,, 2009-093T23:47:47,000T01:00:00,3-Apr-09,CAPS,SPASS Rider,Titan,T52INBND,,Inbound 108TI (T52),Inbound 108TI (T52),,,,,, 2009-093T23:47:47,000T01:30:00,3-Apr-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-093T23:47:48,000T01:00:00,3-Apr-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-094T00:27:47,000T00:58:00,4-Apr-09,RSS,Prime,Titan,BISTATIN,RSS Bistatic ingress observation,RSS Bistatic Obs of Titan T52 (ingress),"Bistatic scattering measurments at three radio wavelengths to determine the physical properties of Titan's surface, including reflectivity, dielectric constant, and roughness.",,,,,, 2009-094T00:47:47,000T02:00:00,4-Apr-09,CAPS,SPASS Rider,Titan,T52CLOSE,,Closest Approach 108TI (T52),Closest Approach 108TI (T52),,,,,, 2009-094T00:47:47,000T00:40:00,4-Apr-09,INMS,Non-SPASS,Titan,TITAN52,,Titan Flyby,Titan observation,,,,,, 2009-094T00:47:48,000T00:41:12,4-Apr-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-094T01:17:47,000T00:11:12,4-Apr-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-094T01:25:47,000T00:34:00,4-Apr-09,RSS,Prime,Titan,OCC,Occultation,RSS OCC of Titan T52,RSS ingress/egress occultation of Titan's atmosphere and ionosphere,,,,,, 2009-094T01:27:47,000T00:40:00,4-Apr-09,INMS,Non-SPASS,Titan,TITAN52,,Titan Flyby,Titan observation,,,,,, 2009-094T01:29:00,000T01:18:48,4-Apr-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-094T01:29:00,012T21:36:00,4-Apr-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo End:SApo,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-094T01:29:00,001T07:50:00,4-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-094T01:29:00,000T00:48:47,4-Apr-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-094T01:29:37,000T00:00:01,4-Apr-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.8 d, inc = 63.3 deg, r = 20.921 Rs, phase = 151 deg",,,,,, 2009-094T01:59:47,000T01:16:00,4-Apr-09,RSS,Prime,Titan,BISTATOUT,RSS Bistatic egress observation,RSS Bistatic Obs of Titan T52 (egress),"Bistatic scattering measurments at three radio wavelengths to determine the physical properties of Titan's surface, including reflectivity, dielectric constant, and roughness.",,,,,, 2009-094T02:07:47,000T00:40:00,4-Apr-09,INMS,Non-SPASS,Titan,TITAN52,,Titan Flyby,Titan observation,,,,,, 2009-094T02:17:47,000T01:30:00,4-Apr-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-094T02:47:47,000T01:00:00,4-Apr-09,CAPS,SPASS Rider,Titan,T52OUTBND,,Outbound 108TI (T52),Outbound 108TI (T52),,,,,, 2009-094T02:47:47,001T06:31:12,4-Apr-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-094T02:47:48,000T01:00:00,4-Apr-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-094T03:15:47,000T00:21:07,4-Apr-09,CIRS,SPASS Rider,Titan,DFPWBIAS,,,Ride with VIMS.,,,,,, 2009-094T03:15:47,000T00:22:00,4-Apr-09,VIMS,SPASS Rider,Titan,TRANS,,Transition to RWA-,"2 cubes obtained during RCS/RWA transition. Secondary pointing: -Y to Titan, -Z to RA/DEC = 340, 0 deg. Phase = 82 deg- (-60,240W).",,,,,, 2009-094T03:37:47,000T01:40:00,4-Apr-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-094T03:37:47,000T01:40:00,4-Apr-09,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-094T03:37:47,000T01:40:00,4-Apr-09,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-094T03:37:47,000T01:40:00,4-Apr-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,VIMS ridealong with CIRS for global mapping. Phase = 80 deg.,,,,,, 2009-094T03:47:47,000T11:12:12,4-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-094T03:47:48,000T20:31:12,4-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-094T05:17:47,000T01:30:00,4-Apr-09,ISS,Prime,Titan,REGMAP,Regional mapping,NAC Regional Map,regional map,,,,,, 2009-094T05:17:47,000T01:30:00,4-Apr-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride with ISS.,,,,,, 2009-094T05:17:47,000T01:30:00,4-Apr-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"VIMS ridealong with ISS. Assume 6 min. dwell times, 1 cube / 10 min for 9. Phase = 75 deg.",,,,,, 2009-094T05:47:47,001T03:31:13,4-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-094T06:47:47,000T04:00:00,4-Apr-09,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2009-094T06:47:47,000T04:00:00,4-Apr-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride with ISS.,,,,,, 2009-094T06:47:47,000T04:00:00,4-Apr-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"VIMS ridealong with ISS for global mapping. 6 min dwell times, 1 cube / 30 min for 8 plus 2 extra cubes.",,,,,, 2009-094T10:47:47,000T03:00:00,4-Apr-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-094T10:47:47,000T03:00:00,4-Apr-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-094T10:47:47,000T03:00:00,4-Apr-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-094T10:47:47,000T03:00:00,4-Apr-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-094T10:47:47,000T03:00:00,4-Apr-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir Comp.,VIMS ridealong with CIRS for global mapping. Obtain 1 cube / 30 min for 6 cubes.,,,,,, 2009-094T13:47:47,000T02:00:00,4-Apr-09,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,MON (NAC Monitor),global map,,,,,, 2009-094T13:47:47,000T02:00:00,4-Apr-09,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Ride with ISS.,,,,,, 2009-094T13:47:47,000T02:00:00,4-Apr-09,VIMS,SPASS Rider,Titan,MONITOR,,Stare at Titan,"VIMS ridealong with ISS for global mapping. 6 min dwell times, 1 cube / 30 min for 4 cubes.",,,,,, 2009-094T15:00:00,000T08:57:36,4-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-094T15:47:47,000T07:36:47,4-Apr-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-094T15:47:47,000T07:36:47,4-Apr-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (6 integrations total = 12 frames, 0.5 Mb/frame)",,,,,, 2009-094T15:47:47,000T07:36:47,4-Apr-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-094T15:47:47,000T07:36:47,4-Apr-09,UVIS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,UVIS Rider to CIRS MIRTMAP,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-094T15:47:47,000T07:36:47,4-Apr-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR mappng,VIMS ridealong with CIRS for global mapping.,,,,,, 2009-094T23:57:36,009T00:59:24,4-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-095T00:14:00,000T09:05:00,5-Apr-09,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2009-095T00:19:00,000T15:07:06,5-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-095T00:19:00,000T09:00:00,5-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-095T01:19:00,000T08:00:00,5-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09095_SP,rider,,,,,, 2009-095T09:19:00,000T04:11:00,5-Apr-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-095T09:19:00,008T15:38:00,5-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-095T09:19:00,011T13:46:00,5-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-095T09:59:00,000T01:15:00,5-Apr-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 70.1 range 0.6 Mkm",,,,,, 2009-095T09:59:00,000T01:15:00,5-Apr-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-095T09:59:00,000T01:15:00,5-Apr-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-095T11:14:00,000T01:56:00,5-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-095T13:10:00,000T02:59:00,5-Apr-09,VIMS,Prime,rings(general),BETPEGOCC,,Ring stellar occ - betPeg,"betPeg occultation, 1 of 3, F-B rings, R0=2.348, Rf=1.422, Rmin=1.422",,,,,, 2009-095T13:10:00,000T02:59:00,5-Apr-09,CIRS,SPASS Rider,rings(general),BETPEGOCC,,CIRS_108RI_BETPEGOCC201_VIMS,rider,,,,,, 2009-095T13:30:00,000T02:00:00,5-Apr-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-095T15:26:06,004T08:59:25,5-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-095T15:30:00,001T17:49:00,5-Apr-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-095T16:09:00,000T04:30:00,5-Apr-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE",Do 6 at priority 2,,,,,, 2009-095T16:09:00,000T04:30:00,5-Apr-09,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_108RI_LATPHASE110_VIMS,rider,,,,,, 2009-095T20:39:00,000T03:00:00,5-Apr-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Narvi and Thrymr observations,Observations of outer moons Narvi and Thrymr.,,,,,, 2009-096T00:19:00,000T09:00:00,6-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-096T01:19:00,000T08:00:00,6-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09096_SP,rider,,,,,, 2009-096T09:59:00,000T01:15:00,6-Apr-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 68.7 range 1 Mkm",,,,,, 2009-096T09:59:00,000T01:15:00,6-Apr-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-096T09:59:00,000T01:15:00,6-Apr-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-096T11:14:00,000T12:25:00,6-Apr-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning S. hemisphere + pole, may be split in half by downlink",,,,,, 2009-097T00:19:00,000T09:00:00,7-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-097T01:19:00,000T08:00:00,7-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09097_SP,rider,,,,,, 2009-097T09:19:00,000T23:45:00,7-Apr-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-097T09:59:00,000T10:00:00,7-Apr-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_108SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2009-097T19:59:00,000T02:00:00,7-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-097T21:59:00,000T00:35:00,7-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-097T21:59:00,000T00:35:00,7-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_108RI_MNRNGSHAD003_ISS,rider,,,,,, 2009-097T22:34:00,000T01:29:00,7-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_108SK_OPNAV971_NAV,rider,,,,,, 2009-098T00:04:00,000T09:00:00,8-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-098T01:04:00,000T08:00:00,8-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09098_SP,rider,,,,,, 2009-098T09:04:00,004T06:00:00,8-Apr-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-098T09:44:00,000T01:15:00,8-Apr-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 63.7 range 1.2 Mkm",,,,,, 2009-098T09:44:00,000T01:15:00,8-Apr-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-098T09:44:00,000T01:15:00,8-Apr-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-098T10:59:00,000T08:00:00,8-Apr-09,CIRS,Prime,rings(general),VTMPS60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-098T10:59:00,000T08:00:00,8-Apr-09,CIRS,SPASS Rider,rings(general),VTMPS60MP,,CIRS_108RI_VTMPS60MP002_SI,,,,,,, 2009-098T10:59:00,000T08:00:00,8-Apr-09,VIMS,SPASS Rider,rings(general),VTMPS60MP,,,null,,,,,, 2009-098T11:00:00,000T09:10:00,8-Apr-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-098T18:59:00,000T01:20:00,8-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-098T18:59:00,000T01:20:00,8-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,SATELLORB,Satellite orbit campaign,CIRS_108OT_SATELLORB003_ISS,rider,,,,,, 2009-098T20:19:00,000T03:05:00,8-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-098T20:19:00,000T03:05:00,8-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_108RI_MNRNGSHAD005_ISS,rider,,,,,, 2009-098T23:41:35,000T00:00:01,8-Apr-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 18.686 Rs, lat = -51 deg, phase = 76 deg",,,,,, 2009-099T00:04:00,000T09:00:00,9-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-099T01:04:00,000T08:00:00,9-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09099_SP,rider,,,,,, 2009-099T09:44:00,000T01:15:00,9-Apr-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 60 range 1 Mkm",,,,,, 2009-099T09:44:00,000T01:15:00,9-Apr-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-099T09:44:00,000T01:15:00,9-Apr-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-099T10:59:00,000T08:00:00,9-Apr-09,CIRS,Prime,rings(general),TMAPS45MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-099T10:59:00,000T08:00:00,9-Apr-09,CIRS,SPASS Rider,rings(general),TMAPS45MP,,CIRS_108RI_TMAPS45MP001_SI,,,,,,, 2009-099T10:59:00,000T08:00:00,9-Apr-09,VIMS,SPASS Rider,rings(general),TMAPS45MP,,,null,,,,,, 2009-099T18:59:00,000T02:00:00,9-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-099T20:59:00,000T01:50:00,9-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-099T20:59:00,000T01:50:00,9-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_108RI_MNRNGSHAD006_ISS,rider,,,,,, 2009-099T22:49:00,000T00:35:00,9-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-100T00:04:00,000T09:00:00,10-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-100T00:25:31,002T19:37:27,10-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-100T01:04:00,000T08:00:00,10-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09100_SP,rider,,,,,, 2009-100T09:44:00,000T05:46:00,10-Apr-09,ISS,Prime,rings(general),SPKMVLFLP,,Lit Face Low Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-100T09:44:00,000T05:46:00,10-Apr-09,CIRS,SPASS Rider,rings(general),SPKMVLFLP,,CIRS_108RI_SPKMVLFLP001_ISS,rider,,,,,, 2009-100T09:44:00,000T05:46:00,10-Apr-09,VIMS,SPASS Rider,rings(general),SPKMVLFLP,,Spoke movie,null,,,,,, 2009-100T15:30:00,000T00:30:00,10-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-100T16:00:00,000T07:24:00,10-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-101T00:04:00,000T09:00:00,11-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-101T01:04:00,000T08:00:00,11-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09101_SP,rider,,,,,, 2009-101T09:04:00,000T01:00:00,11-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAVK,,CIRS_108SK_OPNAVK001_NAV,rider,,,,,, 2009-101T10:05:00,000T10:00:00,11-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-101T20:05:00,000T02:00:00,11-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-101T22:05:00,000T06:44:00,11-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-102T04:49:00,000T01:14:00,12-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_108SK_OPNAV021_NAV,rider,,,,,, 2009-102T06:04:00,000T09:00:00,12-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-102T07:04:00,000T08:00:00,12-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09102_SP,rider,,,,,, 2009-102T15:04:00,000T17:45:00,12-Apr-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-102T15:44:00,000T07:00:00,12-Apr-09,CIRS,Prime,rings(general),TMAPN30LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-102T15:44:00,000T07:00:00,12-Apr-09,CIRS,SPASS Rider,rings(general),TMAPN30LP,,CIRS_108RI_TMAPN30LP001_SI,,,,,,, 2009-102T20:02:58,001T13:25:02,12-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-102T22:44:00,000T00:25:00,12-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-102T23:49:00,000T09:00:00,12-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-103T00:49:00,000T08:00:00,13-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09103_SP,rider,,,,,, 2009-103T08:49:00,003T14:17:00,13-Apr-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-103T09:29:00,000T11:09:00,13-Apr-09,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side",Do 15 unlit side at priority 2 (~every third orbit),,,,,, 2009-103T09:29:00,000T11:09:00,13-Apr-09,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_108RI_APOMOSU130_VIMS,rider,,,,,, 2009-103T20:38:00,000T02:00:00,13-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-103T22:38:00,000T00:30:00,13-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 018 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-103T23:48:00,000T09:00:00,13-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-104T00:48:00,000T08:00:00,14-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09104_SP,rider,,,,,, 2009-104T00:57:00,001T01:45:00,14-Apr-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-104T00:57:00,001T01:45:00,14-Apr-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-104T00:57:00,001T01:45:00,14-Apr-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-104T09:28:00,000T02:11:00,14-Apr-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-104T09:28:00,000T02:11:00,14-Apr-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-104T11:39:00,000T04:15:00,14-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-104T11:39:00,000T04:15:00,14-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_108RI_MNRNGSHAD010_ISS,rider,,,,,, 2009-104T11:39:00,002T11:27:00,14-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-104T15:54:00,000T07:14:00,14-Apr-09,CIRS,Prime,rings(general),SATREFL,,CIRS_108RI_SATREFL104_PRIME;,null,,,,,, 2009-104T15:54:00,000T07:14:00,14-Apr-09,CIRS,SPASS Rider,rings(general),SATREFL,,CIRS_108RI_SATREFL104_SI,,,,,,, 2009-104T23:48:00,000T09:00:00,14-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-105T00:48:00,000T08:00:00,15-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09105_SP,rider,,,,,, 2009-105T02:42:00,003T05:15:00,15-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-105T02:42:00,003T05:15:00,15-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-105T09:28:00,000T01:55:00,15-Apr-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Ijiraq observation,Observation (mosaic) of outer moon Ijiraq,,,,,, 2009-105T11:23:00,000T10:00:00,15-Apr-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_108SA_COMPSIT005,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-105T18:23:00,000T03:00:00,15-Apr-09,RADAR,SPASS Rider,Other,WU4NHIGL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-105T21:23:00,000T01:30:00,15-Apr-09,RADAR,Prime,Titan,NHIGLCAL,,"Distant Titan Radiometry, North High Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-105T23:33:00,000T09:00:00,15-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-106T00:33:00,000T08:00:00,16-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_108IC_DSCAL09106_SP,rider,,,,,, 2009-106T09:13:00,000T01:15:00,16-Apr-09,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 112.6 range 1.3 Mkm",,,,,, 2009-106T09:13:00,000T01:15:00,16-Apr-09,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-106T09:13:00,000T01:15:00,16-Apr-09,UVIS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-106T10:28:00,000T10:05:00,16-Apr-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-106T10:28:00,000T10:05:00,16-Apr-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_108RF_FMOVIE001_ISS,rider,,,,,, 2009-106T10:28:00,000T10:05:00,16-Apr-09,RADAR,SPASS Rider,Other,WU4NMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-106T10:28:00,000T10:05:00,16-Apr-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,Priority 1,,,,,, 2009-106T20:33:00,000T01:30:00,16-Apr-09,RADAR,Prime,Titan,NMIDLCAL,,"Distant Titan Radiometry, North Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-106T22:03:00,000T01:29:00,16-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_108SK_OPNAV061_NAV,rider,,,,,, 2009-106T23:05:00,015T02:32:00,16-Apr-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo End:SAp,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-106T23:05:00,002T09:13:00,16-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-106T23:05:32,000T00:00:01,16-Apr-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 61.7 deg, r = 21.814 Rs, phase = 104 deg",,,,,, 2009-106T23:06:00,000T09:27:00,16-Apr-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-106T23:06:00,001T08:51:00,16-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-106T23:33:00,000T09:00:00,16-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-107T00:33:00,000T08:00:00,17-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09107_SP,rider,,,,,, 2009-107T08:33:00,001T00:00:00,17-Apr-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-107T09:13:00,000T02:47:00,17-Apr-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-107T09:13:00,000T02:47:00,17-Apr-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2009-107T12:00:00,000T08:00:00,17-Apr-09,ISS,Prime,rings(general),LRHPENKMV,,"Encke Ringlet Movie, need 2 of 7","Low res, high phase movies of Encke Ringlets; need 2 of 7, widely spaced.",,,,,, 2009-107T12:00:00,000T08:00:00,17-Apr-09,CIRS,SPASS Rider,rings(general),LRHPENKMV,,CIRS_109RI_LRHPENKMV001_ISS,rider,,,,,, 2009-107T12:00:00,000T08:00:00,17-Apr-09,VIMS,SPASS Rider,rings(general),LRHPENKMV,,Encke gap high phase movie,null,,,,,, 2009-107T20:00:00,000T02:00:00,17-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-107T22:00:00,000T00:53:00,17-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-107T22:00:00,000T00:53:00,17-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_109RI_MNRNGSHAD002_ISS,rider,,,,,, 2009-107T23:33:00,000T09:00:00,17-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-108T00:33:00,000T08:00:00,18-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09108_SP,rider,,,,,, 2009-108T07:57:00,000T04:35:00,18-Apr-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-108T07:57:00,000T04:35:00,18-Apr-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-108T07:57:00,000T04:35:00,18-Apr-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-108T07:57:00,000T00:21:00,18-Apr-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-108T08:18:00,000T04:14:00,18-Apr-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-108T08:33:00,000T23:45:00,18-Apr-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-108T09:13:00,000T03:19:00,18-Apr-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-108T12:32:00,000T06:45:00,18-Apr-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-108T12:32:00,001T09:48:45,18-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-108T12:32:00,000T19:46:00,18-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-108T19:17:00,000T03:21:00,18-Apr-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-108T19:17:00,000T03:21:00,18-Apr-09,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2009-108T19:17:00,000T13:01:00,18-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-108T23:18:00,000T00:34:00,18-Apr-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-108T23:18:00,000T09:00:00,18-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-109T00:18:00,000T08:00:00,19-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09109_SP,rider,,,,,, 2009-109T08:18:00,000T15:14:45,19-Apr-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-109T08:18:00,000T12:02:45,19-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-109T08:18:00,000T14:02:46,19-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-109T08:18:00,002T02:00:00,19-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-109T09:12:59,000T02:07:46,19-Apr-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp. Map,VIMS ridealong with CIRS. Stare at Titan's night side. Phase = 115 deg. Lat/Lon = 55N/85 deg. Template M4.,,,,,, 2009-109T09:13:42,000T05:07:03,19-Apr-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-109T09:13:42,000T02:07:03,19-Apr-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-109T09:13:42,000T05:07:03,19-Apr-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-109T09:13:42,000T05:07:03,19-Apr-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-109T11:20:45,000T03:00:00,19-Apr-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-109T11:20:45,000T03:00:00,19-Apr-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far-IR Nadir comp.,VIMS ridealong with CIRS. Stare at Titan. Phase = 115 deg. Lat/Lon. = 55N/90 deg. Template N.,,,,,, 2009-109T14:20:45,000T01:00:00,19-Apr-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,NGM (NAC Global Map),global map,,,,,, 2009-109T14:20:45,000T01:00:00,19-Apr-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-109T14:20:45,000T01:00:00,19-Apr-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan; Cloud mapping,VIMS ridealong with ISS. Stare at Titan. Phase = 115 deg. Lat/Lon = 55N/90 deg. Template N.,,,,,, 2009-109T15:20:45,000T04:00:00,19-Apr-09,VIMS,Prime,Titan,GLOBCLOUD,,Night side of Titan,Observation of the night side of Titan at phase angle of 110. Look for clouds and emission features.,,,,,, 2009-109T15:20:45,000T04:00:00,19-Apr-09,CIRS,SPASS Rider,Titan,GLOBCLOUD,,,Ride along with VIMS.,,,,,, 2009-109T15:20:45,000T04:00:00,19-Apr-09,ISS,SPASS Rider,Titan,GLOBCLOUD,,RCI (Ridealong Context Imaging),global map,,,,,, 2009-109T19:20:45,000T02:00:00,19-Apr-09,VIMS,Prime,Titan,REGCLDMAP,,Regional Mapping of Titan,"Regional mapping of Titan. Phase = 115 deg. Lat = 52, Lon = 105",,,,,, 2009-109T19:20:45,000T02:00:00,19-Apr-09,CIRS,SPASS Rider,Titan,REGCLDMAP,,,Ride along with VIMS.,,,,,, 2009-109T19:20:45,000T02:00:00,19-Apr-09,ISS,SPASS Rider,Titan,REGCLDMAP,,RCI (Ridealong Context Imaging),global map,,,,,, 2009-109T20:20:45,000T08:00:00,19-Apr-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T53 flyby,"T53 is another flank-out, post-dusk, high altitude flyby that will be a good complement to T52 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2009-109T21:20:45,000T01:25:00,19-Apr-09,UVIS,Prime,Star,ALPERITI,,Titan Occults Alpha Eri,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2009-109T21:20:45,000T01:25:00,19-Apr-09,CIRS,SPASS Rider,Titan,ALPERITI,,,Ride along with VIMS.,,,,,, 2009-109T21:20:45,000T01:25:00,19-Apr-09,VIMS,SPASS Rider,Titan,LMBMAP,,UVIS Stellar Occ.,VIMS ridealong with UVIS. Stellar Occ of Alpha Eri (Eridanus). Phase = 115 deg. Lat/Lon = 55N/110 deg.,,,,,, 2009-109T22:20:45,000T01:00:00,19-Apr-09,CAPS,SPASS Rider,Titan,T53INBND,,Inbound 109TI (T53),Inbound 109TI (T53),,,,,, 2009-109T22:20:45,000T01:30:00,19-Apr-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-109T22:20:46,000T01:00:00,19-Apr-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-109T22:45:45,000T00:37:10,19-Apr-09,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2009-109T22:45:45,000T01:25:00,19-Apr-09,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-109T22:45:45,000T00:37:10,19-Apr-09,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),global map,,,,,, 2009-109T22:45:45,000T03:35:00,19-Apr-09,RADAR,SPASS Rider,Titan,T53WARMUP,,Warmup for T53 Radiometry,,,,,,, 2009-109T22:45:45,000T00:55:00,19-Apr-09,UVIS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,UVIS Rider to CIRS FIRLMBAER,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-109T22:45:45,000T01:25:00,19-Apr-09,VIMS,SPASS Rider,Titan,FIRLMBMAP,,Titan Limb Map.,VIMS ridealong with CIRS. Phase = 125 deg. Lat/Lon = 50N/130 deg,,,,,, 2009-109T23:20:45,000T02:00:00,19-Apr-09,CAPS,SPASS Rider,Titan,T53CLOSE,,Closest Approach 109TI (T53),Closest Approach 109TI (T53),,,,,, 2009-109T23:20:46,000T02:00:00,19-Apr-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-109T23:22:55,000T00:47:50,19-Apr-09,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2009-109T23:22:55,000T00:47:50,19-Apr-09,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),global map,,,,,, 2009-109T23:32:45,000T00:28:00,19-Apr-09,INMS,Non-SPASS,Titan,TITAN53,,Titan Flyby,Titan observation,,,,,, 2009-109T23:50:45,000T01:00:00,19-Apr-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-110T00:00:45,000T00:40:00,20-Apr-09,INMS,Non-SPASS,Titan,TITAN53,,Titan Flyby,Titan observation,,,,,, 2009-110T00:10:45,000T00:36:00,20-Apr-09,UVIS,Prime,Sun,USUNOCC,Solar occultation,USUN_T53 Solar Occ Titan,This is a solar occultation by Titan. Turn occurs prior to this period; EUV solar occultation port centered on sun Slit aligned tangent to limb. Record data during occultation. Turn back occurs after this period.,,,,,, 2009-110T00:10:45,000T00:36:00,20-Apr-09,VIMS,SPASS Rider,Titan,LMBMAP,,UVIS Stellar Occ.,VIMS ridealong with UVIS. Stellar Occ during C/A. Phase range = 160 -> 100 deg. Lat/Lon at C/A = 7.9S/177 deg. Assuming 80 ms integration time. Scan of 250 lines of 64 pixels each.,,,,,, 2009-110T00:40:45,000T00:28:00,20-Apr-09,INMS,Non-SPASS,Titan,TITAN53,,Titan Flyby,Titan observation,,,,,, 2009-110T00:46:45,000T00:49:00,20-Apr-09,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2009-110T00:46:45,000T00:49:00,20-Apr-09,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-110T00:46:45,000T00:49:00,20-Apr-09,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),global map,,,,,, 2009-110T00:46:45,000T00:49:00,20-Apr-09,VIMS,SPASS Rider,Titan,FIRLMBMAP,,Titan Limb Map.,"VIMS ridealong with CIRS. Phase = 80 deg. Lat/Lon = 55S/250 deg. Time for 4 64x64, 160 ms cubes.",,,,,, 2009-110T00:50:45,000T01:30:00,20-Apr-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-110T00:56:45,000T00:39:00,20-Apr-09,UVIS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,UVIS Rider to CIRS FIRLMBAER,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-110T01:08:45,000T14:21:14,20-Apr-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-110T01:20:45,000T01:00:00,20-Apr-09,CAPS,SPASS Rider,Titan,T53OUTBND,,Outbound 109TI (T53),Outbound 109TI (T53),,,,,, 2009-110T01:20:46,000T01:00:00,20-Apr-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-110T01:35:45,000T00:45:00,20-Apr-09,VIMS,Prime,Titan,HIRES,High resolution image,Titan mosaicking; regional mapping.,"Titan mosaicking / regional mapping. Phase ~75 deg. A cube every 5 min. Phase = 76 deg. Lat = -60, Lon = 255 - New territory at 20 km/pixel",,,,,, 2009-110T01:35:45,000T00:45:00,20-Apr-09,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with VIMS.,,,,,, 2009-110T01:55:45,000T00:25:00,20-Apr-09,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),global map,,,,,, 2009-110T02:20:45,000T04:00:00,20-Apr-09,RADAR,Prime,Titan,T53OUTRAD,,T53 Outbound Radiometry,,,,,,, 2009-110T02:20:45,005T22:09:14,20-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-110T02:20:46,000T20:57:14,20-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-110T04:20:45,001T05:57:15,20-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-110T06:20:45,000T02:30:00,20-Apr-09,VIMS,Prime,Titan,MEDRES,Medium resolution global mapping,Regional Mapping of Titan,"Regional mapping and Titan mosaicks. Three mosaics at 80, 160, and 500 ms, plus one 2x2 mosaic",,,,,, 2009-110T06:20:45,000T02:30:00,20-Apr-09,CIRS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,,Ride along with VIMS.,,,,,, 2009-110T06:20:45,000T02:30:00,20-Apr-09,ISS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-110T08:50:45,000T00:30:00,20-Apr-09,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NGM (NAC Global Map),global map,,,,,, 2009-110T08:50:45,000T00:30:00,20-Apr-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2009-110T08:50:45,000T00:30:00,20-Apr-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global mapping,"VIMS ridealong with ISS. Global mapping of Titan. 6 min dwell times, 80 ms cubes of 64 x 64. Template I. Phase = 70 deg. Lat/Lon = 60S/290 deg.",,,,,, 2009-110T09:20:45,000T05:00:00,20-Apr-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Map of Titan,"Global mapping of Titan. Various cubes of 64x64 at 80, 160, 640 ms. One cube of double res at 160 ms.",,,,,, 2009-110T09:20:45,000T05:00:00,20-Apr-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2009-110T09:20:45,000T05:00:00,20-Apr-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-110T14:20:45,000T08:00:00,20-Apr-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-110T14:20:45,000T08:00:00,20-Apr-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-110T14:20:45,000T08:00:00,20-Apr-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-110T14:20:45,000T08:00:00,20-Apr-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR mapping,VIMS ridealong with CIRS. Global mapping of Titan. Multiple cube sets at various integration times. Template A. Phase = 70 deg. Lat/Lon = 60S/290 deg.,,,,,, 2009-110T15:30:00,000T02:00:00,20-Apr-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-110T17:30:00,000T16:48:00,20-Apr-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-110T23:18:00,000T09:00:00,20-Apr-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-110T23:18:00,000T13:10:26,20-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-110T23:18:00,000T09:00:00,20-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-111T00:18:00,000T08:00:00,21-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09111_SP,rider,,,,,, 2009-111T01:00:00,000T06:00:00,21-Apr-09,RPWS,Non-SPASS,Other,MAGTAIL,MAPS magnetotail observation,MAPS MT Campaign,"Part of MT,lowlat MAPS Campaign. Observe the structure and dynamics of Saturn's magnetotail at low latitudes and moderate distances downstream",,,,,, 2009-111T08:18:00,000T02:00:00,21-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-111T09:18:00,000T01:00:00,21-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09511_SP,rider,,,,,, 2009-111T10:18:00,001T21:45:00,21-Apr-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-111T10:18:00,004T14:15:00,21-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-111T10:18:00,004T14:15:00,21-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-111T10:55:00,000T01:15:00,21-Apr-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 64.3 range 0.7 Mkm",,,,,, 2009-111T10:55:00,000T01:15:00,21-Apr-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-111T10:55:00,000T01:15:00,21-Apr-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-111T12:10:00,000T08:30:00,21-Apr-09,CIRS,Prime,rings(general),TDIFS20HP,,CIRS_109RI_TDIFS20HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-111T12:10:00,000T08:30:00,21-Apr-09,CIRS,SPASS Rider,rings(general),TDIFS20HP,,CIRS_109RI_TDIFS20HP001_SI,,,,,,, 2009-111T12:10:00,000T08:30:00,21-Apr-09,ISS,SPASS Rider,rings(general),TDIFS20HP,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-111T12:10:00,000T08:30:00,21-Apr-09,UVIS,SPASS Rider,rings(general),TDIFS20HP,,URSTAR,,,,,,, 2009-111T12:10:00,000T08:30:00,21-Apr-09,VIMS,SPASS Rider,rings(general),TDIFS20HP,,,null,,,,,, 2009-111T12:28:26,003T17:00:52,21-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-111T20:40:00,000T02:00:00,21-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-111T20:40:00,000T02:00:00,21-Apr-09,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CIRS_109RI_SURVEYPTG002_CAPS,rider,,,,,, 2009-111T23:18:00,000T09:00:00,21-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-112T00:18:00,000T08:00:00,22-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09112_SP,rider,,,,,, 2009-112T08:55:00,000T05:00:00,22-Apr-09,ISS,Prime,rings(general),SPKFMLFHP,,Lit Face High Phase Spoke formation Movie,Spoke Movie to observe formation,,,,,, 2009-112T08:55:00,000T05:00:00,22-Apr-09,CIRS,SPASS Rider,rings(general),SPKFMLFHP,,CIRS_109RI_SPKFMLFHP001_ISS,rider,,,,,, 2009-112T08:55:00,000T05:00:00,22-Apr-09,VIMS,SPASS Rider,rings(general),SPKFMLFHP,,Spoke formation movie,null,,,,,, 2009-112T13:55:00,000T04:00:00,22-Apr-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE",Do 6 at priority 2,,,,,, 2009-112T13:55:00,000T04:00:00,22-Apr-09,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_109RI_LATPHASE111_VIMS,rider,,,,,, 2009-112T13:55:00,000T04:00:00,22-Apr-09,UVIS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,URSTAR,,,,,,, 2009-112T17:55:00,000T03:00:00,22-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-112T17:55:00,000T03:00:00,22-Apr-09,RADAR,SPASS Rider,Other,WU4SMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-112T20:55:00,000T01:30:00,22-Apr-09,RADAR,Prime,Titan,SMIDLCAL,,"Distant Titan Radiometry, South Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-112T23:03:00,000T09:00:00,22-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-113T00:03:00,000T08:00:00,23-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09113_SP,rider,,,,,, 2009-113T08:03:00,001T00:00:00,23-Apr-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-113T08:40:00,000T09:15:00,23-Apr-09,CIRS,Prime,rings(general),VTMPS60MP,,CIRS_109RI_VTMPS60MP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-113T08:40:00,000T09:15:00,23-Apr-09,CIRS,SPASS Rider,rings(general),VTMPS60MP,,CIRS_109RI_VTMPS60MP001_SI,,,,,,, 2009-113T08:40:00,000T09:15:00,23-Apr-09,UVIS,SPASS Rider,rings(general),VTMPS60MP,,URSTAR,,,,,,, 2009-113T08:40:00,000T09:15:00,23-Apr-09,VIMS,SPASS Rider,rings(general),VTMPS60MP,,,null,,,,,, 2009-113T17:55:00,000T00:30:00,23-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-113T17:55:00,000T00:30:00,23-Apr-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_109RI_SATELLORB001_ISS,rider,,,,,, 2009-113T18:25:00,000T04:00:00,23-Apr-09,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"intermediate phase, lit-face ring photometry","intermediate lit #7: B = -59, phase = 90, B' = -1.7",,,,,, 2009-113T18:25:00,000T04:00:00,23-Apr-09,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_109RI_PHOTLIT002_ISS,rider,,,,,, 2009-113T18:25:00,000T04:00:00,23-Apr-09,VIMS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,PhotLit mosaic,Main ring photometry,,,,,, 2009-113T23:03:00,000T09:00:00,23-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-114T00:03:00,000T08:00:00,24-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09114_SP,rider,,,,,, 2009-114T02:19:19,000T00:00:01,24-Apr-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 16.939 Rs, lat = -55 deg, phase = 84 deg",,,,,, 2009-114T08:03:00,001T16:30:00,24-Apr-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-114T08:40:00,000T01:15:00,24-Apr-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 49.6 range 1.2 Mkm",,,,,, 2009-114T08:40:00,000T01:15:00,24-Apr-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-114T08:40:00,000T01:15:00,24-Apr-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-114T09:55:00,000T11:05:00,24-Apr-09,ISS,Prime,RingF,FRSTRCHAN,F ring streamer movie,F RING STREAMER/CHANNEL,"Movie of streamer-channel feature raised in F ring by Prometheus apoapse passage. Need as close to 1 Prom orbital period as possible. Sometimes can be day before or day after. Want 12. 6 of 49 as priority 1, 6 of 49 as priority 2.",,,,,, 2009-114T09:55:00,000T11:05:00,24-Apr-09,CIRS,SPASS Rider,RingF,FRSTRCHAN,F ring streamer movie,CIRS_109RF_FRSTRCHAN001_ISS,rider,,,,,, 2009-114T21:00:00,000T00:33:00,24-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-114T21:00:00,000T00:33:00,24-Apr-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_109RI_SATELLORB004_ISS,rider,,,,,, 2009-114T23:03:00,000T09:00:00,24-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-115T00:03:00,000T08:00:00,25-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09115_SP,rider,,,,,, 2009-115T05:29:18,000T19:03:42,25-Apr-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-115T08:40:00,000T06:15:00,25-Apr-09,CIRS,Prime,rings(general),TMAPS20LP,,CIRS_109RI_TMAPS20LP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-115T08:40:00,000T06:15:00,25-Apr-09,CIRS,SPASS Rider,rings(general),TMAPS20LP,,CIRS_109RI_TMAPS20LP001_SI,,,,,,, 2009-115T08:40:00,000T06:15:00,25-Apr-09,ISS,SPASS Rider,rings(general),TMAPS20LP,,,Spoke periodicity movie. riding along on CIRS TMAP obs.,,,,,, 2009-115T08:40:00,000T06:15:00,25-Apr-09,UVIS,SPASS Rider,rings(general),TMAPS20LP,,URSTAR,,,,,,, 2009-115T08:40:00,000T06:15:00,25-Apr-09,VIMS,SPASS Rider,rings(general),TMAPS20LP,,,null,,,,,, 2009-115T15:33:00,000T09:00:00,25-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-115T16:33:00,000T08:00:00,25-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09515_SP,rider,,,,,, 2009-116T00:30:00,002T13:32:00,26-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-116T00:33:00,002T13:29:00,26-Apr-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-116T00:33:00,002T13:29:00,26-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-116T00:33:00,002T13:29:00,26-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-116T00:33:00,002T13:29:00,26-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-116T01:13:00,000T06:32:00,26-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-116T01:13:00,000T06:32:00,26-Apr-09,CIRS,SPASS Rider,Titan,CLOUD,,Titan Composition,Titan composition,,,,,, 2009-116T01:13:00,000T06:32:00,26-Apr-09,UVIS,SPASS Rider,Titan,CLOUD,,Rider to ISS CLOUD,Rider to ISS CLOUD,,,,,, 2009-116T01:13:00,000T06:32:00,26-Apr-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud monitoring campaign,Titan Surface gap-filling of leading hemisphere.,,,,,, 2009-116T03:00:00,000T02:16:32,26-Apr-09,CAPS,Non-SPASS,Titan,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-116T07:45:00,000T03:45:00,26-Apr-09,ISS,Prime,Rhea,RHEARPXLP,Rhea ring search,Image Rhea's equatorial plane at low phase,Image Rhea's equatorial plane at low phase,,,,,, 2009-116T11:30:00,000T09:52:00,26-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-116T11:30:00,000T09:52:00,26-Apr-09,CIRS,SPASS Rider,Titan,CLOUD,,Titan Composition,Titan composition,,,,,, 2009-116T11:30:00,000T09:52:00,26-Apr-09,UVIS,SPASS Rider,Titan,CLOUD,,Rider to ISS CLOUD,Rider to ISS CLOUD,,,,,, 2009-116T11:30:00,000T09:52:00,26-Apr-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud monitoring campaign,Titan Surface gap-filling of leading hemisphere.,,,,,, 2009-116T21:22:00,000T00:45:00,26-Apr-09,ISS,Prime,Titan,LDHEM,,Titan gap filling (TGF),Cloud monitoring,,,,,, 2009-116T21:22:00,000T00:45:00,26-Apr-09,CIRS,SPASS Rider,Titan,LDHEM,,Titan Composition,Titan composition,,,,,, 2009-116T21:22:00,000T00:45:00,26-Apr-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,Cloud mapping and northern latitude mapping,,,,,, 2009-116T22:47:00,000T09:00:00,26-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-116T23:47:00,000T08:00:00,26-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09116_SP,rider,,,,,, 2009-117T08:27:00,000T15:46:00,27-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-117T08:27:00,000T15:46:00,27-Apr-09,CIRS,SPASS Rider,Titan,CLOUD,,Titan Composition,Titan composition,,,,,, 2009-117T08:27:00,000T15:46:00,27-Apr-09,UVIS,SPASS Rider,Titan,CLOUD,,Rider to ISS CLOUD,Rider to ISS CLOUD,,,,,, 2009-117T08:27:00,000T15:46:00,27-Apr-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,Cloud mapping and northern latitude mapping,,,,,, 2009-117T10:00:00,000T02:16:32,27-Apr-09,CAPS,Non-SPASS,Titan,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-118T00:13:00,000T00:45:00,28-Apr-09,ISS,Prime,Titan,LDHEM,,Titan gap filling (TGF),Cloud monitoring,,,,,, 2009-118T00:13:00,000T00:45:00,28-Apr-09,CIRS,SPASS Rider,Titan,LDHEM,,Titan Composition,Titan composition,,,,,, 2009-118T00:13:00,000T00:45:00,28-Apr-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,Cloud mapping and northern latitude mapping,,,,,, 2009-118T00:58:00,000T01:24:00,28-Apr-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-118T00:58:00,000T01:24:00,28-Apr-09,CIRS,SPASS Rider,Titan,CLOUD,,Titan Composition,Titan composition,,,,,, 2009-118T00:58:00,000T01:24:00,28-Apr-09,UVIS,SPASS Rider,Titan,CLOUD,,Rider to ISS CLOUD,Rider to ISS CLOUD,,,,,, 2009-118T00:58:00,000T01:24:00,28-Apr-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,Cloud mapping and northern latitude mapping,,,,,, 2009-118T02:22:00,000T02:00:00,28-Apr-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-118T05:02:00,000T09:00:00,28-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-118T06:02:00,000T08:00:00,28-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09118_SP,rider,,,,,, 2009-118T14:02:00,000T14:40:00,28-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-118T14:02:00,001T00:00:00,28-Apr-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-118T14:02:00,000T14:40:00,28-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-118T14:02:00,001T01:55:00,28-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-118T14:02:00,003T11:35:00,28-Apr-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-118T14:42:00,000T08:10:00,28-Apr-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_109SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole northern hemisphere",,,,,, 2009-118T22:52:00,000T04:00:00,28-Apr-09,CIRS,Prime,rings(general),TMAPN45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-118T22:52:00,000T04:00:00,28-Apr-09,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_109RI_TMAPN45LP001_SI,,,,,,, 2009-118T22:52:00,000T04:00:00,28-Apr-09,VIMS,SPASS Rider,rings(general),TMAPN45LP,,,null,,,,,, 2009-119T02:52:00,000T00:30:00,29-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-119T03:22:00,000T01:00:00,29-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-119T03:22:00,000T01:00:00,29-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_109RI_MNRNGSHAD012_ISS,rider,,,,,, 2009-119T04:42:00,001T05:15:00,29-Apr-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-119T04:42:00,001T05:15:00,29-Apr-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-119T04:42:00,001T05:15:00,29-Apr-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-119T05:02:00,000T09:00:00,29-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-119T06:02:00,000T08:00:00,29-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09119_SP,rider,,,,,, 2009-119T14:02:00,002T11:36:00,29-Apr-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-119T14:42:00,000T01:15:00,29-Apr-09,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 113.5 range 1.2 Mkm",,,,,, 2009-119T14:42:00,000T01:15:00,29-Apr-09,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-119T14:42:00,000T01:15:00,29-Apr-09,UVIS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-119T15:57:00,000T02:00:00,29-Apr-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-119T15:57:00,000T02:00:00,29-Apr-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-119T15:57:00,000T02:00:00,29-Apr-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-119T17:57:00,000T10:00:00,29-Apr-09,VIMS,Prime,rings(general),LPSPOKE,,"Spoke observation, phase angle 50-70 degrees",Priority 1,,,,,, 2009-119T17:57:00,000T10:00:00,29-Apr-09,CIRS,SPASS Rider,rings(general),LPSPOKE,,CIRS_109RI_LPSPOKE001_VIMS,rider,,,,,, 2009-119T17:57:00,000T10:00:00,29-Apr-09,ISS,SPASS Rider,rings(general),LPSPOKE,,ride along with VIMS to look for spokes.,Spoke Periodicity Movie,,,,,, 2009-119T17:57:00,002T07:41:00,29-Apr-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-120T03:57:00,000T08:00:00,30-Apr-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_109SA_COMPSIT005,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole northern hemisphere",,,,,, 2009-120T09:57:00,003T17:40:00,30-Apr-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-120T09:57:00,001T14:11:00,30-Apr-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-120T11:57:00,000T00:30:00,30-Apr-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 020 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-120T12:27:00,000T01:55:00,30-Apr-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-120T12:27:00,000T01:55:00,30-Apr-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_109RI_MNRNGSHAD014_ISS,rider,,,,,, 2009-120T15:02:00,000T09:00:00,30-Apr-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-120T16:02:00,000T08:00:00,30-Apr-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09120_SP,rider,,,,,, 2009-121T00:42:00,000T03:00:00,1-May-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-121T00:42:00,000T03:00:00,1-May-09,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2009-121T03:42:00,000T02:00:00,1-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-121T05:42:00,000T00:40:00,1-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 023 TH OBS SET IN REV 10","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-121T06:22:00,000T08:00:00,1-May-09,CIRS,Prime,rings(general),VTMPN60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-121T06:22:00,000T08:00:00,1-May-09,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_109RI_VTMPN60MP002_SI,,,,,,, 2009-121T06:22:00,000T08:00:00,1-May-09,VIMS,SPASS Rider,rings(general),VTMPN60MP,,,null,,,,,, 2009-121T15:02:00,000T09:00:00,1-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-121T15:32:00,000T08:00:00,1-May-09,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS Ka-TWTA Maintenance,Ka-TWTA maintenance; Pointing = n/a; No DSN tracking required.,,,,,, 2009-121T16:02:00,000T08:00:00,1-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_109IC_DSCAL09121_SP,rider,,,,,, 2009-122T00:08:00,000T05:00:00,2-May-09,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2009-122T00:42:00,000T05:00:00,2-May-09,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_110_SCATTERED_SUNLIGHT_TEST_PRIME,"Sunlight falling on the CIRS telescope can potentially be scattered into the instrument by mirror imperfections. We need to quantify the effect of ring particle impacts on the mirror performance. This requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; continuous radial scans are required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scans will begin 40 degrees from FPB, and will scan to 10 degrees of FPB at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time VIMS will integrate for TBD seconds and CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction back to the initial position; to determine whether scattering is asymmetric with respect to the FPB axis, 3 such scans will be made. 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from 40 degrees +Z to 10 degrees +Z and back to 40 degrees +Z. 2) From 40 degrees in -X on the X axis, to 10 degrees on the -X axis, to 40 degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 10 degrees -Z and back to 40 degrees -Z.",,,,,, 2009-122T01:37:00,003T05:39:00,2-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo Enter:S,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-122T01:37:00,003T05:39:00,2-May-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-122T01:38:00,000T22:24:00,2-May-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-122T01:38:00,002T07:04:00,2-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-122T01:38:13,000T00:00:01,2-May-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 61.3 deg, r = 23.562 Rs, phase = 96 deg",,,,,, 2009-122T05:08:00,001T22:29:00,2-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-122T05:42:00,000T07:20:00,2-May-09,ISS,Prime,Star,CHARGEXF,Instrument calibration,ISS CCD Charge Transfer Calibration,"Two targets: M48 for NAC, Pleiades for WAC. For each rotate around the Y axis 180 degrees in 20 degree steps and image in three filters at each point. Initial secondary will be Pos Z or Neg Z to sun.",,,,,, 2009-122T13:02:00,000T00:30:00,2-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-122T13:32:00,000T01:29:00,2-May-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_110SK_OPNAV221_NAV,rider,,,,,, 2009-122T15:02:00,000T09:00:00,2-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-122T16:02:00,000T08:00:00,2-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09122_SP,rider,,,,,, 2009-123T00:02:00,000T23:44:00,3-May-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-123T00:42:00,000T08:00:00,3-May-09,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observations of 1 of 3 IR stars: CW Leonis, Eta Carinae, Alpha Orionis. Slew to star; settle; execute small box scan; return to waypoint. Observation of each star to take 6 hours; need not be executed contiguously.",,,,,, 2009-123T08:42:00,000T03:24:00,3-May-09,ISS,Prime,rings(general),SPKFMDFHP,,UnLit Face High Phase Spoke formation Movie,Spoke Movie to observe formation,,,,,, 2009-123T08:42:00,000T03:24:00,3-May-09,CIRS,SPASS Rider,rings(general),SPKFMDFHP,,CIRS_110RI_SPKFMDFHP001_ISS,rider,,,,,, 2009-123T12:06:00,000T02:00:00,3-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-123T14:46:00,000T09:00:00,3-May-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-123T14:46:00,000T09:00:00,3-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-123T15:46:00,000T08:00:00,3-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09123_SP,rider,,,,,, 2009-123T23:46:00,001T07:30:00,3-May-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-124T00:26:00,000T08:16:00,4-May-09,ISS,Prime,rings(general),LRHPENKMV,,"Encke Ringlet Movie, need 2 of 7","Low res, high phase movies of Encke Ringlets; need 2 of 7, widely spaced.",,,,,, 2009-124T00:26:00,000T08:16:00,4-May-09,CIRS,SPASS Rider,rings(general),LRHPENKMV,,CIRS_110RI_LRHPENKMV001_ISS,rider,,,,,, 2009-124T00:26:00,000T08:16:00,4-May-09,VIMS,SPASS Rider,rings(general),LRHPENKMV,,Encke gap high phase movie,null,,,,,, 2009-124T03:37:00,000T07:05:00,4-May-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-124T03:37:00,000T07:05:00,4-May-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-124T03:37:00,000T07:05:00,4-May-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-124T08:42:00,000T02:00:00,4-May-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-124T08:42:00,000T02:00:00,4-May-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-124T10:42:00,000T04:00:00,4-May-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-124T10:42:00,000T04:00:00,4-May-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2009-124T10:42:00,000T20:34:00,4-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-124T10:42:00,000T20:34:00,4-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-124T10:42:00,000T20:34:00,4-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-124T14:42:00,000T06:54:00,4-May-09,ISS,Prime,rings(general),SPKMVDFHP,,UnLit Face High Phase Spoke periodicity Movie,Spoke Movie to observe periodicities,,,,,, 2009-124T14:42:00,000T06:54:00,4-May-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_110RI_SPKMVDFHP002_ISS,rider,,,,,, 2009-124T14:42:00,000T06:54:00,4-May-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",null,,,,,, 2009-124T22:16:00,000T09:00:00,4-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-124T23:16:00,000T08:00:00,4-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09124_SP,rider,,,,,, 2009-125T00:00:00,000T00:34:00,5-May-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-125T07:16:00,000T13:38:16,5-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-125T07:16:00,002T00:00:00,5-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo Enter:S,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-125T07:16:00,000T00:43:00,5-May-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-125T07:16:00,000T11:38:16,5-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-125T07:16:00,000T13:38:16,5-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-125T07:16:00,001T15:00:00,5-May-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-125T07:21:00,000T00:02:00,5-May-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S50 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-125T07:59:00,000T00:07:00,5-May-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-125T08:06:00,000T00:05:00,5-May-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-125T08:11:00,000T00:33:00,5-May-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-125T08:11:47,000T04:42:29,5-May-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-125T08:11:47,000T04:42:29,5-May-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-125T08:11:47,000T04:42:29,5-May-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T08:11:47,000T01:42:29,5-May-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Mid-IR Temp Map,VIMS ridealong with CIRS. Stare at Titan. Obtain various cubes at various integration times. Phase = 115 deg. Lat/Lon = 55N/90 deg. Template M4.,,,,,, 2009-125T08:44:00,000T00:22:59,5-May-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-125T09:06:59,000T12:47:17,5-May-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-125T09:54:16,000T03:00:00,5-May-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far IR Nadir Comp.,VIMS ridealong with CIRS. Stare at Titan. Obtain cubes of 64 x 64 at various integration times. Phase = 115 deg Lat/Lon = 55N/90 deg. Template N.,,,,,, 2009-125T12:54:16,000T01:00:00,5-May-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T12:54:16,000T01:00:00,5-May-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride with ISS,,,,,, 2009-125T12:54:16,000T01:00:00,5-May-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan's nightside,"VIMS ridealong with ISS. Stare at Titan. Obtain cubes of 64 x 64 at various time integrations. Phase = 115 deg, Lat/Lon = 55N/95 deg. Template N",,,,,, 2009-125T13:54:16,000T03:50:00,5-May-09,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-125T13:54:16,000T03:50:00,5-May-09,CIRS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-125T13:54:16,000T03:50:00,5-May-09,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T13:54:16,000T03:50:00,5-May-09,UVIS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,UVIS Rider to CIRS MIRLMBMAP,UVIS Rider to CIRS Mid IR Limb observation,,,,,, 2009-125T13:54:16,000T03:50:00,5-May-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS. Mapping of Titan. Obtain 1 mosaic and 2 x 2 mosaic at various integration times. Phase = 115 deg. Lat/Lon = 55N/100 deg. Template R.,,,,,, 2009-125T17:44:16,000T00:20:00,5-May-09,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_110IC_DSCAL09126_SP,rider,,,,,, 2009-125T18:04:16,000T02:35:00,5-May-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-125T18:04:16,000T02:35:00,5-May-09,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-125T18:04:16,000T02:35:00,5-May-09,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T18:04:16,000T02:35:00,5-May-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Far IR Nadir Comp.,VIMS ridealong with CIRS. Obtain 64 x 64 cubes of 160 ms every 15 min. Phase = 120 deg. Lat/Lon = 50N/115 deg. Template T.,,,,,, 2009-125T18:54:16,000T08:00:00,5-May-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T54 flyby,"T54 is another flank-out, post-dusk, high altitude flyby that will be a good complement to T52 and T53 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2009-125T20:39:16,000T01:00:00,5-May-09,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2009-125T20:39:16,000T01:00:00,5-May-09,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-125T20:39:16,000T01:00:00,5-May-09,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T20:39:16,000T01:00:00,5-May-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan,"VIMS ridealong with CIRS during C/A. At C/A, phase = 146.0, Lat/Lon = 15S/173 deg.",,,,,, 2009-125T20:54:16,000T01:15:00,5-May-09,CAPS,SPASS Rider,Titan,T54INBND,,Inbound 110TI (T54),Inbound 110TI (T54),,,,,, 2009-125T20:54:16,000T01:00:00,5-May-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-125T20:54:16,000T01:30:00,5-May-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-125T21:39:16,000T00:30:00,5-May-09,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2009-125T21:39:16,000T00:30:00,5-May-09,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-125T21:39:16,000T00:30:00,5-May-09,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T21:39:16,000T00:30:00,5-May-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan,"VIMS ridealong with CIRS during C/A. At C/A, phase = 146.0, Lat/Lon = 15S/173 deg.",,,,,, 2009-125T21:54:16,000T02:00:00,5-May-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-125T21:54:16,000T00:40:00,5-May-09,INMS,Non-SPASS,Titan,TITAN54,,Titan Flyby,Titan observation,,,,,, 2009-125T22:09:16,000T00:35:00,5-May-09,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2009-125T22:09:16,000T01:30:00,5-May-09,CAPS,SPASS Rider,Titan,T54CLOSE,,Closest Approach 110TI (T54),Closest Approach 110TI (T54),,,,,, 2009-125T22:09:16,000T00:35:00,5-May-09,CIRS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-125T22:09:16,000T00:35:00,5-May-09,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T22:09:16,000T00:35:00,5-May-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan,"VIMS ridealong with CIRS during C/A. At C/A, phase = 146.0, Lat/Lon = 15S/173 deg.",,,,,, 2009-125T22:24:16,000T01:00:00,5-May-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-125T22:34:16,000T00:40:00,5-May-09,INMS,Non-SPASS,Titan,TITAN54,,Titan Flyby,Titan observation,,,,,, 2009-125T22:44:16,000T00:35:00,5-May-09,CIRS,Prime,Titan,HIRES,High resolution image,,Hi-res closest approach science TBD.,,,,,, 2009-125T22:44:16,000T00:35:00,5-May-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan,"VIMS ridealong with CIRS during C/A. At C/A, phase = 146.0, Lat/Lon = 15S/173 deg.",,,,,, 2009-125T23:14:16,000T00:40:00,5-May-09,INMS,Non-SPASS,Titan,TITAN54,,Titan Flyby,Titan observation,,,,,, 2009-125T23:19:16,000T01:35:00,5-May-09,ISS,Prime,Titan,HIRESNA,,HRN (High Resolution NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-125T23:19:16,000T01:35:00,5-May-09,CIRS,SPASS Rider,Titan,HIRESNA,,,Ride along with UVIS EUV-FUV scan,,,,,, 2009-125T23:19:16,000T01:35:00,5-May-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan,VIMS ridealong with ISS. One cube (64 x 64) obtained every 6 min. Phase = 90 deg. Lat/Lon = 60S/265 deg.,,,,,, 2009-125T23:24:16,000T01:30:00,5-May-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-125T23:39:16,000T01:15:00,5-May-09,CAPS,SPASS Rider,Titan,T54OUTBND,,Outbound 110TI (T54),Outbound 110TI (T54),,,,,, 2009-125T23:54:16,000T01:00:00,5-May-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-125T23:54:16,000T07:50:44,5-May-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-126T00:54:16,000T07:00:00,6-May-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-126T00:54:16,000T07:00:00,6-May-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS EUV-FUV scan,,,,,, 2009-126T00:54:16,000T07:00:00,6-May-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-126T00:54:16,000T07:00:00,6-May-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,VIMS ridealong with UVIS. Slow scan across Titan. Phase = 67 deg. Lat/Lon = 55S/290 deg. Template X.,,,,,, 2009-126T00:54:16,008T05:07:44,6-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-126T00:54:16,001T21:00:13,6-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-126T02:54:16,001T04:21:44,6-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-126T07:45:00,000T02:00:00,6-May-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-126T07:54:16,000T05:00:00,6-May-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-126T07:54:16,000T05:00:00,6-May-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-126T07:54:16,000T05:00:00,6-May-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-126T07:54:16,000T05:00:00,6-May-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-126T07:54:16,000T05:00:00,6-May-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,VIMS ridealong with CIRS. Stare at Titan. Obtain various cubes at various integration times. Phase = 60 deg. Lat/Lon = 55S/310. Template C.,,,,,, 2009-126T09:45:00,000T21:31:00,6-May-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-126T12:54:16,000T08:27:00,6-May-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Map,"Global Map of Titan. Cubes of 32x32, 48x48, 64x64 at 80,160,640 ms and repeated at double res. Template B. Phase = 60 deg, Lat/Lon = -55/310 deg.",,,,,, 2009-126T12:54:16,000T08:27:00,6-May-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2009-126T12:54:16,000T08:27:00,6-May-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-126T22:16:00,010T15:28:00,6-May-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-126T22:16:00,000T09:00:00,6-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-126T23:16:00,000T08:00:00,6-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09126_SP,rider,,,,,, 2009-127T07:16:00,010T06:28:00,7-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo Enter:S,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-127T07:16:00,001T23:45:00,7-May-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-127T07:16:00,000T04:14:00,7-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-127T07:56:00,000T03:34:00,7-May-09,ISS,Prime,Titan,ECLIPSE0,,Titan NAC Photopol 90 Phase,Long exposures to search for auroras and lightning on Titan in eclipse. This is one of several possible events but it is one of the best because of proximity to Titan.,,,,,, 2009-127T07:56:00,000T03:33:59,7-May-09,UVIS,SPASS Rider,Titan,ECLIPSE,,Rider to ISS ECLIPSE,Rider to ISS TI_ECLIPSE - to look for emissions from electron/ion impact during eclipse when sunlight is absent,,,,,, 2009-127T11:30:00,000T06:45:00,7-May-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-127T18:15:00,000T03:06:00,7-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-127T18:15:00,006T11:47:00,7-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-127T21:54:29,002T13:56:43,7-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-127T22:01:00,000T09:00:00,7-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-127T23:01:00,000T08:00:00,7-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09127_SP,rider,,,,,, 2009-128T07:41:00,000T01:15:00,8-May-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 53.3 range 1 Mkm",,,,,, 2009-128T07:41:00,000T01:15:00,8-May-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-128T07:41:00,000T01:15:00,8-May-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-128T08:56:00,000T02:55:00,8-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-128T11:51:00,000T08:00:00,8-May-09,CIRS,Prime,rings(general),VTMPS60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-128T11:51:00,000T08:00:00,8-May-09,CIRS,SPASS Rider,rings(general),VTMPS60MP,,CIRS_110RI_VTMPS60MP001_SI,,,,,,, 2009-128T16:51:00,000T03:00:00,8-May-09,RADAR,SPASS Rider,Other,WU4SMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-128T19:51:00,000T01:30:00,8-May-09,RADAR,Prime,Titan,SMIDLCAL,,"Distant Titan Radiometry, South Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-128T22:01:00,000T09:00:00,8-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-128T23:01:00,000T08:00:00,8-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09128_SP,rider,,,,,, 2009-129T07:01:00,001T00:00:00,9-May-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-129T07:41:00,000T01:15:00,9-May-09,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 44.6 range 1.2 Mkm",,,,,, 2009-129T07:41:00,000T01:15:00,9-May-09,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-129T07:41:00,000T01:15:00,9-May-09,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-129T08:56:00,000T00:52:00,9-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-129T08:56:00,000T00:52:00,9-May-09,CIRS,SPASS Rider,InstrumentCalibration,SATELLORB,Satellite orbit campaign,CIRS_110OT_SATELLORB002_ISS,rider,,,,,, 2009-129T09:48:00,000T08:54:00,9-May-09,VIMS,Prime,rings(general),ALPAUROCC,Alpha Aur occultation,Ring stellar occ - alpAur,"B ring, region 1",,,,,, 2009-129T09:48:00,000T08:54:00,9-May-09,CIRS,SPASS Rider,rings(general),ALPAUROCC,Alpha Aur occultation,CIRS_110RI_ALPAUROCC101_VIMS,rider,,,,,, 2009-129T14:38:36,000T00:00:01,9-May-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 15.068 Rs, lat = -54 deg, phase = 84 deg",,,,,, 2009-129T18:42:00,000T02:00:00,9-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-129T20:42:00,000T00:39:00,9-May-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-129T20:42:00,000T00:39:00,9-May-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_110RI_MNRNGSHAD009_ISS,rider,,,,,, 2009-129T22:01:00,000T09:00:00,9-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-129T23:01:00,000T08:00:00,9-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09129_SP,rider,,,,,, 2009-130T00:00:00,002T00:00:00,10-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-130T07:01:00,004T05:59:00,10-May-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-130T07:41:00,000T01:15:00,10-May-09,ISS,Prime,Titan,M60R2CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 35 range 1.2 Mkm",,,,,, 2009-130T07:41:00,000T01:15:00,10-May-09,CIRS,SPASS Rider,Titan,M60R2CLDF,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-130T07:41:00,000T01:15:00,10-May-09,UVIS,SPASS Rider,Titan,M60R2CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-130T08:56:00,000T11:05:00,10-May-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-130T08:56:00,000T11:05:00,10-May-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,CIRS_110RF_FMOVIE002_ISS,rider,,,,,, 2009-130T08:56:00,000T11:05:00,10-May-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,Priority 1,,,,,, 2009-130T11:51:12,002T09:18:17,10-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-130T20:01:00,000T00:30:00,10-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-130T20:31:00,000T01:29:00,10-May-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_110SK_OPNAV301_NAV,rider,,,,,, 2009-130T22:01:00,000T09:00:00,10-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-130T23:01:00,000T08:00:00,10-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09130_SP,rider,,,,,, 2009-131T07:01:00,000T09:10:00,11-May-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-131T07:41:00,000T09:25:00,11-May-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_110SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole northern hemisphere",,,,,, 2009-131T16:06:00,000T03:00:00,11-May-09,RADAR,SPASS Rider,Other,WU4NEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-131T16:07:20,000T00:00:01,11-May-09,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2009-131T17:06:00,000T02:00:00,11-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-131T19:06:00,000T01:30:00,11-May-09,RADAR,Prime,Titan,NEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-131T20:36:00,000T00:30:00,11-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-131T21:46:00,000T09:00:00,11-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-131T22:46:00,000T08:00:00,11-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09131_SP,rider,,,,,, 2009-132T07:26:00,000T02:00:00,12-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-132T09:26:00,000T03:39:00,12-May-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-132T09:26:00,000T03:39:00,12-May-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_110RI_MNRNGSHAD011_ISS,rider,,,,,, 2009-132T13:05:00,000T08:00:00,12-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 1. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Repeat PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-132T21:09:29,001T08:52:31,12-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-132T21:45:00,000T09:00:00,12-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-132T22:45:00,000T08:00:00,12-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09132_SP,rider,,,,,, 2009-133T07:09:00,000T01:31:00,13-May-09,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 81 range 1.1 Mkm",,,,,, 2009-133T07:25:00,000T01:15:00,13-May-09,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-133T07:25:00,000T01:15:00,13-May-09,UVIS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-133T08:40:00,000T02:38:00,13-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-133T11:18:00,000T00:30:00,13-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-133T11:48:00,000T01:23:00,13-May-09,ISS,Prime,Mimas,ENMNSHAD,,Enceladus's shadow on Mimas,Photo op of Enceladus's shadow on Mimas,,,,,, 2009-133T13:11:00,000T05:34:00,13-May-09,CIRS,Prime,rings(general),TMAPN45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-133T13:11:00,000T05:34:00,13-May-09,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_110RI_TMAPN45LP001_SI,,,,,,, 2009-133T18:45:00,000T08:00:00,13-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 2. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Repeat PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-134T02:45:00,000T01:14:00,14-May-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_110SK_OPNAV341_NAV,rider,,,,,, 2009-134T04:00:00,000T09:00:00,14-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-134T05:00:00,000T08:00:00,14-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09134_SP,rider,,,,,, 2009-134T06:02:00,001T07:40:00,14-May-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-134T06:02:00,001T07:40:00,14-May-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-134T06:02:00,001T07:40:00,14-May-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-134T06:02:00,001T07:40:00,14-May-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-134T13:00:00,000T23:45:00,14-May-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-134T13:40:00,000T00:30:00,14-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 018 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-134T14:10:00,000T04:55:00,14-May-09,ISS,Prime,Star,CALSTAR1,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2009-134T19:05:00,000T08:00:00,14-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 3. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Repeat PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-135T03:45:00,000T09:00:00,15-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-135T04:45:00,000T08:00:00,15-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09135_SP,rider,,,,,, 2009-135T12:45:00,000T23:05:00,15-May-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-135T13:25:00,000T07:55:00,15-May-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_110SA_COMPSIT005,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole northern hemisphere",,,,,, 2009-135T13:42:00,000T16:40:00,15-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-135T13:42:00,000T16:40:00,15-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-135T13:42:00,000T16:40:00,15-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-135T21:20:00,000T16:00:00,15-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 5. One 16.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Slew -500.0 mrad about z-axis. Start data capture, stare 125.0 s, stop data capture. Repeat PATTERN 250 times. PATTERN: Slew +4.0 mrad about z-axis. Start data capture, stare 125.0 s, stop data capture.",,,,,, 2009-136T06:22:00,002T14:45:00,16-May-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-136T06:22:00,001T07:23:00,16-May-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-136T06:22:00,002T14:45:00,16-May-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-136T06:22:00,001T07:22:00,16-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-136T11:50:00,000T00:34:00,16-May-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-136T12:24:00,000T01:36:00,16-May-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-136T14:00:00,000T22:45:00,16-May-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-136T14:00:00,000T09:00:00,16-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-136T15:00:00,000T08:00:00,16-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_110IC_DSCAL09136_SP,rider,,,,,, 2009-136T23:40:00,000T12:00:00,16-May-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning N. hemisphere + pole, may be split in half by downlink",,,,,, 2009-137T11:40:00,000T01:40:00,17-May-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-137T13:44:00,003T16:30:00,17-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo Enter:S,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-137T13:44:00,006T01:40:00,17-May-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-137T13:44:00,001T07:23:00,17-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-137T13:45:00,001T07:22:00,17-May-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-137T13:45:00,001T09:00:00,17-May-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-137T13:45:28,000T00:00:01,17-May-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 15.9 d, inc = 60.6 deg, r = 25.434 Rs, phase = 96 deg",,,,,, 2009-137T14:00:00,000T09:00:00,17-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-137T15:00:00,000T08:00:00,17-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09137_SP,rider,,,,,, 2009-137T23:40:00,000T04:35:00,17-May-09,ISS,Prime,Star,CALSTAR1,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2009-138T04:15:00,000T08:00:00,18-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 7. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Repeat PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-138T12:15:00,000T01:29:00,18-May-09,CIRS,SPASS Rider,InstrumentCalibration,OPNAV,Optical navigation image,CIRS_111SK_OPNAV381_NAV,rider,,,,,, 2009-138T13:45:00,000T09:00:00,18-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-138T21:07:00,001T01:05:00,18-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-138T21:07:00,001T01:05:00,18-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-138T21:07:00,001T01:05:00,18-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-138T22:45:00,000T23:59:00,18-May-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-138T23:25:00,000T00:30:00,18-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-138T23:55:00,000T05:09:00,18-May-09,ISS,Prime,Star,CALSTAR1,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2009-139T05:04:00,000T08:00:00,19-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 8. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. UV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Repeat PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-139T13:04:00,000T09:07:00,19-May-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-139T13:44:00,000T09:00:00,19-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-139T14:44:00,000T08:00:00,19-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09139_SP,rider,,,,,, 2009-139T22:12:00,000T10:50:00,19-May-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-139T22:12:00,000T10:50:00,19-May-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-139T22:12:00,000T07:37:00,19-May-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-139T22:12:00,000T10:50:00,19-May-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-139T22:44:00,001T07:30:00,19-May-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-139T23:24:00,000T06:25:00,19-May-09,CIRS,Prime,rings(general),TDIFN20HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-139T23:24:00,000T06:25:00,19-May-09,CIRS,SPASS Rider,rings(general),TDIFN20HP,,CIRS_111RI_TDIFN20HP001_SI,,,,,,, 2009-140T05:49:00,000T06:45:00,20-May-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-140T09:02:00,001T10:39:41,20-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-140T09:02:00,000T21:12:00,20-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-140T12:34:00,000T08:00:00,20-May-09,UVIS,Prime,Saturn,MOS110APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 9. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Repeat PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-140T12:34:00,000T07:26:00,20-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-140T20:00:00,000T10:14:00,20-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-140T21:14:00,000T09:00:00,20-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-140T22:14:00,000T08:00:00,20-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09140_SP,rider,,,,,, 2009-141T06:14:00,001T14:45:00,21-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo Enter:S,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-141T06:14:00,000T14:12:41,21-May-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-141T06:14:00,000T10:12:41,21-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-141T06:14:00,000T14:12:42,21-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-141T07:09:49,000T01:16:52,21-May-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-141T07:09:49,000T01:16:52,21-May-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-141T07:09:49,000T01:16:52,21-May-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-141T07:09:49,000T01:16:52,21-May-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. 48x48 cubes of 160 ms. Phase 123 deg, Lat/Lon = 53 N/100 deg.",,,,,, 2009-141T08:26:41,000T04:00:00,21-May-09,VIMS,Prime,Titan,CLOUDMAP,Cloud map,Cloud Mapping,Stare at Titan for cloud mapping. Obtain 64 x 64 cubes at various integration times. Phase = 125 deg. Lat/Lon = 55N/105 deg. Template O .,,,,,, 2009-141T08:26:41,000T04:00:00,21-May-09,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride along with VIMS.,,,,,, 2009-141T08:26:41,000T04:00:00,21-May-09,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-141T12:26:41,000T06:30:00,21-May-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-141T12:26:41,000T06:30:00,21-May-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with VIMS.,,,,,, 2009-141T12:26:41,000T06:30:00,21-May-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-141T12:26:41,000T06:30:00,21-May-09,RADAR,SPASS Rider,Titan,T55WARMUP,,Warmup for T55,,,,,,, 2009-141T12:26:41,000T06:30:00,21-May-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS Slow scan across Titan. Phase 125 deg, Lat/Lon = 50 N/123 deg.",,,,,, 2009-141T16:26:41,000T10:00:00,21-May-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T55 flyby,"T55 is another flank-out, post-dusk flyby, with a minimum altitude of 1000 km. Therefore, the measurements will provide a description of the draping and the pileup of the external magnetic field around Titan on the nightside hemisphere. It will be also a good complement to T52, T53 and T54 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-141T18:56:41,000T01:18:00,21-May-09,RADAR,Prime,Titan,T55INSCAT,,T55 Inbound Scatterometry,,,,,,, 2009-141T19:26:41,000T01:30:00,21-May-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-141T19:41:41,000T01:00:00,21-May-09,CAPS,SPASS Rider,Titan,T55INBND,,Inbound 111TI (T55),Inbound 111TI (T55),,,,,, 2009-141T20:15:41,000T00:41:00,21-May-09,RADAR,Prime,Titan,T55IHISAR,,T55 Inbound HiSAR,,,,,,, 2009-141T20:26:41,000T00:40:00,21-May-09,INMS,Non-SPASS,Titan,TITAN55,,Titan Flyby,Titan observation,,,,,, 2009-141T20:26:42,000T01:00:00,21-May-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-141T20:41:41,000T01:30:00,21-May-09,CAPS,SPASS Rider,Titan,T55CLOSE,,Closest Approach 111TI (T55),Closest Approach 111TI (T55),,,,,, 2009-141T20:56:41,000T00:12:00,21-May-09,RADAR,Prime,Titan,T55INALT,,T55 Inbound Altimetry,,,,,,, 2009-141T20:56:41,000T01:00:00,21-May-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-141T21:06:41,000T00:40:00,21-May-09,INMS,Non-SPASS,Titan,TITAN55,,Titan Flyby,Titan observation,,,,,, 2009-141T21:08:41,000T00:36:00,21-May-09,RADAR,Prime,Titan,T55INOSAR,,T55 Inbound and Outbound SAR,,,,,,, 2009-141T21:26:42,000T02:00:00,21-May-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-141T21:44:41,000T00:12:00,21-May-09,RADAR,Prime,Titan,T55OUTALT,,T55 Outbound Altimetry,,,,,,, 2009-141T21:46:41,000T00:40:00,21-May-09,INMS,Non-SPASS,Titan,TITAN55,,Titan Flyby,Titan observation,,,,,, 2009-141T21:56:41,000T00:20:00,21-May-09,RADAR,Prime,Titan,T55OHISAR,,T55 outbound HiSAR,,,,,,, 2009-141T21:56:41,000T01:30:00,21-May-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-141T22:11:41,000T00:30:00,21-May-09,CAPS,SPASS Rider,Titan,T55OUTBND,,Outbound 111TI (T55),Outbound 111TI (T55),,,,,, 2009-141T22:26:41,000T03:33:18,21-May-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-141T22:38:22,000T01:18:19,21-May-09,RADAR,Prime,Titan,T55OUTSCT,,T55 Outbound Scatterometry,,,,,,, 2009-141T22:41:41,006T18:30:18,21-May-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-141T23:26:42,000T01:00:00,21-May-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-141T23:56:41,000T02:30:00,21-May-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_111TI_FIRNADMAP002,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-141T23:56:41,000T02:30:00,21-May-09,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-141T23:56:41,000T02:30:00,21-May-09,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-141T23:56:41,000T02:30:00,21-May-09,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan Scan,"VIMS ridealong with CIRS. Stare at Titan. Mosaic of 64x64, 160ms cubes. Phase 55 deg, Lat/Lon = 50S/305 deg.",,,,,, 2009-142T00:26:42,000T20:32:18,22-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-142T02:00:00,000T02:00:00,22-May-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-142T02:26:41,000T04:00:00,22-May-09,CIRS,Prime,Titan,MIRLMPAIR,,,"Integrate on Titan's limb with arrays parallel to limb, paired detector mode, to maximize S/N for detection and characterization of of trace gas species and isotopes.",,,,,, 2009-142T02:26:41,000T04:00:00,22-May-09,CIRS,SPASS Rider,Titan,MIRLMPAIR,,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-142T02:26:41,000T04:00:00,22-May-09,ISS,SPASS Rider,Titan,MIRLMPAIR,,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-142T02:26:41,000T04:00:00,22-May-09,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-142T02:26:41,000T04:00:00,22-May-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,"VIMS ridealong with CIRS. Stare at Titan. 64x64 cubes at 80ms, 2x2 mosaics at 80, 160, 500 ms. Phase = 53 deg, Lat/Lon = 50S/310 deg.",,,,,, 2009-142T02:26:41,001T05:32:19,22-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-142T04:00:00,001T03:59:00,22-May-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-142T06:26:41,000T03:00:00,22-May-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-142T06:26:41,000T03:00:00,22-May-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-142T06:26:41,000T03:00:00,22-May-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-142T06:26:41,000T03:00:00,22-May-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-142T06:26:41,000T03:00:00,22-May-09,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. Obtain 64 x 64 cubes at various exposure times. Phase 53 deg, Lat/Lon = 50S/315 deg.",,,,,, 2009-142T09:26:41,000T02:00:00,22-May-09,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,WPH (WAC Photometry),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-142T09:26:41,000T02:00:00,22-May-09,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Ride along with VIMS.,,,,,, 2009-142T09:26:41,000T02:00:00,22-May-09,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,Stare at Titan,"VIMS ridealong with ISS. Stare at Titan. Continue cubes of 64 x 64 at various exposure times. Phase 50 deg, Lat/Lon = 50S/320 deg.",,,,,, 2009-142T11:26:41,000T08:00:00,22-May-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-142T11:26:41,000T08:00:00,22-May-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (9 integrations total = 18 frames, 0.5 Mb/frame)",,,,,, 2009-142T11:26:41,000T08:00:00,22-May-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-142T11:26:41,000T08:00:00,22-May-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Cloud Mapping,"VIMS ridealong with CIRS. Stare at Titan. Cubes of 32x32, 48x48, 64x64 at various exp times. Phase 50 deg, Lat/Lon = 50S/ 325 deg.",,,,,, 2009-142T20:59:00,003T09:00:00,22-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter:SApo Enter:SApo Enter:S,Range enter= 13.633064 Rs exit= 14.180071 Range altitude= -40620.059 km ... -40114.459,,,,,, 2009-142T20:59:00,000T10:28:04,22-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-142T20:59:00,000T09:00:00,22-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-142T21:59:00,000T08:00:00,22-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09142_SP,rider,,,,,, 2009-143T05:59:00,000T02:00:00,23-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-143T06:59:00,000T01:00:00,23-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09143_SP,rider,,,,,, 2009-143T07:27:04,002T05:43:28,23-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-143T07:59:00,001T22:00:00,23-May-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-143T07:59:00,005T09:13:00,23-May-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-143T08:39:00,000T01:15:00,23-May-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 48.3 range 0.7 Mkm",,,,,, 2009-143T08:39:00,000T01:15:00,23-May-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-143T08:39:00,000T01:15:00,23-May-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-143T09:54:00,000T04:00:00,23-May-09,VIMS,Prime,rings(general),LATPHASE,Latitude phase coverage,"Mid-phase, high elevation LATPHASE",Do 6 at priority 2,,,,,, 2009-143T09:54:00,000T04:00:00,23-May-09,CIRS,SPASS Rider,rings(general),LATPHASE,Latitude phase coverage,CIRS_110RI_LATPHASE_VIMS,rider,,,,,, 2009-143T13:54:00,000T04:00:00,23-May-09,CIRS,Prime,rings(general),TDIFS45HP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-143T13:54:00,000T04:00:00,23-May-09,CIRS,SPASS Rider,rings(general),TDIFS45HP,,CIRS_111RI_TDIFS45HP001_SI,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-143T15:24:00,002T20:02:00,23-May-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-143T17:54:00,000T02:25:00,23-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-143T20:59:00,000T09:00:00,23-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-143T21:59:00,000T08:00:00,23-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09543_SP,rider,,,,,, 2009-144T06:39:00,000T03:00:00,24-May-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-144T06:39:00,000T03:00:00,24-May-09,RADAR,SPASS Rider,Other,WU4SMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-144T09:39:00,000T01:30:00,24-May-09,RADAR,Prime,Titan,SMIDLCAL,,"Distant Titan Radiometry, South Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-144T11:09:00,000T07:49:00,24-May-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_111SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2009-144T20:59:00,000T09:00:00,24-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-144T21:59:00,000T08:00:00,24-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09144_SP,rider,,,,,, 2009-145T01:24:48,000T00:00:01,25-May-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 12.164 Rs, lat = -50 deg, phase = 80 deg",,,,,, 2009-145T05:59:00,001T00:00:00,25-May-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-145T06:39:00,000T01:15:00,25-May-09,ISS,Prime,Titan,M30R2CLDF,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 25.5 range 1.3 Mkm",,,,,, 2009-145T06:39:00,000T01:15:00,25-May-09,CIRS,SPASS Rider,Titan,M30R2CLDF,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-145T06:39:00,000T01:15:00,25-May-09,UVIS,SPASS Rider,Titan,M30R2CLDF,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-145T07:54:00,000T04:00:00,25-May-09,CIRS,Prime,rings(general),TMAPS45MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-145T07:54:00,000T04:00:00,25-May-09,CIRS,SPASS Rider,rings(general),TMAPS45MP,,CIRS_111RI_TMAPS45MP001_SI,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-145T11:54:00,000T06:25:00,25-May-09,ISS,Prime,rings(general),RETARMRLP,,Medium res retargetables,Medium Res Retarg of small ring region satellites. Need 25 of 54.,,,,,, 2009-145T13:10:32,001T19:47:29,25-May-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-145T20:59:00,000T09:00:00,25-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-145T21:59:00,000T08:00:00,25-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09145_SP,rider,,,,,, 2009-146T05:59:00,000T02:21:00,26-May-09,CDA,Prime,DustRAM direction,RPX0040,,CDA RPXing 2009-146T07:00:59 MH,"RPXing at 14.408821 Rs, large ring extention, small/medium inclination",,,,,, 2009-146T05:59:00,000T02:48:59,26-May-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 14.184244 Rs exit= 14.643974 Range altitude= -39378.054 km ... 39484.635,,,,,, 2009-146T05:59:00,004T05:59:00,26-May-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-146T08:47:59,004T03:10:01,26-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.648384 Rs exit= 10.959694 Range altitude= 40221.093 km ... -40233.432,,,,,, 2009-146T09:00:00,000T07:44:00,26-May-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-146T09:00:00,000T07:44:00,26-May-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,Priority 1,,,,,, 2009-146T11:26:00,006T13:18:00,26-May-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-146T16:44:00,000T02:30:00,26-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-146T20:44:00,000T09:00:00,26-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-146T21:44:00,000T08:00:00,26-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09146_SP,rider,,,,,, 2009-147T00:00:00,001T00:00:00,27-May-09,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2009-147T06:43:00,000T02:15:00,27-May-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-147T08:58:00,000T08:00:00,27-May-09,UVIS,Prime,Saturn,MOS111APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 1. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Step out to ~10.0 Rs by repeating PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-147T08:58:01,001T08:13:59,27-May-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-147T16:58:00,000T00:31:00,27-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-147T17:29:00,000T02:34:00,27-May-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-147T20:43:00,000T09:00:00,27-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-147T21:43:00,000T08:00:00,27-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09147_SP,rider,,,,,, 2009-148T06:23:00,000T01:15:00,28-May-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 72.6 range 1.6 Mkm",,,,,, 2009-148T06:23:00,000T01:15:00,28-May-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-148T06:23:00,000T01:15:00,28-May-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-148T07:38:00,000T09:30:00,28-May-09,CIRS,Prime,rings(general),TMAPN45LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-148T07:38:00,000T09:30:00,28-May-09,CIRS,SPASS Rider,rings(general),TMAPN45LP,,CIRS_111RI_TMAPN45LP001_SI,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-148T17:08:00,000T02:55:00,28-May-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-148T17:12:00,001T06:40:00,28-May-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-148T17:12:00,001T06:40:00,28-May-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-148T17:12:00,000T12:32:00,28-May-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-148T17:12:00,000T12:31:00,28-May-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-148T20:43:00,000T09:00:00,28-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-148T21:43:00,000T08:00:00,28-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09148_SP,rider,,,,,, 2009-149T05:43:00,000T18:09:00,29-May-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-149T05:44:00,000T13:48:00,29-May-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-149T06:23:00,000T00:30:00,29-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-149T06:53:00,000T16:00:00,29-May-09,UVIS,Prime,Saturn,MOS111APO,,,"Note: This description treats UVIS_111SA_MOS111APO002_PRIME and UVIS_111SA_MOS111APO003_PRIME as a single 16.0-hour block of observation time. Note: As no data will be collected while Cassini is slewing, actual data volume = (8072.05675 bps, from Alain Jouchoux's spreadsheet)x(150.0 s per stare)x(222 stares) = 268.80x10^6 bits Mosaic scan of Saturn magnetosphere, day 2. One 16.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Slew -444 mrad about z-axis (to -10.0 Rs from Saturn center). Start data capture, stare 150.0 s, stop data capture. Step to +10.0 Rs from Saturn center by repeating PATTERN 221 times. PATTERN: Slew +4.0 mrad about z-axis. Start data capture, stare 150.0 s, stop data capture.",,,,,, 2009-149T19:32:00,000T04:20:00,29-May-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15 Data rate 0 bps, overlaps MAGBOUND request",,,,,, 2009-149T19:32:00,000T16:26:00,29-May-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-149T22:53:00,000T03:25:00,29-May-09,CIRS,Prime,rings(general),SATREFL,,CIRS_111RI_SATREFL149_PRIME;,null,,,,,, 2009-149T22:53:00,000T03:25:00,29-May-09,CIRS,SPASS Rider,rings(general),SATREFL,,CIRS_111RI_SATREFL149_SI,null,,,,,, 2009-149T23:52:00,000T12:06:00,29-May-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-149T23:52:00,003T00:53:00,29-May-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-149T23:52:00,000T03:06:00,29-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-150T02:58:00,000T09:00:00,30-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-150T03:58:00,000T08:00:00,30-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09150_SP,rider,,,,,, 2009-150T04:00:00,000T01:00:00,30-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-150T11:58:00,005T17:54:00,30-May-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-150T11:58:00,002T12:46:00,30-May-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.648384 Rs exit= 10.959694 Range altitude= 40221.093 km ... -40233.432,,,,,, 2009-150T11:58:00,001T10:00:00,30-May-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-150T11:58:00,004T18:24:00,30-May-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-150T11:58:00,001T01:00:00,30-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-150T12:38:00,000T00:36:00,30-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-150T13:14:00,000T04:34:00,30-May-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-150T17:48:00,000T16:00:00,30-May-09,UVIS,Prime,Saturn,MOS111APO,,,"Note: This description treats UVIS_111SA_MOS111APO004_PRIME and UVIS_111SA_MOS111APO005_PRIME as a single 16.0-hour block of observation time. Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.63224 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(242 stares) = 293.02x10^6 bits Mosaic scan of Saturn magnetosphere, day 2. One 16.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Slew -364 mrad about z-axis (to approx. -10.0 Rs from Saturn center). Start data capture, stare 140.0 s, stop data capture. Step to +10.0 Rs from Saturn center by repeating PATTERN 241 times. PATTERN: Slew +3.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-151T09:48:00,000T00:30:00,31-May-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 017 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-151T10:18:00,000T02:00:00,31-May-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-151T12:58:00,000T09:00:00,31-May-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-151T13:58:00,000T08:00:00,31-May-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_111IC_DSCAL09151_SP,rider,,,,,, 2009-151T14:00:00,000T01:00:00,31-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-151T21:58:00,000T14:02:00,31-May-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-151T21:58:00,000T15:00:00,31-May-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-151T22:38:00,000T02:46:00,31-May-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-152T01:24:00,000T08:00:00,1-Jun-09,UVIS,Prime,Saturn,MOS111APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 4. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Step out to ~10.0 Rs by repeating PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-152T09:24:00,000T01:15:00,1-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-152T10:39:00,000T01:39:00,1-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-152T12:00:00,000T02:00:00,1-Jun-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-152T12:58:00,000T09:00:00,1-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-152T14:00:00,000T10:45:00,1-Jun-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-152T15:00:00,000T01:00:00,1-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-152T20:00:00,000T01:00:00,1-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-152T21:58:00,000T02:46:00,1-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-152T23:13:00,000T00:50:00,1-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 021 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-153T00:03:00,000T08:00:00,2-Jun-09,UVIS,Prime,Saturn,MOS111APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 5. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Step out to ~10.0 Rs by repeating PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-153T00:44:00,003T19:28:00,2-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.648384 Rs exit= 10.959694 Range altitude= 40221.093 km ... -40233.432,,,,,, 2009-153T00:44:00,004T04:28:00,2-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-153T00:44:00,000T12:14:00,2-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-153T00:45:00,002T22:21:00,2-Jun-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-153T00:45:00,001T20:57:00,2-Jun-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-153T00:45:08,000T00:00:01,2-Jun-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 58.7 deg, r = 28.339 Rs, phase = 100 deg",,,,,, 2009-153T06:03:00,000T09:55:00,2-Jun-09,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours of downlink required to be tracked at DSS-55 in 1-way mode. 3-hr USO instead of usual 4-hr USO (to give NAV more 2-way data since OTM-199 is the day after).,,,,,, 2009-153T08:03:00,000T04:15:00,2-Jun-09,ISS,Prime,Star,CALSTAR2,Stellar Calibration,ISS Photometric Calibration Star 2,Photometric Calibration Star 2 (77/78 Tau),,,,,, 2009-153T12:53:00,000T09:05:00,2-Jun-09,RSS,SPASS Rider,Titan,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T57 Rev113 Titan occultation experiment on 2009/173.",,,,,, 2009-153T12:58:00,000T09:00:00,2-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-153T14:00:00,000T01:00:00,2-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-153T19:45:00,000T00:45:00,2-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-153T21:58:00,000T14:44:00,2-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-153T22:38:00,000T02:00:00,2-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-154T00:38:00,000T10:34:00,3-Jun-09,ISS,Prime,Other,KIVIUQ,,Kiviuq rotation light curve,Kiviuq rotation light curve,,,,,, 2009-154T12:42:00,000T09:00:00,3-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-154T14:00:00,000T01:00:00,3-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-154T21:42:00,001T00:00:00,3-Jun-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-154T21:42:00,000T15:00:00,3-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-154T22:22:00,000T08:00:00,3-Jun-09,UVIS,Prime,Saturn,MOS111APO,,,"Note: As no data will be collected while Cassini is slewing, actual data volume = (8648.632 bps, from Alain Jouchoux's spreadsheet)x(140.0 s per stare)x(101 stares) = 122.29x10^6 bits Mosaic scan of Saturn magnetosphere, day 1. One 8.0-hr block of time assumed. +z pointing from Saturn S pole to N pole assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 140.0 s, stop data capture. Step out to ~10.0 Rs by repeating PATTERN 100 times. PATTERN: Slew +5.0 mrad about z-axis. Start data capture, stare 140.0 s, stop data capture.",,,,,, 2009-155T00:00:00,000T00:34:00,4-Jun-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-155T06:22:00,000T05:40:00,4-Jun-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-155T12:02:00,000T17:50:00,4-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-155T12:42:00,000T09:00:00,4-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-155T13:42:00,000T05:30:00,4-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09155_SP,rider,,,,,, 2009-155T14:00:00,000T01:00:00,4-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-155T21:42:00,001T07:30:00,4-Jun-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-155T21:42:00,000T08:10:00,4-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-155T22:22:00,000T21:10:00,4-Jun-09,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_112SA_MIRMAP001_PRIME,"Northern hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2009-155T23:06:00,000T06:46:00,4-Jun-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-156T05:52:00,000T00:35:00,5-Jun-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-156T05:52:00,000T00:35:00,5-Jun-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-156T05:52:00,000T00:35:00,5-Jun-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-156T05:52:00,000T00:35:00,5-Jun-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-156T06:27:00,001T11:33:01,5-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-156T06:27:00,000T12:18:00,5-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-156T06:27:00,000T22:45:00,5-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-156T18:45:00,000T10:27:00,5-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-156T20:12:00,000T09:00:00,5-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.648384 Rs exit= 10.959694 Range altitude= 40221.093 km ... -40233.432,,,,,, 2009-156T20:12:00,000T09:00:00,5-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-156T21:12:00,000T08:00:00,5-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09156_SP,rider,,,,,, 2009-157T05:12:00,002T01:45:00,6-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.648384 Rs exit= 10.959694 Range altitude= 40221.093 km ... -40233.432,,,,,, 2009-157T05:12:00,000T13:48:01,6-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-157T05:12:00,000T10:48:01,6-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-157T05:12:00,000T12:48:01,6-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-157T05:12:00,001T21:18:00,6-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-157T06:07:49,000T03:52:12,6-Jun-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-157T06:07:49,000T03:52:12,6-Jun-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-157T06:07:49,000T03:52:12,6-Jun-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-157T06:07:49,000T03:52:12,6-Jun-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-157T06:07:49,000T03:52:12,6-Jun-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. Phase = 129, Lat/Lon = 49N/114. Template N.",,,,,, 2009-157T10:00:01,000T01:00:00,6-Jun-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),WAC Photometry,,,,,, 2009-157T10:00:01,000T01:00:00,6-Jun-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS,,,,,, 2009-157T10:00:01,000T01:00:00,6-Jun-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,"VIMS ridealong with ISS. Stare at Titan. Phase = 129, Lat/Lon = 49N/116. Template N.",,,,,, 2009-157T11:00:01,000T03:50:00,6-Jun-09,VIMS,Prime,Titan,MEDRESDRK,Medium resolution global mapping,Regional Mapping,"Obtain mosaics and 2x2 mosaic at integration times of 80, 160, 500 ms. Phase = 130 deg. Lat/Lon = 50N/120 deg. Template Q .",,,,,, 2009-157T11:00:01,000T03:50:00,6-Jun-09,CIRS,SPASS Rider,Titan,MEDRESDRK,Medium resolution global mapping,,Ride along with ISS,,,,,, 2009-157T11:00:01,000T03:50:00,6-Jun-09,ISS,SPASS Rider,Titan,MEDRESDRK,Medium resolution global mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-157T11:00:01,000T03:50:00,6-Jun-09,RADAR,SPASS Rider,Titan,T56WARMUP,,Warmup for T56,,,,,,, 2009-157T14:50:01,000T03:10:00,6-Jun-09,RADAR,Prime,Titan,T56INRAD,,T56 Inbound Radiometry,,,,,,, 2009-157T16:00:01,000T08:00:00,6-Jun-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T56 flyby,"T56 is another flank-out, post-dusk flyby, with a minimum altitude of 1000 km. As in T55 MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan on the nightside hemisphere. It will be also a good complement to T52, T53, T54 and T55 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-157T18:00:01,000T00:48:00,6-Jun-09,RADAR,Prime,Titan,T56INSCAT,,T56 Inbound Scatterometry,,,,,,, 2009-157T18:00:01,000T01:15:00,6-Jun-09,CAPS,SPASS Rider,Titan,T56INBND,,Inbound 112TI (T56),Inbound 112TI (T56),,,,,, 2009-157T18:00:01,000T01:00:00,6-Jun-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-157T18:00:01,000T01:30:00,6-Jun-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-157T18:49:01,000T00:41:00,6-Jun-09,RADAR,Prime,Titan,T56IHISAR,,T56 Inbound HiSAR,,,,,,, 2009-157T19:00:01,000T02:00:00,6-Jun-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-157T19:00:01,000T00:40:00,6-Jun-09,INMS,Non-SPASS,Titan,TITAN56,,Titan Flyby,Titan observation,,,,,, 2009-157T19:15:01,000T01:30:00,6-Jun-09,CAPS,SPASS Rider,Titan,T56CLOSE,,Closest Approach 112TI (T56),Closest Approach 112TI (T56),,,,,, 2009-157T19:30:01,000T00:12:00,6-Jun-09,RADAR,Prime,Titan,T56INALT,,T56 Inbound Altimetry,,,,,,, 2009-157T19:30:01,000T01:00:00,6-Jun-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-157T19:40:01,000T00:40:00,6-Jun-09,INMS,Non-SPASS,Titan,TITAN56,,Titan Flyby,Titan observation,,,,,, 2009-157T19:42:01,000T00:36:00,6-Jun-09,RADAR,Prime,Titan,T56INOSAR,,T56 Inbound and Outbound SAR,,,,,,, 2009-157T20:18:01,000T00:14:00,6-Jun-09,RADAR,Prime,Titan,T56OUTALT,,T56 Outbound Altimetry,,,,,,, 2009-157T20:20:01,000T00:40:00,6-Jun-09,INMS,Non-SPASS,Titan,TITAN56,,Titan Flyby,Titan observation,,,,,, 2009-157T20:30:01,000T01:30:00,6-Jun-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-157T20:32:01,000T01:09:00,6-Jun-09,CIRS,SPASS Rider,Titan,STOCC,,,Ride along with ISS,,,,,, 2009-157T20:32:01,000T00:21:09,6-Jun-09,UVIS,SPASS Rider,Star,ETAUMATI,,Titan Occults Eta UMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2009-157T20:32:01,000T01:09:00,6-Jun-09,VIMS,SPASS Rider,Titan,LIMBMAP,Limb map,Limb Mapping,"VIMS ridealong with UVIS stellar occ. Titan limb mapping. Phase = 63, Lat/Lon = 57S/291.",,,,,, 2009-157T20:45:01,000T01:15:00,6-Jun-09,CAPS,SPASS Rider,Titan,T56OUTBND,,Outbound 112TI (T56),Outbound 112TI (T56),,,,,, 2009-157T20:53:10,000T00:47:51,6-Jun-09,UVIS,Prime,Star,ETAUMATI,,Titan Occults Eta UMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2009-157T21:00:01,000T01:00:00,6-Jun-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-157T21:00:01,001T09:56:59,6-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-157T21:41:01,000T07:19:00,6-Jun-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-157T21:41:01,000T07:19:00,6-Jun-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with ISS,,,,,, 2009-157T21:41:01,000T07:19:00,6-Jun-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),global map,,,,,, 2009-157T21:41:01,000T03:19:00,6-Jun-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS scan across Titan. Titan limb mapping. Phase = 50, Lat/Lon = 47S/309.",,,,,, 2009-157T22:00:01,000T21:56:59,6-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-157T22:00:01,000T19:59:59,6-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-158T00:00:01,001T06:56:59,7-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-158T01:00:01,000T04:00:00,7-Jun-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS scan across Titan. Titan limb mapping. Phase = 46, Lat/Lon = 45S/315.",,,,,, 2009-158T05:00:01,000T05:00:00,7-Jun-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-158T05:00:01,000T05:00:00,7-Jun-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-158T05:00:01,000T05:00:00,7-Jun-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-158T05:00:01,000T05:00:00,7-Jun-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-158T05:00:01,000T05:00:00,7-Jun-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. Phase = 45, Lat/Lon = 44S/320. Template C.",,,,,, 2009-158T10:00:01,000T09:02:48,7-Jun-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"Various cubes (32x32, 48x48, 64x64) at various exposure times (80, 160, 640 ms). Phase = 50 deg. Lat/Lon = 40S/330 deg. Template B.",,,,,, 2009-158T10:00:01,000T09:02:48,7-Jun-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS,,,,,, 2009-158T10:00:01,000T09:02:48,7-Jun-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-158T18:00:00,000T12:01:07,7-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-158T19:17:00,000T09:40:00,7-Jun-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-158T19:57:00,004T12:10:00,7-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-158T19:57:00,000T09:00:00,7-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-158T20:57:00,000T08:00:00,7-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09158_SP,rider,,,,,, 2009-159T02:30:00,000T04:27:00,8-Jun-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-159T04:57:00,000T02:00:00,8-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-159T05:57:00,000T01:00:00,8-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09159_SP,rider,,,,,, 2009-159T06:01:07,001T14:07:25,8-Jun-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-159T06:57:00,001T23:32:59,8-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.648384 Rs exit= 10.959694 Range altitude= 40221.093 km ... -40233.432,,,,,, 2009-159T06:57:00,001T00:03:00,8-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-159T06:57:00,004T01:10:00,8-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-159T06:57:00,002T20:10:00,8-Jun-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-159T07:35:00,000T07:00:00,8-Jun-09,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-159T07:35:00,000T07:00:00,8-Jun-09,CIRS,SPASS Rider,rings(general),EQLBS,,CIRS_109RI_TMAPS20LP001_SI,,,,,,, 2009-159T07:35:00,000T07:00:00,8-Jun-09,UVIS,SPASS Rider,rings(general),EQLBS,,URSTAR,,,,,,, 2009-159T07:35:00,000T07:00:00,8-Jun-09,VIMS,SPASS Rider,rings(general),EQLBS,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-159T14:35:00,000T04:50:00,8-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-159T14:35:00,000T04:50:00,8-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,,Ride along with ISS.,,,,,, 2009-159T19:57:00,000T09:00:00,8-Jun-09,RSS,SPASS Rider,Titan,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T57 Rev113 Titan occultation experiment on 2009/173.",,,,,, 2009-159T19:57:00,000T09:00:00,8-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-159T20:57:00,000T08:00:00,8-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09559_SP,rider,,,,,, 2009-160T05:30:00,000T01:15:00,9-Jun-09,ISS,Prime,Titan,M30R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 25.8 range 1.1 Mkm",,,,,, 2009-160T05:30:00,000T01:15:00,9-Jun-09,CIRS,SPASS Rider,Titan,M30R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-160T05:30:00,000T01:15:00,9-Jun-09,UVIS,SPASS Rider,Titan,M30R1CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-160T06:45:00,000T01:35:00,9-Jun-09,ISS,Prime,RingF,FRINGHRLF,,High Resolution F Ring Scan,Complete high resolution (0-10Rs) longitudinal scan of the F ring. Lit face. Need at least 3 during XM. 2 of 27 as priority 1 and 1 as priority 2.,,,,,, 2009-160T06:45:00,000T01:35:00,9-Jun-09,CIRS,SPASS Rider,rings(general),FRINGHRLF,,,Ride along with ISS.,,,,,, 2009-160T06:45:00,000T01:35:00,9-Jun-09,VIMS,SPASS Rider,RingF,FRINGHRLF,,F Ring hi-res observation,FMOVIE,,,,,, 2009-160T07:00:00,000T02:00:00,9-Jun-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2009-160T08:20:00,000T01:20:00,9-Jun-09,VIMS,Prime,Saturn,ALPAUROCC,Alpha Aur occultation,Saturn occ - alpAur,alpAur Saturn occultation,,,,,, 2009-160T08:20:00,000T01:20:00,9-Jun-09,CIRS,SPASS Rider,Saturn,ALPAUROCC,Alpha Aur occultation,,Ride along with VIMS.,,,,,, 2009-160T09:00:00,001T02:12:00,9-Jun-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-160T09:40:00,000T04:00:00,9-Jun-09,VIMS,Prime,rings(general),PREEQX,,Equinox observation,"radial scan of 1 ansa, 320 msec, 64*64 cubes",,,,,, 2009-160T09:40:00,000T04:00:00,9-Jun-09,CIRS,SPASS Rider,rings(general),PREEQX,,,Ride along with VIMS.,,,,,, 2009-160T09:40:00,000T04:00:00,9-Jun-09,UVIS,SPASS Rider,rings(general),PREEQX,,URSTAR,,,,,,, 2009-160T13:40:00,000T05:00:00,9-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-160T13:40:00,000T05:00:00,9-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,,Ride along with ISS.,,,,,, 2009-160T14:48:07,000T00:00:01,9-Jun-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 9.523 Rs, lat = -43 deg, phase = 75 deg",,,,,, 2009-160T18:40:00,000T04:00:00,9-Jun-09,VIMS,Prime,rings(general),LPSPOKE,,"Spoke observation, phase angle 50-70 degrees","Stare at B ring (100,000 km) near morning shadow.",,,,,, 2009-160T18:40:00,000T04:00:00,9-Jun-09,CIRS,SPASS Rider,rings(general),LPSPOKE,,,Ride along with VIMS.,,,,,, 2009-160T18:40:00,000T04:00:00,9-Jun-09,UVIS,SPASS Rider,rings(general),LPSPOKE,,URSTAR,,,,,,, 2009-160T20:08:32,001T06:33:47,9-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-160T22:40:00,000T03:00:00,9-Jun-09,ISS,Prime,RingF,HRESFRING,,Hi Res low phase F Ring,"Hi res(<10Rs) and low phase(<45 deg) imaging of the F ring to look at satellites embedded in the F ring, need at least 3 one hour observations of the 86hrs available i.e. 3 of 14.",,,,,, 2009-160T22:40:00,000T03:00:00,9-Jun-09,CIRS,SPASS Rider,rings(general),HRESFRING,,,Ride along with ISS.,,,,,, 2009-160T22:40:00,000T03:00:00,9-Jun-09,VIMS,SPASS Rider,RingF,HRESFRING,,F Ring hi-res observation,FMOVIE,,,,,, 2009-161T02:12:00,000T09:00:00,10-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-161T03:12:00,000T08:00:00,10-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09161_SP,rider,,,,,, 2009-161T06:29:59,000T03:08:00,10-Jun-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 10.965114 Rs exit= 11.496453 Range altitude= -39388.413 km ... 39301.343,,,,,, 2009-161T07:04:59,000T02:00:00,10-Jun-09,CDA,SPASS Rider,DustRAM direction,RPX0050,,CDA RPXing 2009-161T08:04:59 MH,"RPXing at 11.221515 Rs , large ring extention, small/medium inclintn",,,,,, 2009-161T09:37:59,002T19:03:01,10-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S51,Range enter= 11.502431 Rs exit= 8.0284280 Range altitude= 40146.334 km ... -40576.483,,,,,, 2009-161T11:12:00,000T23:59:00,10-Jun-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-161T11:45:00,000T12:56:00,10-Jun-09,ISS,Prime,RingF,FMOVIE,F ring movie,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-161T11:45:00,000T12:56:00,10-Jun-09,CIRS,SPASS Rider,RingF,FMOVIE,F ring movie,,Ride along with ISS.,,,,,, 2009-161T11:45:00,000T12:56:00,10-Jun-09,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Ring movie,FMOVIE,,,,,, 2009-162T02:11:00,000T09:00:00,11-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-162T02:42:19,001T05:24:41,11-Jun-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-162T03:07:00,002T01:34:00,11-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-162T03:11:00,000T08:00:00,11-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09162_SP,rider,,,,,, 2009-162T11:11:00,000T16:19:00,11-Jun-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-162T11:40:00,000T06:05:00,11-Jun-09,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-162T11:40:00,000T06:05:00,11-Jun-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_109RI_TMAPS20LP001_SI,,,,,,, 2009-162T11:40:00,000T06:05:00,11-Jun-09,UVIS,SPASS Rider,rings(general),EQLBN,,URSTAR,,,,,,, 2009-162T11:40:00,000T06:05:00,11-Jun-09,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-162T14:45:00,000T03:00:00,11-Jun-09,RADAR,SPASS Rider,Other,WU4NEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-162T17:45:00,000T01:30:00,11-Jun-09,RADAR,Prime,Titan,NEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-162T19:41:00,000T09:00:00,11-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-162T20:41:00,000T08:00:00,11-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09562_SP,rider,,,,,, 2009-163T03:30:00,000T02:00:00,12-Jun-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-163T05:05:00,000T04:30:00,12-Jun-09,ISS,Prime,rings(general),PHOTDARK,,"intermediate phase, dark-face ring photometry","intermediate unlit #9: B = 53, phase = 61, B' = -0.9",,,,,, 2009-163T05:05:00,000T04:30:00,12-Jun-09,CIRS,SPASS Rider,rings(general),PHOTDARK,,,Ride along with ISS.,,,,,, 2009-163T05:05:00,000T04:30:00,12-Jun-09,VIMS,SPASS Rider,rings(general),PHOTDARK,,PhotDark mosaic,Main ring photometry,,,,,, 2009-163T05:30:00,000T23:11:00,12-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-163T08:07:00,000T20:34:00,12-Jun-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-163T08:07:00,000T20:34:00,12-Jun-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-163T08:07:00,000T20:34:00,12-Jun-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-163T08:07:00,000T20:34:00,12-Jun-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-163T09:35:00,000T06:34:00,12-Jun-09,UVIS,Prime,Star,URZETCEN,Stellar ring occultation,URSTAR,,,,,,, 2009-163T09:35:00,000T06:34:00,12-Jun-09,CIRS,SPASS Rider,Star,URZETCEN,Stellar ring occultation,,Ride along with ISS.,,,,,, 2009-163T16:09:00,000T00:30:00,12-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-163T16:39:00,000T02:41:00,12-Jun-09,CAPS,Prime,Saturn,HLCUSPPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-163T16:39:00,000T02:41:00,12-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,HLCUPSPTG,,,Ride along with CAPS.,,,,,, 2009-163T19:41:00,000T09:00:00,12-Jun-09,RSS,SPASS Rider,Titan,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T57 Rev113 Titan occultation experiment on 2009/173.",,,,,, 2009-163T19:41:00,000T09:00:00,12-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-163T20:41:00,000T08:00:00,12-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09163_SP,rider,,,,,, 2009-164T04:41:00,000T01:21:00,13-Jun-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-164T04:41:00,000T01:21:00,13-Jun-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-164T04:41:00,004T09:27:00,13-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S S51,Range enter= 11.502431 Rs exit= 8.0284280 Range altitude= 40146.334 km ... -40576.483,,,,,, 2009-164T04:41:00,000T00:43:00,13-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-164T04:41:00,000T01:21:00,13-Jun-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-164T04:41:00,000T01:21:00,13-Jun-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-164T04:41:00,004T09:27:00,13-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-164T04:46:00,000T00:02:00,13-Jun-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S51 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-164T05:24:00,000T00:07:00,13-Jun-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-164T05:27:00,000T01:15:00,13-Jun-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 85 range 2.1 Mkm",,,,,, 2009-164T05:27:00,000T01:15:00,13-Jun-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-164T05:27:00,000T01:15:00,13-Jun-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-164T05:31:00,000T00:05:00,13-Jun-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-164T05:36:00,000T00:33:00,13-Jun-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-164T06:02:00,000T07:25:00,13-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-164T06:02:00,000T07:25:00,13-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-164T06:02:00,000T07:25:00,13-Jun-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-164T06:09:00,000T00:22:59,13-Jun-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-164T06:31:59,001T21:54:01,13-Jun-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-164T06:42:00,000T10:00:00,13-Jun-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_112SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-164T13:27:00,003T05:59:00,13-Jun-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-164T13:27:00,000T10:04:00,13-Jun-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-164T13:27:00,001T15:33:00,13-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-164T13:27:00,003T05:59:00,13-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-164T16:42:00,000T02:19:00,13-Jun-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-164T19:41:00,000T09:00:00,13-Jun-09,RSS,SPASS Rider,Titan,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the T57 Rev113 Titan occultation experiment on 2009/173.",,,,,, 2009-164T19:41:00,000T09:00:00,13-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-164T20:41:00,000T06:00:00,13-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09164_SP,rider,,,,,, 2009-164T23:31:00,003T14:38:00,13-Jun-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-165T05:21:00,000T00:30:00,14-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-165T05:51:00,000T04:00:00,14-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-165T05:51:00,000T04:00:00,14-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_112RI_MNRNGSHAD015_ISS,rider,,,,,, 2009-165T09:51:00,000T03:00:00,14-Jun-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-165T09:51:00,000T03:00:00,14-Jun-09,CIRS,SPASS Rider,rings(general),ALPVIR,Alpha Virginis occultation,CIRS_112RI_ALPVIR001_UVIS,rider,,,,,, 2009-165T09:51:00,000T03:00:00,14-Jun-09,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2009-165T12:51:00,000T02:00:00,14-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-165T14:51:00,000T03:55:00,14-Jun-09,VIMS,Prime,rings(general),APOMOSU,,"Apoapse mosaic, unlit side",9 x 4 mosaic of unlit rings; tau_IR = 80 ms?,,,,,, 2009-165T14:51:00,000T03:55:00,14-Jun-09,CIRS,SPASS Rider,rings(general),APOMOSU,,CIRS_112RI_APOMOSU135_VIMS,rider,,,,,, 2009-165T19:26:00,000T09:00:00,14-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-165T20:26:00,000T06:00:00,14-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09165_SP,rider,,,,,, 2009-166T04:26:00,001T00:00:00,15-Jun-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-166T04:53:00,000T05:53:00,15-Jun-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Kiviuq rotation curve,Observation of outer moon Kiviuq,,,,,, 2009-166T05:00:00,004T23:15:00,15-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-166T10:46:00,000T00:30:00,15-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-166T11:16:00,000T03:00:00,15-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-166T14:16:00,000T03:55:00,15-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-166T14:16:00,000T03:55:00,15-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_112RI_MNRNGSHAD019_ISS,rider,,,,,, 2009-166T18:11:00,000T01:14:00,15-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,OPNVAV,,CIRS_112IC_OPNVAV661_NAV,rider,,,,,, 2009-166T19:26:00,000T09:00:00,15-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-166T20:26:00,000T06:00:00,15-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09166_SP,rider,,,,,, 2009-167T04:26:00,000T16:34:00,16-Jun-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-167T04:53:00,000T00:23:00,16-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-167T05:16:00,000T05:00:00,16-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-167T07:16:00,000T03:00:00,16-Jun-09,RADAR,SPASS Rider,Other,WU4SRCCAL,,Warm Up for Microwave Source Calibration,Warmup for calibration and science data collection.,,,,,, 2009-167T07:17:20,000T00:00:01,16-Jun-09,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2009-167T10:16:00,000T08:30:00,16-Jun-09,RADAR,Prime,Other,SRCRADCAL,RADAR microwave source radiometric calibration,Radiometric Microwave Sources Calibration,"Scan the Sun, Saturn, and microwave sources while collecting radiometry data.",,,,,, 2009-167T19:26:00,001T08:59:00,16-Jun-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-167T19:26:00,000T18:42:00,16-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-167T19:26:00,000T09:00:00,16-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-167T20:26:00,000T08:00:00,16-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_112IC_DSCAL09167_SP,rider,,,,,, 2009-167T21:00:00,000T00:34:00,16-Jun-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Second MRO as backup to prevent need for RTC if first one fails due to telemetry issues (as in S46),,,,,, 2009-167T21:34:00,000T01:36:00,16-Jun-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-167T23:10:00,000T14:59:00,16-Jun-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-168T04:53:00,000T11:53:00,17-Jun-09,ISS,Prime,Star,CALSTAR3,Stellar Calibration,ISS Photometric Calibration Star 3,"Photometric Calibration Star 3 (HD 20630 = HR 996, Vmag 4.83, G5V)",,,,,, 2009-168T04:53:00,000T11:53:00,17-Jun-09,VIMS,SPASS Rider,Star,CALSTAR3,Stellar Calibration,,ride along with ISS starcal,,,,,, 2009-168T05:00:00,000T08:00:00,17-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-168T14:08:00,007T23:35:59,17-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 11.502431 Rs exit= 8.0284280 Range altitude= 40146.334 km ... -40576.483,,,,,, 2009-168T14:08:00,004T14:02:00,17-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-168T14:08:00,001T21:32:00,17-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-168T14:09:00,002T06:45:00,17-Jun-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-168T14:09:00,002T06:31:00,17-Jun-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-168T14:09:09,000T00:00:01,17-Jun-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 55.7 deg, r = 30.977 Rs, phase = 104 deg",,,,,, 2009-168T16:46:00,000T01:59:00,17-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-168T19:25:00,000T09:00:00,17-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-168T20:25:00,000T08:00:00,17-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09168_SP,rider,,,,,, 2009-169T04:25:00,002T23:52:00,18-Jun-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-169T04:52:00,000T05:53:00,18-Jun-09,CIRS,Prime,Other,1STARECAR,,Mid-IR Stellar Spectroscopy of Eta Carinae,"Spectroscopic observations of Eta Carinae. Slew to star; settle; execute small box scan; return to waypoint. Observation to take 6 hours. For this observation, safe secondary axis +Z or +X to NSP, or -Z or +X to NEP; spectral resolution 3 cm-1.",,,,,, 2009-169T04:52:00,000T05:53:00,18-Jun-09,VIMS,SPASS Rider,Star,1STAROBS,Stellar spectroscopy,,ride along with CIRS starcal,,,,,, 2009-169T10:45:00,000T08:45:00,18-Jun-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Outer satellites Paaliaq observation,Observation of outer moon Paaliaq,,,,,, 2009-169T19:30:00,000T03:00:00,18-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-169T19:30:00,000T03:00:00,18-Jun-09,RADAR,SPASS Rider,Other,WU4NMIDL,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-169T22:30:00,000T01:30:00,18-Jun-09,RADAR,Prime,Titan,NMIDLCAL,,"Distant Titan Radiometry, North Mid Latitudes",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-170T00:00:00,000T10:10:00,19-Jun-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-170T00:00:00,000T10:10:00,19-Jun-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_113RI_SPKMVDFHP001_ISS,rider,,,,,, 2009-170T00:00:00,000T00:34:00,19-Jun-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-170T11:40:00,001T16:37:00,19-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-170T11:40:00,000T09:00:00,19-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-170T12:40:00,000T04:30:00,19-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09170_SP,rider,,,,,, 2009-170T20:40:00,001T00:00:00,19-Jun-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-170T20:54:00,002T07:16:00,19-Jun-09,MIMI,SPASS Rider,Saturn,SURVEY,Magnetospheric survey,Survey,Cut down to very low data volume to correct gap,,,,,, 2009-170T21:20:00,000T01:15:00,19-Jun-09,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 140.8 range 1.3 Mkm",,,,,, 2009-170T21:20:00,000T01:15:00,19-Jun-09,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-170T21:20:00,000T01:15:00,19-Jun-09,UVIS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-170T22:35:00,000T03:19:00,19-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-170T22:35:00,000T03:19:00,19-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_113RI_MNRNGSHAD002_ISS,rider,,,,,, 2009-171T01:54:00,000T02:21:00,20-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-171T04:15:00,000T06:45:00,20-Jun-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-171T04:15:00,000T06:45:00,20-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-171T11:00:00,000T17:17:00,20-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-171T11:40:00,000T09:00:00,20-Jun-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-171T11:40:00,000T09:00:00,20-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-171T12:40:00,000T04:30:00,20-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09171_SP,rider,,,,,, 2009-171T20:40:00,001T07:30:00,20-Jun-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-171T21:20:00,000T02:00:00,20-Jun-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-171T23:20:00,000T07:40:00,20-Jun-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-171T23:20:00,000T07:40:00,20-Jun-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_113RI_SPKMVDFHP002_ISS,rider,,,,,, 2009-172T04:17:00,001T12:15:35,21-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-172T04:17:00,000T23:53:00,21-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-172T07:00:00,000T04:00:00,21-Jun-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-172T07:00:00,000T04:00:00,21-Jun-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus,,,,,, 2009-172T11:00:00,000T07:30:00,21-Jun-09,CIRS,Prime,rings(general),TDIFN20HP,,CIRS_113RI_TDIFN20HP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-172T11:00:00,000T07:30:00,21-Jun-09,CIRS,SPASS Rider,rings(general),TDIFN20HP,,CIRS_113RI_TDIFN20HP001_SI,,,,,,, 2009-172T19:10:00,000T09:00:00,21-Jun-09,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2009-172T19:10:00,000T09:00:00,21-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-172T20:10:00,000T06:00:00,21-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09172_SP,rider,,,,,, 2009-173T04:10:00,000T13:22:35,22-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-173T04:10:00,000T10:22:35,22-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-173T04:10:00,000T12:22:35,22-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-173T04:10:00,001T14:43:00,22-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-173T05:05:48,000T03:26:47,22-Jun-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-173T05:05:48,000T03:26:47,22-Jun-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-173T05:05:48,000T03:26:47,22-Jun-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-173T05:05:48,000T00:26:47,22-Jun-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. Phase = 140 deg, Lat/Lon = 40N/120. Template M4.",,,,,, 2009-173T05:32:35,000T03:00:00,22-Jun-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. Phase = 140 deg, Lat/Lon = 40N/120. Template N.",,,,,, 2009-173T08:32:35,000T01:00:00,22-Jun-09,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Nightside NAC),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-173T08:32:35,000T01:00:00,22-Jun-09,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with UVIS EUV-FUV scan,,,,,, 2009-173T08:32:35,000T01:00:00,22-Jun-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,"VIMS ridealong with ISS. Stare at Titan. Phase = 140 deg, Lat/Lon = 40N/130. Template N.",,,,,, 2009-173T09:32:35,000T05:33:00,22-Jun-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-173T09:32:35,000T06:45:00,22-Jun-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS EUV-FUV scan,,,,,, 2009-173T09:32:35,000T06:45:00,22-Jun-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS. Scan across Titan. Phase = 145 deg, Lat/Lon = 40N/135. Template X.",,,,,, 2009-173T14:32:35,000T08:00:00,22-Jun-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T57 flyby,"T57 is another flank-out, post-dusk flyby, with a minimum altitude of 1000 km. As in T55 and T56 MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan on the nightside hemisphere. It will be also a good complement to T52, T53, T54, T55 and T56 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-173T15:05:35,000T00:01:00,22-Jun-09,UVIS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-173T15:05:36,000T02:16:59,22-Jun-09,RSS,SPASS Rider,Titan,THERMAL,Thermal stabilization period,RSS Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-173T15:06:35,000T01:11:00,22-Jun-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-173T16:17:35,000T01:05:00,22-Jun-09,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2009-173T16:17:35,000T01:05:00,22-Jun-09,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-173T16:17:35,000T01:05:00,22-Jun-09,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),global map,,,,,, 2009-173T16:17:35,000T01:05:00,22-Jun-09,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-173T16:17:35,000T01:05:00,22-Jun-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping,VIMS ridealong with CIRS. Regional mapping of Titan. Phase = 150 deg. Lat/Lon = 35N/140 deg. Seven 64x64 cubes at 80 ms,,,,,, 2009-173T16:32:35,000T01:00:00,22-Jun-09,CAPS,SPASS Rider,Titan,T57INBND,,Inbound 113TI (T57),Inbound 113TI (T57),,,,,, 2009-173T16:32:35,000T01:00:00,22-Jun-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-173T16:32:35,000T01:30:00,22-Jun-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-173T17:22:35,000T00:50:12,22-Jun-09,RSS,Prime,Titan,OCC,Occultation,RSS OCC of Titan T57,RSS ingress/egress occultation of Titan's atmosphere and ionosphere,,,,,, 2009-173T17:22:35,000T00:49:12,22-Jun-09,CIRS,SPASS Rider,Titan,OCC,Occultation,,Ride along with RSS Occ.,,,,,, 2009-173T17:32:35,000T02:00:00,22-Jun-09,CAPS,SPASS Rider,Titan,T57CLOSE,,Closest Approach 113TI (T57),Closest Approach 113TI (T57),,,,,, 2009-173T17:32:35,000T02:00:00,22-Jun-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-173T17:32:35,000T00:46:00,22-Jun-09,INMS,Non-SPASS,Titan,TITAN57,,Titan Flyby,Titan observation,,,,,, 2009-173T18:02:35,000T01:00:00,22-Jun-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-173T18:11:47,000T00:15:00,22-Jun-09,RADAR,SPASS Rider,Titan,T57WARMUP,,Warmup for T57,,,,,,, 2009-173T18:12:47,000T00:32:18,22-Jun-09,RADAR,Prime,Titan,T57RASAR,,T57 Ride-along SAR with INMS at C/A,,,,,,, 2009-173T18:18:35,000T00:26:30,22-Jun-09,INMS,SPASS Rider,Titan,TITAN57,,Titan Flyby,Prime Titan observation,,,,,, 2009-173T18:45:05,000T00:17:30,22-Jun-09,RADAR,Prime,Titan,T57OUTALT,,T57 Outbound Altimetry,,,,,,, 2009-173T18:45:05,000T00:47:30,22-Jun-09,INMS,Non-SPASS,Titan,TITAN57,,Titan Flyby,Titan observation,,,,,, 2009-173T19:02:35,000T00:20:00,22-Jun-09,RADAR,Prime,Titan,T57OHISAR,,T57 outbound HiSAR,,,,,,, 2009-173T19:02:35,000T01:30:00,22-Jun-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-173T19:32:35,000T01:00:00,22-Jun-09,CAPS,SPASS Rider,Titan,T57OUTBND,,Outbound 113TI (T57),Outbound 113TI (T57),,,,,, 2009-173T19:32:35,000T01:00:00,22-Jun-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-173T19:32:35,001T10:07:24,22-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-173T19:44:16,000T00:48:19,22-Jun-09,RADAR,Prime,Titan,T57OUTSCT,,T57 Outbound Scatterometry,,,,,,, 2009-173T20:32:35,000T03:30:00,22-Jun-09,RADAR,Prime,Titan,T57OUTRAD,,T57 Outbound Radiometry,,,,,,, 2009-173T20:32:35,002T12:04:24,22-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-173T20:32:35,001T09:07:25,22-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-173T22:32:35,001T07:07:25,22-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-174T00:02:35,000T03:00:00,23-Jun-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-174T00:02:35,000T03:00:00,23-Jun-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS EUV-FUV scan,,,,,, 2009-174T00:02:35,000T03:00:00,23-Jun-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),global map,,,,,, 2009-174T00:02:35,000T03:00:00,23-Jun-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS. Scan across Titan. Phase = 40 deg, Lat/Lon = 40S/325. Template G.",,,,,, 2009-174T03:02:35,000T00:30:00,23-Jun-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-174T03:02:35,000T00:30:00,23-Jun-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS,,,,,, 2009-174T03:02:35,000T00:30:00,23-Jun-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Map,"VIMS ridealong with ISS. Global mapping of Titan. Phase = 40 deg, Lat/Lon = 40S/325. Temp. G. Five 64x64 80 ms cubes",,,,,, 2009-174T03:32:35,000T05:00:00,23-Jun-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Map of Titan,"Map of Titan. Obtain 64 x 64 cubes of various exposure lengths. Phase = 36.2 deg, Lat/Lon = 36.2S/326.5 deg. Template = V.",,,,,, 2009-174T03:32:35,000T05:00:00,23-Jun-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS,,,,,, 2009-174T03:32:35,000T05:00:00,23-Jun-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),global map,,,,,, 2009-174T08:32:35,000T08:00:00,23-Jun-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-174T08:32:35,000T08:00:00,23-Jun-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-174T08:32:35,000T08:00:00,23-Jun-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),global map,,,,,, 2009-174T08:32:35,000T08:00:00,23-Jun-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Global Map,VIMS ridealong with CIRS. Global mapping of Titan. Phase = 35 deg. Lat/Lon = 35S/330. Temp. A. Various cubes at varying exp times,,,,,, 2009-174T17:40:00,000T10:00:00,23-Jun-09,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's bistat,Additional downlink pass at Ka-band for improving locally Cassini orbit.,,,,,, 2009-174T17:40:00,000T10:00:00,23-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-174T18:40:00,000T09:00:00,23-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09174_SP,rider,,,,,, 2009-174T18:53:00,000T08:47:00,23-Jun-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-175T03:40:00,000T02:00:00,24-Jun-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-175T03:40:00,000T02:00:00,24-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-175T04:40:00,000T01:00:00,24-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09175_SP,rider,,,,,, 2009-175T05:40:00,000T20:20:00,24-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-175T05:40:00,001T02:57:00,24-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-175T05:40:00,001T02:57:22,24-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-175T05:40:00,002T13:37:00,24-Jun-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-175T06:20:00,000T06:00:00,24-Jun-09,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-175T06:20:00,000T06:00:00,24-Jun-09,CIRS,SPASS Rider,rings(general),EQLBS,,CIRS_113RI_EQLBS001_SI,,,,,,, 2009-175T06:20:00,000T06:00:00,24-Jun-09,VIMS,SPASS Rider,rings(general),EQLBS,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-175T12:20:00,000T06:00:00,24-Jun-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-175T12:20:00,000T06:00:00,24-Jun-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,,Ride along with ISS.,,,,,, 2009-175T12:20:00,000T06:00:00,24-Jun-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-175T18:55:00,000T09:00:00,24-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-175T19:55:00,000T08:00:00,24-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09575_SP,rider,,,,,, 2009-176T02:00:00,000T02:00:00,25-Jun-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2009-176T04:00:00,001T06:09:00,25-Jun-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-176T04:35:00,000T01:15:00,25-Jun-09,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 12.3 range 1.3 Mkm",,,,,, 2009-176T04:35:00,000T01:15:00,25-Jun-09,CIRS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-176T04:35:00,000T01:15:00,25-Jun-09,UVIS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-176T05:45:09,000T00:00:01,25-Jun-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 7.212 Rs, lat = -36 deg, phase = 71 deg",,,,,, 2009-176T05:50:00,000T05:00:00,25-Jun-09,VIMS,Prime,rings(general),PREEQX,,Equinox observation,"radial scan of 1 ansa, 320 msec, 64*64 cubes",,,,,, 2009-176T05:50:00,000T05:00:00,25-Jun-09,CIRS,SPASS Rider,rings(general),PREEQX,,,Ride along with ISS.,,,,,, 2009-176T05:50:00,000T05:00:00,25-Jun-09,UVIS,SPASS Rider,rings(general),PREEQX,,URSTAR,,,,,,, 2009-176T08:37:00,000T08:00:00,25-Jun-09,CAPS,SPASS Rider,Saturn,IMVP7,,MAPS IMVP Campaign,MAPS IMVP Campaign,,,,,, 2009-176T08:37:00,000T08:00:00,25-Jun-09,MIMI,SPASS Rider,Saturn,IMVP7,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=7, near 2400 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2009-176T08:37:00,000T08:00:00,25-Jun-09,MAG,Non-SPASS,Saturn,IMVP7,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9",,,,,, 2009-176T08:37:00,000T08:00:00,25-Jun-09,RPWS,Non-SPASS,co-rotation,IMVP7,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-176T10:50:00,000T03:15:00,25-Jun-09,ISS,Prime,Enceladus,PLMMRMP,,Medium res plume obs at high phase,Medium resolution plume observation at intermed. phase,,,,,, 2009-176T10:50:00,000T03:15:00,25-Jun-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-176T13:43:59,000T00:42:00,25-Jun-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.0346882 Rs exit= 8.1636691 Range altitude= -39606.628 km ... -20176.128,,,,,, 2009-176T14:05:00,000T04:00:00,25-Jun-09,CDA,Prime,DustRAM direction,RPX0060,,CDA RPXing 2009-176T15:06:59 MH,"RPXing at 8.2994493 Rs, vertical Xing outside 7 Rs",,,,,, 2009-176T14:07:00,000T02:00:00,25-Jun-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-176T14:25:59,000T01:22:00,25-Jun-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.1703014 Rs exit= 8.4487186 Range altitude= -19203.311 km ... 19733.986,,,,,, 2009-176T15:47:59,000T00:40:00,25-Jun-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.4559873 Rs exit= 8.5966941 Range altitude= 20706.816 km ... 39170.130,,,,,, 2009-176T16:27:59,007T12:36:01,25-Jun-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 8.6042321 Rs exit= 5.6667681 Range altitude= 40140.553 km ... -40577.514,,,,,, 2009-176T16:37:00,001T18:05:00,25-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-176T16:37:00,001T18:05:00,25-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-176T16:37:00,001T18:05:00,25-Jun-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-176T18:05:00,000T02:00:00,25-Jun-09,ISS,Prime,Mimas,063W011PH,,Mimas,"Turn UVIS_FUV to Mimas; do ftprt with (0,0,-1.03 mrad) offset for CIRS; do ftprt with (0,0,0) mrad offset for UVIS; turn to WP.",,,,,, 2009-176T18:05:00,000T02:00:00,25-Jun-09,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-176T18:05:00,000T02:00:00,25-Jun-09,VIMS,SPASS Rider,Mimas,063W011PH,,,null,,,,,, 2009-176T20:05:00,000T04:35:00,25-Jun-09,VIMS,Prime,rings(general),COMPLODRK,Low phase dark side ring radial scan,"Hi res radial scan, dark side","radial scan of 1 ansa, 320 msec, 64*12 cubes",,,,,, 2009-176T20:05:00,000T04:35:00,25-Jun-09,CIRS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,,Ride along with ISS.,,,,,, 2009-176T20:05:00,000T04:35:00,25-Jun-09,ISS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,RING RADIAL S,"VIMS RADIAL SCAN WAC COLOR RIDE ALONG: up to 8 footprints X 6 COLORS on one ansa, near equinox",,,,,, 2009-176T20:05:00,000T04:35:00,25-Jun-09,UVIS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,URSTAR,,,,,,, 2009-177T01:09:00,000T09:00:00,26-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-177T02:09:00,000T08:00:00,26-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09177_SP,rider,,,,,, 2009-177T10:09:00,001T00:00:00,26-Jun-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-177T10:40:00,000T06:00:00,26-Jun-09,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-177T10:40:00,000T06:00:00,26-Jun-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_113RI_EQLBN001_SI,,,,,,, 2009-177T10:40:00,000T06:00:00,26-Jun-09,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-177T16:40:00,000T02:20:00,26-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-177T16:40:00,000T02:20:00,26-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,,Ride along with ISS.,,,,,, 2009-177T19:00:00,000T04:40:00,26-Jun-09,UVIS,Prime,Star,URMUCEN,,URSTAR,,,,,,, 2009-177T19:00:00,000T04:40:00,26-Jun-09,CIRS,SPASS Rider,Star,URMUCEN,,,Ride along with ISS.,,,,,, 2009-177T19:17:00,002T08:22:00,26-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-178T01:09:00,000T09:00:00,27-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-178T02:09:00,000T08:00:00,27-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09178_SP,rider,,,,,, 2009-178T10:09:00,000T01:51:00,27-Jun-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-178T10:40:00,000T06:55:00,27-Jun-09,UVIS,Prime,Star,URALPLUP,,URSTAR,,,,,,, 2009-178T10:40:00,000T06:55:00,27-Jun-09,CIRS,SPASS Rider,Star,URALPLUP,,,Ride along with ISS.,,,,,, 2009-178T10:42:00,000T03:25:00,27-Jun-09,CAPS,SPASS Rider,Saturn,HLCUSP,,MAPS high latitude cusp campaign,MAPS high latitude cusp campaign,,,,,, 2009-178T10:42:00,000T03:25:00,27-Jun-09,MIMI,SPASS Rider,Saturn,HLCUSP,,MAPS CUSP Campaign,Part of CUSP MAPS Campaign. Observe the high latitude cusp (geometrically) and solar wind entry regions,,,,,, 2009-178T10:42:00,000T03:25:00,27-Jun-09,MAG,Non-SPASS,Saturn,HLCUSP,,MAG MAPS HL Cusp Campaign,"Observe the cusp region from high latitude. HLCUSP are 9>local time>15, |lat| > 50, r > 15",,,,,, 2009-178T10:42:00,000T03:25:00,27-Jun-09,RPWS,Non-SPASS,Saturn,HLCUSP,,MAPS High Latitude Cusp Campaign,Part of High Latitude Cusp MAPS Campaign. Observe cusp near noon on highly inclined orbits,,,,,, 2009-178T12:00:00,000T02:00:00,27-Jun-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-178T14:00:00,001T13:39:00,27-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-178T14:07:00,001T01:25:00,27-Jun-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-178T14:07:00,001T01:25:00,27-Jun-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-178T14:07:00,001T01:25:00,27-Jun-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-178T17:35:00,000T07:00:00,27-Jun-09,CIRS,Prime,rings(general),VTMPN60MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-178T17:35:00,000T07:00:00,27-Jun-09,CIRS,SPASS Rider,rings(general),VTMPN60MP,,CIRS_113RI_VTMPN60MP001_SI,,,,,,, 2009-178T17:35:00,000T07:00:00,27-Jun-09,VIMS,SPASS Rider,rings(general),VTMPN60MP,,"azimuthal scan, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-179T00:54:00,000T09:00:00,28-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-179T01:54:00,000T08:00:00,28-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09179_SP,rider,,,,,, 2009-179T10:10:00,000T01:15:00,28-Jun-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 81.6 range 2.4 Mkm",,,,,, 2009-179T10:10:00,000T01:15:00,28-Jun-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-179T10:10:00,000T01:15:00,28-Jun-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-179T11:25:00,000T00:30:00,28-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-179T11:55:00,000T03:00:00,28-Jun-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-179T11:55:00,000T03:00:00,28-Jun-09,CIRS,SPASS Rider,Saturn,SURVEYPTG,MAPS survey/Prime pointing,,Ride along with ISS.,,,,,, 2009-179T14:55:00,000T03:30:00,28-Jun-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-179T14:55:00,000T03:30:00,28-Jun-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,,Ride along with ISS.,,,,,, 2009-179T15:32:00,003T11:52:00,28-Jun-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-179T15:32:00,002T21:12:00,28-Jun-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-179T15:32:00,000T12:07:00,28-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-179T15:32:00,000T12:07:00,28-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-179T18:39:00,000T09:00:00,28-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-179T19:39:00,000T08:00:00,28-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09579_SP,rider,,,,,, 2009-180T03:39:00,001T23:45:00,29-Jun-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-180T03:39:00,004T00:24:00,29-Jun-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-180T03:39:00,004T01:25:00,29-Jun-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-180T03:39:00,002T23:45:00,29-Jun-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-180T04:00:00,000T09:10:00,29-Jun-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-180T04:19:00,000T05:40:00,29-Jun-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-180T09:59:00,000T08:00:00,29-Jun-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 1. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8968.95195 bps, from Alain's spreadsheet)x(135.0s per stare)x(111 stares) = 134.40x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 110 times. PATTERN: Slew -3.0 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture.",,,,,, 2009-180T18:39:00,000T09:00:00,29-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-180T19:39:00,000T08:00:00,29-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09180_SP,rider,,,,,, 2009-181T04:19:00,000T00:30:00,30-Jun-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-181T04:49:00,000T08:00:00,30-Jun-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 2. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8968.95195 bps, from Alain's spreadsheet)x(135.0s per stare)x(111 stares) = 134.40x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 110 times. PATTERN: Slew -3.0 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture.",,,,,, 2009-181T12:49:00,000T04:55:00,30-Jun-09,CIRS,Prime,rings(general),POLARIZ,,CIRS_113RI_POLARIZ181_PRIME;,null,,,,,, 2009-181T12:49:00,000T04:55:00,30-Jun-09,CIRS,SPASS Rider,rings(general),POLARIZ,,CIRS_113RI_POLARIZ181_SI,,,,,,, 2009-181T18:24:00,000T09:00:00,30-Jun-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-181T19:24:00,000T08:00:00,30-Jun-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09181_SP,rider,,,,,, 2009-182T03:24:00,001T00:00:00,1-Jul-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-182T04:04:00,000T00:40:00,1-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-182T04:44:00,000T08:00:00,1-Jul-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 3. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8968.95195 bps, from Alain's spreadsheet)x(135.0s per stare)x(111 stares) = 134.40x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 110 times. PATTERN: Slew -3.0 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture.",,,,,, 2009-182T12:44:00,000T04:25:00,1-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-182T12:44:00,001T16:21:00,1-Jul-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-182T17:09:00,000T01:14:00,1-Jul-09,CIRS,SPASS Rider,Skeletonrequest,OPNAV,Optical navigation image,CIRS_113SK_OPNAV821_NAV,rider,,,,,, 2009-182T18:24:00,000T09:00:00,1-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-182T19:24:00,000T08:00:00,1-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_113IC_DSCAL09182_SP,rider,,,,,, 2009-183T03:24:00,004T23:18:00,2-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-183T03:24:00,000T16:36:00,2-Jul-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-183T03:24:00,001T01:40:00,2-Jul-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-183T04:04:00,000T08:00:00,2-Jul-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 4. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8968.95195 bps, from Alain's spreadsheet)x(135.0s per stare)x(111 stares) = 134.40x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 110 times. PATTERN: Slew -3.0 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture.",,,,,, 2009-183T12:04:00,000T02:00:00,2-Jul-09,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,Turn to sun; Time: 30 min; target sun for 60 min; tau_IR = 40 & 320 msec; VIS always @ 50ms; Return to waypoint: 30 min,,,,,, 2009-183T14:04:00,000T03:39:00,2-Jul-09,VIMS,Prime,Star,ALPCENCAL,,ALPCEN calibration,"turn to AlpCen; stare 180 min; return to Waypt. RWA required. tau_IR=640 msec, 6*6 cubes.",,,,,, 2009-183T18:23:00,000T09:00:00,2-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-183T20:00:00,000T02:00:00,2-Jul-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-183T22:00:00,000T07:05:00,2-Jul-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-184T04:03:00,000T06:10:00,3-Jul-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-184T04:03:00,000T06:10:00,3-Jul-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-184T05:04:00,004T22:56:00,3-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 8.6042321 Rs exit= 5.6667681 Range altitude= 40140.553 km ... -40577.514,,,,,, 2009-184T05:04:00,004T22:56:00,3-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-184T05:04:00,003T21:38:00,3-Jul-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-184T05:05:00,003T21:37:00,3-Jul-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-184T05:05:00,002T14:33:00,3-Jul-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-184T05:05:25,000T00:00:01,3-Jul-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 15.9 d, inc = 51.2 deg, r = 33.287 Rs, phase = 109 deg",,,,,, 2009-184T10:13:00,003T16:29:00,3-Jul-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-184T10:53:00,000T09:00:00,3-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-184T11:53:00,000T08:00:00,3-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09184_SP,rider,,,,,, 2009-184T20:33:00,000T02:00:00,3-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-184T22:33:00,000T11:40:00,3-Jul-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning N. hemisphere + pole, may be split in half by downlink",,,,,, 2009-185T06:22:00,001T00:00:00,4-Jul-09,VIMS,Non-SPASS,SpacecraftActivity,DECONHIGH,Decontamination,Decontamination - High Power,IR Optics Decontamination at high power (88 Watts). Other instruments can observe during this request.,,,,,, 2009-185T10:53:00,000T09:00:00,4-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-185T11:53:00,000T08:00:00,4-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09185_SP,rider,,,,,, 2009-185T20:33:00,000T04:35:00,4-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-186T01:08:00,000T08:00:00,5-Jul-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 5. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8968.95195 bps, from Alain's spreadsheet)x(135.0s per stare)x(111 stares) = 134.40x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 110 times. PATTERN: Slew -3.0 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture.",,,,,, 2009-186T06:22:00,001T00:00:00,5-Jul-09,VIMS,Non-SPASS,SpacecraftActivity,DECONLOW,Decontamination,Decontamination - High Power,IR Optics Decontamination at high power (88 Watts). Other instruments can observe during this request.,,,,,, 2009-186T10:38:00,000T09:00:00,5-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-186T11:38:00,000T08:00:00,5-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09186_SP,rider,,,,,, 2009-186T19:38:00,001T00:00:00,5-Jul-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-186T20:18:00,000T01:15:00,5-Jul-09,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 147.8 range 1.4 Mkm",,,,,, 2009-186T20:18:00,000T01:15:00,5-Jul-09,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-186T20:18:00,000T01:15:00,5-Jul-09,UVIS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-186T21:33:00,000T02:00:00,5-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-186T23:33:00,000T02:25:00,5-Jul-09,CIRS,Prime,rings(general),TMAPN30MP,,Rings TMAP,null,,,,,, 2009-186T23:33:00,000T02:25:00,5-Jul-09,CIRS,SPASS Rider,rings(general),TMAPN30MP,,CIRS_114RI_TMAPN30MP001_SI,,,,,,, 2009-187T01:58:00,000T08:00:00,6-Jul-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 6. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8968.95195 bps, from Alain's spreadsheet)x(135.0s per stare)x(111 stares) = 134.40x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 110 times. PATTERN: Slew -3.0 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture.",,,,,, 2009-187T10:38:00,000T09:00:00,6-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-187T11:38:00,000T08:00:00,6-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09187_SP,rider,,,,,, 2009-187T19:38:00,001T08:22:00,6-Jul-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-187T20:18:00,000T16:00:00,6-Jul-09,UVIS,Prime,Saturn,MOS113APO,,,"Mosaic scan of Saturn magnetosphere, day 7. One 16.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (9313.91164 bps, from Alain's spreadsheet)x(130.0s per stare)x(266 stares) = 322.08x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Slew -330.0 mrad about z-axis. Start data capture, stare 130.0 s, stop data capture. Repeat PATTERN 265 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 130.0 s, stop data capture.",,,,,, 2009-188T02:42:00,001T01:18:00,7-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-188T02:42:00,000T16:56:00,7-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-188T02:42:00,001T01:18:00,7-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-188T12:18:00,000T06:02:00,7-Jul-09,ISS,Prime,RingE,HPMELR,,E Ring High Phase Observation,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-188T12:18:00,000T06:02:00,7-Jul-09,CIRS,SPASS Rider,RingE,HPMELR,,CIRS_114RE_HPMELR001_ISS,rider,,,,,, 2009-188T19:00:00,000T09:00:00,7-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-188T19:38:00,000T17:26:03,7-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-188T20:00:00,000T08:00:00,7-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09188_SP,rider,,,,,, 2009-189T04:00:00,000T11:17:03,8-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-189T04:00:00,002T00:53:00,8-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 8.6042321 Rs exit= 5.6667681 Range altitude= 40140.553 km ... -40577.514,,,,,, 2009-189T04:00:00,000T12:04:03,8-Jul-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-189T04:00:00,000T11:04:03,8-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-189T04:00:00,000T11:04:03,8-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-189T04:44:59,000T03:19:04,8-Jul-09,VIMS,Prime,Titan,CLOUDMAP,Cloud map,Global and cloud mapping,Stare at Titan for globe and cloud mapping. Phase = 145 deg. Lat/Lon = 35N/125 deg . Temp = O,,,,,, 2009-189T04:44:59,000T03:19:04,8-Jul-09,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Cloud monitor,,,,,, 2009-189T04:44:59,000T03:19:04,8-Jul-09,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-189T08:04:03,000T03:50:00,8-Jul-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-189T08:04:03,000T06:40:00,8-Jul-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Cloud monitor,,,,,, 2009-189T08:04:03,000T03:50:00,8-Jul-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-189T08:04:03,000T03:50:00,8-Jul-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS scan across Titan. Phase = 145 deg, Lat/Lon = 35N/128 deg. Template X.",,,,,, 2009-189T11:54:03,000T02:50:00,8-Jul-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-189T11:54:03,000T02:50:00,8-Jul-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-189T11:54:03,000T04:43:00,8-Jul-09,RADAR,SPASS Rider,Titan,T58WARMUP,,Warmup for T58,,,,,,, 2009-189T11:54:03,000T02:50:00,8-Jul-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS scan across Titan. Phase = 145 deg, Lat/Lon = 35N/133 deg. Template X.",,,,,, 2009-189T13:04:03,000T08:00:00,8-Jul-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T58 flyby,"T58 is the fourth consecutive flank-out, post-dusk flyby with a relatively low altitude at closest approach (1144 km). As in T55, T56 and T57, MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan on the nightside hemisphere. It will be also a good complement to T52, T53, T54, T55, T56 and T57 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-189T14:44:03,000T00:48:00,8-Jul-09,VIMS,Prime,Titan,HIRES,High resolution image,Titan Mosaic,Titan mosaic. Phase = 150 deg. Lat/Lon = 30N/140 deg.,,,,,, 2009-189T14:44:03,000T00:48:00,8-Jul-09,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Cloud monitor,,,,,, 2009-189T14:44:03,000T00:48:00,8-Jul-09,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-189T15:04:03,000T01:00:00,8-Jul-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-189T15:04:03,000T01:15:00,8-Jul-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-189T15:17:03,000T01:02:00,8-Jul-09,CAPS,SPASS Rider,Titan,T58INBND,,Inbound 114TI (T58),Inbound 114TI (T58),,,,,, 2009-189T15:32:03,000T01:05:00,8-Jul-09,UVIS,Prime,Sun,USUNOCC,Solar occultation,USUN_T58 Solar Occ Titan,This is a solar occultation by Titan. Turn occurs prior to this period; EUV solar occultation port centered on sun Slit aligned tangent to limb. Record data during occultation. Turn back occurs after this period.,,,,,, 2009-189T15:32:03,000T01:05:00,8-Jul-09,CIRS,SPASS Rider,Titan,SOLOCC,Solar occultation,,Cloud monitor,,,,,, 2009-189T15:32:03,000T01:05:00,8-Jul-09,VIMS,SPASS Rider,Titan,LIMBMAP,Limb map,Titan solar occ.,VIMS ridealong with UVIS during solar occultation . Phase 154 deg. Lat/Lon = 25N/143 deg.,,,,,, 2009-189T16:04:03,000T02:00:00,8-Jul-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-189T16:04:03,000T00:40:00,8-Jul-09,INMS,Non-SPASS,Titan,TITAN58,,Titan Flyby,Titan observation,,,,,, 2009-189T16:19:03,000T01:30:00,8-Jul-09,CAPS,SPASS Rider,Titan,T58CLOSE,,Closest Approach 114TI (T58),Closest Approach 114TI (T58),,,,,, 2009-189T16:19:03,000T00:15:00,8-Jul-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-189T16:34:03,000T01:00:00,8-Jul-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-189T16:38:03,000T00:52:00,8-Jul-09,RADAR,Prime,Titan,T58INOSAR,,T58 Inbound and Outbound SAR,,,,,,, 2009-189T16:44:03,000T00:40:00,8-Jul-09,INMS,Non-SPASS,Titan,TITAN58,,Titan Flyby,Titan observation,,,,,, 2009-189T17:24:03,000T00:40:00,8-Jul-09,INMS,Non-SPASS,Titan,TITAN58,,Titan Flyby,Titan observation,,,,,, 2009-189T17:30:03,000T00:21:05,8-Jul-09,CIRS,SPASS Rider,Titan,TRANS,,,Cloud monitor,,,,,, 2009-189T17:30:03,000T00:21:05,8-Jul-09,UVIS,SPASS Rider,Star,ETAUMATI,,Titan Occults Eta UMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2009-189T17:30:03,000T00:21:05,8-Jul-09,VIMS,SPASS Rider,Titan,TRANS,,Limb mapping,Cubes obtained during transition to RWA and UVIS stellar occ. Phase = 50 deg. Lat/Lon. = 49S/310 deg.,,,,,, 2009-189T17:34:03,000T00:15:00,8-Jul-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-189T17:49:03,000T01:02:00,8-Jul-09,CAPS,SPASS Rider,Titan,T58OUTBND,,Outbound 114TI (T58),Outbound 114TI (T58),,,,,, 2009-189T17:49:03,000T01:15:00,8-Jul-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-189T17:51:08,000T00:37:55,8-Jul-09,UVIS,Prime,Star,ETAUMATI,,Titan Occults Eta UMa,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2009-189T17:51:08,000T00:37:55,8-Jul-09,CIRS,SPASS Rider,Titan,SOLOCC,Solar occultation,,Cloud monitor,,,,,, 2009-189T17:51:08,000T00:37:55,8-Jul-09,VIMS,SPASS Rider,Titan,LIMBMAP,Limb map,Limb Mapping,"VIMS ridealong with UVIS during stellar occultation for limb mapping. Phase = 35 deg, Lat/Lon = 47S/315 deg.",,,,,, 2009-189T18:04:03,000T01:00:00,8-Jul-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-189T18:04:03,001T08:54:10,8-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-189T18:29:03,000T00:35:00,8-Jul-09,VIMS,Prime,Titan,HIRES,High resolution image,Titan Mosaic,Titan mosaic. Phase = 35 deg. Lat/Lon = 35S/320 deg.,,,,,, 2009-189T18:29:03,000T00:35:00,8-Jul-09,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Cloud monitor,,,,,, 2009-189T18:29:03,000T00:35:00,8-Jul-09,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-189T18:51:03,001T10:01:56,8-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-189T19:04:03,000T01:30:00,8-Jul-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-189T19:04:03,000T01:30:00,8-Jul-09,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-189T19:04:03,000T01:30:00,8-Jul-09,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-189T19:04:03,000T01:30:00,8-Jul-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping,"VIMS ridealong with CIRS. Phase = 35 deg, Lat/Lon = 37S/323 deg. Template S2. 64x64 mosaics at 160ms.",,,,,, 2009-189T19:04:03,001T09:48:57,8-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-189T19:04:03,000T19:25:56,8-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-189T20:34:03,000T01:30:00,8-Jul-09,ISS,Prime,Titan,REGMAP,Regional mapping,REG (Regional Mapping),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-189T20:34:03,000T01:30:00,8-Jul-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Cloud monitor,,,,,, 2009-189T20:34:03,000T01:30:00,8-Jul-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"VIMS ridealong with ISS. Phase = 32 deg, Lat/Lon = 33S/323 deg. Template S2. Continue 64x64 mosaics of 160 ms.",,,,,, 2009-189T21:04:03,001T07:48:57,8-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-189T22:04:03,000T04:00:00,8-Jul-09,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,GLB (Global Mapping),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-189T22:04:03,000T04:00:00,8-Jul-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Cloud monitor,,,,,, 2009-189T22:04:03,000T04:00:00,8-Jul-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"VIMS ridealong with ISS. Global mapping of Titan. Phase = 30 deg, Lat/Lon = 30S/325 deg. Template H.",,,,,, 2009-190T02:04:03,000T03:00:00,9-Jul-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-190T02:04:03,000T03:00:00,9-Jul-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-190T02:04:03,000T03:00:00,9-Jul-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-190T02:04:03,000T03:00:00,9-Jul-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-190T02:04:03,000T03:00:00,9-Jul-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS. Stare at Titan. Phase = 30 deg, Lat/Lon = 30S/330 deg. Template D2. 64x64 cubes at various exposure times.",,,,,, 2009-190T05:04:03,000T02:00:00,9-Jul-09,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,MNA (NAC Monitor),"monitoring for surface/atmosphere changes; attempt to see surface color variations; monitor limb hazes, 1-3 km/px",,,,,, 2009-190T05:04:03,000T02:00:00,9-Jul-09,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Cloud monitor,,,,,, 2009-190T05:04:03,000T02:00:00,9-Jul-09,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,Stare at Titan,"VIMS ridealong with ISS. Stare at Titan. Phase = 30 deg, Lat/Lon = 30S/333 deg. Template D2. 64x64 cubes at various exposure times.",,,,,, 2009-190T07:04:03,000T09:00:00,9-Jul-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping,Stare at Titan for globe and cloud mapping. Phase = 30 deg. Lat/Lon = 30S/335 deg. Temp = B.,,,,,, 2009-190T07:04:03,000T09:00:00,9-Jul-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Cloud monitor,,,,,, 2009-190T14:30:00,000T14:23:00,9-Jul-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-190T16:53:00,000T10:00:00,9-Jul-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-190T16:53:00,000T10:00:00,9-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-190T17:53:00,000T09:00:00,9-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09190_SP,rider,,,,,, 2009-191T02:53:00,000T02:00:00,10-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-191T02:58:13,000T01:54:47,10-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-191T03:53:00,000T01:00:00,10-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09191_SP,rider,,,,,, 2009-191T04:53:00,000T17:59:00,10-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-191T04:53:00,000T20:50:59,10-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 8.6042321 Rs exit= 5.6667681 Range altitude= 40140.553 km ... -40577.514,,,,,, 2009-191T04:53:00,000T21:05:13,10-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-191T04:53:00,000T17:59:00,10-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-191T04:53:00,000T17:59:00,10-Jul-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-191T04:53:00,000T13:07:00,10-Jul-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-191T05:35:00,000T06:00:00,10-Jul-09,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-191T05:35:00,000T06:00:00,10-Jul-09,CIRS,SPASS Rider,rings(general),EQLBS,,CIRS_114RI_EQLBS001_SI,,,,,,, 2009-191T05:35:00,000T06:00:00,10-Jul-09,UVIS,SPASS Rider,rings(general),EQLBS,,URSTAR,,,,,,, 2009-191T05:35:00,000T06:00:00,10-Jul-09,VIMS,SPASS Rider,rings(general),EQLBS,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-191T11:35:00,000T08:00:00,10-Jul-09,ISS,Prime,rings(general),AZSCANLIT,,AZSCAN lit,Inner CD/outer B ring group,,,,,, 2009-191T11:35:00,000T08:00:00,10-Jul-09,CIRS,SPASS Rider,rings(general),AZSCANLIT,,CIRS_114RI_AZSCANLIT001_ISS,rider,,,,,, 2009-191T18:00:00,000T07:58:00,10-Jul-09,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 10 kHz high rate data near expected source of 5 kHz narrowband emission (predicted L=8.1, Lat=+/-30",,,,,, 2009-191T19:35:00,000T04:47:00,10-Jul-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-191T19:35:00,000T04:47:00,10-Jul-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_114RI_EQXSHADOW003_ISS,rider,,,,,, 2009-191T19:35:00,000T04:47:00,10-Jul-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-191T22:09:49,000T00:00:01,10-Jul-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.309 Rs, lat = -28 deg, phase = 67 deg",,,,,, 2009-191T22:52:00,000T05:10:00,10-Jul-09,CAPS,SPASS Rider,Saturn,IMVP5,Inner Magnetosphere vertical profile,MAPS IMVP Campaign,MAPS IMVP Campaign,,,,,, 2009-191T22:52:00,000T05:10:00,10-Jul-09,MIMI,SPASS Rider,Saturn,IMVP5,Inner Magnetosphere vertical profile,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Set up MIMI for Inner Magnetospheric Campaign vertical structure measurement at L=4.5-5, near 1200 LT; maximize pitch angle coverage. Corotation flow into -X, Z half-plane, B field in X, Z plane; or Rotate about Z. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells.",,,,,, 2009-191T22:52:00,000T02:20:32,10-Jul-09,MAG,Non-SPASS,Saturn,IMVP5,Inner Magnetosphere vertical profile,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9",,,,,, 2009-192T01:12:32,000T04:00:00,11-Jul-09,MAG,Non-SPASS,Dione,DITAR,Dione targeted flyby,D2 flyby,Monitor magnetic field perturbations and waves to confirm evidence of plasma pickup observed during the sole previous upstream Dione flyby.,,,,,, 2009-192T01:12:32,000T02:49:28,11-Jul-09,MAG,Non-SPASS,Saturn,IMVP5,Inner Magnetosphere vertical profile,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9 Data rate 0 bps, overlaps DITAR request",,,,,, 2009-192T01:43:59,000T00:38:00,11-Jul-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.6731148 Rs exit= 5.7954338 Range altitude= -39506.109 km ... -20143.872,,,,,, 2009-192T01:58:00,000T02:00:00,11-Jul-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-192T01:58:13,000T02:00:00,11-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-192T01:58:59,000T02:00:00,11-Jul-09,CDA,SPASS Rider,DustRAM direction,RPX0070,,CDA RPXing 2009-192T02:58:59 MMH,"RPXing at 5.9320373 Rs, one crossing in each distance segment",,,,,, 2009-192T02:21:59,000T01:14:00,11-Jul-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 5.8026619 Rs exit= 6.0900814 Range altitude= -19064.912 km ... 19832.881,,,,,, 2009-192T03:35:59,000T00:36:00,11-Jul-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 6.0987617 Rs exit= 6.2514099 Range altitude= 20911.891 km ... 39211.256,,,,,, 2009-192T03:58:00,000T10:02:00,11-Jul-09,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 10 kHz high rate data near expected source of 5 kHz narrowband emission (predicted L=8.1, Lat=+/-30",,,,,, 2009-192T03:58:13,000T23:00:00,11-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-192T04:02:00,002T18:50:00,11-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-192T04:02:00,000T07:35:03,11-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-192T04:11:59,007T17:16:01,11-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 6.2606747 Rs exit= 3.9526153 Range altitude= 40284.539 km ... -40472.049,,,,,, 2009-192T05:12:32,002T17:39:28,11-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-192T07:27:00,000T02:56:00,11-Jul-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-192T10:23:00,000T06:00:00,11-Jul-09,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-192T10:23:00,000T06:00:00,11-Jul-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_114RI_EQLBN001_SI,,,,,,, 2009-192T10:23:00,000T06:00:00,11-Jul-09,UVIS,SPASS Rider,rings(general),EQLBS,,URSTAR,,,,,,, 2009-192T10:23:00,000T06:00:00,11-Jul-09,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-192T11:37:03,002T11:14:57,11-Jul-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-192T14:00:00,000T15:51:00,11-Jul-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-192T17:53:00,000T09:00:00,11-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-192T18:53:00,000T08:00:00,11-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09192_SP,rider,,,,,, 2009-193T02:58:13,000T16:23:47,12-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-193T03:15:00,000T02:05:00,12-Jul-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-193T03:15:00,000T02:05:00,12-Jul-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_114RI_MNRNGSHAD005_ISS,rider,,,,,, 2009-193T05:20:00,000T04:40:00,12-Jul-09,UVIS,Prime,Star,URBETLUP,Stellar occultation,URSTAR,,,,,,, 2009-193T05:20:00,000T04:40:00,12-Jul-09,CIRS,SPASS Rider,rings(general),URBETLUP,Stellar occultation,CIRS_114RI_URBETLUP001_UVIS,rider,,,,,, 2009-193T05:51:00,001T17:01:00,12-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-193T10:22:00,000T09:00:00,12-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-193T11:22:00,000T08:00:00,12-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09193_SP,rider,,,,,, 2009-193T19:22:00,000T03:38:00,12-Jul-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-193T19:45:00,000T01:15:00,12-Jul-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 61 range 2.2 Mkm",,,,,, 2009-193T19:45:00,000T01:15:00,12-Jul-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-193T19:45:00,000T01:15:00,12-Jul-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-193T21:00:00,000T09:07:00,12-Jul-09,CIRS,Prime,rings(general),TMAPN45MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-193T21:00:00,000T09:07:00,12-Jul-09,CIRS,SPASS Rider,rings(general),TMAPN45MP,,CIRS_114RI_TMAPN45MP001_SI,,,,,,, 2009-193T21:00:00,000T08:50:00,12-Jul-09,UVIS,SPASS Rider,rings(general),TMAPN45MP,,URSTAR,,,,,,, 2009-193T21:00:00,000T09:07:00,12-Jul-09,VIMS,SPASS Rider,rings(general),TMAPN45MP,,"azimuthal scan, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-193T23:00:00,000T02:00:00,12-Jul-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-194T01:00:00,000T18:07:00,13-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-194T06:07:00,000T00:30:00,13-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-194T06:37:00,000T02:00:00,13-Jul-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-194T06:37:00,000T02:00:00,13-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,SURVEYPTG,MAPS survey/Prime pointing,CIRS_114SA_SURVEYPTG002_CAPS,rider,,,,,, 2009-194T10:07:00,000T09:00:00,13-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-194T11:07:00,000T08:00:00,13-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09194_SP,rider,,,,,, 2009-194T19:07:00,003T23:45:00,13-Jul-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-194T19:25:00,000T00:30:00,13-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-194T19:55:00,000T12:25:00,13-Jul-09,ISS,Prime,RingF,FMOVIEEQX,,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-194T19:55:00,000T12:25:00,13-Jul-09,CIRS,SPASS Rider,RingF,FMOVIEEQX,,CIRS_114RF_FMOVIEEQXG001_ISS,rider,,,,,, 2009-194T19:55:00,000T12:25:00,13-Jul-09,VIMS,SPASS Rider,RingF,FMOVIEEQX,,F Ring movie,Priority 1,,,,,, 2009-194T22:52:00,001T03:47:00,13-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-194T22:52:00,000T15:08:00,13-Jul-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-194T22:52:00,005T06:23:00,13-Jul-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-194T22:52:00,001T18:45:00,13-Jul-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-195T08:20:00,000T09:00:00,14-Jul-09,UVIS,Prime,Star,URLAMSCO,Stellar occultation,URSTAR,,,,,,, 2009-195T08:20:00,000T09:00:00,14-Jul-09,CIRS,SPASS Rider,rings(general),URLAMSCO,Stellar occultation,CIRS_114RI_URLAMSCO001_UVIS,rider,,,,,, 2009-195T14:00:00,004T07:29:00,14-Jul-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-195T17:37:00,000T09:00:00,14-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-195T18:37:00,000T08:00:00,14-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09195_SP,rider,,,,,, 2009-196T02:39:00,001T02:46:00,15-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-196T02:55:00,000T01:24:00,15-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-196T04:19:00,000T03:20:00,15-Jul-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-196T04:19:00,000T03:20:00,15-Jul-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_114RI_MNRNGSHAD012_ISS,rider,,,,,, 2009-196T07:39:00,000T09:41:00,15-Jul-09,CIRS,Prime,rings(general),TMAPN30MP,,Rings TMAP,null,,,,,, 2009-196T07:39:00,000T09:41:00,15-Jul-09,CIRS,SPASS Rider,rings(general),TMAPN30MP,,CIRS_114RI_TMAPN30MP001_SI,,,,,,, 2009-196T07:39:00,000T09:41:00,15-Jul-09,UVIS,SPASS Rider,rings(general),TMAPN30MP,,URSTAR,,,,,,, 2009-196T07:39:00,000T09:41:00,15-Jul-09,VIMS,SPASS Rider,rings(general),TMAPN30MP,,"azimuthal scan, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-196T17:37:00,003T03:51:00,15-Jul-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-196T17:37:00,000T09:00:00,15-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-196T18:37:00,000T08:00:00,15-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09196_SP,rider,,,,,, 2009-197T02:55:00,000T00:30:00,16-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-197T03:25:00,000T02:00:00,16-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-197T03:25:00,000T02:00:00,16-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_114IC_MAGBNDPTG007_CAPS,rider,,,,,, 2009-197T05:25:00,000T11:35:00,16-Jul-09,CIRS,Prime,rings(general),POLARIZ,,CIRS_114RI_POLARIZ197_PRIME;,null,,,,,, 2009-197T05:25:00,001T00:12:00,16-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-197T05:25:00,000T11:35:00,16-Jul-09,CIRS,SPASS Rider,rings(general),POLARIZ,,CIRS_114RI_POLARIZ197_SI,,,,,,, 2009-197T05:25:00,000T11:35:00,16-Jul-09,UVIS,SPASS Rider,rings(general),POLARIZ,,URSTAR,,,,,,, 2009-197T17:22:00,000T09:00:00,16-Jul-09,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS Operational Readiness Test,"Ka-TWTA maintenance; Pointing = n/a. No DSN tracking required, but if BWG is scheduled for downlink, use it to checkout Ka-band.",,,,,, 2009-197T17:22:00,000T09:00:00,16-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-197T18:22:00,000T08:00:00,16-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09197_SP,rider,,,,,, 2009-198T02:40:00,000T01:57:00,17-Jul-09,VIMS,Prime,Star,ALPSCOCAL,Alpha Sco occultation,alpSco Calibration,Miscellaneous calibration experiments using AlpSco; target star to different pixels in star-finding cube.,,,,,, 2009-198T02:40:00,000T03:57:00,17-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,STARCALIB,,CIRS_114IC_STARCALIB001_VIMS,rider,,,,,, 2009-198T04:37:00,000T02:00:00,17-Jul-09,VIMS,Prime,Star,2STARCAL,Stellar calibration,Stellar Calibrations,"Turn to VX Sgr, stare 40 min; turn to eta Sgr (274.4062, -36.7617); stare 40 min; return to Waypoint",,,,,, 2009-198T05:37:00,000T04:00:00,17-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-198T06:37:00,000T02:00:00,17-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-198T06:37:00,000T02:00:00,17-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_114IC_MAGBNDPTG008_CAPS,rider,,,,,, 2009-198T09:37:00,001T07:22:00,17-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-198T09:52:00,000T09:00:00,17-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-198T10:52:00,000T08:00:00,17-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09198_SP,rider,,,,,, 2009-198T18:52:00,000T05:08:00,17-Jul-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-198T19:10:00,000T05:59:00,17-Jul-09,UVIS,Prime,Star,URSIGSGR,Stellar occultation,URSTAR,,,,,,, 2009-198T19:10:00,000T05:59:00,17-Jul-09,CIRS,SPASS Rider,rings(general),URSIGSGR,Stellar occultation,CIRS_114RI_URSIGSGR001_UVIS,rider,,,,,, 2009-199T00:00:00,000T02:00:00,18-Jul-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-199T01:09:00,000T03:21:00,18-Jul-09,ISS,Prime,Saturn,TISATSHAD,,Titan Shadow Images,NAC images of Titan's shadow on Saturn. It is useful for Titan aerosol science and photo-ops. This is a unique geometry that occurs only a few times the XM and not at all in the nominal mission or XXM. Want 5 of 12.,,,,,, 2009-199T02:00:00,000T16:52:00,18-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-199T04:30:00,000T05:00:00,18-Jul-09,CIRS,Prime,rings(general),POLARIZ,,CIRS_114RI_POLARIZ199_PRIME;,null,,,,,, 2009-199T04:30:00,000T05:00:00,18-Jul-09,CIRS,SPASS Rider,rings(general),POLARIZ,,CIRS_114RI_POLARIZ199_SI,,,,,,, 2009-199T04:30:00,000T05:00:00,18-Jul-09,UVIS,SPASS Rider,rings(general),POLARIZ,,URSTAR,,,,,,, 2009-199T09:52:00,000T09:00:00,18-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-199T10:52:00,000T08:00:00,18-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_114IC_DSCAL09199_SP,rider,,,,,, 2009-199T16:59:00,001T09:22:00,18-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-199T18:52:00,000T02:37:00,18-Jul-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-199T19:15:00,000T10:00:00,18-Jul-09,VIMS,Prime,rings(general),HPSPOKE,,"Spoke observation, phase angle 110-130 degrees",Priority 2,,,,,, 2009-199T19:15:00,000T10:00:00,18-Jul-09,CIRS,SPASS Rider,rings(general),HPSPOKE,,CIRS_114RI_HPSPOKE003_VIMS,rider,,,,,, 2009-199T19:15:00,000T10:00:00,18-Jul-09,UVIS,SPASS Rider,rings(general),HPSPOKE,,URSTAR,,,,,,, 2009-199T21:28:00,005T00:23:00,18-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S52,Range enter= 6.2606747 Rs exit= 3.9526153 Range altitude= 40284.539 km ... -40472.049,,,,,, 2009-199T21:28:00,001T04:53:00,18-Jul-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-199T21:29:00,004T04:28:00,18-Jul-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-199T21:29:00,002T21:07:00,18-Jul-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-199T21:29:05,000T00:00:01,18-Jul-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 15.9 d, inc = 44.5 deg, r = 35.192 Rs, phase = 112 deg",,,,,, 2009-200T00:00:00,000T00:34:00,19-Jul-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-200T05:15:00,000T06:45:00,19-Jul-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-200T05:15:00,000T06:45:00,19-Jul-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-200T12:00:00,000T05:00:00,19-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-200T12:00:00,000T05:00:00,19-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_115IC_MAGBNDPTG001_CAPS,rider,,,,,, 2009-200T12:00:00,003T13:57:00,19-Jul-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-200T17:21:00,000T09:00:00,19-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-200T18:21:00,000T08:00:00,19-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09200_SP,rider,,,,,, 2009-201T02:21:00,001T16:15:00,20-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-201T02:21:00,001T16:15:00,20-Jul-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-201T02:45:00,000T06:40:00,20-Jul-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-201T02:45:00,000T06:40:00,20-Jul-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_115RI_SPKMVDFHP001_ISS,rider,,,,,, 2009-201T02:45:00,000T06:40:00,20-Jul-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-201T09:51:00,000T09:00:00,20-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-201T10:51:00,000T08:00:00,20-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09201_SP,rider,,,,,, 2009-201T19:15:00,000T12:51:00,20-Jul-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-201T19:15:00,000T12:51:00,20-Jul-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_115RI_SPKMVDFHP002_ISS,rider,,,,,, 2009-201T19:15:00,000T12:51:00,20-Jul-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-202T09:36:00,000T09:00:00,21-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-202T10:36:00,000T08:00:00,21-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09202_SP,rider,,,,,, 2009-202T18:36:00,000T12:24:00,21-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-202T18:36:00,001T00:00:00,21-Jul-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-202T18:36:00,001T07:21:00,21-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-202T19:10:00,000T01:15:00,21-Jul-09,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 154.1 range 1.4 Mkm",,,,,, 2009-202T19:10:00,000T01:15:00,21-Jul-09,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-202T19:10:00,000T01:15:00,21-Jul-09,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-202T20:25:00,000T10:35:00,21-Jul-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-202T20:25:00,000T10:35:00,21-Jul-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_115RI_SPKMVDFHP003_ISS,rider,,,,,, 2009-202T20:25:00,000T10:35:00,21-Jul-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-203T07:00:00,000T02:00:00,22-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-203T07:00:00,000T02:00:00,22-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-203T07:00:00,000T02:00:00,22-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_115IC_MAGBNDPTG004_CAPS,rider,,,,,, 2009-203T09:00:00,001T12:51:00,22-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-203T09:36:00,000T09:00:00,22-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-203T10:36:00,000T04:00:00,22-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09203_SP,rider,,,,,, 2009-203T18:36:00,001T03:15:00,22-Jul-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-203T19:10:00,000T10:50:00,22-Jul-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-203T19:10:00,000T10:50:00,22-Jul-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_115RI_SPKMVDFHP004_ISS,rider,,,,,, 2009-203T19:10:00,000T10:50:00,22-Jul-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-204T01:57:00,000T19:54:00,23-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-204T01:57:00,000T19:54:00,23-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-204T01:57:00,000T19:54:00,23-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-204T06:00:00,000T09:31:00,23-Jul-09,ISS,Prime,RingE,HPMELR,,E Ring High Phase Observation,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-204T06:00:00,000T09:31:00,23-Jul-09,CIRS,SPASS Rider,RingE,HPMELR,,CIRS_115RE_HPMELR001_ISS,rider,,,,,, 2009-204T15:51:00,000T06:00:00,23-Jul-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-204T15:51:00,000T06:00:00,23-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-204T16:51:00,000T05:00:00,23-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09204_SP,rider,,,,,, 2009-204T21:51:00,000T15:43:03,23-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-204T21:51:00,002T19:24:59,23-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S52,Range enter= 6.2606747 Rs exit= 3.9526153 Range altitude= 40284.539 km ... -40472.049,,,,,, 2009-204T21:51:00,000T00:43:00,23-Jul-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-204T21:51:00,000T13:43:03,23-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-204T21:51:00,000T15:43:03,23-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-204T21:51:00,001T10:30:00,23-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-204T21:56:00,000T00:02:00,23-Jul-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S52 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-204T22:34:00,000T00:07:00,23-Jul-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-204T22:41:00,000T00:05:00,23-Jul-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-204T22:46:00,000T00:33:00,23-Jul-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-204T22:47:07,000T00:46:56,23-Jul-09,ISS,Prime,Titan,NIGHTNAC,ISS lightning / aurora observation,NNA (Nightside NAC Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-204T22:47:07,000T00:46:56,23-Jul-09,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with ISS.,,,,,, 2009-204T22:47:07,000T00:46:56,23-Jul-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Stare at Titan,VIMS ridealong with ISS. Stare at Titan. Phase = 154 deg. Lat/Lon = 26N/127 deg. Template M3.,,,,,, 2009-204T23:19:00,000T00:22:59,23-Jul-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-204T23:34:03,000T03:00:00,23-Jul-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-204T23:34:03,000T03:00:00,23-Jul-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-204T23:34:03,000T03:00:00,23-Jul-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Stare at Titan,VIMS ridealong with CIRS. Stare at Titan. Phase = 154 deg. Lat/Lon = 26N/128 deg. Template M3,,,,,, 2009-204T23:41:59,000T14:52:04,23-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-205T02:34:03,000T03:00:00,24-Jul-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-205T02:34:03,000T03:00:00,24-Jul-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T02:34:03,000T03:00:00,24-Jul-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,VIMS ridealong with CIRS. Stare at Titan. Phase = 154 deg. Lat/Lon = 26N/131 deg. Template N.,,,,,, 2009-205T05:34:03,000T01:00:00,24-Jul-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T05:34:03,000T01:00:00,24-Jul-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS.,,,,,, 2009-205T05:34:03,000T01:00:00,24-Jul-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,VIMS ridealong with ISS. Stare at Titan. Phase = 154 deg. Lat/Lon = 26N/133 deg. Template N.,,,,,, 2009-205T06:34:03,000T04:00:00,24-Jul-09,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-205T06:34:03,000T04:00:00,24-Jul-09,CIRS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-205T06:34:03,000T04:00:00,24-Jul-09,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T06:34:03,000T04:00:00,24-Jul-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS. Limb mapping of Titan. Phase = 154 deg. Lat/Lon = 26N/134 deg. Template R.,,,,,, 2009-205T10:19:03,000T04:56:00,24-Jul-09,RADAR,SPASS Rider,Titan,T59WARMUP,,Warmup for T59,,,,,,, 2009-205T10:34:03,000T03:00:00,24-Jul-09,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional Mapping,Obtain 64x64 cubes of 160 ms. Phase = 155.0 deg. Lat/Lon = 25N/ 138 deg. Template Y.,,,,,, 2009-205T10:34:03,000T03:00:00,24-Jul-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with VIMS.,,,,,, 2009-205T10:34:03,000T02:50:00,24-Jul-09,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T11:34:03,000T08:00:00,24-Jul-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T59 flyby,"T59 is a polar (south), post-dusk close flyby. MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan on the nightside hemisphere/terminator. It will be also a good complement to T52, T53, T54, T55, T56, T57 and T58 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-205T13:34:03,000T01:13:00,24-Jul-09,CAPS,Prime,Titan,TITANPTG,Titan observation,Prime pointing 115TI (T59),Prime pointing 115TI (T59),,,,,, 2009-205T13:34:03,000T01:00:00,24-Jul-09,CAPS,SPASS Rider,Titan,T59INBND,,Inbound 115TI (T59),Inbound 115TI (T59),,,,,, 2009-205T13:34:03,000T01:41:00,24-Jul-09,CIRS,SPASS Rider,Titan,TITANPTG,Titan observation,,Ride along with CAPS.,,,,,, 2009-205T13:34:03,000T01:00:00,24-Jul-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-205T13:34:03,000T01:30:00,24-Jul-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-205T14:34:03,000T02:00:00,24-Jul-09,CAPS,SPASS Rider,Titan,T59CLOSE,,Closest Approach 115TI (T59),Closest Approach 115TI (T59),,,,,, 2009-205T14:34:03,000T02:00:00,24-Jul-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-205T14:34:03,000T00:45:00,24-Jul-09,INMS,Non-SPASS,Titan,TITAN59,,Titan Flyby,Titan observation,,,,,, 2009-205T14:48:03,000T00:27:00,24-Jul-09,CAPS,Prime,Titan,TITANPTG,Titan observation,Prime pointing 115TI (T59),Prime pointing 115TI (T59),,,,,, 2009-205T15:04:03,000T00:34:00,24-Jul-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-205T15:15:03,000T00:34:00,24-Jul-09,RADAR,Prime,Titan,T59RASAR,,T59 Ride-along SAR with INMS at C/A,,,,,,, 2009-205T15:19:03,000T00:30:00,24-Jul-09,INMS,SPASS Rider,Titan,TITAN59,,Titan Flyby,"Prime Titan observation, INMS is cooperating with RADAR. RADAR will deliver the combined INMS/RADAR pointing design.",,,,,, 2009-205T15:38:03,000T00:26:00,24-Jul-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-205T15:49:03,000T00:35:00,24-Jul-09,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2009-205T15:49:03,000T00:35:00,24-Jul-09,CIRS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-205T15:49:03,000T00:45:00,24-Jul-09,INMS,Non-SPASS,Titan,TITAN59,,Titan Flyby,Titan observation,,,,,, 2009-205T15:57:03,000T00:27:00,24-Jul-09,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T15:57:03,000T01:52:00,24-Jul-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping,VIMS ridealong with CIRS. Regional mapping of Titan. Phase = 42 deg. Lat/Lon = 42S/317 deg.,,,,,, 2009-205T16:04:03,000T01:30:00,24-Jul-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-205T16:24:03,000T00:30:00,24-Jul-09,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2009-205T16:24:03,000T00:30:00,24-Jul-09,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-205T16:24:03,000T00:30:00,24-Jul-09,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T16:34:03,000T01:00:00,24-Jul-09,CAPS,SPASS Rider,Titan,T59OUTBND,,Outbound 115TI (T59),Outbound 115TI (T59),,,,,, 2009-205T16:34:03,000T01:00:00,24-Jul-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-205T16:34:03,000T15:25:56,24-Jul-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-205T16:54:03,000T00:55:00,24-Jul-09,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2009-205T16:54:03,000T00:55:00,24-Jul-09,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-205T16:54:03,000T00:55:00,24-Jul-09,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T17:34:03,001T22:07:56,24-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-205T17:34:03,000T14:25:57,24-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-205T17:49:03,000T00:21:05,24-Jul-09,CIRS,SPASS Rider,Titan,TRANS,,,Ride along with SP.,,,,,, 2009-205T17:49:03,000T00:24:00,24-Jul-09,VIMS,SPASS Rider,Titan,TRANS,,Transititon to RWA,VIMS ridealong during RCS/RWA transition. Phase = 23 deg. Lat/Lon = 23S/325 deg.,,,,,, 2009-205T18:10:08,000T02:23:55,24-Jul-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-205T18:13:03,000T02:21:00,24-Jul-09,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T18:13:03,000T02:21:00,24-Jul-09,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan,VIMS ridealong with CIRS. Scan of Titan. Phase = 23 deg. Lat/Lon = 23S/326 deg. Template E.,,,,,, 2009-205T19:34:03,000T12:46:56,24-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-205T20:34:03,000T02:00:00,24-Jul-09,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-205T20:34:03,000T02:00:00,24-Jul-09,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-205T20:34:03,000T02:00:00,24-Jul-09,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-205T20:34:03,000T02:00:00,24-Jul-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS. Limb mapping of Titan. Phase = 21 deg. Lat/Lon = 21S/329 deg. Template F.,,,,,, 2009-205T23:21:00,000T09:00:00,24-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-206T00:21:00,000T08:00:00,25-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09206_SP,rider,,,,,, 2009-206T08:00:00,000T10:30:35,25-Jul-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-206T08:00:00,000T23:37:23,25-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-206T08:20:59,001T03:18:01,25-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-206T08:21:00,000T02:39:00,25-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-206T08:55:00,000T04:55:00,25-Jul-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-206T08:55:00,000T04:55:00,25-Jul-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_115RI_EQXSHADOW001_ISS,rider,,,,,, 2009-206T08:55:00,000T04:55:00,25-Jul-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-206T11:00:00,002T10:09:00,25-Jul-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-206T13:50:00,000T03:30:00,25-Jul-09,VIMS,Prime,rings(general),COMPHILIT,High phase sunlit ring radial scan,Ring COMPHILIT,Do 4 at priority 1.,,,,,, 2009-206T13:50:00,000T03:30:00,25-Jul-09,CIRS,SPASS Rider,rings(general),COMPHILIT,High phase sunlit ring radial scan,CIRS_115RI_COMPHILIT001_VIMS,rider,,,,,, 2009-206T17:20:00,000T06:00:00,25-Jul-09,CIRS,Prime,rings(general),EQLBS,,CIRS_115RI_EQLBS001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-206T17:20:00,000T06:00:00,25-Jul-09,CIRS,SPASS Rider,rings(general),EQLBS,,CIRS_115RI_EQLBS001_SI,,,,,,, 2009-206T17:20:00,000T06:00:00,25-Jul-09,VIMS,SPASS Rider,rings(general),EQLBS,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-206T18:30:35,000T23:00:00,25-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-207T00:05:00,000T07:30:00,26-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-207T01:05:00,000T03:15:00,26-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09205_SP,rider,,,,,, 2009-207T06:00:00,000T08:00:00,26-Jul-09,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 10 kHz high rate data near expected source of 5 kHz narrowband emission (predicted L=8.1, Lat=+/-30",,,,,, 2009-207T07:37:23,000T08:04:37,26-Jul-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-207T08:25:00,000T07:35:00,26-Jul-09,ISS,Prime,rings(general),AZSCANLIT,,AZSCAN lit,AZSCAN of Strange ringlet to get vertical relief information.,,,,,, 2009-207T08:25:00,000T07:35:00,26-Jul-09,CIRS,SPASS Rider,rings(general),AZSCAN,Azimuthal ring scan,CIRS_115RI_AZSCAN001_ISS,rider,,,,,, 2009-207T11:39:00,000T07:22:00,26-Jul-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-207T14:00:00,000T04:00:00,26-Jul-09,RPWS,Non-SPASS,Saturn,NBANDHI,,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 80 kHz high rate data near expected source of 20 kHz narrowband emission (predicted L=4.2, Lat=+/-20",,,,,, 2009-207T15:42:00,000T03:40:00,26-Jul-09,CAPS,SPASS Rider,Saturn,IMVP3,,MAPS IMVP Campaign,MAPS IMVP Campaign,,,,,, 2009-207T15:42:00,000T03:40:00,26-Jul-09,MAG,Non-SPASS,Saturn,IMVP3,,MAG MAPS IM_VP Campaign,"Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L-shells at a variety of local times and L-shells. IMVP are 30 deg of latitude centered on dL/dlat = 0, when that point is within 10 deg of the equator. L~9 Data rate 0 bps, overlaps INTFLD request.",,,,,, 2009-207T15:42:00,000T03:40:00,26-Jul-09,MIMI,Non-SPASS,Saturn,IMVP3,,MIMI Inner Magnetosphere Vertical Profile,"Setup MIMI for inner magnetosphere vertical equatorial plane crossing observations, any OPMODE or TLM mode.",,,,,, 2009-207T15:42:00,000T03:40:00,26-Jul-09,RPWS,Non-SPASS,co-rotation,IMVP3,,MAPS IM/VP Campaign,"Part of IM/VP MAPS Campaign. Measure the vertical structure and dynamics of the inner magnetosphere on orbits nearly tangent to L shells, at a variety of local times and L shells",,,,,, 2009-207T16:00:00,000T02:00:00,26-Jul-09,CIRS,Prime,Janus,FP3JANUS,,CIRS_115JA_FP3JANUS002_PRIME;,"1.9 MRAD; 64 PHASE; (-46, 25), 08;LT 10 MIN TURNS.",,,,,, 2009-207T16:00:00,000T02:00:00,26-Jul-09,ISS,SPASS Rider,Janus,FP3JANUS,,Janus close flyby,"Janus close flyby, ~94,000 km at CA, 60 deg phase",,,,,, 2009-207T16:00:00,000T02:00:00,26-Jul-09,UVIS,SPASS Rider,Janus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-207T16:00:00,000T02:00:00,26-Jul-09,VIMS,SPASS Rider,Janus,ROTCOLR,,Janus,multiple 16/640 ms.,,,,,, 2009-207T16:04:01,000T00:00:01,26-Jul-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.865 Rs, lat = -19 deg, phase = 65 deg",,,,,, 2009-207T16:15:00,000T02:46:00,26-Jul-09,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE2 flyby,"Monitor the interaction of Tethys with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD & IM/VP requests.",,,,,, 2009-207T17:15:59,000T00:38:00,26-Jul-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9573118 Rs exit= 4.0621272 Range altitude= -39421.324 km ... -20281.667,,,,,, 2009-207T17:30:35,000T02:00:00,26-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-207T17:30:59,000T02:00:00,26-Jul-09,CDA,SPASS Rider,DustRAM direction,RPX0080,,CDA RPXing 2009-207T18:30:59 MMH,"RPXing at 4.2023077 Rs, one crossing in each distance segment",,,,,, 2009-207T17:53:59,000T01:14:00,26-Jul-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.0690305 Rs exit= 4.3832191 Range altitude= -19208.708 km ... 19582.940,,,,,, 2009-207T18:00:00,000T01:50:00,26-Jul-09,ISS,Prime,Enceladus,PLMMP,,Plume Obs. while Enceladus in Rhea's shadow,Plume obs. while Enceladus is eclipsed by Rhea. Intermed. phase obs. LIEN,,,,,, 2009-207T18:00:00,000T01:50:00,26-Jul-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-207T18:00:00,000T01:50:00,26-Jul-09,VIMS,SPASS Rider,Enceladus,PLMMP,,,null,,,,,, 2009-207T18:00:00,000T01:32:00,26-Jul-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-207T19:01:00,000T01:14:00,26-Jul-09,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE2 flyby,Monitor the interaction of Tethys with the Saturnian magnetosphere.,,,,,, 2009-207T19:07:59,000T00:38:00,26-Jul-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.3935678 Rs exit= 4.5921471 Range altitude= 20656.616 km ... 39853.935,,,,,, 2009-207T19:22:00,002T15:05:00,26-Jul-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-207T19:22:00,000T06:58:54,26-Jul-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-207T19:30:35,000T23:00:00,26-Jul-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-207T19:32:00,000T08:00:00,26-Jul-09,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 10 kHz high rate data near expected source of 5 kHz narrowband emission (predicted L=8.1, Lat=+/-30",,,,,, 2009-207T19:45:59,007T19:37:01,26-Jul-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 4.6038113 Rs exit= 2.9513262 Range altitude= 40911.816 km ... -40154.047,,,,,, 2009-207T19:50:00,000T03:40:00,26-Jul-09,VIMS,Prime,rings(general),COMPLODRK,Low phase dark side ring radial scan,"Hi res radial scan, dark side",Priority 1,,,,,, 2009-207T19:50:00,000T03:40:00,26-Jul-09,CIRS,SPASS Rider,rings(general),COMPLODRK,Low phase dark side ring radial scan,CIRS_115RI_COMPLODRK001_VIMS,rider,,,,,, 2009-207T20:15:00,002T14:12:00,26-Jul-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-208T00:05:00,000T08:46:00,27-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-208T01:05:00,000T03:30:00,27-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09208_SP,rider,,,,,, 2009-208T02:20:54,002T08:06:06,27-Jul-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-208T08:51:00,000T01:20:00,27-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_115IC_DEEPSPACE001_NAV,rider,,,,,, 2009-208T10:12:00,000T07:08:00,27-Jul-09,CIRS,Prime,rings(general),EQLBN,,CIRS_115RI_EQLBN001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-208T10:12:00,000T07:08:00,27-Jul-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_115RI_EQLBN001_SI,,,,,,, 2009-208T10:12:00,000T07:08:00,27-Jul-09,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-208T17:20:00,000T04:00:00,27-Jul-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-208T17:20:00,000T04:00:00,27-Jul-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_115RI_MNRNGSHAD003_ISS,rider,,,,,, 2009-208T18:30:35,000T23:50:25,27-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-208T21:09:00,006T18:14:00,27-Jul-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-208T21:20:00,000T06:43:00,27-Jul-09,VIMS,Prime,rings(general),ALPSCOOCC,Alpha Sco occultation,Ring stellar occ - alpSco,"alpSco occultation, F-B rings, R0=2.349, Rf=1.43, Rmin-1.43",,,,,, 2009-208T21:20:00,000T06:43:00,27-Jul-09,CIRS,SPASS Rider,rings(general),ALPSCOOCC,Alpha Sco occultation,CIRS_115RI_ALPSCOOCC101_VIMS,rider,,,,,, 2009-209T04:03:00,000T05:02:00,28-Jul-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-209T04:03:00,000T05:02:00,28-Jul-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_115RI_MNRNGSHAD004_ISS,rider,,,,,, 2009-209T09:21:00,000T09:00:00,28-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-209T10:21:00,000T04:00:00,28-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09209_SP,rider,,,,,, 2009-209T18:21:00,000T01:39:00,28-Jul-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-209T18:35:00,000T12:31:00,28-Jul-09,ISS,Prime,RingF,FRSTRCHAN,F ring streamer movie,F RING STREAMER/CHANNEL,"Movie of streamer-channel feature raised in F ring by Prometheus apoapse passage. Need as close to 1 Prom orbital period as possible. Sometimes can be day before or day after. Want 12. 6 of 49 as priority 1, 6 of 49 as priority 2.",,,,,, 2009-209T18:35:00,000T12:31:00,28-Jul-09,CIRS,SPASS Rider,rings(general),FRSTRCHAN,F ring streamer movie,CIRS_115RI_FRSTRCHAN001_ISS,rider,,,,,, 2009-209T20:00:00,000T02:00:00,28-Jul-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-209T22:00:00,000T20:06:00,28-Jul-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-210T07:06:00,000T00:30:00,29-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-210T09:06:00,000T09:00:00,29-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-210T10:06:00,000T04:00:00,29-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09210_SP,rider,,,,,, 2009-210T10:27:00,009T15:25:00,29-Jul-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-210T10:27:00,005T04:56:00,29-Jul-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-210T10:27:00,009T15:18:00,29-Jul-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-210T18:06:00,003T07:29:00,29-Jul-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-210T18:46:00,000T01:15:00,29-Jul-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86.1 range 2.7 Mkm",,,,,, 2009-210T18:46:00,000T01:15:00,29-Jul-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-210T18:46:00,000T01:15:00,29-Jul-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-210T20:01:00,000T05:00:00,29-Jul-09,ISS,Prime,rings(general),MNRNGSHAD,,Moon Shadows on Rings,"Moon Shadows on Rings. Actual start time and duration will be determined by ultimate purpose of observation: measurements, high res photo ops, low res photo ops, movies, etc. Need 50, want 70. 40-minute turns included, cannot be shifted.",,,,,, 2009-210T20:01:00,000T05:00:00,29-Jul-09,CIRS,SPASS Rider,rings(general),MNRNGSHAD,,CIRS_115RI_MNRNGSHAD005_ISS,rider,,,,,, 2009-211T01:01:00,000T12:49:00,30-Jul-09,ISS,Prime,RingF,FMOVIEEQX,,Long Medium Res F Ring Movie,"Medium Resolution F Ring Movie. This can be an ansa stare, an azimuthal scan or other design. There is often some flexibility in placement - can often be the day before or day after. Want at least 12 during XM. 6 of 61 priority 1, 6 of 61 priority 2",,,,,, 2009-211T01:01:00,000T12:49:00,30-Jul-09,CIRS,SPASS Rider,rings(general),FMOVIEEQX,,CIRS_115RI_FMOVIEEQX001_ISS,rider,,,,,, 2009-211T01:01:00,000T12:49:00,30-Jul-09,VIMS,SPASS Rider,RingF,FMOVIEEQX,,F Ring movie,Priority 1,,,,,, 2009-211T13:50:00,000T00:30:00,30-Jul-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-211T14:20:00,000T02:00:00,30-Jul-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-211T16:35:00,000T09:00:00,30-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-211T17:35:00,000T04:00:00,30-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09211_SP,rider,,,,,, 2009-212T01:55:00,000T04:25:00,31-Jul-09,CIRS,Prime,rings(general),TMAPN25MP,,CIRS_115RI_TMAPN25MP001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-212T01:55:00,000T04:25:00,31-Jul-09,CIRS,SPASS Rider,rings(general),TMAPN25MP,,CIRS_115RI_TMAPN25MP001_SI,,,,,,, 2009-212T01:55:00,000T04:25:00,31-Jul-09,VIMS,SPASS Rider,rings(general),TMAPN25MP,,"azimuthal scan, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-212T06:20:00,000T09:55:00,31-Jul-09,UVIS,Prime,Star,URMUSGR,,URSTAR,,,,,,, 2009-212T06:20:00,000T09:55:00,31-Jul-09,CIRS,SPASS Rider,rings(general),URMUSGR,,CIRS_115RI_URMUSGR001_UVIS,rider,,,,,, 2009-212T16:35:00,000T09:00:00,31-Jul-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-212T17:35:00,000T08:00:00,31-Jul-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09212_SP,rider,,,,,, 2009-213T01:55:00,000T12:20:00,1-Aug-09,VIMS,Prime,Star,6STARCAL,,Stellar Calibrations,"turn to alpCen; stare 2 hr; turn to next star & stare for 2 hr, etc.; return to Waypt. RWA needed. Additional stars (in order): gamCru, etaCar, R_Car, epsMus, alpTrA.",,,,,, 2009-213T14:15:00,000T02:00:00,1-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-213T14:15:00,000T02:00:00,1-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_115IC_DEEPSPACE002_CAPS,rider,,,,,, 2009-213T16:35:00,000T09:00:00,1-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-213T17:35:00,000T08:00:00,1-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09213_SP,rider,,,,,, 2009-214T01:35:00,000T01:25:00,2-Aug-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-214T01:55:00,000T11:10:00,2-Aug-09,VIMS,Prime,rings(general),HPSPOKE,,Spoke observation,Priority 2,,,,,, 2009-214T01:55:00,000T11:10:00,2-Aug-09,CIRS,SPASS Rider,rings(general),HPSPOKE,,CIRS_115RI_HPSPOKE001_VIMS,rider,,,,,, 2009-214T03:00:00,000T02:00:00,2-Aug-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-214T05:00:00,000T20:20:00,2-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-214T13:05:00,000T02:00:00,2-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-214T13:05:00,000T02:00:00,2-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_115IC_DEEPSPACE003_CAPS,rider,,,,,, 2009-214T16:20:00,000T09:00:00,2-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-214T17:20:00,000T08:00:00,2-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_115IC_DSCAL09214_SP,rider,,,,,, 2009-215T00:00:00,000T00:34:00,3-Aug-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-215T01:20:00,000T14:03:00,3-Aug-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-215T01:40:00,000T02:19:00,3-Aug-09,ISS,Prime,Saturn,TISATSHAD,,Titan Shadow Images,NAC images of Titan's shadow on Saturn. It is useful for Titan aerosol science and photo-ops. This is a unique geometry that occurs only a few times the XM and not at all in the nominal mission or XXM. Want 5 of 12.,,,,,, 2009-215T03:59:00,000T10:01:00,3-Aug-09,CIRS,Prime,rings(general),POLARIZ,,CIRS_115RI_POLARIZ215_PRIME;,null,,,,,, 2009-215T03:59:00,000T10:01:00,3-Aug-09,CIRS,SPASS Rider,rings(general),POLARIZ,,CIRS_115RI_POLARIZ215_SI,,,,,,, 2009-215T14:00:00,000T02:00:00,3-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-215T14:00:00,000T02:00:00,3-Aug-09,CIRS,SPASS Rider,SpacecraftRAM direction,DEEPSPACE,Deep space calibration,CIRS_115SRI_DEEPSPACE004_CAPS,rider,,,,,, 2009-215T15:23:00,004T10:29:00,3-Aug-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-215T15:23:00,007T19:52:59,3-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 4.6038113 Rs exit= 2.9513262 Range altitude= 40911.816 km ... -40154.047,,,,,, 2009-215T15:23:00,003T09:42:00,3-Aug-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-215T15:23:00,005T09:42:00,3-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-215T15:23:19,000T00:00:01,3-Aug-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 15.9 d, inc = 34.7 deg, r = 36.638 Rs, phase = 115 deg",,,,,, 2009-215T16:20:00,000T09:00:00,3-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-215T17:20:00,000T08:00:00,3-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09215_SP,rider,,,,,, 2009-216T01:40:00,000T14:20:00,4-Aug-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-216T01:40:00,000T14:20:00,4-Aug-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_116RI_SPKMVDFHP001_ISS,rider,,,,,, 2009-216T01:40:00,000T14:20:00,4-Aug-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-216T16:20:00,000T09:00:00,4-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-216T18:20:00,000T07:00:00,4-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09216_SP,rider,,,,,, 2009-217T02:20:00,000T13:35:00,5-Aug-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-217T02:20:00,000T13:35:00,5-Aug-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_116RI_SPKMVDFHP002_ISS,rider,,,,,, 2009-217T02:20:00,000T13:35:00,5-Aug-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-217T16:20:00,000T09:00:00,5-Aug-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-217T16:20:00,000T09:00:00,5-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-217T17:20:00,000T04:00:00,5-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09217_SP,rider,,,,,, 2009-218T01:45:00,000T02:00:00,6-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-218T01:45:00,000T02:00:00,6-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DEEPSPACE,Deep space calibration,CIRS_116IC_DEEPSPACE005_CAPS,rider,,,,,, 2009-218T03:45:00,000T10:50:00,6-Aug-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-218T03:45:00,000T10:50:00,6-Aug-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_116RI_SPKMVDFHP003_ISS,rider,,,,,, 2009-218T03:45:00,000T10:50:00,6-Aug-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-218T16:05:00,000T09:00:00,6-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-218T17:05:00,000T04:00:00,6-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09218_SP,rider,,,,,, 2009-219T01:05:00,001T00:00:00,7-Aug-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-219T01:45:00,000T01:15:00,7-Aug-09,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 160.3 range 1.3 Mkm",,,,,, 2009-219T01:45:00,000T01:15:00,7-Aug-09,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-219T01:45:00,000T01:15:00,7-Aug-09,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-219T03:00:00,000T12:25:00,7-Aug-09,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-219T03:00:00,000T12:25:00,7-Aug-09,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,CIRS_116RI_SPKMVDFHP004_ISS,rider,,,,,, 2009-219T03:00:00,000T12:25:00,7-Aug-09,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face",ISS rider,,,,,, 2009-219T16:05:00,000T09:00:00,7-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-219T17:05:00,000T04:00:00,7-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09219_SP,rider,,,,,, 2009-220T01:05:00,001T00:00:00,8-Aug-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-220T01:45:00,000T06:45:00,8-Aug-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-220T01:45:00,000T00:07:00,8-Aug-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-220T01:52:00,001T10:11:53,8-Aug-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-220T01:52:00,000T23:13:00,8-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-220T08:30:00,000T07:10:00,8-Aug-09,ISS,Prime,Saturn,NALGTNG,,Lightning/E-ring in CL1 in NAC from ~20-30Rs,"Day WAC/night NAC comparison. Night: Up to 10 min exposures.I/F ~ 1e-4 to 1e-5, CL1, 12 bit, uncompressed. Day:CB2,table,lossy compression. 1 night image per 10 minutes plus a few dayside (not counted in NImages, but in 4.2 Mb/night image)",,,,,, 2009-220T08:30:00,000T02:10:00,8-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-220T10:40:00,000T05:00:00,8-Aug-09,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2009-220T15:40:00,000T09:25:00,8-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-220T16:05:00,000T09:00:00,8-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-220T17:05:00,000T04:00:00,8-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09220_SP,rider,,,,,, 2009-221T01:05:00,000T11:58:53,9-Aug-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-221T01:05:00,000T08:58:53,9-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-221T01:05:00,000T10:58:53,9-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-221T01:05:00,001T01:00:00,9-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-221T02:01:49,000T02:02:04,9-Aug-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,CIRS_116TI_FIRNADCMP_001,"Obtain information on trace constituents in Titan's stratosphere. Integrate on limb at two positions POINTING: Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5-2.0. POINTING: -y to Titan, x away from sun.",,,,,, 2009-221T02:01:49,000T02:02:04,9-Aug-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-221T02:01:49,000T02:02:04,9-Aug-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-221T02:01:49,000T02:02:04,9-Aug-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,VIMS ridealong with CIRS. Stare at Titan. Phase = 162 deg. Lat/Lon = 18N/134 deg. Template N.,,,,,, 2009-221T04:03:53,000T01:00:00,9-Aug-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-221T04:03:53,000T01:00:00,9-Aug-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS.,,,,,, 2009-221T04:03:53,000T01:00:00,9-Aug-09,UVIS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Rider ro ISS PHOTOMWAC,Stare at Titan,,,,,, 2009-221T04:03:53,000T01:00:00,9-Aug-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,VIMS ridealong with ISS. Stare at Titan. Phase = 162 deg. Lat/Lon = 18N/136 deg. Template N.,,,,,, 2009-221T05:03:53,000T03:50:00,9-Aug-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-221T05:03:53,000T03:50:00,9-Aug-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2009-221T05:03:53,000T03:50:00,9-Aug-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-221T05:03:53,000T03:50:00,9-Aug-09,RADAR,SPASS Rider,Titan,T60WARMUP,,Warmup for T60,,,,,,, 2009-221T05:03:53,000T03:50:00,9-Aug-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan,VIMS ridealong with UVIS. Slow scan across Titan. Phase = 162 deg. Lat/Lon = 18N/137 deg. Template P.,,,,,, 2009-221T08:53:53,000T03:10:00,9-Aug-09,RADAR,Prime,Titan,T60INRAD,,T60 Inbound Radiometry,,,,,,, 2009-221T10:03:53,000T08:00:00,9-Aug-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T60 flyby,"T60 is similar to T59. MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan on the nightside hemisphere/terminator. It will be also a good complement to T52, T53, T54, T55, T56, T57, T58 and T59 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-221T12:03:53,000T00:48:00,9-Aug-09,RADAR,Prime,Titan,T60INSCAT,,T60 Inbound Scatterometry,,,,,,, 2009-221T12:03:53,000T01:00:00,9-Aug-09,CAPS,SPASS Rider,Titan,T60INBND,,Inbound 116TI (T60),Inbound 116TI (T60),,,,,, 2009-221T12:03:53,000T01:00:00,9-Aug-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-221T12:03:53,000T01:30:00,9-Aug-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-221T12:52:53,000T00:41:00,9-Aug-09,RADAR,Prime,Titan,T60IHISAR,,T60 Inbound HiSAR,,,,,,, 2009-221T13:03:53,000T02:00:00,9-Aug-09,CAPS,SPASS Rider,Titan,T60CLOSE,,Closest Approach 116TI (T60),Closest Approach 116TI (T60),,,,,, 2009-221T13:03:53,000T02:00:00,9-Aug-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-221T13:03:53,000T00:40:00,9-Aug-09,INMS,Non-SPASS,Titan,TITAN60,,Titan Flyby,Titan observation,,,,,, 2009-221T13:33:53,000T00:12:00,9-Aug-09,RADAR,Prime,Titan,T60INALT,,T60 Inbound Altimetry,,,,,,, 2009-221T13:33:53,000T01:00:00,9-Aug-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-221T13:43:53,000T00:40:00,9-Aug-09,INMS,Non-SPASS,Titan,TITAN60,,Titan Flyby,Titan observation,,,,,, 2009-221T13:45:53,000T00:44:00,9-Aug-09,RADAR,Prime,Titan,T60INOSAR,,T60 Inbound and Outbound SAR,,,,,,, 2009-221T14:23:53,000T00:40:00,9-Aug-09,INMS,Non-SPASS,Titan,TITAN60,,Titan Flyby,Titan observation,,,,,, 2009-221T14:29:53,000T00:22:00,9-Aug-09,CIRS,SPASS Rider,Titan,TRANS,,,Ride along with SP.,,,,,, 2009-221T14:29:53,000T00:22:00,9-Aug-09,ISS,SPASS Rider,SpacecraftActivity,DFPWBIAS,,(TNI) Transition NAC Imaging,viewing during RCS/RWA transition,,,,,, 2009-221T14:29:53,000T00:21:05,9-Aug-09,VIMS,SPASS Rider,Titan,TRANS,,Transition to RWA,VIMS ridealong during RCS/RWA transition. Phase = 34 deg. Lat/Lon = 34S/322 deg.,,,,,, 2009-221T14:33:53,000T01:30:00,9-Aug-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-221T14:51:53,000T01:19:56,9-Aug-09,ISS,Prime,Titan,REGMAP,Regional mapping,NRM (NAC Regional Mapping),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-221T14:51:53,000T01:19:56,9-Aug-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS.,,,,,, 2009-221T14:51:53,000T01:19:56,9-Aug-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping,VIMS ridealong with ISS for regional mapping. Phase = 23 deg. Lat/Lon = 23S/324 deg. Check ISS dwell time of 6 minutes,,,,,, 2009-221T15:03:53,000T01:00:00,9-Aug-09,CAPS,SPASS Rider,Titan,T60OUTBND,,Outbound 116TI (T60),Outbound 116TI (T60),,,,,, 2009-221T15:03:53,000T01:00:00,9-Aug-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-221T15:03:53,000T10:56:06,9-Aug-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-221T16:03:53,002T22:48:06,9-Aug-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-221T16:03:53,000T09:56:06,9-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-221T17:05:00,000T09:00:00,9-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-221T18:03:53,000T08:01:07,9-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-221T18:05:00,000T08:00:00,9-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09221_SP,rider,,,,,, 2009-222T02:00:00,000T10:58:59,10-Aug-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-222T02:00:00,002T12:52:00,10-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-222T02:05:00,001T04:57:00,10-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-222T02:05:00,000T06:18:00,10-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-222T02:35:00,000T06:00:00,10-Aug-09,ISS,Prime,rings(general),SHADBNDLE,,Shadow boundary in the E and G Rings at low elevat,Shadow boundary in the E and G Rings at low elevation angle,,,,,, 2009-222T02:35:00,000T06:00:00,10-Aug-09,CIRS,SPASS Rider,rings(general),SHADBNDLE,,CIRS_116RI_SHADBNDLE001_ISS,rider,,,,,, 2009-222T08:23:00,002T06:29:00,10-Aug-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-222T08:35:00,000T03:00:00,10-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-222T08:35:00,000T03:00:00,10-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_116RI_EQXSHADOW001_ISS,rider,,,,,, 2009-222T08:35:00,000T03:00:00,10-Aug-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-222T11:35:00,000T03:55:00,10-Aug-09,VIMS,Prime,rings(general),HIPHASE,High phase observation,High phase rings,"5x1 mosaic, right ansa, 640 msec",,,,,, 2009-222T11:35:00,000T03:55:00,10-Aug-09,CIRS,SPASS Rider,rings(general),HIPHASE,High phase observation,CIRS_116RI_HIPHASE001_VIMS,rider,,,,,, 2009-222T11:35:00,000T03:55:00,10-Aug-09,ISS,SPASS Rider,rings(general),HIPHASE,High phase observation,Spoke Periodicity Monitoring,WACS of B ring to search for spokes,,,,,, 2009-222T11:35:00,000T03:55:00,10-Aug-09,UVIS,SPASS Rider,rings(general),HIPHASE,High phase observation,URSPEC,,,,,,, 2009-222T12:58:59,000T23:00:00,10-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-222T16:04:00,000T09:00:00,10-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-222T17:04:00,000T08:00:00,10-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09222_SP,rider,,,,,, 2009-223T01:00:00,000T04:00:00,11-Aug-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-223T01:35:00,000T05:00:00,11-Aug-09,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-223T01:35:00,000T05:00:00,11-Aug-09,CIRS,SPASS Rider,rings(general),EQLBS,,CIRS_116RI_EQLBS001_SI,,,,,,, 2009-223T01:35:00,000T05:00:00,11-Aug-09,ISS,SPASS Rider,rings(general),EQLBS,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes as well as support imaging for CIRS,,,,,, 2009-223T01:35:00,000T05:00:00,11-Aug-09,VIMS,SPASS Rider,rings(general),EQLBS,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-223T05:00:00,000T06:00:00,11-Aug-09,RPWS,Non-SPASS,Saturn,NBANDHI,,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 80 kHz high rate data near expected source of 20 kHz narrowband emission (predicted L=4.2, Lat=+/-20",,,,,, 2009-223T06:35:00,000T05:25:00,11-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-223T06:35:00,000T05:25:00,11-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_116RI_EQXSHADOW005_ISS,rider,,,,,, 2009-223T06:35:00,000T05:25:00,11-Aug-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-223T07:02:00,000T08:59:00,11-Aug-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-223T11:00:00,000T08:00:00,11-Aug-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-223T11:15:59,000T00:52:00,11-Aug-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 2.9487388 Rs exit= 2.9638526 Range altitude= -39449.884 km ... -20765.693,,,,,, 2009-223T11:36:57,000T00:00:01,11-Aug-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.933 Rs, lat = -10 deg, phase = 63 deg",,,,,, 2009-223T11:37:00,000T00:15:00,11-Aug-09,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2009-223T11:58:59,000T02:00:00,11-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-223T12:00:00,000T02:00:00,11-Aug-09,CDA,Prime,DustRAM direction,RPX0090,,CDA RPXing 2009-223T13:00:59 MMH,"RPXing at 3.1344180 Rs, one crossing in each distance segment",,,,,, 2009-223T12:07:59,000T01:42:00,11-Aug-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 2.9676246 Rs exit= 3.4176997 Range altitude= -19983.908 km ... 19972.309,,,,,, 2009-223T12:59:00,000T02:00:00,11-Aug-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-223T13:49:59,000T00:52:00,11-Aug-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.4309265 Rs exit= 3.7965396 Range altitude= 20760.288 km ... 39969.197,,,,,, 2009-223T13:58:59,000T23:00:00,11-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-223T14:00:00,000T03:00:00,11-Aug-09,UVIS,Prime,Star,URALPVIR,Stellar occultation,URSTAR,Ingress occ of very bright star at low incidence angle. Gives atmospheric occultation at end of ring occ.,,,,,, 2009-223T14:00:00,000T03:00:00,11-Aug-09,CIRS,SPASS Rider,rings(general),URALPVIR,Stellar occultation,CIRS_116RI_URALPVIR002_UVIS,rider,,,,,, 2009-223T14:41:59,007T20:26:01,11-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.8123311 Rs exit= 16.010420 Range altitude= 40715.420 km ... -33434.979,,,,,, 2009-223T16:01:00,000T22:51:00,11-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-223T17:34:00,000T06:00:00,11-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-223T18:34:00,000T05:00:00,11-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09223_SP,rider,,,,,, 2009-223T19:00:00,000T04:00:00,11-Aug-09,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Campaign,"Part of RPWS Narrow Band Emission campaign, attempt to get 10 kHz high rate data near expected source of 5 kHz narrowband emission (predicted L=8.1, Lat=+/-30",,,,,, 2009-223T23:55:00,000T03:05:00,11-Aug-09,VIMS,Prime,rings(general),POSTEQX,,Equinox observation,Priority 1,,,,,, 2009-223T23:55:00,000T03:05:00,11-Aug-09,CIRS,SPASS Rider,rings(general),POSTEQX,,CIRS_116RI_POSTEQX001_VIMS,rider,,,,,, 2009-223T23:55:00,000T03:05:00,11-Aug-09,UVIS,SPASS Rider,rings(general),POSTEQX,,URSPEC,,,,,,, 2009-224T03:00:00,000T03:00:00,12-Aug-09,CIRS,Prime,rings(general),EQSBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-224T03:00:00,000T03:00:00,12-Aug-09,CIRS,SPASS Rider,rings(general),EQSBS,,CIRS_116RI_EQSBS001_SI,,,,,,, 2009-224T03:00:00,000T03:00:00,12-Aug-09,UVIS,SPASS Rider,rings(general),EQSBS,,URSPEC,,,,,,, 2009-224T03:00:00,000T03:00:00,12-Aug-09,VIMS,SPASS Rider,rings(general),EQSBS,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-224T06:00:00,000T08:34:00,12-Aug-09,ISS,Prime,rings(general),EQXMOSAIC,,Equinox Mosaic,Mosaic of the rings during equinox,,,,,, 2009-224T06:00:00,000T08:34:00,12-Aug-09,CIRS,SPASS Rider,rings(general),EQXMOSAIC,,CIRS_116RI_EQXMOSAIC001_ISS,rider,,,,,, 2009-224T12:58:59,001T11:50:01,12-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-224T14:52:00,001T11:10:00,12-Aug-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-224T14:52:00,001T11:10:00,12-Aug-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-224T14:52:00,000T14:08:00,12-Aug-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-224T14:52:00,006T20:16:00,12-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-224T14:52:00,001T11:10:00,12-Aug-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-224T15:49:00,000T09:00:00,12-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-224T16:49:00,000T08:00:00,12-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09224_SP,rider,,,,,, 2009-225T01:00:00,000T01:15:00,13-Aug-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 60.6 range 2.2 Mkm",,,,,, 2009-225T01:00:00,000T01:15:00,13-Aug-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-225T01:00:00,000T01:15:00,13-Aug-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-225T02:15:00,000T06:00:00,13-Aug-09,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-225T02:15:00,000T06:00:00,13-Aug-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_116RI_EQLBN001_SI,,,,,,, 2009-225T02:15:00,000T06:00:00,13-Aug-09,UVIS,SPASS Rider,rings(general),EQLBN,,URSPEC,,,,,,, 2009-225T02:15:00,000T06:00:00,13-Aug-09,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-225T05:00:00,000T21:02:00,13-Aug-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-225T08:15:00,000T00:30:00,13-Aug-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-225T08:45:00,000T06:30:00,13-Aug-09,CIRS,Prime,rings(general),TMAPN20MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-225T08:45:00,000T06:30:00,13-Aug-09,CIRS,SPASS Rider,rings(general),TMAPN20MP,,CIRS_116RI_TMAPN20MP001_SI,,,,,,, 2009-225T08:45:00,000T06:30:00,13-Aug-09,UVIS,SPASS Rider,rings(general),TMAPN20MP,,URSPEC,,,,,,, 2009-225T08:45:00,000T06:30:00,13-Aug-09,VIMS,SPASS Rider,rings(general),TMAPN20MP,,"azimuthal scan, unlit side","320 ms, 64*12 cubes?",,,,,, 2009-225T15:49:00,000T09:00:00,13-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-225T16:49:00,000T08:00:00,13-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09225_SP,rider,,,,,, 2009-226T00:49:00,000T01:11:00,14-Aug-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-226T01:20:00,000T01:15:00,14-Aug-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 79.6 range 2.6 Mkm",,,,,, 2009-226T01:20:00,000T01:15:00,14-Aug-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-226T01:20:00,000T01:15:00,14-Aug-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-226T02:00:00,000T02:00:00,14-Aug-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-226T02:02:00,002T19:45:00,14-Aug-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-226T02:02:00,005T09:06:00,14-Aug-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-226T02:02:00,009T05:13:00,14-Aug-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-226T02:35:00,000T00:30:00,14-Aug-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-226T03:05:00,000T02:00:00,14-Aug-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-226T03:05:00,000T02:00:00,14-Aug-09,CIRS,SPASS Rider,rings(general),DUSKPTG,,CIRS_116RI_DUSKPTG001_CAPS,rider,,,,,, 2009-226T04:00:00,000T20:34:00,14-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-226T05:05:00,000T08:59:00,14-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-226T05:05:00,000T08:59:00,14-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_116RI_EQXSHADOW013_ISS,rider,,,,,, 2009-226T05:05:00,000T08:59:00,14-Aug-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-226T15:34:00,000T09:00:00,14-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-226T16:34:00,000T08:00:00,14-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09226_SP,rider,,,,,, 2009-227T00:34:00,001T16:30:00,15-Aug-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-227T01:05:00,000T06:45:00,15-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-227T01:05:00,000T06:45:00,15-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_116RI_EQXSHADOW015_ISS,rider,,,,,, 2009-227T01:05:00,000T06:45:00,15-Aug-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-227T08:04:00,000T09:00:00,15-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-227T09:04:00,000T08:00:00,15-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09227_SP,rider,,,,,, 2009-227T17:20:00,000T02:00:00,15-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-227T17:20:00,000T02:00:00,15-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_116IC_MAGBNDPTG006_ISS,rider,,,,,, 2009-227T19:20:00,000T12:10:00,15-Aug-09,CIRS,Prime,rings(general),TMAPN20MP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-227T19:20:00,000T12:10:00,15-Aug-09,CIRS,SPASS Rider,rings(general),TMAPN20MP,,CIRS_116RI_TMAPN20MP002_SI,,,,,,, 2009-227T19:20:00,000T12:10:00,15-Aug-09,UVIS,SPASS Rider,rings(general),TMAPN20MP,,URSPEC,,,,,,, 2009-228T08:04:00,000T09:00:00,16-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-228T09:04:00,000T08:00:00,16-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09228_SP,rider,,,,,, 2009-228T17:04:00,001T00:00:00,16-Aug-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-228T17:40:00,000T07:00:00,16-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-228T17:40:00,000T07:00:00,16-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_116RI_EQXSHADOW018_ISS,rider,,,,,, 2009-228T21:47:00,005T02:35:00,16-Aug-09,CAPS,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-228T21:47:00,000T19:17:00,16-Aug-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-229T00:40:00,000T06:50:00,17-Aug-09,ISS,Prime,Saturn,NALGTNG,,Lightning/E-ring in CL1 in NAC from ~20-30Rs,"Day WAC/night NAC comparison. Night: Up to 10 min exposures.I/F ~ 1e-4 to 1e-5, CL1, 12 bit, uncompressed. Day:CB2,table,lossy compression. 1 night image per 10 minutes plus a few dayside (not counted in NImages, but in 4.2 Mb/night image)",,,,,, 2009-229T08:04:00,000T09:00:00,17-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-229T09:04:00,000T08:00:00,17-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09229_SP,rider,,,,,, 2009-229T17:04:00,001T02:56:00,17-Aug-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-229T17:04:00,001T07:15:00,17-Aug-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-229T17:40:00,000T02:00:00,17-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-229T17:40:00,000T02:00:00,17-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_116IC_MAGBNDPTG008_ISS,rider,,,,,, 2009-229T19:40:00,000T18:24:00,17-Aug-09,VIMS,Prime,rings(general),HPSPOKE,,"Spoke observation, phase angle 110-130 degrees",Priority 2,,,,,, 2009-229T19:40:00,000T18:24:00,17-Aug-09,CIRS,SPASS Rider,rings(general),HPSPOKE,,CIRS_116RI_HPSPOKE001_VIMS,rider,,,,,, 2009-229T19:40:00,000T18:24:00,17-Aug-09,ISS,SPASS Rider,rings(general),HPSPOKE,,Spoke Periodicity Monitoring,WACS of B ring to search for spokes,,,,,, 2009-229T19:40:00,000T18:24:00,17-Aug-09,UVIS,SPASS Rider,rings(general),HPSPOKE,,URSPEC,,,,,,, 2009-230T00:00:00,000T09:10:00,18-Aug-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-230T15:19:00,000T09:00:00,18-Aug-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-230T15:19:00,000T09:00:00,18-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-230T16:19:00,000T08:00:00,18-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_116IC_DSCAL09230_SP,rider,,,,,, 2009-230T20:00:00,000T02:00:00,18-Aug-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-230T22:00:00,000T13:08:00,18-Aug-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-231T00:19:00,000T10:49:00,19-Aug-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-231T00:40:00,000T02:35:00,19-Aug-09,ISS,Prime,Saturn,TISATSHAD,,Titan Shadow Images,NAC images of Titan's shadow on Saturn. It is useful for Titan aerosol science and photo-ops. This is a unique geometry that occurs only a few times the XM and not at all in the nominal mission or XXM. Want 5 of 12.,,,,,, 2009-231T03:15:00,000T08:05:00,19-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-231T03:15:00,000T08:05:00,19-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_116RI_EQXSHADOW022_ISS,rider,,,,,, 2009-231T11:07:59,000T00:00:01,19-Aug-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 20.8 deg, r = 37.601 Rs, phase = 117 deg",,,,,, 2009-231T11:08:00,002T13:14:00,19-Aug-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-231T11:08:00,005T12:56:00,19-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S53,Range enter= 3.8123311 Rs exit= 16.010420 Range altitude= 40715.420 km ... -33434.979,,,,,, 2009-231T11:08:00,002T19:26:00,19-Aug-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-231T11:08:00,005T12:56:00,19-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-231T11:20:00,000T03:40:00,19-Aug-09,ISS,Prime,Saturn,NALGTNG,,Lightning/E-ring in CL1 in NAC from ~20-30Rs,"Day WAC/night NAC comparison. Night: Up to 10 min exposures.I/F ~ 1e-4 to 1e-5, CL1, 12 bit, uncompressed. Day:CB2,table,lossy compression. 1 night image per 10 minutes plus a few dayside (not counted in NImages, but in 4.2 Mb/night image)",,,,,, 2009-231T15:19:00,000T09:00:00,19-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-231T16:19:00,000T08:00:00,19-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09231_SP,rider,,,,,, 2009-232T00:40:00,000T14:15:00,20-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-232T00:40:00,000T14:15:00,20-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_117RI_EQXSHADOW001_ISS,rider,,,,,, 2009-232T11:19:00,000T07:00:00,20-Aug-09,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-26 in 1-way mode.,,,,,, 2009-232T15:19:00,000T09:00:00,20-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-232T16:19:00,000T08:00:00,20-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09232_SP,rider,,,,,, 2009-233T00:40:00,000T20:15:00,21-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-233T00:40:00,000T20:15:00,21-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_117RI_EQXSHADOW003_ISS,rider,,,,,, 2009-233T21:34:00,000T09:00:00,21-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-233T22:34:00,000T08:00:00,21-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09233_SP,rider,,,,,, 2009-234T00:22:00,002T01:40:00,22-Aug-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-234T00:22:00,002T23:42:00,22-Aug-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-234T06:34:00,001T00:00:00,22-Aug-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-234T07:15:00,000T01:15:00,22-Aug-09,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 161.2 range 1.6 Mkm",,,,,, 2009-234T07:15:00,000T01:15:00,22-Aug-09,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-234T07:15:00,000T01:15:00,22-Aug-09,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-234T08:30:00,000T02:00:00,22-Aug-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-234T08:30:00,000T02:00:00,22-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,SURVEYPTG,MAPS survey/Prime pointing,CIRS_117IC_SURVEYPTG001_CAPS,rider,,,,,, 2009-234T10:30:00,000T06:35:00,22-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-234T10:30:00,000T06:35:00,22-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_117RI_EQXSHADOW006_ISS,rider,,,,,, 2009-234T10:30:00,000T06:35:00,22-Aug-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-234T17:05:00,000T02:59:00,22-Aug-09,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"high-phase, lit-face ring photometry","high phase lit #3: B = 6, phase = 130, B' = 0.2",,,,,, 2009-234T17:05:00,000T02:59:00,22-Aug-09,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_117RI_PHOTLIT001_ISS,rider,,,,,, 2009-234T17:05:00,000T02:59:00,22-Aug-09,VIMS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,WAC mosaic?,"160 ms, 32*32 cubes?",,,,,, 2009-234T21:34:00,000T09:00:00,22-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-234T22:34:00,000T08:00:00,22-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09234_SP,rider,,,,,, 2009-235T06:34:00,001T17:30:00,23-Aug-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-235T07:15:00,000T06:45:00,23-Aug-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-235T07:15:00,000T06:45:00,23-Aug-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-235T14:00:00,000T00:40:00,23-Aug-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 028 TH OBS SET IN REV117","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-235T14:00:00,000T12:02:00,23-Aug-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-235T15:04:00,000T09:00:00,23-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-235T16:04:00,000T08:00:00,23-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09235_SP,rider,,,,,, 2009-236T00:30:00,000T14:10:00,24-Aug-09,ISS,Prime,RingE,HPMELR,,E Ring High Phase Observation,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-236T00:30:00,000T14:10:00,24-Aug-09,VIMS,SPASS Rider,RingE,HPMELR,,"E Ring moderate-to-low phase, both ansae","1 sec IR integration time, continuous collection, 64x64 FOV",,,,,, 2009-236T02:02:00,000T22:02:00,24-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-236T02:02:00,000T22:02:00,24-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-236T15:04:00,000T09:00:00,24-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-236T16:04:00,000T04:00:00,24-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09236_SP,rider,,,,,, 2009-237T00:04:00,000T10:47:38,25-Aug-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-237T00:04:00,001T03:33:58,25-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S53,Range enter= 3.8123311 Rs exit= 16.010420 Range altitude= 40715.420 km ... -33434.979,,,,,, 2009-237T00:04:00,000T00:43:00,25-Aug-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-237T00:04:00,000T08:47:38,25-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-237T00:04:00,000T10:47:38,25-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-237T00:04:00,001T06:20:00,25-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-237T00:09:00,000T00:02:00,25-Aug-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S53 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-237T00:47:00,000T00:07:00,25-Aug-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-237T00:54:00,000T00:05:00,25-Aug-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-237T00:59:00,000T00:33:00,25-Aug-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-237T01:00:38,000T02:51:00,25-Aug-09,ISS,Prime,Titan,NIGHTWAC,ISS lightning / aurora observation,WNI (WAC Nightside Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-237T01:00:38,000T02:51:00,25-Aug-09,CIRS,SPASS Rider,Titan,NIGHTWAC,ISS lightning / aurora observation,,Ride along with VIMS.,,,,,, 2009-237T01:32:00,000T00:22:59,25-Aug-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-237T01:54:59,000T09:56:39,25-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-237T03:51:38,000T03:50:00,25-Aug-09,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-237T03:51:38,000T03:50:00,25-Aug-09,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-237T03:51:38,000T03:50:00,25-Aug-09,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-237T03:51:38,000T03:50:00,25-Aug-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping,VIMS ridealong with CIRS. Limb mapping of Titan. Phase = 169 deg. Lat/Lon = 10N/139 deg. Resolution = 89 - 51 km/px. Temp. R. Obtain 2x2 mosaic and mosaics at various exp times.,,,,,, 2009-237T07:26:38,000T03:05:00,25-Aug-09,RADAR,SPASS Rider,Titan,T61WARMUP,,Warmup for T61,,,,,,, 2009-237T07:41:38,000T02:50:00,25-Aug-09,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional Mapping,Regional mapping of Titan. Phase = 169 deg. Lat/Lon = 09N/144 deg. Resolution = 47 - 19 km/px. Temp = Y. Obtain mosaics at 160 ms exp.,,,,,, 2009-237T07:41:38,000T02:50:00,25-Aug-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with SP.,,,,,, 2009-237T08:51:38,000T08:00:00,25-Aug-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T61 flyby,"T61 is an upstream, post-dusk flyby, with a minimum altitude of 1000 km. MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan near the terminator. It will be also a good complement to T52, T53, T54, T55, T56, T57, T58, T59 and T60 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-237T10:31:38,000T01:08:00,25-Aug-09,RADAR,Prime,Titan,T61INSCAT,,T61 Inbound Scatterometry,,,,,,, 2009-237T10:51:38,000T01:14:00,25-Aug-09,CAPS,SPASS Rider,Titan,T61INBND,,Inbound 117TI (T61),Inbound 117TI (T61),,,,,, 2009-237T10:51:38,000T01:00:00,25-Aug-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-237T10:51:38,000T01:00:00,25-Aug-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-237T11:39:38,000T00:42:00,25-Aug-09,RADAR,Prime,Titan,T61IHISAR,,T61 Inbound HiSAR,,,,,,, 2009-237T11:51:38,000T02:00:00,25-Aug-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-237T11:51:38,000T00:40:00,25-Aug-09,INMS,Non-SPASS,Titan,TITAN61,,Titan Flyby,Titan observation,,,,,, 2009-237T11:51:38,000T01:23:00,25-Aug-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-237T12:05:38,000T01:31:00,25-Aug-09,CAPS,SPASS Rider,Titan,T61CLOSE,,Closest Approach 117TI (T61),Closest Approach 117TI (T61),,,,,, 2009-237T12:22:38,000T00:11:00,25-Aug-09,RADAR,Prime,Titan,T61INALT,,T61 Inbound Altimetry,,,,,,, 2009-237T12:31:38,000T00:40:00,25-Aug-09,INMS,Non-SPASS,Titan,TITAN61,,Titan Flyby,Titan observation,,,,,, 2009-237T12:33:38,000T00:43:00,25-Aug-09,RADAR,Prime,Titan,T61INOSAR,,T61 Inbound and Outbound SAR,,,,,,, 2009-237T13:11:38,000T00:40:00,25-Aug-09,INMS,Non-SPASS,Titan,TITAN61,,Titan Flyby,Titan observation,,,,,, 2009-237T13:14:38,000T00:21:05,25-Aug-09,CIRS,SPASS Rider,Titan,ENGR,,,Ride along with SP.,,,,,, 2009-237T13:14:38,000T00:21:05,25-Aug-09,VIMS,SPASS Rider,Titan,ENGR,,Transition to RWA,VIMS ridealong during RCS/RWA transition. Phase = 19 deg. Lat/Lon = 15S/312 deg. Resolution = 3.3 - 6.6 km/px. Obtain four cubes during transition.,,,,,, 2009-237T13:14:38,000T00:37:00,25-Aug-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-237T13:35:43,000T07:45:55,25-Aug-09,VIMS,Prime,Titan,HIRES,High resolution image,Titan Mosaic,"do a 4.4 mosaic followed by two cubes with higher int. Each cube takes 5 minutes with 80 ms integration time. If we cannot have the last cube, it is not a pb, because we can take it at the next observation.",,,,,, 2009-237T13:35:43,000T07:45:55,25-Aug-09,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with VIMS.,,,,,, 2009-237T13:36:38,000T01:15:00,25-Aug-09,CAPS,SPASS Rider,Titan,T61OUTBND,,Outbound 117TI (T61),Outbound 117TI (T61),,,,,, 2009-237T13:51:38,000T01:00:00,25-Aug-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-237T13:51:38,001T00:17:15,25-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-237T14:21:38,000T00:30:00,25-Aug-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-237T14:51:38,001T11:12:22,25-Aug-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-237T14:51:38,001T11:12:22,25-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-237T16:51:38,001T09:12:22,25-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-237T21:21:38,000T00:30:00,25-Aug-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-237T21:21:38,000T00:30:00,25-Aug-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS.,,,,,, 2009-237T21:21:38,000T00:30:00,25-Aug-09,UVIS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Rider ro ISS PHOTOMWAC,Stare at Titan,,,,,, 2009-237T21:21:38,000T00:30:00,25-Aug-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Global mapping,VIMS ridealong with ISS. Global mapping of Titan. Phase = 13 deg. Lat/Lon = 08S/341 deg. Resolution = 84 - 89 km/px. Temp. I. Obtain five 64x64 cubes of 80 ms.,,,,,, 2009-237T21:51:38,000T05:00:00,25-Aug-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,Stare at Titan for global mapping. Phase = 13 deg. Lat/Lon = 08S/342 deg. Resolution = 89 - 141 km/px. Temp = V. Cubes of 64 x 64 at various exp. times.,,,,,, 2009-237T21:51:38,000T05:00:00,25-Aug-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2009-238T02:51:38,000T11:00:00,26-Aug-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"Stare at Titan for global mapping. Phase = 14 deg. Lat/Lon = 07S/347 deg. Resolution = 141 - 265 km/px. Temp = B. Cubes of 32 x 32, 48 x 48 and 64 x 64 at various exp. times.",,,,,, 2009-238T02:51:38,000T11:00:00,26-Aug-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2009-238T03:37:58,000T02:34:00,26-Aug-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.998530 Rs exit= 15.080218 Range altitude= -33520.532 km ... -39954.551,,,,,, 2009-238T06:11:58,001T04:04:00,26-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 15.067938 Rs exit= 4.2886860 Range altitude= -40038.202 km ... -40145.615,,,,,, 2009-238T06:24:00,000T19:40:00,26-Aug-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-238T14:08:54,000T11:55:06,26-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-238T15:04:00,000T09:00:00,26-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-238T16:04:00,000T08:00:00,26-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09238_SP,rider,,,,,, 2009-238T23:00:00,000T03:04:00,26-Aug-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-239T00:04:00,000T02:00:00,27-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-239T01:04:00,000T01:00:00,27-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09239_SP,rider,,,,,, 2009-239T02:04:00,001T12:37:59,27-Aug-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-239T02:04:00,000T11:04:54,27-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-239T02:04:00,000T06:51:00,27-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-239T02:04:00,001T12:38:00,27-Aug-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-239T02:04:00,000T11:06:00,27-Aug-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-239T02:04:00,001T12:39:00,27-Aug-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-239T02:45:00,000T04:00:00,27-Aug-09,VIMS,Prime,rings(general),HIPHASE,High phase observation,High phase rings,"radial 9x1 mosaic, right ansa, 64*24 cubes at 640 msec",,,,,, 2009-239T02:45:00,000T04:00:00,27-Aug-09,CIRS,SPASS Rider,rings(general),HIPHASE,High phase observation,CIRS_117RI_HIPHASE001_VIMS,rider,,,,,, 2009-239T02:45:00,000T04:00:00,27-Aug-09,UVIS,SPASS Rider,rings(general),HIPHASE,High phase observation,URSTAR,,,,,,, 2009-239T06:45:00,000T02:25:00,27-Aug-09,VIMS,Prime,rings(general),ALPORIOCC,Alpha Orion occultation,Ring stellar occ - alpOri,"alpOri occultation, F-D rings, R0=2.343, Rf=1.055, Rmin=1.055",,,,,, 2009-239T06:45:00,000T02:25:00,27-Aug-09,CIRS,SPASS Rider,rings(general),ALPORIOCC,Alpha Orion occultation,CIRS_117RI_ALPORIOCC101_VIMS,rider,,,,,, 2009-239T06:45:00,000T02:25:00,27-Aug-09,UVIS,SPASS Rider,rings(general),ALPORIOCC,Alpha Orion occultation,URSTAR,,,,,,, 2009-239T08:55:00,000T02:55:00,27-Aug-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-239T09:10:00,000T02:20:00,27-Aug-09,UVIS,Prime,Star,URPI4ORI,,URSTAR,"High priority Low-B incidence angle occultation. B=11 degrees. Predicted counts > 10,000 Hz.",,,,,, 2009-239T09:10:00,000T02:20:00,27-Aug-09,CIRS,SPASS Rider,rings(general),URPI4ORI,,CIRS_117RI_URPI4ORI001_UVIS,rider,,,,,, 2009-239T10:15:58,000T02:02:00,27-Aug-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.2877114 Rs exit= 4.4340766 Range altitude= -39851.381 km ... -20252.742,,,,,, 2009-239T10:33:00,000T00:00:01,27-Aug-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.280 Rs, lat = -8 deg, phase = 76 deg",,,,,, 2009-239T10:34:00,000T00:15:00,27-Aug-09,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2009-239T11:30:00,000T01:00:00,27-Aug-09,ISS,Prime,Janus,RNGMNSHAD,,Janus in Ring Shadows,Janus in Ring Shadow,,,,,, 2009-239T11:30:00,000T01:00:00,27-Aug-09,CIRS,SPASS Rider,rings(general),RNGMNSHAD,,CIRS_117RI_RNGMNSHAD001_ISS,rider,,,,,, 2009-239T11:50:00,001T02:52:00,27-Aug-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-239T12:17:58,000T01:42:02,27-Aug-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.4397676 Rs exit= 5.5292055 Range altitude= -19900.998 km ... 19981.454,,,,,, 2009-239T12:30:00,000T01:30:00,27-Aug-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-239T13:08:54,000T02:00:00,27-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-239T13:08:58,000T02:00:00,27-Aug-09,CDA,SPASS Rider,DustRAM direction,RPX0100,,CDA RPXing 2009-239T14:08:58,RPXing at 4.8768982 Rs,,,,,, 2009-239T13:10:00,000T02:00:00,27-Aug-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-239T14:00:00,000T01:00:00,27-Aug-09,ISS,Prime,Telesto,TELESCLOS,,Telesto close flyby,"Telesto close flyby, ~24,700 km at CA, 86 deg phase",,,,,, 2009-239T14:00:00,000T01:00:00,27-Aug-09,UVIS,SPASS Rider,Telesto,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-239T14:00:00,000T01:01:00,27-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 4.4397676 Rs exit= 5.5292055 Range altitude= -19900.998 km ... 19981.454,,,,,, 2009-239T15:00:00,000T02:00:00,27-Aug-09,VIMS,Prime,rings(general),LOWPHASE,Low phase imaging,Low phase observation,"radial 9x1 mosaic on left ansa, starting at F ring & going inwards, 64*64 cubes at 80 msec",,,,,, 2009-239T15:00:00,000T02:00:00,27-Aug-09,CIRS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,CIRS_117RI_LOWPHASE001_VIMS,rider,,,,,, 2009-239T15:00:00,000T02:00:00,27-Aug-09,UVIS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,URSTAR,,,,,,, 2009-239T15:01:00,000T00:58:58,27-Aug-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.4397676 Rs exit= 5.5292055 Range altitude= -19900.998 km ... 19981.454,,,,,, 2009-239T15:08:54,000T23:00:00,27-Aug-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-239T15:10:00,000T06:50:00,27-Aug-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-239T15:59:58,000T01:54:00,27-Aug-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.5420947 Rs exit= 6.3074563 Range altitude= 20338.531 km ... 39788.414,,,,,, 2009-239T17:00:00,000T03:45:00,27-Aug-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-239T17:00:00,000T03:45:00,27-Aug-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_117RI_EQXSHADOW013_ISS,rider,,,,,, 2009-239T17:00:00,000T03:45:00,27-Aug-09,VIMS,SPASS Rider,rings(general),EQXSHADOW,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-239T17:53:58,011T16:21:02,27-Aug-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 6.3217189 Rs exit= 16.010707 Range altitude= 40125.033 km ... -31882.450,,,,,, 2009-239T20:45:00,000T04:00:00,27-Aug-09,VIMS,Prime,rings(general),POSTEQXB,,Equinox observation,Do 1 of 2 at priority 1,,,,,, 2009-239T20:45:00,000T04:00:00,27-Aug-09,CIRS,SPASS Rider,rings(general),POSTEQXB,,CIRS_117RI_POSTEQXB001_VIMS,rider,,,,,, 2009-239T20:45:00,000T04:00:00,27-Aug-09,UVIS,SPASS Rider,rings(general),POSTEQXB,,URSTAR,,,,,,, 2009-240T00:45:00,000T06:00:00,28-Aug-09,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-240T00:45:00,000T06:00:00,28-Aug-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_117RI_EQLBN001_SI,,,,,,, 2009-240T07:19:00,000T09:00:00,28-Aug-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-240T07:19:00,000T09:00:00,28-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-240T08:19:00,000T08:00:00,28-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09240_SP,rider,,,,,, 2009-240T14:08:54,000T11:51:06,28-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-240T14:42:00,001T08:35:00,28-Aug-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-240T14:42:00,001T08:35:00,28-Aug-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-240T14:42:00,001T08:35:00,28-Aug-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-240T14:42:00,001T08:35:00,28-Aug-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-240T14:43:00,010T19:32:00,28-Aug-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-240T16:40:00,000T04:00:00,28-Aug-09,VIMS,Prime,rings(general),POSTEQXB,,Equinox observation,Do 1 of 2 at priority 1,,,,,, 2009-240T16:40:00,000T04:00:00,28-Aug-09,CIRS,SPASS Rider,rings(general),POSTEQXB,,CIRS_117RI_POSTEQXB002_VIMS,rider,,,,,, 2009-240T16:40:00,000T04:00:00,28-Aug-09,UVIS,SPASS Rider,rings(general),POSTEQXB,,URSTAR,,,,,,, 2009-240T20:40:00,000T06:00:00,28-Aug-09,CIRS,Prime,rings(general),TMAPN10LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-240T20:40:00,000T06:00:00,28-Aug-09,CIRS,SPASS Rider,rings(general),TMAPN10LP,,CIRS_117RI_TMAPN10LP002_SI,,,,,,, 2009-241T02:00:00,000T02:00:00,29-Aug-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-241T02:40:00,000T04:20:00,29-Aug-09,VIMS,Prime,Star,4STARCAL,Stellar calibration,Multiple star calibration,"Turn to delOph for 45 min; turn to alpHer for 45 min; turn to 30 Her for 45 min; turn to alpBoo for 45 min; return to Waypt. 12x12 FOV, 16 cubes at 40msec, 6 cubes at 160msec, 2 cubes at 640msec. RWA required.",,,,,, 2009-241T02:40:00,000T04:20:00,29-Aug-09,CIRS,SPASS Rider,rings(general),4STARCAL,Stellar calibration,CIRS_117RI_4STARCAL001_VIMS,rider,,,,,, 2009-241T04:00:00,000T12:19:00,29-Aug-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-241T07:19:00,000T09:00:00,29-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-241T08:19:00,000T08:00:00,29-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09241_SP,rider,,,,,, 2009-241T16:19:00,001T00:00:00,29-Aug-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-241T16:40:00,000T01:15:00,29-Aug-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 61.1 range 2.6 Mkm",,,,,, 2009-241T16:40:00,000T01:15:00,29-Aug-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-241T16:40:00,000T01:15:00,29-Aug-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-241T17:55:00,000T02:00:00,29-Aug-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-241T19:55:00,000T00:30:00,29-Aug-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-241T20:25:00,000T09:24:00,29-Aug-09,ISS,Prime,rings(general),RCOLSCEQX,,8 filter radial scan of main rings; second instanc,"8 filter, 70deg phase, lit face; very near equinox, 25Rs",,,,,, 2009-241T20:25:00,000T09:24:00,29-Aug-09,CIRS,SPASS Rider,rings(general),RCOLSCEQX,,CIRS_117IC_RCOLSCEQX001_ISS,rider,,,,,, 2009-241T20:25:00,000T09:24:00,29-Aug-09,VIMS,SPASS Rider,rings(general),RCOLSCEQX,,"radial scan(?), low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2009-241T23:17:00,001T23:25:00,29-Aug-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-241T23:17:00,001T23:25:00,29-Aug-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-241T23:17:00,003T00:16:00,29-Aug-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-242T07:19:00,000T09:00:00,30-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-242T08:19:00,000T08:00:00,30-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09242_SP,rider,,,,,, 2009-242T16:19:00,005T13:29:00,30-Aug-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-242T16:40:00,000T13:38:00,30-Aug-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-242T16:40:00,000T13:38:00,30-Aug-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP001_ISS,rider,,,,,, 2009-242T16:40:00,000T13:38:00,30-Aug-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-243T07:18:00,000T09:00:00,31-Aug-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-243T08:18:00,000T08:00:00,31-Aug-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09243_SP,rider,,,,,, 2009-243T16:35:00,000T01:15:00,31-Aug-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 87.8 range 3.2 Mkm",,,,,, 2009-243T16:35:00,000T01:15:00,31-Aug-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-243T16:35:00,000T01:15:00,31-Aug-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-243T17:50:00,000T00:30:00,31-Aug-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-243T18:20:00,000T02:00:00,31-Aug-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-243T20:20:00,000T17:55:00,31-Aug-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-243T20:20:00,000T17:55:00,31-Aug-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP003_ISS,rider,,,,,, 2009-243T20:20:00,000T17:55:00,31-Aug-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-243T22:42:00,009T06:51:00,31-Aug-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-243T22:42:00,007T11:33:00,31-Aug-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-243T22:42:00,001T15:50:00,31-Aug-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-244T14:33:00,000T09:00:00,1-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-244T15:33:00,000T08:00:00,1-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09244_SP,rider,,,,,, 2009-244T23:33:00,003T06:15:00,1-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-244T23:50:00,000T14:25:00,1-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-244T23:50:00,000T14:25:00,1-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP004_ISS,rider,,,,,, 2009-244T23:50:00,000T14:25:00,1-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-245T00:00:00,000T00:34:00,2-Sep-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-245T14:32:00,000T09:01:00,2-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-245T14:33:00,000T09:00:00,2-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-245T14:33:00,000T09:00:00,2-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-245T15:33:00,000T08:00:00,2-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09245_SP,rider,,,,,, 2009-245T23:33:00,000T14:59:00,2-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-245T23:50:00,000T13:55:00,2-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-245T23:50:00,000T12:58:00,2-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP005_ISS,rider,,,,,, 2009-245T23:50:00,000T12:58:00,2-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-246T13:45:00,000T00:30:00,3-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 018 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-246T14:32:00,000T09:01:00,3-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-246T14:33:00,000T09:00:00,3-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-246T14:33:00,000T09:00:00,3-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-246T15:33:00,000T08:00:00,3-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09246_SP,rider,,,,,, 2009-246T23:33:00,003T06:00:00,3-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-246T23:50:00,000T01:30:00,3-Sep-09,ISS,Prime,Saturn,TISATSHAD,,Titan Shadow Images,NAC images of Titan's shadow on Saturn. It is useful for Titan aerosol science and photo-ops. This is a unique geometry that occurs only a few times the XM and not at all in the nominal mission or XXM. Want 5 of 12.,,,,,, 2009-247T01:20:00,000T00:30:00,4-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 020 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-247T01:50:00,000T18:25:00,4-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-247T01:50:00,000T18:25:00,4-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP006_ISS,rider,,,,,, 2009-247T01:50:00,000T18:25:00,4-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-247T20:48:00,000T09:00:00,4-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-247T21:48:00,000T08:00:00,4-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09247_SP,rider,,,,,, 2009-248T05:48:00,001T00:00:00,5-Sep-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-248T05:48:00,001T23:45:00,5-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-248T06:20:00,000T12:58:00,5-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-248T06:20:00,000T12:58:00,5-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP007_ISS,rider,,,,,, 2009-248T06:20:00,000T12:58:00,5-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-248T20:48:00,000T09:00:00,5-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-248T21:48:00,000T08:00:00,5-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09248_SP,rider,,,,,, 2009-249T00:00:00,001T00:00:00,6-Sep-09,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2009-249T05:48:00,001T15:12:00,6-Sep-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-249T06:20:00,000T13:25:00,6-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-249T06:20:00,000T13:25:00,6-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP008_ISS,rider,,,,,, 2009-249T06:20:00,000T13:25:00,6-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-249T19:45:00,000T00:30:00,6-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 028 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-249T20:33:00,000T09:00:00,6-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-249T20:33:00,000T09:00:00,6-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-249T21:33:00,000T08:00:00,6-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09249_SP,rider,,,,,, 2009-250T05:33:00,003T00:00:00,7-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-250T05:33:00,001T04:42:00,7-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-250T05:50:00,000T01:15:00,7-Sep-09,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 116.7 range 1.9 Mkm",,,,,, 2009-250T05:50:00,000T01:15:00,7-Sep-09,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-250T05:50:00,000T01:15:00,7-Sep-09,UVIS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-250T07:05:00,000T07:28:00,7-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-250T07:05:00,000T07:28:00,7-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP009_ISS,rider,,,,,, 2009-250T07:05:00,000T07:28:00,7-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-250T14:33:00,000T03:00:00,7-Sep-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Kiviuq,Observation of Kiviuq,,,,,, 2009-250T14:33:00,000T03:00:00,7-Sep-09,RADAR,SPASS Rider,Other,WU4NEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-250T14:34:20,000T00:00:01,7-Sep-09,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2009-250T17:33:00,000T01:30:00,7-Sep-09,RADAR,Prime,Titan,NEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-250T19:03:00,000T01:12:00,7-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 027 TH OB SET IN REV 117","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-250T20:33:00,000T09:00:00,7-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-250T20:33:00,000T09:00:00,7-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-250T21:00:00,000T02:00:00,7-Sep-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-250T21:33:00,000T08:00:00,7-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_117IC_DSCAL09250_SP,rider,,,,,, 2009-250T23:00:00,000T11:15:00,7-Sep-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-251T05:33:00,000T15:00:00,8-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-251T05:50:00,000T14:25:00,8-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_117IC_SPKMVLFHP010_ISS,rider,,,,,, 2009-251T05:50:00,000T14:25:00,8-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-251T10:13:33,000T00:00:01,8-Sep-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 24.0 d, inc = 12.1 deg, r = 48.886 Rs, phase = 104 deg",,,,,, 2009-251T10:15:00,005T12:48:00,8-Sep-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-251T10:15:00,010T16:42:58,8-Sep-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 6.3217189 Rs exit= 16.010707 Range altitude= 40125.033 km ... -31882.450,,,,,, 2009-251T10:15:00,005T12:48:00,8-Sep-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-251T10:15:00,001T10:18:00,8-Sep-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-251T20:33:00,000T09:00:00,8-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-251T20:33:00,000T09:00:00,8-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-251T21:33:00,000T06:00:00,8-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09251_SP,rider,,,,,, 2009-252T05:50:00,000T02:00:00,9-Sep-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-252T05:50:00,000T02:00:00,9-Sep-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-252T05:50:00,000T02:00:00,9-Sep-09,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,,null,,,,,, 2009-252T07:50:00,000T12:25:00,9-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-252T07:50:00,000T11:13:00,9-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_118RI_SPKMVLFHP001_ISS,rider,,,,,, 2009-252T07:50:00,000T11:13:00,9-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-252T20:33:00,000T09:00:00,9-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-252T20:33:00,004T02:30:00,9-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-252T20:33:00,000T09:00:00,9-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-252T21:33:00,000T08:00:00,9-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09252_SP,rider,,,,,, 2009-253T05:33:00,003T17:30:00,10-Sep-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-253T05:33:00,003T17:30:00,10-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-253T05:50:00,000T01:15:00,10-Sep-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 87.8 range 2 Mkm",,,,,, 2009-253T05:50:00,000T01:15:00,10-Sep-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-253T05:50:00,000T01:15:00,10-Sep-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-253T07:05:00,000T12:55:00,10-Sep-09,VIMS,Prime,rings(general),HPSPOKE,,"Spoke observation, phase angle 110-130 degrees",Priority 2,,,,,, 2009-253T07:05:00,000T12:55:00,10-Sep-09,CIRS,SPASS Rider,rings(general),HPSPOKE,,CIRS_118RI_HPSPOKE001_VIMS,rider,,,,,, 2009-253T07:05:00,000T12:55:00,10-Sep-09,UVIS,SPASS Rider,rings(general),HPSPOKE,,URSTAR,,,,,,, 2009-253T20:18:00,000T09:00:00,10-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-253T20:18:00,000T09:00:00,10-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-253T21:18:00,000T06:00:00,10-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09253_SP,rider,,,,,, 2009-254T05:35:00,000T05:43:00,11-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-254T05:35:00,000T05:43:00,11-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_118RI_SPKMVLFHP002_ISS,rider,,,,,, 2009-254T05:35:00,000T05:43:00,11-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-254T11:18:00,000T01:30:00,11-Sep-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-254T11:18:00,000T01:30:00,11-Sep-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-254T11:18:00,000T01:30:00,11-Sep-09,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,,null,,,,,, 2009-254T12:48:00,000T00:57:00,11-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-254T14:03:00,000T09:00:00,11-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-254T14:03:00,000T09:00:00,11-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-254T15:03:00,000T06:00:00,11-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09254_SP,rider,,,,,, 2009-254T23:25:00,000T01:15:00,11-Sep-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 85.4 range 2.5 Mkm",,,,,, 2009-254T23:25:00,000T01:15:00,11-Sep-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-254T23:25:00,000T01:15:00,11-Sep-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-255T00:40:00,000T13:00:00,12-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-255T00:40:00,000T13:00:00,12-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_118RI_SPKMVLFHP003_ISS,rider,,,,,, 2009-255T00:40:00,000T13:00:00,12-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-255T14:03:00,000T09:00:00,12-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-255T14:03:00,000T09:00:00,12-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-255T15:03:00,000T06:00:00,12-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09255_SP,rider,,,,,, 2009-255T23:25:00,000T01:15:00,12-Sep-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 88.8 range 2.8 Mkm",,,,,, 2009-255T23:25:00,000T01:15:00,12-Sep-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-255T23:25:00,000T01:15:00,12-Sep-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-256T00:40:00,000T10:23:00,13-Sep-09,ISS,Prime,rings(general),SPKMVLFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2009-256T00:40:00,000T10:23:00,13-Sep-09,CIRS,SPASS Rider,rings(general),SPKMVLFHP,,CIRS_118RI_SPKMVLFHP004_ISS,rider,,,,,, 2009-256T00:40:00,000T10:23:00,13-Sep-09,VIMS,SPASS Rider,rings(general),SPKMVLFHP,,"Spoke movie, lit face, high phase",ISS rider,,,,,, 2009-256T11:03:00,000T01:30:00,13-Sep-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-256T11:03:00,000T01:30:00,13-Sep-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-256T11:03:00,000T01:30:00,13-Sep-09,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,,null,,,,,, 2009-256T12:33:00,000T01:07:00,13-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-256T14:03:00,000T09:00:00,13-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-256T14:03:00,000T09:00:00,13-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-256T15:03:00,000T08:00:00,13-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09256_SP,rider,,,,,, 2009-256T23:03:00,000T08:55:00,13-Sep-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-256T23:03:00,001T22:39:00,13-Sep-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-256T23:03:00,001T22:39:00,13-Sep-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-256T23:03:00,004T14:57:00,13-Sep-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-256T23:03:00,000T08:55:00,13-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-256T23:03:00,005T06:41:00,13-Sep-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-257T07:58:00,000T01:10:00,14-Sep-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-257T07:58:00,000T01:10:00,14-Sep-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-257T07:58:00,000T01:10:00,14-Sep-09,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,,null,,,,,, 2009-257T07:58:00,003T03:49:00,14-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-257T09:08:00,000T03:00:00,14-Sep-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Ijiraq,Observation of Ijiraq,,,,,, 2009-257T09:08:00,000T03:00:00,14-Sep-09,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,,,,,,,, 2009-257T13:48:00,000T09:00:00,14-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-257T13:48:00,000T09:00:00,14-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-257T15:23:00,000T07:25:00,14-Sep-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-257T16:08:00,000T06:40:00,14-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09257_SP,rider,,,,,, 2009-258T13:48:00,000T09:00:00,15-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-258T13:48:00,000T09:00:00,15-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-258T21:42:00,006T03:18:00,15-Sep-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-258T21:42:00,004T00:51:00,15-Sep-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-259T13:48:00,000T09:00:00,16-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-259T13:48:00,000T09:00:00,16-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-260T00:00:00,000T00:34:00,17-Sep-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-260T11:47:00,002T10:46:00,17-Sep-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-260T13:48:00,000T09:00:00,17-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-260T13:48:00,000T09:00:00,17-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-261T13:48:00,000T09:00:00,18-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-261T13:48:00,000T09:00:00,18-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-261T14:00:00,000T02:00:00,18-Sep-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-261T16:00:00,000T21:29:25,18-Sep-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-262T02:57:58,000T03:10:00,19-Sep-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.998818 Rs exit= 14.858557 Range altitude= -31968.229 km ... -39929.961,,,,,, 2009-262T05:44:00,000T16:49:00,19-Sep-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-262T06:07:58,001T03:26:00,19-Sep-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 14.846180 Rs exit= 4.2805580 Range altitude= -40013.404 km ... -40145.494,,,,,, 2009-262T13:29:25,000T09:03:35,19-Sep-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-262T13:33:00,000T09:00:00,19-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-262T13:33:00,000T09:00:00,19-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-262T14:33:00,000T08:00:00,19-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09262_SP,rider,,,,,, 2009-262T22:33:00,000T13:56:25,19-Sep-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-262T22:33:00,000T09:38:00,19-Sep-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-262T22:33:00,001T15:29:00,19-Sep-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-262T22:33:00,000T13:42:00,19-Sep-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-263T08:11:00,000T03:02:00,20-Sep-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-263T09:33:58,000T00:40:02,20-Sep-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.2794984 Rs exit= 4.4274793 Range altitude= -39855.781 km ... -20162.278,,,,,, 2009-263T09:52:24,000T00:00:01,20-Sep-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.271 Rs, lat = -8 deg, phase = 77 deg",,,,,, 2009-263T10:14:00,000T05:20:00,20-Sep-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.2794984 Rs exit= 4.4274793 Range altitude= -39855.781 km ... -20162.278,,,,,, 2009-263T11:13:00,000T03:39:04,20-Sep-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-263T12:15:00,000T00:15:00,20-Sep-09,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2009-263T12:29:25,000T02:00:00,20-Sep-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-263T12:30:00,000T02:00:00,20-Sep-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-263T12:30:58,000T02:00:00,20-Sep-09,CDA,SPASS Rider,DustRAM direction,RPX0110,,CDA RPXing 2009-263T13:30:58,RPXing at 4.8835416 Rs,,,,,, 2009-263T14:29:25,000T23:00:00,20-Sep-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-263T14:30:00,000T06:30:00,20-Sep-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-263T14:52:04,000T04:00:00,20-Sep-09,MAG,Non-SPASS,Dione,DITAR,Dione targeted flyby,D3 flyby,Monitor magnetic field perturbations and waves to confirm evidence of plasma pickup observed during the sole previous upstream Dione flyby.,,,,,, 2009-263T15:34:00,000T01:41:58,20-Sep-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 5.5413404 Rs exit= 6.3231911 Range altitude= 20069.629 km ... 39688.359,,,,,, 2009-263T16:10:00,000T00:50:00,20-Sep-09,VIMS,Prime,rings(general),LOWPHASE,Low phase imaging,Low phase observation,"radial 6x1 (?) mosaic on left ansa, starting at 100,000 km and going inwards, 64*64 cubes, 80 msec.",,,,,, 2009-263T16:10:00,000T00:50:00,20-Sep-09,CIRS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,CIRS_118RI_LOWPHASE001_VIMS,rider,,,,,, 2009-263T16:10:00,000T00:50:00,20-Sep-09,UVIS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,URSTAR,,,,,,, 2009-263T17:00:00,000T01:15:00,20-Sep-09,UVIS,Prime,Dione,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to star epsilon CMa.,,,,,, 2009-263T17:00:00,000T01:15:00,20-Sep-09,VIMS,SPASS Rider,Dione,OCCULT,,,null,,,,,, 2009-263T17:15:58,011T14:47:02,20-Sep-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 6.3375028 Rs exit= 16.004628 Range altitude= 40021.765 km ... 978.08986,,,,,, 2009-263T18:15:00,000T03:45:00,20-Sep-09,ISS,Prime,rings(general),EQXSHADOW,,Equinox shadow,looking for the shadow of vertical features in the rings during the equinox period,,,,,, 2009-263T18:15:00,000T03:45:00,20-Sep-09,CIRS,SPASS Rider,rings(general),EQXSHADOW,,CIRS_118RI_EQXSHADOW001_ISS,rider,,,,,, 2009-263T18:52:04,000T19:09:56,20-Sep-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-263T21:00:00,001T16:33:00,20-Sep-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-263T22:00:00,000T04:00:00,20-Sep-09,VIMS,Prime,rings(general),POSTEQX,,Equinox observation,"Radial scan, exp= 160 msec => 12 min/ptg",,,,,, 2009-263T22:00:00,000T04:00:00,20-Sep-09,CIRS,SPASS Rider,rings(general),POSTEQX,,CIRS_118RI_POSTEQX001_VIMS,rider,,,,,, 2009-263T22:00:00,000T04:00:00,20-Sep-09,UVIS,SPASS Rider,rings(general),POSTEQX,,URSTAR,,,,,,, 2009-264T02:00:00,000T06:00:00,21-Sep-09,CIRS,Prime,rings(general),EQLBN,,CIRS_118RI_EQLBN001_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-264T02:00:00,000T06:00:00,21-Sep-09,CIRS,SPASS Rider,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-264T02:00:00,000T06:00:00,21-Sep-09,UVIS,SPASS Rider,rings(general),EQLBN,,URSTAR,,,,,,, 2009-264T08:00:00,000T04:03:00,21-Sep-09,ISS,Prime,rings(general),PROPELLR,,Equinox: Look for vertical features in propellers.,Image propellers to look for vertical features during equinox.,,,,,, 2009-264T08:00:00,000T04:03:00,21-Sep-09,CIRS,SPASS Rider,rings(general),PROPELLR,,CIRS_118RI_PROPELLR001_ISS,rider,,,,,, 2009-264T13:29:25,003T08:48:35,21-Sep-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-264T13:33:00,000T09:00:00,21-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-264T13:33:00,000T09:00:00,21-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-264T14:02:00,001T08:30:00,21-Sep-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-264T14:02:00,001T08:30:00,21-Sep-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-264T14:33:00,000T08:00:00,21-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09264_SP,rider,,,,,, 2009-264T22:55:00,000T08:00:00,21-Sep-09,CIRS,Prime,rings(general),TMAPN10LP,,CIRS_118RI_TMAPN10LP002_PRIME;,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-264T22:55:00,000T08:00:00,21-Sep-09,CIRS,SPASS Rider,rings(general),TMAPN10LP,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-264T22:55:00,000T08:00:00,21-Sep-09,UVIS,SPASS Rider,rings(general),TMAPN10LP,,URSTAR,,,,,,, 2009-265T01:00:00,000T21:32:00,22-Sep-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-265T06:55:00,000T04:15:00,22-Sep-09,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"intermediate phase, lit-face ring photometry","intermediate lit #9: B = 12, phase = 61, B' = 0.6",,,,,, 2009-265T06:55:00,000T04:15:00,22-Sep-09,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_118RI_PHOTLIT001_ISS,rider,,,,,, 2009-265T11:10:00,000T02:00:00,22-Sep-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-265T11:10:00,000T02:00:00,22-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DUSKPTG,,CIRS_118IC_DUSKPTG001_CAPS,rider,,,,,, 2009-265T13:33:00,000T09:00:00,22-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-265T13:33:00,001T08:45:00,22-Sep-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-265T13:33:00,000T09:00:00,22-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-265T14:33:00,000T08:00:00,22-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09265_SP,rider,,,,,, 2009-265T22:32:00,000T23:46:00,22-Sep-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-265T22:32:00,001T23:46:00,22-Sep-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-265T22:32:00,001T23:46:00,22-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-265T22:55:00,000T12:53:00,22-Sep-09,ISS,Prime,Titan,NPOLCLD,,(NPC) North Pole Cloud Observation,"Titan Monitoring Campaign, phase 87.8 range 2 Mkm",,,,,, 2009-266T13:18:00,000T09:00:00,23-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-266T13:18:00,000T09:00:00,23-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-266T14:18:00,000T08:00:00,23-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09266_SP,rider,,,,,, 2009-266T22:18:00,000T12:42:00,23-Sep-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-266T22:18:00,001T00:00:00,23-Sep-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-266T22:40:00,000T01:15:00,23-Sep-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 52.6 range 0.8 Mkm",,,,,, 2009-266T22:40:00,000T01:15:00,23-Sep-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,CIRS_118TI_M60R1CLD266_ISS,rider,,,,,, 2009-266T22:40:00,000T01:15:00,23-Sep-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-266T23:55:00,000T00:30:00,23-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-267T00:25:00,000T10:05:00,24-Sep-09,ISS,Prime,rings(general),RCOLSCEQX,,8 filter radial scan of main rings; third instance,"8 filter, 80deg phase, lit face; very near equinox, 31Rs",,,,,, 2009-267T00:25:00,000T10:05:00,24-Sep-09,CIRS,SPASS Rider,rings(general),RCOLSCEQX,,CIRS_118RI_RCOLSCEQX002_ISS,rider,,,,,, 2009-267T10:30:00,000T00:30:00,24-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-267T11:00:00,000T02:00:00,24-Sep-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-267T11:00:00,000T02:00:00,24-Sep-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-267T11:00:00,000T02:00:00,24-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,MAGBNDPTG,MAPS magnetosphere boundary campaign,CIRS_118IC_MAGBNDPTG002_CAPS,rider,,,,,, 2009-267T13:00:00,000T09:07:00,24-Sep-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-267T13:18:00,000T09:00:00,24-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-267T13:18:00,000T09:00:00,24-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-267T14:18:00,000T08:00:00,24-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09267_SP,rider,,,,,, 2009-267T22:07:00,010T05:56:00,24-Sep-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-267T22:18:00,007T09:46:00,24-Sep-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-267T22:18:00,006T22:42:00,24-Sep-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-267T22:18:00,007T16:00:00,24-Sep-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-267T22:18:00,002T06:15:00,24-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-267T22:58:00,000T04:00:00,24-Sep-09,ISS,Prime,Iapetus,HILLSPHE,,Iapetus hill sphere observation,Turn -Y near Iapetus; do 1x2 mosaic; turn to WP.,,,,,, 2009-268T02:58:00,000T09:47:00,25-Sep-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,This segment contains 90 hours of -X offset rolls (CAPS prime) and 72 hours of rolling downlinks (Z axis). RBOT may very well freak out.,,,,,, 2009-268T13:18:00,000T09:00:00,25-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-268T13:18:00,000T09:00:00,25-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-268T14:18:00,000T08:00:00,25-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09268_SP,rider,,,,,, 2009-268T22:58:00,000T16:55:00,25-Sep-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,This segment contains 90 hours of -X offset rolls (CAPS prime) and 72 hours of rolling downlinks (Z axis). RBOT may very well freak out.,,,,,, 2009-269T12:53:00,000T03:00:00,26-Sep-09,CIRS,SPASS Rider,Sun,SWAURCAL,,,"Calibrate during last 3h of CAPS prime (12:53 - 15:53) in order to perform science at 15:53, but only for FP1 (multiplier 0.091).",,,,,, 2009-269T15:53:00,000T03:00:00,26-Sep-09,CIRS,Prime,rings(general),POLARIZ,,CIRS_118RI_POLARIZ266_PRIME;,FP1 only for polarization measurement.,,,,,, 2009-269T15:53:00,000T03:00:00,26-Sep-09,CIRS,SPASS Rider,rings(general),POLARIZ,,CIRS_118RI_POLARIZ269_SI,,,,,,, 2009-269T19:33:00,000T09:00:00,26-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-269T19:33:00,000T09:00:00,26-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-269T20:33:00,000T08:00:00,26-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09269_SP,rider,,,,,, 2009-270T04:33:00,002T08:30:00,27-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-270T05:13:00,000T23:17:00,27-Sep-09,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_118SA_MIRMAP001_PRIME,"Northern hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2009-271T04:30:00,000T00:30:00,28-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 020 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-271T05:33:00,000T09:00:00,28-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-271T05:33:00,000T09:00:00,28-Sep-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-271T05:33:00,000T09:00:00,28-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-271T06:33:00,000T08:00:00,28-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09271_SP,rider,,,,,, 2009-271T14:33:00,000T22:30:00,28-Sep-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,This segment contains 90 hours of -X offset rolls (CAPS prime) and 72 hours of rolling downlinks (Z axis). RBOT may very well freak out.,,,,,, 2009-272T13:03:00,000T09:00:00,29-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-272T13:03:00,002T19:00:00,29-Sep-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-272T13:03:00,000T09:00:00,29-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-272T14:03:00,000T08:00:00,29-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09272_SP,rider,,,,,, 2009-272T22:43:00,000T14:00:00,29-Sep-09,CIRS,Prime,Saturn,MIRTMAP,,CIRS_118SA_MIRTMAP001_PRIME,"Northern hemisphere Determine upper troposphere and tropopause temperature sacrifice longitude coverage for latitude coverage, 10 deg bins",,,,,, 2009-273T12:43:00,000T05:32:00,30-Sep-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,This segment contains 90 hours of -X offset rolls (CAPS prime) and 72 hours of rolling downlinks (Z axis). RBOT may very well freak out.,,,,,, 2009-273T18:15:00,000T00:30:00,30-Sep-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 027 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-273T19:18:00,000T09:00:00,30-Sep-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-273T19:18:00,000T09:00:00,30-Sep-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-273T20:18:00,000T08:00:00,30-Sep-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09273_SP,rider,,,,,, 2009-274T04:18:00,001T01:00:00,1-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,This segment contains 90 hours of -X offset rolls (CAPS prime) and 72 hours of rolling downlinks (Z axis). RBOT may very well freak out.,,,,,, 2009-274T18:38:00,000T09:10:00,1-Oct-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-274T21:00:00,000T02:00:00,1-Oct-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-274T23:00:00,000T09:04:00,1-Oct-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-275T05:18:00,000T09:00:00,2-Oct-09,RSS,SPASS Rider,Earth,SCE6,,Solar Conjunction Experiment (SCE) #6,"Characterize the solar corona at 2 frequency bands (X and Ka1), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2009-275T05:18:00,000T09:00:00,2-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-275T06:18:00,000T08:00:00,2-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_118IC_DSCAL09275_SP,rider,,,,,, 2009-275T08:03:00,002T20:00:00,2-Oct-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S54,Range enter= 6.3375028 Rs exit= 16.004628 Range altitude= 40021.765 km ... 978.08986,,,,,, 2009-275T08:03:00,002T20:00:00,2-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-275T08:03:00,002T20:00:00,2-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-275T08:03:00,000T06:15:00,2-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-275T08:03:17,000T00:00:01,2-Oct-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 23.8 d, inc = 12.2 deg, r = 48.711 Rs, phase = 103 deg",,,,,, 2009-275T08:04:00,002T19:59:00,2-Oct-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-275T08:04:00,002T19:59:00,2-Oct-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-275T14:18:00,000T22:30:00,2-Oct-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_119SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-275T14:18:00,002T04:45:00,2-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-276T08:48:00,000T08:00:00,3-Oct-09,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 4 hours required to be tracked at DSS-25 in 1-way mode.,,,,,, 2009-276T12:48:00,000T05:00:00,3-Oct-09,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2009-276T12:48:00,000T09:00:00,3-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-276T13:48:00,000T08:00:00,3-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09276_SP,rider,,,,,, 2009-276T16:48:00,000T01:00:00,3-Oct-09,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2009-276T22:28:00,000T03:00:00,3-Oct-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-276T22:28:00,000T03:00:00,3-Oct-09,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2009-276T22:28:00,000T00:01:30,3-Oct-09,VIMS,SPASS Rider,Saturn,RAMREAD,,,null,,,,,, 2009-277T01:28:00,000T09:02:00,4-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,This segment contains 90 hours of -X offset rolls (CAPS prime) and 72 hours of rolling downlinks (Z axis). RBOT may very well freak out.,,,,,, 2009-277T19:03:00,000T09:00:00,4-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-277T19:03:00,000T09:00:00,4-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-277T22:03:00,000T06:00:00,4-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09277_SP,rider,,,,,, 2009-278T04:03:00,001T10:15:00,5-Oct-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-278T04:03:00,001T10:15:00,5-Oct-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-278T04:03:00,001T10:15:00,5-Oct-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S54,Range enter= 6.3375028 Rs exit= 16.004628 Range altitude= 40021.765 km ... 978.08986,,,,,, 2009-278T04:03:00,000T00:43:00,5-Oct-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-278T04:03:00,001T10:15:00,5-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-278T04:03:00,006T09:46:00,5-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-278T04:03:00,001T10:15:00,5-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-278T04:08:00,000T00:02:00,5-Oct-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S54 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-278T04:46:00,000T00:07:00,5-Oct-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-278T04:49:00,000T11:41:00,5-Oct-09,VIMS,Prime,rings(general),HPSPOKE,,"Spoke observation, phase angle 110-130 degrees",Priority 2,,,,,, 2009-278T04:49:00,000T11:41:00,5-Oct-09,CIRS,SPASS Rider,rings(general),HPSPOKE,,CIRS_RIRI_HPSPOKE001_VIMS,rider,,,,,, 2009-278T04:53:00,000T00:05:00,5-Oct-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-278T04:58:00,000T00:33:00,5-Oct-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-278T05:00:00,000T12:30:00,5-Oct-09,CDA,Non-SPASS,Other,DECON,Decontamination,Decontamination,,,,,,, 2009-278T05:31:00,000T00:22:59,5-Oct-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-278T05:53:59,001T12:06:01,5-Oct-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-278T16:30:00,000T12:08:00,5-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-278T16:30:00,000T12:08:00,5-Oct-09,ISS,SPASS Rider,Sun,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC image per 10 minutes or otherwise according to CAPS plan.,,,,,, 2009-278T16:30:00,000T12:08:00,5-Oct-09,UVIS,SPASS Rider,Saturn,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2009-279T05:18:00,000T09:00:00,6-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-279T06:18:00,000T08:00:00,6-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09279_SP,rider,,,,,, 2009-279T14:18:00,003T03:39:00,6-Oct-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-279T14:18:00,003T03:39:00,6-Oct-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-279T14:18:00,004T14:31:00,6-Oct-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S54,Range enter= 6.3375028 Rs exit= 16.004628 Range altitude= 40021.765 km ... 978.08986,,,,,, 2009-279T14:18:00,002T00:26:00,6-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-279T14:18:00,002T14:46:00,6-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-279T14:58:00,000T13:25:00,6-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-279T14:58:00,000T13:25:00,6-Oct-09,ISS,SPASS Rider,Sun,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC image per 10 minutes or otherwise according to CAPS plan.,,,,,, 2009-279T14:58:00,000T13:25:00,6-Oct-09,UVIS,SPASS Rider,Saturn,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2009-279T18:00:00,000T00:34:00,6-Oct-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2009-279T18:34:00,000T10:42:00,6-Oct-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-280T04:23:00,000T10:20:00,7-Oct-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-280T05:03:00,000T09:00:00,7-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-280T05:16:00,002T08:48:00,7-Oct-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-280T06:03:00,000T08:00:00,7-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09280_SP,rider,,,,,, 2009-280T14:43:00,000T04:00:00,7-Oct-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-280T18:43:00,000T09:41:00,7-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-280T18:43:00,000T09:41:00,7-Oct-09,ISS,SPASS Rider,Sun,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC image per 10 minutes or otherwise according to CAPS plan.,,,,,, 2009-280T18:43:00,000T09:41:00,7-Oct-09,UVIS,SPASS Rider,Saturn,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2009-281T05:04:00,000T09:00:00,8-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-281T14:44:00,000T06:45:00,8-Oct-09,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2009-281T14:44:00,000T06:45:00,8-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,"Observe magnetospheric boundaries near noon on highly inclined orbits. Data rate 0 bps, overlaps CALROLL request.",,,,,, 2009-281T21:29:00,000T06:55:00,8-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-281T21:29:00,000T06:55:00,8-Oct-09,ISS,SPASS Rider,Sun,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC image per 10 minutes or otherwise according to CAPS plan.,,,,,, 2009-281T21:29:00,000T06:55:00,8-Oct-09,UVIS,SPASS Rider,Saturn,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2009-281T21:29:00,001T05:31:00,8-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-282T05:04:00,000T12:53:00,9-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-282T05:04:00,000T09:00:00,9-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-282T06:04:00,000T08:00:00,9-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09282_SP,rider,,,,,, 2009-282T14:04:00,001T00:00:00,9-Oct-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-282T14:44:00,000T01:15:00,9-Oct-09,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 156.7 range 1.4 Mkm",,,,,, 2009-282T14:44:00,000T01:15:00,9-Oct-09,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-282T14:44:00,000T01:15:00,9-Oct-09,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-282T15:59:00,000T12:25:00,9-Oct-09,VIMS,Prime,rings(general),EG105PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. MAG segment. Do 1 of 3 EG105 phase at priority 2.,,,,,, 2009-282T15:59:00,000T12:25:00,9-Oct-09,CIRS,SPASS Rider,rings(general),EG105PHAS,,CIRS_RIRI_EG105PHAS001_VIMS,rider,,,,,, 2009-282T15:59:00,000T12:25:00,9-Oct-09,ISS,SPASS Rider,rings(general),EG105PHAS,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2009-282T17:57:00,001T16:55:00,9-Oct-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-282T17:57:00,001T19:52:00,9-Oct-09,CAPS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS Survey (solar wind emphasis),MAPS magnetospheric survey with solar wind emphasis,,,,,, 2009-282T17:57:00,001T19:52:00,9-Oct-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-283T03:00:00,001T07:52:00,10-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-283T05:04:00,000T09:00:00,10-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-283T06:04:00,000T08:00:00,10-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09283_SP,rider,,,,,, 2009-283T14:04:00,000T23:45:00,10-Oct-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-283T14:44:00,000T09:25:00,10-Oct-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_119SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-284T00:09:00,000T03:00:00,11-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-284T04:49:00,001T18:32:58,11-Oct-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S54,Range enter= 6.3375028 Rs exit= 16.004628 Range altitude= 40021.765 km ... 978.08986,,,,,, 2009-284T04:49:00,000T09:00:00,11-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-284T05:49:00,000T08:00:00,11-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09284_SP,rider,,,,,, 2009-284T10:52:00,000T02:57:00,11-Oct-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-284T10:52:00,000T02:57:00,11-Oct-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-284T13:49:00,000T16:47:25,11-Oct-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-284T13:49:00,000T06:47:25,11-Oct-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-284T13:49:00,000T14:47:25,11-Oct-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-284T13:49:00,000T16:47:25,11-Oct-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-284T13:49:00,001T12:14:00,11-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-284T14:45:21,000T04:51:04,11-Oct-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,CIRS_119TI_MIDIRTMAP001_PRIME,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-284T14:45:21,000T04:51:04,11-Oct-09,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-284T14:45:21,000T04:51:04,11-Oct-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Slow Titan scan,VIMS ridealong with CIRS. Scan across Titan . Phase = 164 deg. Lat/Lon = 06N/138 deg. Resolution = 175 - 130 km/px. Temp. M3. Slow scan across Titan.,,,,,, 2009-284T19:36:25,000T04:00:00,11-Oct-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-284T19:36:25,000T03:00:00,11-Oct-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-284T19:36:25,000T03:00:00,11-Oct-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,VIMS ridealong with CIRS. Stare at Titan . Phase = 165 deg. Lat/Lon = 06N/142 deg. Resolution = 130 - 100 km/px. Temp. N. Scan across Titan.,,,,,, 2009-284T20:36:25,000T11:24:00,11-Oct-09,INMS,Non-SPASS,Titan,TITAN62,,Titan Flyby,Titan observation,,,,,, 2009-284T22:36:25,000T01:00:00,11-Oct-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,VIMS ridealong with ISS. Stare at Titan. Phase = 165 deg. Lat/Lon = 06N/144 deg. Resolution = 100 - 90 km/px. Temp. N. Obtain 64 x 64 cubes at various exp times for global mapping.,,,,,, 2009-284T23:36:25,000T06:51:00,11-Oct-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-284T23:36:25,000T06:51:00,11-Oct-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS,,,,,, 2009-284T23:36:25,000T06:51:00,11-Oct-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-284T23:36:25,000T06:51:00,11-Oct-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Slow Titan scan,VIMS ridealong with UVIS. Slow scan across Titan . Phase = 165 deg. Lat/Lon = 06N/145 deg. Resolution = 90 - 21 km/px. Temp. X.,,,,,, 2009-285T04:36:25,000T08:00:00,12-Oct-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T62 flyby,"T62 is a south polar, post-dusk flyby, with a minimum altitude of 1000 km. MAG measurements will provide a description of the draping and the pileup of the external magnetic field around Titan near the terminator. It will be also a good complement to T52-T61 in order to characterize the background field for a similar local time with respect to Saturn and different SKR longitudes. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-285T06:27:25,000T00:20:51,12-Oct-09,CIRS,SPASS Rider,SpacecraftActivity,ORSRCS,,,Ride along with ENGR transition,,,,,, 2009-285T06:27:25,000T00:20:51,12-Oct-09,UVIS,SPASS Rider,SpacecraftActivity,ORSRCS,,Solar Occ Titan,This is a solar occultation by Titan. Turn occurs prior to this period; EUV solar occultation port centered on sun Slit aligned tangent to limb. Record data during occultation. Turn back occurs after this period.,,,,,, 2009-285T06:27:25,000T00:20:51,12-Oct-09,VIMS,SPASS Rider,Titan,TRANS,,Transition to RCS,VIMS ridealong durng RWA/RCS transition. Phase = 169 deg. Lat/Lon = 02N/150 deg. Resolution = 21 - 17 km/px. Obtain 64 x 64 cubes for regional mapping during transition.,,,,,, 2009-285T06:36:25,000T01:00:00,12-Oct-09,CAPS,SPASS Rider,Titan,T62INBND,,Inbound 119TI (T62),Inbound 119TI (T62),,,,,, 2009-285T06:36:25,000T01:00:00,12-Oct-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-285T06:36:25,000T01:30:00,12-Oct-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-285T06:48:16,000T00:57:09,12-Oct-09,UVIS,Prime,Sun,USUNOCC,Solar occultation,Solar Occ Titan,This is a solar occultation by Titan. Turn occurs prior to this period; EUV solar occultation port centered on sun Slit aligned tangent to limb. Record data during occultation. Turn back occurs after this period.,,,,,, 2009-285T06:48:16,000T00:57:09,12-Oct-09,CIRS,SPASS Rider,Titan,USUNOCC,Solar occultation,,Ride along with UVIS,,,,,, 2009-285T06:48:16,000T00:57:09,12-Oct-09,VIMS,SPASS Rider,Titan,SOLAROCC,Solar occultation,Solar occ,VIMS ridealong with UVIS solar occ.,,,,,, 2009-285T07:36:25,000T02:00:00,12-Oct-09,CAPS,SPASS Rider,Titan,T62CLOSE,,Closest Approach 119TI (T62),Closest Approach 119TI (T62),,,,,, 2009-285T07:36:25,000T02:00:00,12-Oct-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-285T07:45:25,000T00:30:00,12-Oct-09,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2009-285T07:45:25,000T00:30:00,12-Oct-09,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T07:45:25,000T00:30:00,12-Oct-09,VIMS,SPASS Rider,Titan,LIMBSCAN,Limb scan,Limb scan,VIMS ridealong with CIRS. Slow scan across Titan . Phase = 172 deg. Lat/Lon = 06S/146 deg. Resolution = 7.4 - 2.7 km/px.,,,,,, 2009-285T08:00:25,000T01:12:00,12-Oct-09,INMS,Non-SPASS,Titan,TITAN62,,Titan Flyby,Titan observation,,,,,, 2009-285T08:06:25,000T01:00:00,12-Oct-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-285T08:15:25,000T00:46:00,12-Oct-09,UVIS,Prime,Sun,USUNOCC,Solar occultation,Solar Occ Titan,This is a solar occultation by Titan. Turn occurs prior to this period; EUV solar occultation port centered on sun Slit aligned tangent to limb. Record data during occultation. Turn back occurs after this period.,,,,,, 2009-285T08:15:25,000T00:46:00,12-Oct-09,CIRS,SPASS Rider,Titan,USUNOCC,Solar occultation,,Ride along with UVIS,,,,,, 2009-285T08:15:25,000T00:46:00,12-Oct-09,VIMS,SPASS Rider,Titan,SOLAROCC,Solar occultation,Solar occ,VIMS ridealong with UVIS solar occ,,,,,, 2009-285T09:01:25,000T00:50:00,12-Oct-09,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2009-285T09:01:25,000T00:50:00,12-Oct-09,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-285T09:01:25,000T00:50:00,12-Oct-09,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T09:01:25,000T00:50:00,12-Oct-09,VIMS,SPASS Rider,Titan,FIRLMBMAP,,Titan Scan,VIMS ridealong with CIRS. Scan across Titan . Phase = 26 deg. Lat/Lon = 17S/340 deg. Resolution = 5.0 - 22 km/px.,,,,,, 2009-285T09:06:25,000T01:30:00,12-Oct-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-285T09:12:25,000T11:24:00,12-Oct-09,INMS,Non-SPASS,Titan,TITAN62,,Titan Flyby,Titan observation,,,,,, 2009-285T09:36:25,000T01:00:00,12-Oct-09,CAPS,SPASS Rider,Titan,T62OUTBND,,Outbound 119TI (T62),Outbound 119TI (T62),,,,,, 2009-285T09:36:25,000T01:00:00,12-Oct-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-285T09:51:25,000T01:00:00,12-Oct-09,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2009-285T09:51:25,000T01:00:00,12-Oct-09,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-285T09:51:25,000T01:00:00,12-Oct-09,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T10:36:25,000T16:13:35,12-Oct-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-285T10:36:25,000T15:25:35,12-Oct-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-285T10:51:25,000T00:21:05,12-Oct-09,CIRS,SPASS Rider,SpacecraftActivity,DFPWBIAS,,,Ride along with ENGR transition,,,,,, 2009-285T10:51:25,000T00:21:05,12-Oct-09,VIMS,SPASS Rider,Titan,TRANS,,Transition to RWA,VIMS ridealong durng RCS/RWA transition. Phase = 13 deg. Lat/Lon = 05S/335 deg. Resolution = 22 - 26 km/px. Obtain 64 x 64 cubes for regional mapping during transition.,,,,,, 2009-285T11:12:30,000T06:23:55,12-Oct-09,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2009-285T11:12:30,000T06:23:55,12-Oct-09,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS,,,,,, 2009-285T11:12:30,000T06:23:55,12-Oct-09,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T11:12:30,000T06:23:55,12-Oct-09,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Slow Titan scan,VIMS ridealong with UVIS. Slow scan across Titan . Phase = 13 deg. Lat/Lon = 04S/335 deg. Resolution = 26 - 49 km/px. Temp. X.,,,,,, 2009-285T12:36:25,000T13:25:35,12-Oct-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-285T17:36:25,000T03:00:00,12-Oct-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-285T17:36:25,000T03:00:00,12-Oct-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T17:36:25,000T03:00:00,12-Oct-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,VIMS ridealong with CIRS. Scan across Titan . Phase = 11 deg. Lat/Lon = 01S/340 deg. Resolution = 90 - 121 km/px. Temp. D2.,,,,,, 2009-285T20:36:25,000T02:00:00,12-Oct-09,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,NMO (NAC Monitoring),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T20:36:25,000T02:00:00,12-Oct-09,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Ride along with ISS,,,,,, 2009-285T20:36:25,000T02:00:00,12-Oct-09,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,Global mapping,"VIMS ridealong with ISS. Stare at Titan. Phase = 11 deg. Lat/Lon = 01S/342 deg. Resolution = 121 - 142 km/px. Temp. D2. Obtain 32 x 32, 48 x 48 and 64 x 64 cubes at various exp times for global mapping.",,,,,, 2009-285T20:36:25,000T11:14:46,12-Oct-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-285T22:36:25,000T05:00:00,12-Oct-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,"Titan global mapping. Phase = 11 deg. Lat/Lon = 01S/344 deg. Resolution = 142 - 196 km/px. Temp. B. Obtain 32x32, 48x48 and 64x64 cubes at various exp times for global mapping.",,,,,, 2009-285T22:36:25,000T05:00:00,12-Oct-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-285T23:21:58,000T06:53:02,12-Oct-09,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 15.992610 Rs exit= 9.0007732 Range altitude= 972.91117 km ... -1610.4325,,,,,, 2009-286T02:02:00,000T11:47:00,13-Oct-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-286T02:02:00,000T11:47:00,13-Oct-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-286T02:03:00,000T11:46:00,13-Oct-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-286T02:50:00,000T10:59:00,13-Oct-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-286T04:36:58,000T02:00:00,13-Oct-09,CDA,SPASS Rider,DustRAM direction,RPX0120,,CDA RPXing 2009-286T05:36:58,RPXing at 13.643438 Rs,,,,,, 2009-286T04:49:00,000T09:00:00,13-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-286T05:49:00,000T08:00:00,13-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09286_SP,rider,,,,,, 2009-286T06:15:00,000T07:34:00,13-Oct-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.992610 Rs exit= 9.0007732 Range altitude= 972.91117 km ... -1610.4325,,,,,, 2009-286T07:51:11,000T05:57:49,13-Oct-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-286T13:49:00,001T18:28:00,13-Oct-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-286T13:49:00,001T18:28:00,13-Oct-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-286T13:49:00,000T02:20:58,13-Oct-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.992610 Rs exit= 9.0007732 Range altitude= 972.91117 km ... -1610.4325,,,,,, 2009-286T13:49:00,000T17:02:11,13-Oct-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-286T13:49:00,000T01:06:04,13-Oct-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-286T13:49:00,001T04:45:00,13-Oct-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-286T13:49:00,001T18:29:00,13-Oct-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-286T14:24:00,000T01:05:00,13-Oct-09,VIMS,Prime,Saturn,NHEMDYN,,North Hemisphere dynamics mosaic,"3x2 regional mosaic of northern hemisphere. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2009-286T14:29:00,000T01:00:00,13-Oct-09,ISS,SPASS Rider,Saturn,NHEMDYN,,!!ECLIPSE!!! WAC Saturn lightning search,WAC night side repeated 2xCL1 + 1xHAL at each VIMS footprint. Follow the 3x3 mosaics VIMS pointing (one footprint per 10 min),,,,,, 2009-286T14:55:04,000T04:00:00,13-Oct-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites. Data rate 0 bps, overlaps RHTAR request.",,,,,, 2009-286T14:55:04,000T04:00:00,13-Oct-09,MAG,Non-SPASS,Rhea,RHTAR,Rhea targeted flyby,R2 flyby,"The sole Rhea flyby was a downstream flyby. In order to fully understand if the moon is mass-loading or mass-absorbing type both upstream and downstream flybys are required. The new flybys R2,R3,R4 and R5 will fulfill this requirement.",,,,,, 2009-286T15:50:00,000T04:10:00,13-Oct-09,CIRS,Prime,Rhea,FP1SECLN,CIRS elipse observation,CIRS_119RH_FP1SECLN001_PRIME;,"---LIEN--- SATURN TWT. FP1 entry, (exit; only granted entry). 36>AD>12 mrad. Equatorial, straddles C/A. BEST CASE IN TOUR FOR FP1 ECLIPSE SPATIAL RESOLUTION!!! N 286T16:36:10 (36 mrad, phase=96, LT~05, (-4, 93); target (10, 40) ); C/A 286T16:55:07 (",,,,,, 2009-286T15:50:00,000T04:10:00,13-Oct-09,CIRS,SPASS Rider,Rhea,FP1SECLNX,CIRS elipse observation,Pointing support for Rhea eclipse.,"Four images for pointing verification (two WAC+NAC pairs). Pair #1: UTC=16:30 (40 min. after start of observation). Pair #2 UTC=18:32 (02:42 after start of observation, at exact center time of eclipse - try to set exposure for light refracted around limb of Saturn). Request timing accurate to +/- 1 minute, or call John Pearl (301-286-8487) or Marcia Segura (301-286-6805).",,,,,, 2009-286T15:50:00,000T04:10:00,13-Oct-09,ISS,SPASS Rider,Rhea,FP1SECLN,CIRS elipse observation,Rhea,Rhea,,,,,, 2009-286T15:50:00,000T04:10:00,13-Oct-09,UVIS,SPASS Rider,Rhea,ICYECL,,ICYECL: observe satellite in eclipse,,,,,,, 2009-286T15:50:00,000T04:10:00,13-Oct-09,VIMS,SPASS Rider,Rhea,GEOLOG,Geologic study,,null,,,,,, 2009-286T16:09:58,000T03:50:02,13-Oct-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9845956 Rs exit= 8.9906101 Range altitude= -1615.0948 km ... 4758.2298,,,,,, 2009-286T18:55:04,000T06:19:56,13-Oct-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-286T20:00:00,000T02:25:00,13-Oct-09,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2009-286T20:00:00,000T03:14:00,13-Oct-09,RADAR,SPASS Rider,Other,WU4EQUA,,Warmup for Saturn equatorial map,Warmup for 1st equatorial campaign,,,,,, 2009-286T20:00:00,000T02:25:00,13-Oct-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-286T20:00:00,000T02:25:00,13-Oct-09,VIMS,SPASS Rider,Enceladus,PLMMRHP,,,null,,,,,, 2009-286T20:00:00,000T00:15:00,13-Oct-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9845956 Rs exit= 8.9906101 Range altitude= -1615.0948 km ... 4758.2298,,,,,, 2009-286T20:15:00,000T02:59:00,13-Oct-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9845956 Rs exit= 8.9906101 Range altitude= -1615.0948 km ... 4758.2298,,,,,, 2009-286T22:25:00,000T00:24:00,13-Oct-09,VIMS,Prime,Rhea,RHEA,Rhea,Rhea observation,Image Rhea,,,,,, 2009-286T22:25:00,000T00:24:00,13-Oct-09,CIRS,SPASS Rider,Rhea,RHEA,Rhea,CIRS_119RH_RHEA001_VIMS,rider,,,,,, 2009-286T22:25:00,000T00:24:00,13-Oct-09,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea global color,Rhea 1x1 mosaic,,,,,, 2009-286T22:25:00,000T00:24:00,13-Oct-09,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-286T23:14:00,000T12:16:00,13-Oct-09,RADAR,Prime,Saturn,GLOBALMAP,Global coverage mapping,Saturn first equatorial obs.,map equator; coordinated with VIMS.,,,,,, 2009-286T23:14:00,000T12:16:00,13-Oct-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9845956 Rs exit= 8.9906101 Range altitude= -1615.0948 km ... 4758.2298,,,,,, 2009-287T01:15:00,000T10:55:54,14-Oct-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites. Data rate 0 bps, overlaps INTFLD, MITAR & TETAR requests.",,,,,, 2009-287T01:15:00,000T07:51:00,14-Oct-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-287T04:33:00,000T04:00:00,14-Oct-09,MAG,Non-SPASS,Mimas,MITAR,,M1 flyby,"Monitor the interactio of Mimas with the Saturnian magnetosphere. Data rate 0 bps, overlaps with INTFLD request.",,,,,, 2009-287T05:10:30,000T00:00:01,14-Oct-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.195 Rs, lat = -0 deg, phase = 70 deg",,,,,, 2009-287T06:51:11,000T02:00:00,14-Oct-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-287T06:52:58,000T02:00:00,14-Oct-09,CDA,SPASS Rider,DustRAM direction,RPX0130,,CDA RPXing 2009-287T07:52:58,RPXing at 3.7925509 Rs,,,,,, 2009-287T06:55:00,000T02:00:00,14-Oct-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-287T08:10:54,000T00:55:06,14-Oct-09,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE3 flyby,"Monitor the interaction of Tethys with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD request.",,,,,, 2009-287T08:51:11,000T23:00:00,14-Oct-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-287T09:06:00,000T03:04:54,14-Oct-09,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE3 flyby,Monitor the interaction of Tethys with the Saturnian magnetosphere.,,,,,, 2009-287T11:30:00,000T07:04:00,14-Oct-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9845956 Rs exit= 8.9906101 Range altitude= -1615.0948 km ... 4758.2298,,,,,, 2009-287T12:10:00,000T00:30:00,14-Oct-09,ISS,Prime,Tethys,GEOLOG,Geologic study,Tethys,Tethys,,,,,, 2009-287T12:10:00,000T00:30:00,14-Oct-09,CIRS,SPASS Rider,Tethys,TETHYS,Tethys,CIRS_119TE_TETHYS001_ISS,rider,,,,,, 2009-287T12:10:00,000T00:30:00,14-Oct-09,UVIS,SPASS Rider,Tethys,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2009-287T12:10:00,000T00:30:00,14-Oct-09,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys observation,Image Tethys,,,,,, 2009-287T12:10:54,000T20:06:06,14-Oct-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-287T12:40:00,000T01:25:00,14-Oct-09,ISS,Prime,Mimas,LOWPHASE,Low phase imaging,Mimas,Mimas,,,,,, 2009-287T12:40:00,000T01:25:00,14-Oct-09,CIRS,SPASS Rider,Mimas,MIMAS,Mimas,CIRS_119MI_MIMAS001_ISS,rider,,,,,, 2009-287T12:40:00,000T01:25:00,14-Oct-09,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-287T12:40:00,000T01:25:00,14-Oct-09,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas observation,Image Mimas,,,,,, 2009-287T14:05:00,000T01:05:00,14-Oct-09,ISS,Prime,Enceladus,LOWPHASE,Low phase imaging,Enceladus,Enceladus,,,,,, 2009-287T14:05:00,000T01:05:00,14-Oct-09,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_119EN_ENCEL001_ISS,rider,,,,,, 2009-287T14:05:00,000T01:05:00,14-Oct-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-287T14:05:00,000T01:05:00,14-Oct-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus observation,Image Enceladus,,,,,, 2009-287T15:10:00,000T00:30:00,14-Oct-09,ISS,Prime,Tethys,LOWPHASE,Low phase imaging,Tethys,Tethys,,,,,, 2009-287T15:10:00,000T00:30:00,14-Oct-09,CIRS,SPASS Rider,Tethys,TETHYSLP,,CIRS_119TE_TETHYSLP001_ISS,rider,,,,,, 2009-287T15:10:00,000T00:30:00,14-Oct-09,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-287T15:10:00,000T00:30:00,14-Oct-09,VIMS,SPASS Rider,Tethys,TETHYSLP,,Tethys observation 002,Image Tethys,,,,,, 2009-287T15:53:00,000T02:05:00,14-Oct-09,VIMS,Prime,Saturn,NHEMDYN,,North hemisphere mosaic,"3x3 followed by 1*3 mosaics of northern hemisphere. (10 m in centers: 7 for observing, 3 for repositioning)",,,,,, 2009-287T15:53:00,000T02:05:00,14-Oct-09,ISS,SPASS Rider,Saturn,NHEMDYN,,WAC N hemisp. day movie + NAC lightning search,"3 pickets spaced 1h 30m. 2x1 (day side of half-lit planet) WAC in MT3, CB2, MT2, and BL1.(8 frames per picket 3.5Mb each), data cut by ~30%, changed to CB2 only to cut data.",,,,,, 2009-287T18:34:00,000T09:00:00,14-Oct-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev120 Saturn occultation on 2009/305.",,,,,, 2009-287T18:34:00,003T05:26:00,14-Oct-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.007731 Rs exit= 16.005916 Range altitude= 9372.3738 km ... 3110.4202,,,,,, 2009-287T18:34:00,000T13:43:00,14-Oct-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-287T18:34:00,000T09:00:00,14-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-287T19:34:00,000T08:00:00,14-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09287_SP,rider,,,,,, 2009-288T04:14:00,000T13:41:00,15-Oct-09,VIMS,Prime,Saturn,NHEMDYN,,Northern hemisphere dynamics mosaic 003,Repeated 3x3 global mosaics of the Northern Hemisphere.,,,,,, 2009-288T04:14:00,000T13:41:00,15-Oct-09,ISS,SPASS Rider,Saturn,NHEMDYN,,WAC N hemisp. day movie + NAC lightning search,"11 pickets spaced 1h 30m. 2x1 (day side of half-lit planet) WAC in MT3, CB2, MT2, and BL1.(8 frames per picket 3.5Mb each) +88 images x 4Mb: During VIMS mosaics - NAC CL1 day or night images at each footprint, one image per 10 minutes, data cut by ~30%, f",,,,,, 2009-288T07:51:11,000T19:42:49,15-Oct-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-288T08:17:00,001T09:15:00,15-Oct-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-288T08:17:00,001T09:15:00,15-Oct-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-288T08:17:00,000T15:43:00,15-Oct-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-288T08:17:00,000T10:17:00,15-Oct-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-288T08:18:00,008T08:41:00,15-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-288T18:34:00,000T01:00:00,15-Oct-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-288T18:34:00,000T09:00:00,15-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-288T19:34:00,000T21:58:00,15-Oct-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-289T00:00:00,000T17:32:00,16-Oct-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-289T03:34:00,000T00:56:00,16-Oct-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-289T04:14:00,000T10:38:00,16-Oct-09,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2009-289T04:14:00,000T10:38:00,16-Oct-09,VIMS,SPASS Rider,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFYV ridealong,Ridealong EUVFUV with UVIS,,,,,, 2009-289T04:30:00,000T02:00:00,16-Oct-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-289T06:30:00,000T20:49:00,16-Oct-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-289T14:52:00,000T01:15:00,16-Oct-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 62.2 range 2.4 Mkm",,,,,, 2009-289T14:52:00,000T01:15:00,16-Oct-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-289T14:52:00,000T01:15:00,16-Oct-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-289T16:07:00,000T00:40:00,16-Oct-09,ISS,Prime,Tethys,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Tethys across Titan","Images of mutual event, transit of Tethys across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-289T16:47:00,000T00:52:00,16-Oct-09,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,GLOBAL dynamics mosaic,"3x2 Global mosaic. 6 minutes integration , 2.5 minutes reposition, between frames Repeat",,,,,, 2009-289T16:47:00,000T00:52:00,16-Oct-09,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min. Rduced to 4 images to cut d",,,,,, 2009-289T17:32:00,002T06:05:00,16-Oct-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-289T17:32:00,002T06:05:00,16-Oct-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-289T17:32:00,004T06:28:00,16-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-289T18:19:00,000T09:00:00,16-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-289T19:19:00,000T08:00:00,16-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09289_SP,rider,,,,,, 2009-290T00:00:00,000T00:34:00,17-Oct-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-290T03:19:00,003T23:45:00,17-Oct-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-290T03:59:00,000T01:15:00,17-Oct-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 78.3 range 2.8 Mkm",,,,,, 2009-290T03:59:00,000T01:15:00,17-Oct-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-290T03:59:00,000T01:15:00,17-Oct-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-290T05:14:00,000T01:00:00,17-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-290T06:14:00,000T02:00:00,17-Oct-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-290T08:14:00,000T00:55:00,17-Oct-09,ISS,Prime,Tethys,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Tethys across Titan","Images of mutual event, transit of Tethys across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-290T09:09:00,000T04:00:00,17-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs at ph,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min per footprint. Cycled until observation ends.,,,,,, 2009-290T13:09:00,000T00:30:00,17-Oct-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-290T13:39:00,000T04:00:00,17-Oct-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-290T18:19:00,000T09:00:00,17-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-290T19:19:00,000T08:00:00,17-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09290_SP,rider,,,,,, 2009-291T00:00:00,005T16:59:00,18-Oct-09,CDA,Non-SPASS,Other,RATE010A,,Data rate End:SApo,Range enter= 16.007731 Rs exit= 16.005916 Range altitude= 9372.3738 km ... 3110.4202,,,,,, 2009-291T03:59:00,000T01:00:00,18-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-291T04:59:00,000T12:10:00,18-Oct-09,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2009-291T17:09:00,000T00:30:00,18-Oct-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-291T18:19:00,000T09:00:00,18-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-291T23:37:00,009T10:35:00,18-Oct-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-291T23:37:00,004T17:22:00,18-Oct-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-291T23:37:00,004T17:22:00,18-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-292T03:59:00,000T01:00:00,19-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-292T04:59:00,000T01:00:00,19-Oct-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-292T05:59:00,000T02:52:00,19-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-292T08:51:00,000T00:42:00,19-Oct-09,ISS,Prime,Mimas,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Mimas across Rhea","Images of mutual event, transit of Mimas across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-292T09:33:00,000T08:06:00,19-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs at ph,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min per footprint. Cycled until observation ends.,,,,,, 2009-292T18:19:00,000T09:00:00,19-Oct-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev120 Saturn occultation on 2009/305.",,,,,, 2009-292T18:19:00,000T09:00:00,19-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-293T03:59:00,000T01:00:00,20-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-293T04:59:00,000T00:30:00,20-Oct-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 11","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-293T05:29:00,000T11:55:00,20-Oct-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_119SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-293T05:29:00,000T11:55:00,20-Oct-09,ISS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min. Reduced to 8 mosaics 4 imag",,,,,, 2009-293T05:29:00,000T11:55:00,20-Oct-09,VIMS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 002,Dynamics ridealong with CIRS composition map,,,,,, 2009-293T18:04:00,000T09:00:00,20-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-293T19:04:00,000T08:00:00,20-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09293_SP,rider,,,,,, 2009-294T00:00:00,006T00:00:00,21-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-294T03:04:00,001T00:00:00,21-Oct-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-294T03:44:00,000T13:40:00,21-Oct-09,CIRS,Prime,Saturn,MIRTMAP,,CIRS_119SA_MIRTMAP001_PRIME,"Northern hemisphere Determine upper troposphere and tropopause temperature sacrifice longitude coverage for latitude coverage, 10 deg bins",,,,,, 2009-294T03:44:00,000T13:40:00,21-Oct-09,ISS,SPASS Rider,Saturn,MIRTMAP,,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min. Reduced to 8 mosaics 4 imag",,,,,, 2009-294T03:44:00,000T13:40:00,21-Oct-09,VIMS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 006,Dynamics ridealong with CIRS composition map,,,,,, 2009-294T18:04:00,000T09:00:00,21-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-294T19:04:00,000T08:00:00,21-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_119IC_DSCAL09294_SP,rider,,,,,, 2009-295T03:04:00,000T18:56:00,22-Oct-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-295T03:44:00,000T01:00:00,22-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-295T04:44:00,000T02:39:00,22-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-295T07:23:00,000T00:44:00,22-Oct-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Dione","Images of mutual event, transit of Rhea across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-295T08:07:00,000T03:00:00,22-Oct-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Bestla,Observation of Bestla,,,,,, 2009-295T08:07:00,000T03:00:00,22-Oct-09,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-295T11:07:00,000T06:17:00,22-Oct-09,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2009-295T18:04:00,000T09:00:00,22-Oct-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev120 Saturn occultation on 2009/305.",,,,,, 2009-295T18:04:00,000T09:00:00,22-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-295T22:00:00,000T02:00:00,22-Oct-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-296T00:00:00,000T16:59:00,23-Oct-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-296T03:44:00,000T10:00:00,23-Oct-09,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2009-296T13:44:00,000T12:20:00,23-Oct-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_119SA_COMPSIT005,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-296T13:44:00,000T12:20:00,23-Oct-09,ISS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.Reduced to 8 mosaics/4 im.",,,,,, 2009-296T13:44:00,000T12:20:00,23-Oct-09,VIMS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 004,Dynamics ridealong with CIRS composition map,,,,,, 2009-296T16:58:59,000T00:00:01,23-Oct-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 19.0 d, inc = 0.5 deg, r = 42.294 Rs, phase = 110 deg",,,,,, 2009-296T16:59:00,004T17:13:00,23-Oct-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-296T16:59:00,005T07:01:58,23-Oct-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.007731 Rs exit= 16.005916 Range altitude= 9372.3738 km ... 3110.4202,,,,,, 2009-296T16:59:00,006T09:36:00,23-Oct-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-296T16:59:00,002T20:05:00,23-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-296T16:59:00,002T20:05:00,23-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-297T02:04:00,000T01:00:00,24-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-297T04:04:00,000T09:00:00,24-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-297T05:04:00,000T08:00:00,24-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09297_SP,rider,,,,,, 2009-297T13:44:00,000T03:00:00,24-Oct-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Bestla,Observation of Bestla,,,,,, 2009-297T13:44:00,000T03:00:00,24-Oct-09,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-297T16:44:00,000T02:00:00,24-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-297T18:44:00,000T07:40:00,24-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-297T18:44:00,000T07:40:00,24-Oct-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #1,ISS Lightning ridealong,,,,,, 2009-298T02:24:00,000T01:00:00,25-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-298T03:24:00,000T10:20:00,25-Oct-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-298T04:04:00,000T09:00:00,25-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-298T13:44:00,000T06:40:00,25-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-298T13:44:00,000T06:40:00,25-Oct-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #2,ISS Lightning ridealong,,,,,, 2009-298T20:24:00,000T06:00:00,25-Oct-09,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observation of 1 of 3 IR stars: CW Leonis, Eta Carinae, Alpha Orionis. Slew to star; settle; execute small box scan; return to waypoint. Observation of each star to take 6 hours; need not be executed contiguously.",,,,,, 2009-299T02:24:00,000T01:00:00,26-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-299T04:04:00,000T09:00:00,26-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-299T05:04:00,000T08:00:00,26-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09299_SP,rider,,,,,, 2009-299T13:04:00,001T23:46:00,26-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-299T13:04:00,000T23:46:00,26-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-299T13:44:00,000T01:15:00,26-Oct-09,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 131 range 1.2 Mkm",,,,,, 2009-299T13:44:00,000T01:15:00,26-Oct-09,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-299T13:44:00,000T01:15:00,26-Oct-09,UVIS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-299T14:59:00,000T05:13:00,26-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum . 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-299T14:59:00,000T05:13:00,26-Oct-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #3,ISS Lightning ridealong,,,,,, 2009-299T20:12:00,000T00:41:00,26-Oct-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Tethys","Images of mutual event, transit of Rhea across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-299T20:53:00,000T04:41:00,26-Oct-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-300T00:00:00,003T08:27:00,27-Oct-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-300T01:34:00,000T00:41:00,27-Oct-09,ISS,Prime,Enceladus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Enceladus across Tethys","Images of mutual event, transit of Enceladus across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-300T02:15:00,000T01:00:00,27-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-300T03:50:00,000T09:00:00,27-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-300T04:50:00,000T08:00:00,27-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09300_SP,rider,,,,,, 2009-300T12:50:00,000T21:22:00,27-Oct-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-300T13:30:00,000T05:40:00,27-Oct-09,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_120_SCATTERED_SUNLIGHT_TEST_PRIME,"Sunlight falling on the CIRS telescope can potentially be scattered into the instrument by mirror imperfections. We need to quantify the effect of ring particle impacts on the mirror performance. This requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; continuous radial scans are required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scans will begin 40 degrees from FPB, and will scan to 10 degrees of FPB at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time VIMS will integrate for TBD seconds and CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction back to the initial position; to determine whether scattering is asymmetric with respect to the FPB axis, 3 such scans will be made. 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from 40 degrees +Z to 10 degrees +Z and back to 40 degrees +Z. 2) From 40 degrees in -X on the X axis, to 10 degrees on the -X axis, to 40 degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 10 degrees -Z and back to 40 degrees -Z.",,,,,, 2009-300T19:10:00,000T01:00:00,27-Oct-09,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Titan across Rhea","Images of mutual event, transit of Titan across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-300T20:10:00,000T01:00:00,27-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-300T21:10:00,000T06:00:00,27-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-300T21:10:00,000T06:00:00,27-Oct-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #4,ISS Lightning ridealong,,,,,, 2009-301T03:50:00,000T09:00:00,28-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-301T04:50:00,000T08:00:00,28-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09301_SP,rider,,,,,, 2009-301T10:12:00,001T22:15:00,28-Oct-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-301T10:12:00,003T15:15:00,28-Oct-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-301T12:50:00,002T13:45:00,28-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-301T13:30:00,000T02:00:00,28-Oct-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-301T15:30:00,000T06:55:00,28-Oct-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-301T15:30:00,000T06:55:00,28-Oct-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #5,ISS Lightning ridealong,,,,,, 2009-301T22:25:00,000T01:00:00,28-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-301T23:25:00,000T10:00:00,28-Oct-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_120SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-301T23:25:00,000T10:00:00,28-Oct-09,ISS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.Reduced to 6 mosaics/4 im.",,,,,, 2009-301T23:25:00,000T10:00:00,28-Oct-09,VIMS,SPASS Rider,Saturn,GLODYNA,,Global dynamics CIRS COMPSIT Ridealong,Global mosaic CIRS COMPSIT ridealong,,,,,, 2009-302T00:00:00,003T03:00:00,29-Oct-09,CDA,Non-SPASS,Other,RATE010A,,Data rate Enter:SApo,Range enter= 16.007731 Rs exit= 16.005916 Range altitude= 9372.3738 km ... 3110.4202,,,,,, 2009-302T09:25:00,000T04:00:00,29-Oct-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-302T12:25:00,000T03:00:00,29-Oct-09,RADAR,SPASS Rider,Other,WU4SEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2009-302T12:26:20,000T00:00:01,29-Oct-09,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2009-302T13:25:00,000T02:00:00,29-Oct-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-302T15:25:00,000T01:30:00,29-Oct-09,RADAR,Prime,Titan,SEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2009-302T17:35:00,000T09:00:00,29-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-302T18:35:00,000T08:00:00,29-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09302_SP,rider,,,,,, 2009-303T02:35:00,001T00:00:00,30-Oct-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-303T03:15:00,000T01:15:00,30-Oct-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 85.9 range 1.3 Mkm",,,,,, 2009-303T03:15:00,000T01:15:00,30-Oct-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-303T03:15:00,000T01:15:00,30-Oct-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-303T04:30:00,000T01:00:00,30-Oct-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-303T05:30:00,000T11:25:00,30-Oct-09,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 9 EG130 phase at priority 2.,,,,,, 2009-303T08:27:00,001T17:00:00,30-Oct-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-303T08:27:00,002T04:08:00,30-Oct-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-303T17:35:00,000T09:00:00,30-Oct-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-303T18:35:00,000T08:00:00,30-Oct-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09303_SP,rider,,,,,, 2009-304T02:35:00,001T10:00:00,31-Oct-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-304T02:35:00,000T22:54:00,31-Oct-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-304T03:15:00,000T01:15:00,31-Oct-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86 range 1.3 Mkm",,,,,, 2009-304T03:15:00,000T01:15:00,31-Oct-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-304T03:15:00,000T01:15:00,31-Oct-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-304T04:30:00,000T04:00:00,31-Oct-09,ISS,Prime,Saturn,WALGTNG,Lightning search,WAC Saturn lightning search from ~10Rs,3 2x2 WAC 3x1 N to S stripes of the dark side repeated 3xCL1 + 1xHAL+IR2+UV2 at each footprint. 20 min per footprint.,,,,,, 2009-304T08:30:00,000T03:35:00,31-Oct-09,ISS,Prime,RingE,HPLELR,,E Ring High Phase Observation,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-304T12:05:00,000T12:00:00,31-Oct-09,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 001,"3x3 Global mosaic. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2009-304T12:05:00,000T12:00:00,31-Oct-09,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.Reduced to 8 mosaics/4 im.",,,,,, 2009-305T00:00:00,000T00:34:00,1-Nov-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-305T00:05:00,000T02:50:00,1-Nov-09,CIRS,Prime,Saturn,NADIROCC,Occultation,NADIROCC egress OR ingress,"Helium abundance measurement at the RSS ingress or egress occultation point. If RSS request deleted, this can be, too.",,,,,, 2009-305T01:27:00,000T11:08:00,1-Nov-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-305T01:27:00,000T11:08:00,1-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-305T01:29:00,000T11:06:00,1-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-305T03:00:00,000T12:37:58,1-Nov-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.993903 Rs exit= 9.0042767 Range altitude= 3104.5008 km ... -104.59229,,,,,, 2009-305T03:35:00,000T09:00:00,1-Nov-09,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' mass,Downlink pass at Ka-band for Enceladus' mass determination and for improving locally Cassini orbit.,,,,,, 2009-305T03:35:00,000T09:00:00,1-Nov-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-305T03:35:00,000T09:00:00,1-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-305T04:35:00,000T08:00:00,1-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09305_SP,rider,,,,,, 2009-305T12:35:00,000T18:36:58,1-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-305T12:35:00,000T18:06:58,1-Nov-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-305T12:35:00,000T01:25:00,1-Nov-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-305T12:35:00,000T12:09:00,1-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-305T12:35:00,000T02:00:00,1-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-305T12:50:00,000T01:30:00,1-Nov-09,UVIS,Prime,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-305T12:50:00,000T01:30:00,1-Nov-09,CIRS,SPASS Rider,Rhea,RHEAUVIS,,CIRS_120RH_RHEAUVIS001_UVIS,"rider, FP1 and FP3 only",,,,,, 2009-305T12:50:00,000T02:05:00,1-Nov-09,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS Thermal Stabilization 120 pre-Occ,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-305T12:50:00,000T01:30:00,1-Nov-09,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,from CCR 2/2009,,,,,, 2009-305T14:00:00,000T02:00:00,1-Nov-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2009-305T14:06:58,000T02:00:00,1-Nov-09,CDA,SPASS Rider,DustRAM direction,RPX0140,,CDA RPXing 2009-305T15:06:58,RPXing at 9.2615807 Rs,,,,,, 2009-305T14:35:00,000T01:00:00,1-Nov-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-305T14:57:00,000T00:20:00,1-Nov-09,ISS,Prime,Enceladus,PLMSCECL,,High phase obs with s/c in eclipse,Very High phase obs with s/c in eclipse. Absolutely critical. Vital. WE REALLY NEED THIS!!!!!,,,,,, 2009-305T14:57:00,000T00:20:00,1-Nov-09,CIRS,SPASS Rider,Enceladus,PLMSCECL,,CIRS_120EN_PLMSCECL001_ISS,"rider, FP1 and FP3 only",,,,,, 2009-305T14:57:00,000T00:20:00,1-Nov-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-305T14:57:00,000T00:23:00,1-Nov-09,VIMS,SPASS Rider,Enceladus,PLMSCECL,,Enceladus Plume,from CCR 2/2009,,,,,, 2009-305T15:35:00,000T15:36:58,1-Nov-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-305T15:37:00,000T01:39:00,1-Nov-09,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS Atmospheric Occultation 120 in,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2009-305T15:37:58,000T06:36:02,1-Nov-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9881069 Rs exit= 8.9853125 Range altitude= -111.29710 km ... 3556.8321,,,,,, 2009-305T16:00:00,000T13:42:00,1-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-305T17:16:00,000T00:43:00,1-Nov-09,CIRS,Prime,Enceladus,FP13DKMAP,,CIRS_120EN_FP1DKMAP001_PRIME;,"FP1 and FP3 only, throughout 17:16-17:46, 3 minutes shutter closed, then three 9-minute FP3 full-disk scans at 6 murad/sec. 17:46-17:59, 3 minute FP1 stare at the ring 6 mrad to the right of Enceladus (for background measurement), then 6 minute FP1 stare at Enceladus, then 3 minute stare at the ring 6 mrad to the left of Enceladus.",,,,,, 2009-305T17:16:00,000T00:43:00,1-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-305T17:16:00,000T00:43:00,1-Nov-09,VIMS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,Enceladus,from CCR 2/2009,,,,,, 2009-305T17:59:00,000T00:45:00,1-Nov-09,ISS,Prime,Enceladus,PLMSCECL,,High phase obs with s/c in eclipse,Very High phase obs with s/c in eclipse. Jets obscured by rings.,,,,,, 2009-305T17:59:00,000T00:45:00,1-Nov-09,CIRS,SPASS Rider,Enceladus,ENPLUME,,CIRS_120EN_ENPLUME001_ISS,"rider, FP1 and FP3 only",,,,,, 2009-305T17:59:00,000T00:45:00,1-Nov-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-305T17:59:00,000T00:45:00,1-Nov-09,VIMS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,Enceladus,from CCR 2/2009,,,,,, 2009-305T18:44:00,000T02:02:00,1-Nov-09,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Atmospheric Occultation 120out,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2009-305T21:25:00,000T00:49:00,1-Nov-09,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2009-305T21:25:00,000T00:49:00,1-Nov-09,CIRS,SPASS Rider,Enceladus,PLMHRHP,,CIRS_120EN_PLMHRHP001_ISS,"rider, FP1 and FP3 only",,,,,, 2009-305T21:25:00,000T00:49:00,1-Nov-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-305T21:25:00,000T00:49:00,1-Nov-09,VIMS,SPASS Rider,Enceladus,PLMHRHP,,Enceladus,from CCR 2/2009,,,,,, 2009-305T22:14:00,000T02:58:00,1-Nov-09,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2009-305T22:14:00,000T02:58:00,1-Nov-09,CIRS,SPASS Rider,Enceladus,PLMHRHP,,CIRS_120EN_PLMHRHP002_ISS,"rider, FP1 and FP3 only",,,,,, 2009-305T22:14:00,000T02:58:00,1-Nov-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-305T22:14:00,000T02:58:00,1-Nov-09,VIMS,SPASS Rider,Enceladus,PLMHRHP,,Enceladus,from CCR 2/2009,,,,,, 2009-305T22:14:00,000T00:15:00,1-Nov-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9881069 Rs exit= 8.9853125 Range altitude= -111.29710 km ... 3556.8321,,,,,, 2009-305T22:14:00,000T02:59:58,1-Nov-09,RADAR,Non-SPASS,Other,WARMUP4EN,RADAR warmup,Warmup with data before Enceladus,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2009-305T22:29:00,000T02:21:00,1-Nov-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9881069 Rs exit= 8.9853125 Range altitude= -111.29710 km ... 3556.8321,,,,,, 2009-306T00:44:00,000T08:58:00,2-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites. Data rate 0 bps, overlaps INTFLD, ENTAR requests.",,,,,, 2009-306T00:44:00,000T07:50:00,2-Nov-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-306T00:50:00,000T05:54:00,2-Nov-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 8.9881069 Rs exit= 8.9853125 Range altitude= -111.29710 km ... 3556.8321,,,,,, 2009-306T01:13:58,000T05:28:00,2-Nov-09,RADAR,Prime,Enceladus,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Enceladus,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2009-306T04:38:58,000T00:00:01,2-Nov-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.201 Rs, lat = -0 deg, phase = 70 deg",,,,,, 2009-306T05:42:00,000T01:00:58,2-Nov-09,INMS,Non-SPASS,Enceladus,ENCEL7,,Enceladus encounter,Enceladus observation,,,,,, 2009-306T06:41:58,000T02:00:00,2-Nov-09,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 120EN Campaign,Part of 120EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2009-306T06:42:58,000T01:21:00,2-Nov-09,INMS,Prime,Enceladus,ENCEL7,,Enceladus encounter,Prime Enceladus observation,,,,,, 2009-306T06:42:58,000T01:21:00,2-Nov-09,ISS,SPASS Rider,Enceladus,ENCEL7,,Enceladus Flyby C/A imaging,INMS will drag ISS FOV across Enceladus during closest approach.,,,,,, 2009-306T06:44:00,000T10:16:00,2-Nov-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0014843 Rs exit= 15.992255 Range altitude= 3568.0008 km ... 8060.8021,,,,,, 2009-306T07:00:00,000T01:40:00,2-Nov-09,CDA,SPASS Rider,DustRAM direction,ENC7,,ENC INMS-CDA 2009-306T0:42 MMH,"Enceladus flyby 306T07:42, INMS+CDA, E7, RPXing at 2009-306T08:36:58, 4.3502919 Rs",,,,,, 2009-306T07:11:58,000T01:00:00,2-Nov-09,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-306T07:11:58,000T00:45:00,2-Nov-09,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2009-306T07:36:58,000T00:07:00,2-Nov-09,CIRS,SPASS Rider,Enceladus,ENCEL7,,CIRS_120EN_ENCEL7001_INMS;,Ridealong with INMS plume observation: CIRS fields of view are dragged across Enceladus for about 66 seconds centered on closest approach. Shutter closed first 3 minutes. 15 cm-1 resolution.,,,,,, 2009-306T07:39:58,000T00:04:00,2-Nov-09,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Ride-along with CIRS on high resolution scan across Enceladus,,,,,, 2009-306T07:56:58,000T00:15:00,2-Nov-09,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2009-306T08:03:58,000T00:10:00,2-Nov-09,CIRS,Prime,Enceladus,FP3SPMAP,,CIRS_120EN_FP3SPMAP001_PRIME;,"Stare FP3 at RA 183.03, Dec 4.775 throughout- the stare will begin on dark sky off the limb, then the south pole of Enceladus, and a potentially active fracture at 170 W, 65 S, will sweep through the field of view.",,,,,, 2009-306T08:03:58,000T00:10:00,2-Nov-09,ISS,SPASS Rider,Enceladus,FP3SPMAP,,Enceladus,Enceladus,,,,,, 2009-306T08:03:58,000T00:10:00,2-Nov-09,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Ride-along with CIRS on high resolution scan across Enceladus,,,,,, 2009-306T08:03:58,000T00:10:00,2-Nov-09,VIMS,SPASS Rider,Enceladus,SPFP3MAP,,Enceladus,from CCR 2/2009,,,,,, 2009-306T08:03:58,000T01:38:01,2-Nov-09,INMS,Non-SPASS,Enceladus,ENCEL7,,Enceladus encounter,Enceladus observation,,,,,, 2009-306T08:11:58,000T23:35:01,2-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-306T08:11:58,000T01:23:01,2-Nov-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-306T08:13:58,000T01:28:00,2-Nov-09,UVIS,Prime,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV of plume occulting Saturn,"Image plume with Saturn in the background. Stare at Saturn, targeted such that Enceladus' plume moves from pixel to pixel as Enceladus moves relative to Saturn from the s/c perspective.",,,,,, 2009-306T08:13:58,000T01:28:00,2-Nov-09,CIRS,SPASS Rider,Enceladus,ENUVIS,,CIRS_120EN_ENUVIS001_UVIS,rider,,,,,, 2009-306T08:13:58,000T01:28:00,2-Nov-09,VIMS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,Enceladus,from CCR 2/2009,,,,,, 2009-306T08:34:00,000T01:08:00,2-Nov-09,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2009-306T08:41:58,001T03:53:02,2-Nov-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-306T09:35:00,000T06:25:00,2-Nov-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-306T09:41:58,000T00:22:00,2-Nov-09,CIRS,SPASS Rider,Enceladus,FP1STARE,CIRS FP1 stare,CIRS_120EN_FP1STARE001_ENGR,rider,,,,,, 2009-306T09:41:58,000T00:22:00,2-Nov-09,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV of Plume Occulting Saturn,"Image plume with Saturn in the background. Stare at Saturn, targeted such that Enceladus' plume moves from pixel to pixel as Enceladus moves relative to Saturn from the s/c perspective.",,,,,, 2009-306T09:41:58,000T00:22:00,2-Nov-09,VIMS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,Enceladus,from CCR 2/2009,,,,,, 2009-306T09:42:00,001T02:53:00,2-Nov-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-306T09:42:00,000T22:05:00,2-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-306T10:03:58,000T01:38:00,2-Nov-09,CIRS,Prime,Enceladus,FP3DAYMAP,CIRS FP3 daytime map,CIRS_120EN_ENFP1MAP001_PRIME;,"10:04-11:04 Global FP3 map at 8 murad/sec. 3 swaths? In Saturn transit most of the time (egress 11:00) 11:04-11:07 FP3 stare at deep space (avoiding the rings) at the end of the global map, for calibration. 11:07-11:12 FP1 stare at disk center. 11:12-11:42 180 degree secondary axis turn, with FP3 centered on Enceladus if that is practical. Shutter closed for the first 3 minutes.",,,,,, 2009-306T10:03:58,000T01:38:00,2-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-306T10:03:58,000T01:38:00,2-Nov-09,VIMS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,Enceladus,from CCR 2/2009,,,,,, 2009-306T11:44:00,000T02:20:00,2-Nov-09,VIMS,Prime,Enceladus,ICYLON,Icy satellite longitudinal coverage,Enceladus,from CCR 2/2009,,,,,, 2009-306T11:44:00,000T02:20:00,2-Nov-09,CIRS,SPASS Rider,Enceladus,ENVIMS,,CIRS_120EN_ENVIMS001_VIMS,"rider, FP1 and FP3 only",,,,,, 2009-306T11:44:00,000T02:20:00,2-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-306T14:04:00,000T02:16:00,2-Nov-09,UVIS,Prime,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-306T14:04:00,000T02:16:00,2-Nov-09,CIRS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,CIRS_120TE_ICYLON001_UVIS,"rider, FP1 and FP3 only",,,,,, 2009-306T14:04:00,000T02:14:00,2-Nov-09,ISS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,Tethys,Tethys,,,,,, 2009-306T14:04:00,000T02:12:00,2-Nov-09,VIMS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,Tethys,from CCR 2/2009,,,,,, 2009-306T16:00:00,000T15:49:00,2-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-306T17:00:00,000T09:00:00,2-Nov-09,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' mass,Downlink pass at Ka-band for Enceladus' mass determination and for improving locally Cassini orbit.,,,,,, 2009-306T17:00:00,008T23:57:00,2-Nov-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.004270 Rs exit= 16.006120 Range altitude= 8068.0890 km ... 3097.9046,,,,,, 2009-306T17:00:00,000T09:00:00,2-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-306T18:00:00,000T04:00:00,2-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09307_SP,rider,,,,,, 2009-307T02:40:00,000T06:00:00,3-Nov-09,UVIS,Prime,Dione,ICYSTARE,,ICYSTARE: Investigate volatiles near Dione,Long stare for tenuous atmosphere search.,,,,,, 2009-307T07:47:00,000T04:48:00,3-Nov-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-307T07:47:00,000T04:48:00,3-Nov-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-307T07:49:00,000T04:46:00,3-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-307T12:35:00,001T04:22:00,3-Nov-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-307T12:35:00,001T04:22:00,3-Nov-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-307T12:35:00,000T10:25:00,3-Nov-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-307T12:35:00,001T04:22:00,3-Nov-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-307T12:35:00,001T00:00:00,3-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-307T12:35:00,000T15:00:00,3-Nov-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-307T13:15:00,000T01:15:00,3-Nov-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86 range 2.1 Mkm",,,,,, 2009-307T13:15:00,000T01:15:00,3-Nov-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-307T13:15:00,000T01:15:00,3-Nov-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-307T14:30:00,000T11:05:00,3-Nov-09,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2009-307T23:00:00,000T02:00:00,3-Nov-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-308T01:00:00,001T11:20:00,4-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-308T01:35:00,000T01:00:00,4-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-308T03:35:00,000T09:00:00,4-Nov-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-308T03:35:00,000T09:00:00,4-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-308T04:35:00,000T04:00:00,4-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09308_SP,rider,,,,,, 2009-308T12:35:00,007T04:22:00,4-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-308T12:35:00,000T04:22:00,4-Nov-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-308T13:15:00,000T00:30:00,4-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-308T13:45:00,000T11:55:00,4-Nov-09,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn FIRMAP,"FIRMAP, scanning N. hemisphere + pole, may be split in half by downlink",,,,,, 2009-308T13:45:00,000T11:55:00,4-Nov-09,VIMS,SPASS Rider,Saturn,GLODYNA,,Global dynamics CIRS FIRMAP idealong,Global mosaic CIRS FIRMAP ridealong,,,,,, 2009-308T16:57:00,004T06:00:00,4-Nov-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-308T16:57:00,002T06:00:00,4-Nov-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-308T16:57:00,003T07:03:00,4-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-309T01:40:00,000T01:00:00,5-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-309T03:20:00,000T09:00:00,5-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-309T04:20:00,000T08:00:00,5-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09309_SP,rider,,,,,, 2009-309T12:20:00,001T00:01:00,5-Nov-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-309T13:00:00,000T02:00:00,5-Nov-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-309T15:00:00,000T00:30:00,5-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-309T15:30:00,000T02:11:00,5-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. 2x1 WAC dayside. Cycled while observation lasts.13 images per 90 min,,,,,, 2009-309T15:30:00,000T02:11:00,5-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #8,ISS Lightning ridealong,,,,,, 2009-309T17:41:00,000T01:00:00,5-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-309T18:41:00,000T08:00:00,5-Nov-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_120SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-309T18:41:00,000T08:00:00,5-Nov-09,VIMS,SPASS Rider,Saturn,GLODYNA,,Global dynamics CIRS COMPSIT ridealong,Global mosaic CIRS COMPSIT ridealong,,,,,, 2009-309T22:57:00,001T00:00:00,5-Nov-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-310T03:21:00,000T09:00:00,6-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-310T04:21:00,000T04:00:00,6-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09310_SP,rider,,,,,, 2009-310T12:21:00,005T00:39:00,6-Nov-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-310T13:01:00,000T02:00:00,6-Nov-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-310T15:01:00,000T02:18:00,6-Nov-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-310T17:19:00,000T02:00:00,6-Nov-09,CDA,Prime,Other,ISD000001,,ISD survery campaign,Range enter= 16.004270 Rs exit= 16.006120 Range altitude= 8068.0890 km ... 3097.9046 ISD survery campaign. CDA to articulation= 77deg.,,,,,, 2009-310T19:19:00,000T02:35:00,6-Nov-09,ISS,Prime,Saturn,TITANSHAD,,Titan Shadow Images,NAC images of Titan's shadow on Saturn. It is useful for Titan aerosol science. This is a unique geometry that occurs only a few times the XM and not at all in the nominal mission or XXM.,,,,,, 2009-310T21:54:00,000T03:17:00,6-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. 2x1 WAC dayside. Cycled while observation lasts.13 images per 90 min,,,,,, 2009-310T21:54:00,000T03:17:00,6-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #9,ISS Lightning ridealong,,,,,, 2009-310T22:57:00,004T18:00:00,6-Nov-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-311T01:11:00,000T01:00:00,7-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-311T02:11:00,000T00:30:00,7-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-311T03:21:00,000T09:00:00,7-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-311T04:21:00,000T04:00:00,7-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09311_SP,rider,,,,,, 2009-311T13:01:00,000T00:30:00,7-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-311T13:31:00,000T02:00:00,7-Nov-09,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-311T15:31:00,000T01:40:00,7-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.13 images per 90 min,,,,,, 2009-311T15:31:00,000T01:40:00,7-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #10,ISS Lightning ridealong,,,,,, 2009-311T17:11:00,000T08:00:00,7-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 1. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-312T00:00:00,005T19:21:00,8-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-312T01:11:00,000T01:00:00,8-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-312T02:11:00,000T00:30:00,8-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-312T03:21:00,000T09:00:00,8-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-312T13:01:00,000T00:30:00,8-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-312T13:31:00,000T01:48:00,8-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.13 images per 90 min,,,,,, 2009-312T13:31:00,000T01:48:00,8-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #11,ISS Lightning ridealong,,,,,, 2009-312T15:19:00,000T02:00:00,8-Nov-09,CAPS,Prime,Sun,MAGBNDPTG,MAPS magnetosphere boundary campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-312T17:19:00,000T00:44:00,8-Nov-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Janus","Images of mutual event, transit of Rhea across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-312T18:03:00,000T01:35:00,8-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-312T18:03:00,000T01:35:00,8-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #12,ISS Lightning ridealong,,,,,, 2009-312T19:38:00,000T00:48:00,8-Nov-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Janus","Images of mutual event, transit of Rhea across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-312T20:26:00,000T08:00:00,8-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 2. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-312T22:57:00,004T20:24:00,8-Nov-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-313T04:26:00,000T01:00:00,9-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-313T05:26:00,000T04:30:00,9-Nov-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Bestla,Observation of Bestla,,,,,, 2009-313T05:26:00,000T04:30:00,9-Nov-09,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-313T10:36:00,000T09:00:00,9-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-313T20:16:00,000T08:00:00,9-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 3. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-314T04:16:00,000T09:34:00,10-Nov-09,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2009-314T04:16:00,000T09:34:00,10-Nov-09,VIMS,SPASS Rider,RingE,LRLEMP,,Edge-on observation of E ring around equinox,"Low-res, low elevation, medium phase observation of E ring",,,,,, 2009-314T13:50:00,000T01:36:00,10-Nov-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-314T15:26:00,000T01:00:00,10-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-314T16:26:00,000T10:20:00,10-Nov-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-314T17:06:00,000T09:00:00,10-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-314T18:06:00,000T04:00:00,10-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_120IC_DSCAL09314_SP,rider,,,,,, 2009-315T02:46:00,000T01:15:00,11-Nov-09,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 118.3 range 1.4 Mkm",,,,,, 2009-315T02:46:00,000T01:15:00,11-Nov-09,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-315T02:46:00,000T01:15:00,11-Nov-09,UVIS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-315T04:01:00,000T04:54:00,11-Nov-09,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2009-315T04:01:00,000T04:54:00,11-Nov-09,VIMS,SPASS Rider,RingE,LRLEMP,,Edge-on observation of E ring around equinox,"Low-res, low elevation, medium phase observation of E ring",,,,,, 2009-315T08:55:00,000T00:44:00,11-Nov-09,ISS,Prime,Janus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Janus across Rhea","Images of mutual event, transit of Janus across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-315T09:39:00,000T01:43:00,11-Nov-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-315T11:22:00,000T03:00:00,11-Nov-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-315T11:22:00,000T03:00:00,11-Nov-09,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2009-315T13:00:00,000T02:00:00,11-Nov-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-315T14:22:00,000T08:00:00,11-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 4. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-315T15:00:00,000T01:57:00,11-Nov-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-315T16:57:00,002T02:24:00,11-Nov-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-315T16:57:00,002T02:24:00,11-Nov-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S55,Range enter= 16.004270 Rs exit= 16.006120 Range altitude= 8068.0890 km ... 3097.9046,,,,,, 2009-315T16:57:00,000T19:09:00,11-Nov-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-315T16:57:00,002T02:24:00,11-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-315T16:57:04,000T00:00:01,11-Nov-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 19.0 d, inc = 0.5 deg, r = 42.367 Rs, phase = 110 deg",,,,,, 2009-315T22:22:00,000T00:48:00,11-Nov-09,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Rhea","Images of mutual event, transit of Dione across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-315T23:10:00,000T00:47:00,11-Nov-09,ISS,Prime,Tethys,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Tethys across Enceladus","Images of mutual event, transit of Tethys across Enceladus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-315T23:57:00,000T01:29:00,11-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-316T01:26:00,000T01:00:00,12-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-316T03:06:00,000T09:00:00,12-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-316T04:06:00,000T04:00:00,12-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09316_SP,rider,,,,,, 2009-316T12:06:00,001T07:15:00,12-Nov-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-316T12:46:00,000T03:00:00,12-Nov-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Kiviuq,Observation of Kiviuq,,,,,, 2009-316T12:46:00,000T03:00:00,12-Nov-09,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-316T15:46:00,000T01:00:00,12-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-316T16:46:00,000T05:55:00,12-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts. Cut in half.,,,,,, 2009-316T16:46:00,000T05:55:00,12-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #1,ISS Lightning ridealong,,,,,, 2009-316T22:41:00,000T02:00:00,12-Nov-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-317T00:41:00,000T08:00:00,13-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 5. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-317T08:41:00,000T01:00:00,13-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-317T10:21:00,000T09:00:00,13-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-317T19:21:00,001T06:30:00,13-Nov-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-317T19:21:00,004T14:41:00,13-Nov-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-317T19:21:00,006T04:04:58,13-Nov-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S55,Range enter= 16.004270 Rs exit= 16.006120 Range altitude= 8068.0890 km ... 3097.9046,,,,,, 2009-317T19:21:00,000T00:43:00,13-Nov-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-317T19:21:00,001T04:39:00,13-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-317T19:21:00,001T06:30:00,13-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-317T19:26:00,000T00:02:00,13-Nov-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S55 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-317T20:01:00,000T01:15:00,13-Nov-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 87.7 range 1.7 Mkm",,,,,, 2009-317T20:01:00,000T01:15:00,13-Nov-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-317T20:01:00,000T01:15:00,13-Nov-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-317T20:04:00,000T00:07:00,13-Nov-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-317T20:11:00,000T00:05:00,13-Nov-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-317T20:16:00,000T00:33:00,13-Nov-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-317T20:49:00,000T10:54:00,13-Nov-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,"Startup sequence. Load FSW, MRO, Load IEB from SSR's, MRO",,,,,, 2009-317T21:16:00,000T01:44:00,13-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-317T21:16:00,000T01:44:00,13-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #2,ISS Lightning ridealong,,,,,, 2009-317T23:00:00,000T01:08:00,13-Nov-09,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Titan across Hyperion","Images of mutual event, transit of Titan across Hyperion for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-318T00:08:00,000T08:00:00,14-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 6. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-318T07:43:00,001T06:17:00,14-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-318T08:08:00,000T01:00:00,14-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-318T09:08:00,000T02:00:00,14-Nov-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-318T11:08:00,000T05:03:00,14-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-318T11:08:00,000T05:03:00,14-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #3,ISS Lightning ridealong,,,,,, 2009-318T16:51:00,000T09:00:00,14-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-318T17:51:00,000T08:00:00,14-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09318_SP,rider,,,,,, 2009-319T00:00:00,003T01:37:00,15-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-319T01:51:00,001T09:01:00,15-Nov-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-319T01:51:00,005T00:16:00,15-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-319T02:31:00,000T01:15:00,15-Nov-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 87.4 range 2.1 Mkm",,,,,, 2009-319T02:31:00,000T01:15:00,15-Nov-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-319T02:31:00,000T01:15:00,15-Nov-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-319T03:46:00,000T08:00:00,15-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 7. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-319T11:46:00,000T01:05:00,15-Nov-09,ISS,Prime,Enceladus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Enceladus across Rhea","Images of mutual event, transit of Enceladus across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-319T12:51:00,000T02:00:00,15-Nov-09,CAPS,Prime,Sun,SWAURPTG,MAPS aurora campaign,Prime pointing for solar wind-aurora campaign,Prime pointing for solar wind-aurora campaign,,,,,, 2009-319T14:00:00,000T00:34:00,15-Nov-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2009-319T14:34:00,000T10:42:00,15-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-319T14:51:00,000T01:05:00,15-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-319T16:02:19,000T09:10:00,15-Nov-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,CAPS calibration,CAPS calibration,,,,,, 2009-319T16:36:00,000T09:00:00,15-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-319T17:36:00,000T04:00:00,15-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09319_SP,rider,,,,,, 2009-320T01:16:00,002T00:21:00,16-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-320T02:16:00,000T08:00:00,16-Nov-09,UVIS,Prime,Saturn,MOS120APO,,,"As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.35x10^6 bits Mosaic scan of Saturn magnetosphere, day 8. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture.",,,,,, 2009-320T10:16:00,000T02:40:00,16-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-320T10:16:00,000T02:40:00,16-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #4,ISS Lightning ridealong,,,,,, 2009-320T10:52:00,003T15:10:00,16-Nov-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-320T12:56:00,000T01:00:00,16-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-320T13:56:00,000T02:00:00,16-Nov-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-320T16:36:00,000T09:00:00,16-Nov-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev121 Saturn occultation on 2009/324 and the Rev122 Saturn occultation on 2009/343.",,,,,, 2009-320T16:36:00,000T09:00:00,16-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-321T02:16:00,000T07:30:00,17-Nov-09,ISS,Prime,Star,CHARGEXF,Instrument calibration,ISS CCD Charge Transfer Calibration,"Two targets: M48 for NAC, Pleiades for WAC. For each rotate around the Y axis 180 degrees in 20 degree steps and image in three filters at each point. Initial secondary will be Pos Z or Neg Z to sun.",,,,,, 2009-321T09:46:00,000T01:00:00,17-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-321T10:46:00,000T01:11:00,17-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-321T10:46:00,000T01:11:00,17-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #5,ISS Lightning ridealong,,,,,, 2009-321T11:57:00,000T04:00:00,17-Nov-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-321T16:37:00,000T09:00:00,17-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-321T17:37:00,000T04:00:00,17-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09321_SP,rider,,,,,, 2009-322T01:37:00,001T00:00:00,18-Nov-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-322T01:37:00,000T08:25:00,18-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-322T01:37:00,000T15:00:00,18-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-322T02:17:00,000T10:40:00,18-Nov-09,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly - 1 day. SAT segment.Do 3 of 9 EG130 phase at priority 2.,,,,,, 2009-322T02:17:00,000T10:40:00,18-Nov-09,ISS,SPASS Rider,rings(general),EG130PHAS,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2009-322T06:30:00,000T01:08:16,18-Nov-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-322T09:30:00,000T01:08:16,18-Nov-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-322T10:02:00,000T01:28:00,18-Nov-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-322T10:02:00,000T15:35:00,18-Nov-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-322T11:30:00,000T05:00:00,18-Nov-09,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2009-322T12:57:00,000T01:00:00,18-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-322T13:57:00,000T02:00:00,18-Nov-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-322T16:30:00,001T09:32:00,18-Nov-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-322T16:37:00,000T09:00:00,18-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-322T17:37:00,000T08:00:00,18-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09322_SP,rider,,,,,, 2009-323T01:37:00,000T09:23:00,19-Nov-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-323T01:37:00,001T00:25:00,19-Nov-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-323T02:17:00,000T01:37:00,19-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-323T03:54:00,000T01:03:00,19-Nov-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Titan","Images of mutual event, transit of Rhea across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-323T04:57:00,000T04:40:00,19-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-323T09:37:00,000T02:00:00,19-Nov-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-323T11:00:00,000T02:00:00,19-Nov-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-323T11:37:00,000T11:45:00,19-Nov-09,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaics 001,"Repeats of 3x3 Global mosaic. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2009-323T11:37:00,000T11:45:00,19-Nov-09,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.",,,,,, 2009-323T13:00:00,000T22:37:00,19-Nov-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-323T23:22:00,000T02:50:00,19-Nov-09,CIRS,Prime,Saturn,NADIROCC,Occultation,NADIROCC egress or ingress,"Helium abundance measurement at the RSS egress or ingress occultation point. If RSS request deleted, this can be, too.",,,,,, 2009-323T23:25:58,000T02:46:02,19-Nov-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.994105 Rs exit= 9.0045471 Range altitude= 3091.8218 km ... -193.21948,,,,,, 2009-324T02:02:00,000T09:35:00,20-Nov-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-324T02:02:00,000T09:35:00,20-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-324T02:02:00,000T09:35:00,20-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-324T02:02:00,000T09:35:00,20-Nov-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-324T02:07:00,000T09:30:00,20-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-324T02:12:00,000T14:01:58,20-Nov-09,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 15.994105 Rs exit= 9.0045471 Range altitude= 3091.8218 km ... -193.21948,,,,,, 2009-324T02:37:00,000T09:00:00,20-Nov-09,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' mass,Downlink pass at Ka-band for Enceladus' mass determination and for improving locally Cassini orbit.,,,,,, 2009-324T02:37:00,000T09:00:00,20-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-324T03:37:00,000T08:00:00,20-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09324_SP,rider,,,,,, 2009-324T11:37:00,000T13:33:00,20-Nov-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-324T11:37:00,000T14:02:50,20-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-324T11:37:00,000T03:23:00,20-Nov-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-324T11:37:00,000T12:32:53,20-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-324T11:37:00,000T02:35:00,20-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-324T12:22:00,000T01:24:00,20-Nov-09,UVIS,Prime,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-324T12:22:00,000T01:24:00,20-Nov-09,CIRS,SPASS Rider,Dione,RIDER,Instrument rider,CIRS_121DI_RIDER_UVIS;,FP1 and FP3 only,,,,,, 2009-324T12:22:00,000T01:24:00,20-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-324T14:12:00,000T02:00:00,20-Nov-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-324T14:15:00,000T05:09:00,20-Nov-09,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2009-324T14:15:00,000T05:09:00,20-Nov-09,CIRS,SPASS Rider,Enceladus,RIDER,Instrument rider,CIRS_121EN_RIDER_ISS;,FP1 and FP3 only,,,,,, 2009-324T14:15:00,000T05:09:00,20-Nov-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-324T14:15:00,000T05:09:00,20-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-324T14:16:58,000T02:00:00,20-Nov-09,CDA,SPASS Rider,DustRAM direction,RPX0160,,CDA RPXing 2009-324T15:16:58,RPXing at 9.4689100 Rs,,,,,, 2009-324T15:00:00,000T02:00:00,20-Nov-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2009-324T16:12:00,000T09:12:50,20-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-324T16:13:58,001T02:02:00,20-Nov-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9883790 Rs exit= 8.9841730 Range altitude= -200.04151 km ... 3593.9725,,,,,, 2009-324T17:00:00,000T07:09:53,20-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-324T17:19:00,000T02:05:00,20-Nov-09,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS Thermal Stabilization 120 pre-Occ,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-324T19:24:00,000T02:36:00,20-Nov-09,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Atmospheric Occultation 121out,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2009-324T22:05:50,000T02:04:00,20-Nov-09,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-324T22:05:50,000T02:04:00,20-Nov-09,CIRS,SPASS Rider,Enceladus,RIDER,Instrument rider,CIRS_121EN_RIDER_VIMS;,,,,,,, 2009-324T22:05:50,000T02:04:00,20-Nov-09,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,"Enceladus rider with VIMS, pre-close approach",,,,,, 2009-324T22:05:50,000T02:04:00,20-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-325T00:09:50,000T01:23:00,21-Nov-09,CIRS,Prime,Enceladus,FP1DRKMAP,CIRS FP1 dark side map,CIRS_121EN_FP1DRKMAP001_PRIME;,"Enceladus is in Saturn transit except near the end- egress begins at ~01:26 1) 00:10 - 00:15 Shutter closed, FP1 to Enceladus center. 2) 00:15 - 00:30 N/S pole-to-pole FP1 scan, starting about 6 mrad north of Enceladus and continuing to 6 mrad south, as slowly as necessary to fill the time. 3) 00:30 - 01:00 E/W equatorial FP1 scan, starting about 6 mrad beyond the dark side of Enceladus and continuing to 6 mrad beyond the day side, as slowly as necessary to fill the time. 4) 01:00 - 01:32:50 FP1 raster scan of the entire disk of Enceladus, starting in the north and working south. The design should include about a minute total of FP1 dark sky pointing at the end, once egress is underway.",,,,,, 2009-325T00:09:50,000T01:23:00,21-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-325T00:09:50,000T01:23:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T00:09:53,000T01:30:00,21-Nov-09,INMS,Non-SPASS,Enceladus,ENCEL8,,Enceladus encounter,Enceladus observation,,,,,, 2009-325T00:09:53,000T09:00:07,21-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites. Data rate 0 bps, overlaps ENTAR & INTFLD requests.",,,,,, 2009-325T00:09:53,000T01:10:07,21-Nov-09,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2009-325T01:10:00,000T02:00:00,21-Nov-09,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 121EN Campaign,Part of 121EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2009-325T01:20:00,000T07:50:00,21-Nov-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-325T01:24:50,000T01:30:00,21-Nov-09,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2009-325T01:32:50,000T00:30:00,21-Nov-09,ISS,Prime,Enceladus,PLMHR,,High res plume obs during flyby.,Highest resolution plume observations during flyby.,,,,,, 2009-325T01:32:50,000T00:30:00,21-Nov-09,CIRS,SPASS Rider,Enceladus,RIDER,Instrument rider,CIRS_121EN_RIDER_ISS;,,,,,,, 2009-325T01:32:50,000T00:30:00,21-Nov-09,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,,,,,,, 2009-325T01:32:50,000T00:30:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T01:39:50,000T01:00:00,21-Nov-09,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-325T01:39:53,000T01:00:00,21-Nov-09,INMS,Non-SPASS,Enceladus,ENCEL8,,Enceladus encounter,Enceladus observation,,,,,, 2009-325T02:00:00,000T00:20:00,21-Nov-09,CDA,Non-SPASS,DustRAM direction,ENC8,,CDA Enceladus 325T02:10,"Enceladus flyby E8, ORS prime",,,,,, 2009-325T02:02:50,000T00:01:00,21-Nov-09,CIRS,SPASS Rider,Enceladus,RWA2RCS,,CIRS_121EN_RCS2RWA001_AACS;,Rider: FP3 stare during transition to RWA,,,,,, 2009-325T02:03:50,000T02:36:00,21-Nov-09,CIRS,Prime,Enceladus,FP3HIRES,,CIRS_121EN_FP3HIRES001_PRIME;,"High resolution FP3 scan of Damascus or Baghdad Sulcus, followed by ISS- and VIMS-driven mapping of the sunlit surface on departure. After VIMS portion: 03:40 - 03:55: FP1 fast global raster scan 03:55 - 04:10: ISS 2x2 global mosaic??? 04:10 - 04:39: Global (three-swath?) FP3 map at about 16 murad/sec.",,,,,, 2009-325T02:03:50,000T02:36:00,21-Nov-09,ISS,SPASS Rider,Enceladus,FP3HIRES,,Enceladus,"Enceladus rider with CIRS, close approach",,,,,, 2009-325T02:03:50,000T02:36:00,21-Nov-09,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,,,,,,, 2009-325T02:03:50,000T02:36:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T02:39:50,000T15:05:10,21-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-325T02:39:53,000T01:30:00,21-Nov-09,INMS,Non-SPASS,Enceladus,ENCEL8,,Enceladus encounter,Enceladus observation,,,,,, 2009-325T02:54:50,000T05:15:09,21-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-325T03:10:00,000T22:12:00,21-Nov-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-325T04:09:53,000T03:57:23,21-Nov-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-325T04:39:50,000T00:22:00,21-Nov-09,CIRS,SPASS Rider,Enceladus,RCS2RWA,,CIRS_121EN_RCS2RWA001_AACS;,Rider: FP3 stare during transition to RWA,,,,,, 2009-325T04:39:50,000T00:21:05,21-Nov-09,ISS,SPASS Rider,SpacecraftActivity,DFPWBIAS,,Enceladus,"Enceladus rider with ENGR, post-close approach; during RCS/RWA transition",,,,,, 2009-325T04:39:50,000T00:22:00,21-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-325T04:39:50,000T00:22:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T05:01:50,000T01:38:00,21-Nov-09,CIRS,Prime,Enceladus,FP3DAYMAP,CIRS FP3 daytime map,CIRS_121EN_FP3DAYMAP002_PRIME;,05:02 - 06:00 Global (2 swath?) FP3 scan of Enceladus at 6 murad/sec 06:00 - 06:40 FP1 stare at the center of Enceladus at high spectral resolution.,,,,,, 2009-325T05:01:50,000T01:38:00,21-Nov-09,ISS,SPASS Rider,Enceladus,FP3DAYMAP,CIRS FP3 daytime map,Enceladus,"Enceladus rider with CIRS, post-close approach",,,,,, 2009-325T05:01:50,000T01:38:00,21-Nov-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-325T05:01:50,000T01:38:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T05:15:03,000T00:00:01,21-Nov-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.202 Rs, lat = -0 deg, phase = 70 deg",,,,,, 2009-325T06:20:00,000T09:25:00,21-Nov-09,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' mass,Downlink pass at Ka-band for Enceladus' mass determination and for improving locally Cassini orbit.,,,,,, 2009-325T06:39:50,000T01:00:00,21-Nov-09,UVIS,Prime,Enceladus,ICYSTARE,,ICYSTARE: Investigate volatiles near Enceladus,Long stare for tenuous atmosphere search. Will provide data to associate plume activity with quantity of volatiles near Enceladus. This data will be a tiepoint between plume activity characterized in detail when the spacecraft is close to Enceladus with remote observations of Enceladus and the system.,,,,,, 2009-325T06:39:50,000T01:00:00,21-Nov-09,CIRS,SPASS Rider,Enceladus,RIDER,Instrument rider,CIRS_121EN_RIDER_UVIS;,,,,,,, 2009-325T06:39:50,000T01:00:00,21-Nov-09,ISS,SPASS Rider,Enceladus,ICYSTARE,,Enceladus,"Enceladus rider with UVIS, post-close approach",,,,,, 2009-325T06:39:50,000T01:00:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T08:07:16,000T08:02:37,21-Nov-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-325T08:08:58,000T02:00:00,21-Nov-09,CDA,SPASS Rider,DustRAM direction,RPX0170,,CDA RPXing 2009-325T09:08:58,RPXing at 4.3184560 Rs,,,,,, 2009-325T08:10:00,000T02:00:00,21-Nov-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-325T09:10:00,000T06:25:41,21-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-325T09:45:00,000T05:15:00,21-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-325T10:10:00,000T15:12:00,21-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-325T15:35:41,000T04:00:00,21-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites. Data rate 0 bps, overlaps RHTAR request.",,,,,, 2009-325T15:35:41,000T04:00:00,21-Nov-09,MAG,Non-SPASS,Rhea,RHTAR,Rhea targeted flyby,R3 flyby,"The sole Rhea flyby was a downstream flyby. In order to fully understand if the moon is mass-loading or mass-absorbing type both upstream and downstream flybys are required. The new flybys R2,R3,R4 and R5 will fulfill this requirement.",,,,,, 2009-325T16:09:53,000T09:12:07,21-Nov-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-325T16:30:00,000T00:56:00,21-Nov-09,UVIS,Prime,Rhea,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to beta Ori. Goal is to observe Rhea's ring on ingress when track is close to equatorial. Four minutes after egress slew to kappa Ori. Ingress and egress are not equatorial so this will be used to look for volatiles.,,,,,, 2009-325T16:30:00,000T00:56:00,21-Nov-09,CIRS,SPASS Rider,Rhea,RIDER,Instrument rider,CIRS_121RH_RIDER_UVIS;,FP1 and FP3 only,,,,,, 2009-325T16:30:00,000T00:56:00,21-Nov-09,ISS,SPASS Rider,Rhea,ICYEXO,Icy satellite exosphere,Rhea mapping and stereo,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-325T16:30:00,000T00:56:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T17:26:00,000T00:10:00,21-Nov-09,CIRS,Prime,Rhea,FP1EQSCAN,,CIRS_121RH_FP1EQSCAN001_PRIME;,"Limb-to-limb fast scan along equator, including night and early morning. FP1 and FP3 only. Include about 7 mrad of deep space off the edge of the disk on both sides. If we cannot cover the entire width of Rhea, the night side is higher priority.",,,,,, 2009-325T17:26:00,000T00:10:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T17:36:00,000T00:30:00,21-Nov-09,ISS,Prime,Rhea,REGMAP,Regional mapping,Rhea regional mapping,Do mosaic and stereo coverage of wispy streaks region,,,,,, 2009-325T17:36:00,000T00:30:00,21-Nov-09,CIRS,SPASS Rider,Rhea,RIDER,Instrument rider,CIRS_121RH_RIDER_ISS;,FP1 and FP3 only,,,,,, 2009-325T17:36:00,000T00:30:00,21-Nov-09,UVIS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2009-325T17:36:00,000T00:30:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T17:45:00,000T07:37:00,21-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-325T18:06:00,000T00:40:00,21-Nov-09,VIMS,Prime,Rhea,RHEA,Rhea,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T18:06:00,000T00:40:00,21-Nov-09,CIRS,SPASS Rider,Rhea,RIDER,Instrument rider,CIRS_121RH_RIDER_UVIS;,FP1 and FP3 only,,,,,, 2009-325T18:06:00,000T00:40:00,21-Nov-09,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea equatorial color mapping,VIMS sit'n'stare,,,,,, 2009-325T18:06:00,000T00:40:00,21-Nov-09,UVIS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2009-325T18:15:58,000T07:06:02,21-Nov-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0003448 Rs exit= 15.991357 Range altitude= 3605.0985 km ... 8067.4799,,,,,, 2009-325T18:46:00,000T00:40:00,21-Nov-09,ISS,Prime,Rhea,EQUATCOL,,Rhea equatorial color mapping,Do 1x5 mosaic of equator,,,,,, 2009-325T18:46:00,000T00:40:00,21-Nov-09,CIRS,SPASS Rider,Rhea,RIDER,Instrument rider,CIRS_121RH_RIDER_ISS;,FP1 and FP3 only,,,,,, 2009-325T18:46:00,000T00:40:00,21-Nov-09,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-325T18:46:00,000T00:40:00,21-Nov-09,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,multiple 160/640 ms.,,,,,, 2009-325T19:35:41,000T05:46:19,21-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-326T01:22:00,000T07:00:00,22-Nov-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-326T01:22:00,000T07:00:00,22-Nov-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-326T01:22:00,000T01:30:00,22-Nov-09,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 9.0003448 Rs exit= 15.991357 Range altitude= 3605.0985 km ... 8067.4799,,,,,, 2009-326T01:22:00,000T07:45:16,22-Nov-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-326T01:22:00,000T07:00:00,22-Nov-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-326T01:22:00,000T07:00:00,22-Nov-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-326T01:22:00,000T07:00:00,22-Nov-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-326T02:52:00,000T09:35:00,22-Nov-09,VIMS,Prime,Saturn,NHEMDYN,,Northern Hemisphere dynamics mosaic 001,"3x3 Global mosaics of northern hemisphere, repeated. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2009-326T02:52:00,000T09:35:00,22-Nov-09,ISS,SPASS Rider,Saturn,NHEMDYN,,WAC N hemisp. day movie + NAC lightning search,"6 pickets spaced 1h 30m. 2x1 (day side of half-lit planet) WAC in MT3, CB2, MT2, and BL1.(8 frames per picket 3.5Mb each) +88 images x 4Mb: During VIMS mosaics - NAC CL1 day or night images at each footprint, one image per 10 minutes",,,,,, 2009-326T02:52:00,000T08:11:58,22-Nov-09,CDA,Non-SPASS,Other,RATE080B,,Data rate,Range enter= 9.0003448 Rs exit= 15.991357 Range altitude= 3605.0985 km ... 8067.4799,,,,,, 2009-326T08:22:00,001T09:10:00,22-Nov-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-326T08:22:00,001T09:10:00,22-Nov-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-326T08:22:00,001T09:10:00,22-Nov-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-326T08:22:00,008T09:14:00,22-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-326T08:22:00,001T09:10:00,22-Nov-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-326T09:07:16,000T16:14:44,22-Nov-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-326T11:03:58,008T06:32:02,22-Nov-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.003374 Rs exit= 16.004873 Range altitude= 8074.7003 km ... 2874.0966,,,,,, 2009-326T12:27:00,000T02:00:00,22-Nov-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-326T14:27:00,000T01:15:00,22-Nov-09,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 125 range 1.2 Mkm",,,,,, 2009-326T14:27:00,000T01:15:00,22-Nov-09,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-326T14:27:00,000T01:15:00,22-Nov-09,UVIS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-326T16:22:00,000T09:00:00,22-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-326T17:22:00,000T04:00:00,22-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09326_SP,rider,,,,,, 2009-327T01:22:00,000T23:45:00,23-Nov-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-327T02:52:00,000T01:00:00,23-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-327T03:52:00,000T00:53:00,23-Nov-09,ISS,Prime,Pandora,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Pandora across Epimetheus","Images of mutual event, transit of Pandora across Epimetheus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-327T04:45:00,000T04:00:00,23-Nov-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-327T04:45:00,000T04:00:00,23-Nov-09,ISS,SPASS Rider,Enceladus,ICYATM,Icy satellite system volatile map,Enceladus,Enceladus rider with UVIS,,,,,, 2009-327T08:45:00,000T04:15:00,23-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-327T08:45:00,000T04:15:00,23-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #8,ISS Lightning ridealong,,,,,, 2009-327T13:00:00,000T02:00:00,23-Nov-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-327T15:00:00,000T00:27:00,23-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-327T16:07:00,000T09:00:00,23-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-327T17:32:00,002T05:55:00,23-Nov-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-327T17:32:00,004T22:21:00,23-Nov-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-327T17:32:00,004T06:28:00,23-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-328T01:07:00,005T12:53:00,24-Nov-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-328T01:47:00,000T05:54:00,24-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-328T07:41:00,000T01:00:00,24-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-328T08:41:00,000T01:07:00,24-Nov-09,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Rhea","Images of mutual event, transit of Epimetheus across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-328T09:48:00,000T00:43:00,24-Nov-09,ISS,Prime,Janus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Janus across Rhea","Images of mutual event, transit of Janus across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-328T10:31:00,000T02:00:00,24-Nov-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-328T12:31:00,000T12:07:00,24-Nov-09,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2009-328T12:31:00,000T12:07:00,24-Nov-09,ISS,SPASS Rider,rings(general),EG80PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2009-329T00:38:00,000T00:30:00,25-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-329T02:08:00,000T09:00:00,25-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-329T03:08:00,000T04:00:00,25-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09329_SP,rider,,,,,, 2009-329T11:48:00,000T01:00:00,25-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-329T12:48:00,000T04:00:00,25-Nov-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-329T16:48:00,000T08:40:00,25-Nov-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_121SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-329T16:48:00,000T08:40:00,25-Nov-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #1,CIRS Compsit ridealong,,,,,, 2009-329T23:27:00,003T01:26:00,25-Nov-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-330T01:28:00,000T10:20:00,26-Nov-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-330T02:08:00,000T09:00:00,26-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-330T03:08:00,000T08:00:00,26-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09330_SP,rider,,,,,, 2009-330T11:48:00,000T01:48:00,26-Nov-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-330T11:48:00,000T01:48:00,26-Nov-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-330T13:36:00,000T01:00:00,26-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-330T14:36:00,000T00:30:00,26-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-330T15:06:00,000T00:42:00,26-Nov-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Tethys","Images of mutual event, transit of Rhea across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-330T15:48:00,000T01:35:00,26-Nov-09,ISS,Prime,Rhea,PHOTOOP,,"Photo Op, transit of Rhea across Janus","Photo op Rhea, planet, rings, and shadows.",,,,,, 2009-330T15:48:00,000T01:35:00,26-Nov-09,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-330T17:23:00,000T02:16:00,26-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-330T17:23:00,000T02:16:00,26-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #10,ISS Lightning ridealong,,,,,, 2009-330T19:39:00,000T00:59:00,26-Nov-09,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Titan across Tethys","Images of mutual event, transit of Titan across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-330T20:38:00,000T08:00:00,26-Nov-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_121SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-330T20:38:00,000T08:00:00,26-Nov-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #2,CIRS Compsit ridealong,,,,,, 2009-331T04:38:00,000T00:30:00,27-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-331T05:08:00,000T01:00:00,27-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-331T06:08:00,000T01:24:00,27-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-331T06:08:00,000T01:24:00,27-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #11,ISS Lightning ridealong,,,,,, 2009-331T07:32:00,000T01:06:00,27-Nov-09,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Titan across Mimas","Images of mutual event, transit of Titan across Mimas for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-331T09:38:00,000T09:00:00,27-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-331T10:38:00,000T04:00:00,27-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09331_SP,rider,,,,,, 2009-331T19:18:00,000T01:15:00,27-Nov-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 88.9 range 1.2 Mkm",,,,,, 2009-331T19:18:00,000T01:15:00,27-Nov-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-331T19:18:00,000T01:15:00,27-Nov-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-331T20:33:00,000T08:00:00,27-Nov-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_121SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-331T20:33:00,000T08:00:00,27-Nov-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #3,CIRS Compsit ridealong,,,,,, 2009-332T00:00:00,001T00:53:00,28-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-332T04:33:00,000T01:00:00,28-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-332T05:33:00,000T00:30:00,28-Nov-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-332T06:03:00,000T07:37:00,28-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-332T06:03:00,000T07:37:00,28-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #12,ISS Lightning ridealong,,,,,, 2009-332T13:40:00,000T00:43:00,28-Nov-09,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Tethys","Images of mutual event, transit of Dione across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-332T14:23:00,000T00:50:00,28-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-332T14:23:00,000T00:50:00,28-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #13,ISS Lightning ridealong,,,,,, 2009-332T15:52:00,000T09:00:00,28-Nov-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev122 Saturn occultation on 2009/343.",,,,,, 2009-332T15:53:00,002T01:44:00,28-Nov-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-332T15:53:00,002T01:43:00,28-Nov-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-332T15:53:00,000T09:00:00,28-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-332T16:53:00,000T08:00:00,28-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09332_SP,rider,,,,,, 2009-333T00:53:00,001T10:00:00,29-Nov-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-333T00:53:00,001T10:00:00,29-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-333T00:53:00,001T01:00:00,29-Nov-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-333T01:33:00,000T01:15:00,29-Nov-09,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 78.8 range 1.6 Mkm",,,,,, 2009-333T01:33:00,000T01:15:00,29-Nov-09,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-333T01:33:00,000T01:15:00,29-Nov-09,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-333T02:48:00,000T03:00:00,29-Nov-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-333T02:48:00,000T03:00:00,29-Nov-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-333T05:48:00,000T01:00:00,29-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-333T06:48:00,000T18:25:00,29-Nov-09,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2009-333T06:48:00,000T18:25:00,29-Nov-09,VIMS,SPASS Rider,RingE,LRLEMP,,Edge-on observation of E ring around equinox,"Low-res, low elevation, medium phase observation of E ring.",,,,,, 2009-333T14:00:00,000T04:00:00,29-Nov-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-333T18:00:00,000T23:37:00,29-Nov-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-334T01:53:00,000T09:00:00,30-Nov-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-334T02:53:00,000T08:00:00,30-Nov-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_121IC_DSCAL09334_SP,rider,,,,,, 2009-334T10:53:00,005T00:49:00,30-Nov-09,CAPS,SPASS Rider,Sun,SWAURORA,Solar wind campaign,MAPS solar wind-aurora Campaign,MAPS solar wind-aurora Campaign,,,,,, 2009-334T10:53:00,003T13:07:00,30-Nov-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-334T11:33:00,000T01:15:00,30-Nov-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 79.3 range 2.2 Mkm",,,,,, 2009-334T11:33:00,000T01:15:00,30-Nov-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-334T11:33:00,000T01:15:00,30-Nov-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-334T12:48:00,000T01:30:00,30-Nov-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-334T12:48:00,000T01:30:00,30-Nov-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-334T14:18:00,000T01:00:00,30-Nov-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-334T15:18:00,000T05:42:00,30-Nov-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-334T15:18:00,000T05:42:00,30-Nov-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #14,ISS Lightning ridealong,,,,,, 2009-334T17:36:00,008T06:39:58,30-Nov-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.003374 Rs exit= 16.004873 Range altitude= 8074.7003 km ... 2874.0966,,,,,, 2009-334T17:36:00,008T09:20:00,30-Nov-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-334T17:36:00,003T17:00:00,30-Nov-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-334T17:36:50,000T00:00:01,30-Nov-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 19.0 d, inc = 0.5 deg, r = 42.380 Rs, phase = 109 deg",,,,,, 2009-334T17:37:00,004T18:05:00,30-Nov-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-334T17:37:00,003T17:02:00,30-Nov-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-334T21:00:00,000T04:00:00,30-Nov-09,ISS,Prime,Titan,ECLIPSE0,,Titan NAC Photopol 90 Phase,Long exposures to search for auroras and lightning on Titan in eclipse. This is one of several possible events but distant from Titan,,,,,, 2009-334T21:00:00,000T04:00:00,30-Nov-09,UVIS,SPASS Rider,Titan,ECLIPSE,,Rider to ISS ECLIPSE,Rider to ISS TI_ECLIPSE - to look for emissions from electron/ion impact during eclipse when sunlight is absent,,,,,, 2009-335T00:00:00,000T00:34:00,1-Dec-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-335T01:00:00,000T07:43:00,1-Dec-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_122SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-335T01:00:00,000T07:43:00,1-Dec-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #1,CIRS Compsit ridealong,,,,,, 2009-335T09:23:00,000T09:00:00,1-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-335T10:23:00,000T08:00:00,1-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09335_SP,rider,,,,,, 2009-335T19:03:00,000T02:15:00,1-Dec-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-335T19:03:00,000T02:15:00,1-Dec-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-335T21:18:00,000T00:52:00,1-Dec-09,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Enceladus","Images of mutual event, transit of Rhea across Enceladus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-335T22:10:00,000T15:48:00,1-Dec-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_122SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-335T22:10:00,000T15:48:00,1-Dec-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #2,CIRS Compsit ridealong,,,,,, 2009-336T13:58:00,000T01:00:00,2-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-336T15:38:00,000T09:00:00,2-Dec-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev122 Saturn occultation on 2009/343.",,,,,, 2009-336T15:38:00,000T09:00:00,2-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-336T16:38:00,000T04:00:00,2-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09336_SP,rider,,,,,, 2009-337T01:18:00,000T22:41:00,3-Dec-09,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_122SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2009-337T01:18:00,000T22:41:00,3-Dec-09,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ridealong #1,CIRS MIRMAP ridealong,,,,,, 2009-337T23:59:00,000T01:00:00,3-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-338T00:00:00,001T01:39:00,4-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-338T01:39:00,000T09:00:00,4-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-338T02:39:00,000T08:00:00,4-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09338_SP,rider,,,,,, 2009-338T10:39:00,001T00:00:00,4-Dec-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-338T11:19:00,000T01:30:00,4-Dec-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-338T11:19:00,000T01:30:00,4-Dec-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-338T12:49:00,000T01:00:00,4-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-338T13:49:00,000T08:00:00,4-Dec-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_122SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Northern hemisphere",,,,,, 2009-338T13:49:00,000T08:00:00,4-Dec-09,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #3,CIRS Compsit ridealong,,,,,, 2009-338T21:49:00,000T03:10:00,4-Dec-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-338T21:49:00,000T03:10:00,4-Dec-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #3,ISS Lightning ridealong,,,,,, 2009-339T01:39:00,002T10:18:00,5-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-339T01:39:00,000T09:00:00,5-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-339T02:39:00,000T08:00:00,5-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09339_SP,rider,,,,,, 2009-339T10:39:00,002T21:21:00,5-Dec-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-339T11:19:00,000T01:30:00,5-Dec-09,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2009-339T11:19:00,000T01:30:00,5-Dec-09,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-339T11:42:00,002T00:15:00,5-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-339T11:42:00,003T15:10:00,5-Dec-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,MAPS magnetospheric survey,,,,,, 2009-339T12:49:00,000T02:00:00,5-Dec-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-339T14:49:00,000T01:00:00,5-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-339T15:49:00,000T15:40:00,5-Dec-09,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_122SA_MIRMAP002_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2009-339T15:49:00,000T15:40:00,5-Dec-09,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ridealong #2,CIRS MIRMAP ridealong,,,,,, 2009-340T07:29:00,000T01:00:00,6-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-340T09:09:00,000T09:00:00,6-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-340T10:09:00,000T04:00:00,6-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09340_SP,rider,,,,,, 2009-340T18:49:00,000T01:00:00,6-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-340T19:49:00,000T12:00:00,6-Dec-09,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment.Do 3 of 9 EG130 phase at priority 2.,,,,,, 2009-340T19:49:00,000T12:00:00,6-Dec-09,ISS,SPASS Rider,rings(general),EG130PHAS,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2009-341T07:49:00,000T04:55:00,7-Dec-09,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint. 2x1 WAC dayside. Cycled while observation lasts.,,,,,, 2009-341T07:49:00,000T04:55:00,7-Dec-09,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Lightning Ridealong #5,ISS Lightning ridealong,,,,,, 2009-341T11:57:00,000T12:03:00,7-Dec-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-341T11:57:00,001T14:55:00,7-Dec-09,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2009-341T12:44:00,000T02:00:00,7-Dec-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-341T15:24:00,000T09:00:00,7-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-341T16:24:00,000T04:00:00,7-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09341_SP,rider,,,,,, 2009-342T00:00:00,000T00:24:00,8-Dec-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-342T00:24:00,001T00:35:00,8-Dec-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-342T00:24:00,000T15:00:00,8-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-342T00:30:00,000T06:49:36,8-Dec-09,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2009-342T01:24:00,000T01:00:00,8-Dec-09,ISS,Prime,Saturn,1X2WPXX,,WAC Saturn Photopol 140 Phase,Saturn WAC Photopolarimetry 140 Phase 1X2 mosaic,,,,,, 2009-342T02:24:00,000T12:20:00,8-Dec-09,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 001,"3x3 Global mosaic, centered on equator to support RADAR observations. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2009-342T02:24:00,000T12:30:00,8-Dec-09,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.",,,,,, 2009-342T08:00:00,000T06:00:00,8-Dec-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-342T14:00:00,000T10:24:00,8-Dec-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-342T15:24:00,000T09:35:00,8-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-342T16:09:00,000T08:00:00,8-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09342_SP,rider,,,,,, 2009-343T00:15:58,000T16:46:00,9-Dec-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.992854 Rs exit= 9.0153830 Range altitude= 2868.1728 km ... -306.29270,,,,,, 2009-343T00:24:00,000T10:00:00,9-Dec-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-343T00:59:00,000T01:53:00,9-Dec-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-343T00:59:00,000T08:25:00,9-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-343T01:44:00,000T04:00:00,9-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09343_SP,rider,,,,,, 2009-343T02:52:00,000T19:38:00,9-Dec-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-343T02:52:00,000T06:32:00,9-Dec-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T02:52:00,000T06:32:00,9-Dec-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T02:52:00,000T06:50:00,9-Dec-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T02:56:00,000T06:46:00,9-Dec-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-343T09:24:00,002T00:46:00,9-Dec-09,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T09:24:00,000T16:44:00,9-Dec-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T09:42:00,000T04:43:00,9-Dec-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T09:42:00,001T23:29:00,9-Dec-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-343T10:04:00,000T03:00:00,9-Dec-09,CIRS,Prime,Saturn,NADIROCC,Occultation,NADIROCC egress or ingress,"Helium abundance measurement at the RSS egress occultation point. If RSS request deleted, this can be, too. IF RSS observes both ingress & egress, the NADIROCC that best fits the timeline can be chosen",,,,,, 2009-343T10:24:00,000T00:25:32,9-Dec-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-343T10:49:32,000T22:00:00,9-Dec-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-343T13:04:00,000T02:26:00,9-Dec-09,CDA,Prime,DustRAM direction,RPX0180,,CDA RPXing 2009-343T15:28:58,RPXing at 9.7637359 Rs,,,,,, 2009-343T14:25:00,000T02:00:00,9-Dec-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-343T15:30:00,000T01:54:00,9-Dec-09,ISS,Prime,Enceladus,PLMHRMP,,"High res, intermed. phase obs.",High resolution plume observations.,,,,,, 2009-343T15:39:45,000T02:05:00,9-Dec-09,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS Thermal Stabilization 122 pre-Occ,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-343T16:25:00,000T02:35:00,9-Dec-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-343T17:01:58,000T04:59:02,9-Dec-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.9992114 Rs exit= 8.9945570 Range altitude= -312.83972 km ... 3655.4250,,,,,, 2009-343T17:44:45,000T04:36:15,9-Dec-09,RSS,Prime,Saturn,OCC,Occultation,RSS Atmospheric Occultation 122all,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2009-343T19:00:00,000T13:50:00,9-Dec-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-343T22:01:00,000T10:29:00,9-Dec-09,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 8.9992114 Rs exit= 8.9945570 Range altitude= -312.83972 km ... 3655.4250,,,,,, 2009-343T22:30:00,000T14:43:00,9-Dec-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-343T22:41:00,000T14:32:00,9-Dec-09,RADAR,Prime,Saturn,GLOBALMAP,Global coverage mapping,Saturn second equatorial obs.,map equator; coordinated with VIMS.,,,,,, 2009-344T02:08:00,000T07:51:00,10-Dec-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites. Data rate 0 bps, overlaps INTFLD request.",,,,,, 2009-344T02:08:00,000T07:51:00,10-Dec-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-344T06:04:09,000T00:00:01,10-Dec-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.196 Rs, lat = -0 deg, phase = 71 deg",,,,,, 2009-344T08:30:00,000T02:30:00,10-Dec-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9992114 Rs exit= 8.9945570 Range altitude= -312.83972 km ... 3655.4250,,,,,, 2009-344T08:49:32,000T02:00:00,10-Dec-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-344T08:50:00,000T02:00:00,10-Dec-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-344T08:50:58,000T02:00:00,10-Dec-09,CDA,SPASS Rider,DustRAM direction,RPX0190,,CDA RPXing 2009-344T09:50:58,RPXing at 4.2603992 Rs,,,,,, 2009-344T09:59:00,000T23:08:00,10-Dec-09,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2009-344T10:49:32,000T23:00:00,10-Dec-09,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2009-344T10:50:00,000T06:10:00,10-Dec-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-344T11:00:00,000T02:13:00,10-Dec-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0107320 Rs exit= 15.990450 Range altitude= 3666.5191 km ... 8096.8598,,,,,, 2009-344T13:13:00,000T11:57:00,10-Dec-09,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 002,"3x3 Global mosaics, repeated, centerd on the equator to support RADAR observations. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2009-344T13:13:00,000T19:54:00,10-Dec-09,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,MAPS rings and satellites Campaign,MAPS rings and satellites Campaign,,,,,, 2009-344T13:13:00,000T11:57:00,10-Dec-09,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.",,,,,, 2009-344T13:13:00,000T22:38:58,10-Dec-09,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 9.0107320 Rs exit= 15.990450 Range altitude= 3666.5191 km ... 8096.8598,,,,,, 2009-344T17:00:00,000T16:07:00,10-Dec-09,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2009-345T01:10:00,000T09:00:00,11-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-345T02:10:00,000T08:00:00,11-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09345_SP,rider,,,,,, 2009-345T09:07:00,000T13:56:14,11-Dec-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-345T09:07:00,000T01:03:00,11-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-345T09:11:00,000T00:59:00,11-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-345T09:49:32,000T00:20:28,11-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-345T10:10:00,000T12:53:14,11-Dec-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-345T10:10:00,000T02:53:14,11-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-345T10:10:00,000T07:02:32,11-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-345T10:10:00,003T00:00:00,11-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-345T10:10:00,000T12:53:14,11-Dec-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-345T11:05:56,000T03:57:18,11-Dec-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-345T11:05:56,000T03:57:18,11-Dec-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-345T11:05:56,000T03:57:18,11-Dec-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-345T11:05:56,000T00:57:18,11-Dec-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan scan,Scan across Titan - 130 km/pixel - phase=135 deg,,,,,, 2009-345T11:51:58,001T13:18:02,11-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 16.002477 Rs exit= 38.002797 Range altitude= 8104.0255 km ... -77287.292,,,,,, 2009-345T12:03:14,000T03:00:00,11-Dec-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,Stare at Titan. Phase = 134 deg. Lat/Lon = 01N/11 deg. Resolution = 129 - 98 km/px. Temp. N. Obtain 64x64 cubes at various exp times for global mapping.,,,,,, 2009-345T13:03:14,000T11:00:00,11-Dec-09,INMS,Non-SPASS,Titan,T63INBND,,Titan Flyby,Titan observation,,,,,, 2009-345T15:03:14,000T01:00:00,11-Dec-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-345T15:03:14,000T01:00:00,11-Dec-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS,,,,,, 2009-345T15:03:14,000T01:00:00,11-Dec-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,Stare at Titan. Phase = 134 deg. Lat/Lon = 01N/14 deg. Resolution = 98 - 88 km/px. Temp. N. Obtain 48x48 cubes at various exp times for global mapping.,,,,,, 2009-345T16:03:14,000T04:00:00,11-Dec-09,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-345T16:03:14,000T04:00:00,11-Dec-09,CIRS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-345T16:03:14,000T04:00:00,11-Dec-09,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-345T16:03:14,000T04:00:00,11-Dec-09,RADAR,SPASS Rider,Titan,T63WARMUP,,Warmup for T63 Radiometry,,,,,,, 2009-345T16:03:14,000T04:00:00,11-Dec-09,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-345T16:03:14,000T04:00:00,11-Dec-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan limb mapping.,Titan limb mapping. Phase = 135 deg. Lat/Lon = 01N/16 deg. Resolution = 88 - 50 km/px. Temp. R. Obtain cubes at various exp times for limb mapping.,,,,,, 2009-345T17:12:32,000T03:50:42,11-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-345T20:03:14,000T02:55:00,11-Dec-09,RADAR,Prime,Titan,T63INRAD,,T63 Inbound Radiometry,,,,,,, 2009-345T21:03:14,000T08:00:00,11-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,"Investigate the previously unobserved dusk flank of Saturn's magnetosphere. Data rate 0 bps, overlaps MAGTITAN request.",,,,,, 2009-345T21:03:14,000T08:00:00,11-Dec-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T63 flyby,"T63 is a north polar, dusk, high altitude flyby. In nominal upstream conditions, Cassini would explore the north lobe of the mid-range magnetic tail. With adequate pointing of MAPS plasma instruments, MAG data will also yield valuable information about the pitch angle distribution of Titan's escaping plasma. This flyby will increase our understanding of the properties of Titan's mid range tail acquired during T9. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-345T22:58:14,000T04:50:00,11-Dec-09,CAPS,Prime,Titan,TITANPTG,Titan observation,Prime pointing 122TI (T63),Prime pointing 122TI (T63),,,,,, 2009-345T23:03:14,000T01:00:00,11-Dec-09,CAPS,SPASS Rider,Titan,T63INBND,,Inbound 122TI (T63),Inbound 122TI (T63),,,,,, 2009-345T23:03:14,000T01:00:00,11-Dec-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-345T23:03:14,000T01:00:00,11-Dec-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,Titan regional mapping. Phase = 140 deg. Lat/Lon = 06N/29 deg. Resolution = 19 - 9 km/px. Obtain cubes for regional mapping and mosaics during CAPS observations with Titan within FOV.,,,,,, 2009-345T23:03:14,000T01:00:00,11-Dec-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-346T00:03:14,000T02:00:00,12-Dec-09,CAPS,SPASS Rider,Titan,T63CLOSE,,Closest Approach 122TI (T63),Closest Approach 122TI (T63),,,,,, 2009-346T00:03:14,000T02:00:00,12-Dec-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-346T00:03:14,000T00:40:00,12-Dec-09,INMS,Non-SPASS,Titan,TITAN63,,Titan Flyby,Titan observation,,,,,, 2009-346T00:03:14,000T02:00:00,12-Dec-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-346T00:43:14,000T00:40:00,12-Dec-09,INMS,Non-SPASS,Titan,TITAN63,,Titan Flyby,Titan observation,,,,,, 2009-346T01:23:14,000T00:40:00,12-Dec-09,INMS,Non-SPASS,Titan,TITAN63,,Titan Flyby,Titan observation,,,,,, 2009-346T02:03:14,000T01:00:00,12-Dec-09,CAPS,SPASS Rider,Titan,T63OUTBND,,Outbound 122TI (T63),Outbound 122TI (T63),,,,,, 2009-346T02:03:14,000T01:00:00,12-Dec-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-346T02:03:14,000T11:00:00,12-Dec-09,INMS,Non-SPASS,Titan,T63OUTBND,,Titan Flyby,Titan observation,,,,,, 2009-346T02:03:14,000T01:00:00,12-Dec-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-346T03:03:14,000T14:51:46,12-Dec-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-346T03:03:14,000T00:45:00,12-Dec-09,CIRS,SPASS Rider,Titan,RIDER,Instrument rider,,Ride along with SP turn,,,,,, 2009-346T03:03:14,000T16:08:46,12-Dec-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-346T03:03:14,000T16:08:46,12-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-346T03:48:14,000T01:00:00,12-Dec-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-346T03:48:14,000T01:00:00,12-Dec-09,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-346T03:48:14,000T01:00:00,12-Dec-09,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,Titan regional mapping. Phase = 51 deg. Lat/Lon = 02N/201 deg. Resolution = 24 - 34 km/px. Temp. S2. Obtain 64x64 cubes for regional mapping and mosaics.,,,,,, 2009-346T04:48:14,000T05:15:00,12-Dec-09,ISS,Prime,Titan,GLOBMAPC,Global coverage mapping,NGM (NAC Global Map),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-346T04:48:14,000T05:15:00,12-Dec-09,CIRS,SPASS Rider,Titan,GLOBMAPC,Global coverage mapping,,Ride along with ISS,,,,,, 2009-346T04:48:14,000T05:15:00,12-Dec-09,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Stare at Titan,Stare at Titan. Phase = 49 deg. Lat/Lon = 01N/204 deg. Resolution = 34 - 48 km/px. Temp. S2. Obtain 64x64 cubes for global mapping mosaic.,,,,,, 2009-346T05:03:14,000T07:06:14,12-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-346T10:03:14,000T05:00:00,12-Dec-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,Titan global mapping. Phase = 46 deg. Lat/Lon = 01S/212 deg. Resolution = 88 - 138 km/px. Temp. V. Obtain 64x64 cubes at various exp times for global mapping.,,,,,, 2009-346T10:03:14,000T05:00:00,12-Dec-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS,,,,,, 2009-346T10:03:14,000T05:00:00,12-Dec-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-346T12:09:28,000T07:02:32,12-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-346T13:03:14,001T21:06:46,12-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-346T15:03:14,000T05:00:00,12-Dec-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-346T15:03:14,000T09:00:00,12-Dec-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-346T15:03:14,000T05:00:00,12-Dec-09,UVIS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,UVIS Rider to CIRS MIRTMAP,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-346T15:03:14,000T09:00:00,12-Dec-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan scan,Scan across Titan. Phase = 45 deg. Lat/Lon = 01S/217 deg. Resolution = 138 - 230 km/px. Temp. A(Z).,,,,,, 2009-346T17:55:00,000T01:17:00,12-Dec-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS dusk magnetosphere Campaign,MAPS dusk magnetosphere Campaign,,,,,, 2009-346T19:12:00,000T14:58:00,12-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-346T19:12:00,001T14:58:00,12-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-346T19:12:00,001T14:58:00,12-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-346T19:12:00,000T05:58:00,12-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-346T20:03:14,000T04:00:00,12-Dec-09,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2009-346T20:03:14,000T04:00:00,12-Dec-09,UVIS,SPASS Rider,Titan,COMPMAP,Composition map,UVIS Rider to CIRS COMPMAP,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-347T01:10:00,005T04:43:58,13-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 16.002477 Rs exit= 38.002797 Range altitude= 8104.0255 km ... -77287.292,,,,,, 2009-347T01:10:00,001T09:00:00,13-Dec-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-347T01:10:00,000T09:00:00,13-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-347T02:10:00,000T08:00:00,13-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09347_SP,rider,,,,,, 2009-347T10:10:00,001T00:00:00,13-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-347T10:50:00,000T01:10:00,13-Dec-09,ISS,Prime,Titan,CLOUD,,TMC (Titan Monitoring Campaign),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-347T10:50:00,000T01:10:00,13-Dec-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan stare,Caboose segment for cloud mapping. Phase=47 deg,,,,,, 2009-347T12:00:00,000T02:00:00,13-Dec-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-347T14:00:00,000T10:30:00,13-Dec-09,ISS,Prime,Titan,CLOUD,,TMC (Titan Monitoring Campaign),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-347T14:00:00,000T10:30:00,13-Dec-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan stare,Caboose segment for cloud mapping. Phase=47 deg,,,,,, 2009-348T00:30:00,000T10:20:00,14-Dec-09,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2009-348T01:10:00,000T09:00:00,14-Dec-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev123 Saturn occultation on 2009/359.",,,,,, 2009-348T01:10:00,000T09:00:00,14-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-348T02:10:00,000T08:00:00,14-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09348_SP,rider,,,,,, 2009-348T10:10:00,003T19:37:00,14-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS magnetospheric boundaries Campaign,MAPS magnetospheric boundaries Campaign,,,,,, 2009-348T10:10:00,003T19:44:00,14-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-348T10:10:00,000T23:45:00,14-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-348T10:10:00,003T19:45:00,14-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-348T10:10:00,003T19:44:00,14-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-348T10:10:00,003T19:44:00,14-Dec-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-348T10:50:00,000T01:15:00,14-Dec-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 51.8 range 1.2 Mkm",,,,,, 2009-348T10:50:00,000T01:15:00,14-Dec-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-348T10:50:00,000T01:15:00,14-Dec-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-348T12:05:00,000T02:00:00,14-Dec-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-348T14:05:00,000T10:10:00,14-Dec-09,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. MAG segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2009-348T14:05:00,000T10:10:00,14-Dec-09,CIRS,SPASS Rider,rings(general),EG80PHASE,,CIRS_RIRI_EG80PHASE001_VIMS,rider,,,,,, 2009-349T00:55:00,000T09:00:00,15-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-349T01:55:00,000T08:00:00,15-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09349_SP,rider,,,,,, 2009-349T09:55:00,001T00:00:00,15-Dec-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-349T10:35:00,000T00:53:00,15-Dec-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-349T10:35:00,000T00:53:00,15-Dec-09,CIRS,SPASS Rider,rings(general),SATELLORB,Satellite orbit campaign,CIRS_OTRI_SATELLORB013_ISS,rider,,,,,, 2009-349T11:28:00,000T00:43:00,15-Dec-09,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Janus","Images of mutual event, transit of Epimetheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2009-349T12:11:00,000T12:04:00,15-Dec-09,UVIS,Prime,Saturn,MOS122APO,,,"Mosaic scan of Saturn magnetosphere. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 129.0 s, stop data capture. Repeat PATTERN 189 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 129.0 s, stop data capture.",,,,,, 2009-350T00:00:00,000T00:34:00,16-Dec-09,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS calibration,ELS calibration,,,,,, 2009-350T00:55:00,000T09:00:00,16-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-350T01:55:00,000T08:00:00,16-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09350_SP,rider,,,,,, 2009-350T09:55:00,001T10:05:00,16-Dec-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-350T10:35:00,000T05:40:00,16-Dec-09,ISS,Prime,Iapetus,HILLSPHE,,Iapetus hill sphere observation,Turn -Y to Iapetus; do 1x2 mosaic; turn to WP.,,,,,, 2009-350T16:15:00,000T08:00:00,16-Dec-09,UVIS,Prime,Saturn,MOS122APO,,,"Mosaic scan of Saturn magnetosphere. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 138.0 s, stop data capture. Repeat PATTERN 113 times. PATTERN: Slew -2.5 mrad about z-axis. Start data capture, stare 138.0 s, stop data capture.",,,,,, 2009-351T00:55:00,000T09:00:00,17-Dec-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev123 Saturn occultation on 2009/359.",,,,,, 2009-351T00:55:00,000T09:00:00,17-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-351T01:55:00,000T08:00:00,17-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09351_SP,rider,,,,,, 2009-351T10:35:00,000T00:30:00,17-Dec-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-351T11:05:00,000T02:10:00,17-Dec-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,MAPS Survey w/ prime pointing,,,,,, 2009-351T13:15:00,000T11:00:00,17-Dec-09,UVIS,Prime,Saturn,MOS122APO,,,"Mosaic scan of Saturn magnetosphere. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 142.0 s, stop data capture. Repeat PATTERN 176 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 142.0 s, stop data capture.",,,,,, 2009-351T20:00:00,000T02:00:00,17-Dec-09,INMS,Non-SPASS,Titan,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2009-351T22:00:00,000T07:54:00,17-Dec-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-352T00:55:00,000T09:00:00,18-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-352T01:55:00,000T08:00:00,18-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_122IC_DSCAL09352_SP,rider,,,,,, 2009-352T05:54:00,002T17:21:00,18-Dec-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-352T05:54:00,004T17:32:00,18-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End: S S56,Range enter= 38.002797 Rs exit= 7.7282382 Range altitude= -77287.475 km ... -40085.291,,,,,, 2009-352T05:54:00,002T03:47:00,18-Dec-09,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-352T05:54:00,004T17:32:00,18-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-352T05:54:55,000T00:00:01,18-Dec-09,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 4.9 deg, r = 37.964 Rs, phase = 104 deg",,,,,, 2009-352T05:55:00,002T17:20:00,18-Dec-09,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2009-352T05:55:00,002T17:20:00,18-Dec-09,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2009-352T10:35:00,000T02:26:00,18-Dec-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-352T10:35:00,000T02:26:00,18-Dec-09,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2009-352T13:01:00,000T11:00:00,18-Dec-09,UVIS,Prime,Saturn,MOS122APO,,,"Mosaic scan of Saturn magnetosphere. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 142.0 s, stop data capture. Repeat PATTERN 176 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 142.0 s, stop data capture.",,,,,, 2009-353T00:41:00,000T09:00:00,19-Dec-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev123 Saturn occultation on 2009/359.",,,,,, 2009-353T00:41:00,001T22:34:00,19-Dec-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2009-353T00:41:00,000T09:00:00,19-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-353T01:41:00,000T08:00:00,19-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09353_SP,rider,,,,,, 2009-353T10:21:00,000T01:15:00,19-Dec-09,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 89.3 range 3.2 Mkm",,,,,, 2009-353T10:21:00,000T01:15:00,19-Dec-09,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-353T10:21:00,000T01:15:00,19-Dec-09,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-353T11:36:00,000T01:25:00,19-Dec-09,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2009-353T13:01:00,000T11:00:00,19-Dec-09,UVIS,Prime,Saturn,MOS122APO,,,"Mosaic scan of Saturn magnetosphere. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 142.0 s, stop data capture. Repeat PATTERN 176 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 142.0 s, stop data capture.",,,,,, 2009-354T00:41:00,000T09:00:00,20-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-354T01:41:00,000T08:00:00,20-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09354_SP,rider,,,,,, 2009-354T09:41:00,001T00:00:00,20-Dec-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-354T10:21:00,000T02:40:00,20-Dec-09,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2009-354T13:01:00,000T11:00:00,20-Dec-09,UVIS,Prime,Saturn,MOS122APO,,,"Mosaic scan of Saturn magnetosphere. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 129.0 s, stop data capture. Repeat PATTERN 189times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 129.0 s, stop data capture.",,,,,, 2009-354T23:15:00,002T00:11:00,20-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2009-354T23:15:00,002T00:11:00,20-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-354T23:15:00,002T00:11:00,20-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-354T23:15:00,002T00:11:00,20-Dec-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-355T00:00:00,001T00:00:00,21-Dec-09,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2009-355T00:41:00,000T09:00:00,21-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-355T01:41:00,000T08:00:00,21-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09355_SP,rider,,,,,, 2009-355T09:41:00,001T13:45:00,21-Dec-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,MAPS magnetospheric survey,,,,,, 2009-355T10:21:00,000T02:25:00,21-Dec-09,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Siarnaq,Observation of Siarnaq,,,,,, 2009-355T10:21:00,000T02:25:00,21-Dec-09,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2009-355T12:46:00,000T02:00:00,21-Dec-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2009-355T14:46:00,000T23:00:00,21-Dec-09,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_123SA_MIRMAP001_PRIME;,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2009-356T14:26:00,000T09:00:00,22-Dec-09,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev123 Saturn occultation on 2009/359.",,,,,, 2009-356T14:26:00,000T09:00:00,22-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-356T15:26:00,000T08:00:00,22-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09356_SP,rider,,,,,, 2009-356T23:26:00,000T17:09:00,22-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2009-356T23:26:00,000T17:09:00,22-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-356T23:26:00,002T20:04:00,22-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter: S S56,Range enter= 38.002797 Rs exit= 7.7282382 Range altitude= -77287.475 km ... -40085.291,,,,,, 2009-356T23:26:00,000T00:43:00,22-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-356T23:26:00,000T17:09:00,22-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-356T23:26:00,002T03:43:00,22-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-356T23:26:00,000T17:09:00,22-Dec-09,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2009-356T23:31:00,000T00:02:00,22-Dec-09,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S56 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2009-357T00:09:00,000T00:07:00,23-Dec-09,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2009-357T00:12:00,000T13:34:00,23-Dec-09,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation.,,,,,, 2009-357T00:12:00,000T13:34:00,23-Dec-09,CIRS,SPASS Rider,rings(general),EG130PHAS,,Rider to VIMS E-G Phase,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-357T00:12:00,000T13:34:00,23-Dec-09,ISS,SPASS Rider,rings(general),EG130PHAS,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2009-357T00:16:00,000T00:05:00,23-Dec-09,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2009-357T00:21:00,000T00:33:00,23-Dec-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2009-357T00:54:00,000T00:22:59,23-Dec-09,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2009-357T01:16:59,000T22:09:01,23-Dec-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-357T14:26:00,000T09:00:00,23-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-357T15:26:00,000T08:00:00,23-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09357_SP,rider,,,,,, 2009-357T16:35:00,000T23:05:00,23-Dec-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2009-357T16:35:00,000T23:05:00,23-Dec-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-357T16:35:00,000T23:05:00,23-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-357T16:35:00,000T23:05:00,23-Dec-09,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2009-357T23:26:00,000T00:34:00,23-Dec-09,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2009-358T00:00:00,000T08:00:00,24-Dec-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-358T00:26:00,000T07:19:00,24-Dec-09,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2009-358T00:26:00,000T07:19:00,24-Dec-09,CIRS,SPASS Rider,rings(general),DUSKPTG,,Deep Space,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-358T07:45:00,000T03:00:00,24-Dec-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-358T08:00:00,000T02:00:00,24-Dec-09,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2009-358T10:00:00,000T02:42:00,24-Dec-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-358T10:45:00,000T02:41:00,24-Dec-09,ISS,Prime,Enceladus,PLMPHSB,,Phase Function Observation,Campaign to study phase function of plume. Group B,,,,,, 2009-358T10:45:00,000T02:41:00,24-Dec-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-358T12:42:00,000T10:44:00,24-Dec-09,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-358T14:26:00,000T09:00:00,24-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-358T15:26:00,000T08:00:00,24-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09358_SP,rider,,,,,, 2009-358T15:40:00,002T17:32:00,24-Dec-09,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2009-358T15:40:00,001T06:55:59,24-Dec-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-358T15:40:00,002T17:32:00,24-Dec-09,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2009-358T23:26:00,000T17:31:00,24-Dec-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2009-359T00:26:00,000T06:51:00,25-Dec-09,ISS,Prime,rings(general),SHADBNDLE,,Shadow boundary in the E and G Rings at low elevat,Shadow boundary in the E and G Rings at low elevation angle,,,,,, 2009-359T00:26:00,000T06:51:00,25-Dec-09,CIRS,SPASS Rider,rings(general),SHADBNDLE,,CIRS_RIRI_SHADBNDLE001_ISS,rider,,,,,, 2009-359T03:09:00,000T18:14:00,25-Dec-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-359T07:57:00,000T09:00:00,25-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-359T08:57:00,000T08:00:00,25-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09359_SP,rider,,,,,, 2009-359T16:52:00,000T02:05:00,25-Dec-09,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 123RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2009-359T16:57:00,000T01:40:00,25-Dec-09,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,,,,,,, 2009-359T16:57:00,000T02:03:00,25-Dec-09,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2009-359T18:57:00,000T02:26:00,25-Dec-09,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ansa-to-Ansa Ring Occ - Ingress,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2009-359T19:00:00,000T02:00:00,25-Dec-09,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2009-359T19:30:00,000T01:43:00,25-Dec-09,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 7.7103462 Rs exit= 4.4276298 Range altitude= -39995.239 km ... -20013.073,,,,,, 2009-359T20:00:00,000T04:22:00,25-Dec-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-359T21:00:00,001T12:12:00,25-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-359T21:13:00,000T03:34:00,25-Dec-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 7.7103462 Rs exit= 4.4276298 Range altitude= -39995.239 km ... -20013.073,,,,,, 2009-359T21:23:00,000T03:14:00,25-Dec-09,ISS,Prime,Enceladus,PLMSCECL,,High phase obs with s/c in eclipse,LIEN. Very High phase obs with s/c in eclipse. Absolutely critical. Vital. WE REALLY NEED THIS!!!!!,,,,,, 2009-359T21:23:00,000T03:14:00,25-Dec-09,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 123RI OCC Thermal Stabilization,Thermal stabilization period between the ingress and egress occultations.,,,,,, 2009-359T21:23:00,000T03:14:00,25-Dec-09,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2009-359T21:23:00,000T03:14:00,25-Dec-09,VIMS,SPASS Rider,Enceladus,PLMSCECL,,"Enceladus Plume, high phase",null,,,,,, 2009-359T22:35:59,000T02:46:01,25-Dec-09,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE4 flyby,Monitor the interaction of Tethys with the Saturnian magnetosphere.,,,,,, 2009-360T00:22:00,000T15:38:00,26-Dec-09,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2009-360T00:22:00,001T07:52:00,26-Dec-09,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-360T00:37:00,000T00:39:00,26-Dec-09,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Atmospheric Occultation on rev 123 egress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2009-360T00:47:00,000T00:29:00,26-Dec-09,CDA,Non-SPASS,Other,RATE080B,,Data rate,Range enter= 7.7103462 Rs exit= 4.4276298 Range altitude= -39995.239 km ... -20013.073,,,,,, 2009-360T01:16:00,000T02:42:00,26-Dec-09,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ansa-to-Ansa Ring Occ - Egress,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2009-360T01:16:00,000T03:42:00,26-Dec-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.4079870 Rs exit= 3.8776493 Range altitude= -19860.439 km ... 19976.794,,,,,, 2009-360T01:22:00,000T08:37:00,26-Dec-09,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2009-360T01:22:00,000T01:13:59,26-Dec-09,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE4 flyby,"Monitor the interaction of Tethys with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD request.",,,,,, 2009-360T03:49:00,000T02:00:00,26-Dec-09,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2009-360T03:50:53,000T02:00:00,26-Dec-09,CDA,SPASS Rider,DustRAM direction,RPX0000,,CDA RPXing 2009-360T04:50:53,RPXing at 2.6985712 Rs,,,,,, 2009-360T04:58:00,000T02:27:00,26-Dec-09,ISS,Prime,Prometheus,PROMPROP,,"Prometheus close flyby, Propellor observation","Prometheus close flyby, ~56,300 km at CA, 36 deg phase. followed by propellor imaging",,,,,, 2009-360T04:58:00,000T02:27:00,26-Dec-09,CIRS,SPASS Rider,rings(general),PROMPROP,,Rider to ISS Prometheus and Rings,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-360T04:58:00,000T02:27:00,26-Dec-09,UVIS,SPASS Rider,Prometheus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-360T04:58:00,000T02:27:00,26-Dec-09,VIMS,SPASS Rider,Prometheus,PROMPROP,,Prometheus,Combined Prometheus & Ring propeller obs; multiple 16/640 ms.,,,,,, 2009-360T04:58:00,000T02:27:00,26-Dec-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.4079870 Rs exit= 3.8776493 Range altitude= -19860.439 km ... 19976.794,,,,,, 2009-360T05:40:54,000T00:00:01,26-Dec-09,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.590 Rs, lat = 2 deg, phase = 76 deg",,,,,, 2009-360T07:25:00,000T01:46:12,26-Dec-09,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.4079870 Rs exit= 3.8776493 Range altitude= -19860.439 km ... 19976.794,,,,,, 2009-360T07:35:00,000T02:00:00,26-Dec-09,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-360T07:35:00,000T02:00:00,26-Dec-09,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_123RI_EQLBN001_SI,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2009-360T07:35:00,000T02:00:00,26-Dec-09,UVIS,SPASS Rider,rings(general),EQLBN,,URSTAR,,,,,,, 2009-360T07:35:00,000T02:00:00,26-Dec-09,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2009-360T09:11:12,000T13:30:48,26-Dec-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.8965981 Rs exit= 15.996729 Range altitude= 20056.427 km ... 19099.107,,,,,, 2009-360T09:35:00,000T01:25:00,26-Dec-09,VIMS,Prime,Enceladus,344W001PH,,Enceladus zero-phase,null,,,,,, 2009-360T09:35:00,000T01:25:00,26-Dec-09,ISS,SPASS Rider,Enceladus,344W001PH,,Enceladus spectrophotometry/ phase coverage,VIMS point-and-stare at low phase angle,,,,,, 2009-360T09:35:00,000T01:25:00,26-Dec-09,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-360T09:59:00,000T22:16:00,26-Dec-09,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2009-360T11:00:00,000T02:30:00,26-Dec-09,VIMS,Prime,rings(general),LOWPHASE,Low phase imaging,Low phase observation,Target rings approx 3 deg south of zero-phase point & scan across right ansa from limb to beyond G ring.,,,,,, 2009-360T11:00:00,000T02:30:00,26-Dec-09,CIRS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,CIRS_RIRI_LOWPHASE001_VIMS,rider,,,,,, 2009-360T11:00:00,000T02:30:00,26-Dec-09,ISS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,WAC radial scan in color filters riding on VIMS sc,"6 filter, 6 deg phase, lit face; 5 RS!",,,,,, 2009-360T11:00:00,000T02:30:00,26-Dec-09,UVIS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,URSTAR,,,,,,, 2009-360T13:30:00,000T02:00:00,26-Dec-09,VIMS,Prime,Dione,327W000PH,,Dione zero-phase,null,,,,,, 2009-360T13:30:00,000T02:00:00,26-Dec-09,ISS,SPASS Rider,Dione,327W000PH,,Dione zerophase,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-360T13:30:00,000T02:00:00,26-Dec-09,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2009-360T15:30:00,000T05:12:00,26-Dec-09,CDA,Prime,DustRAM direction,RPX0000,,CDA Rings,"Ring scan 7...9 Rs, CDA to 222 deg.",,,,,, 2009-360T20:42:00,000T02:00:00,26-Dec-09,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"low-latitude, lit-face ring photometry","low latitude lit #1: B = 2, phase ~ 52, B' = 2",,,,,, 2009-360T20:42:00,000T02:00:00,26-Dec-09,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,CIRS_RIRI_PHOTLIT001_ISS,rider,,,,,, 2009-360T20:42:00,000T02:00:00,26-Dec-09,VIMS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,WAC mosaic?,"160 ms, 32*32 cubes?",,,,,, 2009-360T22:42:00,000T01:30:00,26-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 3.8965981 Rs exit= 15.996729 Range altitude= 20056.427 km ... 19099.107,,,,,, 2009-361T00:12:00,000T10:45:12,27-Dec-09,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.8965981 Rs exit= 15.996729 Range altitude= 20056.427 km ... 19099.107,,,,,, 2009-361T00:12:00,000T09:00:00,27-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-361T01:12:00,000T08:00:00,27-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09361_SP,rider,,,,,, 2009-361T08:14:00,000T00:58:00,27-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-361T08:15:00,000T00:57:00,27-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-361T09:12:00,000T13:04:59,27-Dec-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2009-361T09:12:00,000T13:04:59,27-Dec-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-361T09:12:00,000T14:04:59,27-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-361T09:12:00,000T11:04:59,27-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-361T09:12:00,003T00:00:00,27-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-361T10:07:24,000T04:09:35,27-Dec-09,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2009-361T10:07:24,000T04:09:35,27-Dec-09,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-361T10:07:24,000T01:09:35,27-Dec-09,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Global mapping,"Stare at Titan for global mapping. Phase = 136 deg. Lat/Lon = 03N/12 deg. Resolution = 142 - 129 km/px. Temp. = M4. Obtain 32x32, 48x48, 64x64 cubes at 160 and 640 ms exp. times.",,,,,, 2009-361T10:57:12,001T22:14:48,27-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.008632 Rs exit= 3.8707448 Range altitude= 19078.514 km ... -40511.880,,,,,, 2009-361T11:16:59,000T03:00:00,27-Dec-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Global mapping,"Stare at Titan for global mapping. Phase = 136 deg. Lat/Lon = 03N/13 deg. Resolution = 129 - 99 km/px. Temp. = N. Obtain 48x48, 64x64 cubes at 160 and 640 ms exp. times.",,,,,, 2009-361T14:16:59,000T01:00:00,27-Dec-09,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-361T14:16:59,000T01:00:00,27-Dec-09,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS.,,,,,, 2009-361T14:16:59,000T01:00:00,27-Dec-09,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Global mapping,Stare at Titan. Phase = 136 deg. Lat/Lon = 03N/16 deg. Resolution = 99 - 89 km/px. Temp. = N. Obtain 64x64 cubes at 80 and 160 ms exp. times.,,,,,, 2009-361T15:16:59,000T04:00:00,27-Dec-09,CIRS,Prime,Titan,MIRLMPAIR,,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-361T15:16:59,000T04:00:00,27-Dec-09,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2009-361T15:16:59,000T04:00:00,27-Dec-09,ISS,SPASS Rider,Titan,MIRLMPAIR,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-361T15:16:59,000T04:00:00,27-Dec-09,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-361T15:16:59,000T04:00:00,27-Dec-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping,Limb mapping of Titan. Phase = 136 deg. Lat/Lon = 04N/17 deg. Resolution = 89 - 47 km/px. Temp. = R. Obtain various cubes for limb mapping.,,,,,, 2009-361T19:16:59,000T02:45:00,27-Dec-09,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2009-361T19:16:59,000T02:45:00,27-Dec-09,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (3 integrations total = 6 frames, 0.5 Mb/frame)",,,,,, 2009-361T19:16:59,000T04:22:00,27-Dec-09,RADAR,SPASS Rider,Titan,T64WARMUP,,Warmup for T64,,,,,,, 2009-361T19:16:59,000T02:45:00,27-Dec-09,UVIS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,UVIS Rider to CIRS FIRNADMAP,UVIS Rider to CIRS FIRNADMAP,,,,,, 2009-361T19:16:59,000T02:45:00,27-Dec-09,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,Slow scan across Titan. Phase = 136 deg. Lat/Lon = 05N/21 deg. Resolution = 47 - 25 km/px. Temp. = T.,,,,,, 2009-361T20:16:59,000T08:00:00,27-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-361T20:16:59,000T08:00:00,27-Dec-09,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T64 flyby,"T64 is a north polar, dusk, flyby, with a minimum altitude of 1000 km. In nominal upstream conditions, Cassini would explore the north lobe of Titan's magnetic tail, very close to the moon. Due to the location of the point of closest approach, it is potentially important regarding the detection of an intrinsic magnetic field, but not as good as T70. With adequate pointing of MAPS plasma instruments MAG data will be extremely helpful in the identification of escaping particles similar to those that could be seen in T63. If the upstream conditions are similar to T63, T64 will be extremely important to the determination of the structure of Titan's magnetic tail in the dusk sector. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2009-361T21:52:59,000T01:30:00,27-Dec-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-361T22:01:59,000T00:59:00,27-Dec-09,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2009-361T22:01:59,000T00:59:00,27-Dec-09,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-361T22:01:59,000T00:59:00,27-Dec-09,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-361T22:01:59,000T00:59:00,27-Dec-09,UVIS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2009-361T22:01:59,000T00:59:00,27-Dec-09,VIMS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,Regional mapping.,Regional mapping of Titan. Phase = 136 deg. Lat/Lon = 07N/24 deg. Resolution = 21 - 6.5 km/px. Obtain 64x64 cubes at 80 ms exp. times for regional mapping.,,,,,, 2009-361T22:16:59,000T01:00:00,27-Dec-09,CAPS,SPASS Rider,Titan,T64INBD,,Titan Encounter,null,,,,,, 2009-361T22:16:59,000T01:00:00,27-Dec-09,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-361T23:01:59,000T00:37:00,27-Dec-09,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2009-361T23:01:59,000T00:37:00,27-Dec-09,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2009-361T23:01:59,000T00:37:00,27-Dec-09,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-361T23:01:59,000T00:37:00,27-Dec-09,VIMS,SPASS Rider,Titan,FIRLMBCON,,Regional mapping.,Regional mapping of Titan. Phase = 136 deg. Lat/Lon = 07N/24 deg. Resolution = 21 - 6.5 km/px. Obtain 64x64 cubes at 80 ms exp. times for regional mapping.,,,,,, 2009-361T23:16:59,000T02:00:00,27-Dec-09,CAPS,SPASS Rider,Titan,T64CLOSE,,Titan Encounter,null,,,,,, 2009-361T23:16:59,000T02:00:00,27-Dec-09,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-361T23:16:59,000T00:48:00,27-Dec-09,INMS,Non-SPASS,Titan,TITAN64,,Titan Flyby,Titan observation,,,,,, 2009-361T23:22:59,000T01:48:00,27-Dec-09,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2009-361T23:38:59,000T00:20:00,27-Dec-09,RADAR,Prime,Titan,T64INALT,,T64 Inbound Altimetry,,,,,,, 2009-361T23:58:59,000T00:06:00,27-Dec-09,RADAR,Prime,Titan,T64INSAR,,T64 Inbound SAR,,,,,,, 2009-362T00:04:59,000T00:12:00,28-Dec-09,RADAR,Prime,Titan,T64RASAR,,T64 Ride-along SAR with INMS,,,,,,, 2009-362T00:04:59,000T00:12:00,28-Dec-09,INMS,SPASS Rider,Titan,TITAN64,,Titan Flyby,Prime Titan observation,,,,,, 2009-362T00:16:59,000T00:18:00,28-Dec-09,RADAR,Prime,Titan,T64OUTSAR,,T64 Outbound SAR,,,,,,, 2009-362T00:16:59,000T01:00:00,28-Dec-09,INMS,Non-SPASS,Titan,TITAN64,,Titan Flyby,Titan observation,,,,,, 2009-362T00:34:59,000T00:12:00,28-Dec-09,RADAR,Prime,Titan,T64OUTALT,,T64 Outbound Altimetry,,,,,,, 2009-362T00:46:59,000T00:28:00,28-Dec-09,RADAR,Prime,Titan,T64OHISAR,,T64 outbound HiSAR,,,,,,, 2009-362T01:10:59,000T01:30:00,28-Dec-09,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2009-362T01:14:59,000T00:24:00,28-Dec-09,CIRS,SPASS Rider,Titan,RIDER,Instrument rider,,Ride along with VIMS.,,,,,, 2009-362T01:14:59,000T00:21:05,28-Dec-09,VIMS,SPASS Rider,Titan,TRANS,,Transition to RWA,RCS/RWA transition. Phase = 44 deg. Lat/Lon = 00N/206 deg. Resolution = 8.5 km/px. Obtain 64x64 cubes at 160 ms exp.,,,,,, 2009-362T01:16:59,000T01:00:00,28-Dec-09,CAPS,SPASS Rider,Titan,T64OUTBND,,Titan Encounter,null,,,,,, 2009-362T01:16:59,000T01:00:00,28-Dec-09,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2009-362T01:16:59,002T07:55:00,28-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-362T01:36:04,000T00:40:55,28-Dec-09,VIMS,Prime,Titan,HIRES,High resolution image,3x3 Titan Mosaic IT=55 ms; regional mapping,Hi-res regional mapping for Titan mosaics. Phase = 44 deg. Lat/Lon = 03S/207 deg. Resolution = 12 - 19 km/px. Landing site environment,,,,,, 2009-362T01:36:04,000T00:40:55,28-Dec-09,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-362T01:38:59,000T00:38:00,28-Dec-09,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with VIMS.,,,,,, 2009-362T02:16:59,000T03:00:00,28-Dec-09,VIMS,Prime,Titan,REGMAP,Regional mapping,3x3 Titan mosaic IT=80ms regional mapping + 2x2 mo,VIMS regional mapping. Phase = 44 deg. Lat/Lon = 06S/208 deg. Resolution = 19 - 49 km/px. Temp. Y,,,,,, 2009-362T02:16:59,000T16:48:01,28-Dec-09,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2009-362T02:16:59,000T03:00:00,28-Dec-09,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with VIMS.,,,,,, 2009-362T02:16:59,000T03:00:00,28-Dec-09,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-362T02:16:59,000T16:48:01,28-Dec-09,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2009-362T04:16:59,000T14:48:01,28-Dec-09,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2009-362T05:16:59,000T04:00:00,28-Dec-09,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2009-362T05:16:59,000T04:00:00,28-Dec-09,CIRS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-362T05:16:59,000T04:00:00,28-Dec-09,UVIS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,UVIS Rider to CIRS MIRLMBMAP,UVIS Rider to CIRS Mid IR Limb observation,,,,,, 2009-362T05:16:59,000T04:00:00,28-Dec-09,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping,Limb mapping of Titan. Phase = 44 deg. Lat/Lon = 09S/211 deg. Resolution = 49 - 89 km/px. Temp. = F. Obtain various cubes for limb mapping.,,,,,, 2009-362T09:16:59,000T03:00:00,28-Dec-09,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2009-362T09:16:59,000T03:00:00,28-Dec-09,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2009-362T09:16:59,000T03:00:00,28-Dec-09,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-362T09:16:59,000T03:00:00,28-Dec-09,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2009-362T09:16:59,000T03:00:00,28-Dec-09,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Global mapping,Stare at Titan for global mapping. Phase = 44 deg. Lat/Lon = 10S/215 deg. Resolution = 89 - 119 km/px. Temp. = D2. Obtain 64x64 and 48x48 cubes at 160 and 640 ms exp. times.,,,,,, 2009-362T12:16:59,000T02:00:00,28-Dec-09,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,NMO (NAC Monitor),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-362T12:16:59,000T02:00:00,28-Dec-09,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Ride along with ISS.,,,,,, 2009-362T12:16:59,000T02:00:00,28-Dec-09,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,Global mapping,Stare at Titan. Phase = 45 deg. Lat/Lon = 10S/217 deg. Resolution = 119 - 139 km/px. Temp. = D2. Obtain 48x48 cubes at 160 and 640 ms exp. times.,,,,,, 2009-362T14:16:59,000T09:00:00,28-Dec-09,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping,"IT=160 & 640 every other hour VIMS global mapping of Titan. Phase = 45 deg. Lat/Lon = 10S/219 deg. Resolution = 139 - 230 km/px. Temp. = B(Z). Obtain 32x32, 48x48, 64x64 cubes at various exp. times.",,,,,, 2009-362T14:16:59,000T09:00:00,28-Dec-09,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2009-362T14:16:59,000T09:00:00,28-Dec-09,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2009-362T19:05:00,001T14:07:00,28-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2009-362T19:05:00,001T14:07:00,28-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-362T19:05:00,001T14:07:00,28-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-363T00:12:00,000T09:00:00,29-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-363T01:12:00,000T08:00:00,29-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09363_SP,rider,,,,,, 2009-363T09:12:00,001T00:00:00,29-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.008632 Rs exit= 3.8707448 Range altitude= 19078.514 km ... -40511.880,,,,,, 2009-363T09:52:00,000T02:00:00,29-Dec-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-363T09:52:00,000T02:00:00,29-Dec-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan. Cloud mapping.,Caboose segment. VIMS ridealong for cloud mapping. Phase = 47 deg. Lat/Lon = 10S/234 deg. Resolution = 340 km/px. Obtain cubes at exp. times of 80 and 640 ms.,,,,,, 2009-363T11:52:00,000T02:00:00,29-Dec-09,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2009-363T11:52:00,000T02:00:00,29-Dec-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan. Cloud mapping.,Caboose segment. VIMS ridealong for cloud mapping. Phase = 48 deg. Lat/Lon = 10S/236 deg. Resolution = 361 km/px. Obtain cubes at exp. times of 80 and 640 ms.,,,,,, 2009-363T13:52:00,000T01:40:00,29-Dec-09,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2009-363T13:52:00,000T01:40:00,29-Dec-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan. Cloud mapping.,Caboose segment. VIMS ridealong for cloud mapping. Phase = 48 deg. Lat/Lon = 10S/237 deg. Resolution = 382 km/px. Obtain cubes at exp. times of 80 and 640 ms.,,,,,, 2009-363T15:32:00,000T08:00:00,29-Dec-09,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2009-363T15:32:00,000T08:00:00,29-Dec-09,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan. Cloud mapping.,Caboose segment. VIMS ridealong for cloud mapping. Phase = 48 deg. Lat/Lon = 10S/239 deg. Resolution = 400 km/px. Obtain cubes at exp. times of 80 and 640 ms.,,,,,, 2009-364T00:12:00,000T09:00:00,30-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-364T01:12:00,000T08:00:00,30-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09364_SP,rider,,,,,, 2009-364T09:12:00,001T06:18:00,30-Dec-09,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2009-364T09:12:00,001T06:18:00,30-Dec-09,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2009-364T09:12:00,003T18:37:00,30-Dec-09,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.008632 Rs exit= 3.8707448 Range altitude= 19078.514 km ... -40511.880,,,,,, 2009-364T09:12:00,000T23:45:00,30-Dec-09,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2009-364T09:12:00,001T06:18:00,30-Dec-09,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2009-364T09:12:00,003T18:37:00,30-Dec-09,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2009-364T09:52:00,000T01:15:00,30-Dec-09,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 52 range 1.2 Mkm",,,,,, 2009-364T09:52:00,000T01:15:00,30-Dec-09,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-364T09:52:00,000T01:15:00,30-Dec-09,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-364T11:07:00,000T03:40:00,30-Dec-09,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2009-364T14:47:00,000T08:00:00,30-Dec-09,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_123SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2009-364T14:47:00,000T08:00:00,30-Dec-09,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2009-364T22:47:00,000T00:30:00,30-Dec-09,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2009-364T23:57:00,000T09:00:00,30-Dec-09,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2009-365T00:00:00,000T09:10:00,31-Dec-09,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,Full Calibration,null,,,,,, 2009-365T00:57:00,000T08:00:00,31-Dec-09,CIRS,SPASS Rider,InstrumentCalibration,DSCAL09,Deep space calibration,CIRS_123IC_DSCAL09365_SP,rider,,,,,, 2009-365T08:57:00,002T00:01:00,31-Dec-09,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2009-365T09:37:00,000T01:15:00,31-Dec-09,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 57.9 range 1.7 Mkm",,,,,, 2009-365T09:37:00,000T01:15:00,31-Dec-09,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2009-365T09:37:00,000T01:15:00,31-Dec-09,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2009-365T10:52:00,000T23:00:00,31-Dec-09,CIRS,Prime,Saturn,MIRTMAP,,CIRS_123SA_MIRTMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2009-365T15:30:00,005T00:40:00,31-Dec-09,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2009-365T15:30:00,002T12:20:00,31-Dec-09,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2009-365T15:30:00,004T00:20:00,31-Dec-09,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2009-365T15:30:00,002T12:19:00,31-Dec-09,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-001T09:52:00,000T04:00:00,1-Jan-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-001T09:52:00,000T04:00:00,1-Jan-10,CIRS,SPASS Rider,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-001T13:52:00,000T06:40:00,1-Jan-10,VIMS,Prime,Other,PLEIADES,Pleiades,Pleiades,"Turn to Pleiades; Time: 30 min Pleiades: multiple cubes w/64x64 FOV IR @ 640 ms, VIS @ 40000 ms; Time: 6.0 hr 40 min; Volume: 86.5 Mbits; CompRatio: 2.0 Turn to waypoint: 30 min Primary: -y to Pleiades; Secondary: +z to TBD Not time critical. RWA REQUIRED.",,,,,, 2010-001T13:52:00,000T06:40:00,1-Jan-10,CIRS,SPASS Rider,rings(general),PLEIADES,Pleiades,CAL for preceding EQLBS,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-001T20:32:00,000T02:00:00,1-Jan-10,ISS,Prime,Titan,ECLIPSE0,,Titan NAC Photopol 90 Phase,Long exposures to search for auroras and lightning on Titan in eclipse. This is one of several possible events but distant from Titan,,,,,, 2010-001T20:32:00,000T02:00:00,1-Jan-10,UVIS,SPASS Rider,Titan,ECLIPSE,,Rider to ISS ECLIPSE,Rider to ISS TI_ECLIPSE - to look for emissions from electron/ion impact during eclipse when sunlight is absent,,,,,, 2010-001T22:32:00,000T00:46:00,1-Jan-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-001T23:58:00,000T09:00:00,1-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-002T00:58:00,000T08:00:00,2-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_123IC_DSCAL10002_SP,rider,,,,,, 2010-002T08:58:00,000T11:02:00,2-Jan-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-002T09:38:00,000T04:00:00,2-Jan-10,ISS,Prime,rings(general),PHOTDARK,,"intermediate phase, dark-face ring photometry","intermediate unlit #10: B = -10, phase = 102, B' = 2.2",,,,,, 2010-002T09:38:00,000T04:00:00,2-Jan-10,CIRS,SPASS Rider,rings(general),PHOTDARK,,RIDER to ISS Rings Prime Science,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-002T13:38:00,000T04:00:00,2-Jan-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-002T13:38:00,000T04:00:00,2-Jan-10,CIRS,SPASS Rider,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-002T17:38:00,000T05:10:00,2-Jan-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-002T17:38:00,000T05:10:00,2-Jan-10,CIRS,SPASS Rider,rings(general),SWAURPTG,MAPS aurora campaign,CAL for preceding EQLBS,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-002T20:00:00,000T02:00:00,2-Jan-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-002T22:00:00,000T05:50:00,2-Jan-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-002T22:48:00,000T00:30:00,2-Jan-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 017 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-002T23:58:00,000T09:00:00,2-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-003T00:58:00,000T08:00:00,3-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_123IC_DSCAL10003_SP,rider,,,,,, 2010-003T03:49:00,007T20:26:12,3-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.008632 Rs exit= 3.8707448 Range altitude= 19078.514 km ... -40511.880,,,,,, 2010-003T03:49:00,003T04:54:00,3-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-003T03:49:00,000T05:09:00,3-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-003T03:50:00,002T04:53:00,3-Jan-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-003T03:50:00,002T04:53:00,3-Jan-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-003T03:50:30,000T00:00:01,3-Jan-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 21.6 deg, r = 37.515 Rs, phase = 104 deg",,,,,, 2010-003T09:38:00,000T01:15:00,3-Jan-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 80.8 range 2.9 Mkm",,,,,, 2010-003T09:38:00,000T01:15:00,3-Jan-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-003T09:38:00,000T01:15:00,3-Jan-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-003T10:53:00,000T08:00:00,3-Jan-10,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar Port to Sun,Turn to sun; Time: 30 min Solar Port: same 5*7 cross design as on revs A and C; tau_IR = 40 & 320 msec; VIS always @ 50ms; Total time: 8hr; Volume: 240 Mbits; Solar Background Calibration: 4 cubes w/64x64 FOV; Time: 30 min; Turn to waypoint: 30 min,,,,,, 2010-003T18:53:00,000T04:10:00,3-Jan-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-003T19:43:00,000T07:00:00,3-Jan-10,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-55 in 1-way mode.,,,,,, 2010-003T23:38:00,000T09:05:00,3-Jan-10,RSS,SPASS Rider,Saturn,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev124 Saturn gravity observation on 2010/010 and Rev125 Saturn rings and atmospheric occultation on 2010/026.",,,,,, 2010-003T23:43:00,000T09:00:00,3-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-004T00:43:00,000T08:00:00,4-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10004_SP,rider,,,,,, 2010-004T09:00:00,000T06:00:00,4-Jan-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-004T09:23:00,000T03:00:00,4-Jan-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Erriapus,Observation of Erriapus,,,,,, 2010-004T09:23:00,000T03:00:00,4-Jan-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-004T12:23:00,000T08:00:00,4-Jan-10,VIMS,Prime,Star,FOMALHAUT,Fomalhaut,Fomalhaut,"Turn to Fomalhaut; Time: 30 min Fomalhaut: multiple cubes w/32x32 FOV IR @ 640 ms, VIS @ 20000 ms; Time: 7.0 hr 30 min; Volume: 187 Mbits; CompRatio: 3.0 Turn to waypoint: 30 min Primary: -y to Fomalhaut; Secondary: +z to TBD Not time critical. RWA REQUIRED.",,,,,, 2010-004T15:50:00,000T16:53:00,4-Jan-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-004T20:23:00,000T02:40:00,4-Jan-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-004T23:43:00,000T09:00:00,4-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-005T00:43:00,000T08:00:00,5-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10005_SP,rider,,,,,, 2010-005T08:43:00,001T00:00:00,5-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-005T08:43:00,001T00:00:00,5-Jan-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-005T08:43:00,000T00:40:00,5-Jan-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-005T09:23:00,000T06:45:00,5-Jan-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-005T09:23:00,000T06:45:00,5-Jan-10,CIRS,SPASS Rider,rings(general),CALROLL,MAG calibration roll,CAL for following POLARIZ,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-005T09:23:00,000T06:45:00,5-Jan-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-005T16:08:00,000T06:55:00,5-Jan-10,CIRS,Prime,rings(general),POLARIZ,,CIRS_124RI_POLARIZ005_PRIME;,This observation requires 3 unique secondaries separated by approximately 60 degrees.,,,,,, 2010-005T16:08:00,000T06:55:00,5-Jan-10,CIRS,SPASS Rider,rings(general),POLARIZ,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-005T16:08:00,000T00:02:00,5-Jan-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-005T16:10:00,000T16:33:00,5-Jan-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-005T16:10:00,000T16:33:00,5-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-005T23:43:00,000T09:00:00,5-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-006T00:43:00,000T08:00:00,6-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10006_SP,rider,,,,,, 2010-006T08:43:00,002T03:52:00,6-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-006T08:43:00,002T03:52:00,6-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-006T08:43:00,002T22:17:00,6-Jan-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-006T08:43:00,002T03:52:00,6-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-006T08:43:00,003T15:18:00,6-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-006T08:43:00,002T03:52:00,6-Jan-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-006T09:00:00,000T04:00:00,6-Jan-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-006T09:00:00,000T04:00:00,6-Jan-10,CIRS,SPASS Rider,rings(general),MAGBNDPTG,MAPS magnetosphere boundary campaign,CAL before ISS Spoke Movie Rider and CIRS EQLBS,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-006T13:00:00,000T12:55:00,6-Jan-10,ISS,Prime,rings(general),SPKMVDFHP,,unLit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2010-006T13:00:00,000T12:55:00,6-Jan-10,CIRS,SPASS Rider,rings(general),SPKMVDFHP,,Rider to ISS Spoke Movie,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-006T13:00:00,000T12:55:00,6-Jan-10,VIMS,SPASS Rider,rings(general),SPKMVDFHP,,"Spoke movie, dark face, high phase",ISS rider,,,,,, 2010-007T01:55:00,000T05:00:00,7-Jan-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-007T01:55:00,000T05:00:00,7-Jan-10,CIRS,SPASS Rider,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-007T06:55:00,000T09:40:00,7-Jan-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-007T07:13:00,000T09:00:00,7-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-007T08:13:00,000T08:00:00,7-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10007_SP,rider,,,,,, 2010-007T16:35:00,000T15:30:00,7-Jan-10,ISS,Prime,rings(general),LRHPENKMV,,"Encke Ringlet Movie, need 2 of 7","Low res, high phase movies of Encke Ringlets; need 2 of 7, widely spaced in time Also WACs at regular intervals looking for spokes",,,,,, 2010-007T16:35:00,000T15:30:00,7-Jan-10,CIRS,SPASS Rider,rings(general),LRHPENKMV,,Rider to ISS Ring Movie,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-007T16:35:00,000T15:30:00,7-Jan-10,VIMS,SPASS Rider,rings(general),LRHPENKMV,,"Encke gap movie, dark face, high phase",ISS rider,,,,,, 2010-008T08:05:00,000T05:00:00,8-Jan-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-008T08:05:00,000T05:00:00,8-Jan-10,CIRS,SPASS Rider,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-008T12:35:00,000T17:55:00,8-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-008T12:35:00,000T17:55:00,8-Jan-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-008T12:35:00,000T17:55:00,8-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-008T12:35:00,000T15:42:00,8-Jan-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-008T13:28:00,000T09:00:00,8-Jan-10,RSS,SPASS Rider,Saturn,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev124 Saturn gravity observation on 2010/010 and Rev125 Saturn rings and atmospheric occultation on 2010/026.",,,,,, 2010-008T13:28:00,000T09:00:00,8-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-008T14:28:00,000T08:00:00,8-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10008_SP,rider,,,,,, 2010-008T22:50:00,000T12:15:00,8-Jan-10,VIMS,Prime,rings(general),FMOVIE,F ring movie,F Ring movie,"64x12 frame, hi res mode. 640 msec tau_IR.",,,,,, 2010-008T22:50:00,000T12:15:00,8-Jan-10,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,Rider to VIMS F-Ring Movie,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-009T06:30:00,003T00:15:00,9-Jan-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-009T06:30:00,001T16:30:59,9-Jan-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-009T06:30:00,003T01:44:00,9-Jan-10,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2010-009T07:00:00,000T02:00:00,9-Jan-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-009T09:00:00,000T13:29:00,9-Jan-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-009T11:05:00,000T02:00:00,9-Jan-10,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2010-009T11:05:00,000T02:00:00,9-Jan-10,CIRS,SPASS Rider,rings(general),SURVEYPTG,MAPS survey/Prime pointing,CAL after VIMS F-Ring Rider,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-009T13:29:00,000T09:00:00,9-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-009T14:29:00,000T08:00:00,9-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10009_SP,rider,,,,,, 2010-009T22:29:00,000T17:30:00,9-Jan-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-009T23:29:00,000T04:01:00,9-Jan-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-009T23:29:00,000T04:01:00,9-Jan-10,CIRS,SPASS Rider,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-010T00:01:00,002T06:45:00,10-Jan-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-010T03:30:00,000T03:00:00,10-Jan-10,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2010-010T03:30:00,000T03:00:00,10-Jan-10,CIRS,SPASS Rider,rings(general),SHRTMOV,,Rider to ISS Movie,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-010T06:59:00,000T09:00:00,10-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-010T07:59:00,000T08:00:00,10-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10010_SP,rider,,,,,, 2010-010T15:59:00,000T00:07:46,10-Jan-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-010T16:06:46,000T08:50:00,10-Jan-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-010T16:30:00,000T06:50:00,10-Jan-10,ISS,Prime,RingD,PINGPONG,,D Ring Ping Pong,D Ring Ping Pong,,,,,, 2010-010T16:30:00,000T06:50:00,10-Jan-10,CIRS,SPASS Rider,rings(general),PINGPONG,,Rider to ISS Ping Pong,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-010T16:30:00,000T06:50:00,10-Jan-10,VIMS,SPASS Rider,RingD,PINGPONG,,"D ring ping-pong movie, high phase, 7 R_S",ISS rider,,,,,, 2010-010T22:05:00,000T02:05:00,10-Jan-10,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2010-010T23:00:59,000T08:57:00,10-Jan-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-011T00:10:00,000T06:40:00,11-Jan-10,RSS,SPASS Rider,Saturn,GRAVITY,RSS gravity science experiment,RSS Saturn's Gravity Field Experiment,Experiment to determine Saturn's gravity field and infer constraints on its internal structure.,,,,,, 2010-011T00:10:00,000T00:30:00,11-Jan-10,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2010-011T00:15:12,000T00:52:00,11-Jan-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.8552860 Rs exit= 3.4973475 Range altitude= -39757.003 km ... -20362.947,,,,,, 2010-011T00:40:00,000T11:20:00,11-Jan-10,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2010-011T00:56:46,000T02:00:00,11-Jan-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-011T00:57:00,000T02:00:00,11-Jan-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-011T00:58:12,000T02:00:00,11-Jan-10,CDA,SPASS Rider,DustRAM direction,RPX0010,,CDA RPXing 2010-011T01:58:12 MMH,RPXing at 3.2150680 Rs vertical crossing,,,,,, 2010-011T01:00:00,000T00:16:00,11-Jan-10,RPWS,Non-SPASS,Saturn,WHISTLER,RPWS lightning search,Obtain wideband examples of lightning whistlers,Obtain wideband evidence of lightning whistlers. These would verify the existence of lightning already suspected from Saturn Electrostatic Discharges (SED) and would provide information on the electron density along the field line to the source. No pointing requirement.,,,,,, 2010-011T01:07:12,000T01:40:00,11-Jan-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.4843869 Rs exit= 3.0422732 Range altitude= -19568.831 km ... 19830.159,,,,,, 2010-011T02:47:12,000T00:52:00,11-Jan-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.0380872 Rs exit= 3.0084518 Range altitude= 20618.442 km ... 39526.112,,,,,, 2010-011T02:56:46,000T23:00:00,11-Jan-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-011T03:23:15,000T00:00:01,11-Jan-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.999 Rs, lat = 11 deg, phase = 76 deg",,,,,, 2010-011T03:39:12,008T00:37:48,11-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.0103116 Rs exit= 7.5951306 Range altitude= 40241.954 km ... -40068.160,,,,,, 2010-011T07:25:00,000T04:15:00,11-Jan-10,VIMS,Prime,rings(general),RDHRCOMP,High resolution radial scan of ring system,"Radial scan, high resolution.","Lit side scan; joint VIMS/ISS; 80/320 msec tau_IR, 7-8 minute dwells, 64x12 frame, hi res mode.",,,,,, 2010-011T07:25:00,000T04:15:00,11-Jan-10,CIRS,SPASS Rider,rings(general),RDHRCOMP,High resolution radial scan of ring system,Rider to VIMS Composition,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-011T07:25:00,000T04:15:00,11-Jan-10,ISS,SPASS Rider,rings(general),RDHRCOMP,High resolution radial scan of ring system,RING RADIAL SCAN I,"VIMS RADIAL SCAN COLOR RIDE ALONG: up to 8 footprints X 4 COLORS on one ansa, high resolution",,,,,, 2010-011T07:57:59,000T22:47:01,11-Jan-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-011T11:40:00,000T02:15:00,11-Jan-10,UVIS,Prime,Star,URALPVIR,Stellar occultation,URSTAR,"This is an egress occultation that begins with the star behind Saturn. Initial setup should be for an atmospheric occultation, then switch to ring occultation mode. HSP should be on and recording at 1 ms integration period by 2010-011T12:00.",,,,,, 2010-011T11:40:00,000T02:15:00,11-Jan-10,CIRS,SPASS Rider,rings(general),URALPVIR,Stellar occultation,Rider to UVIS Star Occ,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-011T13:55:00,000T01:05:00,11-Jan-10,UVIS,Prime,Star,URBETLIB,,URSTAR,,,,,,, 2010-011T13:55:00,000T01:05:00,11-Jan-10,CIRS,SPASS Rider,rings(general),URBETLIB,,Rider to UVIS Star Occ,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-011T15:00:00,000T01:00:00,11-Jan-10,UVIS,Prime,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-011T16:00:00,000T02:15:00,11-Jan-10,VIMS,Prime,rings(general),SHADSCANL,,"Shadow scan, lit side","Scan parallel to shadow on rings, 160 msec tau_IR, 64x12 frames.",,,,,, 2010-011T16:00:00,000T02:15:00,11-Jan-10,CIRS,SPASS Rider,rings(general),SHADSCANL,,Rider to VIMS Shadow Scan,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-011T18:15:00,000T02:59:00,11-Jan-10,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-011T18:15:00,000T02:59:00,11-Jan-10,CIRS,SPASS Rider,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-011T23:14:00,000T09:00:00,11-Jan-10,RSS,SPASS Rider,Saturn,KADOWN,RSS Ka-Band downlink,GSE pass for Saturn's gravity,Additional downlink pass at Ka-band for Saturn's gravity science and for improving locally Cassini orbit.,,,,,, 2010-011T23:14:00,000T09:00:00,11-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-012T00:14:00,000T08:00:00,12-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10012_SP,rider,,,,,, 2010-012T01:56:46,000T06:17:14,12-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-012T06:45:00,000T14:25:36,12-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-012T06:45:00,000T01:29:00,12-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-012T06:45:00,000T01:29:00,12-Jan-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-012T06:46:00,000T01:28:00,12-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-012T08:14:00,000T12:56:36,12-Jan-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-012T08:14:00,000T13:56:36,12-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-012T08:14:00,000T10:56:36,12-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-012T08:14:00,003T00:00:00,12-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-012T09:07:40,000T05:02:56,12-Jan-10,VIMS,Prime,Titan,CLOUDMAP,Cloud map,Cloud mapping,VIMS - CIRS - VIMS sharing. Stare at Titan for cloud mapping. Phase = 135 deg. Lat/Lon = 10N/14 deg. Resolution = 130 km/px.,,,,,, 2010-012T09:07:40,000T05:02:56,12-Jan-10,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride along with VIMS.,,,,,, 2010-012T09:07:40,000T05:02:56,12-Jan-10,ISS,SPASS Rider,Titan,CLOUDMAP,Cloud map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-012T14:10:36,000T04:00:00,12-Jan-10,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-012T14:10:36,000T04:00:00,12-Jan-10,CIRS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-012T14:10:36,000T04:00:00,12-Jan-10,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-012T14:10:36,000T04:00:00,12-Jan-10,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2010-012T14:10:36,000T04:00:00,12-Jan-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan limb mapping.,VIMS ridealong with CIRS for limb mapping. Phase = 136 deg. Lat/Lon = 10N/18 deg. Resolution = 89 km/px. Temp. R. Obtain cubes at 160 and 640 ms for limb mapping.,,,,,, 2010-012T17:55:36,000T05:00:00,12-Jan-10,RADAR,SPASS Rider,Titan,T65WARMUP,,Warmup for T65,,,,,,, 2010-012T18:10:36,000T02:45:00,12-Jan-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-012T18:10:36,000T02:44:00,12-Jan-10,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-012T18:10:36,000T02:45:00,12-Jan-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-012T18:10:36,000T02:45:00,12-Jan-10,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,VIMS ridealong with CIRS for scan across Titan. Phase = 136 deg. Lat/Lon = 09N/22 deg. Resolution = 47 km/px. Temp. T. Obtain cubes while scanning across Titan.,,,,,, 2010-012T19:10:36,000T08:00:00,12-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-012T19:10:36,000T08:00:00,12-Jan-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T65 flyby,"T65 is almost identical to T64, but over Titan's south pole. In nominal upstream conditions, Cassini would explore the south lobe of Titan's magnetic tail, very close to the moon. A close comparison with T64 and T63 will give important results on the structure of Titan's magnetic tail in the dusk sector. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2010-012T20:55:36,000T01:30:00,12-Jan-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-012T20:56:36,000T01:51:00,12-Jan-10,CAPS,Prime,Titan,T65INPTG,,Titan Encounter,null,,,,,, 2010-012T21:10:36,000T01:00:00,12-Jan-10,CAPS,SPASS Rider,Titan,T65INBD,,Titan Encounter,null,,,,,, 2010-012T21:10:36,000T01:00:00,12-Jan-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-012T22:10:36,000T02:00:00,12-Jan-10,CAPS,SPASS Rider,Titan,T65CLOSE,,Titan Encounter,null,,,,,, 2010-012T22:10:36,000T02:00:00,12-Jan-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-012T22:10:36,000T00:45:00,12-Jan-10,INMS,Non-SPASS,Titan,TITAN65,,Titan Flyby,Titan observation,,,,,, 2010-012T22:25:36,000T01:01:00,12-Jan-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-012T22:47:36,000T00:23:00,12-Jan-10,RADAR,Prime,Titan,T65RASAR,,T65 Ride-along SAR with INMS,,,,,,, 2010-012T22:55:36,000T00:15:00,12-Jan-10,INMS,SPASS Rider,Titan,TITAN65,,Titan Flyby,Prime Titan observation,,,,,, 2010-012T23:10:36,000T00:16:00,12-Jan-10,RADAR,Prime,Titan,T65OUTSAR,,T65 Outbound SAR for Ontario Lacus,,,,,,, 2010-012T23:10:36,000T01:00:00,12-Jan-10,INMS,Non-SPASS,Titan,TITAN65,,Titan Flyby,Titan observation,,,,,, 2010-012T23:26:36,000T01:22:55,12-Jan-10,CAPS,Prime,Titan,T65OUTPTG,,Titan Encounter,null,,,,,, 2010-012T23:26:36,000T01:44:00,12-Jan-10,CIRS,SPASS Rider,Titan,T65OUTPTG,,,Ride along with ISS.,,,,,, 2010-012T23:26:36,000T00:29:00,12-Jan-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-012T23:55:36,000T01:30:00,12-Jan-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-013T00:10:36,000T01:00:00,13-Jan-10,CAPS,SPASS Rider,Titan,T65OUTBND,,Titan Encounter,null,,,,,, 2010-013T00:10:36,000T01:00:00,13-Jan-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-013T00:10:36,002T08:03:23,13-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-013T00:46:36,000T00:24:00,13-Jan-10,CAPS,SPASS Rider,Titan,T65OUTPTG,,Titan Encounter,null,,,,,, 2010-013T00:46:36,000T00:24:00,13-Jan-10,VIMS,SPASS Rider,Titan,TRANS,,Stare at Titan,VIMS ridealong during RCS/RWA transition. Phase = 44 deg. Lat/Lon = 03S/220 deg. Resolution = 159 km/px. Obtain cubes during RCS/RWA transition.,,,,,, 2010-013T01:10:36,000T03:00:00,13-Jan-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-013T01:10:36,000T06:19:23,13-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-013T01:10:36,000T03:00:00,13-Jan-10,CIRS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-013T01:10:36,000T03:00:00,13-Jan-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-013T01:10:36,000T16:19:23,13-Jan-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-013T01:10:36,000T03:00:00,13-Jan-10,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,VIMS ridealong with CIRS for slow scan across Titan. Phase = 43 deg. Lat/Lon = 07S/209 deg. Resolution = 24 km/px. Temp. E. Obtain cubes while scanning across Titan.,,,,,, 2010-013T03:10:36,000T14:19:23,13-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-013T04:10:36,000T04:00:00,13-Jan-10,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-013T04:10:36,000T04:00:00,13-Jan-10,CIRS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-013T04:10:36,000T04:00:00,13-Jan-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan limb mapping.,VIMS ridealong with CIRS for limb mapping. Phase = 43 deg. Lat/Lon = 05S/211 deg. Resolution = 49 km/px. Temp. F. Obtain cubes at 160 and 640 ms for limb mapping.,,,,,, 2010-013T07:30:00,000T10:00:00,13-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-013T08:10:36,000T05:00:00,13-Jan-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-013T08:10:36,000T05:00:00,13-Jan-10,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-013T08:10:36,000T05:00:00,13-Jan-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-013T08:10:36,000T05:00:00,13-Jan-10,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2010-013T08:10:36,000T05:00:00,13-Jan-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,VIMS ridealong with CIRS while staring at Titan. Phase = 44 deg. Lat/Lon = 04S/214 deg. Resolution = 89 km/px. Temp. C. Obtain various cubes while staring at Titan.,,,,,, 2010-013T13:10:36,000T05:21:00,13-Jan-10,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2010-013T13:10:36,000T05:21:00,13-Jan-10,CIRS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-013T13:10:36,000T05:21:00,13-Jan-10,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-013T13:10:36,000T09:00:00,13-Jan-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan scan.,VIMS ridealong with CIRS for scan across Titan. Phase = 44 deg. Lat/Lon = 04S/219 deg. Resolution = 139 km/px. Temp. A(Z). Obtain cubes while scanning across Titan.,,,,,, 2010-013T17:29:59,001T14:44:01,13-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-013T17:30:00,001T14:44:00,13-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-013T17:30:00,001T14:44:00,13-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-013T18:31:36,000T03:39:00,13-Jan-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-013T18:31:36,000T03:39:00,13-Jan-10,ISS,SPASS Rider,Titan,COMPMAP,Composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-013T23:14:00,000T09:00:00,13-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-014T00:14:00,000T08:00:00,14-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10014_SP,rider,,,,,, 2010-014T08:54:00,000T05:06:00,14-Jan-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-014T08:54:00,000T05:06:00,14-Jan-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan for cloud mapping.,Caboose segment. VIMS ridealong with ISS for cloud mapping. Phase = 46 deg. Lat/Lon = 03S/234 deg. Resolution = 342 km/px. Obtain cubes for cloud mapping.,,,,,, 2010-014T14:00:00,000T02:00:00,14-Jan-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-014T14:00:00,000T02:00:00,14-Jan-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan for cloud mapping.,Caboose segment. VIMS ridealong with CAPS for cloud mapping. Phase = 47 deg. Lat/Lon = 03S/238 deg. Resolution = 396 km/px. Obtain cubes for cloud mapping.,,,,,, 2010-014T16:00:00,000T06:34:00,14-Jan-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-014T16:00:00,000T06:34:00,14-Jan-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan for cloud mapping.,Caboose segment. VIMS ridealong with ISS for cloud mapping. Phase = 48 deg. Lat/Lon = 03S/240 deg. Resolution = 418 km/px. Obtain cubes for cloud mapping.,,,,,, 2010-014T23:14:00,000T09:00:00,14-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-015T00:14:00,000T08:00:00,15-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10015_SP,rider,,,,,, 2010-015T08:14:00,001T02:31:00,15-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-015T08:14:00,001T02:31:00,15-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-015T08:14:00,000T23:45:00,15-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-015T08:14:00,001T02:31:00,15-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-015T08:14:00,003T20:03:00,15-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-015T08:14:00,001T02:31:00,15-Jan-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-015T08:54:00,000T01:15:00,15-Jan-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 51.2 range 1.2 Mkm",,,,,, 2010-015T08:54:00,000T01:15:00,15-Jan-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-015T08:54:00,000T01:15:00,15-Jan-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-015T10:09:00,000T11:00:00,15-Jan-10,UVIS,Prime,Saturn,MOS124APO,,,"Mosaic scan of Saturn magnetosphere, day 1. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 129.0 s, stop data capture. Repeat PATTERN 189 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 129.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9386.113 bps, from Alain's spreadsheet)x(129.0s per stare)x(190 stares) = 230.054x10^6 bits",,,,,, 2010-015T21:09:00,000T01:10:00,15-Jan-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-015T22:59:00,000T09:00:00,15-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-015T23:59:00,000T08:00:00,15-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10415_SP,rider,,,,,, 2010-016T00:00:00,000T00:34:00,16-Jan-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-016T07:59:00,001T00:01:00,16-Jan-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-016T08:39:00,000T01:15:00,16-Jan-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 57.3 range 1.7 Mkm",,,,,, 2010-016T08:39:00,000T01:15:00,16-Jan-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-016T08:39:00,000T01:15:00,16-Jan-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-016T09:54:00,000T01:05:00,16-Jan-10,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Janus","Images of mutual event, transit of Epimetheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-016T10:45:00,001T08:55:00,16-Jan-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-016T10:45:00,002T17:32:00,16-Jan-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-016T10:45:00,005T11:00:00,16-Jan-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-016T10:45:00,002T17:32:00,16-Jan-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-016T10:59:00,000T11:21:00,16-Jan-10,UVIS,Prime,Saturn,MOS124APO,,,"Mosaic scan of Saturn magnetosphere, day 2. One 11.0 hr 21 min block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 135.0 s, stop data capture. Repeat PATTERN 189 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 135.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (8968.952 bps, from Alain's spreadsheet)x(135.0s per stare)x(190 stares) = 230.054x10^6 bits",,,,,, 2010-016T23:00:00,000T09:00:00,16-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-017T00:00:00,000T08:00:00,17-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10017_SP,rider,,,,,, 2010-017T08:00:00,001T11:00:00,17-Jan-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-017T08:40:00,000T11:00:00,17-Jan-10,UVIS,Prime,Saturn,MOS124APO,,,"Mosaic scan of Saturn magnetosphere, day 3. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 129.0 s, stop data capture. Repeat PATTERN 189 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 129.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9386.113 bps, from Alain's spreadsheet)x(129.0s per stare)x(190 stares) = 230.054x10^6 bits",,,,,, 2010-017T19:40:00,000T02:40:00,17-Jan-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-017T22:20:00,002T00:25:00,17-Jan-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-017T23:00:00,000T09:00:00,17-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-018T00:00:00,000T08:00:00,18-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10018_SP,rider,,,,,, 2010-018T08:40:00,000T04:55:00,18-Jan-10,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_124_SCATTERED_SUNLIGHT_TEST_PRIME,"Sunlight falling on the CIRS telescope can potentially be scattered into the instrument by mirror imperfections. We need to quantify the effect of ring particle impacts on the mirror performance. This requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; continuous radial scans are required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scans will begin 40 degrees from FPB, and will scan to 10 degrees of FPB at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time VIMS will integrate for TBD seconds and CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction back to the initial position; to determine whether scattering is asymmetric with respect to the FPB axis, 3 such scans will be made. 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from 40 degrees +Z to 10 degrees +Z and back to 40 degrees +Z. 2) From 40 degrees in -X on the X axis, to 10 degrees on the -X axis, to 40 degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 10 degrees -Z and back to 40 degrees -Z.",,,,,, 2010-018T10:35:00,000T03:00:00,18-Jan-10,RADAR,SPASS Rider,Other,WU4SRCCAL,,Warm Up for Microwave Source Calibration,Warmup for calibration and science data collection.,,,,,, 2010-018T13:35:00,000T08:30:00,18-Jan-10,RADAR,Prime,Other,SRCRADCAL,RADAR microwave source radiometric calibration,Radiometric Microwave Sources Calibration,"Scan the Sun, Saturn, and microwave sources while collecting radiometry data.",,,,,, 2010-018T19:00:00,000T04:00:00,18-Jan-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-018T22:45:00,000T09:00:00,18-Jan-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev125 Saturn rings and atmospheric occultation on 2010/026.",,,,,, 2010-018T22:45:00,000T09:00:00,18-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-018T23:00:00,000T05:17:00,18-Jan-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-018T23:45:00,000T08:00:00,18-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_124IC_DSCAL10418_SP,rider,,,,,, 2010-019T04:17:00,002T17:28:00,19-Jan-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-019T04:17:00,004T10:43:00,19-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S57,Range enter= 3.0103116 Rs exit= 7.5951306 Range altitude= 40241.954 km ... -40068.160,,,,,, 2010-019T04:17:00,002T03:28:00,19-Jan-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-019T04:17:00,004T10:43:00,19-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-019T04:17:00,002T17:28:00,19-Jan-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-019T04:17:00,000T03:28:00,19-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-019T04:17:35,000T00:00:01,19-Jan-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 5.2 deg, r = 37.978 Rs, phase = 103 deg",,,,,, 2010-019T08:25:00,000T05:40:00,19-Jan-10,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observation of 1 of 3 IR stars: CW Leonis, Eta Carinae, Alpha Orionis. Slew to star; settle; execute small box scan; return to waypoint. Observation of each star to take 6 hours; need not be executed contiguously.",,,,,, 2010-019T14:05:00,000T08:00:00,19-Jan-10,UVIS,Prime,Saturn,MOS124APO,,,"Mosaic scan of Saturn magnetosphere, day 4. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN 105 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (7913.781 bps, from Alain's spreadsheet)x(153.0s per stare)x(106 stares) = 128.346x10^6 bits",,,,,, 2010-019T22:45:00,001T21:00:00,19-Jan-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-019T22:45:00,000T09:00:00,19-Jan-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev125 Saturn rings and atmospheric occultation on 2010/026.",,,,,, 2010-019T22:45:00,000T09:00:00,19-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-019T23:45:00,000T08:00:00,19-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10019_SP,rider,,,,,, 2010-020T08:25:00,000T01:15:00,20-Jan-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 88.8 range 3.2 Mkm",,,,,, 2010-020T08:25:00,000T01:15:00,20-Jan-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-020T08:25:00,000T01:15:00,20-Jan-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-020T09:40:00,000T11:00:00,20-Jan-10,UVIS,Prime,Saturn,MOS124APO,,,"Mosaic scan of Saturn magnetosphere, day 5. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 142.0 s, stop data capture. Repeat PATTERN 176 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 142.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (8526.821 bps, from Alain's spreadsheet)x(142.0s per stare)x(177 stares) = 214.313x10^6 bits",,,,,, 2010-020T20:40:00,000T01:25:00,20-Jan-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-020T22:45:00,000T09:00:00,20-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-020T23:45:00,000T08:00:00,20-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10020_SP,rider,,,,,, 2010-021T07:45:00,001T00:00:00,21-Jan-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-021T08:25:00,000T11:00:00,21-Jan-10,UVIS,Prime,Saturn,MOS124APO,,,"Mosaic scan of Saturn magnetosphere, day 6. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 142.0 s, stop data capture. Repeat PATTERN 176 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 142.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (8526.821 bps, from Alain's spreadsheet)x(142.0s per stare)x(177 stares) = 214.313x10^6 bits",,,,,, 2010-021T09:00:00,000T06:00:00,21-Jan-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-021T19:25:00,000T02:40:00,21-Jan-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-021T21:45:00,001T17:15:00,21-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-021T21:45:00,001T17:15:00,21-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-021T21:45:00,001T17:15:00,21-Jan-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-021T22:05:00,001T16:55:00,21-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-021T22:45:00,000T09:00:00,21-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-021T23:45:00,000T08:00:00,21-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10021_SP,rider,,,,,, 2010-022T07:45:00,001T07:15:00,22-Jan-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-022T08:25:00,000T20:55:00,22-Jan-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_125SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-023T05:20:00,000T09:40:00,23-Jan-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-023T06:00:00,000T09:00:00,23-Jan-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev125 Saturn rings and atmospheric occultation on 2010/026.",,,,,, 2010-023T06:00:00,000T09:00:00,23-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-023T07:00:00,000T08:00:00,23-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10023_SP,rider,,,,,, 2010-023T15:00:00,001T00:05:00,23-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-023T15:00:00,001T00:05:00,23-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-023T15:00:00,003T03:11:11,23-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S57,Range enter= 3.0103116 Rs exit= 7.5951306 Range altitude= 40241.954 km ... -40068.160,,,,,, 2010-023T15:00:00,000T00:43:00,23-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-023T15:00:00,000T00:46:00,23-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-023T15:00:00,002T10:37:00,23-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-023T15:00:00,001T00:05:00,23-Jan-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-023T15:05:00,000T00:02:00,23-Jan-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S57 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-023T15:43:00,000T00:07:00,23-Jan-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-023T15:46:00,000T06:45:00,23-Jan-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-023T15:46:00,000T06:45:00,23-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-023T15:50:00,000T00:05:00,23-Jan-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-023T15:55:00,000T00:33:00,23-Jan-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-023T16:28:00,000T00:22:59,23-Jan-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-023T16:50:59,001T14:09:01,23-Jan-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-023T22:31:00,000T02:00:00,23-Jan-10,ISS,Prime,rings(general),PHOTDARK,,"low-latitude, dark-face ring photometry","low latitude unlit #2: B = -3.6 phase ~ 120, B' = 2.5",,,,,, 2010-023T22:31:00,000T02:00:00,23-Jan-10,CIRS,SPASS Rider,rings(general),PHOTDARK,,Rider to ISS Photometry,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-023T22:31:00,000T02:00:00,23-Jan-10,VIMS,SPASS Rider,rings(general),PHOTDARK,,WAC mosaic?,"320 ms, 16*16 cubes?",,,,,, 2010-023T22:31:00,000T16:34:00,23-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-024T00:31:00,000T11:20:00,24-Jan-10,VIMS,Prime,rings(general),EG105PHAS,,E/G Ring phase observation,E-G phase observation.,,,,,, 2010-024T00:31:00,000T11:20:00,24-Jan-10,CIRS,SPASS Rider,rings(general),EG105PHAS,,Rider to VIMS E-G Phase,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-024T00:31:00,000T11:20:00,24-Jan-10,ISS,SPASS Rider,rings(general),EG105PHAS,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2010-024T12:31:00,000T09:00:00,24-Jan-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev125 Saturn rings and atmospheric occultation on 2010/026.",,,,,, 2010-024T12:31:00,000T09:00:00,24-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-024T13:31:00,000T08:00:00,24-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10024_SP,rider,,,,,, 2010-024T15:05:00,001T00:05:00,24-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-024T15:05:00,001T00:05:00,24-Jan-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-024T15:05:00,001T00:05:00,24-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-024T15:05:00,001T00:05:00,24-Jan-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-024T22:11:00,000T09:00:00,24-Jan-10,CIRS,Prime,rings(general),POLARIZ,,CIRS_125RI_POLARIZ023_PRIME;,null,,,,,, 2010-024T22:11:00,000T09:00:00,24-Jan-10,CIRS,SPASS Rider,rings(general),POLARIZ,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-025T07:00:00,000T01:37:00,25-Jan-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-025T07:11:00,000T03:50:00,25-Jan-10,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2010-025T07:11:00,000T03:50:00,25-Jan-10,CIRS,SPASS Rider,rings(general),DUSKPTG,,Rider to CAPS for Dark Sky after CIRS Prime,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-025T08:37:00,000T00:34:00,25-Jan-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2010-025T09:11:00,000T12:05:00,25-Jan-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-025T12:16:00,000T09:45:00,25-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-025T13:16:00,000T08:45:00,25-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10025_SP,rider,,,,,, 2010-025T15:10:00,002T07:06:00,25-Jan-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-025T15:10:00,001T08:37:59,25-Jan-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-025T15:10:00,002T16:06:00,25-Jan-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-025T21:16:00,000T10:15:00,25-Jan-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-025T22:01:00,000T09:30:00,25-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-025T23:01:00,000T08:30:00,25-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10425_SP,rider,,,,,, 2010-026T01:37:00,000T15:53:00,26-Jan-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-026T07:31:00,001T08:29:00,26-Jan-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-026T08:00:00,000T03:00:00,26-Jan-10,ISS,Prime,Enceladus,PLMMRHP,,Medium res plume obs at high phase,Medium resolution plume observation at high phase,,,,,, 2010-026T08:00:00,000T03:00:00,26-Jan-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-026T08:00:00,000T03:00:00,26-Jan-10,VIMS,SPASS Rider,Enceladus,PLMMRHP,,"Enceladus Plume, high phase",null,,,,,, 2010-026T11:00:00,000T03:23:00,26-Jan-10,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2010-026T12:38:30,000T02:05:00,26-Jan-10,RSS,SPASS Rider,Enceladus,THERMAL,Thermal stabilization period,RSS 125RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2010-026T14:43:02,000T01:00:00,26-Jan-10,RSS,Prime,Enceladus,OCC,Occultation,Enceladus Plume Occultation,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2010-026T15:43:02,000T01:47:00,26-Jan-10,RSS,Prime,rings(general),THERMAL,Thermal stabilization period,RSS 125RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2010-026T17:30:00,000T22:00:00,26-Jan-10,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2010-026T17:30:02,000T02:22:00,26-Jan-10,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ansa-to-Ansa Ring Occ - Ingress,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2010-026T18:11:11,000T05:18:00,26-Jan-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 7.5770868 Rs exit= 4.5479562 Range altitude= -39966.457 km ... -20065.481,,,,,, 2010-026T19:52:02,000T00:47:00,26-Jan-10,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS Atmospheric Occultation on rev 125 ingress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-026T20:39:02,000T02:24:00,26-Jan-10,VIMS,Prime,rings(general),HIPHASE,High phase observation,High phase observation,Target D ring on right ansa; tau_IR=320 msec.,,,,,, 2010-026T20:39:02,000T02:24:00,26-Jan-10,CIRS,SPASS Rider,rings(general),HIPHASE,High phase observation,Rider to VIMS High Phase,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-026T20:39:02,000T02:24:00,26-Jan-10,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 125RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2010-026T23:03:02,000T00:39:00,26-Jan-10,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Atmospheric Occultation on rev 125 egress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-026T23:29:11,000T08:09:36,26-Jan-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 4.5281554 Rs exit= 3.8918090 Range altitude= -19907.143 km ... 19966.463,,,,,, 2010-026T23:42:02,000T02:31:00,26-Jan-10,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ansa-to-Ansa Ring Occ - Egress,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2010-026T23:47:59,000T08:37:00,26-Jan-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-027T02:01:00,000T02:00:00,27-Jan-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-027T02:01:11,000T02:00:00,27-Jan-10,CDA,SPASS Rider,DustRAM direction,RPX0020,,CDA RPXing 2010-027T03:01:11,RPXing at 2.7518148 Rs,,,,,, 2010-027T02:49:13,000T00:17:47,27-Jan-10,ISS,SPASS Rider,DustRAM direction,DUSTHAZRD,,Close imaging of G-ring arc during hazard period,Imaging of the G ring arc during Dust Hazard Period,,,,,, 2010-027T03:07:00,000T03:13:00,27-Jan-10,ISS,Prime,RingG,GARCPROM,,G Ring Arc/Prometheus Flyby,Extremely close flyby of the G ring arc and Prometheus,,,,,, 2010-027T03:07:00,000T03:13:00,27-Jan-10,CIRS,SPASS Rider,rings(general),GARCPROM,,Rider to ISS G Ring,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-027T03:07:00,000T03:13:00,27-Jan-10,UVIS,SPASS Rider,rings(general),GARCPROM,,Faint Ring Rider,,,,,,, 2010-027T03:07:00,000T03:13:00,27-Jan-10,VIMS,SPASS Rider,Prometheus,GARCPROM,,Prometheus,"Combined G ring arc & Prometheus obs., multiple 16/640 ms.",,,,,, 2010-027T04:06:29,000T00:00:01,27-Jan-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.572 Rs, lat = 3 deg, phase = 77 deg",,,,,, 2010-027T07:00:00,000T02:00:00,27-Jan-10,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-027T07:00:00,000T02:00:00,27-Jan-10,CIRS,SPASS Rider,rings(general),EQLBN,,CIRS_125RI_EQLBN001 SI,"4 frames, timing TBD.",,,,,, 2010-027T07:00:00,000T02:00:00,27-Jan-10,UVIS,SPASS Rider,rings(general),EQLBN,,URSTAR,,,,,,, 2010-027T07:00:00,000T02:00:00,27-Jan-10,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, lit side","160 ms, 64*12 cubes?",,,,,, 2010-027T07:38:47,000T13:07:13,27-Jan-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9109206 Rs exit= 15.998260 Range altitude= 20027.452 km ... 9825.9584,,,,,, 2010-027T08:24:59,000T01:22:14,27-Jan-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-027T09:00:00,000T02:00:00,27-Jan-10,VIMS,Prime,rings(general),LOWPHASE,Low phase imaging,Low phase observation,Target rings approx 3 deg south of zero-phase point & scan across right ansa from limb to F ring.,,,,,, 2010-027T09:00:00,000T02:00:00,27-Jan-10,CIRS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,Rider to VIMS Low Phase,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-027T09:00:00,000T02:00:00,27-Jan-10,ISS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,WAC radial scan in color filters riding on VIMS,"6 filter, 6 deg phase, lit face; 5 RS!",,,,,, 2010-027T09:00:00,000T02:00:00,27-Jan-10,UVIS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,URSTAR,,,,,,, 2010-027T09:47:13,000T04:00:00,27-Jan-10,MAG,Non-SPASS,Dione,DITAR,Dione targeted flyby,D4 flyby,Monitor magnetic field perturbations and waves to confirm evidence of plasma pickup observed during the sole previous upstream Dione flyby.,,,,,, 2010-027T11:00:00,000T01:30:00,27-Jan-10,CIRS,Prime,Dione,FP1DRKMAP,CIRS FP1 dark side map,CIRS_125DI_FP1DRKMAP001_PRIME;,"FP1 and FP3 only. FP1 raster scan. Include a 15 minute ISS mosaic of the illuminated crescent at the end. 23.8 mrad, 120 degrees (30, 74) LT~20 at T11:25. iDigit turn estimates about Z: to: 15+2=17; fro: 13+2=15 min; about X: to: 35+2=37; fro: 21+2=23 min. NEG_Z to NSP or NEG_X to NSP for secondary. SOST LIEN. DESIGN (preliminary): Turn to DI (20 min); fast FP1 map using 25 mrad N-S scans, starting just inside dark limb and working to just inside bright limb (~40 min?); 7-scan FP3 map of lit hemisphere at 16 urad/sec (70 min); return to waypoint (18 min). Stop and dwell 2 min upon arrival, in middle, just before departure for WAC SIs. (Don't have tables for map durations, so times are off).",,,,,, 2010-027T11:00:00,000T01:30:00,27-Jan-10,CIRS,SPASS Rider,Dione,FP1DRKMAP,CIRS FP1 dark side map,125DI_FP1DRKMAP Support Images,3 WAC Support images,,,,,, 2010-027T11:00:00,000T01:30:00,27-Jan-10,ISS,SPASS Rider,Dione,FP1DRKMAP,CIRS FP1 dark side map,Dione mapping,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-027T11:00:00,000T01:30:00,27-Jan-10,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione dark side map,VIMS ridealong with CIRS for Dione mosaic,,,,,, 2010-027T12:30:00,000T01:50:00,27-Jan-10,VIMS,Prime,rings(general),LOWPHASE,Low phase imaging,Low phase observation,Target rings at zero-phase point & scan across right ansa of E ring.,,,,,, 2010-027T12:30:00,000T01:50:00,27-Jan-10,CIRS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,Rider to VIMS Low Phase,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-027T12:30:00,000T01:50:00,27-Jan-10,ISS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,WAC rider on E-ring Low-Phase observations,Low-Phase observation of E ring,,,,,, 2010-027T12:30:00,000T01:50:00,27-Jan-10,UVIS,SPASS Rider,rings(general),LOWPHASE,Low phase imaging,URSTAR,,,,,,, 2010-027T13:47:13,000T16:47:47,27-Jan-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-027T14:20:00,000T02:00:00,27-Jan-10,CIRS,Prime,Dione,FP3DAYMAP,CIRS FP3 daytime map,CIRS_125DI_FP3DAYMAP001_PRIME;,"FP1 and FP3 only. Scan at 6 murad/sec for rider-friendliness 1.05*3 Scans*13 mrad*16/8 = 82 min. or 41 min. at 16 urad/sec. 9.10 mrad, 40 degrees, (11, 183) LT~15. iDigit turn estimates about Z: to: 4+2=6; fro: 3+2=5 min; about X: to: 5+2=7; fro: 5+2=7 min. NEG_Z to NSP or NEG_X to NSP for secondary.",,,,,, 2010-027T14:20:00,000T02:00:00,27-Jan-10,CIRS,SPASS Rider,Dione,FP3DAYMAP,CIRS FP3 daytime map,125DI_FP3DAYMAP Support Images,2 WAC Support images,,,,,, 2010-027T14:20:00,000T02:00:00,27-Jan-10,ISS,SPASS Rider,Dione,FP3DAYMAP,CIRS FP3 daytime map,Dione mapping,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-027T14:20:00,000T02:00:00,27-Jan-10,UVIS,SPASS Rider,Dione,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-027T14:20:00,000T02:00:00,27-Jan-10,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione day side map,VIMS ridealong with CIRS for Dione mosaic,,,,,, 2010-027T15:30:00,000T15:06:00,27-Jan-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-027T16:00:00,000T02:00:00,27-Jan-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-027T16:20:00,000T02:26:00,27-Jan-10,CDA,Prime,rings(general),ERINGSCAN,,CDA ERINGSCAN,Scan,,,,,, 2010-027T18:00:00,000T13:16:00,27-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-027T18:46:00,000T02:00:00,27-Jan-10,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"low-latitude, lit-face ring photometry","low latitude lit #2: B = 2, phase ~ 50, B' = 2.6",,,,,, 2010-027T18:46:00,000T02:00:00,27-Jan-10,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,Rider to ISS Photometry,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-027T18:46:00,000T02:00:00,27-Jan-10,VIMS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,WAC mosaic?,"160 ms, 32*32 cubes?",,,,,, 2010-027T20:46:00,000T01:30:00,27-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 3.9109206 Rs exit= 15.998260 Range altitude= 20027.452 km ... 9825.9584,,,,,, 2010-027T22:16:00,000T09:00:00,27-Jan-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-027T22:16:00,000T09:00:00,27-Jan-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9109206 Rs exit= 15.998260 Range altitude= 20027.452 km ... 9825.9584,,,,,, 2010-027T22:16:00,000T09:00:00,27-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-027T23:16:00,000T06:00:00,27-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10027_SP,rider,,,,,, 2010-028T06:35:00,000T00:41:00,28-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-028T06:36:00,000T00:40:00,28-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-028T07:16:00,000T06:12:49,28-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-028T07:16:00,000T13:12:49,28-Jan-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-028T07:16:00,000T02:04:46,28-Jan-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9109206 Rs exit= 15.998260 Range altitude= 20027.452 km ... 9825.9584,,,,,, 2010-028T07:16:00,000T14:12:49,28-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-028T07:16:00,000T11:12:49,28-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-028T07:16:00,000T13:42:49,28-Jan-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-028T08:07:18,000T04:21:31,28-Jan-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-028T08:07:18,000T04:21:31,28-Jan-10,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (4 integrations total = 8 frames, 0.5 Mb/frame)",,,,,, 2010-028T08:07:18,000T04:21:31,28-Jan-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T08:07:18,000T01:21:31,28-Jan-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan scan.,VIMS ridealong with CIRS for scan across Titan. Phase = 135 deg. Lat/Lon = 01N/010 deg. Resolution = 144 km/px. Obtain cubes while scanning across Titan. Temp. M4.,,,,,, 2010-028T09:20:46,001T12:55:14,28-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.010173 Rs exit= 16.001148 Range altitude= 9797.1698 km ... 3588.9685,,,,,, 2010-028T09:28:49,000T03:00:00,28-Jan-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Titan cloud monitoring,VIMS ridealong with CIRS for Titan cloud monitoring. Phase = 135 deg. Lat/Lon = 01N/012 deg. Resolution = 130 km/px. Obtain cubes of 160 and 640 ms. for cloud monitoring. Temp. N.,,,,,, 2010-028T12:28:49,000T01:00:00,28-Jan-10,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T12:28:49,000T01:00:00,28-Jan-10,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS.,,,,,, 2010-028T12:28:49,000T01:00:00,28-Jan-10,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Titan cloud monitoring,VIMS ridealong with ISS for Titan cloud monitoring. Phase = 135 deg. Lat/Lon = 01N/014 deg. Resolution = 100 km/px. Obtain cubes for cloud monitoring and global mapping. Temp. N.,,,,,, 2010-028T13:28:49,000T06:30:00,28-Jan-10,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2010-028T13:28:49,000T06:30:00,28-Jan-10,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2010-028T13:28:49,000T06:30:00,28-Jan-10,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T13:28:49,000T04:10:00,28-Jan-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,VIMS ridealong with UVIS for slow scan across Titan. Phase = 135 deg. Lat/Lon = 00N/015 deg. Resolution = 89 km/px. Obtain cubes while scanning across Titan. Temp. X.,,,,,, 2010-028T13:28:49,000T07:00:00,28-Jan-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-028T17:38:49,000T02:20:00,28-Jan-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,VIMS ridealong with UVIS for slow scan across Titan. Phase = 133 deg. Lat/Lon = 02S/018 deg. Resolution = 47 km/px. Obtain cubes while scanning across Titan. Temp. X.,,,,,, 2010-028T18:28:49,000T08:00:00,28-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-028T18:28:49,000T08:00:00,28-Jan-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T66 flyby,"First of the two so called 'blind flybys' since MAG is unlikely to detect Titan's induced magnetosphere. Occurring in the same SLT sector as T63 T64 and T65, it will be used to characterize Saturn's background magnetic field variation with SKR longitude at a fixed SLT. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2010-028T19:58:49,000T01:08:00,28-Jan-10,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2010-028T19:58:49,000T01:08:00,28-Jan-10,CIRS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2010-028T19:58:49,000T01:08:00,28-Jan-10,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T19:58:49,000T01:08:00,28-Jan-10,UVIS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2010-028T19:58:49,000T01:08:00,28-Jan-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping,VIMS ridealong with CIRS for regional mapping Titan. Phase = 129 deg. Lat/Lon = 07S/018 deg. Resolution = 22 km/px. Obtain cubes while scanning across Titan. Possible mosaic?,,,,,, 2010-028T20:28:49,000T01:00:00,28-Jan-10,CAPS,SPASS Rider,Titan,T66INBD,,Titan Encounter,null,,,,,, 2010-028T20:28:49,000T01:00:00,28-Jan-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-028T20:58:49,000T00:30:00,28-Jan-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-028T21:06:49,000T00:33:30,28-Jan-10,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols. This observation includes a VIMS atmosphere occultation of alpTau (RA/Dec: 68.980/16.509) from 2010-028T21:32:00 to 21:36:00.,,,,,, 2010-028T21:06:49,000T00:33:30,28-Jan-10,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2010-028T21:06:49,000T00:33:30,28-Jan-10,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T21:06:49,000T00:33:30,28-Jan-10,UVIS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,Rider to CIRS,Rider to CIRS.,,,,,, 2010-028T21:06:49,000T00:33:30,28-Jan-10,VIMS,SPASS Rider,Titan,ALPTAUOCC,Alpha Tau occultation,Titan Alpha Tau occ,Stellar occultation of Alpha Tau. Rider on CIRS_125TI_FIRLMBAER001.,,,,,, 2010-028T21:28:49,000T02:00:00,28-Jan-10,CAPS,SPASS Rider,Titan,T66CLOSE,,Titan Encounter,null,,,,,, 2010-028T21:28:49,000T02:00:00,28-Jan-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-028T21:28:49,000T00:40:00,28-Jan-10,INMS,Non-SPASS,Titan,TITAN66,,Titan Flyby,Titan observation,,,,,, 2010-028T21:28:49,000T02:00:00,28-Jan-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-028T21:40:19,000T00:33:30,28-Jan-10,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2010-028T21:40:19,000T00:33:30,28-Jan-10,CIRS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2010-028T21:40:19,000T00:33:30,28-Jan-10,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T21:40:19,000T00:33:30,28-Jan-10,UVIS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,Rider to CIRS,Rider to CIRS.,,,,,, 2010-028T21:40:19,000T00:33:30,28-Jan-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping,VIMS ridealong with CIRS for regional mapping Titan. Phase = 129 deg. Lat/Lon = 07S/018 deg. Resolution = 22 km/px. Obtain cubes while scanning across Titan. Possible mosaic?,,,,,, 2010-028T22:08:49,000T00:40:00,28-Jan-10,INMS,Non-SPASS,Titan,TITAN66,,Titan Flyby,Titan observation,,,,,, 2010-028T22:13:49,000T02:15:00,28-Jan-10,ISS,Prime,Titan,VHIGHRES,,VHI (Very High-Resolution Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-028T22:13:49,000T02:15:00,28-Jan-10,CIRS,SPASS Rider,Titan,VHIGHRES,,,Ride along with ISS.,,,,,, 2010-028T22:13:49,000T02:15:00,28-Jan-10,UVIS,SPASS Rider,Titan,HIGHRES,High resolution observartion,Rider ro ISS,Mosaic Titan,,,,,, 2010-028T22:13:49,000T02:15:00,28-Jan-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping,"VIMS ridealong with ISS for regional mapping of Titan during C/A. At C/A, phase = 96 deg. Lat/Lon = 53S/297 deg. Resolution = 3.7 km/px. Obtain hi-res mosaics of Titan.",,,,,, 2010-028T22:48:49,000T00:40:00,28-Jan-10,INMS,Non-SPASS,Titan,TITAN66,,Titan Flyby,Titan observation,,,,,, 2010-028T23:28:49,000T01:00:00,28-Jan-10,CAPS,SPASS Rider,Titan,T66OUTBND,,Titan Encounter,null,,,,,, 2010-028T23:28:49,000T01:00:00,28-Jan-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-028T23:28:49,002T07:32:10,28-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-028T23:28:49,000T00:30:00,28-Jan-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-028T23:58:49,002T07:02:11,28-Jan-10,RPWS,Non-SPASS,Sun,OUTSURVEY,Outer magnetospheric survey,Outsurvey,Outsurvey,,,,,, 2010-029T00:28:49,000T07:00:00,29-Jan-10,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2010-029T00:28:49,000T07:00:00,29-Jan-10,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2010-029T00:28:49,000T07:00:00,29-Jan-10,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-029T00:28:49,000T15:56:11,29-Jan-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-029T00:28:49,000T07:00:00,29-Jan-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,VIMS ridealong with UVIS for slow scan across Titan. Phase = 40 deg. Lat/Lon = 10S/213 deg. Resolution = 24 km/px. Obtain cubes while scanning across Titan. Temp. X.,,,,,, 2010-029T00:28:49,000T07:00:00,29-Jan-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-029T01:28:49,000T00:30:00,29-Jan-10,ISS,SPASS Rider,Titan,LMBMAP,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-029T02:28:49,000T13:56:11,29-Jan-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-029T07:28:49,000T05:00:00,29-Jan-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-029T07:28:49,000T08:56:10,29-Jan-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-029T07:28:49,000T05:00:00,29-Jan-10,CIRS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (5 integrations total = 10 frames, 0.5 Mb/frame)",,,,,, 2010-029T07:28:49,000T05:00:00,29-Jan-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-029T07:28:49,000T05:00:00,29-Jan-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Titan cloud monitoring,VIMS ridealong with CIRS for Titan cloud monitoring. Phase = 44 deg. Lat/Lon = 03S/214 deg. Resolution = 89 km/px. Obtain cubes of 160 and 640 ms. for cloud monitoring. Temp. C.,,,,,, 2010-029T12:28:49,000T09:00:00,29-Jan-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping,Global mapping of Titan. Phase = 45 deg. Lat/Lon = 02S/218 deg. Resolution = 140 km/px. Obtain cubes of 160 and 640 ms for global mapping.,,,,,, 2010-029T12:28:49,000T09:00:00,29-Jan-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-029T12:28:49,000T09:00:00,29-Jan-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-029T16:25:00,000T14:51:00,29-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-029T16:25:00,000T05:51:00,29-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-029T16:25:00,001T14:36:00,29-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-029T22:16:00,000T09:00:00,29-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-029T22:16:00,006T00:02:00,29-Jan-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.010173 Rs exit= 16.001148 Range altitude= 9797.1698 km ... 3588.9685,,,,,, 2010-029T22:16:00,000T09:00:00,29-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-029T23:16:00,000T08:00:00,29-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10029_SP,rider,,,,,, 2010-030T00:00:00,000T00:34:00,30-Jan-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-030T04:32:00,000T17:29:00,30-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-030T07:16:00,000T23:45:00,30-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-030T07:16:00,000T23:45:00,30-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-030T07:56:00,000T04:04:00,30-Jan-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-030T07:56:00,000T04:04:00,30-Jan-10,CIRS,SPASS Rider,Titan,CLOUD,,Titan Composition,Titan composition,,,,,, 2010-030T07:56:00,000T04:04:00,30-Jan-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan for cloud mapping.,Caboose segment. VIMS ridealong with ISS for cloud mapping. Phase = 48 deg. Lat/Lon = 01S/233 deg. Resolution = 342 km/px. Obtain cubes for cloud mapping.,,,,,, 2010-030T12:00:00,000T02:00:00,30-Jan-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-030T12:00:00,000T02:00:00,30-Jan-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan for cloud mapping.,Caboose segment. VIMS ridealong with CAPS for cloud mapping. Phase = 48 deg. Lat/Lon = 01S/236 deg. Resolution = 385 km/px. Obtain cubes for cloud mapping.,,,,,, 2010-030T14:00:00,000T07:26:00,30-Jan-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-030T14:00:00,000T07:21:00,30-Jan-10,CIRS,SPASS Rider,Titan,CLOUD,,Titan Composition,Titan composition,,,,,, 2010-030T14:00:00,000T07:21:00,30-Jan-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan for cloud mapping.,Caboose segment. VIMS ridealong with ISS for cloud mapping. Phase = 49 deg. Lat/Lon = 01S/237 deg. Resolution = 407 km/px. Obtain cubes for cloud mapping.,,,,,, 2010-030T22:01:00,000T09:00:00,30-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-030T22:01:00,000T09:00:00,30-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-030T23:01:00,000T08:00:00,30-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10030_SP,rider,,,,,, 2010-030T23:01:00,000T07:00:00,30-Jan-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-031T07:01:00,000T19:24:00,31-Jan-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-031T07:01:00,000T19:24:00,31-Jan-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-031T07:01:00,001T00:00:00,31-Jan-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-031T07:01:00,000T19:24:00,31-Jan-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-031T07:01:00,004T15:17:00,31-Jan-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-031T07:01:00,000T19:24:00,31-Jan-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-031T07:41:00,000T01:15:00,31-Jan-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 52.6 range 1.2 Mkm",,,,,, 2010-031T07:41:00,000T01:15:00,31-Jan-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-031T07:41:00,000T01:15:00,31-Jan-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-031T08:56:00,000T05:44:00,31-Jan-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-031T14:40:00,000T01:16:00,31-Jan-10,ISS,Prime,Prometheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Prometheus across Encelad","Images of mutual event, transit of Prometheus across Enceladus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-031T15:56:00,000T01:25:00,31-Jan-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-031T17:21:00,000T04:00:00,31-Jan-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-031T22:01:00,000T09:00:00,31-Jan-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-031T23:01:00,000T08:00:00,31-Jan-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10031_SP,rider,,,,,, 2010-032T02:25:00,007T15:45:00,1-Feb-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-032T02:25:00,003T19:54:00,1-Feb-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-032T02:25:00,006T21:35:00,1-Feb-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-032T02:25:00,003T09:22:00,1-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-032T07:01:00,001T00:00:00,1-Feb-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-032T07:41:00,000T01:15:00,1-Feb-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 58.8 range 1.7 Mkm",,,,,, 2010-032T07:41:00,000T01:15:00,1-Feb-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-032T07:41:00,000T01:15:00,1-Feb-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-032T08:56:00,000T00:58:00,1-Feb-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-032T09:54:00,000T00:45:00,1-Feb-10,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Janus","Images of mutual event, transit of Epimetheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-032T10:39:00,000T06:27:00,1-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-032T17:06:00,000T00:40:00,1-Feb-10,ISS,Prime,Janus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Janus across Enceladus","Images of mutual event, transit of Janus across Enceladus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-032T17:46:00,000T00:30:00,1-Feb-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-032T18:16:00,000T03:05:00,1-Feb-10,CDA,Prime,DustRAM direction,ISD000,,CDA ISD survey 2010-032T18:16,ISD survey,,,,,, 2010-032T22:01:00,000T09:00:00,1-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-032T23:01:00,000T08:00:00,1-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10032_SP,rider,,,,,, 2010-033T07:01:00,001T13:59:00,2-Feb-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-033T07:41:00,000T01:15:00,2-Feb-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 65.7 range 2.2 Mkm",,,,,, 2010-033T07:41:00,000T01:15:00,2-Feb-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-033T07:41:00,000T01:15:00,2-Feb-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-033T08:56:00,000T00:30:00,2-Feb-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 016 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-033T09:26:00,000T13:11:00,2-Feb-10,ISS,Prime,Other,ERRIAPUS,,Erriapus rotation light curve,Erriapus rotation light curve,,,,,, 2010-033T22:37:00,000T06:00:00,2-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-034T05:17:00,000T09:00:00,3-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-034T06:17:00,000T08:00:00,3-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10034_SP,rider,,,,,, 2010-034T14:57:00,000T01:15:00,3-Feb-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 75.7 range 2.8 Mkm",,,,,, 2010-034T14:57:00,000T01:15:00,3-Feb-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-034T14:57:00,000T01:15:00,3-Feb-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-034T16:12:00,000T09:00:00,3-Feb-10,UVIS,Prime,Saturn,MOS125APO,,,"Mosaic scan of Saturn magnetosphere, day 1. One 9.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (7761.59303 bps, from Alain's spreadsheet)x(156.0s per stare)x(125 stares) = 151.35x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 156.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew +2.0 mrad about z-axis. Start data capture, stare 156.0 s, stop data capture.",,,,,, 2010-034T21:00:00,000T02:00:00,3-Feb-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-034T23:00:00,000T23:19:00,3-Feb-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-035T01:12:00,000T05:55:00,4-Feb-10,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observation of 1 of 3 IR stars: CW Leonis, Eta Carinae, Alpha Orionis. Slew to star; settle; execute small box scan; return to waypoint. Observation of each star to take 6 hours; need not be executed contiguously.",,,,,, 2010-035T07:07:00,000T04:00:00,4-Feb-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Erriapus,Observation of outer moon Erriapus,,,,,, 2010-035T07:07:00,000T04:00:00,4-Feb-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-035T11:47:00,000T10:31:00,4-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-035T11:47:00,000T09:00:00,4-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-035T12:47:00,000T08:00:00,4-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_125IC_DSCAL10035_SP,rider,,,,,, 2010-035T21:27:00,000T01:15:00,4-Feb-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86.2 range 3.2 Mkm",,,,,, 2010-035T21:27:00,000T01:15:00,4-Feb-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-035T21:27:00,000T01:15:00,4-Feb-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-035T22:18:00,007T13:04:46,4-Feb-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.010173 Rs exit= 16.001148 Range altitude= 9797.1698 km ... 3588.9685,,,,,, 2010-035T22:18:00,007T15:47:00,4-Feb-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-035T22:18:00,002T06:44:00,4-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-035T22:18:57,000T00:00:01,4-Feb-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.5 d, inc = 0.3 deg, r = 40.258 Rs, phase = 106 deg",,,,,, 2010-035T22:19:00,003T19:51:00,4-Feb-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-035T22:19:00,007T18:04:13,4-Feb-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-035T22:42:00,000T08:00:00,4-Feb-10,UVIS,Prime,Saturn,MOS125APO,,,"Mosaic scan of Saturn magnetosphere, day 2. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (7913.78113 bps, from Alain's spreadsheet)x(153.0s per stare)x(106 stares) = 128.35x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN 105 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture.",,,,,, 2010-036T06:42:00,000T14:25:00,5-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_126SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-036T06:42:00,000T14:25:00,5-Feb-10,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-036T21:47:00,000T09:00:00,5-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-036T22:47:00,000T08:00:00,5-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10036_SP,rider,,,,,, 2010-037T07:27:00,000T03:00:00,6-Feb-10,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2010-037T07:27:00,000T03:00:00,6-Feb-10,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2010-037T10:27:00,000T05:55:00,6-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-037T16:22:00,000T12:00:00,6-Feb-10,UVIS,Prime,Saturn,MOS125APO,,,"Mosaic scan of Saturn magnetosphere, day 3. One 12.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8181.1386 bps, from Alain's spreadsheet)x(148.0s per stare)x(190 stares) = 230.054x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 148.0 s, stop data capture. Repeat PATTERN 189 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 148.0 s, stop data capture.",,,,,, 2010-038T04:22:00,000T10:40:00,7-Feb-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-038T05:02:00,001T13:08:00,7-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-038T05:02:00,000T09:00:00,7-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-038T06:02:00,000T08:00:00,7-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10038_SP,rider,,,,,, 2010-038T15:02:00,000T05:00:00,7-Feb-10,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_126_SCATTERED_SUNLIGHT_TEST_PRIME,"Sunlight falling on the CIRS telescope can potentially be scattered into the instrument by mirror imperfections. We need to quantify the effect of ring particle impacts on the mirror performance. This requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; continuous radial scans are required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scans will begin 40 degrees from FPB, and will scan to 10 degrees of FPB at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time VIMS will integrate for TBD seconds and CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction back to the initial position; to determine whether scattering is asymmetric with respect to the FPB axis, 3 such scans will be made. 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from 40 degrees +Z to 10 degrees +Z and back to 40 degrees +Z. 2) From 40 degrees in -X on the X axis, to 10 degrees on the -X axis, to 40 degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 10 degrees -Z and back to 40 degrees -Z.",,,,,, 2010-038T20:02:00,000T03:00:00,7-Feb-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Skoll,Observation of Skoll,,,,,, 2010-038T20:02:00,000T03:00:00,7-Feb-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-038T23:02:00,000T12:00:00,7-Feb-10,UVIS,Prime,Saturn,MOS125APO,,,"Mosaic scan of Saturn magnetosphere, day 4. One 12.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (9035.88443 bps, from Alain's spreadsheet)x(134.0s per stare)x(205 stares) = 248.22x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 134.0 s, stop data capture. Repeat PATTERN 204 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 134.0 s, stop data capture.",,,,,, 2010-039T00:00:00,000T18:10:00,8-Feb-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-039T11:32:00,000T09:00:00,8-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-039T12:32:00,000T04:00:00,8-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10039_SP,rider,,,,,, 2010-039T18:10:00,000T02:22:00,8-Feb-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-039T18:10:00,002T10:05:00,8-Feb-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-039T18:10:00,000T02:22:00,8-Feb-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-039T20:32:00,002T07:43:00,8-Feb-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-039T20:32:00,002T07:43:00,8-Feb-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-039T21:02:00,000T06:00:00,8-Feb-10,CAPS,Prime,SolarWind,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-040T03:02:00,000T12:00:00,9-Feb-10,UVIS,Prime,Saturn,MOS125APO,,,"Mosaic scan of Saturn magnetosphere, day 5. One 12.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (7567.553208 bps, from Alain's spreadsheet)x(120.0s per stare)x(222 stares) = 201.6x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 120.0 s, stop data capture. Repeat PATTERN 221 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 120.0 s, stop data capture.",,,,,, 2010-040T15:02:00,000T05:45:00,9-Feb-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-040T21:17:00,000T09:00:00,9-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-040T22:17:00,000T04:00:00,9-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10040_SP,rider,,,,,, 2010-041T06:47:00,000T09:50:00,10-Feb-10,UVIS,Prime,Saturn,MOS125APO,,,"Mosaic scan of Saturn magnetosphere, day 6. One 9-hr 50-min block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (7443.494958 bps, from Alain's spreadsheet)x(122.0s per stare)x(166 stares) = 150.7455x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 122.0 s, stop data capture. Repeat PATTERN 165 times. PATTERN: Slew +2.0 mrad about z-axis. Start data capture, stare 122.0 s, stop data capture.",,,,,, 2010-041T16:37:00,000T04:00:00,10-Feb-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-041T21:17:00,000T09:00:00,10-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-041T22:17:00,000T04:00:00,10-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10041_SP,rider,,,,,, 2010-042T04:15:00,000T11:20:00,11-Feb-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-042T04:15:00,000T11:20:00,11-Feb-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-042T04:15:00,000T11:20:00,11-Feb-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-042T04:15:00,000T11:20:00,11-Feb-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-042T06:42:00,000T06:56:00,11-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_126SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-042T06:42:00,000T06:41:00,11-Feb-10,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-042T13:38:00,000T04:45:00,11-Feb-10,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2010-042T15:35:00,000T22:25:00,11-Feb-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-042T15:35:00,000T00:25:00,11-Feb-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-042T15:35:00,000T14:43:00,11-Feb-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-042T16:00:00,000T05:00:00,11-Feb-10,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2010-042T18:23:00,000T02:30:00,11-Feb-10,ISS,Prime,Enceladus,PLMPHSB,,Phase Function Observation,Campaign to study phase function of plume. Group B,,,,,, 2010-042T18:23:00,000T02:30:00,11-Feb-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-042T21:00:00,000T03:00:00,11-Feb-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-042T21:18:00,000T09:00:00,11-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-042T22:18:00,000T08:00:00,11-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10042_SP,rider,,,,,, 2010-043T00:00:00,000T06:18:00,12-Feb-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-043T06:18:00,000T07:42:00,12-Feb-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-043T06:18:00,000T07:42:00,12-Feb-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-043T06:58:00,000T13:28:00,12-Feb-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 001,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning). Repeat for duration.",,,,,, 2010-043T06:58:00,000T13:28:00,12-Feb-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,Hi phase NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Night side: NAC CL1 images at 3 footprints, 12 2x2 images per hour.",,,,,, 2010-043T11:22:46,000T16:40:00,12-Feb-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.989169 Rs exit= 9.0127052 Range altitude= 3587.5509 km ... 2468.4052,,,,,, 2010-043T14:00:00,000T12:06:00,12-Feb-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-043T14:00:00,002T05:45:00,12-Feb-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-043T14:00:00,000T12:06:00,12-Feb-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-043T14:05:00,002T05:40:30,12-Feb-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-043T16:23:13,000T23:00:00,12-Feb-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-044T02:06:00,001T17:39:00,13-Feb-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-044T02:06:00,000T10:39:59,13-Feb-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-044T02:46:00,000T03:12:00,13-Feb-10,UVIS,Prime,Saturn,USUNOCC,Solar occultation,,"This is an ingress solar occultation of Saturn. EUV solar occultation port centered on Sun. Slit aligned tangent with Saturn limb. Record data during ingress. Exposure start time: 2010-044T03:45:40.0. Exposure end time: 2010-044T05:58:00.0. Total exposure time: 2 hr 12 min 20 sec (7940 sec) Total observation time: 3 hr 12 min (11,520 sec) Note: Data will not be collected during the entire duration of this observation. Total data volume = 18918.883 bps (from Alain Jouchoux's spreadsheet)x7940 sec = 150.216x10^6 bits. Data rate multiplier = data volume/(total observation length*nominal bit rate) = 150.216e6/(11,520*32096) = 0.40627",,,,,, 2010-044T02:46:00,000T03:12:00,13-Feb-10,VIMS,SPASS Rider,Sun,USUNOCC,Solar occultation,Saturn Solar Occultation ingress,Saturn Solar Occultation Ingress. UVIS ridealong,,,,,, 2010-044T04:02:46,000T07:13:14,13-Feb-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9962280 Rs exit= 8.9941290 Range altitude= 2464.8655 km ... -1965.2927,,,,,, 2010-044T05:00:00,000T23:00:00,13-Feb-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-044T05:58:00,000T03:59:00,13-Feb-10,ISS,Prime,Saturn,SOLNGRESS,Solar eclipse limb imaging,ISS_052SA_SOLINGRESS,Solar eclipse limb imaging,,,,,, 2010-044T05:58:00,000T03:59:00,13-Feb-10,CIRS,SPASS Rider,Saturn,SOLNGRESS,Solar eclipse limb imaging,Saturn Limb map during eclipse,only last hour useful for limb observation,,,,,, 2010-044T05:58:00,000T03:59:00,13-Feb-10,VIMS,SPASS Rider,Saturn,SOLNGRESS,Solar eclipse limb imaging,Ridealong with ISS limb observing under solar ecli,Take 64*64 frames with ISS.,,,,,, 2010-044T09:57:00,000T01:19:00,13-Feb-10,CIRS,Prime,Saturn,LIMBINT,Limb integration,CIRS_126SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-044T09:57:00,000T01:19:00,13-Feb-10,CIRS,SPASS Rider,Saturn,LIMBINT,Limb integration,CIRS_126SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-044T11:16:00,000T03:24:00,13-Feb-10,RADAR,SPASS Rider,Other,WU4MIMAS,,Mimas 126 Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-044T11:16:00,000T00:24:00,13-Feb-10,CDA,Non-SPASS,Other,RATE320A,,Data rate,Range enter= 8.9962280 Rs exit= 8.9941290 Range altitude= 2464.8655 km ... -1965.2927,,,,,, 2010-044T11:30:00,000T00:45:00,13-Feb-10,ISS,Prime,Calypso,ROTCOLR,,Calypso,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-044T11:30:00,000T00:45:00,13-Feb-10,CIRS,SPASS Rider,Calypso,ROTCOLR,,Calypso rider,Calypso rider: FP3 and FP1 only,,,,,, 2010-044T11:30:00,000T00:45:00,13-Feb-10,UVIS,SPASS Rider,Calypso,ICYLON,Icy satellite longitudinal coverage,,albedo map,,,,,, 2010-044T11:30:00,000T00:45:00,13-Feb-10,VIMS,SPASS Rider,Calypso,ROTCOLR,,Calypso,"640ms, 160ms pairs",,,,,, 2010-044T11:40:00,000T00:15:00,13-Feb-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9962280 Rs exit= 8.9941290 Range altitude= 2464.8655 km ... -1965.2927,,,,,, 2010-044T11:55:00,000T02:45:00,13-Feb-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9962280 Rs exit= 8.9941290 Range altitude= 2464.8655 km ... -1965.2927,,,,,, 2010-044T12:41:00,000T01:42:00,13-Feb-10,CIRS,Prime,Saturn,LIMBINTB,,CIRS_126SA_LIMBINTB001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-044T12:41:00,000T01:42:00,13-Feb-10,CIRS,SPASS Rider,Saturn,LIMBINTB,,CIRS_126SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-044T12:45:59,000T08:18:00,13-Feb-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-044T12:45:59,000T08:18:00,13-Feb-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-044T14:40:00,000T01:14:00,13-Feb-10,RADAR,Prime,Mimas,SCATTRAD,RADAR Scatterometry / Radiometry,Mimas scatt/rad,Dust RAM hazard,,,,,, 2010-044T14:40:00,000T01:14:00,13-Feb-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9962280 Rs exit= 8.9941290 Range altitude= 2464.8655 km ... -1965.2927,,,,,, 2010-044T15:22:46,000T04:00:00,13-Feb-10,MAG,Non-SPASS,Mimas,MITAR,,M2 flyby,"Monitor the interaction of Mimas with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD request.",,,,,, 2010-044T15:23:00,000T02:00:00,13-Feb-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-044T15:23:13,000T02:00:00,13-Feb-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-044T15:25:46,000T02:00:00,13-Feb-10,CDA,SPASS Rider,DustRAM direction,RPX0030,,CDA RPXing 2010-044T16:25:46,RPXing at 2.9419186 Rs,,,,,, 2010-044T15:54:00,000T13:52:00,13-Feb-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9962280 Rs exit= 8.9941290 Range altitude= 2464.8655 km ... -1965.2927,,,,,, 2010-044T16:11:00,000T00:29:00,13-Feb-10,VIMS,Prime,Saturn,ALPCMIOCC,Alpha CMI occultation,alpCMi Saturn occultation,"alpCMi atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Latitude 20N.",,,,,, 2010-044T16:11:00,000T00:29:00,13-Feb-10,CIRS,SPASS Rider,Saturn,ALPCMIOCC,Alpha CMI occultation,CIRS_126SA_ALPCMIOCC001_VIMS,Ride along with VIMS. Stellar Occ Saturn 20N dark limb secondary places our arrays 20 degrees away from normal to limb at 20N,,,,,, 2010-044T16:54:46,000T00:00:01,13-Feb-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.908 Rs, lat = -0 deg, phase = 74 deg",,,,,, 2010-044T17:23:13,000T23:00:00,13-Feb-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-044T17:55:00,000T00:25:00,13-Feb-10,ISS,Prime,Mimas,GEOLOG,Geologic study,Mimas,Mimas post-close approach,,,,,, 2010-044T17:55:00,000T00:25:00,13-Feb-10,CIRS,SPASS Rider,Mimas,GEOLOG,Geologic study,Mimas,"ISS Mimas rider, FP1, FP3 only",,,,,, 2010-044T17:55:00,000T00:25:00,13-Feb-10,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-044T17:55:00,000T00:25:00,13-Feb-10,VIMS,SPASS Rider,Mimas,GEOLOG,Geologic study,Mimas,"640ms, 160ms pairs",,,,,, 2010-044T18:20:00,000T00:25:00,13-Feb-10,CIRS,Prime,Mimas,FP1DAYMAP,CIRS FP1 daytime map,Mimas CIRS daytime,"Fast FP1 raster scan, FP3 riders but not FP4",,,,,, 2010-044T18:20:00,000T00:25:00,13-Feb-10,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas point and stare,follow cirs,,,,,, 2010-044T18:45:00,000T00:25:00,13-Feb-10,ISS,Prime,Mimas,GEOLOG,Geologic study,Mimas,Mimas post-close approach,,,,,, 2010-044T18:45:00,000T00:25:00,13-Feb-10,CIRS,SPASS Rider,Mimas,GEOLOG,Geologic study,Mimas rider,"ISS Mimas rider, FP1, FP3 only",,,,,, 2010-044T18:45:00,000T00:25:00,13-Feb-10,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,albedo map,,,,,, 2010-044T18:45:00,000T00:25:00,13-Feb-10,VIMS,SPASS Rider,Mimas,GEOLOG,Geologic study,Mimas,"640ms, 160ms pairs",,,,,, 2010-044T19:10:00,000T01:25:00,13-Feb-10,CIRS,Prime,Mimas,FP3DAYMAP,CIRS FP3 daytime map,Mimas CIRS daytime FP3,"Global (or near-global) map consisting of three FP3 scans at a rate not to exceed 6 murad/sec. FP1 riders, but not FP4, to save data volume.",,,,,, 2010-044T19:10:00,000T01:25:00,13-Feb-10,ISS,SPASS Rider,Mimas,FP3DAYMAP,CIRS FP3 daytime map,Mimas,"Mimas post-close approach, CIRS rider.",,,,,, 2010-044T19:10:00,000T01:25:00,13-Feb-10,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-044T19:10:00,000T01:25:00,13-Feb-10,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas cirs scan,follow cirs,,,,,, 2010-044T20:35:00,000T00:15:00,13-Feb-10,ISS,Prime,Mimas,GLOCOL,Global coverage mapping,Mimas,Mimas post-close approach,,,,,, 2010-044T20:35:00,000T00:15:00,13-Feb-10,CIRS,SPASS Rider,Mimas,VIMSRIDER,,Mimas VIMS rider,"ISS Mimas rider, FP1, FP3 only",,,,,, 2010-044T20:35:00,000T00:15:00,13-Feb-10,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-044T20:35:00,000T00:15:00,13-Feb-10,VIMS,SPASS Rider,Mimas,GLOCOL,Global coverage mapping,Mimas cirs scan,follow ISS,,,,,, 2010-044T21:00:00,000T02:55:00,13-Feb-10,CIRS,Prime,Saturn,LIMBINTC,,CIRS_126SA_LIMBINTB001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-044T21:00:00,000T02:55:00,13-Feb-10,CIRS,SPASS Rider,Saturn,LIMBINTC,,CIRS_126SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-044T21:03:59,000T22:41:01,13-Feb-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-044T23:55:00,000T01:10:00,13-Feb-10,ISS,Prime,Tethys,GEOLOG,Geologic study,Tethys,Tethys,,,,,, 2010-044T23:55:00,000T01:10:00,13-Feb-10,CIRS,SPASS Rider,Tethys,GEOLOG,Geologic study,Tethys rider,"ISS Mimas rider, FP1, FP3 only",,,,,, 2010-044T23:55:00,000T01:10:00,13-Feb-10,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-044T23:55:00,000T01:10:00,13-Feb-10,VIMS,SPASS Rider,Tethys,GEOLOG,Geologic study,Tethys,"640ms, 160ms pairs",,,,,, 2010-045T04:34:00,000T09:00:00,14-Feb-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 004,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning). repeat",,,,,, 2010-045T04:34:00,000T09:00:00,14-Feb-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.",,,,,, 2010-045T05:46:46,000T16:42:00,14-Feb-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0106078 Rs exit= 15.999884 Range altitude= -1966.5426 km ... -2116.5618,,,,,, 2010-045T13:34:00,000T00:43:00,14-Feb-10,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Janus","Images of mutual event, transit of Epimetheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-045T14:17:00,000T06:06:00,14-Feb-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-045T16:23:13,000T17:06:47,14-Feb-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-045T19:45:00,001T09:45:00,14-Feb-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-045T19:45:00,001T09:45:00,14-Feb-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-045T19:45:00,000T16:15:00,14-Feb-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-045T19:45:30,007T15:41:30,14-Feb-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-045T21:03:00,001T08:27:00,14-Feb-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-045T21:03:00,000T09:00:00,14-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-045T22:03:00,000T08:00:00,14-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10045_SP,rider,,,,,, 2010-045T22:28:46,007T12:58:14,14-Feb-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.011858 Rs exit= 16.010950 Range altitude= -2116.3150 km ... 3638.8933,,,,,, 2010-046T06:03:00,000T15:00:00,15-Feb-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-046T06:43:00,000T03:30:00,15-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_126SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-046T09:30:00,000T02:00:00,15-Feb-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-046T10:13:00,000T02:00:00,15-Feb-10,ISS,Prime,Titan,LOPHASE,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-046T11:30:00,006T09:30:00,15-Feb-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-046T12:00:00,000T17:30:00,15-Feb-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-046T12:13:00,000T08:10:00,15-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_126SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-046T21:03:00,000T09:00:00,15-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-046T22:03:00,000T04:00:00,15-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10046_SP,rider,,,,,, 2010-047T05:30:00,002T10:00:00,16-Feb-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-047T05:30:00,002T10:00:00,16-Feb-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-047T05:30:00,001T14:58:00,16-Feb-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-047T06:43:00,000T08:30:00,16-Feb-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-047T15:13:00,000T01:30:00,16-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-047T15:13:00,000T01:30:00,16-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-047T16:43:00,000T03:40:00,16-Feb-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 005,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning). repeat",,,,,, 2010-047T21:03:00,000T09:00:00,16-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-047T22:03:00,000T04:00:00,16-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10047_SP,rider,,,,,, 2010-048T06:43:00,000T01:15:00,17-Feb-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 45.1 range 1.6 Mkm",,,,,, 2010-048T06:43:00,000T01:15:00,17-Feb-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-048T06:43:00,000T01:15:00,17-Feb-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-048T07:58:00,000T12:30:00,17-Feb-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 007,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning). repeat",,,,,, 2010-048T20:28:00,000T05:40:00,17-Feb-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-049T02:08:00,000T01:30:00,18-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-049T02:08:00,000T01:30:00,18-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-049T02:08:00,000T13:22:00,18-Feb-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-049T04:18:00,000T11:12:00,18-Feb-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-049T04:18:00,001T15:30:00,18-Feb-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-049T04:18:00,000T09:00:00,18-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-049T05:18:00,000T08:00:00,18-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10049_SP,rider,,,,,, 2010-049T13:43:00,000T01:15:00,18-Feb-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 60.4 range 2.3 Mkm",,,,,, 2010-049T13:43:00,000T01:15:00,18-Feb-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-049T13:43:00,000T01:15:00,18-Feb-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-049T14:58:00,000T13:35:00,18-Feb-10,CIRS,Prime,Saturn,MIRTMAP,,CIRS_126SA_MIRTMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2010-049T15:30:00,007T15:50:00,18-Feb-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-049T15:30:00,000T13:03:00,18-Feb-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-049T15:30:00,003T19:57:00,18-Feb-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-049T15:30:00,006T18:30:00,18-Feb-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-049T15:30:00,003T19:57:00,18-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-050T04:33:00,000T05:50:00,19-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-050T10:48:00,000T09:00:00,19-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-050T11:18:00,000T07:58:00,19-Feb-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-050T11:48:00,000T08:00:00,19-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10050_SP,rider,,,,,, 2010-050T19:48:00,001T10:00:00,19-Feb-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-050T19:48:00,001T10:00:00,19-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-050T20:13:00,000T01:30:00,19-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-050T20:13:00,000T01:30:00,19-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-050T21:43:00,000T22:25:00,19-Feb-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_126SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-051T20:08:00,000T10:05:00,20-Feb-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-051T20:48:00,000T09:00:00,20-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-051T21:48:00,000T08:00:00,20-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10051_SP,rider,,,,,, 2010-052T06:13:00,000T01:30:00,21-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-052T06:13:00,000T01:30:00,21-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-052T07:43:00,000T05:40:00,21-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-052T13:23:00,000T12:45:00,21-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_126SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-052T21:00:00,000T02:00:00,21-Feb-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-052T23:00:00,000T12:27:00,21-Feb-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-053T02:03:00,000T05:00:00,22-Feb-10,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2010-053T02:08:00,000T01:30:00,22-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-053T02:08:00,000T01:30:00,22-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-053T04:03:00,000T09:00:00,22-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-053T05:03:00,000T08:00:00,22-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_126IC_DSCAL10053_SP,rider,,,,,, 2010-053T06:03:00,000T01:00:00,22-Feb-10,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-25 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2010-053T11:27:00,003T19:53:00,22-Feb-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-053T11:27:00,007T07:37:00,22-Feb-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S58,Range enter= 16.011858 Rs exit= 16.010950 Range altitude= -2116.3150 km ... 3638.8933,,,,,, 2010-053T11:27:00,001T08:06:00,22-Feb-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-053T11:27:00,007T07:37:00,22-Feb-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-053T11:27:00,001T22:51:00,22-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-053T11:27:31,000T00:00:01,22-Feb-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.5 d, inc = 0.3 deg, r = 40.256 Rs, phase = 106 deg",,,,,, 2010-053T13:43:00,000T18:40:00,22-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_127SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-054T08:23:00,000T01:30:00,23-Feb-10,ISS,Prime,Iapetus,IAPETUS0,,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-054T08:23:00,000T01:30:00,23-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-054T10:33:00,000T09:00:00,23-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-054T11:33:00,000T08:00:00,23-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10054_SP,rider,,,,,, 2010-054T19:33:00,000T23:45:00,23-Feb-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-054T20:13:00,000T01:30:00,23-Feb-10,ISS,Prime,Iapetus,IAPETUS0,,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-054T21:43:00,000T06:05:00,23-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-055T02:00:00,000T03:18:00,24-Feb-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-055T03:48:00,000T03:00:00,24-Feb-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Skoll,Observation of Skoll,,,,,, 2010-055T05:18:00,000T01:30:00,24-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-055T06:48:00,000T00:47:00,24-Feb-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Enceladus","Images of mutual event, transit of Dione across Enceladus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-055T07:35:00,000T00:33:00,24-Feb-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-055T08:08:00,000T01:30:00,24-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-055T10:18:00,001T21:02:00,24-Feb-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-055T10:18:00,000T09:00:00,24-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-055T11:18:00,000T08:00:00,24-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10055_SP,rider,,,,,, 2010-055T19:18:00,000T22:42:00,24-Feb-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-055T19:48:00,000T14:00:00,24-Feb-10,CIRS,Prime,Saturn,MIRTMAP,,CIRS_127SA_MIRTMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2010-056T10:00:00,000T21:20:00,25-Feb-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-056T10:18:00,000T09:00:00,25-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-056T11:18:00,000T08:00:00,25-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10056_SP,rider,,,,,, 2010-056T18:00:00,000T02:00:00,25-Feb-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-056T19:30:00,000T09:10:00,25-Feb-10,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,Full Calibration,null,,,,,, 2010-056T19:58:00,000T01:30:00,25-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-056T20:00:00,001T23:19:00,25-Feb-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-056T23:08:00,000T01:30:00,25-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-056T23:37:00,000T02:23:00,25-Feb-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-057T00:38:00,000T02:52:00,26-Feb-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Tarvos,Observation of Tarvos,,,,,, 2010-057T02:00:00,000T01:30:00,26-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-057T03:30:00,000T06:08:00,26-Feb-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-057T07:20:00,002T10:05:00,26-Feb-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-057T07:20:00,002T10:05:00,26-Feb-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-057T07:20:00,002T10:05:00,26-Feb-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-057T10:18:00,000T09:00:00,26-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-057T11:18:00,000T08:00:00,26-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10057_SP,rider,,,,,, 2010-057T19:58:00,000T06:02:00,26-Feb-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-058T02:00:00,000T01:30:00,27-Feb-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-058T02:00:00,000T01:30:00,27-Feb-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-058T03:30:00,000T06:09:00,27-Feb-10,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 9 EG130 phase at priority 2.,,,,,, 2010-058T10:19:00,000T09:00:00,27-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-058T11:19:00,000T08:00:00,27-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10058_SP,rider,,,,,, 2010-058T19:19:00,000T23:45:00,27-Feb-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-058T19:59:00,000T04:00:00,27-Feb-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-058T23:59:00,000T03:25:00,27-Feb-10,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 9 EG130 phase at priority 2.,,,,,, 2010-059T03:24:00,000T06:00:00,28-Feb-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-059T10:04:00,000T09:00:00,28-Feb-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-059T11:04:00,000T08:00:00,28-Feb-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10059_SP,rider,,,,,, 2010-059T17:25:00,000T11:50:00,28-Feb-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-059T17:25:00,001T01:39:00,28-Feb-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-059T17:25:00,000T11:50:00,28-Feb-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-059T17:25:00,000T11:50:00,28-Feb-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-059T19:04:00,000T15:56:00,28-Feb-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-059T19:29:00,000T13:05:00,28-Feb-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_127SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-060T00:00:00,000T00:34:00,1-Mar-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-060T05:15:00,000T13:49:00,1-Mar-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-060T05:15:00,000T13:49:00,1-Mar-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-060T10:04:00,000T09:00:00,1-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-060T11:00:00,000T02:00:00,1-Mar-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-060T11:04:00,000T08:00:00,1-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10060_SP,rider,,,,,, 2010-060T13:00:00,000T06:04:00,1-Mar-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-060T19:04:00,000T08:06:00,1-Mar-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-060T19:04:00,000T11:06:00,1-Mar-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-060T19:04:00,000T05:24:46,1-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S58,Range enter= 16.011858 Rs exit= 16.010950 Range altitude= -2116.3150 km ... 3638.8933,,,,,, 2010-060T19:04:00,000T00:43:00,1-Mar-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-060T19:04:00,000T08:06:00,1-Mar-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-060T19:04:00,000T08:09:00,1-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-060T19:09:00,000T00:02:00,1-Mar-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S58 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-060T19:47:00,000T00:07:00,1-Mar-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-060T19:54:00,000T00:05:00,1-Mar-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-060T19:55:00,000T07:04:00,1-Mar-10,ISS,Prime,Enceladus,PLMPHSA,,Phase Function Observation,Campaign to study phase function of plume,,,,,, 2010-060T19:55:00,000T07:04:00,1-Mar-10,CIRS,SPASS Rider,Enceladus,PLMPHSA,,CIRS Enceladus Plume Rider,null,,,,,, 2010-060T19:55:00,000T07:04:00,1-Mar-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-060T19:55:00,000T07:04:00,1-Mar-10,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,multiple 160/640 ms.,,,,,, 2010-060T19:59:00,000T00:33:00,1-Mar-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-060T20:32:00,000T00:22:59,1-Mar-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-060T20:54:59,000T18:45:37,1-Mar-10,INMS,Non-SPASS,Saturn,RHEASURV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-061T00:28:46,000T09:20:14,2-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.998977 Rs exit= 9.0102298 Range altitude= 3637.4295 km ... 2487.6867,,,,,, 2010-061T02:59:00,000T02:07:00,2-Mar-10,UVIS,Prime,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-061T02:59:00,000T02:07:00,2-Mar-10,CIRS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,CIRS Enceladus Plume Rider,null,,,,,, 2010-061T02:59:00,000T02:07:00,2-Mar-10,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,multiple 160/640 ms.,,,,,, 2010-061T03:10:00,000T14:00:37,2-Mar-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T03:10:00,000T12:30:36,2-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T03:13:00,002T01:51:00,2-Mar-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-061T05:06:00,000T00:30:00,2-Mar-10,ISS,Prime,Enceladus,PLMPHSA,,Phase Function Observation,Campaign to study phase function of plume,,,,,, 2010-061T05:06:00,000T00:30:00,2-Mar-10,CIRS,SPASS Rider,Enceladus,PLMPHSA,,CIRS Enceladus Plume Rider,null,,,,,, 2010-061T05:06:00,000T00:30:00,2-Mar-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-061T05:06:00,000T00:30:00,2-Mar-10,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,multiple 160/640 ms.,,,,,, 2010-061T06:10:00,000T10:30:36,2-Mar-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-061T06:14:00,000T03:35:00,2-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-061T07:17:00,000T02:34:00,2-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,Deep Space Calibration,Deep Space Calibration,,,,,, 2010-061T09:49:00,000T00:41:00,2-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 15.998977 Rs exit= 9.0102298 Range altitude= 3637.4295 km ... 2487.6867,,,,,, 2010-061T09:50:00,000T03:25:36,2-Mar-10,RADAR,Non-SPASS,Other,WARMUP4RH,RADAR warmup,Warmup before Rhea,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2010-061T10:30:00,000T02:30:00,2-Mar-10,ISS,Prime,Enceladus,PLMPHSA,,Phase Function Observation,Campaign to study phase function of plume,,,,,, 2010-061T10:30:00,000T02:30:00,2-Mar-10,CIRS,SPASS Rider,Enceladus,PLMPHSA,,CIRS Enceladus Plume Rider,null,,,,,, 2010-061T10:30:00,000T02:30:00,2-Mar-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-061T10:30:00,000T02:30:00,2-Mar-10,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,multiple 160/640 ms.,,,,,, 2010-061T10:30:00,000T02:45:36,2-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.998977 Rs exit= 9.0102298 Range altitude= 3637.4295 km ... 2487.6867,,,,,, 2010-061T12:00:00,000T04:40:36,2-Mar-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T13:15:36,000T03:40:00,2-Mar-10,RADAR,Prime,Rhea,SCATTRAD,RADAR Scatterometry / Radiometry,Scatterometry/Radiometry of Rhea,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2010-061T13:15:36,000T03:40:00,2-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 15.998977 Rs exit= 9.0102298 Range altitude= 3637.4295 km ... 2487.6867,,,,,, 2010-061T15:40:36,000T01:15:00,2-Mar-10,INMS,Non-SPASS,Rhea,INBHIRATE,,INMS Inbound to Rhea riding with RADAR,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-061T15:40:36,000T04:00:00,2-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T15:40:36,000T04:00:00,2-Mar-10,MAG,Non-SPASS,Rhea,RHTAR,Rhea targeted flyby,R4 flyby,"The sole Rhea flyby was a downstream flyby. In order to fully understand if the moon is mass-loading or mass-absorbing type both upstream and downstream flybys are required. The new flybys R2,R3,R4 and R5 will fulfill this requirement.",,,,,, 2010-061T16:40:36,000T02:00:00,2-Mar-10,CAPS,SPASS Rider,Rhea,ENCOUNTER,MAPS Campaign,MAPS 049RH Campaign,Part of 049RH MAPS Campaign. Observe interaction between Rhea and Saturn's magnetosphere,,,,,, 2010-061T16:40:36,000T02:00:00,2-Mar-10,RPWS,Non-SPASS,Rhea,RHCA,Rhea closest approach,Rhea closest approach observations,"RPWS observations in the immediate vicinity of Rhea, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2010-061T16:41:00,000T02:00:00,2-Mar-10,CDA,SPASS Rider,DustRAM direction,RHEA,Rhea,CDA RHEA 2010-061T17:41:00 MMH,Rhea Flyby - dust cloud in Hill sphere - interplanetary dust flux,,,,,, 2010-061T16:55:36,000T01:05:00,2-Mar-10,CAPS,Prime,Rhea,RHEAPTG,,MAPS 049RH Campaign,Part of 049RH MAPS Campaign. Observe interaction between Rhea and Saturn's magnetosphere,,,,,, 2010-061T16:55:36,000T22:04:24,2-Mar-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9937511 Rs exit= 8.9966939 Range altitude= 2484.0718 km ... 713.83608,,,,,, 2010-061T16:55:36,000T01:15:00,2-Mar-10,INMS,Non-SPASS,Rhea,RAMPNT,,INMS Prime with MAPS and ORS riding,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-061T17:10:37,000T01:00:00,2-Mar-10,MIMI,SPASS Rider,Rhea,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-061T18:00:36,000T00:50:00,2-Mar-10,VIMS,Prime,Rhea,RHEA,Rhea,Rhea,multiple 160/640 ms.,,,,,, 2010-061T18:00:36,000T00:50:00,2-Mar-10,CIRS,SPASS Rider,Rhea,VIMSINT,,CIRS Rhea Rider on VIMS integration,null,,,,,, 2010-061T18:00:36,000T00:50:00,2-Mar-10,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea targeted flyby,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-061T18:00:36,000T00:50:00,2-Mar-10,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-061T18:10:36,000T01:30:00,2-Mar-10,INMS,Non-SPASS,Rhea,OBHIRATE,,INMS Outbound to Rhea riding with VIMS,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-061T18:10:37,001T10:53:23,2-Mar-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T18:40:36,000T11:21:24,2-Mar-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-061T18:40:36,000T05:19:24,2-Mar-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T18:50:36,000T03:10:00,2-Mar-10,CIRS,Prime,Rhea,FP1SECLN,CIRS elipse observation,CIRS_127RH_FP1SECLN001_PRIME;,"Provide stare times for VIMS before entry First ten minutes for small FP1 and FP3 maps to characterize temperatures in vicinity of (0, 330). Then ten minutes before eclipse (entry at T19:11) FP1 to (0, 330) until well into penumbra. Then occasionally alternate FP1 to (0, 30) and (0, 330) to observe eclipse in both leading (bright) and trailing (dark) hemispheres. FP1 target (0,330), (0, 30). 32>AD>10; phase=3 degrees; AD permits simultaneous FP1 and FP3 entry obs. Excellent opportunity.",,,,,, 2010-061T18:50:36,000T03:10:00,2-Mar-10,CIRS,SPASS Rider,Rhea,FP1SECLN,CIRS elipse observation,CIRS_127RH_SECLN SI,"Two WAC images; one at exit+5 min. (360T01:30), one shortly before return to waypoint (360T03:55)",,,,,, 2010-061T18:50:36,000T03:10:00,2-Mar-10,ISS,SPASS Rider,Rhea,FP1SECLN,CIRS elipse observation,Rhea targeted flyby,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-061T18:50:36,000T03:10:00,2-Mar-10,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-061T18:50:36,000T03:10:00,2-Mar-10,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,multiple 160/640 ms.,,,,,, 2010-061T19:40:36,000T00:36:57,2-Mar-10,INMS,Non-SPASS,Saturn,RHEASURV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-061T19:40:36,000T06:13:23,2-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-061T20:17:34,000T18:00:00,2-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-061T22:05:00,000T04:10:00,2-Mar-10,UVIS,Prime,Saturn,USUNOCC,Solar occultation,USUN_S127I,This is an egress solar occultation by Saturn. 0) 30 min for turn from WAYPOINT to SUN. EUV solar occultation port centered on sun. Slit aligned tangent to Saturn limb. 1) 20 min observation margin. 2) Start recording data when sun is just under 1 Rs from Saturn center. Activity start time: 2010-061T22:48:52.00. Record data until sun is 2 Rs from Saturn center. Activity end time: 2010-062T01:04:38.00. 3) 20 min observation margin. 4) 30 min for turn from SUN to WAYPOINT. Note: Kernel used to calculate egress start and end times is 070918AP_SCPSE_07261_10191.bsp; start and end times may require updates.,,,,,, 2010-062T00:00:00,000T20:00:00,3-Mar-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-062T00:51:46,000T02:00:00,3-Mar-10,CDA,SPASS Rider,DustRAM direction,RPX0040,,CDA RPXing 2010-062T01:51:46,RPXing at 4.3819965 Rs,,,,,, 2010-062T01:53:59,000T08:17:00,3-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-062T01:53:59,000T08:17:00,3-Mar-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-062T02:55:00,000T09:24:00,3-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-062T03:55:00,000T08:25:00,3-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10A,,Deep Space Calibration,null,,,,,, 2010-062T06:02:00,000T06:17:00,3-Mar-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-062T06:02:29,000T00:00:01,3-Mar-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.915 Rs, lat = -0 deg, phase = 75 deg",,,,,, 2010-062T10:10:59,000T18:53:01,3-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-062T12:19:00,000T02:41:00,3-Mar-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-062T12:20:00,000T02:40:00,3-Mar-10,ISS,Prime,Helene,ROTCOLR,,Helene,Helene,,,,,, 2010-062T12:20:00,000T02:40:00,3-Mar-10,CIRS,SPASS Rider,Helene,ROTCOLR,,Helene Rider,null,,,,,, 2010-062T12:20:00,000T02:40:00,3-Mar-10,UVIS,SPASS Rider,Helene,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-062T12:20:00,000T02:40:00,3-Mar-10,VIMS,SPASS Rider,Helene,ROTCOLR,,Helene,multiple 160/640 ms.,,,,,, 2010-062T14:17:34,000T02:00:00,3-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-062T14:19:46,000T02:00:00,3-Mar-10,CDA,SPASS Rider,DustRAM direction,RPX0050,,CDA RPXing 2010-062T15:19:46,RPXing at 7.1444623 Rs,,,,,, 2010-062T15:00:00,000T17:50:00,3-Mar-10,CAPS,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-062T15:00:00,000T01:00:00,3-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 8.9937511 Rs exit= 8.9966939 Range altitude= 2484.0718 km ... 713.83608,,,,,, 2010-062T16:00:00,000T13:04:00,3-Mar-10,CAPS,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-062T16:00:00,000T02:54:46,3-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.9937511 Rs exit= 8.9966939 Range altitude= 2484.0718 km ... 713.83608,,,,,, 2010-062T16:00:00,000T03:31:00,3-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-062T16:17:34,000T12:46:26,3-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-062T17:00:00,000T12:00:00,3-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10062_SP,rider,,,,,, 2010-062T18:54:46,000T10:09:14,3-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0131716 Rs exit= 15.993033 Range altitude= 720.37724 km ... 3646.0957,,,,,, 2010-062T19:31:00,000T09:33:00,3-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-063T05:04:00,001T13:26:00,4-Mar-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-063T05:04:00,000T01:00:00,4-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 9.0131716 Rs exit= 15.993033 Range altitude= 720.37724 km ... 3646.0957,,,,,, 2010-063T05:04:00,000T10:13:34,4-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-063T05:04:00,000T03:46:00,4-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-063T05:04:00,000T03:46:00,4-Mar-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-063T05:04:00,000T03:48:00,4-Mar-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-063T06:04:00,000T13:45:00,4-Mar-10,CAPS,Prime,Saturn,RNGSATPTG,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-063T06:04:00,000T05:30:46,4-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0131716 Rs exit= 15.993033 Range altitude= 720.37724 km ... 3646.0957,,,,,, 2010-063T08:50:00,001T09:40:00,4-Mar-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-063T08:50:00,001T09:40:00,4-Mar-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-063T08:50:00,001T09:40:00,4-Mar-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-063T08:52:00,007T16:50:00,4-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-063T11:34:46,007T14:07:14,4-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.005022 Rs exit= 16.005966 Range altitude= 3651.3269 km ... 5516.1499,,,,,, 2010-063T15:17:34,006T13:16:26,4-Mar-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-063T19:49:00,000T09:00:00,4-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-063T20:49:00,000T08:00:00,4-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10063_SP,rider,,,,,, 2010-064T04:49:00,000T05:00:00,5-Mar-10,CAPS,Prime,Saturn,DUSKPTG,,Dusk Magnetosphere observations,null,,,,,, 2010-064T05:49:00,000T03:00:00,5-Mar-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-064T09:49:00,000T09:00:00,5-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-064T10:49:00,000T08:00:00,5-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10064_SP,rider,,,,,, 2010-064T18:30:00,002T09:45:00,5-Mar-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-064T18:30:00,002T09:45:00,5-Mar-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-064T18:30:00,002T01:14:00,5-Mar-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-064T19:29:00,000T10:00:00,5-Mar-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-064T19:29:00,000T10:00:00,5-Mar-10,UVIS,SPASS Rider,Titan,CLOUD,,UVIS Rider to ISS Cloud,UVIS Rider to ISS Cloud observation,,,,,, 2010-065T05:29:00,000T03:40:00,6-Mar-10,ISS,Prime,Iapetus,HILLSPHE,,Iapetus hill sphere observation,Turn -Y to Iapetus; do 1x3 NAC mosaic; turn to WP.,,,,,, 2010-065T09:49:00,000T09:00:00,6-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-065T10:49:00,000T08:00:00,6-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10065_SP,rider,,,,,, 2010-065T10:49:00,000T07:00:56,6-Mar-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-065T19:29:00,000T01:15:00,6-Mar-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 53.7 range 2.3 Mkm",,,,,, 2010-065T19:29:00,000T01:15:00,6-Mar-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-065T19:29:00,000T01:15:00,6-Mar-10,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-065T20:44:00,000T12:10:00,6-Mar-10,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. MAG segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2010-066T08:54:00,000T10:20:00,7-Mar-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-066T09:34:00,000T09:00:00,7-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-066T10:34:00,000T08:00:00,7-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10066_SP,rider,,,,,, 2010-066T19:14:00,000T00:30:00,7-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-066T19:44:00,000T07:00:00,7-Mar-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-067T02:44:00,000T15:40:00,8-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 1. One 16.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. This observation will scan across the Saturn system between -10 Rs and +10 Rs from the center. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Slew about z axis to 10.0 Rs from Saturn center. Start data capture, stare 125.0 s, stop data capture. Step back across the Saturn system for a distance of 20 Rs by repeating PATTERN 283 times. PATTERN: Slew -2.0 mrad about z-axis. Start data capture, stare 125.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9686.468 bps, from Alain's spreadsheet)x(125.0s per stare)x(284 stares) = 343.870x10^6 bits",,,,,, 2010-067T02:44:00,000T01:31:00,8-Mar-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-067T04:15:00,007T18:50:00,8-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-067T04:15:00,003T21:27:00,8-Mar-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-067T04:15:00,007T18:50:00,8-Mar-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-067T04:15:00,002T00:19:00,8-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-067T18:24:00,000T00:30:00,8-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-067T19:34:00,000T09:00:00,8-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-067T20:34:00,000T08:00:00,8-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10067_SP,rider,,,,,, 2010-068T05:14:00,000T01:15:00,9-Mar-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 81.7 range 3.3 Mkm",,,,,, 2010-068T05:14:00,000T01:15:00,9-Mar-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-068T05:14:00,000T01:15:00,9-Mar-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-068T06:29:00,000T04:24:30,9-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-068T10:53:30,000T08:00:30,9-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 2. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN 105 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (7913.781 bps, from Alain's spreadsheet)x(153.0s per stare)x(106 stares) = 128.346x10^6 bits",,,,,, 2010-068T10:53:30,000T17:40:30,9-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-068T19:34:00,000T09:00:00,9-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-068T20:34:00,000T08:00:00,9-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10068_SP,rider,,,,,, 2010-068T20:35:00,000T06:55:00,9-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-069T04:34:00,001T21:08:00,10-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-069T05:14:00,000T00:30:00,10-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 018 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-069T05:44:00,000T05:10:00,10-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-069T10:54:00,000T08:00:00,10-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 3. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN 105 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (7913.781 bps, from Alain's spreadsheet)x(153.0s per stare)x(106 stares) = 128.346x10^6 bits",,,,,, 2010-069T19:34:00,000T09:00:00,10-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-069T20:34:00,000T08:00:00,10-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10069_SP,rider,,,,,, 2010-070T04:34:00,000T21:08:00,11-Mar-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-070T05:14:00,000T10:25:00,11-Mar-10,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2010-070T15:39:00,000T03:00:00,11-Mar-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Erriapus,Observation of Erriapus,,,,,, 2010-070T15:39:00,000T03:00:00,11-Mar-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-070T19:19:00,000T09:00:00,11-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-070T20:19:00,000T08:00:00,11-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_127IC_DSCAL10070_SP,rider,,,,,, 2010-071T01:42:00,003T21:23:00,12-Mar-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-071T01:42:00,007T07:18:00,12-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.005022 Rs exit= 18 Range altitude= 3651.3269 km ... 5516.1499,,,,,, 2010-071T01:42:00,000T02:37:00,12-Mar-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-071T01:42:00,007T02:07:00,12-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-071T01:42:00,003T21:23:00,12-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-071T01:42:52,000T00:00:01,12-Mar-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.6 d, inc = 0.4 deg, r = 40.401 Rs, phase = 105 deg",,,,,, 2010-071T04:19:00,006T18:41:00,12-Mar-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-071T04:59:00,000T07:34:00,12-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-071T12:33:00,000T00:47:00,12-Mar-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Titan","Images of mutual event, transit of Dione across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-071T13:20:00,000T08:00:00,12-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 4. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 127.0 s, stop data capture. Repeat PATTERN 124 times. PATTERN: Slew +2.0 mrad about z-axis. Start data capture, stare 127.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9533.9253 bps, from Alain's spreadsheet)x(127.0s per stare)x(125 stares) = 151.351x10^6 bits",,,,,, 2010-071T21:20:00,000T11:19:00,12-Mar-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_128SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-071T21:20:00,000T11:19:00,12-Mar-10,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-072T09:19:00,000T09:00:00,13-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-072T10:19:00,000T08:00:00,13-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10072_SP,rider,,,,,, 2010-072T18:59:00,000T05:25:00,13-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-073T00:24:00,000T08:00:00,14-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 5. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 138.0 s, stop data capture. Repeat PATTERN 113 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 138.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (8773.975 bps, from Alain's spreadsheet)x(138.0s per stare)x(114 stares) = 138.032x10^6 bits",,,,,, 2010-073T09:04:00,000T09:00:00,14-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-073T10:04:00,000T08:00:00,14-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10073_SP,rider,,,,,, 2010-073T18:44:00,000T05:40:00,14-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-074T00:24:00,000T08:00:00,15-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 6. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 138.0 s, stop data capture. Repeat PATTERN 113 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 138.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (8773.975 bps, from Alain's spreadsheet)x(138.0s per stare)x(114 stares) = 138.032x10^6 bits",,,,,, 2010-074T00:24:00,000T18:40:00,15-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-074T09:04:00,000T09:00:00,15-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-074T10:04:00,000T08:00:00,15-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10074_SP,rider,,,,,, 2010-074T19:04:00,000T05:20:00,15-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-074T23:05:00,002T09:40:00,15-Mar-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-074T23:05:00,000T01:19:00,15-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-074T23:05:00,002T09:40:00,15-Mar-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-074T23:05:00,002T09:40:00,15-Mar-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-074T23:05:00,002T09:40:00,15-Mar-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-075T00:24:00,000T08:00:00,16-Mar-10,UVIS,Prime,Saturn,MOS127APO,,,"Mosaic scan of Saturn magnetosphere, day 7. One 8.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 124.0 s, stop data capture. Repeat PATTERN 122 times. PATTERN: Slew +2.5 mrad about z-axis. Start data capture, stare 124.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9764.5848 bps, from Alain's spreadsheet)x(124.0s per stare)x(123 stares) = 148.93x10^6 bits",,,,,, 2010-075T00:24:00,000T02:00:00,16-Mar-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-075T09:04:00,000T09:00:00,16-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-075T10:04:00,000T08:00:00,16-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10075_SP,rider,,,,,, 2010-075T10:04:00,000T06:20:00,16-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-075T18:44:00,000T01:15:00,16-Mar-10,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 157.4 range 1.9 Mkm",,,,,, 2010-075T18:44:00,000T01:15:00,16-Mar-10,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-075T18:44:00,000T01:15:00,16-Mar-10,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-075T19:59:00,000T18:25:00,16-Mar-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_128SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-076T14:24:00,000T04:00:00,17-Mar-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-076T19:04:00,000T09:00:00,17-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-076T20:04:00,000T08:00:00,17-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10076_SP,rider,,,,,, 2010-077T04:04:00,000T14:45:00,18-Mar-10,CAPS,Prime,Saturn,DUSKPTG,,Dusk Magnetosphere observations,null,,,,,, 2010-077T08:45:00,000T12:30:00,18-Mar-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-077T08:45:00,000T12:30:00,18-Mar-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-077T08:45:00,000T12:30:00,18-Mar-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-077T08:45:00,000T12:30:00,18-Mar-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-077T18:49:00,000T09:00:00,18-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-077T19:49:00,000T08:00:00,18-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10077_SP,rider,,,,,, 2010-077T19:49:00,000T07:00:00,18-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-077T19:49:00,000T07:00:00,18-Mar-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-077T21:15:00,003T11:19:00,18-Mar-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-077T21:15:00,000T06:34:00,18-Mar-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-077T21:15:00,000T06:34:00,18-Mar-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-077T21:15:00,000T06:34:00,18-Mar-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-077T23:00:00,000T04:00:00,18-Mar-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-078T03:00:00,000T00:49:00,19-Mar-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-078T03:49:00,000T07:15:00,19-Mar-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-078T03:49:00,000T12:39:09,19-Mar-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-078T03:49:00,000T14:36:00,19-Mar-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-078T03:49:00,000T14:36:00,19-Mar-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-078T03:49:00,000T14:43:00,19-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-078T09:00:00,000T23:28:46,19-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data Rate,Range enter= 18. Rs exit= 9.0126497 Range altitude= 5510.5467 km ... 2175.5981,,,,,, 2010-078T15:05:00,002T17:25:00,19-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-078T15:50:00,000T10:10:00,19-Mar-10,CDA,Prime,DustRAM direction,IN1A,,Inbound,CDA art = 13 deg,,,,,, 2010-078T16:28:09,000T23:00:00,19-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-078T18:25:00,002T05:45:00,19-Mar-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-078T18:25:00,000T22:46:59,19-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-078T18:32:00,002T05:38:30,19-Mar-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-079T02:00:00,000T06:15:00,20-Mar-10,CDA,Prime,DustRAM direction,IN1B,,Inbound,"CDA art = 35 deg , 12 ... 9 Rs",,,,,, 2010-079T08:15:00,000T02:50:00,20-Mar-10,UVIS,Prime,Saturn,USUNOCC,Solar occultation,,This is an ingress solar occultation of Saturn. 0) 30 minutes for turn from WAYPOINT to Sun. EUV solar occultation port centered on sun. Slit aligned tangent to Saturn limb. 1) 20 minute observation margin. 2) Activity start time: 2010-079T07:35:06.0. Record data during occultation. Activity end time: 2010-079T11:37:06.0. 3) 20 minute observation margin. 4) 30 minutes for turn from Sun to WAYPOINT.,,,,,, 2010-079T08:15:00,000T02:49:00,20-Mar-10,VIMS,SPASS Rider,Sun,USUNOCC,Solar occultation,Saturn Solar Occultation ingress,Saturn Solar Occultation Ingress. UVIS ridealong,,,,,, 2010-079T08:28:46,001T01:44:00,20-Mar-10,CDA,Non-SPASS,Other,RATE320,,Data Rate,Range enter= 8.9961 Rs exit= 8.99 Range altitude= 2167.5016 km ... 1098.7666,,,,,, 2010-079T11:05:00,000T08:00:00,20-Mar-10,CDA,Prime,DustRAM direction,IN1C,,Inbound,"CDA equatorial ring scan incoming, RPXing at 4.7434 Rs at 2010-079T16:29:46 7.7 ... 3.6 Rs",,,,,, 2010-079T15:28:00,000T02:00:00,20-Mar-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-079T15:28:09,000T02:00:00,20-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-079T17:11:59,000T08:17:00,20-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-079T17:11:59,000T08:17:00,20-Mar-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-079T17:28:09,000T10:36:59,20-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-079T19:18:00,000T00:47:00,20-Mar-10,VIMS,Prime,Saturn,ALPORIOCC,Alpha Orion occultation,alpOri Saturn occultation,"alpOri atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Secondary axis for CDA. Latitude 36N.",,,,,, 2010-079T19:18:00,000T00:47:00,20-Mar-10,CIRS,SPASS Rider,Saturn,ALPORIOCC,Alpha Orion occultation,CIRS_128SA_ALPORIOCC001_VIMS,Ride along with VIMS. Stellar Occ Saturn 36N dark limb,,,,,, 2010-079T20:05:00,000T00:31:00,20-Mar-10,VIMS,Prime,Saturn,ALPCMAOCC,,alpCMa Saturn occultation,"alpCMa atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Secondary axis for CDA. Latitude 41S.",,,,,, 2010-079T20:05:00,000T00:31:00,20-Mar-10,CIRS,SPASS Rider,Saturn,ALPCMAOCC,,CIRS_128SA_ALPCMAOCC001_VIMS,Ride along with VIMS. Stellar Occ Saturn 41S dark limb arrays are fortuitously normal to limb at 41S for CDA secondary,,,,,, 2010-079T20:36:00,000T01:00:00,20-Mar-10,VIMS,Prime,Saturn,ALPCMIOCC,Alpha CMI occultation,alpCMi Saturn occultation,"alpCMi atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Secondary axis for CDA. Latitude 20N.",,,,,, 2010-079T20:36:00,000T01:00:00,20-Mar-10,CIRS,SPASS Rider,Saturn,ALPCMIOCC,Alpha CMI occultation,CIRS_128SA_ALPCMIOCC001_VIMS,Ride along with VIMS. Stellar Occ Saturn 20N dark limb,,,,,, 2010-079T21:21:54,000T00:00:01,20-Mar-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.913 Rs, lat = -0 deg, phase = 75 deg",,,,,, 2010-079T21:50:00,000T01:50:00,20-Mar-10,CDA,Prime,DustRAM direction,PERI,,Periapse,"CDA equatorial ring scan incoming, RPXing at 4.7434 Rs at 2010-079T16:29:46 2.9...3.4 Rs",,,,,, 2010-079T21:50:00,000T01:50:00,20-Mar-10,VIMS,SPASS Rider,Star,ALPCMICAL,Alpha CMI calibration,alpCMi calibration,alpCMi star calibration; CDA rider,,,,,, 2010-079T23:40:00,000T02:20:00,20-Mar-10,CDA,Prime,DustRAM direction,OUT1A,,outbound,"CDA equatorial ring scan incoming, RPXing at 4.7434 Rs at 2010-079T16:29:46 3.6 ... 4.6 Rs",,,,,, 2010-080T01:28:59,000T22:41:01,21-Mar-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-080T02:00:00,000T04:30:00,21-Mar-10,CDA,Prime,DustRAM direction,OUT1B,,outbound,"CDA equatorial ring scan incoming, RPXing at 4.7434 Rs at 2010-079T16:29:46 4.6 ... 7.1 Rs Tethys and Dione crossing",,,,,, 2010-080T04:00:00,000T02:00:00,21-Mar-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-080T04:05:08,000T02:00:00,21-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-080T06:05:08,000T23:00:00,21-Mar-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-080T06:30:00,000T17:00:00,21-Mar-10,CDA,Prime,DustRAM direction,OUT1C,,outbound,"CDA equatorial ring scan incoming, RPXing at 4.7434 Rs at 2010-079T16:29:46 7.1 ... 14.7 Rs, Rhea orbit Xing",,,,,, 2010-080T10:12:46,000T16:36:14,21-Mar-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data Rate,Range enter= 9.013 Rs exit= 18 Range altitude= 1105.7048 km ... 4132.8606,,,,,, 2010-080T23:30:00,000T06:19:00,21-Mar-10,CDA,Prime,DustRAM direction,OUT1D,,outbound,"CDA equatorial ring scan incoming, RPXing at 4.7434 Rs at 2010-079T16:29:46 14.7 ... 17 Rs",,,,,, 2010-081T00:10:00,001T09:40:00,22-Mar-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-081T00:10:00,001T09:40:00,22-Mar-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-081T00:10:30,000T17:23:30,22-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-081T02:49:00,000T03:00:00,22-Mar-10,RADAR,SPASS Rider,Other,WU4SEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-081T02:49:00,000T06:03:46,22-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data Rate,,,,,,, 2010-081T05:05:08,002T22:28:52,22-Mar-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-081T05:49:00,000T01:30:00,22-Mar-10,RADAR,Prime,Titan,SEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2010-081T08:34:00,001T01:16:00,22-Mar-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-081T08:34:00,000T09:00:00,22-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-081T08:52:46,007T08:08:14,22-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 18 Rs exit= 16.009515 Range altitude= 4138.1776 km ... 4827.1204,,,,,, 2010-081T09:34:00,000T08:00:00,22-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10081_SP,rider,,,,,, 2010-081T09:34:00,000T06:00:00,22-Mar-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-081T17:34:00,002T09:59:30,22-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-081T17:34:00,000T16:16:00,22-Mar-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-081T18:00:00,000T01:15:00,22-Mar-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 37.7 range 2 Mkm",,,,,, 2010-081T18:00:00,000T01:15:00,22-Mar-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-081T18:00:00,000T01:15:00,22-Mar-10,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-081T19:15:00,000T00:30:00,22-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-081T19:45:00,000T06:00:00,22-Mar-10,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2010-081T19:45:00,000T06:00:00,22-Mar-10,CIRS,SPASS Rider,rings(general),DUSKPTG,,Rider to CAPS for Dark Sky after CIRS Prime,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-082T01:45:00,000T10:00:00,23-Mar-10,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. RING segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2010-082T01:45:00,000T10:00:00,23-Mar-10,CIRS,SPASS Rider,rings(general),EG80PHASE,,Rider to VIMS E-G Phase,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-082T09:50:00,002T09:40:00,23-Mar-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-082T09:50:00,001T17:44:00,23-Mar-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-082T09:50:00,001T17:44:00,23-Mar-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-082T09:50:00,001T17:44:00,23-Mar-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-082T11:45:00,000T01:20:00,23-Mar-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Tethys","Images of mutual event, transit of Dione across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-082T13:05:00,000T05:00:00,23-Mar-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-082T18:34:00,000T09:00:00,23-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-082T19:34:00,000T08:00:00,23-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10082_SP,rider,,,,,, 2010-083T04:00:00,000T01:15:00,24-Mar-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 63.1 range 2.7 Mkm",,,,,, 2010-083T04:00:00,000T01:15:00,24-Mar-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-083T04:00:00,000T01:15:00,24-Mar-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-083T05:15:00,000T00:30:00,24-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-083T05:45:00,000T01:00:00,24-Mar-10,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Epimetheus","Images of mutual event, transit of Rhea across Epimetheus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-083T06:45:00,000T11:20:00,24-Mar-10,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2010-083T06:45:00,000T11:20:00,24-Mar-10,CIRS,SPASS Rider,rings(general),LRLEMP,,RIDER to ISS Rings Prime Science,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-083T18:05:00,000T10:09:00,24-Mar-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-083T18:34:00,000T09:00:00,24-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-083T19:34:00,000T08:00:00,24-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10083_SP,rider,,,,,, 2010-084T03:34:00,000T15:56:00,25-Mar-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-084T03:34:00,001T13:45:00,25-Mar-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-084T03:34:00,000T02:25:00,25-Mar-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-084T03:34:00,004T13:26:30,25-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-084T03:34:00,002T14:45:00,25-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-084T04:14:00,000T01:15:00,25-Mar-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 76.1 range 3.1 Mkm",,,,,, 2010-084T04:14:00,000T01:15:00,25-Mar-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-084T04:14:00,000T01:15:00,25-Mar-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-084T05:29:00,000T00:30:00,25-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-084T05:59:00,000T06:45:00,25-Mar-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-084T12:44:00,000T10:15:00,25-Mar-10,UVIS,Prime,Saturn,MOS128APO,,,"Mosaic scan of Saturn magnetosphere, day 2. One 10.25-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (8236.79261 bps, from Alain's spreadsheet)x(147.0s per stare)x(153 stares) = 185.254x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 147.0 s, stop data capture. Repeat PATTERN 152 times. PATTERN: Slew +2.0 mrad about z-axis. Start data capture, stare 147.0 s, stop data capture.",,,,,, 2010-084T12:44:00,000T06:46:00,25-Mar-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-084T19:30:00,007T18:55:00,25-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-084T19:30:00,002T07:49:00,25-Mar-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-084T19:30:00,001T11:15:00,25-Mar-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-084T22:59:00,000T08:40:00,25-Mar-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_128SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-085T08:19:00,000T09:00:00,26-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-085T09:19:00,000T08:00:00,26-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10085_SP,rider,,,,,, 2010-085T17:19:00,001T10:00:00,26-Mar-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-085T18:19:00,000T00:30:00,26-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-085T18:49:00,000T00:43:00,26-Mar-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Tethys","Images of mutual event, transit of Dione across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-085T19:32:00,000T08:35:00,26-Mar-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_128SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-086T04:07:00,000T11:00:00,27-Mar-10,UVIS,Prime,Saturn,MOS128APO,,,"Mosaic scan of Saturn magnetosphere, day 3. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (9368.11251 bps, from Alain's spreadsheet)x(129.0s per stare)x(190 stares) = 230.054x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 129.0 s, stop data capture. Repeat PATTERN 189 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 129.0 s, stop data capture.",,,,,, 2010-086T06:45:00,005T17:15:00,27-Mar-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-086T15:07:00,000T00:52:00,27-Mar-10,ISS,Prime,Janus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Janus across Titan","Images of mutual event, transit of Janus across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-086T15:59:00,000T01:40:00,27-Mar-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 015 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-086T18:19:00,000T09:00:00,27-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-086T18:19:00,000T09:00:00,27-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-086T19:19:00,000T08:00:00,27-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10086_SP,rider,,,,,, 2010-087T03:19:00,001T13:45:00,28-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-087T03:19:00,000T19:41:00,28-Mar-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-087T03:19:00,001T13:42:00,28-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-087T03:19:01,001T13:41:59,28-Mar-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-087T03:20:00,001T04:42:00,28-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-087T03:59:00,000T06:00:00,28-Mar-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-087T09:59:00,000T11:45:00,28-Mar-10,UVIS,Prime,Saturn,MOS128APO,,,"Mosaic scan of Saturn magnetosphere, day 5. One 11.75-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (7712.15614 bps, from Alain's spreadsheet)x(157.0 s per stare)x(177 stares) = 214.313x10^6 bits. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 157.0 s, stop data capture. Repeat PATTERN 176 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 157.0 s, stop data capture.",,,,,, 2010-087T09:59:00,000T12:26:00,28-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-087T21:44:00,000T00:41:00,28-Mar-10,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Janus","Images of mutual event, transit of Rhea across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-087T22:25:00,000T05:59:00,28-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-087T23:00:00,000T04:00:00,28-Mar-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-088T03:00:00,000T14:01:00,29-Mar-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-088T04:24:00,000T03:00:00,29-Mar-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Bebhionn,Observation of Bebhionn,,,,,, 2010-088T04:24:00,000T03:00:00,29-Mar-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-088T08:04:00,000T09:00:00,29-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-088T09:04:00,000T08:00:00,29-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_128IC_DSCAL10088_SP,rider,,,,,, 2010-088T09:04:00,000T07:00:00,29-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-088T09:04:00,000T06:00:00,29-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-088T17:01:00,003T21:24:00,29-Mar-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-088T17:01:00,006T09:48:00,29-Mar-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S S59,Range enter= 16.006364 Rs exit= 16.009515 Range altitude= 4138.1776 km ... 4827.1204,,,,,, 2010-088T17:01:00,003T23:48:00,29-Mar-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-088T17:01:00,006T09:48:00,29-Mar-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-088T17:01:00,001T10:03:00,29-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-088T17:01:54,000T00:00:01,29-Mar-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.6 d, inc = 0.4 deg, r = 40.402 Rs, phase = 105 deg",,,,,, 2010-088T17:04:00,001T10:00:00,29-Mar-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-088T17:44:00,000T03:00:00,29-Mar-10,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2010-088T17:44:00,000T03:00:00,29-Mar-10,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2010-088T20:44:00,000T11:00:00,29-Mar-10,UVIS,Prime,Saturn,MOS128APO,,,"Mosaic scan of Saturn magnetosphere, day 6. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (7811.66783 bps, from Alain's spreadsheet)x(155.0s per stare)x(166 stares) = 200.9942x10^6 bits(bytes?) Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 155.0 s, stop data capture. Repeat PATTERN 165 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 155.0 s, stop data capture.",,,,,, 2010-089T07:44:00,000T09:40:00,30-Mar-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_129SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-089T07:44:00,000T09:40:00,30-Mar-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn CIRS COMPSIT ridealong,Second rotation for winds measurements. Other rotation measurements during MIRMAP and COMPSIT004 ridealong.,,,,,, 2010-089T16:04:00,000T11:00:00,30-Mar-10,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS Ka-TWTA Maintenance,"Ka-TWTA maintenance; Pointing = n/a; No DSN tracking required, but since PIM occurs over DSS-55 downlink, monitor Ka-band.",,,,,, 2010-089T18:04:00,000T09:00:00,30-Mar-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-089T19:03:00,000T07:01:00,30-Mar-10,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2010-089T19:04:00,000T08:00:00,30-Mar-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10089_SP,rider,,,,,, 2010-090T03:04:00,002T11:21:00,31-Mar-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-090T03:44:00,000T04:25:00,31-Mar-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-090T03:54:00,000T09:10:00,31-Mar-10,CAPS,Non-SPASS,InstrumentCalibration,CALIBRATE,Calibration,Full Calibration,null,,,,,, 2010-090T08:09:00,000T23:00:00,31-Mar-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_129SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-090T08:09:00,000T23:00:00,31-Mar-10,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Saturn CIRS COMPSIT ridealong,Third and fourth rotations for winds measurements. Other rotation measurement during COMPSIT001 and COMPSIT004 ridealongs.,,,,,, 2010-091T00:00:00,001T00:00:00,1-Apr-10,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2010-091T07:49:00,000T09:00:00,1-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-091T08:49:00,000T08:00:00,1-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10091_SP,rider,,,,,, 2010-091T17:29:00,000T11:00:00,1-Apr-10,UVIS,Prime,Saturn,MOS128APO,,,"Mosaic scan of Saturn magnetosphere, day 9. One 11.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (6652.79403 bps, from Alain's spreadsheet)x(182.0s per stare)x(142 stares) = 171.935x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 182.0 s, stop data capture. Repeat PATTERN 141 times. PATTERN: Slew +2.0 mrad about z-axis. Start data capture, stare 182.0 s, stop data capture.",,,,,, 2010-092T00:00:00,000T14:25:00,2-Apr-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-092T04:29:00,000T00:57:00,2-Apr-10,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Janus","Images of mutual event, transit of Epimetheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-092T05:26:00,000T01:43:00,2-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-092T07:49:00,000T09:00:00,2-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-092T08:49:00,000T08:00:00,2-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10092_SP,rider,,,,,, 2010-092T14:25:00,002T09:40:00,2-Apr-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-092T14:25:00,002T09:40:00,2-Apr-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-092T14:25:00,001T16:09:00,2-Apr-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-092T14:25:00,002T03:24:00,2-Apr-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-092T16:49:00,000T23:45:00,2-Apr-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-092T17:29:00,000T01:15:00,2-Apr-10,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 153.2 range 1.5 Mkm",,,,,, 2010-092T17:29:00,000T01:15:00,2-Apr-10,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-092T17:29:00,000T01:15:00,2-Apr-10,UVIS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-092T18:44:00,000T12:10:00,2-Apr-10,UVIS,Prime,Saturn,MOS128APO,,,"Mosaic scan of Saturn magnetosphere, day 10. One 12.0-hr block of time assumed. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. As no data will be collected while Cassini is slewing, actual data volume = (9035.88443 bps, from Alain's spreadsheet)x(134.0s per stare)x(205 stares) = 248.216x10^6 bits Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 134.0 s, stop data capture. Repeat PATTERN 204 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 134.0 s, stop data capture.",,,,,, 2010-093T07:34:00,000T09:00:00,3-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-093T08:34:00,000T08:00:00,3-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10093_SP,rider,,,,,, 2010-093T16:34:00,001T10:15:00,3-Apr-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-093T17:14:00,000T17:55:00,3-Apr-10,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 9 EG130 phase at priority 2.,,,,,, 2010-094T06:34:00,000T11:15:00,4-Apr-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-094T11:09:00,000T06:00:00,4-Apr-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-094T17:49:00,000T06:16:00,4-Apr-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-094T17:49:00,000T06:16:00,4-Apr-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-094T17:49:00,000T09:00:00,4-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-094T18:49:00,000T08:00:00,4-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10094_SP,rider,,,,,, 2010-095T00:05:00,000T02:44:00,5-Apr-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-095T00:05:00,000T02:44:00,5-Apr-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-095T00:05:00,000T02:44:00,5-Apr-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-095T00:05:00,000T02:44:00,5-Apr-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-095T02:49:00,000T10:21:00,5-Apr-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-095T02:49:00,000T11:01:39,5-Apr-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-095T02:49:00,001T03:55:46,5-Apr-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S S59,Range enter= 16.006364 Rs exit= 16.009515 Range altitude= 4138.1776 km ... 4827.1204,,,,,, 2010-095T02:49:00,000T00:43:00,5-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-095T02:49:00,000T09:01:39,5-Apr-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-095T02:49:00,001T06:39:00,5-Apr-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-095T02:54:00,000T00:02:00,5-Apr-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S59 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-095T03:32:00,000T00:07:00,5-Apr-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-095T03:39:00,000T00:05:00,5-Apr-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-095T03:44:00,000T00:33:00,5-Apr-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-095T03:44:18,000T02:06:21,5-Apr-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-095T03:44:18,000T02:06:21,5-Apr-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T03:44:18,000T02:06:21,5-Apr-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,VIMS ridealong with CIRS. Stare at Titan. Phase = 161 deg. Lat/Lon = 04N/140 deg. Resolution = 120 km/px. Obtain 160 and 640 msec cubes for global mapping and cloud monitoring. Temp. N,,,,,, 2010-095T04:17:00,000T00:22:59,5-Apr-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-095T04:39:59,000T10:10:40,5-Apr-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-095T05:50:39,000T01:00:00,5-Apr-10,ISS,Prime,Titan,NIGHTWAC,ISS lightning / aurora observation,NWP (Nightside WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T05:50:39,000T01:00:00,5-Apr-10,CIRS,SPASS Rider,Titan,NIGHTWAC,ISS lightning / aurora observation,,Ride along with ISS.,,,,,, 2010-095T05:50:39,000T01:00:00,5-Apr-10,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan,VIMS ridealong with ISS. Stare at Titan. Phase = 161 deg. Lat/Lon = 04N/143 deg. Resolution = 99 km/px. Obtain 160 and 640 msec cubes for global mapping and cloud monitoring. Temp. N,,,,,, 2010-095T06:50:39,000T04:00:00,5-Apr-10,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-095T06:50:39,000T04:00:00,5-Apr-10,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T06:50:39,000T04:00:00,5-Apr-10,ISS,SPASS Rider,Titan,MIRLMPAIR,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T06:50:39,000T04:00:00,5-Apr-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS. Titan limb mapping. Phase = 161 deg. Lat/Lon = 04N/144 deg. Resolution = 89 km/px. Obtain cubes for limb mapping. Temp. R,,,,,, 2010-095T10:50:39,000T02:45:00,5-Apr-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-095T10:50:39,000T02:45:00,5-Apr-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T10:50:39,000T02:45:00,5-Apr-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Titan scan.,VIMS ridealong with CIRS. Scan across Titan. Phase = 161 deg. Lat/Lon = 04N/150 deg. Resolution = 47 km/px. Obtain cubes while scanning across Titan. Temp. T,,,,,, 2010-095T11:50:39,000T01:19:21,5-Apr-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-095T11:50:39,000T08:00:00,5-Apr-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T67 flyby,"Second of the two 'blind flybys' since MAG is unlikely to detect Titan's induced magnetosphere. Occurring in the same SLT sector as T52-T62, it will be used to characterize Saturn's background magnetic field variation with SKR longitude at a fixed SLT. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2010-095T13:10:00,000T00:40:39,5-Apr-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-095T13:35:39,000T01:00:00,5-Apr-10,CIRS,Prime,Titan,FIRLMBCON,,,"Limb condensate search. Four pointings at 100, 130, 160 and 190 km altitude, constant latitude.",,,,,, 2010-095T13:35:39,000T01:00:00,5-Apr-10,CIRS,SPASS Rider,Titan,FIRLMBCON,,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2010-095T13:35:39,000T01:00:00,5-Apr-10,ISS,SPASS Rider,Titan,FIRLMBCON,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T13:35:39,000T01:00:00,5-Apr-10,UVIS,SPASS Rider,Titan,FIRLMBCON,,Rider to CIRS,Rider to CIRS.,,,,,, 2010-095T13:35:39,000T01:00:00,5-Apr-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,VIMS ridealong with CIRS. Regional mapping of Titan. Phase = 152 deg. Lat/Lon = 00N/159 deg. Resolution = 23 km/px. Obtain cubes for Titan mosaic and regional mapping.,,,,,, 2010-095T13:50:39,000T01:00:00,5-Apr-10,CAPS,SPASS Rider,Titan,T67INBD,,Titan Encounter,null,,,,,, 2010-095T13:50:39,000T01:00:00,5-Apr-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-095T13:50:39,000T01:00:00,5-Apr-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-095T14:35:39,000T00:30:00,5-Apr-10,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2010-095T14:35:39,000T00:30:00,5-Apr-10,CIRS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2010-095T14:35:39,000T00:30:00,5-Apr-10,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T14:35:39,000T00:30:00,5-Apr-10,UVIS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,Rider to CIRS,Rider to CIRS.,,,,,, 2010-095T14:35:39,000T00:30:00,5-Apr-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,VIMS ridealong with CIRS. Regional mapping of Titan. Phase = 142 deg. Lat/Lon = 00N/170 deg. Resolution = 12 km/px. Obtain cubes for Titan mosaic and regional mapping.,,,,,, 2010-095T14:50:39,000T02:00:00,5-Apr-10,CAPS,SPASS Rider,Titan,T67CLOSE,,Titan Encounter,null,,,,,, 2010-095T14:50:39,000T02:00:00,5-Apr-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-095T14:50:39,000T00:40:00,5-Apr-10,INMS,Non-SPASS,Titan,TITAN67,,Titan Flyby,Titan observation,,,,,, 2010-095T14:50:39,000T02:00:00,5-Apr-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-095T15:05:39,000T00:30:00,5-Apr-10,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2010-095T15:05:39,000T00:30:00,5-Apr-10,CIRS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,ISS_PHOT_1x1,"ISS WAC support imaging, 2 images per integration (2 integrations total = 4 frames, 0.5 Mb/frame)",,,,,, 2010-095T15:05:39,000T00:30:00,5-Apr-10,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T15:05:39,000T00:30:00,5-Apr-10,UVIS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,Rider to CIRS,Rider to CIRS.,,,,,, 2010-095T15:05:39,000T00:30:00,5-Apr-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,VIMS ridealong with CIRS. Regional mapping of Titan. Phase = 130 deg. Lat/Lon = 00N/182 deg. Resolution = 7.8 km/px. Obtain cubes for Titan mosaic and regional mapping.,,,,,, 2010-095T15:30:39,000T00:40:00,5-Apr-10,INMS,Non-SPASS,Titan,TITAN67,,Titan Flyby,Titan observation,,,,,, 2010-095T15:35:39,000T02:15:00,5-Apr-10,ISS,Prime,Titan,VHIGHRES,,VHI (Very High-Resolution Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T15:35:39,000T02:15:00,5-Apr-10,CIRS,SPASS Rider,Titan,VHIGHRES,,,Ride along with ISS.,,,,,, 2010-095T15:35:39,000T02:15:00,5-Apr-10,UVIS,SPASS Rider,Titan,VHIGHRES,,Rider ro ISS,Mosaic Titan,,,,,, 2010-095T15:40:39,000T02:10:00,5-Apr-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,VIMS ridealong with ISS. Regional mapping of Titan during C/A. Phase = 92 deg. Lat/Lon = 00N/221 deg. Resolution = 4 km/px. Obtain cubes for mosaics and regional mapping.,,,,,, 2010-095T16:10:39,000T00:40:00,5-Apr-10,INMS,Non-SPASS,Titan,TITAN67,,Titan Flyby,Titan observation,,,,,, 2010-095T16:50:39,000T01:00:00,5-Apr-10,CAPS,SPASS Rider,Titan,T67OUTBND,,Titan Encounter,null,,,,,, 2010-095T16:50:39,000T01:00:00,5-Apr-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-095T16:50:39,000T23:43:21,5-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-095T16:50:39,000T01:00:00,5-Apr-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-095T17:50:39,000T02:00:00,5-Apr-10,ISS,Prime,Titan,REGMAP,Regional mapping,NRM (NAC Regional Map),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T17:50:39,000T02:00:00,5-Apr-10,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS.,,,,,, 2010-095T17:50:39,000T02:00:00,5-Apr-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,VIMS ridealong with ISS. Regional mapping of Titan. Phase = 6 deg. Lat/Lon = 00N/319 deg. Resolution = 19 km/px. Obtain cubes for mosaics and regional mapping. Temp. J,,,,,, 2010-095T17:50:39,000T17:34:21,5-Apr-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-095T17:50:39,000T15:34:21,5-Apr-10,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2010-095T19:50:39,000T01:00:00,5-Apr-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-095T19:50:39,000T01:00:00,5-Apr-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T19:50:39,000T01:00:00,5-Apr-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS. Titan limb mapping. Phase = 12 deg. Lat/Lon = 00S/328 deg. Resolution = 39 km/px. Obtain cubes for limb mapping. Temp. J.,,,,,, 2010-095T19:50:39,000T13:34:21,5-Apr-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-095T20:50:39,000T04:00:00,5-Apr-10,ISS,Prime,Titan,GLOBMAP,Global coverage mapping,NRM (NAC Regional Map),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-095T20:50:39,000T04:00:00,5-Apr-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-095T20:50:39,000T04:00:00,5-Apr-10,UVIS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Rider ro ISS,Mosaic Titan,,,,,, 2010-095T20:50:39,000T04:00:00,5-Apr-10,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global mapping,VIMS ridealong with ISS. Global mapping of Titan. Phase = 13 deg. Lat/Lon = 00S/331 deg. Resolution = 49 km/px. Obtain 160 and 640 msec cubes for global mapping and cloud monitoring. Temp. H.,,,,,, 2010-096T00:50:39,000T05:00:00,6-Apr-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping,Global mapping of Titan. Phase = 16 deg. Lat/Lon = 00S/337 deg. Resolution = 89 km/px. Obtain 160 and 640 msec cubes for global mapping.,,,,,, 2010-096T00:50:39,000T05:00:00,6-Apr-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-096T00:50:39,000T05:00:00,6-Apr-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-096T05:50:39,000T00:48:39,6-Apr-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping,Global mapping of Titan. Phase = 18 deg. Lat/Lon = 00S/344 deg. Resolution = 140 km/px. Obtain 160 and 640 msec cubes for global mapping.,,,,,, 2010-096T05:50:39,000T00:48:39,6-Apr-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-096T05:50:39,000T00:48:39,6-Apr-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-096T06:44:46,000T16:58:00,6-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.997483 Rs exit= 9.0000060 Range altitude= 4821.5613 km ... 1527.9025,,,,,, 2010-096T07:34:00,000T09:00:00,6-Apr-10,RSS,SPASS Rider,Dione,KADOWN,RSS Ka-Band downlink,GSE pass for Dione's mass,Downlink pass at Ka-band for Dione's mass determination and for improving locally Cassini orbit.,,,,,, 2010-096T07:34:00,000T09:00:00,6-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-096T08:34:00,000T08:00:00,6-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10096_SP,rider,,,,,, 2010-096T09:25:00,000T07:09:00,6-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-096T09:25:00,000T07:09:00,6-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-096T09:25:00,000T07:09:00,6-Apr-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-096T09:28:00,000T07:06:30,6-Apr-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-096T11:25:00,000T05:18:00,6-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-096T16:34:00,000T11:42:11,6-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-096T16:34:00,000T12:12:02,6-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-096T16:34:00,000T12:19:11,6-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-096T16:34:00,000T10:42:11,6-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-096T16:34:00,001T17:30:00,6-Apr-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-096T16:44:00,000T05:07:00,6-Apr-10,CAPS,Prime,Saturn,RNGSATPTG,Ring / Satellite,Rings and Satellites pointing,null,,,,,, 2010-096T21:51:00,000T03:34:00,6-Apr-10,UVIS,Prime,Saturn,USUNOCC,Solar occultation,USUN_S129I,This is a solar ingress occultation by Saturn. 0) 30 min for turn from WAYPOINT to SUN. EUV solar occultation port centered on san. Slit aligned tangent to Saturn limb. 1) 20 min observation margin. 2) Start recording data when sun is just under 2 Rs from Saturn center. Activity start time: 2010-096T21:41:48.00. Record data until sun is 1 Rs from Saturn center. Activity end time: 2010-097T00:55:20.00. 3) 20 min observation margin. 4) 30 min for turn from SUN to WAYPOINT. Note: Kernel used to calculate ingress start and end times is 070918AP_SCPSE_07261_10191.bsp; start and end times may require updates.,,,,,, 2010-096T21:51:00,000T03:34:00,6-Apr-10,VIMS,SPASS Rider,Saturn,SOLAROCC,Solar occultation,Solar occ rider,"40 msec, solar occ mode",,,,,, 2010-096T23:42:46,001T02:22:00,6-Apr-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9842156 Rs exit= 8.9915281 Range altitude= 1520.2853 km ... 709.94111,,,,,, 2010-097T01:25:00,000T00:10:00,7-Apr-10,ISS,Prime,Dione,PLUMESEAR,,Dione plume search,Sit'n'stare on western limb of Dione for 10 min.,,,,,, 2010-097T01:25:00,000T00:10:00,7-Apr-10,CIRS,SPASS Rider,Dione,PLUMESEAR,,CIRS_129DI_PLUMESEAR001_ISS,Ride with ISS. FP1 and FP3 only,,,,,, 2010-097T01:25:00,000T00:10:00,7-Apr-10,VIMS,SPASS Rider,Dione,PLUMSRCH,,Dione,640ms,,,,,, 2010-097T01:45:11,000T02:46:00,7-Apr-10,CIRS,Prime,Dione,FP1DRKMAP,CIRS FP1 dark side map,CIRS_129DI_FP1DRKMAP001_PRIME;,"Detailed design request, 091023: The sun is occulted by Saturn until 04:16, so we don't need to worry about sun avoidance until then, despite the high phase angle. 01:45 - 02:25 N/S FP3/FP4 limb-to-limb scan, 6 murad/sec, passing through 210 W, 0 N, to look for thermal emission from Dione fractures. 02:25 - 03:05 N/S FP3/FP4 scan, 6 murad/sec, passing through 180 W, 60 N, to look for thermal emission from Dione fractures. Start above north limb, go as far south as time permits. 03:05 - 03:25 Global FP1 scan, Nyquist sampled, with dark sky background, FP1 and FP3 only 03:25 - 04:00 Global FP1 scan, Nyquist sampled, with partial dark sky background (Saturn will be in the background much of the time), FP1 and FP3 only. 04:00 - 04:15 N/S FP3/4 scan, 6 murad/sec, centered on 180 W, 50 N, to look for warm fractures. Solar occultation egress is at 04:16, so after that we need to worry about solar avoidance. 04:16 - 04:30 N/S FP1/FP3 scan at 12 murad/sec near the anti-sun (left) limb (to minimize solar phase angle), if we can without violating sun avoidance constraints. ---------------- Rate multiplier assumes we use FP3 and FP1 thoughout, but use of FP4 for only about half of this observation. Exact times for FP4 use are TBD.",,,,,, 2010-097T01:45:11,000T02:46:00,7-Apr-10,UVIS,SPASS Rider,Dione,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2010-097T01:45:11,000T02:46:00,7-Apr-10,VIMS,SPASS Rider,Dione,ECLIPSE,,Dione Eclipse,multiple 16/640 ms.,,,,,, 2010-097T03:16:02,000T04:00:00,7-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-097T03:16:11,000T04:00:00,7-Apr-10,MAG,Non-SPASS,Dione,DITAR,Dione targeted flyby,D5 flyby,Monitor magnetic field perturbations and waves to confirm evidence of plasma pickup observed during the sole previous upstream Dione flyby.,,,,,, 2010-097T04:16:11,000T02:00:00,7-Apr-10,CAPS,SPASS Rider,Dione,ENCOUNTER,MAPS Campaign,MAPS 129DI Campaign,Part of 049RH MAPS Campaign. Observe interaction between Rhea and Saturn's magnetosphere,,,,,, 2010-097T04:25:41,000T01:41:00,7-Apr-10,RPWS,Non-SPASS,Dione,DICA,,RPWS Dione closest approach observations,"Make high resolution RPWS observations of the magnetosphere - Dione interaction using WBR, WFR, and LP.",,,,,, 2010-097T04:31:11,000T01:00:00,7-Apr-10,CAPS,Prime,Dione,DIONEPTG,Dione observation,MAPS 129DI Campaign,Part of 129DI MAPS Campaign. Observe interaction between Dione and Saturn's magnetosphere,,,,,, 2010-097T04:31:11,000T01:00:00,7-Apr-10,ISS,SPASS Rider,Dione,DIONEPTG,Dione observation,Dione highest-res. snapshots,Shutter along surface,,,,,, 2010-097T04:31:11,000T01:00:00,7-Apr-10,VIMS,SPASS Rider,Dione,CLOSAPPR,,Dione close approach,multiple 16/640 ms.,,,,,, 2010-097T04:46:02,000T01:00:00,7-Apr-10,MIMI,SPASS Rider,Dione,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-097T04:53:11,000T00:46:00,7-Apr-10,INMS,Non-SPASS,Dione,DIONE,Dione,Dione Flyby,Dione observation,,,,,, 2010-097T05:01:46,000T02:00:00,7-Apr-10,CDA,SPASS Rider,DustRAM direction,RPX0080,,CDA RPXing 2010-097T06:01:46,RPXing at 5.9048159 Rs,,,,,, 2010-097T05:06:11,000T00:15:00,7-Apr-10,CIRS,SPASS Rider,Dione,DIONEPTG,Dione observation,CIRS_129DI_DIONEPTG001_CAPS;,"CIRS drag across Dione near close approach in CAPS attitude, for 10 minutes before C/A (allowing for shutter-closed time) and 5 minutes afterwards.",,,,,, 2010-097T05:15:11,000T00:04:00,7-Apr-10,UVIS,SPASS Rider,Dione,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV.,,,,,, 2010-097T05:31:11,000T01:00:00,7-Apr-10,UVIS,Prime,Dione,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV.,,,,,, 2010-097T05:31:11,000T01:00:00,7-Apr-10,CIRS,SPASS Rider,Dione,ICYMAP,Icy satellite surface map,CIRS_129DI_ICYMAP002_UVIS,Ride with UVIS,,,,,, 2010-097T05:31:11,000T01:00:00,7-Apr-10,ISS,SPASS Rider,Dione,ICYMAP,Icy satellite surface map,Dione high-res. snapshots,Shutter while UVIS scans,,,,,, 2010-097T05:31:11,000T01:00:00,7-Apr-10,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione Eclipse,multiple 16/640 ms.,,,,,, 2010-097T05:39:11,000T15:52:39,7-Apr-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-097T05:46:02,001T04:17:58,7-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-097T06:06:11,000T00:53:49,7-Apr-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-097T06:16:11,000T03:47:49,7-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-097T06:31:11,000T01:45:00,7-Apr-10,ISS,Prime,Dione,REGMAP,Regional mapping,Dione sub-Saturn hemisphere mapping,1st hour: Do 21-panel mosaic; last 40 min: do central sit'n'stare.,,,,,, 2010-097T06:31:11,000T01:45:00,7-Apr-10,CIRS,SPASS Rider,Dione,REGMAP,Regional mapping,CIRS_129DI_REGMAP001_ISS,"Ride with ISS, FP1 and FP3 only",,,,,, 2010-097T06:31:11,000T01:45:00,7-Apr-10,UVIS,SPASS Rider,Dione,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-097T07:01:11,000T01:45:00,7-Apr-10,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,multiple 16/640 ms.,,,,,, 2010-097T07:16:11,000T02:05:48,7-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-097T08:31:10,000T01:20:00,7-Apr-10,VIMS,Prime,Dione,DIONE,Dione,Dione,multiple 16/640 ms.,,,,,, 2010-097T08:31:10,000T01:20:00,7-Apr-10,CIRS,SPASS Rider,Dione,DIONE,Dione,CIRS_129DI_DIONE001_VIMS,"Ride with VIMS, FP1 and FP3 only. 3 cm-1 spectral resolution. Shutter closed for the final 5 minutes.",,,,,, 2010-097T08:31:10,000T01:20:00,7-Apr-10,ISS,SPASS Rider,Dione,DIONE,Dione,Dione multi color,Sit'n'stare,,,,,, 2010-097T08:31:10,000T01:20:00,7-Apr-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-097T09:21:59,000T07:35:36,7-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-097T09:21:59,000T07:03:00,7-Apr-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-097T09:51:10,000T01:08:50,7-Apr-10,CIRS,Prime,Dione,FP3DAYMAP,CIRS FP3 daytime map,CIRS_129DI_FP3DAYMAP001_PRIME;,"Daytime FP3 global scan. Shutter closed during the final 3 minutes. Begin the observation at 3 cm-1, continuing from the previous VIMS rider, and obtain 2 minutes of dark sky at 3 cm-1 for calibration of that rider before switching to 15 cm-1 for the remainder of the observation, and beginning the FP3 scan.",,,,,, 2010-097T09:51:10,000T01:08:50,7-Apr-10,ISS,SPASS Rider,Dione,FP3DAYMAP,CIRS FP3 daytime map,Dione global snapshot,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-097T09:51:10,000T01:08:50,7-Apr-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-097T09:51:10,000T01:08:50,7-Apr-10,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,multiple 16/640 ms.,,,,,, 2010-097T10:04:00,000T12:18:30,7-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-097T11:00:00,000T01:30:00,7-Apr-10,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2010-097T11:00:00,000T01:30:00,7-Apr-10,CIRS,SPASS Rider,Enceladus,PLMHRHP,,CIRS_129EN_PLMHRHP002_ISS,"Ride with ISS, FP1 and FP3 only",,,,,, 2010-097T11:00:00,000T01:30:00,7-Apr-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-097T11:00:00,000T01:30:00,7-Apr-10,VIMS,SPASS Rider,Dione,PLMHRMP,,Dione,multiple 16/640 ms.,,,,,, 2010-097T11:46:42,000T04:00:00,7-Apr-10,MAG,Non-SPASS,Mimas,MITAR,,M3 flyby,"Monitor the interaction of Mimas with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD request.",,,,,, 2010-097T12:30:00,000T01:30:00,7-Apr-10,VIMS,SPASS Rider,Janus,ROTCOLR,,Janus,multiple 16/640 ms.,,,,,, 2010-097T12:53:14,000T00:00:01,7-Apr-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.525 Rs, lat = -0 deg, phase = 80 deg",,,,,, 2010-097T12:57:35,000T03:27:24,7-Apr-10,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE5 flyby,"Monitor the interaction of Tethys with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD & MITAR requests.",,,,,, 2010-097T13:30:00,000T02:15:00,7-Apr-10,ISS,Prime,Janus,ROTCOLR,,Janus,Janus and Epimetheus,,,,,, 2010-097T13:30:00,000T02:15:00,7-Apr-10,CIRS,SPASS Rider,Janus,ROTCOLR,,CIRS_129JA_ROTCOLR003_ISS,"Ride with ISS, FP1 and FP3 only",,,,,, 2010-097T13:30:00,000T02:15:00,7-Apr-10,UVIS,SPASS Rider,Janus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-097T14:00:00,000T03:20:00,7-Apr-10,VIMS,SPASS Rider,Dione,PLMHRMP,,Dione,multiple 16/640 ms.,,,,,, 2010-097T15:45:00,000T01:35:00,7-Apr-10,ISS,Prime,Enceladus,PLMHRMP,,High res plume obs at medium phase,High resolution plume observation at high phase,,,,,, 2010-097T15:45:00,000T01:35:00,7-Apr-10,CIRS,SPASS Rider,Enceladus,PLMHRMP,,CIRS_129EN_PLMHRMP001_ISS,"Ride with ISS, FP3 and FP1 only",,,,,, 2010-097T15:45:00,000T01:35:00,7-Apr-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-097T16:24:59,000T00:32:36,7-Apr-10,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE5 flyby,Monitor the interaction of Tethys with the Saturnian magnetosphere.,,,,,, 2010-097T16:57:35,000T01:02:25,7-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-097T18:00:00,000T16:04:00,7-Apr-10,RSS,SPASS Rider,Dione,KADOWN,RSS Ka-Band downlink,GSE pass for Dione's mass,Downlink pass at Ka-band for Dione's mass determination and for improving locally Cassini orbit.,,,,,, 2010-097T18:00:00,000T16:04:00,7-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-097T21:30:00,000T02:00:00,7-Apr-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-097T21:31:50,000T02:00:00,7-Apr-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-097T21:33:46,000T02:00:00,7-Apr-10,CDA,SPASS Rider,DustRAM direction,RPX0090,,CDA RPXing 2010-097T22:33:46,RPXing at 7.2764710 Rs,,,,,, 2010-097T22:22:30,000T17:57:30,7-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-097T23:31:50,000T10:32:10,7-Apr-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-098T02:04:46,000T17:00:00,8-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0072932 Rs exit= 15.997996 Range altitude= 716.56776 km ... 3730.0188,,,,,, 2010-098T03:00:00,000T07:04:00,8-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-098T04:00:00,000T06:04:00,8-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10098_SP,rider,,,,,, 2010-098T10:04:00,000T06:16:00,8-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-098T10:04:00,000T12:27:50,8-Apr-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-098T10:04:00,000T06:16:00,8-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-098T10:04:00,000T06:16:00,8-Apr-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-098T10:04:00,000T06:17:30,8-Apr-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-098T10:44:00,000T03:01:00,8-Apr-10,UVIS,Prime,Star,BETCMA,,Saturn Occults Beta Cma,Both ingress and egress desired,,,,,, 2010-098T13:45:00,000T01:15:00,8-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-098T15:00:00,000T01:15:00,8-Apr-10,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 27.4 range 2 Mkm",,,,,, 2010-098T15:00:00,000T01:15:00,8-Apr-10,CIRS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-098T15:00:00,000T01:15:00,8-Apr-10,UVIS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-098T16:15:00,000T07:00:00,8-Apr-10,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2010-098T16:20:00,001T09:00:00,8-Apr-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-098T16:20:00,001T09:00:00,8-Apr-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-098T16:20:00,001T09:00:00,8-Apr-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-098T16:20:00,001T09:00:00,8-Apr-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-098T16:21:30,009T00:58:30,8-Apr-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-098T19:04:46,008T22:15:14,8-Apr-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.009977 Rs exit= 16.003958 Range altitude= 3735.2780 km ... 1014.5381,,,,,, 2010-098T22:31:50,000T07:28:10,8-Apr-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-098T23:15:00,000T00:30:00,8-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-098T23:45:00,000T00:39:00,8-Apr-10,ISS,Prime,Prometheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Prometheus across Rhea","Images of mutual event, transit of Prometheus across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-099T01:04:00,000T09:00:00,9-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-099T02:04:00,000T08:00:00,9-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10099_SP,rider,,,,,, 2010-099T06:00:00,000T02:00:00,9-Apr-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-099T08:00:00,001T18:19:00,9-Apr-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-099T10:44:00,000T01:15:00,9-Apr-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 51.2 range 2.4 Mkm",,,,,, 2010-099T10:44:00,000T01:15:00,9-Apr-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-099T10:44:00,000T01:15:00,9-Apr-10,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-099T11:59:00,000T00:30:00,9-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-099T12:29:00,000T12:00:00,9-Apr-10,VIMS,Prime,rings(general),EG60PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. MAG segment.,,,,,, 2010-100T00:29:00,000T00:30:00,10-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-100T00:59:00,000T00:55:00,10-Apr-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Titan","Images of mutual event, transit of Dione across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-100T01:20:00,002T03:35:00,10-Apr-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-100T01:20:00,002T03:35:00,10-Apr-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-100T01:20:00,002T03:24:00,10-Apr-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-100T01:54:00,000T14:00:00,10-Apr-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-100T15:54:00,000T00:45:00,10-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-100T17:19:00,000T09:00:00,10-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-100T18:19:00,000T08:00:00,10-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10100_SP,rider,,,,,, 2010-101T02:19:00,001T00:00:00,11-Apr-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-101T02:59:00,000T00:39:00,11-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-101T03:38:00,000T00:41:00,11-Apr-10,ISS,Prime,Epimetheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Epimetheus across Janus","Images of mutual event, transit of Epimetheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-101T04:19:00,000T01:15:00,11-Apr-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 76.5 range 3.1 Mkm",,,,,, 2010-101T04:19:00,000T01:15:00,11-Apr-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-101T04:19:00,000T01:15:00,11-Apr-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-101T05:34:00,000T10:35:00,11-Apr-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-101T16:09:00,000T00:30:00,11-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-101T17:19:00,000T11:36:00,11-Apr-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-101T17:19:00,000T09:00:00,11-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-101T18:19:00,000T08:00:00,11-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10101_SP,rider,,,,,, 2010-102T02:19:00,004T07:41:00,12-Apr-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-102T02:59:00,000T01:15:00,12-Apr-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 88 range 3.3 Mkm",,,,,, 2010-102T02:59:00,000T01:15:00,12-Apr-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-102T02:59:00,000T01:15:00,12-Apr-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-102T04:14:00,000T00:30:00,12-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-102T04:44:00,001T01:40:00,12-Apr-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-102T04:44:00,000T18:55:00,12-Apr-10,CAPS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-102T04:55:00,011T00:40:00,12-Apr-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-102T04:55:00,005T12:26:00,12-Apr-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-102T04:55:00,000T18:44:00,12-Apr-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-102T04:55:00,002T21:08:00,12-Apr-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-103T06:24:00,009T23:11:00,13-Apr-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-103T07:04:00,000T09:00:00,13-Apr-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev130 Saturn atmospheric occultation on 2010/117 and Rev130 Enceladus gravity observation on 2010/117-118.",,,,,, 2010-103T07:04:00,000T09:00:00,13-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-103T08:04:00,000T08:00:00,13-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10103_SP,rider,,,,,, 2010-103T16:44:00,000T23:39:00,13-Apr-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_129SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-104T16:23:00,000T10:20:00,14-Apr-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-104T17:03:00,000T09:00:00,14-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-104T18:03:00,000T08:00:00,14-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10104_SP,rider,,,,,, 2010-105T00:00:00,000T00:34:00,15-Apr-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-105T02:43:00,000T00:30:00,15-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 020 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-105T03:13:00,000T15:10:00,15-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-105T18:23:00,000T05:00:00,15-Apr-10,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_129_SCATTERED_SUNLIGHT_TEST_PRIME,"Sunlight falling on the CIRS telescope can potentially be scattered into the instrument by mirror imperfections. We need to quantify the effect of ring particle impacts on the mirror performance. This requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; continuous radial scans are required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scans will begin 40 degrees from FPB, and will scan to 10 degrees of FPB at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time VIMS will integrate for TBD seconds and CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction back to the initial position; to determine whether scattering is asymmetric with respect to the FPB axis, 3 such scans will be made. 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from 40 degrees +Z to 10 degrees +Z and back to 40 degrees +Z. 2) From 40 degrees in -X on the X axis, to 10 degrees on the -X axis, to 40 degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 10 degrees -Z and back to 40 degrees -Z.",,,,,, 2010-105T23:23:00,000T00:30:00,15-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 022 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-106T00:33:00,000T09:00:00,16-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-106T01:33:00,000T08:00:00,16-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10106_SP,rider,,,,,, 2010-106T10:00:00,000T00:05:00,16-Apr-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,IEB load,,,,,, 2010-106T10:05:00,000T00:33:00,16-Apr-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,MRO,,,,,, 2010-106T10:13:00,000T00:30:00,16-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 024 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-106T10:38:00,000T01:22:00,16-Apr-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-106T10:43:00,000T09:55:00,16-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-106T12:00:00,001T05:21:00,16-Apr-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-106T20:18:00,000T07:00:00,16-Apr-10,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-25 in 1-way mode.,,,,,, 2010-106T20:38:00,000T03:00:00,16-Apr-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Albiorix,Observation of Albiorix,,,,,, 2010-106T20:38:00,000T03:00:00,16-Apr-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-107T00:18:00,000T09:00:00,17-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-107T01:18:00,000T08:00:00,17-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_129IC_DSCAL10107_SP,rider,,,,,, 2010-107T09:58:00,000T00:30:00,17-Apr-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 027 TH OBS SET IN REV 12","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-107T10:28:00,000T09:32:00,17-Apr-10,ISS,Prime,RingE,LRLEMP,,Edge on obs around/after Eqx.,"Low res, low elev., high-phase of E ring",,,,,, 2010-107T17:20:00,008T07:58:00,17-Apr-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.009977 Rs exit= 16.003958 Range altitude= 3735.2780 km ... 1014.5381,,,,,, 2010-107T17:20:00,009T00:54:00,17-Apr-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-107T17:20:00,001T22:13:00,17-Apr-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-107T17:20:49,000T00:00:01,17-Apr-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.4 d, inc = 0.3 deg, r = 44.158 Rs, phase = 100 deg",,,,,, 2010-107T17:21:00,005T12:14:00,17-Apr-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-107T17:21:00,000T22:12:00,17-Apr-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-107T20:00:00,000T06:53:00,17-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-108T02:53:00,000T03:00:00,18-Apr-10,ISS,Prime,Other,OUTERSATS,Icy satellite observaton,Bebhionn,Observation of Bebhionn,,,,,, 2010-108T02:53:00,000T03:00:00,18-Apr-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-108T06:33:00,000T09:00:00,18-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-108T07:33:00,000T08:00:00,18-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10108_SP,rider,,,,,, 2010-108T15:33:00,001T00:00:00,18-Apr-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-108T16:13:00,000T07:00:00,18-Apr-10,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observation of 1 of 3 IR stars: CW Leonis, Eta Carinae, Alpha Orionis. Slew to star; settle; execute small box scan; return to waypoint. Observation of each star to take 6 hours; need not be executed contiguously.",,,,,, 2010-108T16:13:00,000T07:00:00,18-Apr-10,ISS,SPASS Rider,Other,1STAROBS,Stellar spectroscopy,ISS NAC dark current calibration,ISS NAC dark current calibration,,,,,, 2010-108T23:13:00,000T06:40:00,18-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-109T06:33:00,000T09:00:00,19-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-109T07:33:00,000T08:00:00,19-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10109_SP,rider,,,,,, 2010-109T15:33:00,005T09:45:00,19-Apr-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-109T15:33:00,003T14:02:00,19-Apr-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-109T16:13:00,000T22:16:00,19-Apr-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_130SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-110T14:29:00,000T00:59:00,20-Apr-10,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Titan across Dione","Images of mutual event, transit of Titan across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-110T15:28:00,000T07:55:00,20-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-111T00:03:00,000T09:00:00,21-Apr-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev130 Saturn atmospheric occultation on 2010/117 and Rev130 Enceladus gravity observation on 2010/117-118.",,,,,, 2010-111T00:03:00,000T09:00:00,21-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-111T01:03:00,000T08:00:00,21-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10111_SP,rider,,,,,, 2010-111T09:43:00,000T01:15:00,21-Apr-10,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 90 range 1.3 Mkm",,,,,, 2010-111T09:43:00,000T01:15:00,21-Apr-10,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-111T09:43:00,000T01:15:00,21-Apr-10,UVIS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-111T10:58:00,000T12:25:00,21-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-112T00:03:00,000T09:00:00,22-Apr-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev130 Saturn atmospheric occultation on 2010/117.",,,,,, 2010-112T00:03:00,000T09:00:00,22-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-112T01:03:00,000T08:00:00,22-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10112_SP,rider,,,,,, 2010-112T09:43:00,000T01:15:00,22-Apr-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 82 range 1.5 Mkm",,,,,, 2010-112T09:43:00,000T01:15:00,22-Apr-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-112T09:43:00,000T01:15:00,22-Apr-10,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-112T10:58:00,000T12:25:00,22-Apr-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-113T00:03:00,000T09:00:00,23-Apr-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev130 Saturn atmospheric occultation on 2010/117 and Rev130 Enceladus gravity observation on 2010/117-118.",,,,,, 2010-113T00:03:00,000T09:00:00,23-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-113T01:03:00,000T08:00:00,23-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10113_SP,rider,,,,,, 2010-113T05:35:00,002T03:35:00,23-Apr-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-113T05:35:00,002T03:35:00,23-Apr-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-113T05:35:00,002T03:35:00,23-Apr-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-113T05:35:00,000T10:58:00,23-Apr-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-113T09:43:00,000T01:15:00,23-Apr-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 80.5 range 1.7 Mkm",,,,,, 2010-113T09:43:00,000T01:15:00,23-Apr-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-113T09:43:00,000T01:15:00,23-Apr-10,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-113T10:58:00,000T04:55:00,23-Apr-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-113T16:33:00,001T16:37:00,23-Apr-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-113T16:33:00,000T09:00:00,23-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-113T17:33:00,000T08:00:00,23-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10513_SP,rider,,,,,, 2010-114T02:13:00,000T01:15:00,24-Apr-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 82.1 range 1.9 Mkm",,,,,, 2010-114T02:13:00,000T01:15:00,24-Apr-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-114T02:13:00,000T01:15:00,24-Apr-10,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-114T03:28:00,000T12:10:00,24-Apr-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-114T16:18:00,000T09:00:00,24-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-114T17:18:00,000T08:00:00,24-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10114_SP,rider,,,,,, 2010-115T01:18:00,001T00:00:00,25-Apr-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-115T01:58:00,000T07:40:00,25-Apr-10,VIMS,Prime,rings(general),EG130PHAS,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. MAG segment. Do 3 of 9 EG130 phase at priority 2.,,,,,, 2010-115T09:10:00,000T16:08:00,25-Apr-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-115T09:10:00,000T13:50:00,25-Apr-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-115T09:10:00,000T13:50:00,25-Apr-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-115T09:10:00,000T13:50:00,25-Apr-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-115T09:38:00,000T06:00:00,25-Apr-10,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2010-115T16:18:00,000T09:00:00,25-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-115T17:18:00,000T08:00:00,25-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10115_SP,rider,,,,,, 2010-115T23:00:00,000T19:10:00,25-Apr-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-115T23:00:00,000T02:18:00,25-Apr-10,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2010-116T01:18:00,000T15:52:00,26-Apr-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-116T01:18:00,000T14:12:46,26-Apr-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.009977 Rs exit= 16.003958 Range altitude= 3735.2780 km ... 1014.5381,,,,,, 2010-116T01:18:00,000T01:12:00,26-Apr-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-116T01:18:00,000T16:52:00,26-Apr-10,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2010-116T01:58:00,000T15:12:00,26-Apr-10,CAPS,Prime,Saturn,SURVEYPTG,MAPS survey/Prime pointing,MAPS Survey w/ prime pointing,null,,,,,, 2010-116T02:30:00,000T02:00:00,26-Apr-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-116T04:30:00,000T19:41:46,26-Apr-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-116T15:30:46,000T16:16:14,26-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-116T17:10:00,000T04:00:00,26-Apr-10,CIRS,Prime,Saturn,NADIROCC,Occultation,NADIROCC egress or ingress,"Helium abundance measurement at the RSS egress occultation point. If RSS request deleted, this can be, too. IF RSS observes both ingress & egress, the NADIROCC that best fits the timeline can be chosen",,,,,, 2010-116T17:10:00,000T07:36:00,26-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-116T18:10:00,000T13:37:00,26-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-116T18:10:00,000T13:37:00,26-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-116T18:14:00,000T13:33:00,26-Apr-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-116T21:10:00,000T01:55:00,26-Apr-10,ISS,Prime,Enceladus,PLMMRHP,,Medium res plume obs at high phase,Medium resolution plume observation at high phase,,,,,, 2010-116T23:45:00,000T08:02:00,26-Apr-10,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' gravity,Additional downlink pass at Ka-band for Enceladus' gravity science and for improving locally Cassini orbit.,,,,,, 2010-116T23:45:00,000T08:02:00,26-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-117T00:11:46,000T02:00:00,27-Apr-10,CDA,SPASS Rider,DustRAM direction,RPX0100,,CDA RPXing 2010-117T01:11:46,RPXing at 12.261367 Rs,,,,,, 2010-117T00:11:46,000T02:00:00,27-Apr-10,INMS,Non-SPASS,Saturn,RINGPLN,,"Ring Plane Crossing, riding with",Inner magnetospheric survey,,,,,, 2010-117T00:45:00,000T03:30:00,27-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10116_SP,rider,,,,,, 2010-117T00:46:00,000T07:01:00,27-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-117T02:11:46,000T06:36:14,27-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-117T05:42:00,000T02:05:00,27-Apr-10,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS Thermal Stabilization 130 pre-Occ,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2010-117T07:47:00,000T01:35:00,27-Apr-10,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS Atmospheric Occultation 130 in,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-117T07:47:00,000T05:24:00,27-Apr-10,CAPS,SPASS Rider,Saturn,TRINGSAT,,Rings and Satellites,null,,,,,, 2010-117T07:47:00,000T15:23:17,27-Apr-10,CAPS,SPASS Rider,Saturn,WRINGSAT,,Rings and Satellites,null,,,,,, 2010-117T07:47:00,000T15:54:36,27-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-117T07:47:00,000T06:13:00,27-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-117T07:47:00,000T10:22:59,27-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-117T07:47:00,001T17:16:00,27-Apr-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-117T08:48:00,000T13:22:17,27-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-117T09:22:00,000T00:48:00,27-Apr-10,ISS,Prime,Enceladus,TPLMSECL,,High res plume obs at highest phase while s/c in e,High resolution plume observation at highest phase while s/c in eclipse,,,,,, 2010-117T09:22:00,000T02:24:00,27-Apr-10,RSS,Prime,Enceladus,WTHERMAL,,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2010-117T09:22:00,000T00:48:00,27-Apr-10,CIRS,SPASS Rider,Enceladus,TPLUME,,CIRS_121EN_TPLUME_ISS1;,,,,,,, 2010-117T09:22:00,000T02:24:00,27-Apr-10,RSS,SPASS Rider,Enceladus,TTHERMAL,,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2010-117T09:22:00,000T00:48:00,27-Apr-10,UVIS,SPASS Rider,Enceladus,TICYPLU,,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-117T10:10:00,000T01:36:00,27-Apr-10,UVIS,Prime,Enceladus,TICYECL,,ICYECL: Icy satellite eclipse volatile activity,Look for aruroa. Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background. Use ISSNAC to point in order to get both FUV and EUV.,,,,,, 2010-117T10:10:00,000T01:36:00,27-Apr-10,CIRS,SPASS Rider,Enceladus,TICYECL,,CIRS_121EN_TICYECL_UVIS;,,,,,,, 2010-117T10:10:00,000T01:36:00,27-Apr-10,ISS,SPASS Rider,Enceladus,TICYECL,,Enceladus observation,Enceladus RIDER,,,,,, 2010-117T10:10:00,000T01:36:00,27-Apr-10,VIMS,SPASS Rider,Saturn,ENFLUXTUB,,Enceladus,multiple 160/640 ms. search for enceladus flux tube footprint on Saturn,,,,,, 2010-117T11:46:00,000T02:14:00,27-Apr-10,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Atmospheric Occultation 130 out,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-117T13:11:00,000T09:59:17,27-Apr-10,CAPS,SPASS Rider,Saturn,TRINGSAT,,Rings and Satellites,null,,,,,, 2010-117T14:00:00,000T06:07:00,27-Apr-10,ISS,Prime,Enceladus,TPLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase ISS_130EN_PLMHRHP002_PRIME has been incoporated for one long observation,,,,,, 2010-117T14:00:00,001T02:03:00,27-Apr-10,RSS,Prime,Enceladus,WGRAVITY,,RSS Enceladus' Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2010-117T14:00:00,000T06:07:00,27-Apr-10,CIRS,SPASS Rider,Enceladus,TPLUME,,CIRS_121EN_TPLUME_ISS1;,,,,,,, 2010-117T14:00:00,000T06:07:00,27-Apr-10,UVIS,SPASS Rider,Enceladus,TICYPLU,,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-117T14:00:00,000T06:07:00,27-Apr-10,VIMS,SPASS Rider,Enceladus,TENCEL,,Enceladus,multiple 160/640 ms.,,,,,, 2010-117T14:00:00,000T00:15:00,27-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-117T14:15:00,000T05:52:00,27-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-117T17:12:17,000T03:00:00,27-Apr-10,RADAR,Non-SPASS,Other,WARMUP4EN,RADAR warmup,Warmup 4,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2010-117T18:09:59,000T08:01:37,27-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-117T18:09:59,000T07:02:00,27-Apr-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-117T18:10:17,000T05:00:00,27-Apr-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-117T20:07:00,000T03:27:00,27-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-117T20:12:17,000T03:21:00,27-Apr-10,RADAR,Prime,Enceladus,TSCATTRAD,,Scatterometry/Radiometry of EN,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2010-117T21:41:00,000T00:00:01,27-Apr-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.529 Rs, lat = -0 deg, phase = 81 deg",,,,,, 2010-117T22:10:17,000T01:24:00,27-Apr-10,INMS,Non-SPASS,Enceladus,ENCEL9,,Enceladus encounter,Enceladus observation,,,,,, 2010-117T23:10:17,000T02:00:00,27-Apr-10,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 121EN Campaign,Part of 121EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2010-117T23:10:17,000T02:00:00,27-Apr-10,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2010-117T23:34:00,000T01:06:00,27-Apr-10,VIMS,SPASS Rider,Enceladus,TENCDRAG,,Enceladus,"for about 90sec, enceladus drifts across field of view",,,,,, 2010-117T23:34:00,000T03:36:00,27-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-117T23:34:17,000T01:06:00,27-Apr-10,INMS,Prime,Enceladus,TRAMPNT,,Enceladus encounter,Enceladus observation,,,,,, 2010-117T23:34:17,000T01:06:00,27-Apr-10,INMS,Non-SPASS,Enceladus,WENCEL9,,Enceladus encounter,Enceladus observation,,,,,, 2010-117T23:41:36,000T01:00:00,27-Apr-10,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-118T00:03:17,000T00:10:00,28-Apr-10,CIRS,SPASS Rider,Enceladus,TRAMPNT,,CIRS_121EN_ TRAMPNT001;,"10 minutes around c/a, for ORS drag at c/a (FOV is on Enceladus for 78 seconds, but we need baseline on either side too). Shutter closed for the first 3 minutes",,,,,, 2010-118T00:09:17,000T00:02:00,28-Apr-10,ISS,SPASS Rider,Enceladus,TRAMPNT,,Enceladus observation,Enceladus rider,,,,,, 2010-118T00:09:17,000T00:02:00,28-Apr-10,UVIS,SPASS Rider,Enceladus,TICYMAP,,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-118T00:15:00,000T03:00:00,28-Apr-10,RADAR,Non-SPASS,Other,WARMUP4RH,RADAR warmup,Warmup 4 RH,Warmup for scatterometry and simultaneous radiometry of icy satellite.,,,,,, 2010-118T00:23:46,000T02:00:00,28-Apr-10,CDA,SPASS Rider,DustRAM direction,RPX0110,,CDA RPXing 2010-118T01:23:46,RPXing at 4.4071604 Rs,,,,,, 2010-118T00:40:17,000T00:22:00,28-Apr-10,CIRS,SPASS Rider,Enceladus,TSPDRIFT,,CIRS_130EN_TSPDRIFT_ENGR;,Designed to drift across the south polar region during the RCS/RWA transition,,,,,, 2010-118T00:40:17,000T00:22:00,28-Apr-10,ISS,SPASS Rider,Enceladus,TRADWBIAS,,Enceladus observation,Enceladus rider,,,,,, 2010-118T00:40:17,000T00:22:00,28-Apr-10,UVIS,SPASS Rider,Enceladus,TICYLON,,,Map uv albedo,,,,,, 2010-118T00:40:17,000T00:22:00,28-Apr-10,VIMS,SPASS Rider,Enceladus,TENCEL,,Enceladus,multiple 160/640 ms.,,,,,, 2010-118T00:40:17,000T01:30:00,28-Apr-10,INMS,Non-SPASS,Enceladus,ENCEL9,,Enceladus encounter,Enceladus observation,,,,,, 2010-118T00:41:36,001T00:28:24,28-Apr-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-118T01:02:17,000T00:38:00,28-Apr-10,ISS,Prime,Enceladus,TGEOLG,,Enceladus observation,Enceladus mosaic,,,,,, 2010-118T01:02:17,000T00:38:00,28-Apr-10,CIRS,SPASS Rider,Enceladus,TGEOLG,,CIRS_121EN_TGEOLG_ISS1;,,,,,,, 2010-118T01:02:17,000T00:38:00,28-Apr-10,UVIS,SPASS Rider,Enceladus,TICYLON,,,Map uv albedo,,,,,, 2010-118T01:02:17,000T00:38:00,28-Apr-10,VIMS,SPASS Rider,Enceladus,TENCEL,,Enceladus,multiple 160/640 ms.,,,,,, 2010-118T01:10:17,000T23:52:43,28-Apr-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-118T01:10:17,000T01:09:43,28-Apr-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-118T01:11:59,000T00:58:18,28-Apr-10,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2010-118T01:40:17,000T01:30:00,28-Apr-10,UVIS,Prime,Enceladus,TICYLON,,Investigate volatiles near Enceladus,"Long stare for tenuous atmosphere search, absorption signature with Saturn as source. Enceladus is transiting in front of Saturn.",,,,,, 2010-118T01:40:17,000T01:30:00,28-Apr-10,CIRS,SPASS Rider,Enceladus,TICYLON,,CIRS_130EN_TICYLON001_UVIS;,,,,,,, 2010-118T01:40:17,000T01:30:00,28-Apr-10,ISS,SPASS Rider,Enceladus,TICYLON,,Enceladus observation,Enceladus rider,,,,,, 2010-118T01:40:17,000T01:30:00,28-Apr-10,VIMS,SPASS Rider,Enceladus,TENCEL,,Enceladus,multiple 160/640 ms.,,,,,, 2010-118T02:10:17,000T22:52:42,28-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-118T02:10:17,000T22:52:43,28-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-118T02:20:00,000T04:00:00,28-Apr-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-118T03:10:00,000T02:23:00,28-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-118T03:15:00,000T02:18:00,28-Apr-10,RADAR,Prime,Rhea,TSCATTRAD,,130RH,Point -Z axis at target and execute raster scan(s) centered on target. Obtain simultaneous scatterometry and radiometry.,,,,,, 2010-118T05:33:00,000T05:19:46,28-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.991973 Rs exit= 9.0149540 Range altitude= 1011.1205 km ... -758.54515,,,,,, 2010-118T05:33:00,000T03:11:00,28-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-118T08:44:00,000T02:16:00,28-Apr-10,VIMS,Prime,Enceladus,TLOWPHASE,,Enceladus,multiple 160/640 ms.,,,,,, 2010-118T08:44:00,000T02:16:00,28-Apr-10,CIRS,SPASS Rider,Enceladus,TLOPHASE,,CIRS_130EN_TLOPHASE001_UVIS;,"FP1, FP3 only",,,,,, 2010-118T08:44:00,000T02:16:00,28-Apr-10,ISS,SPASS Rider,Enceladus,TLOWPHAE,,Enceladus observation,Enceladus rider point-and-stare,,,,,, 2010-118T08:44:00,000T02:16:00,28-Apr-10,UVIS,SPASS Rider,Enceladus,TICYLON,,,Map uv albedo,,,,,, 2010-118T10:52:46,000T14:10:14,28-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0054693 Rs exit= 15.996677 Range altitude= 2610.2502 km ... 5668.0104,,,,,, 2010-118T11:00:00,000T03:18:00,28-Apr-10,VIMS,Prime,Rhea,TRHEA,,Enceladus,multiple 160/640 ms. 1x2 mosaic with long stares for VIMS+ISS,,,,,, 2010-118T11:00:00,000T03:18:00,28-Apr-10,CIRS,SPASS Rider,Rhea,TVIMS,,CIRS_130EN_TVIMS001_UVIS;,3 cm-1 spectral resolution,,,,,, 2010-118T11:00:00,000T03:18:00,28-Apr-10,ISS,SPASS Rider,Rhea,TRHEA,,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-118T11:00:00,000T03:18:00,28-Apr-10,UVIS,SPASS Rider,Rhea,TICYLON,,,Map uv albedo,,,,,, 2010-118T16:03:00,000T09:00:00,28-Apr-10,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' gravity,Additional downlink pass at Ka-band for Enceladus' gravity science and for improving locally Cassini orbit.,,,,,, 2010-118T16:03:00,000T10:00:00,28-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-118T17:03:00,000T08:00:00,28-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10118_SP,rider,,,,,, 2010-119T01:03:00,001T09:02:00,29-Apr-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-119T01:03:00,000T01:14:00,29-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0054693 Rs exit= 15.996677 Range altitude= 2610.2502 km ... 5668.0104,,,,,, 2010-119T01:03:00,000T13:44:00,29-Apr-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-119T01:03:00,000T00:07:00,29-Apr-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-119T01:03:00,009T02:01:00,29-Apr-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-119T01:10:00,001T08:55:00,29-Apr-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-119T01:10:00,001T08:55:00,29-Apr-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-119T01:10:00,001T08:55:00,29-Apr-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-119T02:17:00,000T01:35:46,29-Apr-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0054693 Rs exit= 15.996677 Range altitude= 2610.2502 km ... 5668.0104,,,,,, 2010-119T02:18:00,000T02:49:00,29-Apr-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 001,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-119T02:18:00,000T02:49:00,29-Apr-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.",,,,,, 2010-119T03:52:46,008T23:11:14,29-Apr-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.008660 Rs exit= 16.001753 Range altitude= 5672.8320 km ... 4110.1690,,,,,, 2010-119T06:47:00,000T08:00:00,29-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10119_SP,rider,,,,,, 2010-119T14:47:00,001T00:00:00,29-Apr-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-119T15:27:00,000T11:00:00,29-Apr-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 002,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-119T15:27:00,000T11:00:00,29-Apr-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie + NAC lightning search,"2x2 mosaic made of corners of VIMS 3x3 90-minute mosaics plus a central footprint of night side row of VIMS mosaic. Day side: WAC in MT3, CB3, CB2, MT2, and BL1. Night side: NAC CL1 images at 3 footprints, 13 images per 90 min.",,,,,, 2010-120T00:00:00,000T00:34:00,30-Apr-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-120T00:37:00,000T02:50:00,30-Apr-10,RADAR,SPASS Rider,Other,WU4NEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-120T02:27:00,000T01:00:00,30-Apr-10,ISS,Prime,Saturn,1X2WPH20,Photopolarimetry,WAC Saturn Photopol 20 Phase,Saturn WAC Photopolarimetry 20 Phase 1X2 mosaic,,,,,, 2010-120T03:27:00,000T01:40:00,30-Apr-10,RADAR,Prime,Titan,NEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2010-120T05:47:00,000T09:00:00,30-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-120T06:47:00,000T08:00:00,30-Apr-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10120_SP,rider,,,,,, 2010-120T10:05:00,002T03:25:00,30-Apr-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-120T10:05:00,002T03:25:00,30-Apr-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-120T10:05:00,002T03:25:00,30-Apr-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-120T10:05:00,002T03:25:00,30-Apr-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-120T14:47:00,007T04:13:00,30-Apr-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-120T15:27:00,000T07:25:00,30-Apr-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-120T23:32:00,000T09:00:00,30-Apr-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-121T00:32:00,000T08:00:00,1-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10121_SP,rider,,,,,, 2010-121T09:12:00,000T10:00:00,1-May-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_130SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-121T09:12:00,000T10:00:00,1-May-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Compsit ridealong with CIRS,CIRS ridealong,,,,,, 2010-121T19:12:00,000T03:25:00,1-May-10,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2010-121T19:12:00,000T03:25:00,1-May-10,ISS,SPASS Rider,rings(general),EG80PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2010-121T23:17:00,000T09:00:00,1-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-122T00:17:00,000T08:00:00,2-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10122_SP,rider,,,,,, 2010-122T08:57:00,000T04:50:00,2-May-10,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,Added 08/20/09: E-G phase observation. Can be shifted roughly +/- 1 day. SAT segment. Do 3 of 11 EG80 phase at priority 2.,,,,,, 2010-122T08:57:00,000T04:50:00,2-May-10,ISS,SPASS Rider,rings(general),EG80PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2010-122T13:30:00,011T03:10:00,2-May-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-122T13:30:00,005T13:34:00,2-May-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-122T13:30:00,000T19:27:00,2-May-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-122T13:30:00,002T02:17:00,2-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-122T13:47:00,000T06:00:00,2-May-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-122T19:47:00,000T02:50:00,2-May-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-122T23:17:00,000T09:00:00,2-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-123T00:17:00,000T08:00:00,3-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10123_SP,rider,,,,,, 2010-123T08:57:00,000T06:10:00,3-May-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-123T15:07:00,001T08:53:00,3-May-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-123T15:47:00,000T09:00:00,3-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-123T16:47:00,000T08:00:00,3-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10523_SP,rider,,,,,, 2010-124T01:27:00,000T12:00:00,4-May-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-124T13:27:00,000T02:20:00,4-May-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-124T13:27:00,000T02:20:00,4-May-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-124T15:47:00,002T13:30:00,4-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-124T15:47:00,000T09:00:00,4-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-124T16:47:00,000T08:00:00,4-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10124_SP,rider,,,,,, 2010-125T00:00:00,006T01:00:00,5-May-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-125T01:27:00,000T20:55:00,5-May-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_130SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-125T22:22:00,000T10:20:00,5-May-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-125T23:02:00,000T09:00:00,5-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-125T23:02:00,000T09:00:00,5-May-10,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev131 Enceladus gravity observation on 2010/137-138 and Rev131 Titan gravity observation on 2010/139.",,,,,, 2010-125T23:02:00,000T09:00:00,5-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-126T00:02:00,000T08:00:00,6-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10126_SP,rider,,,,,, 2010-126T08:42:00,000T01:15:00,6-May-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 81.4 range 1.5 Mkm",,,,,, 2010-126T08:42:00,000T01:15:00,6-May-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-126T08:42:00,000T01:15:00,6-May-10,UVIS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-126T09:57:00,000T11:15:00,6-May-10,ISS,Prime,Other,BEBHIONN,,Bebhionn rotation curve,Observation of outer satellite Bebhionn,,,,,, 2010-126T09:57:00,000T11:15:00,6-May-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-126T21:12:00,000T06:00:00,6-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-127T03:12:00,000T01:25:00,7-May-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-127T03:12:00,000T01:25:00,7-May-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-127T05:17:00,000T09:00:00,7-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-127T05:17:00,000T09:00:00,7-May-10,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev131 Enceladus gravity observation on 2010/137-138 and Rev131 Titan gravity observation on 2010/139.",,,,,, 2010-127T05:17:00,000T21:47:00,7-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-127T05:17:00,000T09:00:00,7-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-127T06:17:00,000T08:00:00,7-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_130IC_DSCAL10127_SP,rider,,,,,, 2010-127T14:57:00,000T23:19:00,7-May-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_130SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-127T14:57:00,000T23:13:00,7-May-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Compsit ridealong with CIRS,CIRS ridealong,,,,,, 2010-127T19:00:00,000T02:00:00,7-May-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-127T21:00:00,000T06:04:00,7-May-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-128T03:04:00,005T13:36:00,8-May-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-128T03:04:00,008T23:18:46,8-May-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.008660 Rs exit= 16.001753 Range altitude= 5672.8320 km ... 4110.1690,,,,,, 2010-128T03:04:00,001T20:56:00,8-May-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-128T03:04:00,009T02:01:00,8-May-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-128T03:04:00,001T19:42:00,8-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-128T03:04:17,000T00:00:01,8-May-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.5 d, inc = 0.3 deg, r = 44.288 Rs, phase = 99 deg",,,,,, 2010-128T15:16:00,000T09:00:00,8-May-10,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev131 Enceladus gravity observation on 2010/137-138 and Rev131 Titan gravity observation on 2010/139.",,,,,, 2010-128T15:16:00,000T09:00:00,8-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-128T16:16:00,000T08:00:00,8-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10128_SP,rider,,,,,, 2010-129T00:56:00,000T20:50:00,9-May-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_131SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-129T00:56:00,000T20:50:00,9-May-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Compsit ridealong with CIRS,CIRS ridealong,,,,,, 2010-129T22:46:00,000T09:00:00,9-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-129T22:46:00,000T09:00:00,9-May-10,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev131 Enceladus gravity observation on 2010/137-138 and Rev131 Titan gravity observation on 2010/139.",,,,,, 2010-129T22:46:00,001T06:15:00,9-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-129T22:46:00,000T09:00:00,9-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-129T23:46:00,000T08:00:00,9-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10129_SP,rider,,,,,, 2010-130T00:00:00,000T02:00:00,10-May-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-130T02:00:00,001T12:01:00,10-May-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-130T08:26:00,000T01:15:00,10-May-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 79.6 range 2.9 Mkm",,,,,, 2010-130T08:26:00,000T01:15:00,10-May-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-130T08:26:00,000T01:15:00,10-May-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-130T09:41:00,000T09:20:00,10-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-130T19:01:00,000T06:00:00,10-May-10,CIRS,Prime,Other,1STAROBS,Stellar spectroscopy,Mid-IR Stellar Spectroscopy,"Spectroscopic observation of 1 of 3 IR stars: CW Leonis, Eta Carinae, Alpha Orionis. Slew to star; settle; execute small box scan; return to waypoint. Observation of each star to take 6 hours; need not be executed contiguously.",,,,,, 2010-131T01:00:00,002T15:40:00,11-May-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-131T01:01:00,000T03:00:00,11-May-10,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2010-131T01:01:00,000T03:00:00,11-May-10,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2010-131T05:01:00,001T09:00:00,11-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-131T05:01:00,000T09:00:00,11-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-131T06:01:00,000T08:00:00,11-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10131_SP,rider,,,,,, 2010-131T14:01:00,001T00:00:00,11-May-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-131T14:20:00,000T09:27:28,11-May-10,CAPS,Non-SPASS,SolarWind,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-131T14:41:00,000T13:40:00,11-May-10,CIRS,Prime,Saturn,MIRTMAP,,CIRS_131SA_MIRTMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2010-132T05:01:00,000T09:00:00,12-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-132T06:01:00,000T08:00:00,12-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10132_SP,rider,,,,,, 2010-132T14:01:00,003T17:30:00,12-May-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-132T14:01:00,000T23:45:00,12-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-132T14:41:00,000T06:55:00,12-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Solar wind pointing,null,,,,,, 2010-132T14:45:00,000T03:54:40,12-May-10,CAPS,SPASS Rider,co-rotation,IONCALDV,,MAPS ion calibration DV request,null,,,,,, 2010-132T20:00:00,000T00:55:28,12-May-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-132T21:36:00,000T01:30:00,12-May-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-132T21:36:00,000T01:30:00,12-May-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-132T21:36:00,000T04:45:52,12-May-10,CAPS,Non-SPASS,SolarWind,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-132T23:06:00,000T05:00:00,12-May-10,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_131_SCATTERED_SUNLIGHT_TEST_PRIME,"Sunlight falling on the CIRS telescope can potentially be scattered into the instrument by mirror imperfections. We need to quantify the effect of ring particle impacts on the mirror performance. This requires monitoring of scattered IR solar radiation as a function of offset angle from the sun; continuous radial scans are required for this. CIRS to operate at 15.5 cm-1 resolution (4.75 sec/frame, 38 RTI), detector pairs. Scans will begin 40 degrees from FPB, and will scan to 10 degrees of FPB at TBD rate; Scan will stop every 10 degrees for TBD seconds; during this time VIMS will integrate for TBD seconds and CIRS will close its shutter for TBD seconds; the procedure will be repeated in the reverse direction back to the initial position; to determine whether scattering is asymmetric with respect to the FPB axis, 3 such scans will be made. 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from 40 degrees +Z to 10 degrees +Z and back to 40 degrees +Z. 2) From 40 degrees in -X on the X axis, to 10 degrees on the -X axis, to 40 degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 10 degrees -Z and back to 40 degrees -Z.",,,,,, 2010-133T04:46:00,000T09:00:00,13-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-133T05:46:00,000T08:00:00,13-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10133_SP,rider,,,,,, 2010-133T06:00:00,000T04:41:36,13-May-10,CAPS,Non-SPASS,SolarWind,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-133T13:46:00,000T02:54:00,13-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-133T14:26:00,000T06:00:00,13-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-133T16:40:00,002T03:25:00,13-May-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-133T16:40:00,002T03:25:00,13-May-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-133T16:40:00,002T03:25:00,13-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-133T16:40:00,000T05:51:00,13-May-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-133T20:26:00,000T01:25:00,13-May-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-133T20:26:00,000T01:25:00,13-May-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,iCYLON: Longitude / Phase Space Coverage,Map uv albedo as a function of longitude and phase space,,,,,, 2010-133T22:31:00,000T09:00:00,13-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-133T23:31:00,000T08:00:00,13-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10533_SP,rider,,,,,, 2010-134T08:11:00,000T10:10:00,14-May-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_131SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-134T18:21:00,000T02:00:00,14-May-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Magnetospheric boundary w/ prime pointing,null,,,,,, 2010-134T20:21:00,000T01:30:00,14-May-10,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Turn -Y to Iapetus; do 1x1 mosaic; turn to WP.,,,,,, 2010-134T20:21:00,000T01:30:00,14-May-10,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-134T22:31:00,000T09:00:00,14-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-134T23:31:00,000T08:00:00,14-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10134_SP,rider,,,,,, 2010-135T00:00:00,000T09:10:00,15-May-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of Data ---,null,,,,,, 2010-135T08:11:00,000T10:00:00,15-May-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 003,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-135T18:11:00,000T03:40:00,15-May-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-135T20:05:00,001T08:55:00,15-May-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-135T20:05:00,001T08:55:00,15-May-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-135T20:05:00,000T14:30:00,15-May-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-135T22:31:00,000T09:00:00,15-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-135T23:31:00,000T08:00:00,15-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10135_SP,rider,,,,,, 2010-136T07:31:00,000T05:59:00,16-May-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-136T08:11:00,000T06:40:00,16-May-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,Several slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-136T10:35:00,000T01:25:00,16-May-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-136T12:00:00,000T05:00:00,16-May-10,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2010-136T13:30:00,000T02:00:00,16-May-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-136T14:51:00,000T11:00:00,16-May-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 004,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-136T15:30:00,000T22:01:00,16-May-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-136T17:00:00,000T12:00:00,16-May-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-137T02:22:46,000T11:08:14,17-May-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate End: S S60,Range enter= 15.989755 Rs exit= 9.0039027 Range altitude= 4106.3591 km ... 1743.8539,,,,,, 2010-137T04:31:00,000T09:00:00,17-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-137T05:00:00,000T08:31:00,17-May-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-137T05:00:00,000T08:31:00,17-May-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-137T05:00:00,000T08:31:00,17-May-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-137T05:00:00,000T08:31:00,17-May-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-137T05:05:00,000T08:26:00,17-May-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-137T05:31:00,000T08:00:00,17-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10137_SP,rider,,,,,, 2010-137T13:31:00,000T16:03:03,17-May-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-137T13:31:00,000T03:00:00,17-May-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-137T13:31:00,000T05:49:46,17-May-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate Enter: S S60,Range enter= 15.989755 Rs exit= 9.0039027 Range altitude= 4106.3591 km ... 1743.8539,,,,,, 2010-137T13:31:00,000T00:43:00,17-May-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-137T13:31:00,000T14:33:39,17-May-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-137T13:31:00,001T17:44:00,17-May-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-137T13:36:00,000T00:02:00,17-May-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S60 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-137T14:02:00,000T04:41:10,17-May-10,UVIS,Prime,Dione,ICYSTARE,,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-137T14:02:00,000T04:41:00,17-May-10,ISS,SPASS Rider,Dione,ICYSTARE,,Dione plume search,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-137T14:14:00,000T00:07:00,17-May-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-137T14:21:00,000T00:05:00,17-May-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-137T14:26:00,000T00:33:00,17-May-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-137T14:59:00,000T00:22:59,17-May-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-137T15:21:59,000T06:38:01,17-May-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-137T16:31:00,000T12:33:39,17-May-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-137T19:05:00,000T04:03:00,17-May-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-137T19:05:00,000T04:03:00,17-May-10,VIMS,SPASS Rider,Enceladus,PLMHRP,,Enceladus,Enceladus,,,,,, 2010-137T19:06:05,000T04:01:55,17-May-10,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2010-137T19:20:46,001T02:22:00,17-May-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9881203 Rs exit= 8.9948183 Range altitude= 1738.0753 km ... -243.89619,,,,,, 2010-137T22:00:00,000T02:00:00,17-May-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-137T23:08:00,000T03:08:00,17-May-10,UVIS,Prime,Saturn,USUNOCC,Solar occultation,,This is an egress solar occultation of Saturn. 0) 30 minutes for turn from WAYPOINT to Sun. EUV solar occultation port centered on Sun. Slit aligned tangent to Saturn limb. 1) 20 minute observation margin. 2) Record data during egress. Egress start time: 2010-137T23:59:16.0. Egress end time: 2010-138T02:17:00.0. 3) 20 minute observation margin. 4) 30 minutes for turn from Sun to WAYPOINT.,,,,,, 2010-137T23:08:00,000T03:08:00,17-May-10,VIMS,SPASS Rider,Sun,USUNOCC,Solar occultation,Saturn Solar Occultation,Saturn Solar Occultation Egress.,,,,,, 2010-138T00:00:00,000T04:04:39,18-May-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-138T02:21:39,000T01:34:00,18-May-10,CIRS,Prime,Dione,FP3SECLN,,CIRS_131DI_FP3SECLN001_PRIME;,"FP13 N?, FP1 X; 5.3-3.9; equatorial, LT~08;stable pointing. Entry at 2010-138T03:03:18.",,,,,, 2010-138T02:21:39,000T01:34:00,18-May-10,CIRS,SPASS Rider,Dione,FP3SECLN,,CIRS_131DI_F3SECLN SI,"Two NAC images: one at entry-4 min. (i.e., at 138T02:59, Dione still in sunlight; tolerance +/- 1 minute); one shortly before turn to handoff (i.e., at 138T03:23, still in eclipse darkness; tolerance +/- 2 minutes).",,,,,, 2010-138T02:21:39,000T01:34:00,18-May-10,ISS,SPASS Rider,Dione,FP3SECLN,,Dione,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-138T02:21:39,000T01:34:00,18-May-10,UVIS,SPASS Rider,Dione,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background. Use ISSNAC to point in order to get both FUV and EUV.,,,,,, 2010-138T03:05:00,000T01:59:39,18-May-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-138T03:05:46,000T02:00:00,18-May-10,CDA,SPASS Rider,DustRAM direction,RPX0120,,CDA RPXing 2010-138T04:05:46,RPXing at 4.7428067 Rs,,,,,, 2010-138T03:55:39,000T00:29:00,18-May-10,CIRS,Prime,Enceladus,FP1DRKMAP,CIRS FP1 dark side map,CIRS_131EN_FP1DRKMAP001_PRIME;,"03:55:39 to 04:22:39 An FP1 global raster scan at 15cm-1, Saturn & rings are behind Enceladus, as slow as possible to complete the scan in this time. [Nyquist sampling will take ~10 mins at this distance] 04:22:39 to 04:24:39 Dark sky observations at 15cm-1. Start of Saturn transit egress is at 04:21:39 so observations will have to be made on the non-Saturn side. Make as many observations as possible in the time before the waypoint turn.",,,,,, 2010-138T03:55:39,000T00:29:00,18-May-10,ISS,SPASS Rider,Enceladus,FP1DRKMAP,CIRS FP1 dark side map,Enceladus close approach,Pre-close approach observation,,,,,, 2010-138T03:55:39,000T00:29:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,iCYLON: Longitude / Phase Space Coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-138T03:55:39,000T00:29:00,18-May-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2010-138T04:04:03,000T07:58:56,18-May-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-138T04:04:39,000T01:40:00,18-May-10,INMS,Non-SPASS,Enceladus,ENCEL10,,Enceladus encounter,Enceladus observation,,,,,, 2010-138T04:04:39,000T00:54:20,18-May-10,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2010-138T04:24:39,000T00:56:00,18-May-10,UVIS,Prime,Enceladus,ICYLIMB,,Limb Scan,Map volatiles off-limb,,,,,, 2010-138T04:24:39,000T00:56:00,18-May-10,VIMS,SPASS Rider,Enceladus,LIMBSCAN,Limb scan,Enceladus,Enceladus,,,,,, 2010-138T04:58:59,000T07:04:00,18-May-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-138T05:04:39,000T02:00:00,18-May-10,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 121EN Campaign,Part of 121EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2010-138T05:09:39,000T01:45:00,18-May-10,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2010-138T05:20:39,000T00:12:00,18-May-10,ISS,Prime,Enceladus,PLMHR,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2010-138T05:20:39,000T00:12:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-138T05:20:39,000T00:12:00,18-May-10,VIMS,SPASS Rider,Enceladus,PLMHR,,Enceladus,Enceladus,,,,,, 2010-138T05:32:39,000T00:48:00,18-May-10,UVIS,Prime,Sun,ICYSUNOCC,,Enceladus Plume Solar Occultation,This is an ingress/egress solar occultation of Enceladus' plume. EUV solar occultation port centered on sun. Slit aligned such that boresight doesn't rotate. Record data during entire time UVIS is pointed at the sun.,,,,,, 2010-138T05:32:39,000T00:48:00,18-May-10,VIMS,SPASS Rider,Sun,PLUMEOCC,,Enceladus plume occultation,Solar Occultation of plumes,,,,,, 2010-138T05:34:03,000T01:00:00,18-May-10,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-138T05:44:39,000T00:40:00,18-May-10,INMS,Non-SPASS,Enceladus,ENCEL10,,Enceladus encounter,Enceladus observation,,,,,, 2010-138T06:20:39,000T00:44:00,18-May-10,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus close approach,Post-close approach observation,,,,,, 2010-138T06:20:39,000T00:44:00,18-May-10,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_131EN_ENCEL001_ISS;,Rider. Shutter closed last 4 minutes,,,,,, 2010-138T06:20:39,000T00:44:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-138T06:20:39,000T00:44:00,18-May-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2010-138T06:24:39,000T01:40:00,18-May-10,INMS,Non-SPASS,Enceladus,ENCEL10,,Enceladus encounter,Enceladus observation,,,,,, 2010-138T06:34:03,001T00:40:57,18-May-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-138T07:04:39,000T00:31:00,18-May-10,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2010-138T07:04:39,001T00:10:21,18-May-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-138T07:04:39,000T00:31:00,18-May-10,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_131EN_ENCEL001_VIMS;,Rider. Shutter closed last 4 minutes,,,,,, 2010-138T07:04:39,000T00:31:00,18-May-10,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus close approach,Post-close approach observation,,,,,, 2010-138T07:04:39,000T00:31:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,iCYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2010-138T07:35:39,000T00:20:00,18-May-10,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus close approach,Post-close approach observation,,,,,, 2010-138T07:35:39,000T00:20:00,18-May-10,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_131EN_ENCEL002_ISS;,Rider. Shutter closed last 4 minutes,,,,,, 2010-138T07:35:39,000T00:20:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,iCYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2010-138T07:35:39,000T00:20:00,18-May-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2010-138T07:55:39,000T01:09:00,18-May-10,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2010-138T07:55:39,000T01:09:00,18-May-10,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,CIRS_131EN_ENCEL002_VIMS;,Rider. Shutter closed last 4 minutes,,,,,, 2010-138T07:55:39,000T01:09:00,18-May-10,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus close approach,Post-close approach observation,,,,,, 2010-138T07:55:39,000T01:09:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,iCYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2010-138T08:04:39,000T23:10:55,18-May-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-138T08:31:30,000T00:00:01,18-May-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.518 Rs, lat = -0 deg, phase = 81 deg",,,,,, 2010-138T09:04:39,000T02:00:00,18-May-10,CIRS,Prime,Enceladus,FP3DAYMAP,CIRS FP3 daytime map,CIRS_131EN_FP3DAYMAP001_PRIME;,"Dark sky is behind Enceladus for the entire observation period. 09:04:39 to 10:25:39 South ? North Scans of Enceladus? disk with FP3/4, start along sub/scft longitude, then include as many scans of the disk as possible (3 would be nice) at ~ 6 mu rads/s, at 15cm-1 spectral resolution. 10:25:39 to 10:53:39 FP1 stare at the centre of Enceladus, the FP1 FOV is ~ same size as Enceladus? disk, dark sky behind, at 3cm-1 spectral resolution. 10:53:39 to 11:04:39 Dark sky FP1 (3cm-1 resolution) and FP3/FP4 observations (15cm-1), and shutter closed to the final 4 minutes as turn back to waypoint, at 15cm-1 spectral resolution. Take time out of FP1 stare if required.",,,,,, 2010-138T09:04:39,000T02:00:00,18-May-10,ISS,SPASS Rider,Enceladus,FP3DAYMAP,CIRS FP3 daytime map,Enceladus close approach,Post-close approach observation,,,,,, 2010-138T09:04:39,000T02:00:00,18-May-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,iCYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2010-138T09:04:39,000T02:00:00,18-May-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2010-138T11:10:00,000T03:13:00,18-May-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-138T12:02:59,000T03:42:01,18-May-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-138T15:45:00,000T15:30:00,18-May-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-138T21:42:46,000T16:58:00,18-May-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 9.0106028 Rs exit= 15.999209 Range altitude= -240.67472 km ... 1359.3670,,,,,, 2010-138T22:15:00,000T09:00:00,18-May-10,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' mass,Downlink pass at Ka-band for Enceladus' mass determination and Titan's gravity science and for improving locally Cassini orbit.,,,,,, 2010-138T22:15:00,000T09:00:00,18-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-138T23:13:46,000T02:00:00,18-May-10,CDA,SPASS Rider,DustRAM direction,RPX0130,,CDA RPXing 2010-139T00:13:46,RPXing at 10.154819 Rs,,,,,, 2010-138T23:15:00,000T08:00:00,18-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10138_SP,rider,,,,,, 2010-139T07:15:00,000T06:40:00,19-May-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-139T07:15:00,000T18:09:20,19-May-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-139T07:15:00,000T19:09:20,19-May-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-139T07:15:00,000T04:40:00,19-May-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-139T07:15:00,000T04:42:00,19-May-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-139T08:10:04,000T05:44:16,19-May-10,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2010-139T08:10:04,000T05:44:16,19-May-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan.,VIMS ridealong with CIRS for scans across Titan. Phase = 144 deg. Lat/Lon. = 00S/02 deg. Resolution = 196 km/px. Temp. M2. Obtain cubes while scanning across Titan.,,,,,, 2010-139T08:10:20,000T05:44:00,19-May-10,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-139T11:55:00,000T13:29:20,19-May-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-139T11:55:00,000T11:29:20,19-May-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-139T11:57:00,002T19:03:00,19-May-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-139T13:54:20,000T00:30:00,19-May-10,ISS,Prime,Titan,LRMONITOR,Long range monitor,LRM (Long Range Monitoring),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-139T13:54:20,000T00:30:00,19-May-10,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with ISS.,,,,,, 2010-139T13:54:20,000T00:30:00,19-May-10,VIMS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,Stare at Titan.,Stare at Titan for global mapping. Phase = 144 deg. Lat/Lon. = 00S/08 deg. Resolution = 135 km/px. Temp. M2. Obtain cubes of various exp times for global mapping.,,,,,, 2010-139T14:24:20,000T03:00:00,19-May-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-139T14:24:20,000T03:00:00,19-May-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-139T14:24:20,000T03:00:00,19-May-10,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2010-139T14:24:20,000T03:00:00,19-May-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,Stare at Titan for global mapping. Phase = 144 deg. Lat/Lon. = 00S/09 deg. Resolution = 129 km/px. Temp. N. Obtain cubes of various exp times for global mapping.,,,,,, 2010-139T14:40:46,006T17:23:14,19-May-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.011218 Rs exit= 4.4241223 Range altitude= 1362.3381 km ... 40091.277,,,,,, 2010-139T16:19:20,000T02:05:00,19-May-10,RSS,SPASS Rider,Titan,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2010-139T17:24:20,000T01:00:00,19-May-10,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-139T17:24:20,000T01:00:00,19-May-10,CIRS,SPASS Rider,Titan,NIGHTNAC,ISS lightning / aurora observation,,Ride along with ISS.,,,,,, 2010-139T17:24:20,000T01:00:00,19-May-10,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan.,Stare at Titan for global mapping. Phase = 145 deg. Lat/Lon. = 01S/12 deg. Resolution = 99 km/px. Temp. N. Obtain cubes of various exp times for global mapping.,,,,,, 2010-139T18:24:20,000T18:00:00,19-May-10,RSS,SPASS Rider,Titan,GRAVITY,RSS gravity science experiment,RSS Titan's Gravity Field Experiment,"Experiment to determine Titan's gravity field, including its Love number, and infer constraints on its internal structure.",,,,,, 2010-139T23:24:20,000T08:00:00,19-May-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-139T23:24:20,000T08:00:00,19-May-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T68 flyby,"T68 is a south polar, dusk flyby, with a minimum altitude of 1400 km. In nominal upstream conditions, Cassini would explore the south lobe of Titan's magnetic tail, close to the moon. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2010-140T01:24:20,000T01:00:00,20-May-10,CAPS,SPASS Rider,Titan,T68INBD,,Titan Encounter,null,,,,,, 2010-140T01:24:20,000T01:00:00,20-May-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-140T01:39:20,000T01:00:00,20-May-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-140T02:24:20,000T02:00:00,20-May-10,CAPS,SPASS Rider,Titan,T68CLOSE,,Titan Encounter,null,,,,,, 2010-140T02:24:20,000T02:00:00,20-May-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-140T02:24:20,000T00:40:00,20-May-10,INMS,Non-SPASS,Titan,TITAN68,,Titan Flyby,Titan observation,,,,,, 2010-140T02:39:20,000T01:30:00,20-May-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-140T03:04:20,000T00:40:00,20-May-10,INMS,Non-SPASS,Titan,TITAN68,,Titan Flyby,Titan observation,,,,,, 2010-140T03:44:20,000T00:40:00,20-May-10,INMS,Non-SPASS,Titan,TITAN68,,Titan Flyby,Titan observation,,,,,, 2010-140T04:09:20,000T01:00:00,20-May-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-140T04:24:20,000T01:00:00,20-May-10,CAPS,SPASS Rider,Titan,T68OUTBND,,Titan Encounter,null,,,,,, 2010-140T04:24:20,000T01:00:00,20-May-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-140T04:24:20,002T02:35:39,20-May-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-140T05:24:20,000T06:30:00,20-May-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-140T05:24:20,000T16:45:39,20-May-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-140T07:24:20,000T14:45:40,20-May-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-140T11:54:20,000T18:31:40,20-May-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-140T12:24:20,000T04:00:00,20-May-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-140T12:24:20,000T04:00:00,20-May-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-140T12:24:20,000T04:00:00,20-May-10,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2010-140T12:24:20,000T04:00:00,20-May-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,Stare at Titan for global mapping. Phase = 31 deg. Lat/Lon. = 05N/213 deg. Resolution = 88 km/px. Temp. C. Obtain cubes of various exp times for global mapping.,,,,,, 2010-140T16:24:20,000T04:40:44,20-May-10,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2010-140T16:24:20,000T04:40:44,20-May-10,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-140T16:24:20,000T04:40:44,20-May-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan.,VIMS ridealong with CIRS for scans across Titan. Phase = 31 deg. Lat/Lon. = 05N/218 deg. Resolution = 138 km/px. Temp. A. Obtain cubes while scanning across Titan.,,,,,, 2010-140T22:00:00,000T09:00:00,20-May-10,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's gravity,Additional downlink pass at Ka-band for Titan's gravity science and for improving locally Cassini orbit.,,,,,, 2010-140T22:00:00,000T09:00:00,20-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-140T22:10:00,001T08:50:00,20-May-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-140T22:10:00,001T08:50:00,20-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-140T23:00:00,000T08:00:00,20-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10140_SP,rider,,,,,, 2010-141T06:26:00,002T00:09:00,21-May-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-141T07:40:00,000T02:00:00,21-May-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-141T07:40:00,000T02:00:00,21-May-10,CIRS,SPASS Rider,Titan,MONITOR,,,Ride along with ISS.,,,,,, 2010-141T07:40:00,000T02:00:00,21-May-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan cloud monitoring,Caboose segment. Stare at Titan for cloud mapping. Phase = 33 deg. Lat/Lon. = 05N/230 deg. Resolution = 284 km/px. Obtain cubes of various exp times for cloud mapping.,,,,,, 2010-141T09:40:00,000T08:00:00,21-May-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-141T09:40:00,000T08:00:00,21-May-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan cloud monitoring,Caboose segment. Stare at Titan for cloud mapping. Phase = 33 deg. Lat/Lon. = 05N/231 deg. Resolution = 305 km/px. Obtain cubes of various exp times for cloud mapping.,,,,,, 2010-141T17:40:00,000T02:10:00,21-May-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-141T19:40:00,000T01:40:00,21-May-10,CIRS,SPASS Rider,Titan,MONITOR,,,Ride along with ISS.,,,,,, 2010-141T20:30:00,000T01:30:00,21-May-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan cloud monitoring,Caboose segment. Stare at Titan for cloud mapping. Phase = 35 deg. Lat/Lon. = 05N/239 deg. Resolution = 411 km/px. Obtain cubes of various exp times for cloud mapping.,,,,,, 2010-141T22:00:00,000T09:00:00,21-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-141T23:00:00,000T08:00:00,21-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10141_SP,rider,,,,,, 2010-142T07:00:00,001T09:35:00,22-May-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-142T07:00:00,001T06:15:00,22-May-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-142T07:00:00,001T09:35:00,22-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-142T07:00:00,004T01:04:00,22-May-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-142T07:00:00,001T09:35:00,22-May-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-142T07:40:00,000T01:15:00,22-May-10,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 37.3 range 1.1 Mkm",,,,,, 2010-142T07:40:00,000T01:15:00,22-May-10,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-142T07:40:00,000T01:15:00,22-May-10,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-142T08:55:00,000T06:00:00,22-May-10,ISS,Prime,Iapetus,HILLSPHE,,Iapetus hill sphere observation,Turn -Y to Iapetus; do 1x3 mosaic; turn to WP.,,,,,, 2010-142T14:55:00,000T04:00:00,22-May-10,UVIS,Prime,Enceladus,ICYATM,Icy satellite system volatile map,ICYATM: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of Enceladus. Observations will test connection of volatile changes to plume eruptions.,,,,,, 2010-142T18:55:00,000T08:40:00,22-May-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-143T04:15:00,000T09:00:00,23-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-143T05:15:00,000T08:00:00,23-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10143_SP,rider,,,,,, 2010-143T06:35:00,000T10:00:00,23-May-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-143T13:15:00,000T23:45:00,23-May-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-143T13:55:00,000T01:15:00,23-May-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 44.9 range 1.7 Mkm",,,,,, 2010-143T13:55:00,000T01:15:00,23-May-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-143T13:55:00,000T01:15:00,23-May-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-143T15:10:00,000T12:10:00,23-May-10,ISS,Prime,Star,CALSTAR1,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2010-143T16:35:00,005T06:55:00,23-May-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-143T16:35:00,002T15:29:00,23-May-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-143T16:35:00,000T05:00:00,23-May-10,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2010-143T16:35:00,000T20:25:00,23-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-143T21:35:00,005T01:55:00,23-May-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-144T04:00:00,000T12:00:00,24-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-144T04:00:00,000T09:00:00,24-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-144T05:00:00,000T08:00:00,24-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10144_SP,rider,,,,,, 2010-144T13:00:00,001T19:04:00,24-May-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-144T13:00:00,001T19:04:00,24-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-144T13:40:00,000T12:10:00,24-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-145T02:30:00,000T10:30:00,25-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-145T04:00:00,000T09:00:00,25-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-145T05:00:00,000T08:00:00,25-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10145_SP,rider,,,,,, 2010-145T13:00:00,000T03:00:00,25-May-10,RADAR,SPASS Rider,Other,WU4SRCCAL,,Warm Up for Microwave Source Calibration,Warmup for calibration and science data collection.,,,,,, 2010-145T13:40:00,000T02:20:00,25-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-145T16:00:00,000T07:59:00,25-May-10,RADAR,Prime,Other,SRCRADCAL,RADAR microwave source radiometric calibration,Radiometric Microwave Sources Calibration,"Scan the Sun, Saturn, and microwave sources while collecting radiometry data.",,,,,, 2010-145T23:59:00,000T01:50:00,25-May-10,VIMS,Prime,Star,3STARCAL,Stellar calibration,Stellar Calibrations,"Turn to X Oph, stare 30 min; turn to R Aql (286.5921,8.2300); stare 30 min; turn to W Aql (288.8424,-7.0489); stare for 30 min; return to Waypoint",,,,,, 2010-145T23:59:00,000T07:00:00,25-May-10,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-34 in 1-way mode.,,,,,, 2010-146T02:29:00,000T10:30:00,26-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-146T03:59:00,000T09:00:00,26-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-146T06:59:00,000T06:00:00,26-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_131IC_DSCAL10146_SP,rider,,,,,, 2010-146T08:04:00,002T15:26:00,26-May-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-146T08:04:00,007T19:16:46,26-May-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.011218 Rs exit= 4.4241223 Range altitude= 1362.3381 km ... 40091.277,,,,,, 2010-146T08:04:00,002T04:40:00,26-May-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-146T08:04:00,003T14:40:00,26-May-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-146T08:04:00,002T15:26:00,26-May-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-146T08:04:00,000T04:55:00,26-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-146T08:04:39,000T00:00:01,26-May-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 12.1 deg, r = 37.792 Rs, phase = 91 deg",,,,,, 2010-146T13:39:00,000T09:00:00,26-May-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_132SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-146T22:39:00,000T03:10:00,26-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-147T02:29:00,000T10:30:00,27-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-147T03:59:00,000T09:00:00,27-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-147T04:59:00,000T08:00:00,27-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10147_SP,rider,,,,,, 2010-147T12:59:00,003T10:00:00,27-May-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-147T13:39:00,000T01:15:00,27-May-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 76.7 range 3.1 Mkm",,,,,, 2010-147T13:39:00,000T01:15:00,27-May-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-147T13:39:00,000T01:15:00,27-May-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-147T14:54:00,000T01:30:00,27-May-10,ISS,Prime,InstrumentCalibration,CALLAMP,ISS Wide angle camera calibration lamp exposure,ISS WAC CAL LAMP,ISS WAC Cal Lamp exposures,,,,,, 2010-147T16:24:00,000T10:40:00,27-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-148T03:44:00,000T09:00:00,28-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-148T04:44:00,000T08:00:00,28-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10148_SP,rider,,,,,, 2010-148T12:44:00,001T00:00:00,28-May-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-148T13:24:00,000T06:36:00,28-May-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-148T20:00:00,000T07:04:00,28-May-10,UVIS,Prime,Star,URLAMAQL,,URSTAR,"Slow chord occ with turnaround in mid-A ring. Ingress half is better if request must be shortened, but any fraction is better than nothing. Baseline can be obtained either in Encke Gap or Roche Division. Low-incidence angle star (B=7.5 degrees). Expected count rate 1800 Hz.",,,,,, 2010-148T23:30:00,002T18:30:00,28-May-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-148T23:30:00,000T13:14:00,28-May-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-148T23:30:00,000T13:14:00,28-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-148T23:30:00,000T13:14:00,28-May-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-149T03:44:00,000T09:00:00,29-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-149T04:00:00,000T12:00:00,29-May-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-149T04:44:00,000T08:00:00,29-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10149_SP,rider,,,,,, 2010-149T12:44:00,000T14:00:00,29-May-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-149T12:44:00,002T05:16:00,29-May-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-149T12:44:00,002T17:16:00,29-May-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-149T12:44:00,000T16:31:00,29-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-149T12:44:00,003T16:08:00,29-May-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-150T00:00:00,000T00:34:00,30-May-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-150T03:15:00,000T02:00:00,30-May-10,ISS,Prime,rings(general),PHOTLIT,Ring system photometry,"low-latitude, lit-face ring photometry","low latitude lit #3: B = 8, phase ~ 102, B' = 4.4.",,,,,, 2010-150T03:15:00,000T02:00:00,30-May-10,CIRS,SPASS Rider,rings(general),PHOTLIT,Ring system photometry,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-150T05:15:00,000T06:45:00,30-May-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-150T05:15:00,000T06:45:00,30-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-150T12:00:00,000T11:30:00,30-May-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-150T12:00:00,001T06:00:00,30-May-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-150T13:59:00,000T09:00:00,30-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-150T14:59:00,000T08:00:00,30-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10150_SP,rider,,,,,, 2010-150T23:30:00,000T08:45:00,30-May-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-151T08:15:00,000T03:30:00,31-May-10,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-151T08:15:00,000T03:30:00,31-May-10,CIRS,SPASS Rider,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-151T08:15:00,000T03:30:00,31-May-10,UVIS,SPASS Rider,rings(general),EQLBN,,URSPEC,,,,,,, 2010-151T08:15:00,000T03:30:00,31-May-10,VIMS,SPASS Rider,rings(general),EQLBN,,"radial scan, low phase, lit side","320 ms, 64*12 cubes?",,,,,, 2010-151T13:44:00,000T09:00:00,31-May-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-151T14:44:00,000T08:00:00,31-May-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10151_SP,rider,,,,,, 2010-151T18:00:00,001T04:44:00,31-May-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-151T18:00:00,001T10:45:00,31-May-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-151T18:00:00,001T04:44:00,31-May-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-151T18:00:00,001T04:44:00,31-May-10,RPWS,Non-SPASS,Sun,DUSKMSPH,,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries on dusk flank",,,,,, 2010-151T22:44:00,000T13:20:00,31-May-10,VIMS,Prime,rings(general),FMOVIE,F ring movie,F Ring movie,"64x12 frame, hi res mode. 640 msec tau_IR.",,,,,, 2010-151T22:44:00,000T13:20:00,31-May-10,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-151T22:44:00,000T13:20:00,31-May-10,ISS,SPASS Rider,rings(general),FMOVIE,F ring movie,Medium Res F ring Movie,F Ring Movie Rider,,,,,, 2010-152T06:00:00,000T04:00:00,1-Jun-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-152T10:00:00,000T12:44:00,1-Jun-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-152T13:44:00,000T09:00:00,1-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-152T14:44:00,000T08:00:00,1-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10152_SP,rider,,,,,, 2010-152T22:44:00,001T00:00:00,1-Jun-10,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,SAP Bits,null,,,,,, 2010-152T22:44:00,002T13:29:00,1-Jun-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-152T22:44:00,001T00:00:00,1-Jun-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-152T22:44:00,000T06:01:00,1-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-152T23:15:00,000T04:15:00,1-Jun-10,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-152T23:15:00,000T04:15:00,1-Jun-10,CIRS,SPASS Rider,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-152T23:15:00,000T04:15:00,1-Jun-10,UVIS,SPASS Rider,rings(general),EQLBN,,URSPEC,,,,,,, 2010-153T03:30:00,000T08:59:00,2-Jun-10,ISS,Prime,rings(general),SHRTMOV,,Short movies of select features,Short movies of select features,,,,,, 2010-153T03:30:00,000T08:59:00,2-Jun-10,CIRS,SPASS Rider,rings(general),SHRTMOV,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-153T03:30:00,000T08:59:00,2-Jun-10,VIMS,SPASS Rider,rings(general),SHRTMOV,,"Stare at rings, lit face","320 ms, 64x64 or as required",,,,,, 2010-153T04:45:00,000T17:59:00,2-Jun-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-153T04:45:00,002T07:28:00,2-Jun-10,MIMI,Non-SPASS,Saturn,MAGDYN,MAPS magnetosphere dynamics campaign,MIMI Magnetospheric Dymanics,"Setup MIMI for magnetospheric dynamics observations, INCA imaging, any OPMODE or TLM mode.",,,,,, 2010-153T04:52:00,002T05:42:00,2-Jun-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-153T13:44:00,000T09:00:00,2-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-153T22:44:00,000T00:10:04,2-Jun-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-153T22:44:00,000T04:38:59,2-Jun-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-153T22:54:04,000T06:30:00,2-Jun-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-153T23:59:00,000T03:16:00,2-Jun-10,CIRS,Prime,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-153T23:59:00,000T03:01:00,2-Jun-10,CIRS,SPASS Rider,rings(general),EQLBN,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-153T23:59:00,000T03:01:00,2-Jun-10,UVIS,SPASS Rider,rings(general),EQLBN,,URSPEC,,,,,,, 2010-154T03:20:46,000T01:36:00,3-Jun-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.4053542 Rs exit= 3.5649847 Range altitude= 39707.511 km ... 20323.824,,,,,, 2010-154T03:22:59,000T08:43:00,3-Jun-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-154T04:56:46,000T02:55:53,3-Jun-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 3.5485253 Rs exit= 2.7454832 Range altitude= 19882.938 km ... -19879.201,,,,,, 2010-154T05:24:00,000T02:00:00,3-Jun-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-154T05:24:04,000T02:00:00,3-Jun-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-154T05:25:46,000T02:00:00,3-Jun-10,CDA,SPASS Rider,DustRAM direction,RPX0140,,CDA RPXing 2010-154T06:25:46,RPXing at 2.9566906 Rs,,,,,, 2010-154T05:55:00,000T01:55:00,3-Jun-10,VIMS,Prime,rings(general),OMICETOCC,OmiCet occultation,omiCet ring occultation,omiCet ring occultation. Priority 1.,,,,,, 2010-154T05:55:00,000T01:55:00,3-Jun-10,CIRS,SPASS Rider,rings(general),OMICETOCC,OmiCet occultation,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-154T05:55:00,000T01:55:00,3-Jun-10,ISS,SPASS Rider,rings(general),OMICETOCC,OmiCet occultation,OMICET OCC OF F RING,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-154T05:55:00,000T01:55:00,3-Jun-10,UVIS,SPASS Rider,Star,OMICETOCC,OmiCet occultation,URSTAR,,,,,,, 2010-154T07:24:04,000T23:00:00,3-Jun-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-154T07:43:17,000T00:00:01,3-Jun-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.739 Rs, lat = -6 deg, phase = 89 deg",,,,,, 2010-154T07:50:00,000T01:00:00,3-Jun-10,ISS,Prime,Pandora,PANDOCLOS,,Pandora close flyby,"Pandora close flyby, ~97,500 km at CA, 42 deg phase",,,,,, 2010-154T07:50:00,000T01:00:00,3-Jun-10,CIRS,SPASS Rider,Pandora,PANDOCLOS,,CIRS_132PA_PANDOCLOS_ISS,"FP3+FP4 only. AD~1 mrad, phase 30-20, sub S/C~(-15, 85)",,,,,, 2010-154T07:50:00,000T01:00:00,3-Jun-10,UVIS,SPASS Rider,Pandora,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map UV albedo as a function of longitude and phase angle,,,,,, 2010-154T07:50:00,000T01:00:00,3-Jun-10,VIMS,SPASS Rider,Pandora,PANDOCLOS,,Pandora,multiple 16/640 ms.,,,,,, 2010-154T07:52:39,000T02:01:05,3-Jun-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 2.7467390 Rs exit= 3.2711579 Range altitude= -20267.219 km ... -39835.062,,,,,, 2010-154T08:50:00,000T13:40:00,3-Jun-10,ISS,Prime,rings(general),PROPELLR,,Propeller tracking,Image rings at high resolution to track propellers. Full longitudinal coverage to reacquire giant propellers,,,,,, 2010-154T08:50:00,000T13:40:00,3-Jun-10,CIRS,SPASS Rider,rings(general),PROPELLR,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-154T09:53:44,000T17:10:00,3-Jun-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 3.2857018 Rs exit= 12.006661 Range altitude= -40070.397 km ... -40061.432,,,,,, 2010-154T10:56:29,000T01:09:30,3-Jun-10,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE6 flyby,"Monitor the interaction of Tethys with the Saturnian magnetosphere. Data rate 0 bps, overlaps INTFLD request.",,,,,, 2010-154T12:05:59,000T02:50:30,3-Jun-10,MAG,Non-SPASS,Tethys,TETAR,Tethys targeted flyby,TE6 flyby,Monitor the interaction of Tethys with the Saturnian magnetosphere.,,,,,, 2010-154T14:56:29,000T03:34:53,3-Jun-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-154T18:31:22,000T04:00:00,3-Jun-10,MAG,Non-SPASS,Rhea,RHTAR,Rhea targeted flyby,R5 flyby,"The sole Rhea flyby was a downstream flyby. In order to fully understand if the moon is mass-loading or mass-absorbing type both upstream and downstream flybys are required. The new flybys R2,R3,R4 and R5 will fulfill this requirement.",,,,,, 2010-154T22:30:00,000T02:30:00,3-Jun-10,CIRS,Prime,Rhea,FP3DAYMAP,CIRS FP3 daytime map,CIRS_132RH_FP3DAYMAP001_PRIME;,"Draft agreement with UVIS, ISS, and VIMS on 091020: 22:30 Turn to Rhea 22:40 Single s. polar ISS image, stay 2 minutes for VIMS. 22:42 Start FP1 fast raster scan at Nyquist sampling at 15cm-1 23:05 ISS mosaic, 1 minute dwells (2x3 mosaic?) 23:20 VIMS stare 23:40 Start FP3 scan, as slow as possible to get global scan and 3 minutes of dark sky (probably need to be ~ 12 mu rads/s to get 2 full scans in) at 15cm-1 00:45 Start turn back to waypoint 01:00 Back to waypoint Voyager-class. C/A at 154T20:31:20 21.8, 102, (-48, 107), LT~19. 1.05*6 scans*17 mrad*16/16 = 107 min. or 3 scans = 53 miin. iDigit turn estimates about Z: to: 5+2=7; fro: 4+2=6 min; about X: to: 8+2=10; fro: 6+2=8 min. NEG_X or NEG_Z to NSP for secondary. FP3 and FP1 only",,,,,, 2010-154T22:30:00,000T02:30:00,3-Jun-10,ISS,SPASS Rider,Rhea,FP3DAYMAP,CIRS FP3 daytime map,Rhea,"South-pole ftprt first, then FP1 raster scan, then 2x3 global NAC mosaic (1 min dwell), then VIMS sit'n'stare, then CIRS FP3 scan",,,,,, 2010-154T22:30:00,000T02:30:00,3-Jun-10,UVIS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-154T22:30:00,000T02:30:00,3-Jun-10,VIMS,SPASS Rider,Rhea,FP3DAYMAP,CIRS FP3 daytime map,Rhea,multiple 16/640 ms.,,,,,, 2010-154T22:31:22,000T12:03:38,3-Jun-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-155T03:03:44,000T10:16:00,4-Jun-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 12.020940 Rs exit= 15.996924 Range altitude= -39997.456 km ... -18632.255,,,,,, 2010-155T03:13:00,000T09:00:00,4-Jun-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev133 Saturn rings and atmospheric occultation on 2010/169-170.",,,,,, 2010-155T03:13:00,000T09:00:00,4-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-155T04:13:00,000T06:00:00,4-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10155_SP,rider,,,,,, 2010-155T06:24:04,000T05:48:56,4-Jun-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-155T10:34:00,000T01:39:00,4-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-155T10:35:00,000T01:38:00,4-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-155T12:13:00,000T12:13:27,4-Jun-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-155T12:13:00,000T12:13:27,4-Jun-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-155T12:13:00,000T13:13:27,4-Jun-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-155T12:13:00,000T10:13:27,4-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-155T12:13:00,003T17:30:00,4-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-155T13:08:02,000T04:00:25,4-Jun-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,Global mapping of Titan. Phase = 149 deg. Lat/Lon = 05S/13 deg. Resolution = 129 km/px. Temp. O. Obtain cubes of various exposure times for global mapping.,,,,,, 2010-155T13:08:02,000T04:00:25,4-Jun-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2010-155T13:08:02,000T04:00:25,4-Jun-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-155T13:19:44,006T18:07:16,4-Jun-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.008717 Rs exit= 16.001514 Range altitude= -18559.322 km ... -25721.644,,,,,, 2010-155T17:08:27,000T04:18:00,4-Jun-10,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-155T17:08:27,000T04:18:00,4-Jun-10,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-155T17:08:27,000T04:18:00,4-Jun-10,RADAR,SPASS Rider,Titan,T69WARMUP,,Warmup for T69,,,,,,, 2010-155T17:08:27,000T04:18:00,4-Jun-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS for limb mapping of Titan. Phase = 150 deg. Lat/Lon = 04S/17 deg. Resolution = 89 km/px. Temp. R. Obtain cubes of various exposure times for limb mapping.,,,,,, 2010-155T21:26:27,000T03:00:00,4-Jun-10,RADAR,Prime,Titan,T69INRAD,,T69 Inbound Radiometry,,,,,,, 2010-155T22:26:27,000T08:00:00,4-Jun-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T69 flyby,"T69 is a north polar, dusk flyby, with a minimum altitude of 2100 km. In nominal upstream conditions, Cassini would explore the edge of the north lobe of Titan's magnetic tail. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2010-155T22:26:28,000T08:00:00,4-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-156T00:26:27,000T00:48:00,5-Jun-10,RADAR,Prime,Titan,T69INSCAT,,T69 Inbound Scatterometry,,,,,,, 2010-156T00:26:27,000T01:00:00,5-Jun-10,CAPS,SPASS Rider,Titan,T69INBD,,Titan Encounter,null,,,,,, 2010-156T00:26:27,000T01:00:00,5-Jun-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-156T00:26:27,000T01:00:00,5-Jun-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-156T01:14:27,000T00:57:00,5-Jun-10,RADAR,Prime,Titan,T69IHISAR,,T69 Inbound HiSAR,,,,,,, 2010-156T01:26:27,000T02:00:00,5-Jun-10,CAPS,SPASS Rider,Titan,T69CLOSE,,Titan Encounter,null,,,,,, 2010-156T01:26:27,000T02:00:00,5-Jun-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-156T01:26:27,000T00:40:00,5-Jun-10,INMS,Non-SPASS,Titan,TITAN69,,Titan Flyby,Titan observation,,,,,, 2010-156T01:26:27,000T02:00:00,5-Jun-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-156T02:06:27,000T00:40:00,5-Jun-10,INMS,Non-SPASS,Titan,TITAN69,,Titan Flyby,Titan observation,,,,,, 2010-156T02:11:27,000T02:15:00,5-Jun-10,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,"Regional mapping of Titan during C/A. At C/A, phase = 87 deg. Lat/Lon = 87N/09 deg. Resolution = 1.0 km/px. Obtain mosaics of Ligeia mare (~80N lat, 248W lon). Obtain 4x4 mosaics between 70 and 20 N latitutde (area should cover Selk crater).",,,,,, 2010-156T02:11:27,000T02:15:00,5-Jun-10,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with VIMS.,,,,,, 2010-156T02:11:27,000T02:15:00,5-Jun-10,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-156T02:46:27,000T00:40:00,5-Jun-10,INMS,Non-SPASS,Titan,TITAN69,,Titan Flyby,Titan observation,,,,,, 2010-156T03:26:27,000T06:50:00,5-Jun-10,CAPS,SPASS Rider,Titan,T69OUTBND,,Titan Encounter,null,,,,,, 2010-156T03:26:27,000T01:00:00,5-Jun-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-156T03:26:27,003T02:16:32,5-Jun-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-156T03:26:27,000T01:00:00,5-Jun-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-156T04:26:27,000T07:00:00,5-Jun-10,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2010-156T04:26:27,000T07:00:00,5-Jun-10,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with VIMS.,,,,,, 2010-156T04:26:27,000T07:00:00,5-Jun-10,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-156T04:26:27,000T16:38:32,5-Jun-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-156T04:26:27,000T03:00:00,5-Jun-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan.,VIMS ridealong with UVIS for slow scan across Titan. Phase = 30 deg. Lat/Lon = 06N/208 deg. Resolution = 19 km/px. Temp. X. Obtain cubes while scanning across Titan.,,,,,, 2010-156T06:26:27,000T14:38:33,5-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-156T07:26:27,000T04:00:00,5-Jun-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan.,VIMS ridealong with UVIS for slow scan across Titan. Phase = 30 deg. Lat/Lon = 02N/210 deg. Resolution = 49 km/px. Temp. X. Obtain cubes while scanning across Titan.,,,,,, 2010-156T10:16:27,002T19:26:33,5-Jun-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-156T11:26:27,000T03:00:00,5-Jun-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-156T11:26:27,000T03:00:00,5-Jun-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-156T11:26:27,000T03:00:00,5-Jun-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,VIMS ridealong with CIRS for global mapping of Titan. Phase = 31 deg. Lat/Lon = 01N/214 deg. Resolution = 89 km/px. Temp. D2. Obtain cubes of various integrations for global mapping of Titan.,,,,,, 2010-156T14:26:27,000T02:00:00,5-Jun-10,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,NAM (NAC Monitor),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-156T14:26:27,000T02:00:00,5-Jun-10,CIRS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,,Ride along with VIMS.,,,,,, 2010-156T14:26:27,000T02:00:00,5-Jun-10,VIMS,SPASS Rider,Titan,MONITORNA,Monitoring of surface and atmosphere,Stare at Titan.,VIMS ridealong with ISS for global mapping of Titan. Phase = 31 deg. Lat/Lon = 00N/217 deg. Resolution = 119 km/px. Temp. D2. Obtain cubes of various integrations for global mapping of Titan.,,,,,, 2010-156T16:26:27,000T02:06:35,5-Jun-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping,Global mapping of Titan. Phase = 31 deg. Lat/Lon = 00N/218 deg. Resolution = 139 km/px. Temp. B(Z). Obtain cubes of various exposure times for global mapping.,,,,,, 2010-156T16:26:27,000T02:06:35,5-Jun-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2010-156T16:26:27,000T02:06:35,5-Jun-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-156T20:58:00,000T09:00:00,5-Jun-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev133 Saturn rings and atmospheric occultation on 2010/169-170.",,,,,, 2010-156T21:05:00,002T08:38:00,5-Jun-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-156T21:05:00,001T08:53:00,5-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-156T21:58:00,000T08:00:00,5-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10156_SP,rider,,,,,, 2010-157T07:28:00,000T04:32:00,6-Jun-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-157T07:28:00,000T04:32:00,6-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 33 deg. Lat/Lon = 00S/230 deg. Resolution = 284 km/px. Obtain cubes of various integrations for cloud monitoring.,,,,,, 2010-157T12:00:00,000T02:00:00,6-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-157T14:00:00,000T04:48:00,6-Jun-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-157T14:00:00,000T04:48:00,6-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 34 deg. Lat/Lon = 00S/236 deg. Resolution = 362 km/px. Obtain cubes of various integrations for cloud monitoring.,,,,,, 2010-157T19:28:00,000T01:30:00,6-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-157T20:58:00,000T09:00:00,6-Jun-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev133 Saturn rings and atmospheric occultation on 2010/169-170.",,,,,, 2010-157T21:58:00,000T08:00:00,6-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10157_SP,rider,,,,,, 2010-158T05:58:00,000T23:45:00,7-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-158T07:13:00,000T06:47:00,7-Jun-10,RADAR,SPASS Rider,Other,WU4SEQUA,,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-158T07:28:00,000T04:32:00,7-Jun-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-158T07:28:00,000T02:30:00,7-Jun-10,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-158T07:28:00,000T04:32:00,7-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 38 deg. Lat/Lon = 01S/248 deg. Resolution = 539 km/px. Obtain cubes of various integrations for cloud monitoring.,,,,,, 2010-158T12:00:00,000T02:00:00,7-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-158T14:00:00,000T01:30:00,7-Jun-10,RADAR,Prime,Titan,SEQUACAL,,"Distant Titan Radiometry, South Equatorial Latitud",Obtain distant Titan radiometer science and calibration data.,,,,,, 2010-158T15:30:00,000T04:33:00,7-Jun-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-158T15:30:00,000T04:33:00,7-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 40 deg. Lat/Lon = 01S/254 deg. Resolution = 635 km/px. Obtain cubes of various integrations for cloud monitoring.,,,,,, 2010-158T21:43:00,000T08:00:00,7-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10158_SP,rider,,,,,, 2010-159T04:00:00,000T12:00:00,8-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-159T05:43:00,000T09:07:00,8-Jun-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-159T05:43:00,000T09:07:00,8-Jun-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-159T05:43:00,001T00:00:00,8-Jun-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-159T05:43:00,000T09:07:00,8-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-159T05:43:00,003T01:44:00,8-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-159T05:43:00,000T09:07:00,8-Jun-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-159T06:18:00,000T13:50:00,8-Jun-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-159T14:50:00,005T09:15:00,8-Jun-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-159T14:50:00,002T16:37:00,8-Jun-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-159T14:50:00,000T15:33:00,8-Jun-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-159T14:50:00,002T16:37:00,8-Jun-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-159T20:43:00,000T09:00:00,8-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-159T21:43:00,000T08:00:00,8-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10159_SP,rider,,,,,, 2010-160T05:43:00,000T18:17:00,9-Jun-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-160T06:23:00,000T06:45:00,9-Jun-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales. Added to improve calibration for T70, conditions are not ideal but is maximum distance reached outside magnetopause before T70.",,,,,, 2010-160T06:23:00,000T06:45:00,9-Jun-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-160T13:08:00,000T05:24:00,9-Jun-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-160T13:08:00,004T10:57:00,9-Jun-10,MAG,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAG MAPS SWAURORA Campaign,Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth-based observations of Saturn's aurora.,,,,,, 2010-160T20:42:00,000T09:00:00,9-Jun-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev133 Saturn rings and atmospheric occultation on 2010/169-170.",,,,,, 2010-160T20:42:00,000T09:00:00,9-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-160T21:42:00,000T08:00:00,9-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_132IC_DSCAL10160_SP,rider,,,,,, 2010-161T00:00:00,000T02:00:00,10-Jun-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-161T02:00:00,001T05:27:00,10-Jun-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-161T04:00:00,000T12:00:00,10-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-161T06:22:00,000T01:15:00,10-Jun-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 57.7 range 2.5 Mkm",,,,,, 2010-161T06:22:00,000T01:15:00,10-Jun-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-161T06:22:00,000T01:15:00,10-Jun-10,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-161T07:37:00,000T23:00:00,10-Jun-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_132SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-162T06:37:00,000T04:05:00,11-Jun-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-162T07:27:00,002T16:38:00,11-Jun-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-162T07:27:00,006T18:14:44,11-Jun-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.008717 Rs exit= 16.001514 Range altitude= -18559.322 km ... -25721.644,,,,,, 2010-162T07:27:00,001T01:33:00,11-Jun-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-162T07:27:00,006T20:58:00,11-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-162T07:27:00,002T16:38:00,11-Jun-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-162T07:28:02,000T00:00:01,11-Jun-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 2.0 deg, r = 37.903 Rs, phase = 91 deg",,,,,, 2010-162T08:00:00,000T12:00:00,11-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-162T13:12:00,000T09:00:00,11-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-162T14:12:00,000T08:00:00,11-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10162_SP,rider,,,,,, 2010-162T22:12:00,000T13:15:00,11-Jun-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-162T22:12:00,001T15:25:00,11-Jun-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-162T22:12:00,000T14:43:00,11-Jun-10,RPWS,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,"MAPS MB,D Campaign","Part of MB,D MAPS Campaign. Observe magnetospheric boundaries near noon on highly inclined orbits",,,,,, 2010-163T09:00:00,000T04:00:00,12-Jun-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-163T12:57:00,000T09:00:00,12-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-163T13:00:00,000T22:42:00,12-Jun-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-163T13:57:00,000T08:00:00,12-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10163_SP,rider,,,,,, 2010-163T21:57:00,000T04:10:00,12-Jun-10,ISS,Prime,Star,CALSTAR2,Stellar Calibration,ISS Photometric Calibration Star 2,Photometric Calibration Star 2 (77/78 Tau),,,,,, 2010-164T02:42:00,000T09:00:00,13-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-164T03:42:00,000T08:00:00,13-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10164_SP,rider,,,,,, 2010-164T11:42:00,001T00:00:00,13-Jun-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-164T12:22:00,000T01:15:00,13-Jun-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86.1 range 3.3 Mkm",,,,,, 2010-164T12:22:00,000T01:15:00,13-Jun-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-164T12:22:00,000T01:15:00,13-Jun-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-164T12:22:00,000T01:15:00,13-Jun-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 86.1 range 3.3 Mkm",,,,,, 2010-164T13:37:00,000T06:00:00,13-Jun-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-164T19:37:00,000T04:28:00,13-Jun-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-164T22:55:00,000T00:34:00,13-Jun-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-165T00:05:00,002T17:40:00,14-Jun-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-165T00:05:00,002T17:40:00,14-Jun-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-165T00:05:00,000T11:37:00,14-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-165T02:42:00,000T09:00:00,14-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-165T03:42:00,000T08:00:00,14-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10165_SP,rider,,,,,, 2010-165T04:00:00,000T12:00:00,14-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-165T11:42:00,003T00:18:00,14-Jun-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-165T11:42:00,002T06:03:00,14-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-165T12:22:00,000T08:00:00,14-Jun-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_133SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-165T20:22:00,000T05:10:00,14-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-166T01:32:00,000T16:30:00,15-Jun-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-166T20:12:00,000T09:00:00,15-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-166T21:12:00,000T04:00:00,15-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10166_SP,rider,,,,,, 2010-167T05:12:00,000T13:29:00,16-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-167T17:45:00,001T10:35:00,16-Jun-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,MAPS Survey,null,,,,,, 2010-167T17:45:00,001T10:35:00,16-Jun-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-167T17:45:00,000T06:15:00,16-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-167T20:12:00,000T09:00:00,16-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-167T21:12:00,000T04:00:00,16-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10167_SP,rider,,,,,, 2010-168T00:00:00,001T04:20:00,17-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-168T05:12:00,000T07:28:00,17-Jun-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_133SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-168T12:00:00,000T02:00:00,17-Jun-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-168T12:40:00,000T07:26:00,17-Jun-10,CAPS,Prime,Saturn,DUSKPTG,,MAPS Survey w/ prime pointing,null,,,,,, 2010-168T14:00:00,000T15:11:00,17-Jun-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-168T20:11:00,000T09:00:00,17-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-168T21:11:00,000T04:00:00,17-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10168_SP,rider,,,,,, 2010-169T01:41:44,000T16:40:00,18-Jun-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 15.989641 Rs exit= 9.0011789 Range altitude= -25711.046 km ... -17490.421,,,,,, 2010-169T04:20:00,000T21:02:30,18-Jun-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-169T04:20:00,002T05:20:00,18-Jun-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-169T04:20:00,000T22:24:59,18-Jun-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-169T04:25:00,002T05:14:00,18-Jun-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-169T05:11:00,000T06:35:00,18-Jun-10,CAPS,Prime,Saturn,RNGSATPTG,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-169T05:11:00,000T16:30:00,18-Jun-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-169T11:46:00,000T09:00:00,18-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-169T12:46:00,000T04:00:00,18-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10169_SP,rider,,,,,, 2010-169T16:00:00,001T08:00:00,18-Jun-10,RPWS,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAPS RS Campaign,"Part of RS MAPS Campaign. Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-169T18:21:44,001T01:22:19,18-Jun-10,CDA,Non-SPASS,Other,RATE320,,Data rate,Range enter= 8.9844428 Rs exit= 8.9998808 Range altitude= -17464.734 km ... 12286.584,,,,,, 2010-169T18:41:00,000T02:15:00,18-Jun-10,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 133RI OCC Thermal Stabilization,A period of thermal stabilization is required immediately prior to any radio science experiment and test using Ka-band or S-band.,,,,,, 2010-169T20:41:00,000T21:19:00,18-Jun-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-169T20:56:00,000T02:08:10,18-Jun-10,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ansa-to-Ansa Ring Occ - Ingress,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2010-169T23:04:10,000T00:44:00,18-Jun-10,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS Atmospheric Occultation on rev 133 ingress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-169T23:48:10,000T02:21:30,18-Jun-10,CAPS,Prime,Saturn,RNGSATPTG,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-170T01:22:30,001T08:17:30,19-Jun-10,CAPS,SPASS Rider,Saturn,RINGSAT,Ring solar occultation,Rings and Satellites,null,,,,,, 2010-170T02:09:40,000T00:37:20,19-Jun-10,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Atmospheric Occultation on rev 133 egress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-170T02:44:59,000T08:34:00,19-Jun-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-170T02:44:59,000T08:34:00,19-Jun-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-170T02:47:00,000T02:44:47,19-Jun-10,RSS,Prime,rings(general),OCC,Occultation,RSS XM Ansa-to-Ansa Ring Occ - Egress,"XM series of ansa-to-ansa RSS ring occultations spanning the entire ring system on ingress and egress. For these events, we will observe at Ka, X and S bands, subject to power constraints. Observations will commence after a 2-hour period of thermal stabilization and RSS WARMUP mode. We will commence observations with 30 minute free-space baseline and calibration period, followed by the occultation and a subsequent 30 minute free-space baseline and calibration period.",,,,,, 2010-170T05:27:00,000T02:00:00,19-Jun-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-170T05:27:37,000T02:00:00,19-Jun-10,CDA,SPASS Rider,DustRAM direction,RPX0150,,CDA RPXing 2010-170T06:27:37,RPXing at 2.6786408 Rs,,,,,, 2010-170T07:02:42,000T00:00:01,19-Jun-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.623 Rs, lat = 1 deg, phase = 89 deg",,,,,, 2010-170T07:04:00,000T13:36:00,19-Jun-10,CAPS,Prime,Saturn,RNGSATPTG,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-170T11:18:59,000T22:21:01,19-Jun-10,MAG,Non-SPASS,co-rotation,RNGSAT,Ring / Satellite,MAG MAPS RS Campaign,"Observe Saturn's inner magnetosphere and the interactions between icy satellites, rings and the magnetosphere. Measure properties of a statistically significant number of satellite L-shell crossings distributed among the satellites and in longitudinal distance from the satellites.",,,,,, 2010-170T18:00:00,000T02:00:00,19-Jun-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-170T19:44:03,000T15:26:57,19-Jun-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate End: S S61,Range enter= 9.0166044 Rs exit= 15.989779 Range altitude= 12291.049 km ... 11671.218,,,,,, 2010-170T20:00:00,000T17:01:59,19-Jun-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-170T20:40:00,000T03:39:00,19-Jun-10,CAPS,Prime,Saturn,RNGSATPTG,Ring / Satellite,Rings and Satellites,null,,,,,, 2010-171T00:19:00,000T11:32:00,20-Jun-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-171T02:11:00,000T09:00:00,20-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-171T03:11:00,000T04:00:00,20-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10171_SP,rider,,,,,, 2010-171T09:39:00,000T01:32:00,20-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-171T09:40:00,000T13:47:43,20-Jun-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-171T09:40:00,000T01:31:00,20-Jun-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-171T09:40:00,000T01:31:00,20-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-171T11:11:00,000T12:16:43,20-Jun-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-171T11:11:00,000T01:11:03,20-Jun-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate Enter: S S61,Range enter= 9.0166044 Rs exit= 15.989779 Range altitude= 12291.049 km ... 11671.218,,,,,, 2010-171T11:11:00,000T10:16:43,20-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-171T11:11:00,005T09:59:00,20-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-171T12:06:26,000T03:21:17,20-Jun-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-171T12:06:26,000T03:21:17,20-Jun-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-171T12:06:26,000T00:21:17,20-Jun-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Global Mapping,VIMS ridealong with CIRS. Global mapping of Titan. Phase = 149 deg. Lat/Lon = 02N/13 deg. Resolution = 133 km/px. Temp. M4. Obtain cubes of various exposure times for global mapping.,,,,,, 2010-171T12:22:03,005T08:47:57,20-Jun-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 16.001658 Rs Range altitude= 11666.811 km ... -40235.975,,,,,, 2010-171T12:27:43,000T03:00:00,20-Jun-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,VIMS ridealong with CIRS. Stare at Titan. Phase = 149 deg. Lat/Lon = 02N/13 deg. Resolution = 129 km/px. Temp. N. Obtain cubes of various exposure times for global mapping.,,,,,, 2010-171T13:01:59,000T11:25:44,20-Jun-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-171T15:27:43,000T01:00:00,20-Jun-10,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-171T15:27:43,000T01:00:00,20-Jun-10,CIRS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,,Ride along with ISS,,,,,, 2010-171T15:27:43,000T01:00:00,20-Jun-10,VIMS,SPASS Rider,Titan,PHOTOMWAC,Photometry map,Stare at Titan.,VIMS ridealong with ISS for global mapping of Titan. Phase = 149 deg. Lat/Lon = 02N/16 deg. Resolution = 99 km/px. Temp. N. Obtain cubes of various exposure times for global mapping while staring at Titan.,,,,,, 2010-171T16:27:43,000T04:00:00,20-Jun-10,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-171T16:27:43,000T04:00:00,20-Jun-10,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-171T16:27:43,000T04:00:00,20-Jun-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,VIMS ridealong with CIRS for Titan limb mapping. Phase = 149 deg. Lat/Lon = 02N/17 deg. Resolution = 89 km/px. Temp. R. Obtain cubes for limb mapping.,,,,,, 2010-171T20:27:43,000T02:45:00,20-Jun-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-171T20:27:43,000T02:45:00,20-Jun-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-171T20:37:43,000T02:45:00,20-Jun-10,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan Scan.,VIMS ridealong with CIRS slow scan across Titan. Phase = 149 deg. Lat/Lon = 03N/21 deg. Resolution = 47 km/px. Temp. T. Obtain cubes while scanning across Titan.,,,,,, 2010-171T21:27:43,000T08:00:00,20-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-171T21:27:43,000T03:31:00,20-Jun-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T70 flyby,"T70 is the flyby with highest priority for MAG. With an unprecedented altitude of 880 km at closest approach (in the dayside ionosphere), the measurements obtained by MAG will provide important pieces of evidence in favor or against the presence of a dynamo generated magnetic field. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2010-171T23:12:43,000T01:02:00,20-Jun-10,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2010-171T23:12:43,000T01:00:00,20-Jun-10,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-171T23:12:43,000T01:00:00,20-Jun-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,VIMS ridealong with CIRS for regional mapping of Titan. Phase = 148 deg. Lat/Lon = 06N/24 deg. Resolution = 21 km/px. Obtain mosaics for regional mapping of Titan.,,,,,, 2010-171T23:27:43,000T01:00:00,20-Jun-10,CAPS,SPASS Rider,Titan,T70INBD,,Titan Encounter,null,,,,,, 2010-171T23:27:43,000T01:00:00,20-Jun-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-171T23:27:43,000T01:00:00,20-Jun-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-172T00:14:43,000T00:44:00,21-Jun-10,CIRS,SPASS Rider,Titan,T70INPTG,,,Ride along with ISS,,,,,, 2010-172T00:15:43,000T00:43:00,21-Jun-10,CAPS,Prime,Titan,T70INPTG,,Titan Encounter,null,,,,,, 2010-172T00:27:43,000T02:00:00,21-Jun-10,CAPS,SPASS Rider,Titan,T70CLOSE,,Titan Encounter,null,,,,,, 2010-172T00:27:43,000T02:00:00,21-Jun-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-172T00:27:43,000T00:40:00,21-Jun-10,INMS,Non-SPASS,Titan,TITAN70,,Titan Flyby,Titan observation,,,,,, 2010-172T00:27:43,000T02:00:00,21-Jun-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-172T00:58:43,000T00:56:00,21-Jun-10,CIRS,SPASS Rider,Titan,T70CA,,,Ride along with ISS,,,,,, 2010-172T00:58:43,000T00:56:00,21-Jun-10,MAG,SPASS Rider,Titan,MAGTITAN,MAG Titan observation,T70 flyby,"T70 is the flyby with highest priority for MAG. With an unprecedented altitude of 880 km at closest approach (in the dayside ionosphere), the measurements obtained by MAG will provide important pieces of evidence in favor or against the presence of a dynamo generated magnetic field. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2010-172T01:07:43,000T00:40:00,21-Jun-10,INMS,Non-SPASS,Titan,TITAN70,,Titan Flyby,Titan observation,,,,,, 2010-172T01:47:43,000T00:40:00,21-Jun-10,INMS,Non-SPASS,Titan,TITAN70,,Titan Flyby,Titan observation,,,,,, 2010-172T01:54:43,000T00:40:00,21-Jun-10,CIRS,SPASS Rider,Titan,ALPVIRTI,,,Ride along with ISS,,,,,, 2010-172T01:54:43,000T00:21:05,21-Jun-10,UVIS,SPASS Rider,Star,ALPVIRTI,,Titan Occults Alpha Vir,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2010-172T01:54:43,000T00:21:05,21-Jun-10,VIMS,SPASS Rider,Titan,TRANS,,Transition to RWA,VIMS ridealong while transitioning from RCS to RWA. Phase = 139 deg. Lat/Lon = 25N/27 deg. Resolution = 3.3 km/px. Obtain cubes during RCS/RWA transition.,,,,,, 2010-172T01:54:43,000T03:33:00,21-Jun-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T70 flyby,"T70 is the flyby with highest priority for MAG. With an unprecedented altitude of 880 km at closest approach (in the dayside ionosphere), the measurements obtained by MAG will provide important pieces of evidence in favor or against the presence of a dynamo generated magnetic field. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2010-172T02:15:43,000T00:18:55,21-Jun-10,VIMS,SPASS Rider,Titan,LMBMAP,,Limb mapping.,"VIMS ridealong with UVIS for stellar occ and Titan limb mapping. Phase = 139 deg. Lat/Lon = 25N/27 deg. Resolution = 3.3 km/px. Obtain cubes for stellar occ and limb mapping of Titan. Note, RCS/RWA transition occur during this time.",,,,,, 2010-172T02:15:48,000T00:18:55,21-Jun-10,UVIS,Prime,Star,ALPVIRTI,,Titan Occults Alpha Vir,UVIS FUV Occultation slit boresite on star for the entire time. Note: Start time may change depending on trajectory updates.,,,,,, 2010-172T02:27:43,000T01:00:00,21-Jun-10,CAPS,SPASS Rider,Titan,T70OUTBND,,Titan Encounter,null,,,,,, 2010-172T02:27:43,000T01:00:00,21-Jun-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-172T02:27:43,003T08:28:42,21-Jun-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-172T02:27:43,000T01:00:00,21-Jun-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-172T02:34:43,000T00:53:00,21-Jun-10,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,Regional mapping of Titan. Phase = 31 deg. Lat/Lon = 03S/207 deg. Resolution = 15 km/px. Obtain mosaics for regional mapping of Titan,,,,,, 2010-172T02:34:43,000T00:53:00,21-Jun-10,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS,,,,,, 2010-172T03:04:43,000T00:23:00,21-Jun-10,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-172T03:27:43,000T03:00:00,21-Jun-10,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,Regional mapping of Titan. Phase = 31 deg. Lat/Lon = 04S/208 deg. Resolution = 19 km/px. Continue mosaics for regional mapping of Titan,,,,,, 2010-172T03:27:43,000T17:02:17,21-Jun-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-172T03:27:43,000T03:00:00,21-Jun-10,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS,,,,,, 2010-172T03:27:43,000T03:00:00,21-Jun-10,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-172T03:27:43,000T17:02:42,21-Jun-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-172T05:27:43,000T15:02:17,21-Jun-10,MAG,Non-SPASS,Saturn,DUSKMSPH,,MAG MAPS DUSKMSPH Campaign,Investigate the previously unobserved dusk flank of Saturn's magnetosphere.,,,,,, 2010-172T06:27:43,000T03:30:00,21-Jun-10,VIMS,Prime,Titan,MEDRES,Medium resolution global mapping,Regional mapping of Titan.,Regional mapping of Titan. Phase = 32 deg. Lat/Lon = 08S/211 deg. Resolution = 49 km/px. Obtain mosaics for medium res. regional mapping of Titan,,,,,, 2010-172T06:27:43,000T03:30:00,21-Jun-10,CIRS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,,Ride along with ISS,,,,,, 2010-172T06:27:43,000T03:30:00,21-Jun-10,ISS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-172T09:57:43,000T00:30:00,21-Jun-10,ISS,Prime,Titan,PHOTOMWAC,Photometry map,WPH (WAC Photometry),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-172T09:57:43,000T00:30:00,21-Jun-10,CIRS,SPASS Rider,Titan,RIDER,Instrument rider,,Ride along with ISS,,,,,, 2010-172T09:57:43,000T00:30:00,21-Jun-10,VIMS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,Global Mapping,VIMS ridealong with ISS for global mapping of Titan. Phase = 33 deg. Lat/Lon = 08S/214 deg. Resolution = 83 km/px. Temp. I. Obtain 64x64 cubes for global mapping.,,,,,, 2010-172T10:27:43,000T05:00:00,21-Jun-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan.,Global mapping of Titan. Phase = 33 deg. Lat/Lon = 09S/214 deg. Resolution = 88 km/px. Obtain cubes for global mapping of Titan,,,,,, 2010-172T10:27:43,000T05:00:00,21-Jun-10,CIRS,SPASS Rider,Titan,RIDER,Instrument rider,,Ride along with ISS,,,,,, 2010-172T10:27:43,000T05:00:00,21-Jun-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-172T19:56:00,000T09:00:00,21-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-172T20:30:00,002T20:00:00,21-Jun-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-172T20:30:00,002T14:26:00,21-Jun-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-172T20:30:00,001T08:26:00,21-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-172T20:56:00,000T08:00:00,21-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10172_SP,rider,,,,,, 2010-173T05:36:00,000T02:00:00,22-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-173T07:36:00,000T10:10:00,22-Jun-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-173T07:36:00,000T10:10:00,22-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 35 deg. Lat/Lon = 09S/230 deg. Resolution = 284 km/px.,,,,,, 2010-173T18:26:00,000T01:30:00,22-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-173T18:26:00,000T01:30:00,22-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 35 deg. Lat/Lon = 09S/233 deg. Resolution = 322 km/px.,,,,,, 2010-173T19:56:00,000T09:00:00,22-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-173T20:56:00,000T08:00:00,22-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10173_SP,rider,,,,,, 2010-174T04:56:00,001T07:15:00,23-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-174T05:36:00,000T06:24:00,23-Jun-10,ISS,Prime,Titan,CLOUD,,Titan cloud monitoring and gap filling (TCM),Cloud monitoring,,,,,, 2010-174T12:00:00,000T02:00:00,23-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-174T14:00:00,000T01:15:00,23-Jun-10,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 39 range 1.1 Mkm",,,,,, 2010-174T14:00:00,000T01:15:00,23-Jun-10,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-174T14:00:00,000T01:15:00,23-Jun-10,UVIS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-174T14:00:00,000T01:15:00,23-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with ISS for cloud monitoring. Phase = 41 deg. Lat/Lon = 09S/254 deg. Resolution = 626 km/px.,,,,,, 2010-174T15:15:00,000T10:01:00,23-Jun-10,CIRS,Prime,rings(general),POLARIZ,,CIRS_133RI_POLARIZ173_PRIME;,null,,,,,, 2010-174T15:15:00,000T10:00:00,23-Jun-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud Monitoring.,Caboose segment. VIMS ridealong with CIRS for cloud monitoring. Phase = 41 deg. Lat/Lon = 09S/255 deg. Resolution = 640 km/px.,,,,,, 2010-175T01:56:00,000T09:00:00,24-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-175T02:56:00,000T08:00:00,24-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10175_SP,rider,,,,,, 2010-175T10:56:00,000T01:15:00,24-Jun-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 46.1 range 1.7 Mkm",,,,,, 2010-175T10:56:00,000T01:15:00,24-Jun-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-175T10:56:00,001T10:14:00,24-Jun-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-175T10:56:00,000T01:15:00,24-Jun-10,UVIS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-175T10:56:00,000T01:15:00,24-Jun-10,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 46.1 range 1.7 Mkm",,,,,, 2010-175T10:56:00,001T10:14:00,24-Jun-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-175T10:56:00,001T10:14:00,24-Jun-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-175T12:00:00,000T08:00:00,24-Jun-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-175T12:11:00,000T06:45:00,24-Jun-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales. Added to improve calibration for T70, conditions are not ideal but is maximum distance reached outside magnetopause after T70.",,,,,, 2010-175T12:11:00,000T06:45:00,24-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-175T16:30:00,001T04:40:00,24-Jun-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-175T18:56:00,000T04:15:00,24-Jun-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-175T18:56:00,000T04:15:00,24-Jun-10,CIRS,SPASS Rider,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-175T18:56:00,001T02:14:00,24-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-175T23:11:00,000T04:49:00,24-Jun-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-176T04:00:00,000T08:10:00,25-Jun-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-176T12:10:00,000T09:00:00,25-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-176T13:10:00,000T08:00:00,25-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10176_SP,rider,,,,,, 2010-176T21:10:00,005T16:50:00,25-Jun-10,CAPS,SPASS Rider,SolarWind,SWAURORA,Solar wind campaign,MAPS Solar Wind/Aurora/SKR,null,,,,,, 2010-176T21:10:00,001T08:14:00,25-Jun-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-176T21:10:00,001T08:13:00,25-Jun-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Range enter= 16.001658 Rs Range altitude= 11666.811 km ... -40235.975,,,,,, 2010-176T21:10:00,000T00:43:00,25-Jun-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-176T21:10:00,001T15:15:00,25-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-176T21:10:00,001T08:13:00,25-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-176T21:10:00,001T08:13:00,25-Jun-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-176T21:15:00,000T00:02:00,25-Jun-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S61 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-176T21:50:00,000T01:30:00,25-Jun-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 55.9 requested range 2.3 Mkm",,,,,, 2010-176T21:50:00,000T01:30:00,25-Jun-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-176T21:50:00,000T01:30:00,25-Jun-10,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-176T21:53:00,000T00:07:00,25-Jun-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-176T22:00:00,000T00:05:00,25-Jun-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-176T22:05:00,000T00:33:00,25-Jun-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-176T22:38:00,000T00:22:59,25-Jun-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-176T23:00:59,001T06:23:01,25-Jun-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-176T23:20:00,000T04:30:00,25-Jun-10,CIRS,Prime,rings(general),EQLBS,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-177T03:35:00,000T13:55:00,26-Jun-10,UVIS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2010-177T03:50:00,000T13:40:00,26-Jun-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-177T03:50:00,000T13:40:00,26-Jun-10,ISS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC 2x2 image per 3.20 minutes. 20.8 Mbits/hr following ISS_119SU_SWAURPTG001_CAPS,,,,,, 2010-177T18:10:00,000T10:30:00,26-Jun-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-177T19:40:00,000T09:00:00,26-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-177T20:40:00,000T08:00:00,26-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_133IC_DSCAL10177_SP,rider,,,,,, 2010-178T04:40:00,000T09:45:00,27-Jun-10,ISS,Prime,Star,CALSTAR3,Stellar Calibration,ISS Photometric Calibration Star 3,"Photometric Calibration Star 3 (HD 20630 = HR 996, Vmag 4.83, G5V)",,,,,, 2010-178T05:23:00,005T15:16:00,27-Jun-10,CDA,Non-SPASS,Other,RATE010A,,Data rate,Background data rate,,,,,, 2010-178T05:23:00,005T15:16:00,27-Jun-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-178T05:24:00,004T08:36:00,27-Jun-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-178T05:24:00,000T09:36:00,27-Jun-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-178T05:25:58,000T00:00:01,27-Jun-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 19.1 deg, r = 37.556 Rs, phase = 92 deg",,,,,, 2010-178T06:00:00,000T12:00:00,27-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-178T12:25:00,000T05:00:00,27-Jun-10,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2010-178T14:25:00,000T03:05:00,27-Jun-10,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2010-178T14:25:00,000T03:05:00,27-Jun-10,ISS,SPASS Rider,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,Spica calibration,Rider to UVIS calibration of Spica. ISS Calibrations for UV filters and to test if bleed charge can be used for calibration,,,,,, 2010-178T15:00:00,000T01:37:00,27-Jun-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-178T16:37:00,000T00:34:00,27-Jun-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2010-178T17:11:00,002T17:29:00,27-Jun-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-178T17:25:00,000T11:00:00,27-Jun-10,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-25 in 1-way mode. No rolling during first 3 hours (USO).,,,,,, 2010-178T17:25:00,003T06:35:00,27-Jun-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-178T19:25:00,000T09:00:00,27-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-178T20:25:00,000T08:00:00,27-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10178_SP,rider,,,,,, 2010-179T04:25:00,000T05:35:00,28-Jun-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-179T04:25:00,000T05:35:00,28-Jun-10,ISS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC 2x2 image per 3.20 minutes. 20.8 Mbits/hr following ISS_119SU_SWAURPTG001_CAPS,,,,,, 2010-179T04:35:00,000T05:50:00,28-Jun-10,UVIS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2010-179T10:25:00,000T10:30:00,28-Jun-10,CDA,SPASS Rider,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-179T11:55:00,000T09:00:00,28-Jun-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev135 Saturn atmospheric occultation on 2010/205.",,,,,, 2010-179T11:55:00,000T09:00:00,28-Jun-10,RPWS,Non-SPASS,Saturn,SWAURORA,Solar wind campaign,MAPS SW2 Campaign,Part of SW2 MAPS Campaign. Monitor the solar wind while Cassini is well upstream of Saturn's bow shock in coordination with RPWS and Earth based observations of Saturn's aurora,,,,,, 2010-179T11:55:00,000T09:00:00,28-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-179T12:55:00,000T08:00:00,28-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10179_SP,rider,,,,,, 2010-179T21:35:00,000T01:30:00,28-Jun-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 74.8 requested range 3.1 Mkm",,,,,, 2010-179T21:35:00,000T01:30:00,28-Jun-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-179T21:35:00,000T01:30:00,28-Jun-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-179T23:05:00,000T10:00:00,28-Jun-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_134SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Southern hemisphere",,,,,, 2010-180T04:30:00,000T12:00:00,29-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-180T09:05:00,000T04:00:00,29-Jun-10,CAPS,Prime,InstrumentCalibration,CALIBRATE,Calibration,Full Calibration,null,,,,,, 2010-180T09:05:00,000T09:10:00,29-Jun-10,UVIS,SPASS Rider,InstrumentCalibration,CALIBRATE,Calibration,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2010-180T13:05:00,000T11:55:00,29-Jun-10,CAPS,Prime,SolarWind,SWAURPTG,MAPS aurora campaign,MAPS Survey w/ prime pointing,null,,,,,, 2010-180T14:05:00,000T00:55:28,29-Jun-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-180T18:15:00,000T06:45:00,29-Jun-10,ISS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,NAC aurora stare,CL1 NAC 2x2 image per 3.20 minutes. 20.8 Mbits/hr following ISS_119SU_SWAURPTG001_CAPS,,,,,, 2010-180T18:15:00,000T06:45:00,29-Jun-10,UVIS,SPASS Rider,SolarWind,SWAURPTG,MAPS aurora campaign,Auroral imaging during solar wind campaign,Fixed Stare at the auroral zone,,,,,, 2010-181T01:40:00,000T09:00:00,30-Jun-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-181T02:40:00,000T08:00:00,30-Jun-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10181_SP,rider,,,,,, 2010-181T10:40:00,001T00:00:00,30-Jun-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-181T11:00:00,000T09:00:00,30-Jun-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-181T11:20:00,000T01:00:00,30-Jun-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 8 satellites if visible",,,,,, 2010-181T12:20:00,000T12:40:00,30-Jun-10,ISS,Prime,rings(general),SPKMVDFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2010-182T00:00:00,000T11:20:00,1-Jul-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-182T02:40:00,000T08:00:00,1-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10182_SP,rider,,,,,, 2010-182T10:40:00,002T17:29:00,1-Jul-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-182T11:00:00,000T09:00:00,1-Jul-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-182T11:20:00,000T06:45:00,1-Jul-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-182T14:00:00,000T22:00:00,1-Jul-10,CAPS,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,Magnetospheric Boundaries Campaign,null,,,,,, 2010-182T14:00:00,000T22:00:00,1-Jul-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-182T18:05:00,000T10:24:00,1-Jul-10,ISS,Prime,rings(general),SPKMVDFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2010-182T18:05:00,000T17:50:00,1-Jul-10,MAG,Non-SPASS,Sun,MAGBOUND,MAPS magnetosphere boundary campaign,MAG MAPS MAGBOUND Campaign,Observe magnetospheric boundaries near noon on highly inclined orbits.,,,,,, 2010-183T04:29:00,000T05:00:00,2-Jul-10,CIRS,Prime,rings(general),TMAPS,,,null,,,,,, 2010-183T04:29:00,000T05:00:00,2-Jul-10,ISS,SPASS Rider,rings(general),TMAPS,,,Spoke periodicity movie. riding along on CIRS TMAP obs.,,,,,, 2010-183T11:39:00,000T09:00:00,2-Jul-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev135 Saturn atmospheric occultation on 2010/205.",,,,,, 2010-183T11:55:00,002T12:20:00,2-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-183T12:00:00,000T08:39:00,2-Jul-10,CAPS,SPASS Rider,Saturn,DUSKMSPH,,Dusk Magnetosphere observations,null,,,,,, 2010-183T12:00:00,001T16:09:00,2-Jul-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-183T12:39:00,000T08:00:00,2-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10183_SP,rider,,,,,, 2010-183T20:39:00,001T07:30:00,2-Jul-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-183T20:39:00,001T07:30:00,2-Jul-10,CDA,Non-SPASS,Other,RATE010A,,Data rate,Background data rate,,,,,, 2010-183T20:39:00,001T05:00:00,2-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-183T21:19:00,000T16:10:00,2-Jul-10,ISS,Prime,rings(general),SPKMVDFHP,,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2010-184T13:29:00,000T05:00:00,3-Jul-10,CIRS,Prime,rings(general),TMAPS,,,"Either cut focal plane, or co-add",,,,,, 2010-184T13:29:00,000T05:00:00,3-Jul-10,ISS,SPASS Rider,rings(general),TMAPS,,,Spoke periodicity movie. riding along on CIRS TMAP obs.,,,,,, 2010-184T20:09:00,000T04:00:00,3-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10184_SP,rider,,,,,, 2010-185T01:39:00,000T02:30:00,4-Jul-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-185T04:09:00,000T07:15:00,4-Jul-10,ISS,Prime,RingD,DRCLOSE,,D Ring Close-in observation,D Ring Close-In Observation,,,,,, 2010-185T04:09:00,002T06:00:00,4-Jul-10,MIMI,SPASS Rider,Saturn,PERIAPSIS,,MIMI Periapsis survey,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-185T04:09:00,000T07:15:00,4-Jul-10,VIMS,SPASS Rider,RingD,DRCLOSE,,Stare at D ring,"320 ms, 64x64 or as required",,,,,, 2010-185T04:09:00,002T06:00:00,4-Jul-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-185T04:09:00,000T21:33:00,4-Jul-10,CDA,Non-SPASS,Other,RATE010A,,Data rate,Background data rate,,,,,, 2010-185T04:09:00,000T07:15:00,4-Jul-10,CIRS,Non-SPASS,rings(general),DRCLOSE,,,null,,,,,, 2010-185T04:09:00,000T00:51:00,4-Jul-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-185T04:09:00,002T04:05:00,4-Jul-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-185T05:00:00,000T15:24:00,4-Jul-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-185T11:24:00,000T09:00:00,4-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-185T12:24:00,000T08:00:00,4-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10185_SP,rider,,,,,, 2010-185T18:00:00,000T22:00:00,4-Jul-10,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2010-185T20:24:00,000T06:09:12,4-Jul-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-185T20:55:00,000T01:05:00,4-Jul-10,ISS,Prime,rings(general),PROPELLR,,Propeller tracking,Image rings at high resolution to track propellers.,,,,,, 2010-185T20:55:00,000T01:05:00,4-Jul-10,CIRS,Non-SPASS,rings(general),PROPELLR,,,null,,,,,, 2010-185T22:00:00,000T02:15:00,4-Jul-10,CIRS,Prime,Enceladus,GLOBAL,Polarimetry,CIRS_134EN_GLOBAL001_PRIME;,"Global FP3, FP4 scans of the southern hemisphere of Enceladus, and an FP1 stare. Purpose: thermal output monitoring All scans should be long enough that both FP3 *and* FP4 cover the entire specified target. Details: 22:00 to 22:04 Set up for following FP3/4 scan, with shutter closed. 22:04 to 22:20 Limb to limb FP3/4 scan, 6 murad/sec, FP3/4 center passing through the center of Enceladus. 22:20 to 22:40 Repeat (in the opposite direction, to avoid having to move back to the starting location), but biased southward so the edge of the FP3/4 fovs just touches the lower limb. 22:40 to 22:50 FP1 disk-integrated stare, centered on disk, 3 cm-1 resolution. 22:50 to 23:00 FP1 stare, centered on south pole, 3 cm-1 resolution. 23:00 to 23:25 Limb to limb FP3/4 scan, 6 murad/sec, biased southward so the edge of the FP3/4 fovs just touches the lower limb. 23:25 to 23:50 Very slow FP3/FP4 scan, ~3 murad/sec, covering just the region south of 60 S with both detectors. Again, the edge of the scan should just touch the lower limb of Enceladus. 23:50 to 00:15 Repeat (in the opposite direction, to avoid having to move back to the starting location), again with the edge of the scan just touching the lower limb of Enceladus. Resolution 15 cm-1 unless otherwise noted.",,,,,, 2010-185T22:00:00,000T02:15:00,4-Jul-10,ISS,SPASS Rider,Enceladus,GLOBAL,Polarimetry,Enceladus,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-185T22:00:00,000T02:15:00,4-Jul-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,,,,,,, 2010-185T22:00:00,000T02:15:00,4-Jul-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus composition,Enceladus mapping,,,,,, 2010-186T00:15:00,000T03:30:00,5-Jul-10,UVIS,Prime,Saturn,ENAURFOOT,,Search for Enceladus Auroral Footprint,"Slow repeated slews across Saturn's auroral zone, emphasizing Enceladus-related auroras This means slews should cover 55-90 latitude. They should also cover the sub-Enceladus longitude between 60-70 latitude.",,,,,, 2010-186T00:15:00,000T00:25:00,5-Jul-10,MAG,Non-SPASS,Enceladus,ENAURFOOT,,EnAurFoot PIE,MAPS EnAurFoot PIE observation,,,,,, 2010-186T00:40:00,000T03:05:00,5-Jul-10,MAG,Non-SPASS,Enceladus,ENAURFOOT,,EnAurFoot PIE,MAPS EnAurFoot PIE observation Overlaps another request so zero datarate.,,,,,, 2010-186T00:40:00,000T09:00:00,5-Jul-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-186T01:42:00,000T03:52:00,5-Jul-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 3.9306312 Rs exit= 2.9991815 Range altitude= -39872.758 km ... 39862.488,,,,,, 2010-186T02:32:00,000T02:00:00,5-Jul-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-186T02:33:12,000T02:00:00,5-Jul-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-186T02:37:00,000T02:00:00,5-Jul-10,CDA,SPASS Rider,DustRAM direction,RPX0000,,CDA RPXing 2010-186T03:37:00,RPXing at 3.1857510 Rs,,,,,, 2010-186T04:20:00,000T03:55:00,5-Jul-10,VIMS,Prime,rings(general),HIRESLLP,,High Resolution Ring Monitor,"Lit face, low phase (98-32 degrees).. Target Daphnis first 25 min.",,,,,, 2010-186T04:20:00,000T00:30:00,5-Jul-10,ISS,SPASS Rider,rings(general),HIRESLLP,,Daphnis close flyby,"daphnis close flyby, ~80,000, 70 deg phase",,,,,, 2010-186T04:20:00,000T03:55:00,5-Jul-10,CIRS,Non-SPASS,rings(general),HIRESLLP,,,null,,,,,, 2010-186T04:33:12,000T23:00:00,5-Jul-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-186T05:01:39,000T00:00:01,5-Jul-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 2.967 Rs, lat = 10 deg, phase = 88 deg",,,,,, 2010-186T05:34:00,003T04:35:00,5-Jul-10,CDA,Non-SPASS,Other,RATE010B,,Data rate,Background data rate,,,,,, 2010-186T08:15:00,000T04:00:00,5-Jul-10,UVIS,Prime,Star,URALPVIR,Stellar occultation,URSTAR,Ingress occ of very bright star at low incidence angle. Gives atmospheric occultation at end of ring occ.,,,,,, 2010-186T08:15:00,000T04:00:00,5-Jul-10,UVIS,SPASS Rider,Star,URALPVIR,Stellar occultation,Support Imaging,NAC and WAC support images at: 2010-186T09:05:42 2010-186T09:42:49,,,,,, 2010-186T08:15:00,000T04:00:00,5-Jul-10,CIRS,Non-SPASS,rings(general),URALPVIR,Stellar occultation,,null,,,,,, 2010-186T09:40:00,001T10:42:45,5-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-186T12:15:00,000T07:00:00,5-Jul-10,CIRS,Prime,rings(general),P50L30S15,,,null,,,,,, 2010-186T12:15:00,000T07:00:00,5-Jul-10,CIRS,SPASS Rider,rings(general),P50L30S15,,,Priority: M/N~1/2; other opps exist unless otherwise noted.,,,,,, 2010-186T19:15:00,000T04:00:00,5-Jul-10,UVIS,Prime,rings(general),RINGMAP,,URSPEC,Dedicated UV spectral mapping of Saturn's rings. Spatial variation of UV albedo and water absorption edge indicative of scattering center size scale.,,,,,, 2010-186T19:15:00,000T04:00:00,5-Jul-10,CIRS,Non-SPASS,rings(general),RINGMAP,,,null,,,,,, 2010-187T01:09:00,000T09:00:00,6-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-187T02:09:00,000T08:00:00,6-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10187_SP,rider,,,,,, 2010-187T03:33:12,000T06:35:48,6-Jul-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-187T08:14:00,000T01:55:00,6-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-187T10:09:00,000T12:13:45,6-Jul-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-187T10:09:00,000T12:13:45,6-Jul-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-187T10:09:00,000T02:13:45,6-Jul-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-187T10:09:00,002T00:00:00,6-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-187T11:07:45,000T04:15:00,6-Jul-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-187T11:07:45,000T04:15:00,6-Jul-10,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2010-187T11:07:45,000T04:15:00,6-Jul-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Global mapping.,VIMS ridealong with CIRS for global mapping of Titan. Phase = 146 deg. Lat/Lon = 09N/13 deg. Resolution = 133 km/px. Temp. N and M4. Obtain cubes of various exposure times for global mapping.,,,,,, 2010-187T12:22:45,000T11:00:00,6-Jul-10,INMS,Non-SPASS,Titan,T71INBND,,Titan flyby,Titan observation,,,,,, 2010-187T15:22:45,000T03:00:00,6-Jul-10,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-187T15:22:45,000T03:00:00,6-Jul-10,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2010-187T15:22:45,000T03:00:00,6-Jul-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping.,VIMS ridealong with CIRS for limb mapping of Titan. Phase = 146 deg. Lat/Lon = 09N/17 deg. Resolution = 89 km/px. Temp. R1. Obtain cubes of various exposure times for limb mapping.,,,,,, 2010-187T15:22:45,000T03:00:00,6-Jul-10,RADAR,Non-SPASS,Titan,T71WARMUP,,Warmup for T71,,,,,,, 2010-187T18:22:45,000T03:45:00,6-Jul-10,RADAR,Prime,Titan,T71INRAD,,T71 Inbound Radiometry,,,,,,, 2010-187T20:22:45,000T08:00:00,6-Jul-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T71 flyby,"T71 is a low altitude, pre-dusk flyby over the south pole. Its geometry is similar to T70. This will allow a comparison of the field line geometry in the induced magnetosphere. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2010-187T22:07:45,000T01:26:00,6-Jul-10,RADAR,Prime,Titan,T71FCAPS,,T71 Request for CAPS Inbound,,,,,,, 2010-187T22:07:45,000T01:26:00,6-Jul-10,CAPS,SPASS Rider,Titan,T71INPTG,,Titan Encounter,null,,,,,, 2010-187T22:22:45,000T04:00:00,6-Jul-10,CAPS,SPASS Rider,Titan,T71CLOSE,,Closest Approach 134TI (T71),Closest Approach 117TI (T61),,,,,, 2010-187T22:22:45,000T01:00:00,6-Jul-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-187T22:22:45,000T01:00:00,6-Jul-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-187T23:22:45,000T02:00:00,6-Jul-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-187T23:22:45,000T00:30:00,6-Jul-10,INMS,Non-SPASS,Titan,TITAN71,,Titan Flyby,Titan observation,,,,,, 2010-187T23:22:45,000T00:42:00,6-Jul-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-187T23:34:45,000T00:30:00,6-Jul-10,RADAR,Prime,Titan,T71FCAPS,,T71 Request for CAPS Inbound,,,,,,, 2010-187T23:34:45,000T00:30:00,6-Jul-10,CAPS,SPASS Rider,Titan,T71INPTG,,Titan Encounter,null,,,,,, 2010-187T23:52:45,000T00:25:30,6-Jul-10,INMS,Non-SPASS,Titan,TITAN71,,Titan Flyby,Titan observation,,,,,, 2010-188T00:04:45,000T00:36:00,7-Jul-10,RADAR,Prime,Titan,T71RASAR,,T71 Ride-along SAR with INMS at C/A,,,,,,, 2010-188T00:04:45,000T00:36:00,7-Jul-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-188T00:18:15,000T00:08:40,7-Jul-10,INMS,Non-SPASS,Titan,TITAN71,,Titan Flyby,Titan observation,,,,,, 2010-188T00:26:55,000T00:55:50,7-Jul-10,INMS,Non-SPASS,Titan,TITAN71,,Titan Flyby,Titan observation,,,,,, 2010-188T00:40:45,000T00:10:00,7-Jul-10,RADAR,Prime,Titan,T71FCAPS,,T71 Request for CAPS Outbound,,,,,,, 2010-188T00:40:45,000T00:10:00,7-Jul-10,CAPS,SPASS Rider,Titan,T71INPTG,,Titan Encounter,null,,,,,, 2010-188T00:40:45,000T00:42:00,7-Jul-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-188T01:12:45,000T01:25:00,7-Jul-10,RADAR,Prime,Titan,T71FCAPS,,T71 Request for CAPS Outbound,,,,,,, 2010-188T01:12:45,000T01:25:00,7-Jul-10,CAPS,SPASS Rider,Titan,T71INPTG,,Titan Encounter,null,,,,,, 2010-188T01:22:45,000T01:00:00,7-Jul-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-188T01:22:45,000T11:00:00,7-Jul-10,INMS,Non-SPASS,Titan,T71OUTBND,,Titan flyby,Titan observation,,,,,, 2010-188T01:22:45,000T01:00:00,7-Jul-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-188T02:22:45,001T07:46:15,7-Jul-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-188T02:22:45,002T07:46:15,7-Jul-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-188T02:37:45,000T03:45:00,7-Jul-10,RADAR,Prime,Titan,T71OUTRAD,,T71 Outbound Radiometry,,,,,,, 2010-188T04:22:45,001T05:46:15,7-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-188T06:22:45,000T03:00:00,7-Jul-10,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional Mapping,2.2 mosaic for Regional mapping of Titan. Phase = 35 deg. Lat/Lon = 04S/208 deg. Resolution = 58 km/px. Obtain cubes for regional mapping of Titan.,,,,,, 2010-188T06:22:45,000T03:00:00,7-Jul-10,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS.,,,,,, 2010-188T06:22:45,000T03:00:00,7-Jul-10,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-188T09:22:45,000T05:00:00,7-Jul-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Regional Mapping,Global mapping of Titan. Phase = 35 deg. Lat/Lon = 04S/210 deg. Resolution = 88 km/px. Obtain cubes for global mapping of Titan,,,,,, 2010-188T09:22:45,000T05:00:00,7-Jul-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-188T09:22:45,000T05:00:00,7-Jul-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-188T12:22:45,000T21:46:15,7-Jul-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-188T14:22:45,000T03:35:00,7-Jul-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping + cloud,Global mapping of Titan. Phase = 36 deg. Lat/Lon = 03S/214 deg. Resolution = 139 km/px.,,,,,, 2010-188T14:22:45,000T03:35:00,7-Jul-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-188T14:22:45,000T03:35:00,7-Jul-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-188T18:54:00,000T06:15:00,7-Jul-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev135 Saturn atmospheric occultation on 2010/205.",,,,,, 2010-188T18:54:00,000T15:15:00,7-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-188T19:54:00,000T05:15:00,7-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10188_SP,rider,,,,,, 2010-189T02:09:00,000T08:00:00,8-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10189_SP,rider,,,,,, 2010-189T10:09:00,001T00:00:00,8-Jul-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-189T10:09:00,001T00:00:00,8-Jul-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Background data rate,,,,,, 2010-189T10:09:00,001T00:00:00,8-Jul-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Titan flyby,Titan observation,,,,,, 2010-189T10:09:00,001T00:00:00,8-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-189T10:09:00,001T00:00:00,8-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-189T10:49:00,000T02:00:00,8-Jul-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS MAGBOUND w/ prime pointing,null,,,,,, 2010-189T12:49:00,000T10:10:00,8-Jul-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-189T12:49:00,000T10:10:00,8-Jul-10,ISS,SPASS Rider,Titan,COMPMAP,Composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-189T12:49:00,000T11:40:00,8-Jul-10,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Cloud Mapping,Cloud mapping of Titan during caboose segment. Phase = 38 deg. Lat/Lon = 03S/232 deg. Resolution = 374 km/px.,,,,,, 2010-189T23:39:00,000T11:10:00,8-Jul-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-190T02:09:00,000T08:00:00,9-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10190_SP,rider,,,,,, 2010-190T10:09:00,005T18:12:00,9-Jul-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-190T10:09:00,005T18:12:00,9-Jul-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-190T10:09:00,005T18:12:00,9-Jul-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Background data rate,,,,,, 2010-190T10:09:00,000T23:44:00,9-Jul-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-190T10:09:00,002T00:24:00,9-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-190T10:09:00,001T23:44:00,9-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-190T10:49:00,000T01:30:00,9-Jul-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 42.7 requested range 1.2 Mkm",,,,,, 2010-190T10:49:00,000T01:30:00,9-Jul-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-190T10:49:00,000T01:30:00,9-Jul-10,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 42.7 range 1.2 Mkm",,,,,, 2010-190T12:19:00,000T11:54:00,9-Jul-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-190T12:19:00,000T11:54:00,9-Jul-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-191T00:00:00,001T00:00:00,10-Jul-10,RPWS,Non-SPASS,InstrumentCalibration,PIM,Periodic Instrument maintenance,RPWS PIM,"Perform RPWS PIM, Bias the Langmuir Probe to remove any contamination",,,,,, 2010-191T00:53:00,000T09:00:00,10-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-191T01:53:00,000T08:00:00,10-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10191_SP,rider,,,,,, 2010-191T09:53:00,001T00:00:00,10-Jul-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-191T10:33:00,000T13:40:00,10-Jul-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_134SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-191T10:33:00,000T13:40:00,10-Jul-10,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP ridealong,CIRS Ridealong for full Saturn rotation,,,,,, 2010-192T00:53:00,000T09:00:00,11-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-192T01:53:00,000T08:00:00,11-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10192_SP,rider,,,,,, 2010-192T09:53:00,003T18:28:00,11-Jul-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-192T09:53:00,003T18:28:00,11-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-192T10:33:00,000T06:45:00,11-Jul-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-192T17:18:00,000T05:00:00,11-Jul-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 botsim, MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-192T17:18:00,000T05:00:00,11-Jul-10,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS WIND5HR Ridealong #1,ISS WIND5HR Ridealong for half Saturn rotation,,,,,, 2010-192T17:18:00,012T09:34:00,11-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-192T17:18:00,000T05:00:00,11-Jul-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-192T22:18:00,000T06:00:00,11-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_134SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-192T22:18:00,000T06:00:00,11-Jul-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #1,CIRS Ridealong for half Saturn rotation,,,,,, 2010-192T22:18:00,000T06:00:00,11-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-193T04:18:00,000T05:00:00,12-Jul-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 botsim, MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-193T04:18:00,000T05:00:00,12-Jul-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-193T09:18:00,000T06:00:00,12-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_134SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-193T09:18:00,000T06:00:00,12-Jul-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong #2,CIRS Ridealong for half Saturn rotation,,,,,, 2010-193T09:18:00,000T06:00:00,12-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-193T18:38:00,000T09:00:00,12-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-193T20:08:00,000T04:00:00,12-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10193_SP,rider,,,,,, 2010-194T04:18:00,000T05:00:00,13-Jul-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 botsim, MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-194T04:18:00,000T05:00:00,13-Jul-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-194T09:18:00,000T06:00:00,13-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_134SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-194T09:18:00,000T06:00:00,13-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-194T15:18:00,000T05:00:00,13-Jul-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 botsim, MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-194T15:18:00,000T05:00:00,13-Jul-10,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS WIND5HR Ridealong #4,ISS WIND5HR Ridealong for half Saturn rotation,,,,,, 2010-194T15:18:00,000T05:00:00,13-Jul-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-194T20:18:00,000T03:00:00,13-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_134SA_COMPSIT005,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-194T20:18:00,000T03:00:00,13-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-195T00:00:00,000T01:08:00,14-Jul-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-195T00:53:00,000T09:00:00,14-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-195T01:53:00,000T04:00:00,14-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_134IC_DSCAL10195_SP,rider,,,,,, 2010-195T10:33:00,000T20:00:00,14-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_134SA_COMPSIT006,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-195T10:33:00,000T20:00:00,14-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-196T04:18:59,000T00:00:01,15-Jul-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 19.9 d, inc = 4.5 deg, r = 43.515 Rs, phase = 97 deg",,,,,, 2010-196T04:21:00,005T05:39:00,15-Jul-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-196T04:21:00,011T04:45:00,15-Jul-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-196T04:21:00,009T10:45:00,15-Jul-10,CDA,Non-SPASS,Other,RATE010A,,Data rate,Background data rate,,,,,, 2010-196T04:21:00,000T01:39:00,15-Jul-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-196T04:21:00,008T19:29:00,15-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-196T06:00:00,000T02:00:00,15-Jul-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-196T06:33:00,000T11:00:00,15-Jul-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-196T06:33:00,000T11:00:00,15-Jul-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-196T08:00:00,003T01:37:00,15-Jul-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-196T17:33:00,000T04:00:00,15-Jul-10,ISS,Prime,Other,KIVPHA,,Kiviuq,Observation of irregular moon of Saturn. Timing flexible within apoapsis period.,,,,,, 2010-196T17:33:00,000T04:00:00,15-Jul-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-196T21:33:00,000T01:30:00,15-Jul-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 62.3 requested range 3.8 Mkm",,,,,, 2010-196T21:33:00,000T01:30:00,15-Jul-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-196T21:33:00,000T01:30:00,15-Jul-10,UVIS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-196T21:33:00,000T01:30:00,15-Jul-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 62.3 range 3.8 Mkm",,,,,, 2010-197T00:38:00,000T09:00:00,16-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-197T01:38:00,000T08:00:00,16-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10197_SP,rider,,,,,, 2010-197T10:00:00,000T09:00:00,16-Jul-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-197T10:18:00,000T13:00:00,16-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_135SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-197T10:18:00,000T13:00:00,16-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-197T23:28:00,000T00:30:00,16-Jul-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-198T00:38:00,000T09:00:00,17-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-198T01:38:00,000T08:00:00,17-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10198_SP,rider,,,,,, 2010-198T10:00:00,000T09:00:00,17-Jul-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-198T10:18:00,000T13:39:00,17-Jul-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-198T10:18:00,000T13:39:00,17-Jul-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-199T00:37:00,000T09:00:00,18-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-199T01:37:00,000T08:00:00,18-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10199_SP,rider,,,,,, 2010-199T09:37:00,000T23:45:00,18-Jul-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-199T10:00:00,000T09:00:00,18-Jul-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-199T10:17:00,000T02:00:00,18-Jul-10,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 botsim, MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-199T10:17:00,000T02:00:00,18-Jul-10,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-199T12:17:00,000T09:00:00,18-Jul-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_135SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-199T12:17:00,000T09:00:00,18-Jul-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-199T21:17:00,000T02:00:00,18-Jul-10,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 botsim, MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-199T21:17:00,000T02:00:00,18-Jul-10,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-200T00:22:00,000T09:00:00,19-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-200T01:22:00,000T08:00:00,19-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10200_SP,rider,,,,,, 2010-200T09:22:00,005T01:38:00,19-Jul-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-200T10:00:00,000T09:00:00,19-Jul-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-200T10:02:00,001T11:00:00,19-Jul-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_135SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-200T10:02:00,000T23:59:00,19-Jul-10,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP ridealong,CIRS Ridealong for 2.5 full Saturn rotations,,,,,, 2010-201T10:00:00,002T05:00:00,20-Jul-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-201T21:02:00,000T00:30:00,20-Jul-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-202T00:22:00,000T09:00:00,21-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-202T01:22:00,000T08:00:00,21-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10202_SP,rider,,,,,, 2010-202T10:02:00,000T19:30:00,21-Jul-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-202T10:02:00,000T19:30:00,21-Jul-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-203T05:32:00,000T01:30:00,22-Jul-10,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 30.7 requested range 1.9 Mkm",,,,,, 2010-203T05:32:00,000T01:30:00,22-Jul-10,CIRS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-203T05:32:00,000T01:30:00,22-Jul-10,UVIS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-203T05:32:00,000T01:30:00,22-Jul-10,VIMS,SPASS Rider,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 30.7 range 1.9 Mkm",,,,,, 2010-203T07:02:00,000T14:00:00,22-Jul-10,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,~15X1 NAC stripe N to S on the dark side repeated 2x in CL1 at each footprint. 10 min/footprint 2x2 sum. Cycled while observation lasts.,,,,,, 2010-203T15:00:00,000T18:06:00,22-Jul-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-204T00:07:00,000T09:00:00,23-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-204T01:07:00,000T08:00:00,23-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10204_SP,rider,,,,,, 2010-204T09:06:00,003T00:00:00,23-Jul-10,MIMI,SPASS Rider,Saturn,PERIAPSIS,,MIMI Survey,"Near equatorial periapsis. Ride on Prime pointing, ask for secondary that keeps sun out of INCA, LEMMS FOVs.",,,,,, 2010-204T09:47:00,000T05:55:00,23-Jul-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-204T09:47:00,000T05:55:00,23-Jul-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-204T17:52:00,000T09:00:00,23-Jul-10,RSS,SPASS Rider,Saturn,KADOWN,RSS Ka-Band downlink,Gravity Science Enhancement (GSE),"Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation.",,,,,, 2010-204T17:52:00,000T09:00:00,23-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-204T18:52:00,000T04:00:00,23-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10604_SP,rider,,,,,, 2010-204T23:50:00,002T06:50:00,23-Jul-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-205T02:52:00,000T20:43:00,24-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-205T03:32:00,000T10:01:00,24-Jul-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 001 for Deep Atmospheres Ca,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-205T03:32:00,000T10:01:00,24-Jul-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,Hi phase NAC lightning search,"Night NAC 3x2 mosaic CL1 CL2, (I/F 1e-4 4x4 sum) and (1.e-3 2x2 sum) repeated 20 times at each footprint + once per footprint 1x1 summed WAC in CB2 at I/F 5e-3 for ring-illuminated clouds. 33min50 per footprint, see",,,,,, 2010-205T11:00:00,000T02:00:00,24-Jul-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-205T11:28:00,000T02:15:00,24-Jul-10,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS Thermal Stabilization 135 pre-Occ,null,,,,,, 2010-205T13:00:00,001T20:06:00,24-Jul-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-205T13:43:00,000T02:09:00,24-Jul-10,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS SA Atmospheric Occultayion Ingress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2010-205T15:06:00,000T04:08:00,24-Jul-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.4982790 Rs exit= 15.993782 Range altitude= -39920.531 km ... 15898.514,,,,,, 2010-205T15:46:00,000T03:29:00,24-Jul-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,NAC night. ? during the eclipse,"Night NAC 3x2 mosaic CL1 CL2, (I/F 1e-4 4x4 sum) and (1.e-3 2x2 sum) repeated 20 times at each footprint + once per footprint 1x1 summed WAC in CB2 at I/F 5e-3 for ring- illuminated clouds. 33min50 per footprint,",,,,,, 2010-205T16:02:00,000T03:13:00,24-Jul-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 002 for Deep Atmospheres Ca,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-205T19:15:00,000T02:27:00,24-Jul-10,VIMS,Prime,rings(general),OMICETOCC,OmiCet occultation,omiCet Ring Occultation,"Radial occ, dark face. Ends behind Saturn (unlit limb).",,,,,, 2010-205T19:15:00,000T16:27:00,24-Jul-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.4982790 Rs exit= 15.993782 Range altitude= -39920.531 km ... 15898.514,,,,,, 2010-205T19:15:00,000T02:57:00,24-Jul-10,RADAR,Non-SPASS,Other,WU4SAGM,,Warmup for Saturn Global Map PIE.,"Warmup for Saturn global map-1 in PIE. Actual data volume usage is going to be only for 15 minutes, 0.9 Mb (not 3 hours, 10.8 Mb).",,,,,, 2010-205T22:12:00,000T13:00:00,24-Jul-10,RADAR,Prime,Saturn,GLOBALMAP,Global coverage mapping,Saturn Global Map PIE.,Saturn global map-1 in PIE.,,,,,, 2010-205T23:35:00,000T07:25:00,24-Jul-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-206T00:19:00,000T02:00:00,25-Jul-10,CDA,Non-SPASS,DustRAM direction,RPX0010,,CDA RPXing 2010-206T01:19:00,RPXing at 3.7311961 Rs,,,,,, 2010-206T00:20:00,000T02:00:00,25-Jul-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-206T03:13:43,000T00:00:01,25-Jul-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.438 Rs, lat = 3 deg, phase = 83 deg",,,,,, 2010-206T07:00:00,001T02:06:00,25-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-206T11:42:00,000T11:44:00,25-Jul-10,VIMS,Prime,Saturn,GLOBDYN,Saturn Global dynamics,Global dynamics mosaic 003 for Deep Atmospheres Ca,"3x3 Global mosaic, centered on equator. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-206T11:42:00,000T11:41:00,25-Jul-10,ISS,SPASS Rider,Saturn,GLOBDYN,Saturn Global dynamics,WAC global day movie,"3x3 day mosaic, WAC in Mt2,CB2, and 2x2 MT3, and BL1 once at each fp",,,,,, 2010-206T11:42:00,000T21:38:00,25-Jul-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.4982790 Rs exit= 15.993782 Range altitude= -39920.531 km ... 15898.514,,,,,, 2010-207T00:06:00,000T09:00:00,26-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-207T06:40:00,000T02:26:00,26-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-207T09:06:00,001T05:54:00,26-Jul-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-207T09:06:00,001T23:15:00,26-Jul-10,CAPS,Non-SPASS,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2010-207T09:06:00,000T09:54:00,26-Jul-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-207T09:06:00,000T10:40:00,26-Jul-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-207T09:06:00,004T09:45:00,26-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-207T09:20:00,004T09:31:00,26-Jul-10,CDA,Non-SPASS,Other,RATE010B,,Data rate,Background data rate,,,,,, 2010-207T09:28:00,000T14:07:00,26-Jul-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-207T19:00:00,000T02:00:00,26-Jul-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-207T19:46:00,003T23:05:00,26-Jul-10,MAG,Non-SPASS,Other,LOWLATAPO,,LowLatApo PIE,MAPS LowLatApo PIE observation Split for sequence boundary,,,,,, 2010-207T21:00:00,003T21:51:00,26-Jul-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-207T23:35:00,000T01:23:00,26-Jul-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Rhea","Images of mutual event, transit of Dione across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-208T00:58:00,000T00:47:00,27-Jul-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-208T01:45:00,000T01:15:00,27-Jul-10,ISS,Prime,Prometheus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Prometheus across Janus","Images of mutual event, transit of Prometheus across Janus for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-208T03:00:00,000T07:00:00,27-Jul-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-208T10:00:00,000T22:21:00,27-Jul-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-208T15:00:00,002T05:00:00,27-Jul-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-209T08:21:00,000T12:00:00,28-Jul-10,CAPS,Non-SPASS,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2010-209T08:21:00,000T10:30:00,28-Jul-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-209T09:51:00,000T09:00:00,28-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-209T10:51:00,000T08:00:00,28-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10209_SP,rider,,,,,, 2010-209T12:00:00,000T01:08:00,28-Jul-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-209T18:51:00,000T01:30:00,28-Jul-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 49 requested range 2.6 Mkm",,,,,, 2010-209T18:51:00,000T01:30:00,28-Jul-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-209T18:51:00,000T01:30:00,28-Jul-10,UVIS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,"UVIS will be riding with the design determined by the prime instrument, ISS",,,,,, 2010-209T18:51:00,000T01:30:00,28-Jul-10,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, phase 49 range 2.6 Mkm",,,,,, 2010-209T20:21:00,000T10:39:00,28-Jul-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-209T20:21:00,001T11:30:00,28-Jul-10,CAPS,Non-SPASS,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2010-210T07:00:00,000T14:00:00,29-Jul-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-210T20:00:00,000T22:51:00,29-Jul-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-210T21:00:00,000T10:51:00,29-Jul-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-211T07:51:00,000T11:00:00,30-Jul-10,CAPS,Non-SPASS,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2010-211T09:51:00,000T09:00:00,30-Jul-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-211T10:51:00,000T08:00:00,30-Jul-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10211_SP,rider,,,,,, 2010-211T18:51:00,004T07:21:00,30-Jul-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-211T18:51:00,004T07:21:00,30-Jul-10,CAPS,Non-SPASS,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2010-211T18:51:00,004T07:21:00,30-Jul-10,CDA,Non-SPASS,Other,RATE010C,,Data rate,Background data rate,,,,,, 2010-211T18:51:00,000T00:43:00,30-Jul-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-211T18:51:00,000T02:16:00,30-Jul-10,MAG,Non-SPASS,Other,LOWLATAPO,,LowLatApo PIE,MAPS LowLatApo PIE observation Split for sequence boundary,,,,,, 2010-211T18:51:00,004T07:21:00,30-Jul-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-211T18:56:00,000T00:02:00,30-Jul-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S62 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-211T19:31:00,000T01:30:00,30-Jul-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 72.6, range = 3.4 Mkm.",,,,,, 2010-211T19:34:00,000T00:07:00,30-Jul-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-211T19:37:00,000T01:30:00,30-Jul-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 72.6 requested range 3.4 Mkm",,,,,, 2010-211T19:37:00,000T01:30:00,30-Jul-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-211T19:41:00,000T00:05:00,30-Jul-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-211T19:46:00,000T00:33:00,30-Jul-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-211T20:19:00,000T00:30:00,30-Jul-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-211T20:49:00,002T22:02:00,30-Jul-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-211T21:07:00,000T06:45:00,30-Jul-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-212T03:52:00,000T06:00:00,31-Jul-10,ISS,Prime,Iapetus,HILLSPHE,,Iapetus hill sphere observation,Turn -Y to Iapetus; do 1x5 mosaic; turn to WP.,,,,,, 2010-212T03:52:00,001T05:44:00,31-Jul-10,MAG,Non-SPASS,Other,LOWLATAPO,,LowLatApo PIE,MAPS LowLatApo PIE observation Split for sequence boundary,,,,,, 2010-212T09:52:00,000T04:00:00,31-Jul-10,ISS,Prime,Other,ALBSUP,,Albiorix,Observation of irregular moon of Saturn. Timing flexible within inbound part of apoapsis segment. RA/Dec (10.7 hrs/+47 deg) on 31 Jul very close to Iapetus's RA/Dec (10.3 hrs/+35 deg).,,,,,, 2010-212T13:52:00,000T08:00:00,31-Jul-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-212T21:52:00,000T09:34:00,31-Jul-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-213T09:36:00,002T09:00:00,1-Aug-10,MAG,Non-SPASS,Other,LOWLATAPO,,LowLatApo PIE,MAPS LowLatApo PIE observation Split for sequence boundary,,,,,, 2010-213T09:36:00,002T09:00:00,1-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-213T09:36:00,000T09:00:00,1-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-213T10:36:00,000T08:00:00,1-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10213_SP,rider,,,,,, 2010-213T19:00:00,000T09:00:00,1-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-213T19:16:00,000T11:30:00,1-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-214T06:46:00,000T00:30:00,2-Aug-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-214T07:16:00,000T11:45:00,2-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-214T18:51:00,000T00:34:00,2-Aug-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2010-214T19:00:00,000T09:00:00,2-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-214T19:25:00,001T06:47:05,2-Aug-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-214T20:31:00,000T10:55:00,2-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-215T09:36:00,000T09:00:00,3-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-215T10:36:00,000T08:00:00,3-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_135IC_DSCAL10215_SP,rider,,,,,, 2010-215T18:36:00,007T21:19:00,3-Aug-10,MAG,Non-SPASS,Other,LOWLATAPO,,LowLatApo PIE,MAPS LowLatApo PIE observation Split for sequence boundary,,,,,, 2010-215T19:16:00,000T14:00:00,3-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-216T02:12:00,009T05:37:00,4-Aug-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-216T02:12:00,009T05:37:00,4-Aug-10,CAPS,Non-SPASS,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2010-216T02:12:00,009T10:34:00,4-Aug-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate,Background data rate,,,,,, 2010-216T02:12:00,003T16:08:00,4-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-216T02:12:04,000T00:00:01,4-Aug-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 19.9 d, inc = 4.7 deg, r = 43.524 Rs, phase = 97 deg",,,,,, 2010-216T02:12:05,000T02:00:00,4-Aug-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-216T04:12:05,006T21:22:55,4-Aug-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-216T09:16:00,000T14:00:00,4-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-216T23:16:00,000T15:24:00,4-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-217T16:50:00,000T09:00:00,5-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-217T17:50:00,000T08:00:00,5-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10217_SP,rider,,,,,, 2010-218T02:00:00,000T09:00:00,6-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-218T02:30:00,000T14:00:00,6-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-218T16:30:00,000T00:30:00,6-Aug-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-218T17:00:00,000T14:10:00,6-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-219T09:20:00,000T09:00:00,7-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-219T10:20:00,000T08:00:00,7-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10219_SP,rider,,,,,, 2010-219T18:20:00,002T00:00:00,7-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-219T19:00:00,000T01:30:00,7-Aug-10,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 138 requested range 1.9 Mkm",,,,,, 2010-219T19:00:00,000T01:30:00,7-Aug-10,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-219T19:00:00,000T01:30:00,7-Aug-10,VIMS,SPASS Rider,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 138 deg, range = 1.9 Mkm",,,,,, 2010-219T19:00:00,000T09:00:00,7-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-219T20:30:00,000T05:40:00,7-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-220T02:10:00,000T05:00:00,8-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-220T09:20:00,000T09:00:00,8-Aug-10,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-55 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2010-220T09:20:00,000T09:00:00,8-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-220T10:20:00,000T08:00:00,8-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10220_SP,rider,,,,,, 2010-220T11:20:00,000T01:00:00,8-Aug-10,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,HGA Boresight Calibration; Pointing=XBAND to Earth + crosshair maneuver. Last hour (crosshair maneuver) required to be tracked at DSS-55 in 1-way mode. Playback of telemetry required afterwards for C-Kernel generation.,,,,,, 2010-220T19:00:00,000T01:30:00,8-Aug-10,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 140.1 requested range 1.3 Mkm",,,,,, 2010-220T19:00:00,000T01:30:00,8-Aug-10,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-220T19:00:00,000T01:30:00,8-Aug-10,VIMS,SPASS Rider,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 140 deg, range = 1.3 Mkm",,,,,, 2010-220T20:30:00,000T00:30:00,8-Aug-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-220T21:00:00,000T03:40:00,8-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-221T00:40:00,000T06:30:00,9-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-221T01:00:00,000T04:00:00,9-Aug-10,CAPS,SPASS Rider,co-rotation,IONCALDV,,MAPS ion calibration DV request,null,,,,,, 2010-221T06:00:00,000T01:08:00,9-Aug-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-221T09:20:00,000T09:00:00,9-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-221T10:20:00,000T08:00:00,9-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10221_SP,rider,,,,,, 2010-221T18:20:00,003T03:15:00,9-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-221T19:00:00,000T08:00:00,9-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-222T03:00:00,000T05:00:00,10-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-222T08:00:00,000T07:55:00,10-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-222T16:35:00,000T09:00:00,10-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-222T17:35:00,000T08:00:00,10-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10222_SP,rider,,,,,, 2010-223T01:35:00,001T00:00:00,11-Aug-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-223T02:15:00,000T04:00:00,11-Aug-10,ISS,Prime,Other,KIVPHA,,Kiviuq,Observation of irregular moon of Saturn. Timing flexible within a few days.,,,,,, 2010-223T06:37:00,000T05:18:00,11-Aug-10,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-223T11:55:00,000T04:00:00,11-Aug-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2010-223T15:55:00,001T15:54:00,11-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-223T16:35:00,000T09:00:00,11-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-223T17:35:00,000T08:00:00,11-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10223_SP,rider,,,,,, 2010-224T01:35:00,001T06:14:00,12-Aug-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-224T02:15:00,000T02:00:00,12-Aug-10,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 58.7 requested range 0.4 Mkm",,,,,, 2010-224T02:15:00,000T02:00:00,12-Aug-10,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-224T02:15:00,000T02:00:00,12-Aug-10,VIMS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 59 deg, range = 0.4 Mkm",,,,,, 2010-224T04:15:00,000T16:24:00,12-Aug-10,ISS,Prime,Other,ALBROT,,Albiorix,Observation of irregular moon of Saturn.,,,,,, 2010-224T04:15:00,000T16:24:00,12-Aug-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-224T21:35:00,000T10:14:00,12-Aug-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-224T22:49:00,000T09:00:00,12-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-224T23:49:00,000T08:00:00,12-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10224_SP,rider,,,,,, 2010-225T07:49:00,000T14:11:59,13-Aug-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-225T07:49:00,000T13:41:59,13-Aug-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-225T07:49:00,000T02:41:59,13-Aug-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-225T07:49:00,000T12:41:59,13-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-225T07:49:00,001T04:41:00,13-Aug-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-225T08:29:00,000T02:00:00,13-Aug-10,ISS,Prime,Titan,M30R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 19.5 requested range 0.7 Mkm",,,,,, 2010-225T08:29:00,000T02:00:00,13-Aug-10,CIRS,SPASS Rider,Titan,M30R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-225T08:29:00,000T02:00:00,13-Aug-10,VIMS,SPASS Rider,Titan,M30R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 20 deg, range = 0.7 Mkm",,,,,, 2010-225T10:29:00,000T02:21:00,13-Aug-10,ISS,Prime,Dione,PLUMESEAR,,Dione plume search,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-225T10:29:00,000T02:21:00,13-Aug-10,CIRS,SPASS Rider,Dione,PLUMESEAR,,136DI_PLUMESEAR001,"FP1, FP3, only",,,,,, 2010-225T10:29:00,000T02:21:00,13-Aug-10,UVIS,SPASS Rider,Dione,ICYPLU,Observe Enceladus plumes,ICYPLU: Dione Plume Search,Look for Dione volatiles,,,,,, 2010-225T10:29:00,000T02:21:00,13-Aug-10,VIMS,SPASS Rider,Dione,DIONE,Dione,,null,,,,,, 2010-225T10:30:59,000T10:00:00,13-Aug-10,INMS,Non-SPASS,Saturn,E11INBND,,Enceladus flyby,Enceladus observation,,,,,, 2010-225T12:46:00,001T18:26:00,13-Aug-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.5784066 Rs exit= 15.998061 Range altitude= -39984.575 km ... 14989.279,,,,,, 2010-225T12:50:00,000T02:10:00,13-Aug-10,ISS,Prime,Enceladus,PLMLRHP,,Low res plume obs at high phase,High resolution plume observation at low phase,,,,,, 2010-225T12:50:00,000T03:10:00,13-Aug-10,CIRS,SPASS Rider,Enceladus,PLMLRHP,,136EN_PLMLRHP001,FP1 and FP3 only,,,,,, 2010-225T12:50:00,000T02:10:00,13-Aug-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-225T12:50:00,000T03:10:00,13-Aug-10,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,,null,,,,,, 2010-225T15:00:00,000T01:00:00,13-Aug-10,ISS,Prime,Enceladus,PLMSCECL,,High-phase Plume obs during eclipse,High resolution plume observation at low phase,,,,,, 2010-225T15:00:00,000T01:00:00,13-Aug-10,UVIS,SPASS Rider,Enceladus,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2010-225T16:00:00,000T02:55:00,13-Aug-10,CIRS,Prime,Dione,FP3SECLN,,CIRS_Best-FP3DI-Eclipse_136DI_FP3SECLN001,"Turn from waypoint (ca. 20- min.); make slow 3-scan FP3 map of lit hemisphere (include Deep Space) [Spencer addition, given the extra time: and also scan as much of the night side as possible in case of endogenic emission]; at T17:30 target FP3 to (-15, 30) with secondary NEG_X to NSP, (0.0, TBD, 0.0); eclipse entry at T17:40:40; at T18:10:00 point PF3 10 mrad off bright limb for 10 min of deep space; if possible, return to previous pointing until return to waypoint (ca. 30- min.). 15.5 cm-1, blink (or odds/evens?), shutter closed for 6 min. just before end of initial turn, at beginning of return to waypoint. NAC, WAC support images at T17:35:00.",,,,,, 2010-225T16:00:00,000T02:55:00,13-Aug-10,CIRS,SPASS Rider,Dione,FP3SECLN,,CIRS_136DI_FP3SECLN SI,"One NAC, one WAC at 2010-225T17:35:00",,,,,, 2010-225T16:00:00,000T02:55:00,13-Aug-10,ISS,SPASS Rider,Dione,FP3SECLN,,Dione,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-225T16:00:00,000T02:55:00,13-Aug-10,UVIS,SPASS Rider,Dione,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2010-225T16:00:00,000T02:55:00,13-Aug-10,VIMS,SPASS Rider,Dione,FP3SECLN,,,null,,,,,, 2010-225T18:55:00,000T00:35:00,13-Aug-10,CIRS,Prime,Enceladus,DRKPLUME,,CIRS_136EN_DRKPLUME001,"ISS plume imaging before Saturn transit ingress at 19:08, then slow FP3/4 scans of south polar region",,,,,, 2010-225T18:55:00,000T00:35:00,13-Aug-10,ISS,SPASS Rider,Enceladus,DRKPLUME,,Enceladus,Enceladus,,,,,, 2010-225T18:55:00,000T00:35:00,13-Aug-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-225T18:55:00,000T00:35:00,13-Aug-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2010-225T19:34:59,000T01:55:00,13-Aug-10,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at low phase,,,,,, 2010-225T19:34:59,000T01:55:00,13-Aug-10,CIRS,SPASS Rider,Enceladus,PLMHRHP,,136EN_PLMHRHP002,,,,,,, 2010-225T19:34:59,000T01:55:00,13-Aug-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-225T19:34:59,000T01:55:00,13-Aug-10,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,,null,,,,,, 2010-225T20:30:59,000T01:30:00,13-Aug-10,INMS,Non-SPASS,Enceladus,ENCEL11,,Enceladus encounter,Enceladus observation,,,,,, 2010-225T20:30:59,000T04:00:00,13-Aug-10,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2010-225T20:30:59,000T01:00:00,13-Aug-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-225T21:25:00,000T03:05:59,13-Aug-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-225T21:29:59,000T03:00:00,13-Aug-10,CIRS,Prime,Enceladus,HIRES,High resolution image,CIRS_136EN_HIRES001,"All FP3/4 scans should be at 12 murad/sec if possible. The FP1 scan will presumably be faster 21:31 - 21:41 Pair of abutting FP3/4 scans centered on ~75 S, 180 W 21:41 - 21:51 ISS plume imaging 21:51 - 22:01 Pair of abutting FP3/4 scans centered on ~82 S, 210 W 22:01 - 22:06 ISS plume imaging (e.g. Baghdad/Plume 1 on the terminator) 22:06 - 22:16 Pair of abutting FP3/4 scans centered on ~72 S, 180 W 22:16 - 22:26 FP1 scan from 65 S, 310 W to ~85 S, 150 W 22:26 - 22:31 FP3 scan centered on 79 S, 320 W (Damascus fork) Secondary axis: 21:31 - 22:22, POS_X to NSP 22:22 - 22:41, NEG_X to RAM 21:41 - 23:43, NEG_X to NSP Sun hits radiator at 23:43 so some add'l 2nd axis change is then needed",,,,,, 2010-225T21:29:59,000T03:00:00,13-Aug-10,CIRS,SPASS Rider,Enceladus,HIRES,High resolution image,CIRS_136EN HIRES001 SI,"One NAC at 21:58:46, exposed for the sunlit crescent, 2x2 binned, 8-bit, lossy compression One NAC at about 22:06:15, exposed for the sunlit crescent, 2x2 binned, 8-bit, lossy compression One NAC at 22:29:00, exposed for Saturn shine (1 second exposure recommended: should be adequate SNR for pointing, and will have only ~2 pixels of smear). Unbinned (1x1), 12-bit, lossless compression",,,,,, 2010-225T21:29:59,000T03:00:00,13-Aug-10,ISS,SPASS Rider,Enceladus,HIRES,High resolution image,Enceladus,Enceladus close approach,,,,,, 2010-225T21:29:59,000T03:00:00,13-Aug-10,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-225T21:29:59,000T03:00:00,13-Aug-10,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2010-225T21:30:59,000T02:00:00,13-Aug-10,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 136EN Campaign,Part of 120EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2010-225T21:30:59,000T02:00:00,13-Aug-10,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2010-225T22:00:59,000T01:00:00,13-Aug-10,MIMI,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS RS Campaign,"Part of RS MAPS Campaign. Icy moon encounter. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-225T22:00:59,000T01:00:00,13-Aug-10,INMS,Non-SPASS,Enceladus,ENCEL11,,Enceladus encounter,Enceladus observation,,,,,, 2010-225T22:07:00,000T02:00:00,13-Aug-10,CDA,SPASS Rider,DustRAM direction,RPX0020,,CDA RPXing 2010-225T23:07:00,RPXing at 3.7576862 Rs,,,,,, 2010-225T23:00:59,001T08:48:01,13-Aug-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-225T23:00:59,000T01:30:00,13-Aug-10,INMS,Non-SPASS,Enceladus,ENCEL11,,Enceladus encounter,Enceladus observation,,,,,, 2010-225T23:30:59,001T08:18:01,13-Aug-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-225T23:30:59,000T01:00:00,13-Aug-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-226T00:29:59,000T01:45:00,14-Aug-10,UVIS,Prime,Star,URBETORI,,URSTAR,PIE ring stellar occ (very low incidence angle; such occs are rare and particularly valuable).,,,,,, 2010-226T00:29:59,000T01:45:00,14-Aug-10,UVIS,SPASS Rider,Star,URBETORI,,Support Imaging,NAC and WAC support images at 2010-226T01:45:24 2010-226T01:30:58,,,,,, 2010-226T00:29:59,000T01:45:00,14-Aug-10,VIMS,SPASS Rider,Star,URBETORI,,,Stellar Occ Enceladus,,,,,, 2010-226T00:29:59,000T01:45:00,14-Aug-10,ISS,Non-SPASS,Star,URBETORI,,,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-226T00:30:59,000T10:00:00,14-Aug-10,INMS,Non-SPASS,Saturn,E11OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2010-226T00:30:59,000T04:19:01,14-Aug-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-226T01:04:02,000T00:00:01,14-Aug-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.457 Rs, lat = 3 deg, phase = 83 deg",,,,,, 2010-226T02:14:59,000T00:45:00,14-Aug-10,VIMS,Prime,Enceladus,ENCEL,Enceladus,,null,,,,,, 2010-226T02:14:59,000T00:45:00,14-Aug-10,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,136EN_ENCEL001_VIMS,,,,,,, 2010-226T02:14:59,000T00:45:00,14-Aug-10,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus post-close approach,,,,,, 2010-226T02:14:59,000T00:45:00,14-Aug-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2010-226T04:50:00,001T02:59:00,14-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-226T05:30:00,000T07:00:00,14-Aug-10,ISS,Prime,Tethys,TETHYS,Tethys,Tethys,Tethys,,,,,, 2010-226T05:30:00,000T07:00:00,14-Aug-10,CIRS,SPASS Rider,Tethys,TETHYS,Tethys,136TE_TETHYS001,"FP1 and FP3 only, to save data volume",,,,,, 2010-226T05:30:00,000T07:00:00,14-Aug-10,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2010-226T05:30:00,000T07:00:00,14-Aug-10,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,,null,,,,,, 2010-226T10:30:59,000T21:18:01,14-Aug-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-226T12:30:00,000T19:19:00,14-Aug-10,MIMI,SPASS Rider,Saturn,SPONGEOV,,MIMI Magnetospheric Dymanics,,,,,,, 2010-226T12:30:00,000T16:00:00,14-Aug-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-226T14:00:00,000T02:16:32,14-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-226T22:49:00,000T09:00:00,14-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-226T23:49:00,000T08:00:00,14-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10226_SP,rider,,,,,, 2010-227T00:00:00,000T04:33:04,15-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-227T04:30:00,000T03:19:00,15-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-227T07:12:00,008T18:06:00,15-Aug-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.010041 Rs exit= 8.6093724 Range altitude= 14962.691 km ... -40048.959,,,,,, 2010-227T07:49:00,003T08:30:00,15-Aug-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-227T07:49:00,002T00:00:00,15-Aug-10,MIMI,SPASS Rider,Saturn,SPONGEOV,,MIMI Magnetospheric Dymanics,,,,,,, 2010-227T07:49:00,008T17:29:00,15-Aug-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-227T07:49:00,000T10:27:00,15-Aug-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-227T07:49:00,002T00:00:00,15-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-227T07:49:00,003T08:30:00,15-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-227T07:49:00,002T00:00:00,15-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-227T08:00:00,000T13:00:00,15-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10627_SP,rider,,,,,, 2010-227T08:15:00,000T10:30:00,15-Aug-10,RSS,Prime,Earth,LGATEST,,LGA TEST,A test to verify that scientifically-useful Doppler data can be acquired with LGA moving and over a cone angle +/- 30 degrees from Earth point,,,,,, 2010-227T09:00:00,000T02:16:32,15-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-227T18:16:00,000T02:00:00,15-Aug-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-227T20:16:00,001T11:33:00,15-Aug-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-227T22:34:00,000T09:00:00,15-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-227T23:34:00,000T08:00:00,15-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10227_SP,rider,,,,,, 2010-228T00:00:00,000T02:16:32,16-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-228T08:00:00,000T13:20:00,16-Aug-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_136SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-228T09:00:00,000T04:33:16,16-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-228T21:20:00,000T01:00:00,16-Aug-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-228T22:49:00,000T09:00:00,16-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-228T23:49:00,000T08:00:00,16-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10228_SP,rider,,,,,, 2010-229T00:00:00,000T02:16:32,17-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-229T07:49:00,001T00:00:00,17-Aug-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-229T07:49:00,000T07:56:00,17-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-229T08:00:00,000T01:30:00,17-Aug-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 78.1 requested range 2.9 Mkm",,,,,, 2010-229T08:00:00,000T01:30:00,17-Aug-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-229T08:00:00,000T01:30:00,17-Aug-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 78 deg, range = 2.9 Mkm",,,,,, 2010-229T09:45:00,000T06:00:00,17-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10529_SP,rider,,,,,, 2010-229T15:45:00,000T06:45:00,17-Aug-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-229T22:30:00,013T18:18:00,17-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-229T22:49:00,000T09:00:00,17-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-229T23:49:00,000T08:00:00,17-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10229_SP,rider,,,,,, 2010-230T07:49:00,005T17:35:29,18-Aug-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-230T07:59:00,000T08:20:00,18-Aug-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS MAGBOUND w/ prime pointing,null,,,,,, 2010-231T01:19:00,000T14:45:00,19-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-231T01:19:00,000T14:45:00,19-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-231T01:30:00,000T12:00:00,19-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10231_SP,rider,,,,,, 2010-231T10:25:00,001T06:00:00,19-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-231T16:04:00,000T09:00:00,19-Aug-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev137 Saturn rings occultation on 2010/245.",,,,,, 2010-232T01:04:00,000T15:00:00,20-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10532_SP,rider,,,,,, 2010-232T01:04:00,000T15:00:00,20-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-232T01:04:00,000T15:00:00,20-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-232T16:04:00,000T09:00:00,20-Aug-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev137 Saturn rings occultation on 2010/245.",,,,,, 2010-233T01:04:00,003T00:14:00,21-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-233T01:04:00,001T06:15:00,21-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-233T01:14:00,000T08:00:00,21-Aug-10,CIRS,Prime,Other,CWSTAROBS,,Mid-IR Stellar Spectroscopy of CW Leo,"Spectroscopic observations of IR star CW Leonis. Slew to star at (146.9862, 13.2786); execute small box scan, integrating at each position; return to waypoint. Observation duration 8 hours (typically 2x40 min turns + 3x15 min deep space + 4x90 min stares).",,,,,, 2010-233T01:14:00,000T08:00:00,21-Aug-10,CIRS,SPASS Rider,Other,CWSTAROBS,,CIRS_136OT CW Leo SI,"4 clear NACs, at 2010-233T02:54, 2010-233T04:38, 2010-233T06:22, and 2010-233T08:06. Exposure information: Spectral class=F, V magnitude=13.0",,,,,, 2010-233T09:14:00,000T11:35:00,21-Aug-10,CAPS,Prime,Saturn,MAGBNDPTG,MAPS magnetosphere boundary campaign,MAPS MAGBOUND w/ prime pointing,null,,,,,, 2010-233T20:49:00,000T11:05:00,21-Aug-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-233T22:19:00,000T09:00:00,21-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-233T23:19:00,000T08:00:00,21-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10233_SP,rider,,,,,, 2010-234T07:19:00,001T17:59:00,22-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-234T07:54:00,001T12:55:00,22-Aug-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-235T22:19:00,000T09:00:00,23-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-235T22:30:00,000T04:33:04,23-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-235T23:19:00,000T08:00:00,23-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_136IC_DSCAL10235_SP,rider,,,,,, 2010-236T01:18:00,002T05:46:00,24-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-236T01:18:00,007T15:30:00,24-Aug-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-236T01:18:00,007T15:30:00,24-Aug-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.010041 Rs exit= 8.6093724 Range altitude= 14962.691 km ... -40048.959,,,,,, 2010-236T01:18:00,006T05:30:00,24-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-236T01:24:29,000T00:00:01,24-Aug-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.0 d, inc = 4.6 deg, r = 43.691 Rs, phase = 97 deg",,,,,, 2010-236T01:24:29,000T02:00:00,24-Aug-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-236T03:24:29,008T20:53:31,24-Aug-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-236T07:19:00,001T12:40:00,24-Aug-10,CDA,Prime,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-236T07:59:00,000T01:30:00,24-Aug-10,VIMS,SPASS Rider,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 117 deg, range = 1.6 Mkm",,,,,, 2010-237T22:04:00,000T09:00:00,25-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-237T23:04:00,000T08:00:00,25-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10237_SP,rider,,,,,, 2010-238T07:04:00,003T14:44:00,26-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-238T08:00:00,000T09:00:00,26-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8)",,,,,, 2010-238T14:33:00,000T15:00:00,26-Aug-10,ISS,Prime,Other,HYRROT,Observe irregular moon Hyrrokkin,Hyrrokkin,Observation of irregular moon of Saturn.,,,,,, 2010-238T14:33:00,000T15:00:00,26-Aug-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-239T05:33:00,000T15:00:00,27-Aug-10,ISS,Prime,Other,GREROT,,Greip,Observation of irregular moon of Saturn.,,,,,, 2010-239T05:33:00,000T15:00:00,27-Aug-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-239T09:00:00,001T06:00:00,27-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-239T22:03:00,000T09:00:00,27-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-239T23:03:00,000T03:00:00,27-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10239_SP,rider,,,,,, 2010-240T00:00:00,000T01:08:00,28-Aug-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-240T07:40:00,000T01:30:00,28-Aug-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 77 requested range 1.7 Mkm",,,,,, 2010-240T07:40:00,000T01:30:00,28-Aug-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-240T07:40:00,000T01:30:00,28-Aug-10,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 77 deg, range = 1.7 Mkm",,,,,, 2010-240T08:00:00,000T10:00:00,28-Aug-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-240T09:10:00,001T09:30:00,28-Aug-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_137SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-241T18:40:00,000T01:00:00,29-Aug-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-241T21:48:00,001T19:00:00,29-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-241T21:48:00,000T09:00:00,29-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-241T22:48:00,000T08:00:00,29-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10241_SP,rider,,,,,, 2010-242T06:48:00,001T00:00:00,30-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-242T07:23:00,000T22:55:00,30-Aug-10,ISS,Prime,Other,KIVROT,,Kiviuq,Observation of irregular moon of Saturn.,,,,,, 2010-242T07:23:00,000T22:55:00,30-Aug-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-243T06:48:00,000T10:00:00,31-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-243T07:48:00,000T09:00:00,31-Aug-10,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev137 Saturn rings occultation on 2010/245.",,,,,, 2010-243T07:48:00,000T09:00:00,31-Aug-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-243T08:48:00,000T08:00:00,31-Aug-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10243_SP,rider,,,,,, 2010-243T09:00:00,000T02:16:32,31-Aug-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 64 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-243T16:48:00,001T07:30:00,31-Aug-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-243T16:48:00,001T07:30:00,31-Aug-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-243T16:48:00,001T07:30:00,31-Aug-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.010041 Rs exit= 8.6093724 Range altitude= 14962.691 km ... -40048.959,,,,,, 2010-243T16:48:00,001T07:30:00,31-Aug-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-243T16:48:00,001T05:27:00,31-Aug-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-243T19:25:00,000T17:35:00,31-Aug-10,ISS,Prime,rings(general),HPLELR,,Faint Ring High Phase Observation,Observation of faint rings at low elevation angles and high phase,,,,,, 2010-243T19:25:00,000T17:35:00,31-Aug-10,CIRS,SPASS Rider,rings(general),HPLELR,,,CIRS Rider to ISS High Phase Rings Observation in XD 136/137,,,,,, 2010-244T15:18:00,000T09:00:00,1-Sep-10,RSS,SPASS Rider,rings(general),KADOWN,RSS Ka-Band downlink,GSE pass for ring occultation,Downlink pass at Ka-band for improving locally Cassini orbit for rings science.,,,,,, 2010-244T15:18:00,000T09:00:00,1-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-244T20:18:00,000T04:00:00,1-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10244_SP,rider,,,,,, 2010-244T22:15:00,000T02:03:00,1-Sep-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-245T00:18:00,002T06:15:00,2-Sep-10,MIMI,SPASS Rider,Saturn,RNGSAT,Ring / Satellite,MIMI Satellite & Ring Interactions,"Part of RS MAPS Campaign. Observe the interaction between the magnetospheric hot ion and electron distributions, rings, and icy satellites. Pointing: Corotation ram in -X, +/-Z half-plane; B field in X, Z plane. Measure properties of a statistically significant number of satellite L shell crossings distributed amoung the satellites and in longitudinal distance from the satellites.",,,,,, 2010-245T00:18:00,002T06:15:00,2-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-245T00:18:00,000T13:02:00,2-Sep-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.010041 Rs exit= 8.6093724 Range altitude= 14962.691 km ... -40048.959,,,,,, 2010-245T00:18:00,000T10:42:00,2-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-245T00:18:00,000T21:47:00,2-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-245T00:18:00,002T04:47:00,2-Sep-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-245T00:58:00,000T05:54:00,2-Sep-10,VIMS,Prime,rings(general),FMOVIE,F ring movie,F Ring movie,"64x12 frame, hi res mode. 640 msec tau_IR. In order to satisfy ISS and CIRS requirements, primary pointing will be to a ring radius-longitude to be determined.",,,,,, 2010-245T00:58:00,000T05:54:00,2-Sep-10,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,,null,,,,,, 2010-245T00:58:00,000T05:54:00,2-Sep-10,ISS,SPASS Rider,rings(general),FMOVIE,F ring movie,Medium Res F ring Movie,F Ring Movie Rider,,,,,, 2010-245T06:52:00,000T03:00:00,2-Sep-10,CIRS,Prime,rings(general),EQLBS,,,,,,,,, 2010-245T06:52:00,000T03:00:00,2-Sep-10,CIRS,SPASS Rider,rings(general),EQLBS,,,,,,,,, 2010-245T06:52:00,000T03:00:00,2-Sep-10,UVIS,SPASS Rider,rings(general),EQLBS,,URSPEC,,,,,,, 2010-245T08:27:00,000T02:25:00,2-Sep-10,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 137RI OCC Thermal Stabilization,A 2 hrs 5 min period of thermal stabilization is required immediately prior to any radio science experiment using Ka- or S-band.,,,,,, 2010-245T10:52:00,000T03:44:00,2-Sep-10,RSS,Prime,rings(general),OCC,Occultation,RSS Bridge Ring Occ - Ingress,"A Bridge Sequence RSS ingress ring occultation. Available power on 2010-245 allows simultaneous Ka, X and S bands observations. The observations will commence after a 2-hour period of thermal stabilization.",,,,,, 2010-245T11:00:00,000T02:00:00,2-Sep-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-245T13:00:00,000T09:39:00,2-Sep-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-245T13:20:00,000T09:21:00,2-Sep-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.5933172 Rs exit= 15.990178 Range altitude= -39953.174 km ... 14426.832,,,,,, 2010-245T14:36:00,000T02:57:00,2-Sep-10,VIMS,Prime,rings(general),HIPHASE,High phase observation,High Phase Ring Monitor,Dark face.,,,,,, 2010-245T14:36:00,000T02:57:00,2-Sep-10,CIRS,SPASS Rider,rings(general),HIPHASE,High phase observation,,null,,,,,, 2010-245T14:36:00,000T02:57:00,2-Sep-10,ISS,SPASS Rider,rings(general),HIPHASE,High phase observation,High-phase observations of rings,High-Phase observations of rings.,,,,,, 2010-245T14:36:00,000T02:57:00,2-Sep-10,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 137RI OCC Thermal Stabilization,The spacecraft Ka- and S-band need to remain thermally stable during the priod between ingress and egress occultations.,,,,,, 2010-245T17:33:00,000T02:17:00,2-Sep-10,RSS,Prime,rings(general),OCC,Occultation,RSS Bridge Sequence Ring Occ - Egress,"A Bridge Sequence RSS egress ring occultation. Available power on 2010-245 allows simultaneous Ka, X and S bands observations. The observations will commence after a 2-hour period of thermal stabilization.",,,,,, 2010-245T21:33:00,000T09:00:00,2-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-245T21:40:00,000T04:00:00,2-Sep-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-245T22:05:00,000T07:20:00,2-Sep-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-245T22:33:00,000T08:00:00,2-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10245_SP,rider,,,,,, 2010-245T22:39:00,000T02:00:00,2-Sep-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-245T22:41:00,000T02:00:00,2-Sep-10,CDA,SPASS Rider,DustRAM direction,RPX0030,,CDA RPXing 2010-245T23:41:00,RPXing at 3.7714719 Rs,,,,,, 2010-245T22:41:00,000T02:00:00,2-Sep-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.5933172 Rs exit= 15.990178 Range altitude= -39953.174 km ... 14426.832,,,,,, 2010-246T00:39:00,000T05:54:00,3-Sep-10,INMS,Non-SPASS,Saturn,RINGPLN,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-246T00:41:00,001T07:07:00,3-Sep-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.5933172 Rs exit= 15.990178 Range altitude= -39953.174 km ... 14426.832,,,,,, 2010-246T01:40:01,000T00:00:01,3-Sep-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.462 Rs, lat = 3 deg, phase = 84 deg",,,,,, 2010-246T05:25:00,001T01:08:00,3-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-246T06:33:00,001T00:00:00,3-Sep-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-246T07:13:00,000T03:27:00,3-Sep-10,ISS,Prime,Dione,DIONE,Dione,Dione,"FP1 and FP3 (CIRS) scans first, then 22-panel mosaic for ISS, then 2 sit'n'stares for VIMS.",,,,,, 2010-246T07:13:00,000T03:27:00,3-Sep-10,CIRS,SPASS Rider,Dione,DIONE,Dione,CIRS_137DI_DIONE001_ISS;,"North polar mapping, fracture and nightside thermal mapping",,,,,, 2010-246T07:13:00,000T01:45:00,3-Sep-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,During CIRS portion of the timeline ride along on FP3 scan but not FP1 scan. The FP3 scan is ~07:40 to 08:58.,,,,,, 2010-246T07:13:00,000T03:27:00,3-Sep-10,VIMS,SPASS Rider,Dione,DIONE,Dione,DIONE mapping,Dione composition,,,,,, 2010-246T08:58:00,000T01:42:00,3-Sep-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,During CIRS portion of the timeline ride along on FP3 scan but not FP1 scan. The FP3 scan is ~07:40 to 08:58.,,,,,, 2010-246T11:00:00,000T02:20:00,3-Sep-10,ISS,Prime,rings(general),BMOVIE,B ring movie,"B-ring ansa movie, part 1","Part 1 of 3-part B-ring ansa movie, which is interleaved with two CIRS scans.",,,,,, 2010-246T11:00:00,000T02:20:00,3-Sep-10,CIRS,SPASS Rider,rings(general),BMOVIE,B ring movie,,null,,,,,, 2010-246T11:00:00,000T02:20:00,3-Sep-10,VIMS,SPASS Rider,rings(general),BMOVIE,B ring movie,B Ring composition,160 msec exposures interleaved with longer integration time (640 msec).,,,,,, 2010-246T13:20:00,000T01:30:00,3-Sep-10,CIRS,Prime,rings(general),EQLBN,,,,,,,,, 2010-246T13:20:00,000T01:30:00,3-Sep-10,CIRS,SPASS Rider,rings(general),EQLBN,,,,,,,,, 2010-246T13:20:00,000T01:30:00,3-Sep-10,UVIS,SPASS Rider,rings(general),EQLBN,,URSPEC,,,,,,, 2010-246T14:50:00,000T02:20:00,3-Sep-10,ISS,Prime,rings(general),BMOVIE,B ring movie,"B-ring ansa movie, part 2","Part 2 of 3-part B-ring ansa movie, which is interleaved with two CIRS scans.",,,,,, 2010-246T14:50:00,000T02:20:00,3-Sep-10,CIRS,SPASS Rider,rings(general),BMOVIE,B ring movie,,null,,,,,, 2010-246T14:50:00,000T02:20:00,3-Sep-10,VIMS,SPASS Rider,rings(general),BMOVIE,B ring movie,B Ring composition,160 msec exposures interleaved with longer integration time (640 msec).,,,,,, 2010-246T17:10:00,000T01:30:00,3-Sep-10,CIRS,Prime,rings(general),EQLBN,,,,,,,,, 2010-246T17:10:00,000T01:30:00,3-Sep-10,CIRS,SPASS Rider,rings(general),EQLBN,,,,,,,,, 2010-246T17:10:00,000T01:30:00,3-Sep-10,UVIS,SPASS Rider,rings(general),EQLBN,,URSPEC,,,,,,, 2010-246T18:40:00,000T02:13:00,3-Sep-10,ISS,Prime,rings(general),BMOVIE,B ring movie,"B-ring ansa movie, part 3","Part 3 of 3-part B-ring ansa movie, which is interleaved with two CIRS scans.",,,,,, 2010-246T18:40:00,000T02:13:00,3-Sep-10,CIRS,SPASS Rider,rings(general),BMOVIE,B ring movie,,null,,,,,, 2010-246T18:40:00,000T02:13:00,3-Sep-10,VIMS,SPASS Rider,rings(general),BMOVIE,B ring movie,B Ring composition,160 msec exposures interleaved with longer integration time (640 msec).,,,,,, 2010-246T21:33:00,000T09:00:00,3-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-246T22:33:00,000T08:00:00,3-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10246_SP,rider,,,,,, 2010-247T05:05:00,000T01:28:00,4-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-247T06:33:00,002T00:00:00,4-Sep-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-247T06:33:00,002T00:00:00,4-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-247T06:33:00,000T12:23:00,4-Sep-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-247T06:33:00,002T00:00:00,4-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-247T06:33:00,002T00:00:00,4-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-247T07:13:00,000T16:00:00,4-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-247T07:13:00,000T16:00:00,4-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-247T07:48:00,001T22:45:00,4-Sep-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S S63,Range enter= 16.002150 Rs exit= 8.6158938 Range altitude= 14399.748 km ... -40035.005,,,,,, 2010-247T18:56:00,000T02:00:00,4-Sep-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-247T20:56:00,001T09:37:00,4-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-247T23:13:00,000T03:39:00,4-Sep-10,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map,"3x3 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-247T23:13:00,000T03:39:00,4-Sep-10,ISS,SPASS Rider,Saturn,REGMAP,Regional mapping,Day WAC and probably some night NAC,"Rider on VIMS to monitor day side clouds in WAC every hour, or search for lightning at the night side with NAC",,,,,, 2010-248T02:52:00,000T01:07:00,5-Sep-10,ISS,Prime,Telesto,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Telesto across Rhea","Images of mutual event, transit of Telesto across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-248T03:59:00,000T15:24:00,5-Sep-10,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map #2,"3x3 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-248T03:59:00,000T15:24:00,5-Sep-10,ISS,SPASS Rider,Saturn,REGMAP,Regional mapping,Day WAC and probably some night NAC,"Rider on VIMS to monitor day side clouds in WAC every hour, or search for lightning at the night side with NAC",,,,,, 2010-248T21:33:00,000T09:00:00,5-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-248T22:33:00,000T08:00:00,5-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10248_SP,rider,,,,,, 2010-249T06:33:00,006T18:11:00,6-Sep-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-249T06:33:00,003T17:02:00,6-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-249T06:33:00,006T18:11:00,6-Sep-10,CDA,Non-SPASS,Other,RATE001A,,Data rate,Datarate request to cover the given time frame with the necessary dv and data rate,,,,,, 2010-249T06:33:00,000T00:43:00,6-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-249T06:33:00,003T00:25:00,6-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-249T06:33:00,002T23:45:00,6-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-249T06:38:00,000T00:02:00,6-Sep-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S63 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-249T07:16:00,000T00:07:00,6-Sep-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-249T07:19:00,000T23:04:00,6-Sep-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_137SA_MIRMAP002_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-249T07:23:00,000T00:05:00,6-Sep-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-249T07:28:00,000T00:33:00,6-Sep-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-249T08:01:00,000T00:30:00,6-Sep-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-249T08:31:00,003T15:29:00,6-Sep-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-250T06:23:00,000T00:30:00,7-Sep-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-250T07:33:00,000T09:00:00,7-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-250T08:33:00,000T08:00:00,7-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10250_SP,rider,,,,,, 2010-250T17:13:00,000T05:00:00,7-Sep-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-250T17:13:00,000T05:00:00,7-Sep-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-250T17:13:00,000T05:00:00,7-Sep-10,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2010-250T19:00:00,000T21:00:00,7-Sep-10,CDA,Non-SPASS,Other,DECON,Decontamination,Decon Activity,Decon activity before ISD survey at apoapse,,,,,, 2010-250T22:13:00,000T06:00:00,7-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_137SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-250T22:13:00,000T06:00:00,7-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-251T04:13:00,000T05:00:00,8-Sep-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-251T04:13:00,000T05:00:00,8-Sep-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-251T04:13:00,000T05:00:00,8-Sep-10,VIMS,Non-SPASS,Saturn,WIND5HR,,Wind Observation #2,Ride-along with ISS,,,,,, 2010-251T09:13:00,000T09:55:00,8-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-251T09:13:00,000T09:55:00,8-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-251T19:08:00,000T01:30:00,8-Sep-10,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 113.6 requested range 1.5 Mkm",,,,,, 2010-251T19:08:00,000T01:30:00,8-Sep-10,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-251T19:08:00,000T01:30:00,8-Sep-10,VIMS,SPASS Rider,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 114 deg, range = 1.5 Mkm",,,,,, 2010-251T21:18:00,000T09:00:00,8-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-251T23:03:00,000T07:15:00,8-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10251_SP,rider,,,,,, 2010-252T00:00:00,000T01:08:00,9-Sep-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-252T06:18:00,003T14:44:00,9-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-252T06:58:00,000T06:45:00,9-Sep-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-252T07:00:00,000T10:00:00,9-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-252T13:43:00,000T05:00:00,9-Sep-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-252T13:43:00,013T06:37:00,9-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-252T13:43:00,000T05:00:00,9-Sep-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-252T13:43:00,000T05:00:00,9-Sep-10,VIMS,Non-SPASS,Saturn,WIND5HR,,Wind Observation #3,Ride-along with ISS,,,,,, 2010-252T18:43:00,000T06:00:00,9-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_137SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-252T18:43:00,000T06:00:00,9-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-252T23:35:00,003T01:09:00,9-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-253T00:00:00,000T00:34:00,10-Sep-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2010-253T00:34:00,003T00:12:00,10-Sep-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-253T00:43:00,000T05:00:00,10-Sep-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-253T00:43:00,000T05:00:00,10-Sep-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-253T00:43:00,000T05:00:00,10-Sep-10,VIMS,Non-SPASS,Saturn,WIND5HR,,Wind Observation #4,Ride-along with ISS,,,,,, 2010-253T05:43:00,000T06:00:00,10-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_137SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-253T05:43:00,000T06:00:00,10-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-253T07:00:00,000T10:00:00,10-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-253T11:43:00,000T05:00:00,10-Sep-10,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-253T11:43:00,000T05:00:00,10-Sep-10,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-253T11:43:00,000T05:00:00,10-Sep-10,VIMS,Non-SPASS,Saturn,WIND5HR,,Wind Observation #5,Ride-along with ISS,,,,,, 2010-253T17:43:00,000T00:30:00,10-Sep-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-253T18:13:00,000T01:30:00,10-Sep-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 73.2 requested range 1.5 Mkm",,,,,, 2010-253T18:13:00,000T01:30:00,10-Sep-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-253T18:13:00,000T01:30:00,10-Sep-10,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 73 deg, range = 1.5 Mkm",,,,,, 2010-253T20:23:00,000T10:20:00,10-Sep-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-253T21:03:00,000T09:00:00,10-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-253T22:03:00,000T08:00:00,10-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10253_SP,rider,,,,,, 2010-254T06:43:00,001T02:39:00,11-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_137SA_COMPSIT004,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-254T06:43:00,001T02:39:00,11-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-254T07:00:00,000T10:00:00,11-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-255T13:12:00,000T04:10:00,12-Sep-10,ISS,Prime,Other,HYRPHA,,Hyrrokkin,Observation of irregular moon of Saturn.,,,,,, 2010-255T21:02:00,000T03:42:00,12-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-255T21:02:00,000T09:00:00,12-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-255T22:02:00,000T08:00:00,12-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_137IC_DSCAL10255_SP,rider,,,,,, 2010-256T00:44:00,009T04:48:00,13-Sep-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-256T00:44:00,009T04:48:00,13-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-256T00:44:00,009T10:54:00,13-Sep-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.002150 Rs exit= 8.6158938 Range altitude= 14399.748 km ... -40035.005,,,,,, 2010-256T00:44:00,004T05:03:00,13-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-256T00:46:00,000T02:00:05,13-Sep-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-256T00:46:05,000T00:00:01,13-Sep-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 19.9 d, inc = 4.6 deg, r = 43.542 Rs, phase = 96 deg",,,,,, 2010-256T02:46:05,003T03:00:55,13-Sep-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-256T06:42:00,000T10:10:00,13-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_138SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-256T06:42:00,000T10:10:00,13-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-256T16:52:00,000T00:30:00,13-Sep-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-256T17:22:00,000T01:30:00,13-Sep-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 68.4 requested range 2.3 Mkm",,,,,, 2010-256T17:22:00,000T01:30:00,13-Sep-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-256T17:22:00,000T01:30:00,13-Sep-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 68 deg, range = 2.3 Mkm",,,,,, 2010-256T21:02:00,000T09:00:00,13-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-256T22:02:00,000T08:00:00,13-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10256_SP,rider,,,,,, 2010-257T06:42:00,000T13:25:00,14-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-257T06:42:00,000T13:25:00,14-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-257T07:00:00,000T10:00:00,14-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-257T20:47:00,000T09:00:00,14-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-257T21:47:00,000T08:00:00,14-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10257_SP,rider,,,,,, 2010-258T06:00:00,000T10:00:00,15-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-258T06:27:00,000T02:00:00,15-Sep-10,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-258T06:27:00,000T02:00:00,15-Sep-10,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-258T06:27:00,000T02:00:00,15-Sep-10,VIMS,Non-SPASS,Saturn,WIND2HR,,2-hr Wind Observation #1,Ride-along with ISS,,,,,, 2010-258T08:27:00,000T09:00:00,15-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_138SA_COMPSIT002,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-258T08:27:00,000T09:00:00,15-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-258T17:27:00,000T02:00:00,15-Sep-10,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-258T17:27:00,000T02:00:00,15-Sep-10,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-258T17:27:00,000T02:00:00,15-Sep-10,VIMS,Non-SPASS,Saturn,WIND2HR,,2-hr Wind Observation #2,Ride-along with ISS,,,,,, 2010-258T20:47:00,000T09:00:00,15-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-258T21:47:00,000T08:00:00,15-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10258_SP,rider,,,,,, 2010-259T05:47:00,001T00:00:00,16-Sep-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-259T06:00:00,000T10:00:00,16-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-259T06:27:00,000T13:40:00,16-Sep-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_138SA_MIRMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-259T20:47:00,000T09:00:00,16-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-259T21:47:00,000T08:00:00,16-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10259_SP,rider,,,,,, 2010-260T05:47:00,004T10:00:00,17-Sep-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-260T05:47:00,004T14:48:00,17-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-260T06:27:00,000T16:00:00,17-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-260T06:27:00,000T16:00:00,17-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-260T22:27:00,000T00:30:00,17-Sep-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-260T22:57:00,000T07:10:00,17-Sep-10,ISS,Prime,Other,KIVSUP,,Kiviuq,Observation of irregular moon of Saturn.,,,,,, 2010-261T06:47:00,000T09:00:00,18-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-261T07:47:00,000T08:00:00,18-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10261_SP,rider,,,,,, 2010-261T16:27:00,000T02:00:00,18-Sep-10,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-261T16:27:00,000T02:00:00,18-Sep-10,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-261T16:27:00,000T02:00:00,18-Sep-10,VIMS,Non-SPASS,Saturn,WIND2HR,,2-hr Wind Observation #3,Ride-along with ISS,,,,,, 2010-261T18:27:00,000T09:00:00,18-Sep-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_138SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-261T18:27:00,000T09:00:00,18-Sep-10,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2010-261T18:27:00,000T09:00:00,18-Sep-10,VIMS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS Compsit Ridealong,Ridealong with CIRS,,,,,, 2010-262T03:27:00,000T02:00:00,19-Sep-10,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2010-262T03:27:00,000T02:00:00,19-Sep-10,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2010-262T03:27:00,000T02:00:00,19-Sep-10,VIMS,Non-SPASS,Saturn,WIND2HR,,2-hr Wind Observation #4,Ride-along with ISS,,,,,, 2010-262T06:47:00,000T09:00:00,19-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-262T07:47:00,000T08:00:00,19-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10262_SP,rider,,,,,, 2010-262T16:27:00,000T13:40:00,19-Sep-10,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,CIRS_138SA_MIRMAP002_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2010-262T16:27:00,000T13:40:00,19-Sep-10,VIMS,Non-SPASS,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ridealong,Ridealong with CIRS,,,,,, 2010-263T06:47:00,000T09:00:00,20-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-263T07:47:00,000T08:00:00,20-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10263_SP,rider,,,,,, 2010-263T16:27:00,000T13:40:00,20-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-263T16:27:00,000T13:40:00,20-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-264T06:47:00,000T09:00:00,21-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-264T07:47:00,000T08:00:00,21-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10264_SP,rider,,,,,, 2010-264T15:47:00,000T13:45:00,21-Sep-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-264T16:27:00,000T01:30:00,21-Sep-10,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 154.5 requested range 2.1 Mkm",,,,,, 2010-264T16:27:00,000T01:30:00,21-Sep-10,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-264T17:27:00,000T02:25:00,21-Sep-10,ISS,Non-SPASS,Saturn,REGMAP,Regional mapping,Night NAC lightning search,Rider on VIMS to search for lightning at the night side with NAC,,,,,, 2010-264T17:57:00,000T01:55:00,21-Sep-10,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map #1,"3x3 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-264T20:32:00,000T08:00:00,21-Sep-10,MIMI,SPASS Rider,Saturn,OVSPONGE,,Sponge bits,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-264T20:32:00,000T09:00:00,21-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-264T20:35:00,002T06:50:00,21-Sep-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-264T21:32:00,000T08:00:00,21-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10664_SP,rider,,,,,, 2010-264T21:32:00,000T06:00:00,21-Sep-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-264T23:00:00,000T04:33:04,21-Sep-10,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2010-265T05:32:00,001T23:45:00,22-Sep-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-265T05:32:00,001T23:45:00,22-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-265T05:32:00,000T15:24:35,22-Sep-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-265T06:12:00,000T06:32:00,22-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-265T06:12:00,000T06:52:00,22-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-265T11:38:00,001T18:30:00,22-Sep-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 8.5998408 Rs exit= 15.999876 Range altitude= -39939.023 km ... 13744.244,,,,,, 2010-265T13:04:00,000T03:03:00,22-Sep-10,VIMS,Prime,rings(general),HIPHASE,High phase observation,High Phase Ring Monitor,Dark face.,,,,,, 2010-265T16:07:00,000T02:49:00,22-Sep-10,UVIS,Prime,Saturn,USUNOCC,Solar occultation,Solar Occ Egress,This is a PIE. This is an egress solar occultation of Saturn. Following timing to be adusted to available time. EUV solar occultation port centered on Sun. 1) 20 minute observation margin. 2) Record data during egress. Data collection start time: 2010-265T16:38:22.0. Data collection end time: 2010-265T17:56:33.0. 3) 20 minute observation margin. 4) 30 minutes for turn to waypoint. Total data collection time: 4691s Total observation request duration: 9540 s bps (from Alain's spreadsheet): 18918.883 bps Total data volume: 88.74848e+6 bits Times at start and end of egress based on 091005 kernel.,,,,,, 2010-265T16:07:00,000T02:49:00,22-Sep-10,VIMS,SPASS Rider,Saturn,USUNOCC,Solar occultation,Saturn Solar Occultation egress,Saturn Solar Occultation egress. UVIS ridealong.,,,,,, 2010-265T19:16:00,000T02:09:00,22-Sep-10,ISS,Prime,Enceladus,PLMHRHP,,High res plume obs at high phase,High resolution plume observation at high phase,,,,,, 2010-265T19:16:00,000T01:55:00,22-Sep-10,CIRS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,CIRS_138EN_PLUME001_ISS,"rider, FP1 and FP3 only",,,,,, 2010-265T19:16:00,000T01:55:00,22-Sep-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-265T19:16:00,000T02:09:00,22-Sep-10,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,enceladus plume,null,,,,,, 2010-265T20:20:00,000T07:25:00,22-Sep-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-265T20:56:35,000T00:30:00,22-Sep-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-265T20:57:00,000T02:00:00,22-Sep-10,CDA,Non-SPASS,DustRAM direction,RPX0040,,CDA RPXing 2010-265T21:57:00,RPXing at 3.7798492 Rs,,,,,, 2010-265T21:00:00,000T02:00:00,22-Sep-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-265T21:26:35,000T01:00:00,22-Sep-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-265T22:05:00,000T01:05:00,22-Sep-10,VIMS,Prime,Saturn,ALPORIOCC,Alpha Orion occultation,alpOri Saturn Atmosphere Occultation,"Unlit limb, high N latitude.",,,,,, 2010-265T22:05:00,000T01:05:00,22-Sep-10,CIRS,SPASS Rider,Saturn,ALPORIOCC,Alpha Orion occultation,CIRS_138SA_ALPORIOCC001_VIMS,Ride along with VIMS. Stellar Occ Saturn,,,,,, 2010-265T22:26:35,000T00:30:00,22-Sep-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-265T22:56:35,000T23:00:00,22-Sep-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-265T23:10:00,000T02:07:00,22-Sep-10,UVIS,Prime,Star,URBETORI,,URSTAR,,,,,,, 2010-265T23:10:00,000T02:07:00,22-Sep-10,UVIS,SPASS Rider,Star,URBETORI,,Support Imaging,NAC and WAC support images at 2010-266T00:38:15 2010-266T00:24:06,,,,,, 2010-265T23:10:00,000T02:07:00,22-Sep-10,ISS,Non-SPASS,Star,URBETORI,,UVIS occultation rider,UVIS occultation rider,,,,,, 2010-265T23:58:56,000T00:00:01,22-Sep-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.456 Rs, lat = 3 deg, phase = 84 deg",,,,,, 2010-266T01:17:00,000T06:00:00,23-Sep-10,CIRS,Prime,Saturn,LIMBINT,Limb integration,CIRS_138SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-266T01:17:00,000T06:00:00,23-Sep-10,UVIS,Non-SPASS,Titan,LMBINT,,Rider to CIRS,Rider to CIRS.,,,,,, 2010-266T03:45:00,001T01:32:00,23-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-266T07:17:00,000T05:28:00,23-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-266T07:17:00,000T05:28:00,23-Sep-10,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2010-266T07:17:00,000T05:28:00,23-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-266T12:45:00,000T02:00:00,23-Sep-10,ISS,Prime,Enceladus,GLOCOLR,,Low phase Enceladus observation,Low phase Enceladus observation,,,,,, 2010-266T12:45:00,000T02:00:00,23-Sep-10,CIRS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,CIRS_138EN_PLUME002_ISS,"rider, FP1 and FP3 only",,,,,, 2010-266T12:45:00,000T02:00:00,23-Sep-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-266T12:45:00,000T02:00:00,23-Sep-10,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,enceladus plume,enceladus plume,,,,,, 2010-266T14:45:00,000T04:52:00,23-Sep-10,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2010-266T14:45:00,000T04:52:00,23-Sep-10,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2010-266T20:17:00,000T09:00:00,23-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-266T21:56:35,000T07:20:25,23-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-266T22:02:00,000T07:15:00,23-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10266_SP,rider,,,,,, 2010-267T03:25:00,000T01:52:00,24-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-267T05:17:00,000T11:21:41,24-Sep-10,MIMI,SPASS Rider,Saturn,DUSKMSPH,,MIMI Magnetospheric Dymanics,"Part of Dusk Magnetosphere MAPS Campaign. Set up MIMI for with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dusk-side magnetosphere at a variety of radial distances.",,,,,, 2010-267T05:17:00,000T11:21:41,24-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-267T05:17:00,000T01:21:41,24-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-267T05:17:00,000T11:21:41,24-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-267T05:17:00,002T01:00:00,24-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-267T06:08:00,010T14:54:00,24-Sep-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 16.011850 Rs exit= 39.100677 Range altitude= 13716.615 km ... -103198.92,,,,,, 2010-267T06:12:41,000T03:26:00,24-Sep-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-267T06:12:41,000T03:26:00,24-Sep-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T06:12:41,000T03:26:00,24-Sep-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,VIMS ridealong with CIRS. Stare at Titan for global mapping. Phase = 144 deg. Lat/Lon = 02N/06 deg. Resolution = 135 km/px. Obtain cubes for global mapping of Titan. Template N.,,,,,, 2010-267T06:38:41,000T11:00:00,24-Sep-10,INMS,Non-SPASS,Saturn,T72INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-267T09:38:41,000T04:00:00,24-Sep-10,CIRS,Prime,Titan,MIRLMPAIR,,,"Obtain temperatures in Titan's stratosphere at 225 km with FP4, FP3 at higher altitude. Measurement at a single latitude.",,,,,, 2010-267T09:38:41,000T04:00:00,24-Sep-10,ISS,SPASS Rider,Titan,MIRLMPAIR,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T09:38:41,000T04:00:00,24-Sep-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping.,VIMS ridealong with CIRS. Titan limb mapping. Phase = 143 deg. Lat/Lon = 02N/09 deg. Resolution = 90 km/px. Obtain cubes for limb mapping of Titan. Template R.,,,,,, 2010-267T13:38:41,000T02:45:00,24-Sep-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-267T13:38:41,000T02:45:00,24-Sep-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T13:38:41,000T02:45:00,24-Sep-10,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Titan scan.,VIMS ridealong with CIRS while scanning across Titan. Phase = 140 deg. Lat/Lon = 01N/10 deg. Resolution = 49 km/px. Obtain cubes while scanning across Titan. Template T.,,,,,, 2010-267T16:23:41,000T01:00:00,24-Sep-10,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2010-267T16:23:41,000T01:00:00,24-Sep-10,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T16:23:41,000T02:00:00,24-Sep-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,VIMS ridealong with CIRS for regional mapping of Titan. Phase = 134 deg. Lat/Lon = 01S/06 deg. Resolution = 22 km/px. Obtain cubes for regional mapping of Titan prior to C/A..,,,,,, 2010-267T16:23:41,000T01:00:00,24-Sep-10,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2010-267T16:38:41,000T01:00:00,24-Sep-10,CAPS,SPASS Rider,Titan,T72INBND,,Inbound 138TI (T72),Inbound 117TI (T61),,,,,, 2010-267T16:38:41,000T01:00:00,24-Sep-10,MIMI,SPASS Rider,Titan,TITANIN,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-267T16:38:41,000T04:00:00,24-Sep-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T72 flyby,"T72 is an upstream, pre-dusk, high altitude (>4000 km) ?blind? flyby that will be useful to characterize the background field in which Titan sits in. We assign grade two priority. Data rate: 1976bps (32vps).",,,,,, 2010-267T17:23:41,000T00:30:00,24-Sep-10,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2010-267T17:23:41,000T00:30:00,24-Sep-10,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T17:38:41,000T02:00:00,24-Sep-10,CAPS,SPASS Rider,Titan,T72CLOSE,,Closest Approach 138TI (T72),Closest Approach 117TI (T61),,,,,, 2010-267T17:38:41,000T02:00:00,24-Sep-10,MIMI,SPASS Rider,Titan,TITANCA,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-267T17:38:41,000T02:00:00,24-Sep-10,INMS,Non-SPASS,Titan,TITAN72,,Titan Flyby,Titan observation,,,,,, 2010-267T17:38:41,000T02:00:00,24-Sep-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-267T17:53:41,000T00:30:00,24-Sep-10,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2010-267T17:53:41,000T00:30:00,24-Sep-10,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T18:23:41,000T02:30:00,24-Sep-10,VIMS,Prime,Titan,HIGHRES,High resolution observartion,Regional mapping.,Regional mapping of Titan during C/A. Phase = 84 deg. Lat/Lon = 12S/316 deg. Resolution = 4.7 km/px. Obtain mosaics for regional mapping during C/A.,,,,,, 2010-267T18:23:41,000T02:30:00,24-Sep-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-267T18:23:41,000T02:30:00,24-Sep-10,ISS,SPASS Rider,Titan,HIGHRES,High resolution observartion,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T19:38:41,000T01:00:00,24-Sep-10,CAPS,SPASS Rider,Titan,T72OUTBND,,Outbound 138TI (T72),Outbound 117TI (T61),,,,,, 2010-267T19:38:41,000T01:00:00,24-Sep-10,MIMI,SPASS Rider,Titan,TITANOUT,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-267T19:38:41,000T11:00:00,24-Sep-10,INMS,Non-SPASS,Saturn,T72OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-267T20:38:41,001T09:38:19,24-Sep-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-267T20:38:41,001T09:38:19,24-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-267T20:38:41,001T14:38:19,24-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-267T20:53:41,000T06:45:00,24-Sep-10,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2010-267T20:53:41,000T06:45:00,24-Sep-10,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2010-267T20:53:41,000T06:45:00,24-Sep-10,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-267T20:53:41,000T02:45:00,24-Sep-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,VIMS ridealong with UVIS while scanning across Titan. Phase = 25 deg. Lat/Lon = 05S/214 deg. Resolution = 22 km/px. Obtain cubes while scanning across Titan. Template X.,,,,,, 2010-267T23:38:41,000T04:00:00,24-Sep-10,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,VIMS ridealong with UVIS while scanning across Titan. Phase = 31 deg. Lat/Lon = 04S/209 deg. Resolution = 49 km/px. Obtain cubes while scanning across Titan. Template X.,,,,,, 2010-268T03:38:41,000T05:00:00,25-Sep-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping.,Global mapping of Titan. Phase = 34 deg. Lat/Lon = 03S/210 deg. Resolution = 89 km/px. Temp. V. Obtain cubes of various exposure times for global mapping.,,,,,, 2010-268T03:38:41,000T05:00:00,25-Sep-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-268T03:38:41,000T05:00:00,25-Sep-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-268T06:38:41,000T23:38:19,25-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-268T08:38:41,000T08:25:00,25-Sep-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping.,Global mapping of Titan. Phase = 35 deg. Lat/Lon = 02S/213 deg. Resolution = 140 km/px. Temp. B. Obtain cubes of various exposure times for global mapping.,,,,,, 2010-268T08:38:41,000T08:25:00,25-Sep-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2010-268T08:38:41,000T08:25:00,25-Sep-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-268T19:32:00,000T10:45:00,25-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-268T20:32:00,000T09:45:00,25-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10268_SP,rider,,,,,, 2010-269T06:17:00,006T05:43:00,26-Sep-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-269T06:17:00,008T14:45:00,26-Sep-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-269T06:17:00,001T22:45:00,26-Sep-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-269T06:17:00,000T03:00:00,26-Sep-10,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-269T06:17:00,002T09:00:00,26-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-269T09:00:00,001T06:00:00,26-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-269T09:17:00,000T02:00:00,26-Sep-10,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2010-269T11:17:00,000T06:45:00,26-Sep-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-269T18:02:00,007T17:40:00,26-Sep-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-269T20:17:00,000T09:00:00,26-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-269T21:17:00,000T08:00:00,26-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10269_SP,rider,,,,,, 2010-270T06:00:00,000T01:30:00,27-Sep-10,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 43.7 requested range 1.3 Mkm",,,,,, 2010-270T06:00:00,000T01:30:00,27-Sep-10,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-270T06:00:00,000T01:30:00,27-Sep-10,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 44 deg, range = 1.3 Mkm",,,,,, 2010-270T07:30:00,000T04:00:00,27-Sep-10,CAPS,Prime,co-rotation,IONCALPTG,,MAPS ion calibration,null,,,,,, 2010-270T07:30:00,000T04:00:00,27-Sep-10,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2010-270T11:30:00,000T07:50:00,27-Sep-10,CAPS,Prime,Saturn,SWAURPTG,MAPS aurora campaign,MAPS solar wind/aurora w/ prime pointing,null,,,,,, 2010-270T11:30:00,000T01:08:00,27-Sep-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-270T20:02:00,000T09:00:00,27-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-270T21:02:00,000T08:00:00,27-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10270_SP,rider,,,,,, 2010-271T05:02:00,000T10:15:00,28-Sep-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-271T06:17:00,000T09:00:00,28-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-271T07:17:00,000T08:00:00,28-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10271_SP,rider,,,,,, 2010-271T15:17:00,006T05:45:00,28-Sep-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-271T15:17:00,006T05:45:00,28-Sep-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-272T20:02:00,000T09:00:00,29-Sep-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-272T21:02:00,000T08:00:00,29-Sep-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10272_SP,rider,,,,,, 2010-273T06:00:00,000T10:00:00,30-Sep-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-274T06:00:00,000T10:00:00,1-Oct-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-274T19:47:00,000T09:00:00,1-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-274T20:47:00,000T08:00:00,1-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10274_SP,rider,,,,,, 2010-275T12:00:00,002T09:02:00,2-Oct-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-276T13:32:00,000T09:00:00,3-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-276T14:32:00,000T08:00:00,3-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_138IC_DSCAL10276_SP,rider,,,,,, 2010-276T22:32:00,000T04:00:00,3-Oct-10,ISS,Prime,Other,KIVPHA,,Kiviuq,Observation of irregular moon of Saturn.,,,,,, 2010-276T22:32:00,000T04:00:00,3-Oct-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-277T00:00:00,001T06:00:00,4-Oct-10,CDA,Non-SPASS,DustRAM direction,ISD,,CDA ISD,"CDA to interstellar dust direction (approx 259, 8 in heliocentric ecliptical coord.)",,,,,, 2010-277T02:32:00,000T04:00:00,4-Oct-10,ISS,Prime,Other,SIAPHA,,Siarnaq,Observation of irregular moon of Saturn.,,,,,, 2010-277T02:32:00,000T04:00:00,4-Oct-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-277T06:32:00,000T05:00:00,4-Oct-10,ISS,Prime,Other,HYRRES,,Hyrrokkin,Observation of irregular moon of Saturn.,,,,,, 2010-277T06:32:00,000T05:00:00,4-Oct-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-277T11:32:00,000T16:10:00,4-Oct-10,CAPS,Prime,Saturn,SWAURPTG,MAPS aurora campaign,MAPS solar wind/aurora w/ prime pointing,null,,,,,, 2010-277T11:42:00,000T05:00:00,4-Oct-10,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2010-277T16:42:00,006T11:35:00,4-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-277T20:47:52,000T00:00:01,4-Oct-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 23.8 d, inc = 3.0 deg, r = 48.780 Rs, phase = 101 deg",,,,,, 2010-277T21:02:00,003T20:58:00,4-Oct-10,MIMI,SPASS Rider,Saturn,SWAURORA,Solar wind campaign,MAPS SWAurora Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2010-277T21:02:00,006T07:15:00,4-Oct-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-277T21:02:00,006T07:15:00,4-Oct-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 16.011850 Rs exit= 39.100677 Range altitude= 13716.615 km ... -103198.92,,,,,, 2010-277T21:02:00,000T02:00:00,4-Oct-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-277T21:02:00,002T03:30:00,4-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-277T23:02:00,006T05:15:00,4-Oct-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-278T04:00:00,000T11:15:00,5-Oct-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-278T05:47:00,000T09:00:00,5-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-278T06:47:00,000T08:00:00,5-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10278_SP,rider,,,,,, 2010-278T15:15:00,001T01:00:00,5-Oct-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_139SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-279T16:15:00,000T01:00:00,6-Oct-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-279T19:32:00,000T09:00:00,6-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-279T20:32:00,000T08:00:00,6-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10279_SP,rider,,,,,, 2010-280T00:32:00,004T03:45:00,7-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-280T05:15:00,001T08:00:00,7-Oct-10,UVIS,Prime,Saturn,MOS138APO,,,"Mosaic scan of Saturn magnetosphere, first 32.0-hr block of time. Scan pattern of the UVIS slit boresight is a rectangle with Saturn at the midpoint of the lower edge. The rectangle extends out to +/- 10 Rs along the east-west direction and from 0 to approx. 2.88 Rs northward. (The two 32-hr blocks combine to form three east-west swaths stretching from -10 Rs to +10 Rs; one swath lies along the Saturn equator, while the second lies just north and the third lies just south.) Allowances of 30 minutes for turn to/from waypoint and 20 minutes observation margin have been included at each end of the observation. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 275.0 s, stop data capture. Repeat PATTERN-A 111 times. Slew -0.064 rad about the x-axis. Start data capture, stare 275.0 s, stop data capture. Repeat PATTERN-B 222 times. Return boresight to Saturn center: slew +0.064 rad about the x-axis and +0.222222 rad about the z-axis. PATTERN-A: Slew +1.5 mrad about z-axis. Start data capture, stare 275.0 s, stop data capture. PATTERN-B: Slew -1.5 mrad about z-axis. Start data capture, stare 275.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (4402.94005 bps, from Alain Jouchoux's spreadsheet)x(275.0s per stare)x(335 stares) = 405.6209x10^6 bits.",,,,,, 2010-281T13:15:00,000T04:00:00,8-Oct-10,ISS,Prime,Other,KIVPHA,,Kiviuq,Observation of irregular moon of Saturn.,,,,,, 2010-281T13:15:00,000T04:00:00,8-Oct-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-281T18:00:00,002T10:17:00,8-Oct-10,MIMI,SPASS Rider,Saturn,MAGBOUND,MAPS magnetosphere boundary campaign,MAPS MB/A Campaign,"Part of MB/A MAPS Campaign. Set up MIMI for magnetospheric boundaries campaign with corotation pointing. Pointing: -X to corotation, Saturn B in X, Z plane; or spin about Z. Observe dawn-side magnetospheric boundaries at a variety of radial distances.",,,,,, 2010-281T19:32:00,000T09:00:00,8-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-281T20:32:00,000T08:00:00,8-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10281_SP,rider,,,,,, 2010-282T05:15:00,001T08:00:00,9-Oct-10,UVIS,Prime,Saturn,MOS138APO,,,"Mosaic scan of Saturn magnetosphere, second 32.0-hr block of time. Scan pattern of the UVIS slit boresight is a rectangle with Saturn at the midpoint of the lower edge. The rectangle extends out to +/- 10 Rs along the east-west direction and from 0 to approx. 2.88 Rs southward. (The two 32-hr blocks combine to form three east-west swaths stretching from -10 Rs to +10 Rs; one swath lies along the Saturn equator, while the second lies just north and the third lies just south.) Allowances of 30 minutes for turn to/from waypoint and 20 minutes observation margin have been included at each end of the observation. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Slew from WAYPOINT to Saturn center. Align slit with Saturn spin axis. Start data capture, stare 275.0 s, stop data capture. Repeat PATTERN-A 111 times. Slew +0.064 rad about the x-axis. Start data capture, stare 275.0 s, stop data capture. Repeat PATTERN-B 222 times. Return boresight to Saturn center: slew -0.064 rad about the x-axis and -0.222222 rad about the z-axis. PATTERN-A: Slew -1.5 mrad about z-axis. Start data capture, stare 275.0 s, stop data capture. PATTERN-B: Slew +1.5 mrad about z-axis. Start data capture, stare 275.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (4402.94005 bps, from Alain Jouchoux's spreadsheet)x(275.0s per stare)x(335 stares) = 405.6209x10^6 bits.",,,,,, 2010-283T19:17:00,000T09:00:00,10-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-283T20:17:00,000T08:00:00,10-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10283_SP,rider,,,,,, 2010-284T04:17:00,003T23:45:00,11-Oct-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-284T04:17:00,004T14:44:00,11-Oct-10,CDA,Non-SPASS,Other,RATE001,,Data rate,Datarate request to cover the given time frame with the necessary dv and data rate,,,,,, 2010-284T04:17:00,000T00:43:00,11-Oct-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-284T04:17:00,003T23:45:00,11-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-284T04:17:00,017T14:04:00,11-Oct-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-284T04:17:00,003T23:45:00,11-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-284T04:22:00,000T00:02:00,11-Oct-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S64 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-284T04:47:00,000T13:00:00,11-Oct-10,CDA,Prime,DustRAM direction,ISD0020,,CDA ISD 2010-301T18:21:00,ISD observation around apoapse 2010-301T18:21:00 49.167032 Rs,,,,,, 2010-284T05:00:00,000T00:07:00,11-Oct-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-284T05:07:00,000T00:05:00,11-Oct-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-284T05:12:00,000T00:33:00,11-Oct-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-284T05:45:00,000T00:30:00,11-Oct-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-284T06:15:00,003T00:02:00,11-Oct-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-284T19:17:00,000T09:00:00,11-Oct-10,RSS,SPASS Rider,Earth,SCE7,,Solar Conjunction Experiment (SCE) #7,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2010-284T19:17:00,000T09:00:00,11-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-284T20:17:00,000T08:00:00,11-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10284_SP,rider,,,,,, 2010-285T00:00:00,000T01:08:00,12-Oct-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-285T05:00:00,000T01:30:00,12-Oct-10,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 152.5 requested range 1.2 Mkm",,,,,, 2010-285T05:00:00,000T01:30:00,12-Oct-10,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-285T06:30:00,000T01:00:00,12-Oct-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-285T07:30:00,000T03:00:00,12-Oct-10,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2010-285T19:17:00,000T09:00:00,12-Oct-10,RSS,SPASS Rider,Earth,SCE7,,Solar Conjunction Experiment (SCE) #7,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2010-285T19:17:00,000T09:00:00,12-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-285T20:17:00,000T08:00:00,12-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10285_SP,rider,,,,,, 2010-286T04:47:00,000T12:30:00,13-Oct-10,ISS,Prime,rings(general),HPLELR,,Faint Ring High Phase Observation,Observation of faint rings at low elevation angles and high phase,,,,,, 2010-286T04:47:00,000T12:30:00,13-Oct-10,CIRS,SPASS Rider,rings(general),HPLELR,,,null,,,,,, 2010-286T04:47:00,000T12:30:00,13-Oct-10,VIMS,SPASS Rider,rings(general),HPLELR,,Rings high phase observation,ISS rider - 1000 msec integration time,,,,,, 2010-286T17:17:00,000T11:00:00,13-Oct-10,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-34 in 1-way mode. No rolling during 3 hours USO from 2010-286T19:17:00 till 2010-286T22:17:00.,,,,,, 2010-286T19:17:00,000T09:00:00,13-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-286T20:17:00,000T08:00:00,13-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10286_SP,rider,,,,,, 2010-287T04:52:00,000T13:30:00,14-Oct-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-287T04:52:00,000T13:30:00,14-Oct-10,ISS,SPASS Rider,Titan,COMPMAP,Composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-287T04:52:00,000T13:30:00,14-Oct-10,VIMS,SPASS Rider,Titan,COMPMAP,Composition map,XD - Titan Monitoring Campaign,"range is 178,000 to 175,000 km - phase is less than 90 during the last 3 hours",,,,,, 2010-287T06:17:00,000T00:34:00,14-Oct-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2010-287T06:51:00,000T21:11:00,14-Oct-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-287T19:02:00,000T09:00:00,14-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-287T20:02:00,000T08:00:00,14-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10287_SP,rider,,,,,, 2010-288T04:02:00,000T14:18:00,15-Oct-10,VIMS,Prime,Dione,DIONE,Dione,Dione composition,Dione composition,,,,,, 2010-288T04:02:00,000T14:18:00,15-Oct-10,CIRS,SPASS Rider,Dione,DIONE,Dione,,"FP3, FP1 only",,,,,, 2010-288T04:02:00,000T14:18:00,15-Oct-10,ISS,SPASS Rider,Dione,DIONE,Dione,Dione plume search,Sit'n'stare at high phase,,,,,, 2010-288T04:02:00,000T14:18:00,15-Oct-10,UVIS,SPASS Rider,Dione,ICYSTARE,,ICYSTARE: Deep integration to see volatiles,Map volatiles in system in immediate neighborhood of satelliite.,,,,,, 2010-288T04:02:00,003T00:00:00,15-Oct-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-288T04:02:00,000T10:38:44,15-Oct-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-288T04:02:00,001T11:48:00,15-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-288T04:02:00,000T09:58:00,15-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-288T14:00:00,002T06:50:00,15-Oct-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-288T14:40:44,000T12:39:16,15-Oct-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-288T18:20:00,000T09:00:00,15-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-288T19:01:00,002T00:10:00,15-Oct-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.087078 Rs exit= 13.993632 Range altitude= -39994.170 km ... 11248.706,,,,,, 2010-288T19:20:00,000T08:00:00,15-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10288_SP,rider,,,,,, 2010-289T03:20:00,000T03:55:00,16-Oct-10,ISS,Prime,Enceladus,PLMSCECL,,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-289T03:20:00,000T03:55:00,16-Oct-10,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,FP3/4 Enceladus Observations,FP3 Rider Observations of Enceladus taken during ISS Plume observation. No FP4,,,,,, 2010-289T03:20:00,000T03:55:00,16-Oct-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-289T03:20:00,000T03:55:00,16-Oct-10,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,Plume composition,Plume composition,,,,,, 2010-289T03:20:00,000T10:20:44,16-Oct-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-289T08:46:00,000T02:30:00,16-Oct-10,VIMS,Prime,Saturn,OMICETOCC,OmiCet occultation,omiCet Saturn occultation,"omiCet atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec.",,,,,, 2010-289T08:46:00,000T02:30:00,16-Oct-10,CIRS,SPASS Rider,Saturn,OMICETOCC,OmiCet occultation,CIRS_139SA_OMICETOCC001_VIMS,PIE Collaboration with VIMS. Stellar Occ Saturn ingress T09:29 at 10N dark limb,,,,,, 2010-289T08:46:00,000T02:30:00,16-Oct-10,ISS,Non-SPASS,Saturn,OMICETOCC,OmiCet occultation,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2010-289T11:16:00,000T05:59:00,16-Oct-10,CIRS,Prime,Mimas,MIMAS,Mimas,FP1/3 Observations of Mimas,6 murad/s scans plus 15 min sit and stare. FP1 and FP3 only,,,,,, 2010-289T11:16:00,000T05:59:00,16-Oct-10,ISS,SPASS Rider,Mimas,MIMAS,Mimas,CIRS prime Mimas observation,ISS rider on CIRS prime,,,,,, 2010-289T11:16:00,000T05:59:00,16-Oct-10,UVIS,SPASS Rider,Mimas,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2010-289T11:16:00,000T05:59:00,16-Oct-10,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas composition,Mimas composition,,,,,, 2010-289T13:40:00,000T02:00:00,16-Oct-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-289T13:40:44,000T00:30:00,16-Oct-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-289T13:42:00,000T02:00:00,16-Oct-10,CDA,SPASS Rider,DustRAM direction,RPX0000,,CDA RPXing 2010-289T14:42:00,RPXing at 4.6574407 Rs,,,,,, 2010-289T14:10:44,000T01:30:00,16-Oct-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-289T15:40:44,000T23:00:00,16-Oct-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-289T15:50:00,000T04:20:00,16-Oct-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-289T17:15:00,000T01:30:00,16-Oct-10,ISS,Prime,Pallene,PALENCLOS,,Pallene close flyby,"ORS observation during ~36,130 km flyby of Pallene.",,,,,, 2010-289T17:15:00,000T01:30:00,16-Oct-10,CIRS,SPASS Rider,Pallene,PALENCLOS,,CIRS Observations of Pallene,FP1 and FP3 Observations of Pallene,,,,,, 2010-289T17:15:00,000T01:30:00,16-Oct-10,UVIS,SPASS Rider,Pallene,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2010-289T17:15:00,000T01:30:00,16-Oct-10,VIMS,SPASS Rider,Pallene,ICYLON,Icy satellite longitudinal coverage,composition,composition,,,,,, 2010-289T17:56:40,000T00:00:01,16-Oct-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.101 Rs, lat = 2 deg, phase = 80 deg",,,,,, 2010-289T18:45:00,000T02:30:00,16-Oct-10,VIMS,Prime,Saturn,ALPHYAOCC,,alpHya Saturn occultation,"alpHya atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec.",,,,,, 2010-289T18:45:00,000T02:30:00,16-Oct-10,CIRS,SPASS Rider,Saturn,ALPHYAOCC,,CIRS_139SA_ALPHYAOCC001_VIMS,PIE Collaboration with VIMS. Stellar Occ Saturn ingress T19:30 32S dark limb,,,,,, 2010-289T18:45:00,000T02:30:00,16-Oct-10,ISS,Non-SPASS,Saturn,ALPHYAOCC,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2010-289T20:10:00,001T07:52:00,16-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-290T00:15:00,000T01:30:00,17-Oct-10,CIRS,Prime,Dione,DIONE,Dione,FP1/3 Observations of Dione,FP1/3 Scans of Dione,,,,,, 2010-290T00:15:00,000T01:30:00,17-Oct-10,ISS,SPASS Rider,Dione,DIONE,Dione,Dione high phase,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-290T00:15:00,000T01:30:00,17-Oct-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2010-290T00:15:00,000T01:30:00,17-Oct-10,VIMS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione composition,Dione composition,,,,,, 2010-290T01:45:00,000T01:30:00,17-Oct-10,ISS,Prime,Dione,REGMAP,Regional mapping,Dione mapping,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-290T01:45:00,000T01:30:00,17-Oct-10,CIRS,SPASS Rider,Dione,REGMAP,Regional mapping,CIRS ISS RIDER,FP1 and FP3 only,,,,,, 2010-290T01:45:00,000T01:30:00,17-Oct-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2010-290T01:45:00,000T01:30:00,17-Oct-10,VIMS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,Dione composition,Dione composition,,,,,, 2010-290T05:30:00,000T01:30:00,17-Oct-10,CIRS,Prime,Rhea,RHEA,Rhea,Thermal Mapping of Rhea,"Thermal Mapping of Rhea's Surface, FP1 and FP3 only",,,,,, 2010-290T05:30:00,000T01:30:00,17-Oct-10,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea high phase,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-290T05:30:00,000T01:30:00,17-Oct-10,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2010-290T05:30:00,000T01:30:00,17-Oct-10,VIMS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,Rhea composition,Rhea composition,,,,,, 2010-290T07:00:00,000T01:30:00,17-Oct-10,ISS,Prime,Rhea,REGMAP,Regional mapping,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-290T07:00:00,000T01:30:00,17-Oct-10,CIRS,SPASS Rider,Rhea,REGMAP,Regional mapping,CIRS ISS RIDER,FP1 and FP3 only,,,,,, 2010-290T07:00:00,000T01:30:00,17-Oct-10,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2010-290T07:00:00,000T01:30:00,17-Oct-10,VIMS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,Rhea composition,Rhea composition,,,,,, 2010-290T14:40:44,000T13:21:16,17-Oct-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-290T16:02:00,000T11:00:00,17-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10290_SP,rider,,,,,, 2010-290T19:11:00,010T23:10:00,17-Oct-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.006526 Rs exit= 13.097546 Range altitude= 11229.343 km ... -40000.425,,,,,, 2010-290T20:50:00,000T07:12:00,17-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-291T04:02:00,020T09:02:00,18-Oct-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-291T04:02:00,000T08:30:00,18-Oct-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-291T04:02:00,007T09:47:00,18-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-291T04:02:00,010T14:19:00,18-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-291T05:00:00,000T01:00:00,18-Oct-10,ISS,Prime,Other,SFAD,,SATELLITE ORBIT CAMPAIGN,"Turn to Rhea, take 12-bit RGB triplet. Other targets as per usual SATELLORB plan if time available",,,,,, 2010-291T06:00:00,000T08:00:00,18-Oct-10,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slow slews across the auroral oval,,,,,, 2010-291T06:00:00,000T08:00:00,18-Oct-10,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2010-291T06:00:00,000T08:00:00,18-Oct-10,VIMS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Aurorae UVIS Slew,Ridealong with UVIS slew observations of aurorae,,,,,, 2010-291T12:32:00,000T02:00:00,18-Oct-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-291T14:00:00,000T02:00:00,18-Oct-10,ISS,Prime,Titan,SFAD,,Scientist for a Day,"Images of mutual event, transit of Tethys & Enceladus across Titan",,,,,, 2010-291T14:32:00,010T03:49:00,18-Oct-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-291T16:00:00,000T01:30:00,18-Oct-10,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 45.8 requested range 2.3 Mkm",,,,,, 2010-291T16:00:00,000T01:30:00,18-Oct-10,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-291T20:00:00,000T02:00:00,18-Oct-10,ISS,Prime,Titan,SFAD,,Scientist for a Day,Images of mutual event. Dione passes near Titan then is eclipsed by Saturn before Titan is then eclipsed by saturn.,,,,,, 2010-291T22:00:00,000T12:00:00,18-Oct-10,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Far-IR map,Measure temperatures at 15 cm-1 Either hemisphere,,,,,, 2010-292T12:33:00,000T09:00:00,19-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-292T14:33:00,000T07:00:00,19-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10292_SP,rider,,,,,, 2010-292T21:33:00,001T19:45:00,19-Oct-10,CDA,Prime,DustRAM direction,ISD0020,,CDA ISD 2010-301T18:21:00,ISD observation around apoapse 2010-301T18:21:00 49.167032 Rs,,,,,, 2010-294T18:48:00,000T09:00:00,21-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-294T19:48:00,000T08:00:00,21-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10294_SP,rider,,,,,, 2010-295T03:48:00,003T10:00:00,22-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-295T05:00:00,000T01:00:00,22-Oct-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 13","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-295T06:00:00,001T04:30:00,22-Oct-10,CIRS,Prime,Saturn,MIRTMAP,,CIRS_139SA_MIRTMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2010-295T06:00:00,001T04:30:00,22-Oct-10,ISS,Non-SPASS,Saturn,MIRTMAP,,Scientist for a Day,Saturn Atmosphere Movie,,,,,, 2010-296T12:33:00,000T04:30:00,23-Oct-10,ISS,Prime,Other,HYRPHA,,Hyrrokkin,Observation of irregular moon of Saturn.,,,,,, 2010-296T18:33:00,000T09:00:00,23-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-296T19:33:00,000T08:00:00,23-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10296_SP,rider,,,,,, 2010-297T06:00:00,000T08:00:00,24-Oct-10,CIRS,Prime,Other,ECSTAROBS,,Mid-IR Stellar Spectroscopy of Eta Carinae,"Spectroscopic observations of IR star Eta Carinae. Slew to star at (161.262, -59.686); execute small box scan, integrating at each position; return to waypoint. Observation duration 8 hours. Request 4 NAC SI of star field (timing TBD). SI exposure information: Spectral class=A, V magnitude=8.0",,,,,, 2010-297T06:00:00,000T08:00:00,24-Oct-10,CIRS,SPASS Rider,Other,ECSTAROBS,,CIRS_139OT Eta Carinae SI,"4 Clear NAC Support Images at: 2010-297T06:50:00, 2010-297T08:35:00, 2010-297T10:20, 2010-297T12:00:00. Exposure information: Spectral class=A, V magnitude=8.0.",,,,,, 2010-297T14:00:00,000T08:00:00,24-Oct-10,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_136_SCATTERED_SUNLIGHT_TEST_PRIME,"Monitor scattered IR solar radiation as a function of offset angle from the sun using radial scans. CIRS to operate at 15.5 cm-1 resolution (4.825 sec/frame, 39 RTI), detector pairs, FP4. FPB scans will begin TBD degrees from Sun, and will scan to 12 degrees of Sun at TBD rate; Scan will stop every 10 degrees for TBD seconds; (the procedure will be repeated in the reverse direction back to the initial position;) to determine whether scattering is asymmetric with respect to the FPB axis, additional scans will be made. . . . . REDESIGN NEEDED HERE . . . 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from TBD degrees +Z to 12 degrees +Z and back to 40 degrees +Z. 2) From TBD degrees in -X on the X axis, to 12 degrees on the -X axis, to TBD degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 12 degrees -Z and back to TBD degrees -Z. ACTUALLY: IN, UP, DOWN, DOWN, UP, BACK WILL DO: || || || || || || || ||||| ||||||||||||||||| * ||||| || || || || || || ||",,,,,, 2010-298T04:48:00,000T09:00:00,25-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-298T05:48:00,000T08:00:00,25-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10298_SP,rider,,,,,, 2010-298T13:48:00,001T13:15:00,25-Oct-10,VIMS,Prime,Star,TRANSIT,,Transit,"Occultation mode, tau_IR = 1 second",,,,,, 2010-298T13:49:00,001T23:44:00,25-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-298T13:49:00,003T04:32:00,25-Oct-10,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-298T13:49:00,003T04:32:00,25-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-300T00:00:00,000T01:08:00,27-Oct-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-300T05:33:00,000T08:00:00,27-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_139IC_DSCAL10300_SP,rider,,,,,, 2010-300T13:33:00,000T08:00:00,27-Oct-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-300T21:33:00,001T05:30:00,27-Oct-10,CDA,Prime,DustRAM direction,ISD0020,,CDA ISD,ISD observation around apoapse 2010-301T18:21:00 49.167032 Rs,,,,,, 2010-300T21:33:00,001T16:00:00,27-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-301T18:05:53,000T00:00:01,28-Oct-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 24.0 d, inc = 3.0 deg, r = 49.120 Rs, phase = 100 deg",,,,,, 2010-301T18:21:00,011T01:00:00,28-Oct-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.006526 Rs exit= 13.097546 Range altitude= 11229.343 km ... -40000.425,,,,,, 2010-301T18:21:00,000T02:00:00,28-Oct-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-301T18:21:00,013T01:58:00,28-Oct-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-301T18:21:00,000T19:12:00,28-Oct-10,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-301T18:21:00,009T18:43:00,28-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-301T20:21:00,009T16:43:00,28-Oct-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-302T03:03:00,000T11:27:00,29-Oct-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-302T04:33:00,000T09:00:00,29-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-302T05:33:00,000T08:00:00,29-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10302_SP,rider,,,,,, 2010-302T13:33:00,006T13:30:00,29-Oct-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-302T13:33:00,006T13:30:00,29-Oct-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-302T14:30:00,000T01:30:00,29-Oct-10,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 88.3 requested range 1.8 Mkm",,,,,, 2010-302T14:30:00,000T01:30:00,29-Oct-10,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-302T14:30:00,000T01:30:00,29-Oct-10,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 88 deg, range = 1.8 Mkm.",,,,,, 2010-302T16:00:00,000T01:00:00,29-Oct-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-302T17:48:00,000T16:20:00,29-Oct-10,ISS,Prime,Other,KARROT,,Kari,Observation of irregular moon of Saturn.,,,,,, 2010-302T17:48:00,000T16:20:00,29-Oct-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-303T10:08:00,000T16:40:00,30-Oct-10,ISS,Prime,Other,BERROT,,Bergelmir,Observation of irregular moon of Saturn.,,,,,, 2010-303T10:08:00,000T16:40:00,30-Oct-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-304T02:18:00,000T11:00:00,31-Oct-10,RSS,SPASS Rider,Earth,PIM,Periodic Instrument maintenance,RSS Ka-TWTA Maintenance,"Ka-TWTA maintenance; Pointing = n/a; Normally, no DSN tracking required during PIMs, but this PIM will also be prep for the Rev141 RSS Enceladus gravity observation (E12) on DOY DOY 334. SP requested tracking over DSS-65. RSS needs DSS-55 (or DSS-54, but slight preference for DSS-55). Can SP switch to DSS-55 so that the downlink and RSS will be over one pass?",,,,,, 2010-304T04:18:00,000T09:00:00,31-Oct-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-304T05:18:00,000T08:00:00,31-Oct-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10304_SP,rider,,,,,, 2010-304T13:18:00,001T04:45:00,31-Oct-10,CDA,Prime,DustRAM direction,ISD0020,,CDA ISD,ISD observation around apoapse 2010-301T18:21:00 49.167032 Rs,,,,,, 2010-305T19:03:00,000T08:00:00,1-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10305_SP,rider,,,,,, 2010-306T18:03:00,000T09:00:00,2-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-306T19:03:00,000T08:00:00,2-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10306_SP,rider,,,,,, 2010-307T18:03:00,000T09:00:00,3-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-307T19:03:00,000T08:00:00,3-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10307_SP,rider,,,,,, 2010-308T18:03:00,000T09:00:00,4-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-308T19:03:00,000T08:00:00,4-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10308_SP,rider,,,,,, 2010-309T03:03:00,000T10:31:00,5-Nov-10,CDA,Prime,DustRAM direction,ISD0020,,CDA ISD 2010-301T18:21:00,ISD observation around apoapse 2010-301T18:21:00 49.167032 Rs,,,,,, 2010-309T03:03:00,002T10:01:00,5-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-309T03:03:00,002T10:01:00,5-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-309T13:34:00,000T13:00:00,5-Nov-10,ISS,Prime,rings(general),PHOEBEHOL,,Observation of Saturn's shadow on the Phoebe ring,Stare at edge of Saturn's Shadow on the Phoebe Ring,,,,,, 2010-309T13:34:00,000T13:00:00,5-Nov-10,CIRS,SPASS Rider,rings(general),PHOEBEHOL,,,null,,,,,, 2010-310T03:03:00,002T09:46:00,6-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-310T04:04:00,000T09:00:00,6-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-310T05:04:00,000T08:00:00,6-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10310_SP,rider,,,,,, 2010-310T13:45:00,000T12:15:00,6-Nov-10,ISS,Prime,rings(general),HPLELR,,Faint Ring High Phase Observation,Observation of faint rings at low elevation angles and high phase,,,,,, 2010-310T13:45:00,000T12:15:00,6-Nov-10,CIRS,SPASS Rider,rings(general),HRLELR,,,null,,,,,, 2010-310T13:45:00,000T12:15:00,6-Nov-10,VIMS,SPASS Rider,rings(general),HPLELR,,Rings high phase observation,ISS rider - 1000 msec integration time,,,,,, 2010-311T04:04:00,000T09:00:00,7-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-311T05:04:00,000T08:00:00,7-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10311_SP,rider,,,,,, 2010-311T13:04:00,003T07:15:00,7-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-311T13:04:00,000T10:38:00,7-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-311T13:04:00,002T03:11:00,7-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-311T13:04:00,000T23:45:00,7-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-311T13:44:00,000T13:25:00,7-Nov-10,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map,"3x3 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-311T13:44:00,000T13:25:00,7-Nov-10,ISS,Non-SPASS,Saturn,REGMAP,Regional mapping,Night NAC lightning search,Rider on VIMS to search for lightning at the night side with NAC,,,,,, 2010-311T23:42:00,000T02:00:00,7-Nov-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-312T01:42:00,000T11:07:00,8-Nov-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-312T03:49:00,000T09:00:00,8-Nov-10,CAPS,Non-SPASS,Saturn,BURST4K,4 kbps burst,Burst of 4kbps data,Burst of 4kbps data,,,,,, 2010-312T03:49:00,000T09:00:00,8-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-312T04:49:00,000T08:00:00,8-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10312_SP,rider,,,,,, 2010-312T12:49:00,000T02:09:16,8-Nov-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-312T12:49:00,000T01:35:00,8-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-312T13:29:00,000T03:40:00,8-Nov-10,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map,"3x3 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-312T13:29:00,000T03:40:00,8-Nov-10,ISS,Non-SPASS,Saturn,REGMAP,Regional mapping,Night NAC lightning search,Rider on VIMS to search for lightning at the night side with NAC,,,,,, 2010-312T14:24:00,002T05:55:00,8-Nov-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-312T14:58:16,000T11:50:44,8-Nov-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-312T17:49:00,000T09:00:00,8-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-312T19:21:00,002T00:10:00,8-Nov-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.084237 Rs exit= 13.994108 Range altitude= -39952.663 km ... 10972.274,,,,,, 2010-313T02:49:00,000T11:09:16,9-Nov-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-313T03:29:00,000T04:26:00,9-Nov-10,ISS,Prime,Saturn,LIMBSCAN,Limb scan,Saturn Limb Scan,Sun behind Saturn limb,,,,,, 2010-313T09:00:00,000T03:00:00,9-Nov-10,CIRS,Prime,Dione,FP3SECLX,,CIRS Dione Observations,"3 NAC Support Images; timing: 2010-313T10:22:00, 2010-313T10:58:00, 2010-313T11:25:00 Observe Dione eclipse exit: 2010-313 (Nov. 09) Entry: T08:24:17, AD=08.3, Phase=118, S/C (-7, 113); LT=4.1 Begin: T09:00:00, AD=09.2, Phase=110, S/C (-7, 108); LT=4.7 Exit: T10:17:53, AD=10.9, Phase=087, S/C (-7, 092); LT=6.2 C/A: T10:56:18, AD=11.2, Phase=074, S/C (-6, 082); LT=7.1 End: T12:00:00, AD=10.5, Phase=067, S/C (-4, 067); LT=8.6 A rough design outline (not yet run through PDT) is: 09:00-09:10 Turn from waypoint. 09:10-10:00 FP3 map of dark/eclipsed disk (four 11 mrad scans at 16 urad/sec). 10:00-10:03 A 1-minute FP1 baseline stare at each of (0, 123) and (0, 63). 10:03-11:05 FP3 pre-exit/exit stare at (0, 50). [SI#1, SI#2] 11:05-11:20 FUV N-S scan of illuminated disk (11 mrad at 12 urad/sec). 11:20-11:30? ISS 2x2 mosaic of disk (<2 min dwells). 11:30?-11:40 FP3 final stare at (0,50). [SI#3] 11:40-11:45 A 1-minute FP1 baseline stare at each of (0, 63) and (0, 50). 11:45-12:00 Return to waypoint.",,,,,, 2010-313T09:00:00,000T03:00:00,9-Nov-10,CIRS,SPASS Rider,Dione,FP3SECLX,,CIRS_140DI_FP3SECLX001 eclipse support images,"Eclipse exit: T10:17:53, AD=10.9, Phase=087, S/C (-7, 092); LT=6.2 3 clear NAC SI, at the following UTC: 2010-313T10:22:00, 2010-313T10:58:00, and 2010-313T11:25:00.",,,,,, 2010-313T09:00:00,000T03:00:00,9-Nov-10,ISS,SPASS Rider,Dione,FP3SECLX,,Dione eclipse exit,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-313T09:00:00,000T03:00:00,9-Nov-10,UVIS,SPASS Rider,Dione,ICYECL,,ICYECL: Icy satellite eclipse volatile activity,Integrate on satellite to observe any post-eclipse brightening that may be associated with volatile activity. Begin when satellite is in eclipse to get background.,,,,,, 2010-313T09:00:00,000T03:00:00,9-Nov-10,VIMS,SPASS Rider,Dione,FP3SECLX,,Dione composition,follow cirs,,,,,, 2010-313T12:00:00,000T02:45:00,9-Nov-10,VIMS,Prime,Saturn,ALPCETOCC,,alpCet Saturn occultation,"alpCet atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Secondary axis for CIRS. Latitude 75N. Ingress/egress.",,,,,, 2010-313T12:00:00,000T02:45:00,9-Nov-10,CIRS,SPASS Rider,Saturn,ALPCETOCC,,CIRS_140SA_ALPCETOCC001_VIMS,Collaborative with VIMS. Stellar Occ Saturn 75N ingress T12:37 CIRS arrays off north limb for duration of occultation permits 30 minute integration on limb to get helium abundance egress at T13:05,,,,,, 2010-313T12:00:00,000T02:45:00,9-Nov-10,ISS,SPASS Rider,Saturn,ALPCETOCC,,Stellar Occultation by Saturn NAC Rider,NAC high resolution limb images during star occ,,,,,, 2010-313T13:58:00,000T02:00:00,9-Nov-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-313T13:58:16,000T00:30:00,9-Nov-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-313T14:00:00,000T02:00:00,9-Nov-10,CDA,SPASS Rider,DustRAM direction,RPX0010,,CDA RPXing 2010-313T15:00:00,RPXing at 4.6662753 Rs,,,,,, 2010-313T14:28:16,000T01:30:00,9-Nov-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-313T15:00:00,000T04:00:00,9-Nov-10,CIRS,Prime,Enceladus,ENCELADUS,Enceladus,Enceladus Thermal Mapping,"Notes from 2010/03/05 SOST meeting. Phase angle gets down to 1.5 degrees at 18:47, near the end. Mosaic at higher phase angle, sit on one spot near the end. Specific plan, 10/04/16: 15:00 Start turn from waypoint 15:15 2x2 NAC mosaic, 2 minute dwells 15:30 FP1 raster scan 15:40 N/S 6 murad/sec FP3/FP4 scan 16:20 2x2 NAC mosaic, 2 minute dwells 16:35 FP1 raster scan 16:50 N/S 6 murad/sec FP3/FP4 scan 17:30 N/S 6 murad/sec FP3/FP4 scan 18:10 Stare at disk center. 18:45 Start turn back to waypoint",,,,,, 2010-313T15:00:00,000T04:00:00,9-Nov-10,ISS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,CIRS prime Encladus observation (PIE),ISS rider on CIRS prime,,,,,, 2010-313T15:00:00,000T04:00:00,9-Nov-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2010-313T15:00:00,000T04:00:00,9-Nov-10,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Dione composition,follow cirs,,,,,, 2010-313T15:58:16,000T23:00:00,9-Nov-10,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2010-313T16:15:00,000T04:10:00,9-Nov-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-313T18:16:29,000T00:00:01,9-Nov-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.100 Rs, lat = 2 deg, phase = 80 deg",,,,,, 2010-313T19:00:00,000T02:00:00,9-Nov-10,VIMS,Prime,Saturn,HIRESMAP,High resolution map,Hi-Res Map,"Single 3x4 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning). 4 frame lengths east-west by 3 frame lengths north-south.",,,,,, 2010-313T20:25:00,000T23:54:00,9-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-313T21:00:00,000T04:00:00,9-Nov-10,CIRS,Prime,Saturn,LIMBZON,,CIRS_140SA_LIMBZON001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb New obs type: A zonal scan at the equator to monitor the vertical structure of the temperature wave seen by Li et al. Need to sample at least 120 degrees of longitude, so 4 hours of integration needed. 15cm-1 is enough for temperature sounding.",,,,,, 2010-313T21:00:00,000T04:00:00,9-Nov-10,CIRS,SPASS Rider,Saturn,LIMBZON,,support images,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2010-313T21:00:00,000T04:00:00,9-Nov-10,ISS,SPASS Rider,Saturn,LIMBZON,,ISS Rider to CIRS LIMBMAP,Limb images of Saturn,,,,,, 2010-313T21:00:00,000T04:00:00,9-Nov-10,UVIS,Non-SPASS,Saturn,LIMBZON,,Ride along with CIRS LIMBZON of Saturn,EUV and FUV Ride along with CIRS LIMBZON of Saturn,,,,,, 2010-314T01:00:00,000T08:09:00,10-Nov-10,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map,"3x3 Regional map , on hemisphere not vignetted by rings. 10-minute centers (7 mins for science, 3 for repositioning)",,,,,, 2010-314T01:00:00,000T08:09:00,10-Nov-10,ISS,SPASS Rider,Saturn,REGMAP,Regional mapping,Day WAC and probably some night NAC,"Rider on VIMS to monitor day side clouds in WAC every hour, or search for lightning at the night side with NAC",,,,,, 2010-314T11:19:00,000T09:00:00,10-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-314T12:19:00,000T08:00:00,10-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10314_SP,rider,,,,,, 2010-314T14:58:16,000T05:20:44,10-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-314T19:31:00,000T00:48:00,10-Nov-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.007004 Rs exit= 14.008347 Range altitude= 10952.614 km ... -1205.0592,,,,,, 2010-314T20:19:00,000T15:18:01,10-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-314T20:19:00,002T00:45:00,10-Nov-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.007004 Rs exit= 14.008347 Range altitude= 10952.614 km ... -1205.0592,,,,,, 2010-314T20:19:00,000T05:18:01,10-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-314T20:19:00,000T15:18:01,10-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-314T20:19:00,000T19:18:01,10-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-314T20:19:00,000T01:50:00,10-Nov-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-314T21:14:00,000T03:23:01,10-Nov-10,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2010-314T21:14:00,000T03:23:01,10-Nov-10,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-314T21:14:00,000T03:23:01,10-Nov-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 146 deg. SSC Lat/Lon = 1.041N/3.38 deg, SS Lat/Lon = 6.913N/216.138 deg. Alt = 327280.66 km, range = 329855.66 km Resolution = 164 km/px. Obtain cubes while scanning across Titan. Template M4.",,,,,, 2010-314T22:09:00,001T22:55:00,10-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-315T00:37:01,000T04:00:00,11-Nov-10,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2010-315T00:37:01,000T04:00:00,11-Nov-10,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T00:37:01,000T04:00:00,11-Nov-10,UVIS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2010-315T00:37:01,000T04:00:00,11-Nov-10,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 147 deg. SSC Lat/Lon = 0.777N/7.296 deg, SS Lat/Lon = 6.915N/219.35 deg. Alt = 255748.98 km, range = 258323.98 km Resolution = 128 km/px. Obtain cubes while scanning across Titan. Template M.",,,,,, 2010-315T01:37:01,000T11:00:00,11-Nov-10,INMS,Non-SPASS,Saturn,T73INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-315T04:37:01,000T04:00:00,11-Nov-10,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2010-315T04:37:01,000T04:00:00,11-Nov-10,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T04:37:01,000T04:00:00,11-Nov-10,UVIS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,UVIS Rider to CIRS MIRLMBMAP,UVIS Rider to CIRS Mid IR Limb observation,,,,,, 2010-315T04:37:01,000T04:00:00,11-Nov-10,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan Limb Scan.,"VIMS ridealong with CIRS while limb scanning. Phase = 148 deg. SSC Lat/Lon = 0.181N/12.243 deg, SS Lat/Lon = 6.917N/223.11 deg. Alt = 174776.8 km, range = 177351.8 km Resolution = 87 km/px. Obtain cubes while scanning across Titan's limb. Template R.",,,,,, 2010-315T08:37:01,000T02:45:00,11-Nov-10,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2010-315T08:37:01,000T02:45:00,11-Nov-10,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T08:37:01,000T02:45:00,11-Nov-10,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan Scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 151 deg. SSC Lat/Lon = 01.394S/18.597 deg, SS Lat/Lon = 6.919N/226.87 deg. Alt = 95627.77 km, range = 98200.77 km Resolution = 48 km/px. Obtain cubes while scanning across Titan. Template T.",,,,,, 2010-315T11:22:01,000T01:50:00,11-Nov-10,CAPS,Prime,Titan,T73INPTG,,Titan Encounter,null,,,,,, 2010-315T11:22:01,000T01:50:00,11-Nov-10,CIRS,SPASS Rider,Titan,T73INPTG,,,Ride along with UVIS.,,,,,, 2010-315T11:37:01,000T01:00:00,11-Nov-10,CAPS,SPASS Rider,Titan,T73INBND,,Inbound 140TI (T73),Inbound 117TI (T61),,,,,, 2010-315T11:37:01,000T01:00:00,11-Nov-10,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-315T11:37:01,000T04:00:00,11-Nov-10,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T73 flyby,"T73 is a pre-dusk, high altitude (>4000 km) ?blind? flyby over the south pole of Titan that will be useful to characterize the background field in which Titan sits in. We assign grade two priority. Data rate: 988bps (16vps).",,,,,, 2010-315T11:37:01,000T01:00:00,11-Nov-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-315T12:37:01,000T02:00:00,11-Nov-10,CAPS,SPASS Rider,Titan,T73CLOSE,,Closest Approach 140TI (T73),Closest Approach 117TI (T61),,,,,, 2010-315T12:37:01,000T02:00:00,11-Nov-10,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-315T12:37:01,000T02:00:00,11-Nov-10,INMS,Non-SPASS,Titan,TITAN73,,Titan Flyby,Titan observation,,,,,, 2010-315T12:37:01,000T02:00:00,11-Nov-10,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2010-315T13:12:01,000T01:10:00,11-Nov-10,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2010-315T13:12:01,000T01:10:00,11-Nov-10,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T13:12:01,000T02:40:00,11-Nov-10,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,"VIMS ridealong with CIRS during C/A for regional mapping of Titan. Phase = 154 deg. SSC Lat/Lon = 26.024S/69.435 deg, SS Lat/Lon = 6.921N/231.178 deg. Alt = 10402.619 km, range = 12977.619 km Resolution = 5.2 km/px. Obtain cubes for regional mapping of Titan during C/A.",,,,,, 2010-315T13:12:01,000T01:10:00,11-Nov-10,UVIS,Non-SPASS,Titan,FIRLMBT,Far Infrared limb tracking,Rider to CIRS,Rider to CIRS.,,,,,, 2010-315T14:22:01,000T00:30:00,11-Nov-10,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2010-315T14:22:01,000T00:30:00,11-Nov-10,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T14:37:01,000T01:00:00,11-Nov-10,CAPS,SPASS Rider,Titan,T73OUTBND,,Outbound 140TI (T73),Outbound 117TI (T61),,,,,, 2010-315T14:37:01,000T01:00:00,11-Nov-10,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2010-315T14:37:01,000T11:00:00,11-Nov-10,INMS,Non-SPASS,Saturn,T73OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-315T14:37:01,000T01:00:00,11-Nov-10,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2010-315T14:52:01,000T01:00:00,11-Nov-10,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2010-315T14:52:01,000T01:00:00,11-Nov-10,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T14:52:01,000T01:00:00,11-Nov-10,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2010-315T15:37:01,001T05:27:00,11-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-315T15:37:01,001T05:26:59,11-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-315T15:37:01,001T05:26:59,11-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-315T15:52:01,000T02:45:00,11-Nov-10,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping.,Regional mapping of Titan. Phase = 45 deg. SSC Lat/Lon = 7.821S/191.14 deg. SS Lat/Lon = 6.923N/233.684 deg. Alt = 44255.5 km range = 46830.5 km. Resolution = 22 km/px. Obtain mosaics for regional mapping of Titan. Template Y.,,,,,, 2010-315T15:52:01,000T02:45:00,11-Nov-10,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with UVIS.,,,,,, 2010-315T15:52:01,000T02:45:00,11-Nov-10,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T18:37:01,000T04:00:00,11-Nov-10,VIMS,Prime,Titan,MEDRES,Medium resolution global mapping,Regional mapping.,Regional mapping of Titan at medium resolution with 2x2 mosaic. Phase = 38 deg. SSC Lat/Lon = 3.868S/199.879 deg. SS Lat/Lon = 6.924N/236.269 deg. Alt = 97810.0 km range = 100385.0 km. Resolution = 49 km/px. Obtain mosaics for regional mapping of Titan. Template I.,,,,,, 2010-315T18:37:01,000T04:00:00,11-Nov-10,CIRS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,,Ride along with UVIS.,,,,,, 2010-315T18:37:01,000T04:00:00,11-Nov-10,ISS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-315T22:37:01,000T05:00:00,11-Nov-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping.,Global mapping of Titan. Phase = 35 deg. SSC Lat/Lon = 2.339S/205.827 deg. SS Lat/Lon = 6.926N/240.028 deg. Alt = 176796.8 km range = 179371.8 km. Resolution = 88 km/px. Obtain cubes of various exposure times for global mapping of Titan. Template V.,,,,,, 2010-315T22:37:01,000T05:00:00,11-Nov-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with UVIS.,,,,,, 2010-315T22:37:01,000T05:00:00,11-Nov-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-316T01:37:01,000T19:26:59,12-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-316T03:37:01,000T04:31:59,12-Nov-10,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping.,Global mapping of Titan. Phase = 34 deg. SSC Lat/Lon = 1.635S/211.264 deg. SS Lat/Lon = 6.929N/244.727 deg. Alt = 276794.5 km range = 279369.5 km. Resolution = 138 km/px. Obtain cubes of exposure times for global mapping of Titan. Template B.,,,,,, 2010-316T03:37:01,000T04:32:00,12-Nov-10,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with UVIS.,,,,,, 2010-316T03:37:01,000T04:31:59,12-Nov-10,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-316T10:34:00,000T10:30:00,12-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-316T11:34:00,000T09:30:00,12-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10316_SP,rider,,,,,, 2010-316T21:04:00,011T22:31:00,12-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-316T21:04:00,007T04:52:00,12-Nov-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.007004 Rs exit= 14.008347 Range altitude= 10952.614 km ... -1205.0592,,,,,, 2010-316T21:04:00,002T05:15:00,12-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-316T21:04:00,001T12:36:00,12-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-316T21:04:00,007T04:53:00,12-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-316T21:04:00,000T14:00:00,12-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-316T22:00:00,000T08:00:00,12-Nov-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-316T22:00:00,000T08:00:00,12-Nov-10,ISS,SPASS Rider,Titan,COMPMAP,Composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-316T22:00:00,000T08:00:00,12-Nov-10,VIMS,SPASS Rider,Titan,COMPMAP,Composition map,XD - Titan Monitoring Campaign,"range is 660,000 to 833,000 km - phase is 35",,,,,, 2010-317T00:00:00,000T01:08:00,13-Nov-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-317T04:00:00,000T03:00:00,13-Nov-10,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-317T07:00:00,000T02:00:00,13-Nov-10,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2010-317T11:04:00,006T14:53:00,13-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-317T11:04:00,000T09:00:00,13-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-317T12:04:00,000T08:00:00,13-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10317_SP,rider,,,,,, 2010-317T20:40:00,000T06:30:00,13-Nov-10,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 39.1 requested range 1.1 Mkm",,,,,, 2010-317T20:40:00,000T06:30:00,13-Nov-10,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-317T20:40:00,000T06:30:00,13-Nov-10,VIMS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 39 deg, range = 1.1 Mkm.",,,,,, 2010-318T03:10:00,000T01:00:00,14-Nov-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-318T04:10:00,000T05:30:00,14-Nov-10,ISS,Prime,Other,RHEAL4,,Rhea L4 satellite search,Satellite search around Rhea L4 Lagrange point.,,,,,, 2010-318T09:40:00,000T07:00:00,14-Nov-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-318T16:40:00,010T02:55:00,14-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-318T17:19:00,000T09:00:00,14-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-318T18:19:00,000T08:00:00,14-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10318_SP,rider,,,,,, 2010-319T02:19:00,000T07:00:00,15-Nov-10,ISS,Prime,Other,TARRES,,Tarvos,Observation of irregular moon of Saturn.,,,,,, 2010-319T02:19:00,000T07:00:00,15-Nov-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-319T02:19:00,001T00:00:00,15-Nov-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-319T09:19:00,000T08:00:00,15-Nov-10,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2010-319T17:19:00,000T09:00:00,15-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-319T18:19:00,000T08:00:00,15-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10319_SP,rider,,,,,, 2010-320T02:19:00,003T23:38:00,16-Nov-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-320T03:00:00,000T04:00:00,16-Nov-10,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2010-320T03:00:00,000T04:00:00,16-Nov-10,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2010-320T07:00:00,001T08:00:00,16-Nov-10,UVIS,Prime,Saturn,MOS140APO,,,"System scan of Saturn magnetosphere hydrogen, day 1. Allowances of 30 minutes for turn to waypoint at end of observation and 20 minutes observation margin at each end of the observation have been included . EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. 0) Start at WAYPOINT (Saturn center). 1) Align slit with Saturn spin axis. 2) Start data capture, stare 133.0 s, stop data capture. 3) Repeat PATTERN-A 67 times. 4) Slew -0.064 rad about the x-axis. 5) Start data capture, stare 133.0 s, stop data capture. 6) Repeat PATTERN-B 134 times. 7) Slew -0.064 rad about the x-axis. 8) Start data capture, stare 133.0 s, stop data capture. 9) Repeat PATTERN-A 134 times. 10) Repeat steps 4 through 9 11) Turn back to WAYPOINT PATTERN-A: Slew -1.5 mrad about z-axis. Start data capture, stare 133.0 s, stop data capture. PATTERN-B: Slew +1.5 mrad about z-axis. Start data capture, stare 133.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9103.82341 bps, from Alain Jouchoux's spreadsheet)x(333.0s per stare)x(608stares) = 736.172x10^6 bits.",,,,,, 2010-321T17:19:00,000T09:00:00,17-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-321T18:19:00,000T08:00:00,17-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10321_SP,rider,,,,,, 2010-322T06:30:00,000T01:00:00,18-Nov-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-322T09:00:00,000T16:00:00,18-Nov-10,UVIS,Prime,Saturn,MOS140APO,,,,,,,,, 2010-323T03:20:00,000T09:00:00,19-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-323T04:20:00,000T08:00:00,19-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_140IC_DSCAL10323_SP,rider,,,,,, 2010-323T16:30:00,000T16:00:00,19-Nov-10,UVIS,Prime,Saturn,MOS140APO,,,"System scan of Saturn magnetosphere hydrogen, day 3. Allowances of 30 minutes for turn to waypoint at end of observation and 20 minutes observation margin at each end of the observation have been included . EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. 0) Start at WAYPOINT (Saturn center). 1) Align slit with Saturn spin axis. 2) Go to where the system scan ended on day 2 by slewing +128 mrad about the x-axis and +64.5 mrad about the z-axis. 2) Start data capture, stare 128.0 s, stop data capture. 3) Repeat PATTERN-A 24 times. 4) Slew +0.064 rad about the x-axis. 5) Start data capture, stare 128.0 s, stop data capture. 6) Repeat PATTERN-B 134 times. 7) Slew +0.064 rad about the x-axis. 8) Start data capture, stare 128.0 s, stop data capture. 9) Repeat PATTERN-A 134 times. 10) Turn back to WAYPOINT. PATTERN-A: Slew +1.5 mrad about z-axis. Start data capture, stare 128.0 s, stop data capture. PATTERN-B: Slew -1.5 mrad about z-axis. Start data capture, stare 128.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (9459.44151 bps, from Alain Jouchoux's spreadsheet)x(128.0s per stare)x(295 stares) = 357.189x10^6 bits.",,,,,, 2010-324T01:56:00,004T17:39:00,20-Nov-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S65,Range enter= 14.007004 Rs exit= 14.008347 Range altitude= 10952.614 km ... -1205.0592,,,,,, 2010-324T01:56:53,000T00:00:01,20-Nov-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.6 d, inc = 0.0 deg, r = 44.521 Rs, phase = 95 deg",,,,,, 2010-324T01:57:00,000T02:00:00,20-Nov-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-324T01:57:00,004T17:38:00,20-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-324T01:57:00,004T17:38:00,20-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-324T03:57:00,001T22:08:00,20-Nov-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-324T08:30:00,000T12:00:00,20-Nov-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-324T10:50:00,000T09:00:00,20-Nov-10,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev141 Enceladus gravity observation on 2010/334 (E12). Can SP switch from DSS-15 to DSS-25 so that downlink and RSS can be over one Goldstone pass?",,,,,, 2010-324T10:50:00,000T09:00:00,20-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-324T11:50:00,000T08:00:00,20-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10324_SP,rider,,,,,, 2010-324T20:30:00,000T01:00:00,20-Nov-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-324T21:30:00,000T16:30:00,20-Nov-10,ISS,Prime,RingE,ERNGVERT,,Edge-on obs E-ring observation after Equinox.,Low elevation observation of E ring at moderate phase.,,,,,, 2010-324T21:30:00,000T16:30:00,20-Nov-10,CIRS,SPASS Rider,rings(general),ERNGVERT,,,null,,,,,, 2010-324T21:30:00,000T16:30:00,20-Nov-10,VIMS,SPASS Rider,RingE,ERNGVERT,,E ring observation,ISS rider - 1000 msec integration time,,,,,, 2010-325T11:00:00,000T03:00:00,21-Nov-10,RADAR,Non-SPASS,Other,WU4ENGTST,RADAR engineering test warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2010-325T11:01:20,000T00:00:01,21-Nov-10,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2010-325T14:00:00,000T02:00:00,21-Nov-10,RADAR,Prime,Saturn,ENGTEST,Engineering test,Engineering Test of Diagnostic Modes,Engineering test of diagnostic modes on the flight unit.,,,,,, 2010-325T17:05:00,000T09:00:00,21-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-325T18:05:00,000T08:00:00,21-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10325_SP,rider,,,,,, 2010-326T02:05:00,000T23:45:00,22-Nov-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-326T03:00:00,000T01:00:00,22-Nov-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-326T04:00:00,000T12:00:00,22-Nov-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_141SA_COMPSIT003,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-326T16:50:00,000T09:00:00,22-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-326T17:50:00,000T08:00:00,22-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10326_SP,rider,,,,,, 2010-327T01:50:00,000T03:00:00,23-Nov-10,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2010-327T01:50:00,001T17:45:00,23-Nov-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-327T04:50:00,001T04:15:00,23-Nov-10,CDA,Prime,DustRAM direction,ISD0021,,CDA ISD,ISD observation around apoapse 2010-324T01:56:00 44.566453 Rs,,,,,, 2010-328T10:35:00,000T09:00:00,24-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-328T11:35:00,000T08:00:00,24-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10328_SP,rider,,,,,, 2010-328T19:35:00,002T23:45:00,24-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-328T19:35:00,004T13:06:00,24-Nov-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S65,Range enter= 14.007004 Rs exit= 14.008347 Range altitude= 10952.614 km ... -1205.0592,,,,,, 2010-328T19:35:00,000T00:43:00,24-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-328T19:35:00,002T23:45:00,24-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-328T19:35:00,004T16:01:00,24-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-328T19:35:00,002T23:45:00,24-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-328T19:40:00,000T00:02:00,24-Nov-10,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S65 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2010-328T19:41:00,000T13:09:00,24-Nov-10,CDA,Prime,DustRAM direction,ISD0021,,CDA ISD,ISD observation around apoapse 2010-324T01:56:00 44.566453 Rs,,,,,, 2010-328T20:18:00,000T00:07:00,24-Nov-10,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-328T20:25:00,000T00:05:00,24-Nov-10,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-328T20:30:00,000T00:33:00,24-Nov-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2010-328T21:03:00,000T00:30:00,24-Nov-10,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2010-328T21:33:00,002T11:27:00,24-Nov-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-329T10:20:00,000T09:00:00,25-Nov-10,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev141 Enceladus gravity observation on 2010/334 (E12).",,,,,, 2010-329T10:20:00,000T09:00:00,25-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-329T11:20:00,000T08:00:00,25-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10329_SP,rider,,,,,, 2010-329T19:20:00,000T13:30:00,25-Nov-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2010-330T00:00:00,000T01:08:00,26-Nov-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-330T10:20:00,000T09:00:00,26-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-330T11:20:00,000T08:00:00,26-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10330_SP,rider,,,,,, 2010-330T20:30:00,000T01:30:00,26-Nov-10,ISS,Prime,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 153.2 requested range 2 Mkm",,,,,, 2010-330T20:30:00,000T01:30:00,26-Nov-10,CIRS,SPASS Rider,Titan,M180R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-330T20:30:00,000T01:30:00,26-Nov-10,VIMS,SPASS Rider,Titan,M180R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 153 deg, range = 2 Mkm.",,,,,, 2010-330T22:30:00,000T11:00:00,26-Nov-10,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Stares at a fixed location on the auroral oval.,,,,,, 2010-330T22:30:00,000T11:00:00,26-Nov-10,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,null,,,,,, 2010-330T22:30:00,000T11:00:00,26-Nov-10,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC aurora stare,CL1 NAC 4x4 images. 10 Mbits/hr,,,,,, 2010-330T22:30:00,000T11:00:00,26-Nov-10,VIMS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Auroral Stare,Auroral Stare ridealong with UVIS,,,,,, 2010-331T09:00:00,000T00:34:00,27-Nov-10,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2010-331T09:34:00,000T09:46:00,27-Nov-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-331T10:20:00,000T09:00:00,27-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-331T11:20:00,000T08:00:00,27-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10331_SP,rider,,,,,, 2010-331T19:20:00,000T15:01:00,27-Nov-10,ISS,Prime,Hyperion,FLYBY,,Hyperion flyby,"ORS observation during 140,000 - 160,000 km flyby of Hyperion.",,,,,, 2010-331T19:20:00,000T15:01:00,27-Nov-10,CIRS,SPASS Rider,Hyperion,FLYBY,,Hyperion Flyby,null,,,,,, 2010-331T19:20:00,000T15:01:00,27-Nov-10,UVIS,SPASS Rider,Hyperion,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-331T19:20:00,000T15:01:00,27-Nov-10,VIMS,SPASS Rider,Hyperion,FLYBY,,,null,,,,,, 2010-331T19:20:00,002T15:33:59,27-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-331T19:20:00,001T00:01:00,27-Nov-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-331T19:20:00,002T10:45:00,27-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-331T19:20:00,001T10:44:00,27-Nov-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-332T10:21:00,000T09:00:00,28-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-332T11:21:00,000T08:00:00,28-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10332_SP,rider,,,,,, 2010-332T19:21:00,000T05:05:00,28-Nov-10,ISS,Prime,Hyperion,FLYBY,,Hyperion flyby,"ORS observation during 290,000 - 380,000 km flyby of Hyperion.",,,,,, 2010-332T19:21:00,000T05:05:00,28-Nov-10,CIRS,SPASS Rider,Hyperion,FLYBY,,Hyperion Flyby,null,,,,,, 2010-332T19:21:00,000T05:05:00,28-Nov-10,UVIS,SPASS Rider,Hyperion,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-332T19:21:00,000T05:05:00,28-Nov-10,VIMS,SPASS Rider,Hyperion,FLYBY,,,null,,,,,, 2010-332T19:21:00,000T23:39:00,28-Nov-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-333T02:36:00,000T09:00:00,29-Nov-10,RSS,SPASS Rider,Enceladus,KADOWN,RSS Ka-Band downlink,GSE pass for Enceladus' gravity,Additional downlink pass at Ka-band for Enceladus' gravity science and for improving locally Cassini orbit.,,,,,, 2010-333T02:36:00,000T09:00:00,29-Nov-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-333T03:36:00,000T08:00:00,29-Nov-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10333_SP,rider,,,,,, 2010-333T06:04:00,000T05:32:00,29-Nov-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-333T08:41:00,002T01:44:00,29-Nov-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.995363 Rs exit= 13.990559 Range altitude= -1204.3170 km ... 478.21114,,,,,, 2010-333T11:36:00,000T10:58:00,29-Nov-10,UVIS,Prime,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-333T11:36:00,000T10:58:00,29-Nov-10,CIRS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,Rhea Flyby,null,,,,,, 2010-333T11:36:00,000T10:58:00,29-Nov-10,VIMS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,,null,,,,,, 2010-333T11:36:00,000T23:47:59,29-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-333T11:36:00,002T01:27:00,29-Nov-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-333T19:00:00,000T02:00:00,29-Nov-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-333T21:00:00,000T02:53:59,29-Nov-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-333T22:34:05,000T03:38:55,29-Nov-10,CDA,Prime,Other,RINGSHAD,,CDA Ring Shadow Crossing1_7Rs,CDA Ring Shadow Crossing @ 7Rs; Objective code RC1a,,,,,, 2010-333T23:53:59,000T10:00:00,29-Nov-10,INMS,Non-SPASS,Enceladus,E12INBND,,Enceladus flyby,Enceladus observation,,,,,, 2010-334T01:48:59,000T02:05:00,30-Nov-10,RSS,SPASS Rider,Enceladus,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2010-334T03:53:59,000T03:00:00,30-Nov-10,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus' Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2010-334T06:05:00,000T03:48:59,30-Nov-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-334T06:53:59,000T02:30:00,30-Nov-10,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus,Enceladus plume PIE,,,,,, 2010-334T06:53:59,000T02:30:00,30-Nov-10,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume Observation,null,,,,,, 2010-334T06:53:59,000T02:30:00,30-Nov-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-334T06:53:59,000T02:30:00,30-Nov-10,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2010-334T07:48:00,000T02:00:00,30-Nov-10,CDA,SPASS Rider,DustRAM direction,RPX0020,,CDA RPXing 2010-334T08:48:00,RPXing at 3.6161463 Rs,,,,,, 2010-334T07:48:00,000T02:00:00,30-Nov-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-334T09:23:59,000T01:00:00,30-Nov-10,CIRS,Prime,Enceladus,DRKMAP,,141EN_DRKMAP001,Nightside observations of Enceladus.,,,,,, 2010-334T09:23:59,000T01:00:00,30-Nov-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-334T09:32:59,000T00:00:01,30-Nov-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.567 Rs, lat = 0 deg, phase = 86 deg",,,,,, 2010-334T09:53:59,000T04:00:00,30-Nov-10,INMS,Non-SPASS,Enceladus,ENCEL12,,Enceladus encounter,Enceladus observation,,,,,, 2010-334T09:53:59,000T04:00:00,30-Nov-10,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2010-334T10:23:59,000T03:00:00,30-Nov-10,RSS,Prime,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus' Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2010-334T10:53:59,000T09:00:00,30-Nov-10,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 141EN Campaign,Part of 141EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2010-334T11:06:29,000T01:35:00,30-Nov-10,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2010-334T11:23:59,010T04:51:01,30-Nov-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-334T11:23:59,000T01:00:00,30-Nov-10,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 141,BIT_OVERLAY_300,,,,,, 2010-334T11:51:59,000T00:06:00,30-Nov-10,CIRS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Rider ORS Drag,null,,,,,, 2010-334T11:51:59,000T00:06:00,30-Nov-10,ISS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,Enceladus close approach,ISS rider on RSS flyby; secondary axis optimized for ORS to sweep Enceladus,,,,,, 2010-334T11:51:59,000T00:06:00,30-Nov-10,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-334T13:23:59,000T01:00:00,30-Nov-10,CIRS,Prime,Enceladus,DAYMAP,,141EN_DAYMAP001,Dayside observations of Enceladus.,,,,,, 2010-334T13:23:59,000T01:00:00,30-Nov-10,ISS,SPASS Rider,Enceladus,DAYMAP,,Enceladus post-close approach,ISS rider on CIRS Enceladus observation,,,,,, 2010-334T13:23:59,000T01:00:00,30-Nov-10,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-334T13:23:59,000T01:00:00,30-Nov-10,VIMS,SPASS Rider,Enceladus,DAYMAP,,,null,,,,,, 2010-334T13:53:59,000T10:00:00,30-Nov-10,INMS,Non-SPASS,Enceladus,E12OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2010-334T13:53:59,001T11:27:01,30-Nov-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-334T14:23:59,000T02:30:00,30-Nov-10,VIMS,Prime,Enceladus,ENCELADUS,Enceladus,Enceladus close approach,Enceladus close approach,,,,,, 2010-334T14:23:59,000T02:30:00,30-Nov-10,CIRS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus VIMS rider,null,,,,,, 2010-334T14:23:59,000T02:30:00,30-Nov-10,ISS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus post-close approach,Rider on VIMS Enceladus observation,,,,,, 2010-334T14:23:59,000T02:30:00,30-Nov-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-334T16:53:59,000T03:00:00,30-Nov-10,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus' Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2010-334T19:53:59,001T05:27:01,30-Nov-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-334T19:56:00,000T06:40:00,30-Nov-10,UVIS,Prime,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-334T19:56:00,000T06:40:00,30-Nov-10,CIRS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,Enceladus Thermal Mapping,null,,,,,, 2010-334T19:56:00,000T06:40:00,30-Nov-10,ISS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,Enceladus post-close approach,ISS rider on UVIS Enceladus observation,,,,,, 2010-334T19:56:00,000T06:40:00,30-Nov-10,VIMS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,,null,,,,,, 2010-334T23:53:59,000T11:42:01,30-Nov-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-335T03:36:00,000T08:00:00,1-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10335_SP,rider,,,,,, 2010-335T10:25:00,009T05:50:00,1-Dec-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.003535 Rs exit= 14.000623 Range altitude= 477.97167 km ... -1131.2580,,,,,, 2010-335T11:36:00,000T04:45:00,1-Dec-10,ISS,Prime,Other,RHEAL4,,Rhea L4 satellite search,Satellite search around Rhea L4 Lagrange point.,,,,,, 2010-335T11:36:00,000T13:45:00,1-Dec-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-335T13:03:00,000T12:18:00,1-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-335T16:21:00,000T09:00:00,1-Dec-10,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2010-335T16:21:00,000T09:00:00,1-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-336T01:21:00,017T23:02:00,2-Dec-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-336T01:21:00,000T01:39:00,2-Dec-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-336T01:21:00,000T13:30:00,2-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-336T01:21:00,005T23:46:00,2-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-336T03:00:00,000T02:00:00,2-Dec-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-336T05:00:00,006T20:07:00,2-Dec-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-336T14:51:00,001T00:00:00,2-Dec-10,MAG,Prime,Other,MAPSROLL,,MAPS Offset Rolls,"Offset rolls similar to MAG calrolls. Use in periods where MAPS downlink rolls are removed due to RBOT ""2 out of 3"" rule. Suitable for MAPS science. Unlike MAG calrolls orbital location is not critical. Duration 5hrs or greater preferred (typical roll period approx 53mins). MAG data at survey rate.",,,,,, 2010-337T14:51:00,003T10:15:00,3-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-337T16:21:00,000T09:00:00,3-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-337T17:21:00,000T08:00:00,3-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10337_SP,rider,,,,,, 2010-338T04:00:00,000T01:00:00,4-Dec-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-338T05:00:00,000T12:00:00,4-Dec-10,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_141SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2010-338T05:00:00,000T12:00:00,4-Dec-10,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT ridealong,Compsit ridealong with CIRS,,,,,, 2010-338T17:00:00,000T13:00:00,4-Dec-10,ISS,Prime,RingE,ERNGVERC,,Edge-on obs E-ring observation after Equinox.,Low elevation observation of E ring at moderate phase.,,,,,, 2010-338T17:00:00,000T13:00:00,4-Dec-10,CIRS,SPASS Rider,rings(general),ERNGVERC,,,null,,,,,, 2010-339T09:51:00,000T09:00:00,5-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-339T10:51:00,000T08:00:00,5-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10339_SP,rider,,,,,, 2010-339T19:30:00,000T01:30:00,5-Dec-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 71.6 requested range 3.4 Mkm",,,,,, 2010-339T19:30:00,000T01:30:00,5-Dec-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-339T19:30:00,000T01:30:00,5-Dec-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 72 deg, range = 3.4 Mkm.",,,,,, 2010-339T21:00:00,000T01:00:00,5-Dec-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-339T22:00:00,000T08:30:00,5-Dec-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2010-340T06:30:00,000T01:14:00,6-Dec-10,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Tethys","Images of mutual event, transit of Dione across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2010-340T16:06:00,000T09:00:00,6-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-340T17:06:00,000T08:00:00,6-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10340_SP,rider,,,,,, 2010-341T01:06:00,000T13:31:00,7-Dec-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-341T14:37:00,004T11:23:00,7-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-341T16:07:00,000T09:00:00,7-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-341T17:07:00,000T08:00:00,7-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10341_SP,rider,,,,,, 2010-342T01:07:00,000T15:00:00,8-Dec-10,CDA,Prime,DustRAM direction,ISD0022,,CDA ISD,ISD observation around apoapse 2010-344T16:15:00 44.446001 Rs,,,,,, 2010-342T01:07:00,002T15:08:00,8-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-342T16:07:00,000T09:00:00,8-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-342T17:07:00,000T08:00:00,8-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10342_SP,rider,,,,,, 2010-343T01:07:00,000T14:45:00,9-Dec-10,CDA,Prime,DustRAM direction,ISD0022,,CDA ISD 2010-344T16:15:00,ISD observation around apoapse 2010-344T16:15:00 44.446001 Rs,,,,,, 2010-343T01:07:00,000T23:45:00,9-Dec-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-343T15:52:00,000T09:00:00,9-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-343T16:52:00,000T08:00:00,9-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_141IC_DSCAL10343_SP,rider,,,,,, 2010-344T00:52:00,001T13:30:00,10-Dec-10,CDA,Prime,DustRAM direction,ISD0022,,CDA ISD 2010-344T16:15:00,ISD observation around apoapse 2010-344T16:15:00 44.446001 Rs,,,,,, 2010-344T00:52:00,000T15:23:00,10-Dec-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-344T16:15:00,009T05:42:00,10-Dec-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.003535 Rs exit= 14.000623 Range altitude= 477.97167 km ... -1131.2580,,,,,, 2010-344T16:15:00,000T00:45:00,10-Dec-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-344T16:15:00,009T18:08:00,10-Dec-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-344T16:15:00,000T23:37:00,10-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-344T16:15:03,000T00:00:01,10-Dec-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.6 d, inc = 0.1 deg, r = 44.403 Rs, phase = 94 deg",,,,,, 2010-344T17:00:00,000T02:00:00,10-Dec-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-344T19:00:00,007T05:23:00,10-Dec-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-345T00:00:00,000T01:08:00,11-Dec-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-345T15:52:00,000T09:00:00,11-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-345T15:52:00,000T09:00:00,11-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-345T16:52:00,000T08:00:00,11-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10345_SP,rider,,,,,, 2010-346T00:52:00,007T14:31:00,12-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-346T02:00:00,000T12:00:00,12-Dec-10,MAG,Prime,Other,MAPSROLL,,MAPS Offset Rolls,"Offset rolls similar to MAG calrolls. Use in periods where MAPS downlink rolls are removed due to RBOT ""2 out of 3"" rule. Suitable for MAPS science. Unlike MAG calrolls orbital location is not critical. Duration 5hrs or greater preferred (typical roll period approx 53mins). MAG data at survey rate.",,,,,, 2010-346T14:00:00,000T23:30:00,12-Dec-10,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,"Stare at E or G ring ansa, 1 second integration.",,,,,, 2010-346T14:00:00,000T23:30:00,12-Dec-10,CIRS,SPASS Rider,rings(general),EG80PHASE,,,null,,,,,, 2010-346T14:00:00,000T23:30:00,12-Dec-10,ISS,Non-SPASS,rings(general),EG80PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2010-346T14:00:00,007T10:23:00,12-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-347T15:37:00,000T09:00:00,13-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-347T16:37:00,000T08:00:00,13-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10347_SP,rider,,,,,, 2010-348T00:37:00,000T13:30:00,14-Dec-10,CDA,Prime,DustRAM direction,ISD0022,,CDA ISD 2010-344T16:15:00,ISD observation around apoapse 2010-344T16:15:00 44.446001 Rs,,,,,, 2010-348T15:37:00,000T09:00:00,14-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-348T16:37:00,000T08:00:00,14-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10348_SP,rider,,,,,, 2010-349T00:37:00,000T13:31:00,15-Dec-10,CDA,Prime,DustRAM direction,ISD0022,,CDA ISD 2010-344T16:15:00,ISD observation around apoapse 2010-344T16:15:00 44.446001 Rs,,,,,, 2010-349T15:38:00,000T09:00:00,15-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-349T16:38:00,000T08:00:00,15-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10349_SP,rider,,,,,, 2010-350T00:38:00,000T07:00:00,16-Dec-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2010-350T09:08:00,000T09:00:00,16-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-350T10:08:00,000T08:00:00,16-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10350_SP,rider,,,,,, 2010-350T18:08:00,000T21:15:00,16-Dec-10,CDA,Prime,DustRAM direction,ISD0022,,CDA ISD 2010-344T16:15:00,ISD observation around apoapse 2010-344T16:15:00 44.446001 Rs,,,,,, 2010-351T15:23:00,000T09:00:00,17-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-351T16:23:00,000T08:00:00,17-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10351_SP,rider,,,,,, 2010-352T00:23:00,001T00:00:00,18-Dec-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-352T15:23:00,000T09:00:00,18-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-352T16:23:00,000T08:00:00,18-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10352_SP,rider,,,,,, 2010-353T00:23:00,001T00:00:00,19-Dec-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-353T02:00:00,000T11:00:00,19-Dec-10,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2010-353T02:00:00,000T11:00:00,19-Dec-10,VIMS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Auroral Stare,Auroral Stare ridealong with UVIS,,,,,, 2010-353T15:23:00,000T03:56:00,19-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-353T15:23:00,000T09:00:00,19-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-353T16:23:00,000T08:00:00,19-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10353_SP,rider,,,,,, 2010-353T19:19:00,000T05:04:00,19-Dec-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-353T21:57:00,001T02:11:00,19-Dec-10,CDA,Non-SPASS,Other,RATE040,,Data rate,Range enter= 13.987647 Rs exit= 13.989891 Range altitude= -1130.3581 km ... 129.30430,,,,,, 2010-354T00:23:00,000T23:45:26,20-Dec-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-354T00:23:00,000T07:37:00,20-Dec-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-354T00:23:00,000T19:02:00,20-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-354T00:23:00,001T09:12:00,20-Dec-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-354T01:03:00,000T02:00:00,20-Dec-10,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 57.4 requested range 0.9 Mkm",,,,,, 2010-354T01:03:00,000T02:00:00,20-Dec-10,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-354T01:03:00,000T01:30:00,20-Dec-10,VIMS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 57 deg, range = 0.9 Mkm.",,,,,, 2010-354T04:15:00,000T03:57:00,20-Dec-10,VIMS,Prime,Dione,DIONE,Dione,Enceladus plume,Dione composition,,,,,, 2010-354T04:15:00,000T03:57:00,20-Dec-10,CIRS,SPASS Rider,Dione,DIONE,Dione,VIMS rider for Dione Observation,null,,,,,, 2010-354T04:15:00,000T03:57:00,20-Dec-10,ISS,SPASS Rider,Dione,DIONE,Dione,Dione plume search,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2010-354T04:15:00,000T03:57:00,20-Dec-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-354T08:00:00,000T02:00:00,20-Dec-10,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2010-354T08:12:00,000T02:18:00,20-Dec-10,VIMS,Prime,Dione,DIONE,Dione,Enceladus plume,Dione composition,,,,,, 2010-354T08:12:00,000T02:18:00,20-Dec-10,CIRS,SPASS Rider,Dione,DIONE,Dione,VIMS rider for Dione Observation,null,,,,,, 2010-354T08:12:00,000T02:18:00,20-Dec-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-354T10:00:00,000T03:08:26,20-Dec-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-354T10:23:00,000T14:15:26,20-Dec-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-354T10:30:00,000T03:55:00,20-Dec-10,CIRS,Prime,Dione,FP3NITE,,FP3/4 Dione Observations,null,,,,,, 2010-354T10:30:00,000T03:55:00,20-Dec-10,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-354T10:30:00,000T03:55:00,20-Dec-10,VIMS,SPASS Rider,Dione,FP3NITE,,Dione,Dione,,,,,, 2010-354T13:08:26,000T10:00:00,20-Dec-10,INMS,Non-SPASS,Enceladus,E13INBND,,Enceladus flyby,Enceladus observation,,,,,, 2010-354T14:25:00,000T00:30:00,20-Dec-10,ISS,Prime,Dione,REGMAP,Regional mapping,Dione wispy streaks,1x3 mosaic of Dione crescent,,,,,, 2010-354T14:25:00,000T00:30:00,20-Dec-10,CIRS,SPASS Rider,Dione,REGMAP,Regional mapping,Dione observation ISS rider,null,,,,,, 2010-354T14:25:00,000T00:30:00,20-Dec-10,VIMS,SPASS Rider,Dione,REGMAP,Regional mapping,Dione,Dione,,,,,, 2010-354T15:15:00,000T04:40:00,20-Dec-10,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus,Enceladus plume PIE,,,,,, 2010-354T15:15:00,000T04:40:00,20-Dec-10,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,CIRS Rider for ISS Icy Plume Observation,null,,,,,, 2010-354T15:15:00,000T04:40:00,20-Dec-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-354T15:15:00,000T04:40:00,20-Dec-10,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,Enceladus plume,Enceladus plume,,,,,, 2010-354T19:25:00,000T03:43:26,20-Dec-10,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2010-354T19:55:00,000T00:40:00,20-Dec-10,CIRS,Prime,Enceladus,NITEMAP,,Night map of Enceladus,null,,,,,, 2010-354T19:55:00,000T00:40:00,20-Dec-10,ISS,SPASS Rider,Enceladus,NITEMAP,,Enceladus pre-close approach,Rider on CIRS Enceladus observation,,,,,, 2010-354T19:55:00,000T00:40:00,20-Dec-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-354T19:55:00,000T00:40:00,20-Dec-10,VIMS,SPASS Rider,Enceladus,NITEMAP,,Enceladus nite,Enceladus,,,,,, 2010-354T20:12:00,000T02:00:00,20-Dec-10,CDA,SPASS Rider,DustRAM direction,RPX0030,,CDA RPXing 2010-354T21:12:00,RPXing at 3.7772502 Rs,,,,,, 2010-354T20:12:00,000T02:00:00,20-Dec-10,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2010-354T20:42:00,000T02:03:00,20-Dec-10,VIMS,Prime,Saturn,ALPORIOCC,Alpha Orion occultation,alpOri Saturn occultation,"alpOri atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec.",,,,,, 2010-354T20:42:00,000T02:03:00,20-Dec-10,CIRS,SPASS Rider,Saturn,ALPORIOCC,Alpha Orion occultation,CIRS_142SA_ALPORIOCC001_VIMS,PIE Collaboration with VIMS. Stellar Occ Saturn ingress T21:25 48N dark limb egress T22:34 45N bright limb,,,,,, 2010-354T22:45:00,000T01:30:00,20-Dec-10,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus,Enceladus plume PIE,,,,,, 2010-354T22:45:00,000T01:30:00,20-Dec-10,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,CIRS ISS RIDER,null,,,,,, 2010-354T22:45:00,000T01:30:00,20-Dec-10,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus,Enceladus composition,,,,,, 2010-354T22:45:26,000T01:30:00,20-Dec-10,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2010-354T22:49:02,000T00:00:01,20-Dec-10,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.578 Rs, lat = 0 deg, phase = 86 deg",,,,,, 2010-354T23:08:26,000T01:06:34,20-Dec-10,INMS,Non-SPASS,Enceladus,ENCEL13,,Enceladus encounter,Enceladus observation,,,,,, 2010-354T23:08:26,000T04:00:00,20-Dec-10,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2010-355T00:08:00,000T02:00:00,21-Dec-10,CDA,SPASS Rider,DustRAM direction,EN013,,CDA Encel 355T01:08 48km,"Encealdus flyby 48 km, v=6.2 km/s",,,,,, 2010-355T00:08:00,000T02:00:00,21-Dec-10,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.987647 Rs exit= 13.989891 Range altitude= -1130.3581 km ... 129.30430,,,,,, 2010-355T00:08:26,000T02:00:00,21-Dec-10,CAPS,SPASS Rider,Enceladus,ENCOUNTER,MAPS Campaign,MAPS 142EN Campaign,Part of 142EN MAPS Campaign. Observe interaction between Enceladus and Saturn's magnetosphere,,,,,, 2010-355T00:15:00,000T01:58:40,21-Dec-10,INMS,Prime,Enceladus,ENCEL13,,Enceladus encounter,Enceladus observation,,,,,, 2010-355T00:33:26,000T01:10:00,21-Dec-10,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2010-355T00:38:26,010T06:51:34,21-Dec-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-355T00:38:26,000T01:00:00,21-Dec-10,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 142,BIT_OVERLAY_300,,,,,, 2010-355T02:08:00,000T21:33:00,21-Dec-10,CDA,Non-SPASS,Other,RATE040,,Data rate,Range enter= 13.987647 Rs exit= 13.989891 Range altitude= -1130.3581 km ... 129.30430,,,,,, 2010-355T02:08:26,001T00:14:34,21-Dec-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-355T02:13:40,000T01:01:20,21-Dec-10,ISS,Prime,Enceladus,ORSCA,,Enceladus post-close approach,ORS observation after close approach,,,,,, 2010-355T02:13:40,000T01:01:20,21-Dec-10,CIRS,SPASS Rider,Enceladus,ORSCA,,CIRS Rider for ISS observation of Enceladus,null,,,,,, 2010-355T02:13:40,000T01:01:20,21-Dec-10,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2010-355T02:13:40,000T01:01:20,21-Dec-10,VIMS,SPASS Rider,Enceladus,ORSCA,,Enceladus,Enceladus composition,,,,,, 2010-355T02:13:40,000T00:54:46,21-Dec-10,INMS,Non-SPASS,Enceladus,ENCEL13,,Enceladus encounter,Enceladus observation,,,,,, 2010-355T03:08:26,000T10:00:00,21-Dec-10,INMS,Non-SPASS,Enceladus,E13OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2010-355T03:08:26,000T23:14:34,21-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-355T03:25:00,000T03:35:00,21-Dec-10,VIMS,Prime,Enceladus,ENCEL,Enceladus,Enceladus plume,Enceladus plume,,,,,, 2010-355T03:25:00,000T03:35:00,21-Dec-10,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,"Enceladus observation, VIMS rider",null,,,,,, 2010-355T03:25:00,000T03:35:00,21-Dec-10,ISS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus post-close approach,Rider on VIMS Enceladus observation,,,,,, 2010-355T03:25:00,000T03:35:00,21-Dec-10,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2010-355T09:35:00,000T16:48:00,21-Dec-10,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-355T13:08:26,000T13:14:34,21-Dec-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-355T16:23:00,000T09:00:00,21-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-355T17:23:00,000T09:00:00,21-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10355_SP,rider,,,,,, 2010-355T23:41:00,009T07:49:00,21-Dec-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.002878 Rs exit= 14.009375 Range altitude= 128.73870 km ... -1028.8273,,,,,, 2010-356T02:23:00,018T06:48:00,22-Dec-10,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2010-356T02:23:00,000T14:20:00,22-Dec-10,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-356T02:23:00,002T11:07:00,22-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-356T02:23:00,009T05:07:00,22-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-356T02:38:00,000T11:00:00,22-Dec-10,ISS,Prime,Other,SIAROT,,Siarnaq,Observation of irregular moon of Saturn.,,,,,, 2010-356T02:38:00,000T11:00:00,22-Dec-10,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2010-356T15:08:00,000T09:00:00,22-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-356T16:08:00,000T08:00:00,22-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10356_SP,rider,,,,,, 2010-356T16:43:00,000T01:22:00,22-Dec-10,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2010-356T18:05:00,001T16:04:00,22-Dec-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-357T01:00:00,000T01:30:00,23-Dec-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 71.5 requested range 2.5 Mkm",,,,,, 2010-357T01:00:00,000T01:30:00,23-Dec-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-357T01:00:00,000T01:30:00,23-Dec-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 72 deg, range = 2.5 Mkm.",,,,,, 2010-357T02:30:00,000T01:00:00,23-Dec-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-357T03:30:00,000T10:00:00,23-Dec-10,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2010-357T03:30:00,000T10:00:00,23-Dec-10,VIMS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Auroral lew,Auroral Slew ridealong with UVIS,,,,,, 2010-357T13:30:00,000T07:00:00,23-Dec-10,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2010-357T20:30:00,000T04:00:00,23-Dec-10,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2010-357T20:30:00,000T04:00:00,23-Dec-10,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2010-358T01:09:00,000T09:00:00,24-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-358T02:09:00,000T08:00:00,24-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10358_SP,rider,,,,,, 2010-358T10:09:00,001T00:00:00,24-Dec-10,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-358T11:00:00,000T01:30:00,24-Dec-10,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 88.9 requested range 2.8 Mkm",,,,,, 2010-358T11:00:00,000T01:30:00,24-Dec-10,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2010-358T11:00:00,000T01:30:00,24-Dec-10,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 89 deg, range = 2.8 Mkm.",,,,,, 2010-358T12:30:00,000T01:00:00,24-Dec-10,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2010-358T13:30:00,000T10:30:00,24-Dec-10,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2010-359T00:00:00,006T09:55:00,25-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2010-359T01:09:00,000T09:00:00,25-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-359T02:09:00,000T08:00:00,25-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10359_SP,rider,,,,,, 2010-359T10:09:00,005T21:22:00,25-Dec-10,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2010-359T14:00:00,001T08:00:00,25-Dec-10,UVIS,Prime,Saturn,MOS142APO,,,"O I and H I scan of Saturn magnetosphere, day 1. 32 hour block of time. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Waypoint at start of observation is assumed to be Saturn center. Allowance for 20 minutes observation margin at start and end, and 30 minutes for turn back to waypoint at the end. Start at Saturn center. Align slit with Saturn spin axis. Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN A 61 times. Repeat this sequence twice: 1) Slew +64 mrad about x-axis 2) Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN B 120 times. 3) Slew +64 mrad about x-axis 4) Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN A 120 times. Scan pattern is 4.5 swaths extending from -4 Rs to +4 Rs E-W. Over the two days of the system scan, N-S extent is approx. -13 Rs to +13 Rs. PATTERN A: Slew +1.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. PATTERN B: Slew -1.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (7913.78113 bps, from Alain's spreadsheet)x(153.0s per stare)x(545 stares) = 659.891x10^6 bits",,,,,, 2010-360T00:00:00,000T01:08:00,26-Dec-10,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2010-361T01:09:00,000T09:00:00,27-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-361T02:09:00,000T08:00:00,27-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10361_SP,rider,,,,,, 2010-361T10:09:00,001T14:45:00,27-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-361T14:00:00,001T08:00:00,27-Dec-10,UVIS,Prime,Saturn,MOS142APO,,,"O I and H I scan of Saturn magnetosphere, day 2. 32 hour block of time. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Waypoint at start of observation is assumed to be Saturn center. Allowance for 20 minutes observation margin at start and end, and 30 minutes for turn back to waypoint at the end. Start at Saturn center. Align slit with Saturn spin axis. Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN B 61 times. Repeat this sequence twice: 1) Slew -64 mrad about x-axis 2) Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN A 120 times. 3) Slew -64 mrad about x-axis 4) Start data capture, stare 153.0 s, stop data capture. Repeat PATTERN B 120 times. Scan pattern is 4.5 swaths extending from -4 Rs to +4 Rs E-W. Over the two days of the system scan, N-S extent is approx. -13 Rs to +13 Rs. PATTERN A: Slew +1.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. PATTERN B: Slew -1.5 mrad about z-axis. Start data capture, stare 153.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (7913.78113 bps, from Alain's spreadsheet)x(153.0s per stare)x(545 stares) = 659.891x10^6 bits",,,,,, 2010-363T00:54:00,000T09:00:00,29-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-363T01:54:00,000T08:00:00,29-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10363_SP,rider,,,,,, 2010-363T09:54:00,000T13:31:00,29-Dec-10,CDA,Prime,DustRAM direction,ISD0023,,CDA ISD 2010-365T07:30:00,ISD observation around apoapse 2010-365T07:30:00 44.706183 Rs,,,,,, 2010-364T00:55:00,000T09:00:00,30-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-364T01:55:00,000T08:00:00,30-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10364_SP,rider,,,,,, 2010-364T09:55:00,000T13:30:00,30-Dec-10,CDA,Prime,DustRAM direction,ISD0023,,CDA ISD 2010-365T07:30:00,ISD observation around apoapse 2010-365T07:30:00 44.706183 Rs,,,,,, 2010-365T00:55:00,000T09:00:00,31-Dec-10,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2010-365T01:55:00,000T08:00:00,31-Dec-10,CIRS,SPASS Rider,InstrumentCalibration,DSCAL10,,CIRS_142IC_DSCAL10365_SP,rider,,,,,, 2010-365T07:30:00,009T07:51:00,31-Dec-10,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.002878 Rs exit= 14.009375 Range altitude= 128.73870 km ... -1028.8273,,,,,, 2010-365T07:30:00,009T01:41:00,31-Dec-10,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2010-365T07:30:00,009T01:41:00,31-Dec-10,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2010-365T07:30:51,000T00:00:01,31-Dec-10,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.7 d, inc = 0.1 deg, r = 44.665 Rs, phase = 94 deg",,,,,, 2010-365T07:31:00,000T01:02:00,31-Dec-10,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-365T08:33:00,000T01:27:00,31-Dec-10,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2010-365T09:55:00,000T14:45:00,31-Dec-10,CDA,Prime,DustRAM direction,ISD0023,,CDA ISD 2010-365T07:30:00,ISD observation around apoapse 2010-365T07:30:00 44.706183 Rs,,,,,, 2010-365T09:55:00,000T05:00:00,31-Dec-10,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2010-365T10:00:00,000T23:40:00,31-Dec-10,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2010-365T14:55:00,008T18:16:00,31-Dec-10,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-001T00:40:00,000T09:00:00,1-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-001T01:40:00,000T08:00:00,1-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11001_SP,rider,,,,,, 2011-001T09:40:00,000T15:00:00,1-Jan-11,CDA,Prime,DustRAM direction,ISD0023,,CDA ISD 2010-365T07:30:00,ISD observation around apoapse 2010-365T07:30:00 44.706183 Rs,,,,,, 2011-001T09:40:00,001T00:00:00,1-Jan-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-002T00:40:00,000T10:20:00,2-Jan-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-002T00:40:00,000T09:00:00,2-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-002T01:40:00,000T08:00:00,2-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11002_SP,rider,,,,,, 2011-002T09:40:00,000T14:20:00,2-Jan-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-002T11:00:00,000T01:00:00,2-Jan-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-002T12:00:00,000T12:00:00,2-Jan-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_143SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-003T00:00:00,000T23:00:00,3-Jan-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn MIRMAP,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-003T00:00:00,000T00:05:00,3-Jan-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Load IEB from SSR's, MRO",,,,,, 2011-003T00:05:00,000T00:33:00,3-Jan-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-003T00:38:00,001T23:22:00,3-Jan-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-004T07:55:00,000T09:00:00,4-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-004T08:55:00,000T08:00:00,4-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11004_SP,rider,,,,,, 2011-004T16:55:00,001T06:00:00,4-Jan-11,CDA,Prime,DustRAM direction,ISD0023,,CDA ISD 2010-365T07:30:00,ISD observation around apoapse 2010-365T07:30:00 44.706183 Rs,,,,,, 2011-005T00:00:00,000T00:34:00,5-Jan-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-005T00:34:00,003T08:52:00,5-Jan-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-006T00:25:00,000T09:00:00,6-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-006T01:25:00,000T08:00:00,6-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11005_SP,rider,,,,,, 2011-006T11:00:00,000T01:00:00,6-Jan-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-006T13:30:00,000T08:30:00,6-Jan-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-007T00:11:00,000T09:00:00,7-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-007T01:11:00,000T08:00:00,7-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11006_SP,rider,,,,,, 2011-007T09:11:00,000T14:34:00,7-Jan-11,ISS,Prime,Other,TARROT,,Tarvos,Observation of irregular moon of Saturn.,,,,,, 2011-007T09:11:00,000T14:34:00,7-Jan-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-008T00:00:00,000T01:08:00,8-Jan-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-008T00:26:00,000T09:00:00,8-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-008T01:26:00,000T08:00:00,8-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11007_SP,rider,,,,,, 2011-008T09:26:00,000T14:45:00,8-Jan-11,ISS,Prime,RingE,ERNGVRHP,,High-Phase Edge-on obs E-ring observation after Eq,Low elevation observation of E ring at high phase.,,,,,, 2011-008T09:26:00,000T14:45:00,8-Jan-11,CIRS,SPASS Rider,rings(general),ERNGVRHP,,,null,,,,,, 2011-008T09:26:00,000T11:34:00,8-Jan-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-008T21:00:00,000T02:00:00,8-Jan-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-008T23:00:00,000T10:11:00,8-Jan-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-009T00:11:00,000T09:00:00,9-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-009T01:11:00,000T08:00:00,9-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11008_SP,rider,,,,,, 2011-009T09:11:00,001T18:42:25,9-Jan-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-009T09:11:00,000T04:06:51,9-Jan-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-009T09:11:00,001T03:39:00,9-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-009T09:11:00,001T19:12:25,9-Jan-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-009T09:11:00,000T03:33:00,9-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-009T09:55:00,000T03:11:00,9-Jan-11,VIMS,Prime,Saturn,REGMAP,Regional mapping,Saturn Regional Map,"Regional Map 3*2 centered on equator, repeat two more times and add a few extra images at the end",,,,,, 2011-009T09:55:00,000T03:11:00,9-Jan-11,ISS,Non-SPASS,Saturn,REGMAP,Regional mapping,Night NAC lightning search,Rider on VIMS to search for lightning spectrum at the night side with NAC and to monitor clouds illuminated by rings with WAC.,,,,,, 2011-009T12:44:00,001T21:39:00,9-Jan-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-009T13:06:00,000T09:25:00,9-Jan-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,This is a PIE. One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-009T13:06:00,000T09:25:00,9-Jan-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-009T13:17:51,000T12:42:09,9-Jan-11,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-009T15:21:00,002T01:46:00,9-Jan-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.996392 Rs exit= 13.996275 Range altitude= -1027.7861 km ... 1980.6234,,,,,, 2011-010T00:11:00,000T09:00:00,10-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-010T01:41:00,000T08:00:00,10-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11009_SP,rider,,,,,, 2011-010T02:00:00,000T02:00:00,10-Jan-11,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2011-010T04:00:00,000T08:17:51,10-Jan-11,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-010T10:21:00,000T04:28:00,10-Jan-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,This is a PIE. One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-010T10:21:00,000T04:28:00,10-Jan-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-010T10:21:00,000T04:28:00,10-Jan-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-010T12:00:00,000T02:00:00,10-Jan-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-010T12:17:51,000T00:30:00,10-Jan-11,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-010T12:18:00,000T02:00:00,10-Jan-11,CDA,SPASS Rider,DustRAM direction,RPX0040,,CDA RPXing 2011-010T13:18:00,RPXing at 4.1669315 Rs,,,,,, 2011-010T12:47:51,000T01:30:00,10-Jan-11,INMS,SPASS Rider,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-010T12:50:00,000T06:55:00,10-Jan-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-010T14:17:51,000T02:35:34,10-Jan-11,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-010T14:49:00,000T02:42:00,10-Jan-11,VIMS,Prime,Saturn,ALPCMAOCC,,alpCMa Saturn occultation,"alpCMa atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec.",,,,,, 2011-010T14:49:00,000T02:42:00,10-Jan-11,CIRS,SPASS Rider,Saturn,ALPCMAOCC,,CIRS_143SA_ALPCMAOCC001_VIMS,PIE Collaboration with VIMS. Stellar Occ Saturn ingress T15:35 60S dark limb egress T16:22 60S bright limb,,,,,, 2011-010T14:49:00,000T02:42:00,10-Jan-11,ISS,SPASS Rider,Saturn,ALPCMAOCC,,Photometric Calibration Ridealong,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-010T16:13:38,000T00:00:01,10-Jan-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.578 Rs, lat = 0 deg, phase = 86 deg",,,,,, 2011-010T16:53:25,000T10:00:00,10-Jan-11,INMS,Non-SPASS,Rhea,R3INBND,,Rhea flyby,Rhea observation,,,,,, 2011-010T17:31:00,000T02:30:00,10-Jan-11,VIMS,Prime,Saturn,RLEOOCC,R Leo occultation,R Leo Saturn occultation,"R Leo atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec.",,,,,, 2011-010T17:31:00,000T02:30:00,10-Jan-11,CIRS,SPASS Rider,Saturn,RLEOOCC,R Leo occultation,CIRS_143SA_RLEOOCC001_VIMS,PIE Collaboration with VIMS. Stellar Occ Saturn ingress T18:14 40N dark limb egress 45N T19:40 bright limb,,,,,, 2011-010T17:31:00,000T02:30:00,10-Jan-11,ISS,SPASS Rider,Saturn,RLEOOCC,R Leo occultation,R Leo Ridealong,Point and stare; cycle camera commands.,,,,,, 2011-010T19:45:00,000T07:08:25,10-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-010T20:01:00,000T07:52:00,10-Jan-11,VIMS,Prime,Saturn,REGMAP,Regional mapping,Saturn Regional Map #2,"Regional Map 3*2 centered on equator, repeat seven more times",,,,,, 2011-010T20:01:00,000T07:52:00,10-Jan-11,CIRS,SPASS Rider,Saturn,REGMAP,Regional mapping,VIMS rider for good spatial res obs,rider,,,,,, 2011-010T20:01:00,000T08:02:00,10-Jan-11,ISS,Non-SPASS,Saturn,REGMAP,Regional mapping,Night NAC lightning search,Rider on VIMS to search for lightning spectrum at the night side with NAC and to monitor clouds illuminated by rings with WAC.,,,,,, 2011-011T02:53:25,000T01:15:00,11-Jan-11,INMS,Non-SPASS,Rhea,RHEA3,,Rhea encounter,Rhea observation,,,,,, 2011-011T02:53:25,000T04:00:00,11-Jan-11,MAG,Non-SPASS,Rhea,RHTAR,Rhea targeted flyby,Rhea targeted flyby,Monitor the interaction of Rhea with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2011-011T03:53:25,000T02:00:00,11-Jan-11,CAPS,SPASS Rider,Rhea,ENCOUNTER,MAPS Campaign,MAPS 143RH Campaign,Part of 143RH MAPS Campaign. Observe interaction between Rhea and Saturn's magnetosphere,,,,,, 2011-011T04:08:00,000T01:30:00,11-Jan-11,CDA,SPASS Rider,Other,RHEAFLYBY,,CDA_RHEA Flyby,CDA RHEA FLYBY; objective code RN1a,,,,,, 2011-011T04:08:25,000T01:24:00,11-Jan-11,CAPS,Prime,Rhea,RHEAPTG,,MAPS 143RH Campaign,Part of143RH MAPS Campaign. Observe interaction between Rhea and Saturn's magnetosphere,,,,,, 2011-011T04:08:25,000T01:30:00,11-Jan-11,INMS,SPASS Rider,Rhea,RHEA3,,Rhea encounter,Rhea observation,,,,,, 2011-011T04:08:25,000T01:24:00,11-Jan-11,ISS,SPASS Rider,Rhea,RHEAPTG,,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-011T04:08:25,000T01:30:00,11-Jan-11,RPWS,Non-SPASS,Rhea,RHCA,Rhea closest approach,Rhea closest approach observations,"RPWS observations in the immediate vicinity of Rhea, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2011-011T04:23:25,006T04:18:35,11-Jan-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-011T04:23:25,000T01:00:00,11-Jan-11,MIMI,Non-SPASS,Rhea,ENCNTROV,,MIMI Rhea 143,BIT_OVERLAY_300,,,,,, 2011-011T04:50:25,000T00:06:00,11-Jan-11,UVIS,SPASS Rider,Rhea,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2011-011T05:32:25,000T04:06:00,11-Jan-11,ISS,Prime,Rhea,RHEA,Rhea,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-011T05:38:25,000T04:00:00,11-Jan-11,CIRS,SPASS Rider,Rhea,RHEA,Rhea,CIRS ISS RIDER,null,,,,,, 2011-011T05:38:25,000T02:00:00,11-Jan-11,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-011T05:38:25,000T01:15:00,11-Jan-11,INMS,Non-SPASS,Rhea,RHEA3,,Rhea encounter,Rhea observation,,,,,, 2011-011T05:53:25,001T11:32:35,11-Jan-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-011T06:53:25,000T10:00:00,11-Jan-11,INMS,Non-SPASS,Rhea,R3OUTBND,,Rhea flyby,Rhea observation,,,,,, 2011-011T06:53:25,001T10:32:35,11-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-011T10:23:00,000T04:13:00,11-Jan-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-011T14:36:00,000T05:08:00,11-Jan-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-011T15:16:00,000T14:00:00,11-Jan-11,VIMS,Prime,Saturn,REGMAP,Regional mapping,Saturn Regional Map #3,"Regional Map 3*2 centered on equator, repeat thirteen more times",,,,,, 2011-011T15:16:00,000T14:00:00,11-Jan-11,CIRS,SPASS Rider,Saturn,REGMAP,Regional mapping,VIMS rider for good spatial res obs,rider,,,,,, 2011-011T15:16:00,000T14:00:00,11-Jan-11,ISS,Non-SPASS,Saturn,REGMAP,Regional mapping,Night NAC lightning search,Rider on VIMS to search for lightning spectrum at the night side with NAC and to monitor clouds illuminated by rings with WAC.,,,,,, 2011-011T16:53:25,001T00:32:35,11-Jan-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-011T17:07:00,005T15:35:00,11-Jan-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S66,Range enter= 14.009241 Rs exit= 14.011157 Range altitude= 1984.8706 km ... 4188.2766,,,,,, 2011-011T19:44:00,000T21:42:00,11-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-012T07:26:00,000T09:00:00,12-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-012T07:26:00,000T09:00:00,12-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-012T08:26:00,000T09:00:00,12-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11012_SP,rider,,,,,, 2011-012T17:26:00,004T15:16:00,12-Jan-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-012T17:26:00,001T23:01:00,12-Jan-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-012T17:26:00,003T03:34:00,12-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-012T17:26:00,004T15:16:00,12-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-012T19:00:00,000T08:00:00,12-Jan-11,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_143_SCATTERED_SUNLIGHT_TEST_PRIME,"Monitor scattered IR solar radiation as a function of offset angle from the sun using radial scans. CIRS to operate at 15.5 cm-1 resolution (4.825 sec/frame, 39 RTI), detector pairs, FP4. FPB scans will begin TBD degrees from Sun, and will scan to 12 degrees of Sun at TBD rate; Scan will stop every 10 degrees for TBD seconds; (the procedure will be repeated in the reverse direction back to the initial position;) to determine whether scattering is asymmetric with respect to the FPB axis, additional scans will be made. . . . . REDESIGN NEEDED HERE . . . 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from TBD degrees +Z to 12 degrees +Z and back to 40 degrees +Z. 2) From TBD degrees in -X on the X axis, to 12 degrees on the -X axis, to TBD degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 12 degrees -Z and back to TBD degrees -Z. ACTUALLY: IN, UP, DOWN, DOWN, UP, BACK WILL DO: || || || || || || || ||||| ||||||||||||||||| * ||||| || || || || || || ||",,,,,, 2011-013T03:00:00,000T02:57:00,13-Jan-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2011-013T07:27:00,000T09:00:00,13-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-013T08:27:00,000T08:00:00,13-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11013_SP,rider,,,,,, 2011-013T16:27:00,000T14:30:00,13-Jan-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-014T07:27:00,000T09:00:00,14-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-014T08:27:00,000T08:00:00,14-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11014_SP,rider,,,,,, 2011-014T16:27:00,001T00:00:00,14-Jan-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-014T17:05:00,000T10:10:00,14-Jan-11,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2011-014T17:05:00,000T10:10:00,14-Jan-11,VIMS,SPASS Rider,Titan,COMPMAP,Composition map,Stare at Titan.,"VIMS ridealong with CIRS compsite observations; phase = 68 deg, range = 1 Mkm.",,,,,, 2011-015T03:15:00,000T02:00:00,15-Jan-11,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 88.8 requested range 0.8 Mkm",,,,,, 2011-015T03:15:00,000T02:00:00,15-Jan-11,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-015T03:15:00,000T02:00:00,15-Jan-11,VIMS,SPASS Rider,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 89 deg, range = 0.8 Mkm.",,,,,, 2011-015T07:27:00,000T09:00:00,15-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-015T08:27:00,000T08:00:00,15-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11015_SP,rider,,,,,, 2011-015T16:27:00,001T16:15:00,15-Jan-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-015T18:00:00,000T02:00:00,15-Jan-11,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 67.7 requested range 1 Mkm",,,,,, 2011-015T18:00:00,000T02:00:00,15-Jan-11,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-015T18:00:00,000T02:00:00,15-Jan-11,VIMS,SPASS Rider,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 68 deg, range = 1 Mkm.",,,,,, 2011-015T20:00:00,000T01:00:00,15-Jan-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-015T21:00:00,000T08:00:00,15-Jan-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-016T05:00:00,001T03:42:00,16-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-016T23:42:00,000T09:00:00,16-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-017T00:42:00,000T08:00:00,17-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11016_SP,rider,,,,,, 2011-017T08:42:00,002T18:40:00,17-Jan-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-017T08:42:00,003T12:46:00,17-Jan-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S66,Range enter= 14.009241 Rs exit= 14.011157 Range altitude= 1984.8706 km ... 4188.2766,,,,,, 2011-017T08:42:00,000T00:43:00,17-Jan-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-017T08:42:00,012T06:47:00,17-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-017T08:42:00,003T12:46:00,17-Jan-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-017T08:42:00,003T12:46:00,17-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-017T08:47:00,000T00:02:00,17-Jan-11,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S66 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2011-017T08:52:00,001T20:50:00,17-Jan-11,CDA,Prime,DustRAM direction,ISD0024,,CDA ISD 2011-020T21:28:00,ISD observation around apoapse 2011-020T21:28:00 44.284368 Rs,,,,,, 2011-017T09:25:00,000T00:07:00,17-Jan-11,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-017T09:32:00,000T00:05:00,17-Jan-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-017T09:37:00,000T00:33:00,17-Jan-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-017T10:10:00,000T00:30:00,17-Jan-11,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2011-017T10:40:00,000T02:36:00,17-Jan-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-017T13:16:00,003T08:12:00,17-Jan-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-019T03:12:00,000T13:00:00,19-Jan-11,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-26 (used to be DSS-25 before Revision1) in 1-way mode. No rolling during 3-hour USO from 2011-021T06:58:00 till 2011-021T09:58:00.,,,,,, 2011-019T07:12:00,000T09:00:00,19-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-019T08:12:00,000T08:00:00,19-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_143IC_DSCAL11019_SP,rider,,,,,, 2011-019T15:28:00,000T20:00:00,19-Jan-11,CDA,SPASS Rider,DustRAM direction,ISD0024,,CDA ISD 2011-020T21:28:00,ISD observation around apoapse 2011-020T21:28:00 44.284368 Rs,,,,,, 2011-019T18:30:00,000T23:00:00,19-Jan-11,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T Map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-020T03:22:00,009T12:07:00,20-Jan-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-020T17:30:00,000T01:30:00,20-Jan-11,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Dione","Images of mutual event, transit of Rhea across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-020T21:28:00,009T04:28:59,20-Jan-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.009241 Rs exit= 14.011157 Range altitude= 1984.8706 km ... 4188.2766,,,,,, 2011-020T21:28:00,000T01:37:00,20-Jan-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-020T21:28:00,020T10:38:00,20-Jan-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-020T21:28:00,008T18:01:00,20-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-020T21:28:02,000T00:00:01,20-Jan-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.4 d, inc = 0.3 deg, r = 44.239 Rs, phase = 93 deg",,,,,, 2011-020T23:05:00,000T00:34:00,20-Jan-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-020T23:39:00,008T08:43:00,20-Jan-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-021T06:58:00,000T09:00:00,21-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-021T07:58:00,000T08:00:00,21-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11021_SP,rider,,,,,, 2011-021T17:00:00,000T01:30:00,21-Jan-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 76.7 requested range 3.4 Mkm",,,,,, 2011-021T17:00:00,000T01:30:00,21-Jan-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-021T17:00:00,000T01:30:00,21-Jan-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 77 deg, range = 3.4 Mkm.",,,,,, 2011-021T18:30:00,000T01:00:00,21-Jan-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-021T19:30:00,000T16:00:00,21-Jan-11,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,"Stare at E or G ring ansa, 1 second integration.",,,,,, 2011-021T19:30:00,000T16:00:00,21-Jan-11,CIRS,SPASS Rider,rings(general),EG80PHASE,,,null,,,,,, 2011-021T19:30:00,000T16:00:00,21-Jan-11,ISS,Non-SPASS,rings(general),EG80PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2011-022T12:30:00,000T16:58:00,22-Jan-11,ISS,Prime,Other,IJIROT,,Ijiraq,Observation of irregular moon of Saturn.,,,,,, 2011-022T12:30:00,000T16:58:00,22-Jan-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-023T05:28:00,000T10:30:00,23-Jan-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-023T06:58:00,000T09:00:00,23-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-023T07:58:00,000T08:00:00,23-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11023_SP,rider,,,,,, 2011-023T15:58:00,001T19:45:00,23-Jan-11,CDA,Prime,DustRAM direction,ISD0024,,CDA ISD 2011-020T21:28:00,ISD observation around apoapse 2011-020T21:28:00 44.284368 Rs,,,,,, 2011-025T00:00:00,000T01:08:00,25-Jan-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-025T13:13:00,000T09:00:00,25-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-025T14:13:00,000T08:00:00,25-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11025_SP,rider,,,,,, 2011-025T22:13:00,001T13:15:00,25-Jan-11,CDA,Prime,DustRAM direction,ISD0024,,CDA ISD 2011-020T21:28:00,ISD observation around apoapse 2011-020T21:28:00 44.284368 Rs,,,,,, 2011-027T12:58:00,000T09:00:00,27-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-027T13:58:00,000T08:00:00,27-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11027_SP,rider,,,,,, 2011-027T23:00:00,000T11:00:00,27-Jan-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS_144SA_COMPSIT001,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-028T10:00:00,000T11:00:00,28-Jan-11,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2011-028T10:00:00,000T11:00:00,28-Jan-11,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare,"CL1 NAC 4x4 images. 10 Mbits/hr, only 05:32:00 of the 11 hours is a stare",,,,,, 2011-028T10:00:00,000T11:00:00,28-Jan-11,VIMS,,Saturn,AURSTARE,Saturn aurora,Auroral Stare,Auroral Stare ridealong with UVIS,,,,,, 2011-028T23:59:00,000T03:00:00,28-Jan-11,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2011-029T00:00:20,000T00:00:01,29-Jan-11,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2011-029T02:59:00,000T02:00:00,29-Jan-11,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2011-029T06:29:00,000T09:00:00,29-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-029T07:29:00,000T08:00:00,29-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11029_SP,rider,,,,,, 2011-029T08:22:00,000T02:00:00,29-Jan-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-029T10:22:00,000T05:07:00,29-Jan-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-029T15:29:00,000T12:50:00,29-Jan-11,UVIS,Prime,Dione,ICYSTARE,,ICYSTARE: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of satellite.,,,,,, 2011-029T15:29:00,000T12:50:00,29-Jan-11,CIRS,SPASS Rider,Dione,ICYSTARE,,,null,,,,,, 2011-029T15:29:00,000T12:50:00,29-Jan-11,ISS,SPASS Rider,Dione,ICYSTARE,,Dione plume search,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-029T15:29:00,003T16:15:00,29-Jan-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-029T15:29:00,000T06:16:23,29-Jan-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-029T15:29:00,001T07:56:00,29-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-029T15:29:00,000T07:51:00,29-Jan-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-029T21:45:23,000T23:00:00,29-Jan-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-029T23:20:00,002T07:00:00,29-Jan-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-030T01:56:59,002T01:46:00,30-Jan-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.998191 Rs exit= 13.993001 Range altitude= 4182.8016 km ... 1456.0734,,,,,, 2011-030T06:29:00,000T09:00:00,30-Jan-11,RSS,SPASS Rider,Titan,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev145 Titan gravity observation on 2011/049-050 (T74).",,,,,, 2011-030T06:29:00,000T09:00:00,30-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-030T07:29:00,000T08:00:00,30-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11030_SP,rider,,,,,, 2011-030T16:09:00,000T00:40:00,30-Jan-11,VIMS,SPASS Rider,Enceladus,WAYPTTURN,Waypoint turn,,null,,,,,, 2011-030T16:49:00,000T03:36:00,30-Jan-11,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-030T16:49:00,000T03:36:00,30-Jan-11,CIRS,SPASS Rider,Enceladus,PLMHPR,,,null,,,,,, 2011-030T16:49:00,000T03:36:00,30-Jan-11,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2011-030T16:49:00,000T03:36:00,30-Jan-11,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2011-030T20:25:00,000T07:35:00,30-Jan-11,CIRS,Prime,Mimas,MIMAS,Mimas,Thermal Mapping of Mimas,null,,,,,, 2011-030T20:25:00,000T07:35:00,30-Jan-11,ISS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas flyby,"ORS observation, CIRS rider",,,,,, 2011-030T20:25:00,000T07:35:00,30-Jan-11,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-030T20:25:00,000T05:35:00,30-Jan-11,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,,null,,,,,, 2011-030T20:45:00,000T02:00:00,30-Jan-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-030T20:45:23,000T02:00:00,30-Jan-11,INMS,Non-SPASS,Saturn,PLUMERPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-030T20:45:59,000T02:00:00,30-Jan-11,CDA,SPASS Rider,DustRAM direction,RPX0050,,CDA RPXing 2011-030T21:45:59,RPXing at 5.0533252 Rs,,,,,, 2011-030T22:45:23,000T23:00:00,30-Jan-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-030T23:25:00,000T07:00:00,30-Jan-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-031T02:50:17,000T00:00:01,31-Jan-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.559 Rs, lat = -0 deg, phase = 87 deg",,,,,, 2011-031T04:00:00,000T01:30:00,31-Jan-11,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-031T04:00:00,000T01:30:00,31-Jan-11,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2011-031T04:00:00,000T01:30:00,31-Jan-11,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2011-031T04:00:00,000T01:30:00,31-Jan-11,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2011-031T05:30:00,000T02:00:00,31-Jan-11,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus post-close approach,ORS observation after close approach,,,,,, 2011-031T05:30:00,000T02:00:00,31-Jan-11,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2011-031T05:30:00,000T02:00:00,31-Jan-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-031T05:30:00,000T02:00:00,31-Jan-11,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2011-031T06:25:00,002T01:19:00,31-Jan-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-031T07:30:00,000T01:30:00,31-Jan-11,ISS,Prime,Mimas,MIMAS,Mimas,Mimas flyby,ORS observation,,,,,, 2011-031T07:30:00,000T01:30:00,31-Jan-11,CIRS,SPASS Rider,Mimas,MIMAS,Mimas,,null,,,,,, 2011-031T07:30:00,000T01:30:00,31-Jan-11,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-031T07:30:00,000T01:30:00,31-Jan-11,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,,null,,,,,, 2011-031T09:00:00,000T03:00:00,31-Jan-11,ISS,Prime,Helene,HELENE,,Helene flyby,ORS observation,,,,,, 2011-031T09:00:00,000T03:00:00,31-Jan-11,CIRS,SPASS Rider,Helene,HELENE,,,null,,,,,, 2011-031T09:00:00,000T03:00:00,31-Jan-11,UVIS,SPASS Rider,Helene,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-031T09:00:00,000T03:00:00,31-Jan-11,VIMS,SPASS Rider,Helene,HELENE,,,null,,,,,, 2011-031T12:00:00,000T01:30:00,31-Jan-11,VIMS,Prime,Mimas,MIMAS,Mimas,,MIMAS,,,,,, 2011-031T12:00:00,000T01:30:00,31-Jan-11,CIRS,SPASS Rider,Mimas,MIMAS,Mimas,,null,,,,,, 2011-031T12:00:00,000T01:30:00,31-Jan-11,ISS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas flyby,"ORS observation, VIMS rider",,,,,, 2011-031T12:00:00,000T01:30:00,31-Jan-11,UVIS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-031T13:30:00,000T02:30:00,31-Jan-11,UVIS,Prime,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-031T13:30:00,000T02:30:00,31-Jan-11,CIRS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,,null,,,,,, 2011-031T13:30:00,000T02:30:00,31-Jan-11,ISS,SPASS Rider,Mimas,ICYLON,Icy satellite longitudinal coverage,Mimas flyby,"ORS observation, UVIS rider",,,,,, 2011-031T13:30:00,000T02:30:00,31-Jan-11,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,,null,,,,,, 2011-031T16:03:59,000T02:00:00,31-Jan-11,CDA,SPASS Rider,DustRAM direction,RPX0060,,CDA RPXing 2011-031T17:03:59,RPXing at 9.4587730 Rs,,,,,, 2011-031T16:04:00,000T02:00:00,31-Jan-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-031T21:45:23,000T09:58:37,31-Jan-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-031T22:44:00,000T09:00:00,31-Jan-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-031T23:44:00,000T08:00:00,31-Jan-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11031_SP,rider,,,,,, 2011-032T03:42:59,009T04:22:01,1-Feb-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.005969 Rs exit= 14.001548 Range altitude= 1460.4504 km ... 3613.8943,,,,,, 2011-032T06:20:00,001T01:24:00,1-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-032T07:44:00,001T00:00:00,1-Feb-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-032T08:29:00,000T03:40:00,1-Feb-11,ISS,Prime,Other,L5MIMAS,,Mimas L5 satellite search,Satellite search around Mimas L5 Lagrange point.,,,,,, 2011-032T08:29:00,000T03:40:00,1-Feb-11,CIRS,SPASS Rider,Other,L5MIMAS,,,Deep-space calibration during ISS Mimas Trojan search?,,,,,, 2011-032T08:29:00,000T03:40:00,1-Feb-11,VIMS,SPASS Rider,Other,L5MIMAS,,,null,,,,,, 2011-032T12:09:00,000T03:20:00,1-Feb-11,ISS,Prime,Other,MIMASL4,,Mimas L4 satellite search,Satellite search around Mimas L4 Lagrange point.,,,,,, 2011-032T12:09:00,000T03:20:00,1-Feb-11,CIRS,SPASS Rider,Other,MIMASL4,,,Data Volume Added Again following SOST June 25th Meeting Name correction.,,,,,, 2011-032T12:09:00,000T03:20:00,1-Feb-11,VIMS,SPASS Rider,Other,MIMASL4,,,null,,,,,, 2011-032T22:44:00,000T09:00:00,1-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-032T23:44:00,000T08:00:00,1-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11032_SP,rider,,,,,, 2011-033T07:44:00,015T12:47:00,2-Feb-11,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2011-033T07:44:00,008T00:22:00,2-Feb-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-033T07:44:00,003T23:46:00,2-Feb-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-033T07:44:00,008T00:22:00,2-Feb-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-033T07:44:00,002T00:00:00,2-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-033T08:24:00,000T18:22:00,2-Feb-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-034T02:46:00,000T01:04:00,3-Feb-11,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Dione","Images of mutual event, transit of Rhea across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-034T03:50:00,000T16:44:00,3-Feb-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-034T22:44:00,000T09:00:00,3-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-034T23:44:00,000T08:00:00,3-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11034_SP,rider,,,,,, 2011-035T07:44:00,003T23:31:00,4-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-035T08:24:00,000T01:30:00,4-Feb-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 41.9 requested range 2.4 Mkm",,,,,, 2011-035T08:24:00,000T01:30:00,4-Feb-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-035T08:24:00,000T01:30:00,4-Feb-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 42 deg, range = 2.4 Mkm.",,,,,, 2011-035T09:54:00,000T01:00:00,4-Feb-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-035T14:22:00,001T02:38:00,4-Feb-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-036T17:00:00,000T04:00:00,5-Feb-11,ISS,Prime,Other,IJISUP,,Ijiraq,Observation of irregular moon of Saturn.,,,,,, 2011-036T22:30:00,000T09:00:00,5-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-036T23:30:00,000T08:00:00,5-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11036_SP,rider,,,,,, 2011-037T07:30:00,000T07:00:00,6-Feb-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-037T14:30:00,001T06:15:00,6-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-037T14:30:00,010T06:16:00,6-Feb-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-038T08:05:00,000T20:00:00,7-Feb-11,CDA,SPASS Rider,DustRAM direction,ISD0025,,CDA ISD 2011-041T08:05:00,ISD observation around apoapse 2011-041T08:05:00 44.270410 Rs,,,,,, 2011-038T22:15:00,000T09:00:00,7-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-038T23:15:00,000T08:00:00,7-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11038_SP,rider,,,,,, 2011-039T07:15:00,000T13:45:00,8-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-039T07:15:00,002T00:50:00,8-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-039T21:00:00,000T15:00:00,8-Feb-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-040T00:00:00,000T01:08:00,9-Feb-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-040T02:05:00,000T20:00:00,9-Feb-11,CDA,SPASS Rider,DustRAM direction,ISD0025,,CDA ISD 2011-041T08:05:00,ISD observation around apoapse 2011-041T08:05:00 44.270410 Rs,,,,,, 2011-040T12:00:00,000T04:00:00,9-Feb-11,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2011-040T12:00:00,000T04:00:00,9-Feb-11,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2011-040T16:00:00,000T04:45:00,9-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-040T22:15:00,000T09:00:00,9-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-040T23:15:00,000T08:00:00,9-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_144IC_DSCAL11040_SP,rider,,,,,, 2011-041T07:15:00,000T13:15:00,10-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-041T08:05:00,009T04:01:59,10-Feb-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.005969 Rs exit= 14.001548 Range altitude= 1460.4504 km ... 3613.8943,,,,,, 2011-041T08:05:00,001T22:55:00,10-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-041T08:05:57,000T00:00:01,10-Feb-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 20.4 d, inc = 0.3 deg, r = 44.226 Rs, phase = 93 deg",,,,,, 2011-041T08:06:00,000T02:00:00,10-Feb-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-041T08:06:00,024T04:33:00,10-Feb-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-041T08:06:00,006T03:40:00,10-Feb-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-041T10:06:00,005T10:40:00,10-Feb-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-041T18:05:00,000T20:00:00,10-Feb-11,CDA,SPASS Rider,DustRAM direction,ISD0025,,CDA ISD 2011-041T08:05:00,ISD observation around apoapse 2011-041T08:05:00 44.270410 Rs,,,,,, 2011-041T20:30:00,000T10:30:00,10-Feb-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-041T22:00:00,000T09:00:00,10-Feb-11,RSS,SPASS Rider,Titan,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev145 Titan gravity observation on 2011/049-050 (T74).",,,,,, 2011-041T22:00:00,000T09:00:00,10-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-041T23:00:00,000T08:00:00,10-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11041_SP,rider,,,,,, 2011-042T11:00:00,000T09:30:00,11-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-042T22:00:00,000T09:00:00,11-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-042T23:00:00,000T08:00:00,11-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11042_SP,rider,,,,,, 2011-043T07:00:00,000T15:00:00,12-Feb-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-043T07:00:00,004T04:46:00,12-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-043T12:05:00,000T20:00:00,12-Feb-11,CDA,SPASS Rider,DustRAM direction,ISD0025,,CDA ISD 2011-041T08:05:00,ISD observation around apoapse 2011-041T08:05:00 44.270410 Rs,,,,,, 2011-043T22:00:00,000T12:30:00,12-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-044T12:00:00,000T09:00:00,13-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-044T13:00:00,000T08:00:00,13-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11044_SP,rider,,,,,, 2011-044T21:00:00,000T13:16:00,13-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-045T11:46:00,000T09:00:00,14-Feb-11,RSS,SPASS Rider,Titan,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev145 Titan gravity observation on 2011/049-050 (T74).",,,,,, 2011-045T11:46:00,000T09:00:00,14-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-045T12:46:00,000T08:00:00,14-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11045_SP,rider,,,,,, 2011-045T20:46:00,000T15:00:00,14-Feb-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-046T11:46:00,000T09:00:00,15-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-046T12:46:00,000T08:00:00,15-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11046_SP,rider,,,,,, 2011-046T20:46:00,000T15:00:00,15-Feb-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-046T20:46:00,001T00:00:00,15-Feb-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-047T11:46:00,000T09:00:00,16-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-047T11:46:00,000T09:00:00,16-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-047T12:46:00,000T08:00:00,16-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11047_SP,rider,,,,,, 2011-047T20:46:00,000T13:15:00,16-Feb-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-047T20:46:00,000T23:45:00,16-Feb-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-047T20:46:00,000T23:45:00,16-Feb-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-047T20:46:00,000T23:45:00,16-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-048T11:31:00,000T09:00:00,17-Feb-11,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's gravity,Additional downlink pass at Ka-band for Titan's gravity science and for improving locally Cassini orbit.,,,,,, 2011-048T11:31:00,000T09:00:00,17-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-048T12:31:00,000T08:00:00,17-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11048_SP,rider,,,,,, 2011-048T20:31:00,000T07:33:11,17-Feb-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-048T20:31:00,000T07:33:11,17-Feb-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-048T20:31:00,000T15:33:11,17-Feb-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-048T20:31:00,001T12:55:00,17-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-048T21:26:00,000T06:38:11,17-Feb-11,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 152 deg. SSC Lat/Lon = 0.043S/136.331 deg. SS Lat/Lon = 8.307N/288.512 deg. Alt = 372008 km, range = 374583 km. Resolution = 186 km/px. Temp. M4.",,,,,, 2011-048T21:26:10,000T06:38:00,17-Feb-11,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-048T21:26:11,000T06:38:00,17-Feb-11,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,"Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template M4, no ISS dwells.",,,,,, 2011-049T01:59:11,000T02:05:00,18-Feb-11,RSS,SPASS Rider,Titan,THERMAL,Thermal stabilization period,RSS thermal stabilization,A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance.,,,,,, 2011-049T04:04:11,001T00:00:00,18-Feb-11,CAPS,Prime,Titan,T74PTG,,Titan Encounter,null,,,,,, 2011-049T04:04:11,000T08:00:00,18-Feb-11,CAPS,SPASS Rider,Titan,T74INBND,,Inbound 145TI (T74),null,,,,,, 2011-049T04:04:11,001T00:00:00,18-Feb-11,CIRS,SPASS Rider,Titan,RIDER,Instrument rider,,Rider along with CAPS flyby.,,,,,, 2011-049T04:04:11,001T00:00:00,18-Feb-11,RSS,SPASS Rider,Titan,GRAVITY,RSS gravity science experiment,RSS Titan's Gravity Field Experiment,Experiment to determine Titan's gravity field and ultimately the dynamics Love number.,,,,,, 2011-049T04:04:11,000T11:00:00,18-Feb-11,INMS,Non-SPASS,Saturn,T74INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-049T12:04:11,000T08:00:00,18-Feb-11,CAPS,SPASS Rider,Titan,T74CLOSE,,Closest Approach 145TI (T74),null,,,,,, 2011-049T12:04:11,000T08:00:00,18-Feb-11,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T74 flyby,"T74 is a post-dusk, upstream, high altitude (3639 km) ?blind? flyby that will be useful to characterize the background field in which Titan sits in. We assign grade two priority. Data rate: 988bps (16vps).",,,,,, 2011-049T14:04:11,000T01:00:00,18-Feb-11,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-049T14:04:11,000T01:00:00,18-Feb-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-049T15:04:11,000T02:00:00,18-Feb-11,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-049T15:04:11,000T02:00:00,18-Feb-11,INMS,Non-SPASS,Titan,TITAN74,,Titan Flyby,Titan observation,,,,,, 2011-049T15:04:11,000T02:00:00,18-Feb-11,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2011-049T17:04:11,000T01:00:00,18-Feb-11,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-049T17:04:11,000T11:00:00,18-Feb-11,INMS,Non-SPASS,Saturn,T74OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-049T17:04:11,000T01:00:00,18-Feb-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-049T18:04:11,001T02:26:49,18-Feb-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-049T20:04:11,000T08:00:00,18-Feb-11,CAPS,SPASS Rider,Titan,T74OUTBND,,Outbound 145TI (T74),null,,,,,, 2011-049T20:04:11,001T00:26:49,18-Feb-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-050T04:04:11,000T06:31:00,19-Feb-11,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template A2: ISS dwells at begin and end.,,,,,, 2011-050T04:04:11,000T06:31:00,19-Feb-11,ISS,,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-050T04:04:11,000T06:31:00,19-Feb-11,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 31 deg. SSC Lat/Lon = 0.012S/347.206 deg. SS Lat/Lon = 8.322N/317.230 deg. Alt = 238673 km, range = 241248 km. Resolution = 119 km/px. Temp. A2.",,,,,, 2011-050T04:04:11,000T16:26:49,19-Feb-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-050T04:04:11,000T00:34:44,19-Feb-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-050T04:38:55,000T15:52:05,19-Feb-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-050T09:26:00,000T11:05:00,19-Feb-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-050T11:31:00,000T09:00:00,19-Feb-11,RSS,SPASS Rider,Titan,KADOWN,RSS Ka-Band downlink,GSE pass for Titan's gravity,Additional downlink pass at Ka-band for Titan's gravity science and for improving locally Cassini orbit.,,,,,, 2011-050T11:31:00,000T09:00:00,19-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-050T12:06:59,002T03:14:00,19-Feb-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.988849 Rs exit= 13.987865 Range altitude= 3607.5046 km ... 1228.0865,,,,,, 2011-050T12:31:00,000T08:00:00,19-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11050_SP,rider,,,,,, 2011-050T20:31:00,000T07:09:00,19-Feb-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-050T20:31:00,000T01:29:00,19-Feb-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-050T20:31:00,000T07:07:55,19-Feb-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-050T20:31:00,000T00:40:00,19-Feb-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-050T20:31:00,002T10:00:00,19-Feb-11,MIMI,Non-SPASS,co-rotation,PERIAPSOV,,MAPS Periapsis Pie Campaign Overlay,Overlay: adding 950 bps overlay to bring data rate to 1800 for MIMI for MAPS Periapsis PIE,,,,,, 2011-050T20:31:00,001T21:31:00,19-Feb-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-050T21:11:00,000T22:10:00,19-Feb-11,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2011-050T22:00:00,001T07:25:00,19-Feb-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-051T00:00:00,001T06:00:00,20-Feb-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-051T03:38:00,000T02:00:00,20-Feb-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-051T03:38:55,000T00:30:00,20-Feb-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-051T03:40:00,000T02:00:00,20-Feb-11,CDA,Prime,DustRAM direction,RPX0070,,CDA RPXing 2011-051T04:39:59,RPXing at 7.2060720 Rs,,,,,, 2011-051T04:08:55,000T01:30:00,20-Feb-11,INMS,SPASS Rider,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-051T05:38:55,000T23:00:00,20-Feb-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-051T05:40:00,000T13:41:00,20-Feb-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-051T13:43:58,000T00:00:01,20-Feb-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.712 Rs, lat = -0 deg, phase = 97 deg",,,,,, 2011-051T19:21:00,000T11:50:00,20-Feb-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-051T21:31:00,000T09:00:00,20-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-051T22:31:00,000T08:00:00,20-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11051_SP,rider,,,,,, 2011-052T04:38:55,001T01:52:05,21-Feb-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-052T05:25:00,000T08:17:00,21-Feb-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-052T06:31:00,000T02:00:00,21-Feb-11,CDA,Prime,DustRAM direction,RPX0080,,CDA RPXing 2011-052T07:31:59,RPXing at 10.869244 Rs,,,,,, 2011-052T06:32:00,000T02:00:00,21-Feb-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-052T07:11:00,000T09:19:00,21-Feb-11,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2011-052T12:31:00,000T03:59:00,21-Feb-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-052T13:42:00,000T02:48:00,21-Feb-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-052T15:20:59,012T21:18:01,21-Feb-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.000563 Rs exit= 14.008117 Range altitude= 1233.2287 km ... 3604.0107,,,,,, 2011-052T16:30:00,000T05:01:00,21-Feb-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,This is a PIE. One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-052T16:30:00,000T14:01:00,21-Feb-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-052T16:30:00,000T14:01:00,21-Feb-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-052T18:02:00,000T12:29:00,21-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-052T21:31:00,000T09:00:00,21-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-052T22:31:00,000T08:00:00,21-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11052_SP,rider,,,,,, 2011-053T06:31:00,013T06:31:00,22-Feb-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-053T06:31:00,000T02:06:00,22-Feb-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-053T06:31:00,011T08:56:00,22-Feb-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-053T06:31:00,009T06:46:00,22-Feb-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-053T07:11:00,000T03:00:00,22-Feb-11,ISS,Prime,Other,SIAPHA,,Siarnaq,Observation of irregular moon of Saturn.,,,,,, 2011-053T07:11:00,000T03:00:00,22-Feb-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-053T08:37:00,000T02:00:00,22-Feb-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-053T10:11:00,000T10:25:00,22-Feb-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-053T10:37:00,000T19:39:00,22-Feb-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-053T21:16:00,000T09:00:00,22-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-053T22:16:00,000T08:00:00,22-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11053_SP,rider,,,,,, 2011-054T06:16:00,007T07:01:00,23-Feb-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-054T06:56:00,000T14:11:00,23-Feb-11,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T Map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-054T21:07:00,000T05:00:00,23-Feb-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-054T21:07:00,000T05:00:00,23-Feb-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-055T00:00:00,000T01:08:00,24-Feb-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-055T02:07:00,000T06:00:00,24-Feb-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-055T02:07:00,000T06:00:00,24-Feb-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT ridealong,CIRS COMPSIT Ridealong for 6 hrs,,,,,, 2011-055T02:07:00,000T06:00:00,24-Feb-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-055T08:07:00,000T05:00:00,24-Feb-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-055T08:07:00,000T05:00:00,24-Feb-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-055T13:07:00,000T06:00:00,24-Feb-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-055T13:07:00,000T06:00:00,24-Feb-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT ridealong,CIRS COMPSIT Ridealong for 6 hrs,,,,,, 2011-055T13:07:00,000T06:00:00,24-Feb-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-055T21:17:00,000T09:00:00,24-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-055T22:17:00,000T08:00:00,24-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11055_SP,rider,,,,,, 2011-056T06:57:00,000T01:30:00,25-Feb-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 70.7 requested range 3.2 Mkm",,,,,, 2011-056T06:57:00,000T01:30:00,25-Feb-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-056T06:57:00,000T01:30:00,25-Feb-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 71 deg, range = 3.2 Mkm.",,,,,, 2011-056T08:27:00,000T05:00:00,25-Feb-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-056T08:27:00,000T05:00:00,25-Feb-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-056T13:27:00,000T06:00:00,25-Feb-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-056T13:27:00,000T06:00:00,25-Feb-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-056T19:27:00,000T05:00:00,25-Feb-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-056T19:27:00,000T05:00:00,25-Feb-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-057T00:27:00,000T02:00:00,26-Feb-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-057T00:27:00,000T02:00:00,26-Feb-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT ridealong,CIRS COMPSIT Ridealong for 2 hrs,,,,,, 2011-057T00:27:00,000T06:00:00,26-Feb-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-057T02:27:00,000T05:00:00,26-Feb-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-057T02:27:00,000T05:00:00,26-Feb-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-057T07:27:00,000T06:00:00,26-Feb-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-057T11:27:00,000T06:00:00,26-Feb-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-057T13:27:00,000T05:00:00,26-Feb-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-057T13:27:00,000T05:00:00,26-Feb-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-057T21:02:00,000T09:00:00,26-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-057T22:02:00,000T08:00:00,26-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11057_SP,rider,,,,,, 2011-058T06:42:00,000T01:30:00,27-Feb-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 86.8 requested range 3.1 Mkm",,,,,, 2011-058T06:42:00,000T01:30:00,27-Feb-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-058T06:42:00,000T01:30:00,27-Feb-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 87 deg, range = 3.1 Mkm.",,,,,, 2011-058T08:12:00,000T10:40:00,27-Feb-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-058T18:52:00,000T11:50:00,27-Feb-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-058T21:02:00,000T09:00:00,27-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-058T22:02:00,000T08:00:00,27-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11058_SP,rider,,,,,, 2011-059T06:42:00,000T11:00:00,28-Feb-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-059T06:42:00,000T11:00:00,28-Feb-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT ridealong,CIRS COMPSIT Ridealong for 11 hrs,,,,,, 2011-059T06:42:00,000T11:00:00,28-Feb-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-059T20:12:00,000T09:35:00,28-Feb-11,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,"HGA Boresight Calibration. Pointing=XBAND to Earth + crosshair maneuver. Telemetry OFF, TWNC ON for 1-hr calibration from 2011-059T22:17:00 to 2011-059T23:17:00. Required to be tracked by DSS-55 (or DSS-54). Keep Ka-band ON until EOT at 2011-060T05:47:00. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2011-059T20:47:00,000T09:00:00,28-Feb-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-059T21:47:00,000T08:00:00,28-Feb-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11059_SP,rider,,,,,, 2011-059T22:17:00,000T01:00:00,28-Feb-11,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,"HGA Boresight Calibration. Pointing=XBAND to Earth + crosshair maneuver. Telemetry OFF, TWNC ON for 1-hr calibration from 2011-059T22:17:00 to 2011-059T23:17:00. Required to be tracked by DSS-55 (or DSS-54). Keep Ka-band ON until EOT at 2011-060T05:47:00. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2011-060T06:27:00,000T21:10:00,1-Mar-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn MIRMAP,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-060T06:27:00,000T21:10:00,1-Mar-11,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP ridealong,CIRS MIRMAP Ridealong for 21 hrs,,,,,, 2011-061T04:17:00,000T09:00:00,2-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-061T05:17:00,000T08:00:00,2-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11061_SP,rider,,,,,, 2011-061T13:17:00,001T00:00:00,2-Mar-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-061T13:57:00,000T13:40:00,2-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-062T04:17:00,000T09:00:00,3-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-062T05:17:00,000T08:00:00,3-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11062_SP,rider,,,,,, 2011-062T12:39:00,000T20:00:00,3-Mar-11,CDA,SPASS Rider,DustRAM direction,ISD0026,,CDA ISD 2011-065T12:39:00,ISD observation around apoapse 2011-065T12:39:00 54.182163 Rs,,,,,, 2011-062T13:17:00,002T23:22:00,3-Mar-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-062T13:17:00,002T23:22:00,3-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-062T13:57:00,000T01:30:00,3-Mar-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 85.2 requested range 2 Mkm",,,,,, 2011-062T13:57:00,000T01:30:00,3-Mar-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-062T13:57:00,000T01:30:00,3-Mar-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 85 deg, range = 2 Mkm.",,,,,, 2011-062T15:27:00,000T22:00:00,3-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-062T15:27:00,000T22:00:00,3-Mar-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT ridealong,CIRS COMPSIT Ridealong for 22 hrs,,,,,, 2011-062T15:27:00,000T22:00:00,3-Mar-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-063T13:27:00,000T12:40:00,4-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-064T04:17:00,000T09:00:00,5-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-064T05:17:00,000T08:00:00,5-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_145IC_DSCAL11064_SP,rider,,,,,, 2011-064T06:39:00,000T20:00:00,5-Mar-11,CDA,SPASS Rider,DustRAM direction,ISD0026,,CDA ISD 2011-065T12:39:00,ISD observation around apoapse 2011-065T12:39:00 54.182163 Rs,,,,,, 2011-064T13:57:00,000T01:30:00,5-Mar-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 66.8 requested range 2.2 Mkm",,,,,, 2011-064T13:57:00,000T01:30:00,5-Mar-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-064T13:57:00,000T01:30:00,5-Mar-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 67 deg, range = 2.2 Mkm.",,,,,, 2011-064T15:27:00,000T07:00:00,5-Mar-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-064T22:27:00,000T05:00:00,5-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-064T22:27:00,000T05:00:00,5-Mar-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-064T22:27:00,001T14:35:00,5-Mar-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-065T03:27:00,000T06:00:00,6-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-065T03:27:00,000T06:00:00,6-Mar-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-065T09:27:00,000T05:00:00,6-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-065T09:27:00,000T05:00:00,6-Mar-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-065T12:39:00,001T00:23:00,6-Mar-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S67,Range enter= 14.000563 Rs exit= 14.008117 Range altitude= 1233.2287 km ... 3604.0107,,,,,, 2011-065T12:39:00,000T02:00:00,6-Mar-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-065T12:39:00,001T00:23:00,6-Mar-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-065T12:39:00,000T15:23:00,6-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-065T12:39:20,000T00:00:01,6-Mar-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 27.9 d, inc = 0.4 deg, r = 54.127 Rs, phase = 83 deg",,,,,, 2011-065T14:27:00,000T11:00:00,6-Mar-11,ISS,Prime,Saturn,HIRESGLOB,,High resolution color NAC global map,Every 0.5 hour a 6x1 North to South mosaic of the illuminated half of Saturn spending ~ 10 minutes on this mosaic and then wait/stare. CB2 GRN BL1 NAC and once per mosaic CB2 WAC,,,,,, 2011-065T14:27:00,000T11:00:00,6-Mar-11,CIRS,,Saturn,HIRESGLOB,,Saturn apoapsis COMPSIT in between ISS mosaics,,,,,,, 2011-065T14:27:00,000T06:00:00,6-Mar-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-065T14:39:00,000T22:23:00,6-Mar-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-065T22:39:00,000T14:23:00,6-Mar-11,CDA,SPASS Rider,DustRAM direction,ISD0026,,CDA ISD 2011-065T12:39:00 End: S67,ISD observation around apoapse 2011-065T12:39:00 54.182163 Rs,,,,,, 2011-066T04:02:00,000T09:00:00,7-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-066T04:02:00,000T09:00:00,7-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-066T05:02:00,000T08:00:00,7-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11066_SP,rider,,,,,, 2011-066T13:02:00,000T05:37:00,7-Mar-11,CDA,SPASS Rider,DustRAM direction,ISD0026,,CDA ISD 2011-065T12:39:00 Enter: S67,ISD observation around apoapse 2011-065T12:39:00 54.182163 Rs,,,,,, 2011-066T13:02:00,014T15:31:00,7-Mar-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-066T13:02:00,011T21:04:59,7-Mar-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S67,Range enter= 14.000563 Rs exit= 14.008117 Range altitude= 1233.2287 km ... 3604.0107,,,,,, 2011-066T13:02:00,000T00:43:00,7-Mar-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-066T13:02:00,002T17:58:00,7-Mar-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-066T13:02:00,014T15:31:00,7-Mar-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_146",,,,,, 2011-066T13:02:00,001T15:01:00,7-Mar-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 250 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-066T13:02:00,003T14:46:00,7-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-066T13:07:00,000T00:02:00,7-Mar-11,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S67 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2011-066T13:45:00,000T00:07:00,7-Mar-11,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-066T13:48:00,000T01:30:00,7-Mar-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 62.3 requested range 2.9 Mkm",,,,,, 2011-066T13:48:00,000T01:30:00,7-Mar-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-066T13:48:00,000T01:30:00,7-Mar-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 62 deg, range = 2.9 Mkm.",,,,,, 2011-066T13:52:00,000T00:05:00,7-Mar-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-066T13:57:00,000T00:33:00,7-Mar-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-066T14:30:00,000T00:30:00,7-Mar-11,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2011-066T15:00:00,003T09:00:00,7-Mar-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-066T15:18:00,000T18:35:00,7-Mar-11,ISS,Prime,Saturn,SATMONIT,,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-067T09:53:00,000T16:00:00,8-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-067T09:53:00,000T16:00:00,8-Mar-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-067T16:39:00,000T20:00:00,8-Mar-11,CDA,SPASS Rider,DustRAM direction,ISD0026,,CDA ISD 2011-065T12:39:00,ISD observation around apoapse 2011-065T12:39:00 54.182163 Rs,,,,,, 2011-068T04:03:00,000T09:00:00,9-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-068T05:03:00,000T08:00:00,9-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11068_SP,rider,,,,,, 2011-068T13:43:00,000T01:30:00,9-Mar-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 69.5 requested range 3.6 Mkm",,,,,, 2011-068T13:43:00,000T01:30:00,9-Mar-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-068T13:43:00,000T01:30:00,9-Mar-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 70 deg, range = 3.6 Mkm.",,,,,, 2011-068T15:13:00,000T05:00:00,9-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-068T15:13:00,000T05:00:00,9-Mar-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Winds Ride-along,Wind observations Ride-along with ISS,,,,,, 2011-068T15:13:00,000T05:00:00,9-Mar-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-068T20:13:00,000T06:00:00,9-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-069T02:13:00,000T05:00:00,10-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-069T02:13:00,000T05:00:00,10-Mar-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Winds Ride-along,Wind observations Ride-along with ISS,,,,,, 2011-069T02:13:00,000T05:00:00,10-Mar-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-069T07:00:00,011T21:33:00,10-Mar-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-069T07:13:00,000T05:00:00,10-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-069T07:13:00,000T05:00:00,10-Mar-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Winds Ride-along,Wind observations Ride-along with ISS,,,,,, 2011-069T07:13:00,000T05:00:00,10-Mar-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-069T12:13:00,000T06:00:00,10-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-069T18:13:00,000T05:00:00,10-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-069T18:13:00,000T05:00:00,10-Mar-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Winds Ride-along,Wind observations Ride-along with ISS,,,,,, 2011-069T18:13:00,000T05:00:00,10-Mar-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-070T00:00:00,000T01:08:00,11-Mar-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-070T00:00:00,000T00:34:00,11-Mar-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-070T00:34:00,008T02:02:56,11-Mar-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-070T03:48:00,000T09:00:00,11-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-070T03:48:00,000T09:00:00,11-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-070T04:48:00,000T08:00:00,11-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11070_SP,rider,,,,,, 2011-070T12:00:00,001T06:00:00,11-Mar-11,CDA,Non-SPASS,Other,DECON,Decontamination,Decon Activity,"usual decon activity occuring roughly every 3 months - 6Ext_Mem_Load Cmd will occur at 2011-070T14:00. That's roughly one hour after the D/L having ZERO carryover. So, expectations is that there is no issue due to SSR swap and FSW-Load from SSR. Activity do NOT need any additional DV.",,,,,, 2011-070T12:48:00,003T14:45:00,11-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-070T13:28:00,000T01:30:00,11-Mar-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 82.5 requested range 4 Mkm",,,,,, 2011-070T13:28:00,000T01:30:00,11-Mar-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-070T13:28:00,000T01:30:00,11-Mar-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 82 deg, range = 4 Mkm.",,,,,, 2011-070T14:58:00,000T16:00:00,11-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-070T14:58:00,000T16:00:00,11-Mar-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-071T06:58:00,000T11:00:00,12-Mar-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn MIRMAP,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-071T06:58:00,000T11:00:00,12-Mar-11,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ride-along,Ride-along with CIRS MIRMAP,,,,,, 2011-071T17:58:00,000T06:00:00,12-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-071T17:58:00,000T06:00:00,12-Mar-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT Ride-along,Ride-along with CIRS COMPSIT,,,,,, 2011-072T03:33:00,000T09:00:00,13-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-072T04:33:00,000T08:00:00,13-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11072_SP,rider,,,,,, 2011-072T13:13:00,000T05:00:00,13-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-072T13:13:00,000T05:00:00,13-Mar-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-072T18:13:00,000T06:00:00,13-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-072T18:13:00,000T06:00:00,13-Mar-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT Ride-along,Ride-along with CIRS COMPSIT,,,,,, 2011-073T00:13:00,000T05:00:00,14-Mar-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2 (botsim once an hour), MT2, MT3(2x2) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-073T00:13:00,000T05:00:00,14-Mar-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-073T05:13:00,000T06:00:00,14-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-073T05:13:00,000T06:00:00,14-Mar-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT Ride-along,Ride-along with CIRS COMPSIT,,,,,, 2011-073T11:13:00,000T01:40:00,14-Mar-11,ISS,Prime,Saturn,SATMONIT,,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-073T14:23:00,000T11:00:00,14-Mar-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn MIRMAP,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-073T14:23:00,000T11:00:00,14-Mar-11,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ride-along,Ride-along with CIRS MIRMAP,,,,,, 2011-074T03:33:00,007T01:00:00,15-Mar-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 150 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-074T03:33:00,000T09:00:00,15-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-074T03:33:00,000T09:00:00,15-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-074T04:33:00,000T08:00:00,15-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11074_SP,rider,,,,,, 2011-074T12:33:00,003T18:54:00,15-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-074T13:13:00,000T22:00:00,15-Mar-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn MIRMAP,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-074T13:13:00,000T22:00:00,15-Mar-11,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ride-along,Ride-along with CIRS MIRMAP,,,,,, 2011-075T11:53:00,000T13:55:00,16-Mar-11,ISS,Prime,Other,SKAROT,,Skathi,Observation of irregular moon of Saturn.,,,,,, 2011-076T03:18:00,000T09:00:00,17-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-076T04:18:00,000T08:00:00,17-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11076_SP,rider,,,,,, 2011-076T12:58:00,000T16:00:00,17-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-076T12:58:00,000T16:00:00,17-Mar-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-077T04:58:00,000T11:00:00,18-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-077T04:58:00,000T11:00:00,18-Mar-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT Ride-along,Ride-along with CIRS COMPSIT,,,,,, 2011-077T15:58:00,000T09:10:00,18-Mar-11,ISS,Prime,Saturn,NALGTNG,,Lightning search in CL1 in NAC from ~20-30Rs,-35 stare NAC 4x4-summed frames in CL1 CL2,,,,,, 2011-077T15:58:00,000T09:10:00,18-Mar-11,VIMS,SPASS Rider,Saturn,NALGTNG,,ISS Ligtning Ride-along,Ride-along with ISS Lightning,,,,,, 2011-078T02:36:56,000T23:00:00,19-Mar-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-078T04:18:00,000T08:00:00,19-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11078_SP,rider,,,,,, 2011-078T07:27:00,000T04:51:00,19-Mar-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-078T10:06:59,000T15:08:01,19-Mar-11,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 13.995423 Rs exit= 13.992545 Range altitude= 3597.6194 km ... 1243.4029,,,,,, 2011-078T12:18:00,002T03:45:00,19-Mar-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-078T12:58:00,000T05:02:00,19-Mar-11,VIMS,Prime,Saturn,DEEPDYN,,Deep dynamics mosaic for Deep Atmopsheres Campaign,"5 2(rows)x3(columns) Global mosaics, one collected each hour throughout the 5-hrs duration. Mosaic is centered on the equator at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction, with border between them along the equator. 10-minute intervals between frame centers (7 mins for science, 3 for repositioning). Each of these mosaics should take an hour.",,,,,, 2011-078T12:58:00,000T05:02:00,19-Mar-11,CIRS,SPASS Rider,Saturn,DEEPDYN,,VIMS rider for good spatial res obs,rider,,,,,, 2011-078T18:00:00,000T03:00:00,19-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,This is a PIE. One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-078T18:00:00,000T03:00:00,19-Mar-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-078T18:00:00,000T03:00:00,19-Mar-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-078T21:00:00,000T06:00:00,19-Mar-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-079T01:15:00,000T17:15:00,20-Mar-11,CDA,Non-SPASS,Other,RATE080B,,Data rate,Range enter= 13.995423 Rs exit= 13.992545 Range altitude= 3597.6194 km ... 1243.4029,,,,,, 2011-079T01:15:00,000T03:00:00,20-Mar-11,RADAR,Non-SPASS,Other,WU4SAGM,,Warmup for Saturn V/R/V Deep Atmosphere.,Warmup for global map-1 in SWG PIEs.,,,,,, 2011-079T01:36:00,000T02:00:00,20-Mar-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-079T01:36:56,000T00:30:00,20-Mar-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-079T01:37:59,000T02:00:00,20-Mar-11,CDA,SPASS Rider,DustRAM direction,RPX0090,,CDA RPXing 2011-079T02:37:59,RPXing at 7.2295132 Rs,,,,,, 2011-079T02:06:56,000T01:30:00,20-Mar-11,INMS,SPASS Rider,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-079T03:36:00,000T17:24:00,20-Mar-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-079T03:36:56,000T23:00:00,20-Mar-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-079T04:00:00,000T14:15:00,20-Mar-11,RADAR,Prime,Saturn,GLOBALMAP,Global coverage mapping,Saturn V/R/V Deep Atmosphere.,Saturn global map-1 in EQ-PIEs. peri=2011-079T11:45:00; 224268 km.,,,,,, 2011-079T11:45:07,000T00:00:01,20-Mar-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.716 Rs, lat = -0 deg, phase = 98 deg",,,,,, 2011-079T18:30:00,000T18:52:59,20-Mar-11,CDA,Non-SPASS,Other,RATE080C,,Data rate,Range enter= 13.995423 Rs exit= 13.992545 Range altitude= 3597.6194 km ... 1243.4029,,,,,, 2011-079T19:00:00,000T17:45:00,20-Mar-11,VIMS,Prime,Saturn,DEEPDYN,,Deep dynamics mosaic for Deep Atmopsheres Campaign,"17 2(rows)x3(columns) Global mosaics, one collected each hour throughout the first 17-hrs, followed by a final tier of 3 at the end.. Mosaic is centered on the equator at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction, with border between them along the equator. 10-minute intervals between frame centers (7 mins for science, 3 for repositioning). Each of these mosaics should take an hour.",,,,,, 2011-079T19:00:00,000T17:45:00,20-Mar-11,CIRS,SPASS Rider,Saturn,DEEPDYN,,VIMS rider for good spatial res obs,rider,,,,,, 2011-080T02:36:56,001T01:56:04,21-Mar-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-080T04:29:59,000T02:00:00,21-Mar-11,CDA,SPASS Rider,DustRAM direction,RPX0100,,CDA RPXing 2011-080T05:29:59,RPXing at 10.847353 Rs,,,,,, 2011-080T12:45:00,000T04:38:00,21-Mar-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,This is a PIE. One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-080T12:45:00,000T04:38:00,21-Mar-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-080T12:45:00,000T04:38:00,21-Mar-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-080T13:22:59,012T21:28:01,21-Mar-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.005239 Rs exit= 14.002102 Range altitude= 1248.5606 km ... 3597.5935,,,,,, 2011-080T16:03:00,000T03:30:00,21-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-080T19:33:00,000T09:00:00,21-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-080T20:33:00,000T08:00:00,21-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11080_SP,rider,,,,,, 2011-081T04:33:00,015T12:45:00,22-Mar-11,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2011-081T04:33:00,000T01:27:00,22-Mar-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-081T04:33:00,011T21:00:00,22-Mar-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-081T04:33:00,012T06:18:00,22-Mar-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-081T04:33:00,012T06:18:00,22-Mar-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-081T05:13:00,000T11:20:00,22-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-081T06:00:00,000T02:00:00,22-Mar-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-081T08:00:00,012T02:51:00,22-Mar-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-081T16:33:00,000T13:00:00,22-Mar-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-082T05:33:00,000T02:15:00,23-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-082T09:18:00,000T09:00:00,23-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-082T10:18:00,000T08:00:00,23-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11082_SP,rider,,,,,, 2011-082T18:18:00,000T12:00:00,23-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-083T06:18:00,000T13:00:00,24-Mar-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-083T19:18:00,000T12:15:00,24-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-084T07:33:00,000T10:30:00,25-Mar-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-084T09:03:00,000T09:00:00,25-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-084T10:03:00,000T08:00:00,25-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11084_SP,rider,,,,,, 2011-084T18:03:00,000T08:00:00,25-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-085T00:00:00,000T01:08:00,26-Mar-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-085T02:03:00,000T04:00:00,26-Mar-11,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2011-085T02:03:00,000T04:00:00,26-Mar-11,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2011-085T06:03:00,000T13:00:00,26-Mar-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-085T19:03:00,000T12:30:00,26-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-086T09:03:00,000T09:00:00,27-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-086T10:03:00,000T08:00:00,27-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11086_SP,rider,,,,,, 2011-086T18:03:00,000T12:00:00,27-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-087T06:03:00,000T13:00:00,28-Mar-11,CAPS,Prime,Earth,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-087T19:03:00,000T12:15:00,28-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-088T08:48:00,000T09:00:00,29-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-088T09:48:00,000T08:00:00,29-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11088_SP,rider,,,,,, 2011-088T17:48:00,000T01:30:00,29-Mar-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 81.5 requested range 4 Mkm",,,,,, 2011-088T17:48:00,000T01:30:00,29-Mar-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-088T17:48:00,000T01:30:00,29-Mar-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 82 deg, range = 4 Mkm.",,,,,, 2011-088T19:18:00,000T15:00:00,29-Mar-11,CAPS,Prime,co-rotation,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-089T10:18:00,000T06:00:00,30-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-089T16:18:00,000T15:00:00,30-Mar-11,ISS,Prime,Other,SKAROT,,Skathi,Observation of irregular moon of Saturn.,,,,,, 2011-090T08:48:00,000T09:00:00,31-Mar-11,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2011-090T08:48:00,000T09:00:00,31-Mar-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-090T09:48:00,000T08:00:00,31-Mar-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11090_SP,rider,,,,,, 2011-090T10:51:00,000T20:00:00,31-Mar-11,CDA,SPASS Rider,DustRAM direction,ISD0027,,CDA ISD 2011-093T10:51:00,ISD observation around apoapse 2011-093T10:51:00 54.182708 Rs,,,,,, 2011-090T17:48:00,000T05:15:00,31-Mar-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-090T23:03:00,000T17:00:00,31-Mar-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-090T23:03:00,000T17:00:00,31-Mar-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-091T16:03:00,000T15:00:00,1-Apr-11,CAPS,Prime,co-rotation,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-092T04:51:00,000T20:00:00,2-Apr-11,CDA,SPASS Rider,DustRAM direction,ISD0027,,CDA ISD 2011-093T10:51:00,ISD observation around apoapse 2011-093T10:51:00 54.182708 Rs,,,,,, 2011-092T08:33:00,000T09:00:00,2-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-092T09:33:00,000T08:00:00,2-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_146IC_DSCAL11092_SP,rider,,,,,, 2011-093T01:33:00,000T07:00:00,3-Apr-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-093T08:33:00,000T17:00:00,3-Apr-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-093T08:33:00,000T17:00:00,3-Apr-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-093T08:33:00,000T05:00:00,3-Apr-11,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2011-093T10:51:00,012T21:17:59,3-Apr-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.005239 Rs exit= 14.002102 Range altitude= 1248.5606 km ... 3597.5935,,,,,, 2011-093T10:51:00,000T02:00:00,3-Apr-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-093T10:51:00,014T23:27:00,3-Apr-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-093T10:51:00,003T06:27:00,3-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-093T10:51:20,000T00:00:01,3-Apr-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 27.9 d, inc = 0.4 deg, r = 54.127 Rs, phase = 82 deg",,,,,, 2011-093T12:51:00,012T01:39:00,3-Apr-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-093T13:33:00,012T13:15:00,3-Apr-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-093T20:51:00,000T20:00:00,3-Apr-11,CDA,SPASS Rider,DustRAM direction,ISD0027,,CDA ISD 2011-093T10:51:00,ISD observation around apoapse 2011-093T10:51:00 54.182708 Rs,,,,,, 2011-094T01:33:00,000T05:30:00,4-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-094T08:33:00,000T09:00:00,4-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-094T09:33:00,000T08:00:00,4-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11094_SP,rider,,,,,, 2011-094T17:33:00,000T15:00:00,4-Apr-11,CAPS,Prime,co-rotation,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-095T08:33:00,000T17:00:00,5-Apr-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-095T08:33:00,000T17:00:00,5-Apr-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-095T14:51:00,000T20:00:00,5-Apr-11,CDA,SPASS Rider,DustRAM direction,ISD0027,,CDA ISD 2011-093T10:51:00,ISD observation around apoapse 2011-093T10:51:00 54.182708 Rs,,,,,, 2011-096T01:33:00,000T05:15:00,6-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-096T08:18:00,000T09:00:00,6-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-096T09:18:00,000T08:00:00,6-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11096_SP,rider,,,,,, 2011-096T17:18:00,000T01:30:00,6-Apr-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 75.4 requested range 2 Mkm",,,,,, 2011-096T17:18:00,000T01:30:00,6-Apr-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-096T17:18:00,000T01:30:00,6-Apr-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 75 deg, range = 2 Mkm.",,,,,, 2011-096T17:18:00,003T17:30:00,6-Apr-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-096T17:18:00,007T23:30:00,6-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-096T18:48:00,000T12:30:00,6-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-097T07:18:00,000T17:00:00,7-Apr-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-097T07:18:00,000T17:00:00,7-Apr-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-098T01:48:00,000T09:00:00,8-Apr-11,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2011-098T01:48:00,000T09:00:00,8-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-098T02:48:00,000T08:00:00,8-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11098_SP,rider,,,,,, 2011-098T10:48:00,000T15:00:00,8-Apr-11,CAPS,Prime,co-rotation,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-099T01:48:00,000T17:00:00,9-Apr-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-099T01:48:00,000T17:00:00,9-Apr-11,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2011-099T01:48:00,000T17:00:00,9-Apr-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-099T18:48:00,000T05:30:00,9-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-100T00:00:00,000T01:08:00,10-Apr-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-100T01:48:00,000T09:00:00,10-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-100T02:48:00,000T08:00:00,10-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11100_SP,rider,,,,,, 2011-100T10:48:00,000T11:00:00,10-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-100T10:48:00,005T18:42:00,10-Apr-11,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2011-100T21:48:00,000T15:00:00,10-Apr-11,CAPS,Prime,co-rotation,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-101T12:48:00,000T11:15:00,11-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-102T01:33:00,000T09:00:00,12-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-102T02:33:00,000T08:00:00,12-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11102_SP,rider,,,,,, 2011-102T10:33:00,000T01:30:00,12-Apr-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 87.8 requested range 3.2 Mkm",,,,,, 2011-102T10:33:00,000T01:30:00,12-Apr-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-102T10:33:00,000T01:30:00,12-Apr-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 88 deg, range = 3.2 Mkm.",,,,,, 2011-102T12:03:00,000T12:00:00,12-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-103T01:33:00,000T09:00:00,13-Apr-11,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2011-103T01:33:00,000T09:00:00,13-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-103T02:33:00,000T08:00:00,13-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11103_SP,rider,,,,,, 2011-103T10:33:00,000T15:00:00,13-Apr-11,CAPS,Prime,co-rotation,LLAROLPTG,,MAPS low latitude apoapsis w/ prime pointing,null,,,,,, 2011-104T01:33:00,000T04:45:00,14-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-104T07:48:00,000T09:00:00,14-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-104T08:48:00,000T08:00:00,14-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11104_SP,rider,,,,,, 2011-104T16:48:00,000T05:47:00,14-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-104T16:48:00,001T12:40:00,14-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-105T00:05:00,000T05:55:00,15-Apr-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-105T06:00:00,000T11:23:00,15-Apr-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-105T06:00:00,000T11:23:00,15-Apr-11,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2011-105T06:00:00,000T11:30:00,15-Apr-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-105T14:30:00,000T02:00:00,15-Apr-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-105T16:30:00,000T10:18:00,15-Apr-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-105T17:48:00,000T09:00:00,15-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-105T18:48:00,000T08:00:00,15-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11105_SP,rider,,,,,, 2011-106T02:48:00,000T09:00:00,16-Apr-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere prime pointing,null,,,,,, 2011-106T02:48:00,000T20:48:47,16-Apr-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-106T02:48:00,000T02:22:00,16-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-106T05:10:00,000T11:58:00,16-Apr-11,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2011-106T05:28:00,002T04:50:00,16-Apr-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-106T05:30:00,002T00:48:00,16-Apr-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-106T08:08:59,002T03:14:00,16-Apr-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.989404 Rs exit= 13.988790 Range altitude= 3591.1961 km ... 1263.7245,,,,,, 2011-106T17:08:00,000T10:20:00,16-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-106T17:48:00,000T09:00:00,16-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-106T18:48:00,000T08:00:00,16-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11106_SP,rider,,,,,, 2011-106T23:36:00,000T02:00:00,16-Apr-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-106T23:36:47,000T00:30:00,16-Apr-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-106T23:37:59,000T02:00:00,16-Apr-11,CDA,SPASS Rider,DustRAM direction,RPX0110,,CDA RPXing 2011-107T00:37:59,RPXing at 7.2336422 Rs,,,,,, 2011-107T00:00:00,001T00:00:00,17-Apr-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-107T00:06:47,000T01:30:00,17-Apr-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-107T01:36:47,000T01:11:13,17-Apr-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-107T02:48:00,000T04:00:00,17-Apr-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere prime pointing,null,,,,,, 2011-107T02:48:00,000T21:48:47,17-Apr-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-107T03:28:00,000T06:30:00,17-Apr-11,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2011-107T06:48:00,000T02:30:00,17-Apr-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere prime pointing,null,,,,,, 2011-107T09:45:58,000T00:00:01,17-Apr-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.711 Rs, lat = -0 deg, phase = 98 deg",,,,,, 2011-107T09:58:00,000T02:30:00,17-Apr-11,VIMS,Prime,Saturn,ALPCMIOCC,Alpha CMI occultation,alpCMi Saturn occultation,"alpCMi atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. After the occ, at time 11:02, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation occurred (latitude 33.5N).",,,,,, 2011-107T09:58:00,000T02:30:00,17-Apr-11,CIRS,,Saturn,ALPCMIOCC,Alpha CMI occultation,CIRS_147SA_ALPCMIOCC001_VIMS,Collab with VIMS. Stellar Occ Saturn ingress T10:41 35N dark limb,,,,,, 2011-107T09:58:00,001T00:20:00,17-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-107T12:28:00,000T10:40:00,17-Apr-11,UVIS,Prime,Saturn,AURORA,Saturn aurora,Saturn Aurora,"Target Saturn's auroral zone at high latitude. Make repeated slow continuous slews across the auroral zone, with a flyback between slow slews. J.C Gerard would like the target to be the north aurora.",,,,,, 2011-107T12:28:00,000T10:40:00,17-Apr-11,CIRS,SPASS Rider,Saturn,AURORA,Saturn aurora,,null,,,,,, 2011-107T12:28:00,000T10:40:00,17-Apr-11,VIMS,SPASS Rider,Saturn,AURORA,Saturn aurora,UVIS Auroral Ridealong,Auroral UVIS Ridealong,,,,,, 2011-108T00:36:47,000T09:41:13,18-Apr-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-108T01:18:00,000T09:00:00,18-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-108T02:18:00,000T08:00:00,18-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11108_SP,rider,,,,,, 2011-108T02:25:59,000T02:00:00,18-Apr-11,CDA,SPASS Rider,DustRAM direction,RPX0120,,CDA RPXing 2011-108T03:25:59,RPXing at 10.814206 Rs,,,,,, 2011-108T06:18:00,000T04:00:00,18-Apr-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-108T10:18:00,000T00:40:00,18-Apr-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-108T10:18:00,000T06:42:39,18-Apr-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-108T10:18:00,000T14:42:39,18-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-108T10:18:00,002T23:45:00,18-Apr-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_147_T75",,,,,, 2011-108T10:18:00,000T03:46:00,18-Apr-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-108T10:58:00,000T17:02:39,18-Apr-11,CAPS,SPASS Rider,Titan,T75INBND,,Inbound 147TI (T75),null,,,,,, 2011-108T11:13:00,000T20:17:39,18-Apr-11,CAPS,Prime,Titan,T75PTG,,Titan Encounter,null,,,,,, 2011-108T11:13:00,000T20:17:39,18-Apr-11,CIRS,SPASS Rider,Titan,T75PTG,,,Rider along with CAPS flyby.,,,,,, 2011-108T11:22:59,007T04:40:01,18-Apr-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo End: S68,Range enter= 14.001492 Rs exit= 14.011283 Range altitude= 1268.9020 km ... 4042.2535,,,,,, 2011-108T14:04:00,002T19:59:00,18-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-108T17:00:39,000T11:00:00,18-Apr-11,INMS,Non-SPASS,Saturn,T75INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-109T01:00:39,000T08:00:00,19-Apr-11,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T75 flyby,"T75 is a post-dusk, high altitude (9995 km) equatorial flyby across Titan's induced magnetic tail downstream from the moon. As in previous flyby T9, the geometry for T75 is ideal to study the structure of the magnetotail and possibly the current sheet that separates its two lobes. Adequate pointing from CAPS will lead to important measurements of the ion and electron species escaping from the moon as a result of its interaction with Saturn's magnetospheric flow. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2011-109T03:00:39,000T01:00:00,19-Apr-11,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-109T03:00:39,000T01:00:00,19-Apr-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-109T04:00:39,000T02:00:00,19-Apr-11,CAPS,SPASS Rider,Titan,T75CLOSE,,Closest Approach 147TI (T75),null,,,,,, 2011-109T04:00:39,000T02:00:00,19-Apr-11,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-109T04:00:39,000T02:00:00,19-Apr-11,INMS,Non-SPASS,Titan,TITAN75,,Titan Flyby,Titan observation,,,,,, 2011-109T04:00:39,000T02:00:00,19-Apr-11,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2011-109T06:00:39,000T01:00:00,19-Apr-11,CAPS,SPASS Rider,Titan,T75OUTBND,,Outbound 147TI (T75),null,,,,,, 2011-109T06:00:39,000T01:00:00,19-Apr-11,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-109T06:00:39,000T11:00:00,19-Apr-11,INMS,Non-SPASS,Saturn,T75OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-109T06:00:39,000T01:00:00,19-Apr-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-109T07:00:39,002T03:02:21,19-Apr-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-109T07:30:39,000T06:30:00,19-Apr-11,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2011-109T07:30:39,000T06:30:00,19-Apr-11,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2011-109T07:30:39,000T06:30:00,19-Apr-11,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-109T07:30:39,000T06:30:00,19-Apr-11,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 26 deg, SSC Lat/Lon = 0.015N/185.866 W deg, SS Lat/Lon = 9.157N/210.721 W deg. Alt = 48263 km. Range = 50838 km. Resolution = 24 km/px. Temp. X",,,,,, 2011-109T09:00:39,002T01:02:21,19-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-109T14:00:39,000T08:37:21,19-Apr-11,UVIS,Prime,Titan,HDACSTARE,,HDAC observation of Titan (stare),HDAC observation of Titan (stare). EUV and FUV will also be taking data with the setup like the setup for EUVFUV,,,,,, 2011-109T14:00:39,000T08:37:21,19-Apr-11,CIRS,SPASS Rider,Titan,HDACSTARE,,,Ride along with UVIS.,,,,,, 2011-109T14:00:39,000T08:37:21,19-Apr-11,ISS,SPASS Rider,Titan,HDACSTARE,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-109T14:00:39,000T08:37:21,19-Apr-11,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 17 deg, SSC Lat/Lon = 0.005N/202.302 W deg, SS Lat/Lon = 9.160N/216.832 W deg. Alt = 175394 km. Range = 177969 km. Resolution = 88 km/px. Temp. X extended.",,,,,, 2011-109T17:00:39,001T17:02:21,19-Apr-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-110T01:03:00,000T09:00:00,20-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-110T02:03:00,000T08:00:00,20-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11110_SP,rider,,,,,, 2011-110T10:03:02,000T05:39:58,20-Apr-11,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2011-110T10:43:00,000T05:00:00,20-Apr-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-110T10:43:00,000T05:00:00,20-Apr-11,CIRS,SPASS Rider,Titan,CLOUD,,ISS rider Titan low phase,Rider to ISS Titan cloud monitor,,,,,, 2011-110T10:43:00,000T05:00:00,20-Apr-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"Titan Cloud Monitoring; phase = 24 deg, SSC Lat/Lon = 0.004N/204.432 deg. SS Lat/Lon = 9.161/218.398 deg. Alt = 208513 km, range = 211088 km. Resolution = 104 km/px. Obtain cubes for cloud mapping during caboose segment.",,,,,, 2011-110T15:43:00,000T02:00:00,20-Apr-11,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2011-110T17:43:00,000T05:00:00,20-Apr-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-110T17:43:00,000T05:00:00,20-Apr-11,CIRS,SPASS Rider,Titan,CLOUD,,ISS rider Titan low phase,Rider to ISS Titan cloud monitor,,,,,, 2011-110T17:43:00,000T05:00:00,20-Apr-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"Titan Cloud Monitoring; phase = 14 deg, SSC Lat/Lon = 0.003N/211.877 deg. SS Lat/Lon = 9.164/224.978 deg. Alt = 349699 km, range = 352274 km. Resolution = 175 km/px. Obtain cubes for cloud mapping during caboose segment.",,,,,, 2011-110T23:33:00,000T10:30:00,20-Apr-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-111T01:03:00,000T09:00:00,21-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-111T02:03:00,000T08:00:00,21-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11111_SP,rider,,,,,, 2011-111T10:03:00,004T05:59:59,21-Apr-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-111T10:03:00,000T23:45:00,21-Apr-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-111T10:03:00,002T06:45:00,21-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-111T10:03:00,004T06:00:00,21-Apr-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_147",,,,,, 2011-111T10:03:00,000T03:00:00,21-Apr-11,RADAR,Non-SPASS,Other,WU4ENGTST,RADAR engineering test warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2011-111T10:03:00,004T06:00:00,21-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-111T13:03:00,000T02:00:00,21-Apr-11,RADAR,Prime,Saturn,ENGTEST,Engineering test,Engineering Test of Diagnostic Modes,Engineering test of diagnostic modes on the flight unit.,,,,,, 2011-111T16:00:00,000T08:00:00,21-Apr-11,CIRS,Prime,Other,STRALTCAL,Stray light calibration,CIRS_REV_147_SCATTERED_SUNLIGHT_TEST_PRIME,"Monitor scattered IR solar radiation as a function of offset angle from the sun using radial scans. CIRS to operate at 15.5 cm-1 resolution (4.825 sec/frame, 39 RTI), detector pairs, FP4. FPB scans will begin TBD degrees from Sun, and will scan to 12 degrees of Sun at TBD rate; Scan will stop every 10 degrees for TBD seconds; (the procedure will be repeated in the reverse direction back to the initial position;) to determine whether scattering is asymmetric with respect to the FPB axis, additional scans will be made. . . . . REDESIGN NEEDED HERE . . . 1) From just to the -X side of the Z axis (to protect the radiator), the first scan will be from TBD degrees +Z to 12 degrees +Z and back to 40 degrees +Z. 2) From TBD degrees in -X on the X axis, to 12 degrees on the -X axis, to TBD degrees on the -X axis. 3) From just to the -X side of the -Z axis (to protect the radiator), scan from 40 degrees -Z to 12 degrees -Z and back to TBD degrees -Z. ACTUALLY: IN, UP, DOWN, DOWN, UP, BACK WILL DO: || || || || || || || ||||| ||||||||||||||||| * ||||| || || || || || || ||",,,,,, 2011-112T00:48:00,000T09:00:00,22-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-112T01:48:00,000T08:00:00,22-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11112_SP,rider,,,,,, 2011-112T09:48:00,001T00:00:00,22-Apr-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-112T11:00:00,000T01:00:00,22-Apr-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-112T12:00:00,000T11:00:00,22-Apr-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-113T00:48:00,000T09:00:00,23-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-113T01:48:00,000T08:00:00,23-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11113_SP,rider,,,,,, 2011-113T09:48:00,001T19:45:00,23-Apr-11,CDA,Prime,DustRAM direction,ISD0028,,CDA ISD 2011-119T03:06:00,ISD observation around apoapse 2011-119T03:06:00 48.264302 Rs,,,,,, 2011-113T09:48:00,002T06:15:00,23-Apr-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-113T16:48:00,001T23:15:00,23-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-115T00:00:00,000T01:08:00,25-Apr-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-115T07:03:00,000T09:00:00,25-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-115T08:03:00,000T08:00:00,25-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11115_SP,rider,,,,,, 2011-115T16:03:00,012T16:43:59,25-Apr-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-115T16:03:00,003T11:03:00,25-Apr-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo Enter: S68,Range enter= 14.001492 Rs exit= 14.011283 Range altitude= 1268.9020 km ... 4042.2535,,,,,, 2011-115T16:03:00,000T00:43:00,25-Apr-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-115T16:03:00,001T20:57:00,25-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-115T16:03:00,003T11:03:00,25-Apr-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_147_148",,,,,, 2011-115T16:03:00,003T11:03:00,25-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-115T16:08:00,000T00:02:00,25-Apr-11,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S68 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2011-115T16:46:00,000T00:07:00,25-Apr-11,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-115T16:53:00,000T00:05:00,25-Apr-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-115T16:58:00,000T00:33:00,25-Apr-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEB from SSR's, MRO",,,,,, 2011-115T17:00:00,000T01:30:00,25-Apr-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 47.1 requested range 3.3 Mkm",,,,,, 2011-115T17:00:00,000T01:30:00,25-Apr-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-115T17:00:00,000T01:30:00,25-Apr-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 47 deg, range = 3.3 Mkm.",,,,,, 2011-115T17:31:00,000T00:30:00,25-Apr-11,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2011-115T18:01:00,002T22:02:00,25-Apr-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-115T18:30:00,000T00:30:00,25-Apr-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-115T19:00:00,000T01:00:00,25-Apr-11,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Dione","Images of mutual event, transit of Rhea across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-115T20:00:00,000T01:30:00,25-Apr-11,ISS,Prime,Saturn,MONITOR,,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-115T21:30:00,000T23:00:00,25-Apr-11,CIRS,Prime,Saturn,MIRTMAP,,CIRS_147SA_MIRTMAP001_PRIME,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-116T20:30:00,000T01:30:00,26-Apr-11,ISS,Prime,Saturn,MONITOR,,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-116T20:33:00,000T13:00:00,26-Apr-11,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,RSS USO characterization plus PIM. Pointing=XBAND to Earth. First 3 hours required to be tracked at DSS-25 (or DSS-26) in 1-way mode. No rolling during 3-hour USO from 2011-117T00:33:00 till 2011-117T03:33:00. Keep Ka-band ON till end of downlink to satisfy PIM requirement.,,,,,, 2011-117T00:33:00,000T09:00:00,27-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-117T01:33:00,000T08:00:00,27-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11116_SP,rider,,,,,, 2011-117T13:00:00,000T08:00:00,27-Apr-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-117T21:00:00,010T11:47:00,27-Apr-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-118T00:33:00,000T09:00:00,28-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-118T01:33:00,000T08:00:00,28-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11117_SP,rider,,,,,, 2011-118T09:33:00,000T14:45:00,28-Apr-11,CDA,Prime,DustRAM direction,ISD0028,,CDA ISD 2011-119T03:06:00,ISD observation around apoapse 2011-119T03:06:00 48.264302 Rs,,,,,, 2011-118T16:03:00,000T00:34:00,28-Apr-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-118T16:37:00,000T10:29:00,28-Apr-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-119T00:18:00,000T09:00:00,29-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-119T01:18:00,000T08:00:00,29-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_147IC_DSCAL11118_SP,rider,,,,,, 2011-119T03:06:00,010T15:40:58,29-Apr-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.001492 Rs exit= 14.011283 Range altitude= 1268.9020 km ... 4042.2535,,,,,, 2011-119T03:06:00,000T06:12:00,29-Apr-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-119T03:06:00,009T05:41:00,29-Apr-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-119T03:06:00,000T22:12:00,29-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-119T03:06:02,000T00:00:01,29-Apr-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 23.4 d, inc = 0.4 deg, r = 48.220 Rs, phase = 76 deg",,,,,, 2011-119T09:18:00,000T15:00:00,29-Apr-11,CDA,Prime,DustRAM direction,ISD0028,,CDA ISD 2011-119T03:06:00,ISD observation around apoapse 2011-119T03:06:00 48.264302 Rs,,,,,, 2011-119T09:18:00,001T00:00:00,29-Apr-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-120T00:18:00,000T09:00:00,30-Apr-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-120T01:18:00,000T08:00:00,30-Apr-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11119_SP,rider,,,,,, 2011-120T01:18:00,000T07:00:00,30-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-120T08:18:00,007T16:29:00,30-Apr-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-120T09:18:00,001T13:29:00,30-Apr-11,CDA,Prime,DustRAM direction,ISD0028,,CDA ISD 2011-119T03:06:00,ISD observation around apoapse 2011-119T03:06:00 48.264302 Rs,,,,,, 2011-120T09:18:00,005T15:59:00,30-Apr-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-122T00:17:00,000T09:00:00,2-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-122T01:17:00,000T08:00:00,2-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11121_SP,rider,,,,,, 2011-122T11:00:00,000T15:00:00,2-May-11,VIMS,Prime,rings(general),EG80PHASE,,E/G Ring phase observation,"Stare at E or G ring ansa, 1 second integration.",,,,,, 2011-122T11:00:00,000T15:00:00,2-May-11,CIRS,SPASS Rider,rings(general),EG80PHASE,,,null,,,,,, 2011-122T11:00:00,000T15:00:00,2-May-11,ISS,Non-SPASS,rings(general),EG80PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2011-123T02:00:00,000T01:00:00,3-May-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-123T06:32:00,000T09:00:00,3-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-123T07:32:00,000T08:00:00,3-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11123_SP,rider,,,,,, 2011-123T15:32:00,000T13:15:00,3-May-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-124T06:17:00,000T09:00:00,4-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-124T07:17:00,000T08:00:00,4-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11124_SP,rider,,,,,, 2011-124T16:00:00,000T23:00:00,4-May-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-124T16:00:00,000T23:00:00,4-May-11,ISS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-125T16:17:00,000T09:00:00,5-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-125T17:17:00,000T08:00:00,5-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11125_SP,rider,,,,,, 2011-126T01:17:00,001T00:00:00,6-May-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-126T03:00:00,000T12:10:00,6-May-11,ISS,Prime,Star,CALSTAR1,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2011-126T16:17:00,000T09:00:00,6-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-126T17:17:00,000T08:00:00,6-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11126_SP,rider,,,,,, 2011-127T01:17:00,001T07:30:00,7-May-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-127T06:00:00,000T01:00:00,7-May-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-127T08:30:00,000T12:00:00,7-May-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-127T23:47:00,000T09:00:00,7-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-128T00:47:00,000T08:00:00,8-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11127_SP,rider,,,,,, 2011-128T00:47:00,000T08:00:00,8-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-128T08:47:00,000T12:06:45,8-May-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-128T08:47:00,000T02:06:45,8-May-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-128T08:47:00,000T06:06:45,8-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-128T08:47:00,001T14:45:00,8-May-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-128T08:47:00,001T07:16:00,8-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-128T09:42:00,000T04:11:45,8-May-11,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2011-128T09:42:00,000T04:11:45,8-May-11,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T09:42:00,000T04:11:45,8-May-11,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS. Phase = 137 deg, SSC Lat/Lon = 0.003N/143.121 deg, SS Lat/Lon = 9.411N/281.214 deg. Alt = 262333 km, range = 264908 km. Resolution = 131 km/px. Template M4 and N1. Obtain cubes of Titan of various exp times.",,,,,, 2011-128T09:42:00,000T04:11:45,8-May-11,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2011-128T10:53:45,000T11:00:00,8-May-11,INMS,Non-SPASS,Saturn,T76INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-128T13:53:45,000T04:00:00,8-May-11,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2011-128T13:53:45,000T04:00:00,8-May-11,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T13:53:45,000T04:00:00,8-May-11,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan limb mapping.,"VIMS ridealong with CIRS for limb mapping. Phase = 137 deg, SSC Lat/Lon = 0.003N/147.288 deg, SS Lat/Lon = 9.413N/285.127 deg. Alt = 177943 km, range = 180518 km. Resolution = 89 km/px. Template R. Obtain cubes of Titan's limb.",,,,,, 2011-128T14:53:45,000T04:00:00,8-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-128T17:53:45,000T02:30:00,8-May-11,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2011-128T17:53:45,000T02:30:00,8-May-11,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T17:53:45,000T02:45:00,8-May-11,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 136 deg, SSC Lat/Lon = 0.004N/152.111 deg, SS Lat/Lon = 9.415N/288.884 deg. Alt = 97739 km, range = 100314 km. Resolution = 49 km/px. Template T. Obtain cubes while scanning across Titan.",,,,,, 2011-128T18:53:45,000T08:00:00,8-May-11,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T76 flyby,"T76 is a post-dusk, upstream equatorial flyby at 1862 km altitude, similar to prime mission T34 flyby. During T76 MAG will investigate the structure of Titan's induced magnetosphere along the ram direction while being on the dayside, a geometry which is ideal for pressure balance studies. The high altitude of periapsis (above the exobase) however limits the study of diffusion of magnetic field within the ionosphere. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2011-128T20:23:45,000T01:00:00,8-May-11,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2011-128T20:23:45,000T01:00:00,8-May-11,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T20:23:45,000T01:00:00,8-May-11,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2011-128T20:38:45,000T02:05:00,8-May-11,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Titan regional mapping.,"VIMS ridealong with CIRS prior to C/A. Phase = 133 deg, SSC Lat/Lon = 0.007N/157.903 deg, SS Lat/Lon = 9.416N/291.467 deg. Alt = 42917 km, range = 45492 km. Resolution = 21 km/px. Obtain mosaics/cubes of Titan.",,,,,, 2011-128T20:53:45,000T01:00:00,8-May-11,CAPS,SPASS Rider,Titan,T76INBND,,Inbound 148TI (T76),null,,,,,, 2011-128T20:53:45,000T01:00:00,8-May-11,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-128T20:53:45,000T01:15:00,8-May-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-128T21:23:45,000T00:45:00,8-May-11,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2011-128T21:23:45,000T00:45:00,8-May-11,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T21:53:45,000T02:00:00,8-May-11,CAPS,SPASS Rider,Titan,T76CLOSE,,Closest Approach 148TI (T76),null,,,,,, 2011-128T21:53:45,000T02:00:00,8-May-11,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-128T21:53:45,000T02:00:00,8-May-11,INMS,Non-SPASS,Titan,TITAN76,,Titan Flyby,Titan observation,,,,,, 2011-128T22:08:45,000T00:35:00,8-May-11,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2011-128T22:08:45,000T00:35:00,8-May-11,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T22:08:45,000T01:30:00,8-May-11,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2011-128T22:43:45,000T02:25:00,8-May-11,VIMS,Prime,Titan,HIRES,High resolution image,Hires regional mapping of Titan.,"Regional mapping of Titan during C/A. At C/A, Phase = 47 deg, SSC Lat/Lon = 0.044N/247.625 deg, SS Lat/Lon = 9.417N/293.580 deg. Alt = 1873 km, range = 4448 km. Resolution = 0.94 km/px. Obtain hires mosaics for regional mapping.",,,,,, 2011-128T22:43:45,000T02:25:00,8-May-11,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with ISS.,,,,,, 2011-128T22:43:45,000T02:25:00,8-May-11,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-128T23:38:45,000T01:15:00,8-May-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-128T23:53:45,000T01:00:00,8-May-11,CAPS,SPASS Rider,Titan,T76OUTBND,,Outbound 148TI (T76),null,,,,,, 2011-128T23:53:45,000T01:00:00,8-May-11,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-128T23:53:45,000T11:00:00,8-May-11,INMS,Non-SPASS,Saturn,T76OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-129T00:53:45,001T09:38:15,9-May-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-129T01:08:45,000T00:45:00,9-May-11,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,"Regional mapping of Titan. Phase = 42 deg, SSC Lat/Lon = 0.003S/337.371 deg, SS Lat/Lon = 9.418N/295.693 deg. Alt = 42914 km, range = 45914 km. Resolution = 21 km/px. Obtain mosaics for regional mapping.",,,,,, 2011-129T01:08:45,000T00:45:00,9-May-11,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with ISS.,,,,,, 2011-129T01:08:45,000T00:45:00,9-May-11,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-129T01:53:45,000T06:00:00,9-May-11,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2011-129T01:53:45,000T06:00:00,9-May-11,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with ISS.,,,,,, 2011-129T01:53:45,000T06:00:00,9-May-11,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-129T01:53:45,000T06:00:00,9-May-11,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 44 deg, SSC Lat/Lon = 0.004S/339.555 deg, SS Lat/Lon = 9.419N/296.397 deg. Alt = 57842 km, range = 60417 km. Resolution = 29 km/px. Template X. Obtain cubes while scanning across Titan.",,,,,, 2011-129T02:53:45,000T04:00:00,9-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-129T06:53:45,001T03:38:15,9-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-129T07:53:45,000T05:00:00,9-May-11,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan.,"Global mapping of Titan. Phase = 47 deg, SSC Lat/Lon = 0.007S/348.305 deg, SS Lat/Lon = 9.421N/302.031 deg. Alt = 178303 km, range = 180878 km. Resolution = 89 km/px. Template V. Obtain cubes for global mapping.",,,,,, 2011-129T07:53:45,000T05:00:00,9-May-11,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with ISS.,,,,,, 2011-129T07:53:45,000T05:00:00,9-May-11,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-129T10:53:45,000T01:17:48,9-May-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-129T12:11:33,000T22:20:27,9-May-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-129T12:53:45,000T08:13:15,9-May-11,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,"Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template A2, sit and stare for ISS at start and end.",,,,,, 2011-129T12:53:45,000T08:13:00,9-May-11,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-129T12:53:45,000T08:13:15,9-May-11,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Stare at Titan.,"VIMS ridealong with CIRS for global mapping. Phase = 48 deg, SSC Lat/Lon = 0.007S/353.697 deg, SS Lat/Lon = 9.424N/306.726 deg. Alt = 281584 km, range = 284159 km. Resolution = 141 km/px. Template A2. Obtain cubes of various exp times.",,,,,, 2011-129T16:03:00,000T18:29:00,9-May-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-129T18:46:58,000T02:13:02,9-May-11,CDA,Non-SPASS,Other,RATE080B,,Data rate,Range enter= 13.999007 Rs exit= 13.998289 Range altitude= 4035.5659 km ... -1506.4272,,,,,, 2011-129T21:00:00,002T01:40:58,9-May-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.999007 Rs exit= 13.998289 Range altitude= 4035.5659 km ... -1506.4272,,,,,, 2011-129T23:32:00,020T10:44:00,9-May-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-129T23:32:00,000T09:00:00,9-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-130T00:32:00,000T10:00:00,10-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11129_SP,rider,,,,,, 2011-130T00:32:00,000T07:00:00,10-May-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-130T10:32:00,002T21:59:59,10-May-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-130T10:32:00,000T00:39:33,10-May-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-130T10:32:00,002T22:00:00,10-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-130T10:32:00,001T14:53:00,10-May-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-130T11:11:00,000T02:00:00,10-May-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-130T11:11:33,000T00:30:00,10-May-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-130T11:11:58,000T02:00:00,10-May-11,CDA,SPASS Rider,DustRAM direction,RPX0130,,CDA RPXing 2011-130T12:11:58,RPXing at 7.5447559 Rs,,,,,, 2011-130T11:12:00,000T02:28:00,10-May-11,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2011-130T11:12:00,000T02:28:00,10-May-11,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,South Pole aurora phase=170 sun angle=15.8 degrees,,,,,, 2011-130T11:12:00,000T02:28:00,10-May-11,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC clear aurora movie,"Auroral movie LOOPED in 4x4 CL1CL1 repeated untill observation lasts, see ISS_133SW_SWAURPTG005_CAPS, add the 04040 trigger at the beginning and the end",,,,,, 2011-130T11:12:00,000T02:28:00,10-May-11,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Ridealong,Auroral UVIS Ridealong,,,,,, 2011-130T11:41:33,000T01:30:00,10-May-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-130T12:00:00,000T18:00:00,10-May-11,RPWS,Non-SPASS,Saturn,SEDDF,Saturn Electrical Discharge direction finding,SED Direction-finding,"Perform direction-finding on SED to a) verify source in Saturn's atmosphere (or refute this and find source in rings), and b) if source is in atmosphere, use location to characterize the location of thunderstorms. No pointing requirement",,,,,, 2011-130T13:11:33,000T23:00:00,10-May-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-130T13:40:00,000T01:20:00,10-May-11,VIMS,Prime,Saturn,OMICETOCC,OmiCet occultation,omiCet Saturn occultation,"omiCet atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. At 14:20, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation ingess occurred.",,,,,, 2011-130T13:40:00,000T01:20:00,10-May-11,CIRS,,Saturn,OMICETOCC,OmiCet occultation,CIRS_148SA_OMICETOCC001_VIMS,Collaboration with VIMS. Stellar Occ Saturn ingress T14:01 at 28N dark limb CIRS limb integration 1420-1500 Star RA=34.836 Dec = -2.977,,,,,, 2011-130T15:00:00,000T01:30:00,10-May-11,ISS,Prime,Enceladus,PLMMPMR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-130T15:00:00,000T01:30:00,10-May-11,CIRS,SPASS Rider,Enceladus,PLMMPMR,Observe Enceladus' plumes,,null,,,,,, 2011-130T15:00:00,000T01:30:00,10-May-11,VIMS,SPASS Rider,Enceladus,PLMMPMR,Observe Enceladus' plumes,Enceladus plume,Enceladus plume,,,,,, 2011-130T16:52:00,000T06:00:00,10-May-11,CIRS,Prime,Saturn,LIMBINT,Limb integration,CIRS_148SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2011-130T16:52:00,000T06:00:00,10-May-11,VIMS,SPASS Rider,Saturn,LIMBINT,Limb integration,CIRS Limbint Ridealong,Limb integration CIRS Ridealong,,,,,, 2011-130T20:43:54,000T00:00:01,10-May-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.888 Rs, lat = -0 deg, phase = 118 deg",,,,,, 2011-130T23:32:00,000T09:00:00,10-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-131T00:32:00,000T08:00:00,11-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11130_SP,rider,,,,,, 2011-131T09:12:00,000T01:30:00,11-May-11,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 23.3 requested range 1.7 Mkm",,,,,, 2011-131T09:12:00,000T01:30:00,11-May-11,CIRS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-131T09:12:00,000T01:30:00,11-May-11,VIMS,SPASS Rider,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 23 deg, range = 1.7 Mkm.",,,,,, 2011-131T10:42:00,000T12:10:00,11-May-11,VIMS,Prime,Saturn,NHEMMAP,,Saturn Northern Hem Mosaic Mosaic,"10 (2 rows)x3(columns) Regional mosaics, one collected each hour throughout the 12-hrs duration. Lowest row (tier) of the mosaic is centered at the String of Pearl latitude at 34 degrees Planetiocentric at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 10-minute intervals between frame centers (7 mins for science, 3 for repositioning). Each of these mosaics should take an hour.",,,,,, 2011-131T10:42:00,000T12:10:00,11-May-11,CIRS,SPASS Rider,Saturn,NHEMMAP,,Rider,VIMS rider,,,,,, 2011-131T12:11:33,000T20:20:27,11-May-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-131T22:40:58,018T11:34:02,11-May-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.010562 Rs exit= 14.009879 Range altitude= -1503.2973 km ... 4138.7502,,,,,, 2011-131T23:32:00,000T09:00:00,11-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-132T00:32:00,000T08:00:00,12-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11131_SP,rider,,,,,, 2011-132T01:25:00,001T07:07:00,12-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-132T08:32:00,000T10:41:00,12-May-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-132T09:12:00,000T01:30:00,12-May-11,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 10.6 requested range 2.3 Mkm",,,,,, 2011-132T09:12:00,000T01:30:00,12-May-11,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-132T09:12:00,000T01:30:00,12-May-11,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 11 deg, range = 2.3 Mkm.",,,,,, 2011-132T10:42:00,000T06:18:00,12-May-11,VIMS,Prime,rings(general),RPX10PH,Ring plane crossing,Ring Plane Crossing near 10 deg phase.,"Cube Size (X,Z) = 64*12? Time per SC pointing (mins) = 10, Number of cubes = 36, Volume (Mbits) = 100, Stare at 1 ansa as Cassini crosses ring plane and opening angle is less than 0.015 deg. X-axis in ring plane preferred. Distance 20 R_S. tau_IR = 640 msec.",,,,,, 2011-132T10:42:00,000T06:18:00,12-May-11,CIRS,SPASS Rider,rings(general),RPX10PH,Ring plane crossing,Rider,VIMS rider,,,,,, 2011-132T10:42:00,000T06:18:00,12-May-11,ISS,SPASS Rider,rings(general),RPX10PH,Ring plane crossing,RING PLANE CROSSING NEAR 10 DEG PHASE,Rider on VIMS RPX observation,,,,,, 2011-132T17:00:00,000T05:52:00,12-May-11,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2011-132T17:00:00,000T05:52:00,12-May-11,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,aurora phase=11 range=20.3-22.1 Rs,,,,,, 2011-132T17:00:00,000T05:52:00,12-May-11,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC clear aurora movie,"Auroral movie LOOPED in 4x4 CL1CL1 repeated untill observation lasts, see ISS_133SW_SWAURPTG005_CAPS, add the 04040 trigger at the beginning and the end",,,,,, 2011-132T17:00:00,000T05:52:00,12-May-11,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Ridealong,Auroral UVIS Ridealong,,,,,, 2011-132T19:13:00,000T02:00:00,12-May-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-132T21:13:00,000T11:19:00,12-May-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-132T23:32:00,000T09:00:00,12-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-133T00:32:00,000T08:00:00,13-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11132_SP,rider,,,,,, 2011-133T08:32:00,034T21:24:59,13-May-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-133T08:32:00,010T23:14:00,13-May-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-133T08:32:00,002T11:28:00,13-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-133T08:32:00,002T20:59:00,13-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-133T10:00:00,000T14:00:00,13-May-11,ISS,Prime,Other,SUTROT,,Suttungr,Observation of irregular moon of Saturn.,,,,,, 2011-133T10:00:00,000T14:00:00,13-May-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-134T00:00:00,000T03:00:00,14-May-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2011-134T05:46:00,000T09:00:00,14-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-134T06:46:00,000T08:00:00,14-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11134_SP,rider,,,,,, 2011-134T16:00:00,001T04:00:00,14-May-11,ISS,Prime,Other,4S12ROT,,S/2004_S12 (S12_2004),Observation of irregular moon of Saturn.,,,,,, 2011-134T16:00:00,001T04:00:00,14-May-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-135T20:00:00,000T07:00:00,15-May-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-136T03:00:00,015T04:15:00,16-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-136T05:31:00,003T23:45:00,16-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-136T05:31:00,000T09:00:00,16-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-136T06:31:00,000T08:00:00,16-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11136_SP,rider,,,,,, 2011-136T15:30:00,000T01:30:00,16-May-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 55.6 requested range 3.1 Mkm",,,,,, 2011-136T15:30:00,000T01:30:00,16-May-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-136T15:30:00,000T01:30:00,16-May-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 56 deg, range = 3.1 Mkm.",,,,,, 2011-136T17:00:00,000T01:00:00,16-May-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-136T18:00:00,001T08:00:00,16-May-11,UVIS,Prime,Saturn,MOS148APO,,,"Mosaic scan of Saturn magnetosphere to image hydrogen, day 1. Days 1 and 3 scan patterns form an S shape. Day 2 scan pattern is a rectangle which fills in the spaces between the arms of the S. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turn to waypoint at end. 0) Start at Saturn center. Align slit with Saturn spin axis. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. 1) Start data capture, stare 193.0 s, stop data capture. 2) Repeat Pattern A 147 times. 3) Slew +128 mrad about x-axis. Start data capture, stare 193.0 s, stop data capture. 4) Repeat Pattern B 194 times. 5) Slew to waypoint. Pattern A: Slew +1.5 mrad about z-axis. Start data capture, stare 193.0 s, stop data capture. Pattern B: Slew -1.5 mrad about z-axis. Start data capture, stare 193.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (6273.61924 bps, from Alain's spreadsheet)x(193.0s per stare)x(443 stares) = 536.4x10^6 bits",,,,,, 2011-138T05:16:00,000T09:00:00,18-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-138T06:16:00,000T08:00:00,18-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11138_SP,rider,,,,,, 2011-138T15:30:00,000T01:30:00,18-May-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 63.8 requested range 2.8 Mkm",,,,,, 2011-138T15:30:00,000T01:30:00,18-May-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-138T15:30:00,000T01:30:00,18-May-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 64 deg, range = 2.8 Mkm.",,,,,, 2011-138T17:00:00,000T01:00:00,18-May-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-138T18:00:00,001T08:00:00,18-May-11,UVIS,Prime,Saturn,MOS148APO,,,"Mosaic scan of Saturn magnetosphere to image hydrogen, day 2. Days 1 and 3 scan patterns form an S shape. Day 2 scan pattern is a rectangle which fills in the spaces between the arms of the S. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turn to waypoint at end. 0) Start at Saturn center. Align slit with Saturn spin axis. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. 1) Slew +64 mrad about x-axis. Start data capture, stare 163.0 s, stop data capture. 2) Repeat Pattern A 127 times. 3) Slew -128 mrad about x-axis. Start data capture, stare 163.0 s, stop data capture. 4) Repeat Pattern B 254 times. 5) Slew +128 mrad about x-axis. Start data capture, stare 163.0 s, stop data capture. 6) Repeat Pattern A 127 times. 7) Slew to waypoint. Pattern A: Slew +1.5 mrad about z-axis. Start data capture, stare 163.0 s, stop data capture. Pattern B: Slew -1.5 mrad about z-axis. Start data capture, stare 163.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (7428.27309 bps, from Alain's spreadsheet)x(163.0s per stare)x(512 stares) = 619.93x10^6 bits",,,,,, 2011-140T05:16:00,004T17:14:00,20-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-140T05:16:00,000T09:00:00,20-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-140T06:16:00,000T08:00:00,20-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11140_SP,rider,,,,,, 2011-140T14:16:00,000T13:30:00,20-May-11,CDA,Prime,DustRAM direction,ISD0029,,CDA ISD 2011-150T10:15:00,ISD observation around apoapse 2011-150T10:15:00 67.863347 Rs,,,,,, 2011-141T05:16:00,000T09:00:00,21-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-141T06:16:00,000T08:00:00,21-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11141_SP,rider,,,,,, 2011-141T15:20:00,000T05:00:00,21-May-11,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Titan across Dione","Images of mutual event, transit of Titan across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-141T20:20:00,000T16:00:00,21-May-11,VIMS,Prime,rings(general),EG45PHASE,,E/G Ring phase observation,"Stare at E or G ring ansa, 1 second integration.",,,,,, 2011-141T20:20:00,000T16:00:00,21-May-11,CIRS,SPASS Rider,rings(general),EG45PHASE,,,null,,,,,, 2011-141T20:20:00,000T16:00:00,21-May-11,ISS,Non-SPASS,rings(general),EG45PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2011-142T15:01:00,000T09:00:00,22-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-142T16:01:00,000T08:00:00,22-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11142_SP,rider,,,,,, 2011-143T00:01:00,000T22:45:00,23-May-11,CDA,Prime,DustRAM direction,ISD0029,,CDA ISD 2011-150T10:15:00,ISD observation around apoapse 2011-150T10:15:00 67.863347 Rs,,,,,, 2011-143T22:46:00,000T09:00:00,23-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-143T23:46:00,000T08:00:00,23-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11143_SP,rider,,,,,, 2011-144T07:46:00,000T14:44:00,24-May-11,CAPS,Prime,Other,SWSKRPTG,,Solar wind pointing,CAPS control of spacecraft pointing (data volume covered in another request),,,,,, 2011-144T07:46:00,000T23:44:00,24-May-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-144T22:30:00,003T23:45:00,24-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-144T22:30:00,000T09:00:00,24-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-144T23:30:00,000T08:00:00,24-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11144_SP,rider,,,,,, 2011-145T07:30:00,001T13:30:00,25-May-11,CAPS,Prime,Other,SWSKRPTG,,Solar wind pointing,CAPS control of spacecraft pointing (data volume covered in another request),,,,,, 2011-145T07:30:00,005T02:46:00,25-May-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-146T22:30:00,000T09:00:00,26-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-146T23:30:00,000T08:00:00,26-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11146_SP,rider,,,,,, 2011-147T07:30:00,001T13:15:00,27-May-11,CAPS,Prime,Other,SWSKRPTG,,Solar wind pointing,CAPS control of spacecraft pointing (data volume covered in another request),,,,,, 2011-148T22:15:00,001T12:00:00,28-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-148T22:15:00,000T09:00:00,28-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-148T23:15:00,000T08:00:00,28-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_148IC_DSCAL11148_SP,rider,,,,,, 2011-149T07:15:00,001T13:30:00,29-May-11,CAPS,Prime,Other,SWSKRPTG,,Solar wind pointing,CAPS control of spacecraft pointing (data volume covered in another request),,,,,, 2011-150T10:15:00,018T11:33:58,30-May-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.010562 Rs exit= 14.009879 Range altitude= -1503.2973 km ... 4138.7502,,,,,, 2011-150T10:15:32,000T00:00:01,30-May-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 39.1 d, inc = 0.4 deg, r = 67.794 Rs, phase = 62 deg",,,,,, 2011-150T10:16:00,000T02:00:00,30-May-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-150T10:16:00,017T19:41:00,30-May-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_148_149",,,,,, 2011-150T10:16:00,002T11:43:00,30-May-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-150T12:16:00,008T11:44:00,30-May-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-150T22:15:00,000T09:00:00,30-May-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-150T23:15:00,000T08:00:00,30-May-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11150_SP,rider,,,,,, 2011-151T07:15:00,000T08:00:00,31-May-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-151T15:15:00,001T05:14:00,31-May-11,CDA,Prime,DustRAM direction,ISD0029,,CDA ISD 2011-150T10:15:00,ISD observation around apoapse 2011-150T10:15:00 67.863347 Rs,,,,,, 2011-151T15:15:00,016T14:42:00,31-May-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-152T21:59:00,003T23:45:00,1-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-152T21:59:00,000T09:00:00,1-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-152T22:59:00,000T08:00:00,1-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11152_SP,rider,,,,,, 2011-153T06:59:00,001T13:30:00,2-Jun-11,CDA,Prime,DustRAM direction,ISD0029,,CDA ISD 2011-150T10:15:00,ISD observation around apoapse 2011-150T10:15:00 67.863347 Rs,,,,,, 2011-154T21:59:00,000T09:00:00,3-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-154T22:59:00,000T08:00:00,3-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11154_SP,rider,,,,,, 2011-155T08:00:00,000T01:30:00,4-Jun-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 86 requested range 3.8 Mkm",,,,,, 2011-155T08:00:00,000T01:30:00,4-Jun-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-155T08:00:00,000T01:30:00,4-Jun-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 86 deg, range = 3.8 Mkm.",,,,,, 2011-155T09:30:00,000T01:00:00,4-Jun-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-155T21:00:00,000T23:14:00,4-Jun-11,CDA,Prime,DustRAM direction,ISD0029,,CDA ISD,ISD observation around apoapse 2011-150T10:15:00 67.863347 Rs,,,,,, 2011-156T21:44:00,000T09:00:00,5-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-156T21:44:00,000T09:00:00,5-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-156T22:44:00,000T08:00:00,5-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11156_SP,rider,,,,,, 2011-157T06:44:00,001T13:30:00,6-Jun-11,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Observation of Iapetus around closest approach,,,,,, 2011-157T06:44:00,001T13:30:00,6-Jun-11,CIRS,,Iapetus,IAPETUS,Iapetus observation,,,,,,,, 2011-157T06:44:00,001T13:30:00,6-Jun-11,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2011-157T06:44:00,001T13:30:00,6-Jun-11,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus S pole 1.7mrad,Iapetus,,,,,, 2011-157T06:44:00,003T06:00:00,6-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-158T21:44:00,000T09:00:00,7-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-158T22:44:00,000T08:00:00,7-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11158_SP,rider,,,,,, 2011-159T00:00:00,001T05:00:00,8-Jun-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-159T06:44:00,000T19:30:00,8-Jun-11,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Observation of Iapetus and its Hill sphere,,,,,, 2011-159T06:44:00,000T19:30:00,8-Jun-11,CIRS,,Iapetus,IAPETUS,Iapetus observation,,null,,,,,, 2011-159T06:44:00,000T19:30:00,8-Jun-11,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2011-159T06:44:00,000T19:30:00,8-Jun-11,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus S pole 1.7mrad,Iapetus,,,,,, 2011-160T03:44:00,000T09:00:00,9-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-160T04:44:00,000T08:00:00,9-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11160_SP,rider,,,,,, 2011-160T05:00:00,008T00:57:00,9-Jun-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-160T12:44:00,000T15:16:00,9-Jun-11,ISS,Prime,Iapetus,IAPETUS,Iapetus observation,Iapetus,Observation of Iapetus and its Hill sphere,,,,,, 2011-160T12:44:00,000T15:16:00,9-Jun-11,CIRS,,Iapetus,IAPETUS,Iapetus observation,,null,,,,,, 2011-160T12:44:00,000T15:16:00,9-Jun-11,UVIS,SPASS Rider,Iapetus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2011-160T12:44:00,000T15:16:00,9-Jun-11,VIMS,SPASS Rider,Iapetus,IAPETUS,Iapetus observation,Iapetus S pole 1.7mrad,Iapetus,,,,,, 2011-160T12:44:00,001T15:14:00,9-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-161T04:00:00,000T12:00:00,10-Jun-11,ISS,Prime,Star,CANOPUS1,,ISS PSF calibration,Point to bright star Canopus,,,,,, 2011-162T03:43:00,000T09:00:00,11-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-162T03:58:00,002T08:30:00,11-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-162T04:43:00,000T08:00:00,11-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11162_SP,rider,,,,,, 2011-162T14:00:00,000T01:30:00,11-Jun-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 58.3 requested range 2.8 Mkm",,,,,, 2011-162T14:00:00,000T01:30:00,11-Jun-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-162T14:00:00,000T01:30:00,11-Jun-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 58 deg, range = 2.8 Mkm.",,,,,, 2011-162T15:30:00,000T01:00:00,11-Jun-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-162T16:30:00,001T08:00:00,11-Jun-11,UVIS,Prime,Saturn,MOS148APO,,,"Mosaic scan of Saturn magnetosphere to image hydrogen, day 3. Days 1 and 3 scan patterns form an S shape. Day 2 scan pattern is a rectangle which fills in the spaces between the arms of the S. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turn to waypoint at end. 0) Start at Saturn center. Align slit with Saturn spin axis. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. 1) Start data capture, stare 193.0 s, stop data capture. 2) Repeat Pattern A 147 times. 3) Slew -128 mrad about x-axis. Start data capture, stare 193.0 s, stop data capture. 4) Repeat Pattern B 194 times. 5) Slew to waypoint. Pattern A: Slew -1.5 mrad about z-axis. Start data capture, stare 193.0 s, stop data capture. Pattern B: Slew +1.5 mrad about z-axis. Start data capture, stare 193.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (6273.61924 bps, from Alain's spreadsheet)x(193.0s per stare)x(443 stares) = 536.4x10^6 bits",,,,,, 2011-162T18:00:00,000T01:08:00,11-Jun-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-164T03:28:00,000T09:00:00,13-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-164T04:28:00,000T08:00:00,13-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11164_SP,rider,,,,,, 2011-164T12:28:00,002T17:30:00,13-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-164T14:00:00,000T01:30:00,13-Jun-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 66.7 requested range 3.1 Mkm",,,,,, 2011-164T14:00:00,000T01:30:00,13-Jun-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-164T14:00:00,000T01:30:00,13-Jun-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 67 deg, range = 3.1 Mkm.",,,,,, 2011-164T15:30:00,000T02:00:00,13-Jun-11,ISS,Prime,Saturn,MONITOR,,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-164T17:30:00,000T23:00:00,13-Jun-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-164T17:30:00,000T23:00:00,13-Jun-11,ISS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-165T16:30:00,000T01:00:00,14-Jun-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 14","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-165T17:30:00,000T01:30:00,14-Jun-11,ISS,Prime,Saturn,MONITOR,,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-165T21:13:00,000T09:00:00,14-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-165T22:13:00,000T08:00:00,14-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11165_SP,rider,,,,,, 2011-166T06:53:00,000T12:00:00,15-Jun-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-166T20:58:00,000T09:00:00,15-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-166T21:58:00,000T08:00:00,15-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11166_SP,rider,,,,,, 2011-167T05:58:00,000T23:59:00,16-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-167T07:00:00,000T10:00:00,16-Jun-11,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2011-167T17:00:00,000T01:45:00,16-Jun-11,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Titan","Images of mutual event, transit of Rhea across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-167T20:57:00,000T09:00:00,16-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-167T21:57:00,000T08:00:00,16-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11167_SP,rider,,,,,, 2011-168T05:57:00,002T23:44:59,17-Jun-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-168T05:57:00,000T09:26:42,17-Jun-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-168T05:57:00,002T23:45:00,17-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-168T05:57:00,002T23:45:00,17-Jun-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. RINGS_149",,,,,, 2011-168T05:57:00,000T13:08:00,17-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-168T11:00:00,000T09:15:00,17-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-168T15:23:42,000T14:33:18,17-Jun-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-168T19:05:00,002T09:21:00,17-Jun-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-168T20:57:00,000T09:00:00,17-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-168T21:48:58,000T20:21:02,17-Jun-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997601 Rs exit= 13.989670 Range altitude= 4131.9984 km ... -1598.2827,,,,,, 2011-168T21:57:00,000T08:00:00,17-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11168_SP,rider,,,,,, 2011-169T05:57:00,000T08:26:42,18-Jun-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-169T06:40:00,000T07:20:00,18-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-169T14:00:00,000T01:00:00,18-Jun-11,CDA,Prime,Other,ERING,E ring observation,CDA ERING _01,CDA ERING_01; objective code RC1b,,,,,, 2011-169T14:23:00,000T03:00:00,18-Jun-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-169T14:23:42,000T00:30:00,18-Jun-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-169T14:53:42,000T01:30:00,18-Jun-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-169T15:00:00,000T03:10:00,18-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-169T16:23:42,000T23:00:00,18-Jun-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-169T17:23:00,000T11:15:00,18-Jun-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-169T18:10:00,000T02:30:00,18-Jun-11,ISS,Prime,Helene,HELENCLOS,,Helene close flyby,Observation during flyby of Helene.,,,,,, 2011-169T18:10:00,000T02:30:00,18-Jun-11,CIRS,,Helene,HELENCLOS,,,"CIRS would like a single 5 mrad scan, with the FP3 detector scan centered on the disk, at 6 murad/sec, sometime around 20:00 UT, though we are fairly flexible. Ideally, but with lower priority, follow the FP3 scan with a 2-minute FP1 stare, with FP1 centered on Helene.",,,,,, 2011-169T18:10:00,000T02:30:00,18-Jun-11,UVIS,SPASS Rider,Helene,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Map uv albedo,,,,,, 2011-169T18:10:00,000T02:30:00,18-Jun-11,VIMS,SPASS Rider,Helene,HELENCLOS,,Titan Monitoring Campaign,ISS Helene flyby,,,,,, 2011-169T18:10:00,000T02:30:00,18-Jun-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate3,Range enter= 13.997601 Rs exit= 13.989670 Range altitude= 4131.9984 km ... -1598.2827,,,,,, 2011-169T20:40:00,000T01:20:00,18-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-169T20:40:00,001T05:00:58,18-Jun-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate2,Range enter= 13.997601 Rs exit= 13.989670 Range altitude= 4131.9984 km ... -1598.2827,,,,,, 2011-169T22:00:00,000T01:00:00,18-Jun-11,CDA,Prime,Other,ERING,E ring observation,CDA ERING _03,CDA ERING_03; objective code RC1b,,,,,, 2011-169T23:00:00,000T03:00:00,18-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-169T23:45:34,000T00:00:01,18-Jun-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.884 Rs, lat = -0 deg, phase = 119 deg",,,,,, 2011-170T02:00:00,000T01:00:00,19-Jun-11,CDA,Prime,Other,ERING,E ring observation,CDA ERING _04,CDA ERING_04; objective code RC1b,,,,,, 2011-170T03:00:00,000T02:00:00,19-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-170T05:00:00,000T01:00:00,19-Jun-11,CDA,Prime,Other,ERING,E ring observation,CDA ERING _05,CDA ERING_05; objective code RC1b,,,,,, 2011-170T06:00:00,000T03:00:00,19-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-170T09:00:00,000T01:00:00,19-Jun-11,CDA,Prime,Other,ERING,E ring observation,CDA ERING _06,CDA ERING_06; objective code RC1b,,,,,, 2011-170T10:00:00,000T03:00:00,19-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-170T13:00:00,000T01:00:00,19-Jun-11,CDA,Prime,Other,ERING,E ring observation,CDA ERING _07,CDA ERING_07; objective code RC1b,,,,,, 2011-170T14:00:00,000T04:30:00,19-Jun-11,CDA,Prime,DustRAM direction,ORBT,,CDA Periapse,RPXing at 7.4866611 Rs,,,,,, 2011-170T15:23:42,000T14:18:18,19-Jun-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-170T20:42:00,000T09:00:00,19-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-170T21:42:00,000T08:00:00,19-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11170_SP,rider,,,,,, 2011-171T01:40:58,000T04:01:02,20-Jun-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.001953 Rs exit= 14.007414 Range altitude= -1595.2083 km ... 5303.2338,,,,,, 2011-171T04:26:00,000T01:16:00,20-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-171T05:42:00,000T11:20:01,20-Jun-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-171T05:42:00,001T15:00:00,20-Jun-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.001953 Rs exit= 14.007414 Range altitude= -1595.2083 km ... 5303.2338,,,,,, 2011-171T05:42:00,000T00:50:01,20-Jun-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-171T05:42:00,000T08:50:01,20-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-171T05:42:00,002T02:00:00,20-Jun-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-171T05:42:00,002T02:00:00,20-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-171T06:27:00,000T03:05:01,20-Jun-11,UVIS,Prime,Titan,HDACSTARE,,HDAC observation of Titan (stare),HDAC observation of Titan (stare). EUV and FUV will also be taking data with the setup like the setup for EUVFUV,,,,,, 2011-171T06:27:00,000T09:35:01,20-Jun-11,RADAR,SPASS Rider,Titan,T77WARMUP,,Warmup for T77,,,,,,, 2011-171T06:32:01,000T11:00:00,20-Jun-11,INMS,Non-SPASS,Saturn,T77INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-171T06:37:00,000T09:25:01,20-Jun-11,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Cloud monitor,,,,,, 2011-171T06:37:00,000T02:55:01,20-Jun-11,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 163 deg, SSC Lat/Lon = 0.003S/1.462 deg, SS Lat/Lon = 10.008N/167.746 deg. Alt = 237580 km, range = 240155 km. Resolution = 119 km/px. Template X-extended. Obtain cubes of Titan while scanning.",,,,,, 2011-171T06:42:01,000T02:50:00,20-Jun-11,ISS,SPASS Rider,Titan,HDACSTARE,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-171T09:32:01,000T06:30:00,20-Jun-11,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2011-171T09:32:01,000T06:30:00,20-Jun-11,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-171T09:32:01,000T06:30:00,20-Jun-11,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 163 deg, SSC Lat/Lon = 0.003S/4.638 deg, SS Lat/Lon = 10.009N/170.488 deg. Alt = 177745 km, range = 180320 km. Resolution = 89 km/px. Template X. Obtain cubes of Titan while scanning across disk.",,,,,, 2011-171T14:32:01,000T08:00:00,20-Jun-11,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T77 flyby,"T77 is a noon, equatorial flyby across Titan's wake at a short distance (1382 km altitude). This geometry is suitable to continue the characterization of the magnetic tail close to Titan and the spatial distribution of escaping particles downstream from the moon combining MAG and RPWS and CAPS data. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2011-171T16:02:01,000T01:18:00,20-Jun-11,RADAR,Prime,Titan,T77INSCAT,,T77 Inbound Scatterometry,,,,,,, 2011-171T16:32:01,000T01:00:00,20-Jun-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-171T17:02:01,000T00:45:00,20-Jun-11,CAPS,SPASS Rider,Titan,T77INBND,,Inbound 149TI (T77),null,,,,,, 2011-171T17:20:01,000T00:42:00,20-Jun-11,RADAR,Prime,Titan,T77IHISAR,,T77 Inbound HiSAR,,,,,,, 2011-171T17:32:01,000T02:00:00,20-Jun-11,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-171T17:32:01,000T02:00:00,20-Jun-11,INMS,Non-SPASS,Titan,TITAN77,,Titan Flyby,Titan observation,,,,,, 2011-171T17:32:01,000T02:00:00,20-Jun-11,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2011-171T17:47:01,000T01:30:00,20-Jun-11,CAPS,SPASS Rider,Titan,T77CLOSE,,Closest Approach 149TI (T77),null,,,,,, 2011-171T18:02:01,000T00:12:00,20-Jun-11,RADAR,Prime,Titan,T77INALT,,T77 Inbound Altimetry,,,,,,, 2011-171T18:14:01,000T00:36:00,20-Jun-11,RADAR,Prime,Titan,T77INOSAR,,T77 Inbound and Outbound SAR,,,,,,, 2011-171T18:50:01,000T00:12:00,20-Jun-11,RADAR,Prime,Titan,T77OUTALT,,T77 Outbound Altimetry,,,,,,, 2011-171T19:02:01,000T00:42:00,20-Jun-11,RADAR,Prime,Titan,T77OHISAR,,T77 Outbound HiSAR,,,,,,, 2011-171T19:17:01,000T00:45:00,20-Jun-11,CAPS,SPASS Rider,Titan,T77OUTBND,,Outbound 149TI (T77),null,,,,,, 2011-171T19:32:01,000T11:00:00,20-Jun-11,INMS,Non-SPASS,Saturn,T77OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-171T19:32:01,000T01:00:00,20-Jun-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-171T19:44:01,000T01:18:00,20-Jun-11,RADAR,Prime,Titan,T77OUTSCT,,T77 Outbound Scatterometry,,,,,,, 2011-171T20:02:01,003T15:39:59,20-Jun-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-171T21:02:01,000T02:30:00,20-Jun-11,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2011-171T21:02:01,000T02:30:00,20-Jun-11,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-171T21:02:01,000T02:30:00,20-Jun-11,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 19 deg, SSC Lat/Lon = 0.000S/197.539 deg, SS Lat/Lon = 10.016N/181.302 deg. Alt = 47668 km, range = 50243 km. Resolution = 24 km/px. Template E. Obtain cubes of Titan while scanning across disk.",,,,,, 2011-171T22:32:01,001T09:09:59,20-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-171T23:32:01,000T04:00:00,20-Jun-11,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2011-171T23:32:01,000T04:00:00,20-Jun-11,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-171T23:32:01,000T04:00:00,20-Jun-11,UVIS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,UVIS Rider to CIRS MIRLMBMAP,UVIS Rider to CIRS Mid IR Limb observation,,,,,, 2011-171T23:32:01,000T04:00:00,20-Jun-11,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan limb mapping.,"VIMS ridealong with CIRS for limb mapping of Titan. Phase = 21 deg, SSC Lat/Lon = 0.003S/202.222 deg, SS Lat/Lon = 10.017N/183.652 deg. Alt = 97333 km, range = 99908 km. Resolution = 50 km/px. Template F. Obtain cubes of Titan's limb.",,,,,, 2011-172T03:32:01,000T05:00:00,21-Jun-11,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan.,"Global mapping of Titan. Phase = 22 deg, SSC Lat/Lon = 0.005S/206.890 deg, SS Lat/Lon = 10.019N/187.413 deg. Alt = 177248 km, range = 179823 km. Resolution = 89 km/px. Template V. Obtain cubes for global mapping.",,,,,, 2011-172T03:32:01,000T05:00:00,21-Jun-11,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Cloud monitor,,,,,, 2011-172T03:32:01,000T05:00:00,21-Jun-11,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-172T06:32:01,001T01:09:59,21-Jun-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-172T08:32:01,000T09:44:59,21-Jun-11,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,"Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template A2: two or more dwells for ISS, 30 mins duration.",,,,,, 2011-172T08:32:01,000T09:44:59,21-Jun-11,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-172T08:32:01,000T09:44:59,21-Jun-11,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Stare at Titan.,"VIMS ridealong with CIRS. Phase = 22 deg, SSC Lat/Lon = 0.005S/211.734 deg, SS Lat/Lon = 10.022N/192.115 deg. Alt = 278318 km, range = 280893 km. Resolution = 139 km/px. Template A2. Obtain cubes of Titan of various exp times.",,,,,, 2011-172T20:42:00,002T15:00:00,21-Jun-11,CDA,Non-SPASS,Other,RATE010A,,Data rate End:SApo,Range enter= 14.001953 Rs exit= 14.007414 Range altitude= -1595.2083 km ... 5303.2338,,,,,, 2011-172T20:42:00,000T09:00:00,21-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-172T21:42:00,000T10:00:00,21-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11172_SP,rider,,,,,, 2011-173T07:42:00,002T04:00:00,22-Jun-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-173T07:42:00,002T19:00:00,22-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-173T07:42:00,007T12:14:00,22-Jun-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-173T07:42:00,002T19:00:00,22-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-173T09:00:00,000T07:30:00,22-Jun-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-173T09:00:00,000T07:30:00,22-Jun-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-173T09:00:00,000T07:30:00,22-Jun-11,VIMS,SPASS Rider,Titan,TEA,,TEA,TEA - Titan Monitoring Campaign,,,,,, 2011-173T20:42:00,000T09:00:00,22-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-173T21:42:00,000T08:00:00,22-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11173_SP,rider,,,,,, 2011-174T05:42:00,000T21:00:00,23-Jun-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-174T05:42:00,000T21:00:00,23-Jun-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-174T05:42:00,000T21:00:00,23-Jun-11,VIMS,SPASS Rider,Titan,TEA,,TEA,TEA - Titan Monitoring Campaign,,,,,, 2011-175T02:42:00,000T09:00:00,24-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-175T03:42:00,000T08:00:00,24-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11175_SP,rider,,,,,, 2011-175T11:42:00,000T15:00:00,24-Jun-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition low phase,,,,,, 2011-175T11:42:00,000T15:00:00,24-Jun-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-175T11:42:00,000T15:00:00,24-Jun-11,VIMS,SPASS Rider,Titan,TEA,,TEA,TEA - Titan Monitoring Campaign,,,,,, 2011-175T11:42:00,008T23:27:59,24-Jun-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-175T11:42:00,005T08:14:00,24-Jun-11,CDA,Non-SPASS,Other,RATE010B,,Data rate End:SApo,Range enter= 14.001953 Rs exit= 14.007414 Range altitude= -1595.2083 km ... 5303.2338,,,,,, 2011-175T11:42:00,001T00:00:00,24-Jun-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-175T12:00:00,000T01:08:00,24-Jun-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-176T02:42:00,002T08:59:00,25-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-176T02:42:00,004T17:14:00,25-Jun-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 250 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_149_150",,,,,, 2011-176T02:42:00,004T17:14:00,25-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-176T02:42:00,000T09:00:00,25-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-176T03:42:00,000T08:00:00,25-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11176_SP,rider,,,,,, 2011-176T11:42:00,001T13:29:00,25-Jun-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-176T11:42:00,000T13:29:00,25-Jun-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-176T11:42:00,004T08:14:00,25-Jun-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-177T19:56:00,000T20:00:00,26-Jun-11,CDA,SPASS Rider,DustRAM direction,ISD0030,,CDA ISD 2011-180T19:56:00,ISD observation around apoapse 2011-180T19:56:00 45.692357 Rs,,,,,, 2011-178T02:41:00,000T09:00:00,27-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-178T03:41:00,000T08:00:00,27-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11178_SP,rider,,,,,, 2011-178T11:41:00,000T08:00:00,27-Jun-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-178T19:41:00,001T05:15:00,27-Jun-11,CDA,Prime,DustRAM direction,ISD0030,,CDA ISD 2011-180T19:56:00,ISD observation around apoapse 2011-180T19:56:00 45.692357 Rs,,,,,, 2011-178T19:41:00,001T21:45:00,27-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-180T02:26:00,000T09:00:00,29-Jun-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-180T03:26:00,000T08:00:00,29-Jun-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_149IC_DSCAL11180_SP,rider,,,,,, 2011-180T11:26:00,001T13:30:00,29-Jun-11,CDA,Prime,DustRAM direction,ISD0030,,CDA ISD 2011-180T19:56:00,ISD observation around apoapse 2011-180T19:56:00 45.692357 Rs,,,,,, 2011-180T17:26:00,000T05:00:00,29-Jun-11,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2011-180T19:56:00,003T15:14:00,29-Jun-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S69,Range enter= 14.001953 Rs exit= 14.007414 Range altitude= -1595.2083 km ... 5303.2338,,,,,, 2011-180T19:56:00,000T02:00:00,29-Jun-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-180T19:56:00,003T15:14:00,29-Jun-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_149_150",,,,,, 2011-180T19:56:00,003T15:14:00,29-Jun-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-180T19:56:07,000T00:00:01,29-Jun-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 21.7 d, inc = 0.4 deg, r = 45.646 Rs, phase = 45 deg",,,,,, 2011-180T21:56:00,003T13:14:00,29-Jun-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-180T22:26:00,003T12:44:00,29-Jun-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-182T02:26:00,000T09:00:00,1-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-182T03:26:00,000T08:00:00,1-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11182_SP,rider,,,,,, 2011-182T11:26:00,001T13:14:00,1-Jul-11,CDA,Prime,DustRAM direction,ISD0030,,CDA ISD 2011-180T19:56:00,ISD observation around apoapse 2011-180T19:56:00 45.692357 Rs,,,,,, 2011-182T16:00:00,000T07:00:00,1-Jul-11,ISS,Non-SPASS,InstrumentCalibration,WACDARK,ISS Wide Angle Camera dark current calibration,ISS WAC dark current calibration,ISS WAC dark current calibration,,,,,, 2011-182T23:00:00,000T07:00:00,1-Jul-11,ISS,Non-SPASS,InstrumentCalibration,NACDARK,ISS Narrow Angle Camera dark current calibration,ISS NAC dark current calibration,ISS NAC dark current calibration,,,,,, 2011-184T02:10:00,000T09:00:00,3-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-184T03:10:00,000T08:00:00,3-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11184_SP,rider,,,,,, 2011-184T11:10:00,005T23:43:59,3-Jul-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-184T11:10:00,006T03:22:58,3-Jul-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S69,Range enter= 14.001953 Rs exit= 14.007414 Range altitude= -1595.2083 km ... 5303.2338,,,,,, 2011-184T11:10:00,000T00:43:00,3-Jul-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-184T11:10:00,005T23:44:00,3-Jul-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-184T11:10:00,005T23:44:00,3-Jul-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_150",,,,,, 2011-184T11:10:00,005T23:44:00,3-Jul-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-184T11:15:00,000T00:02:00,3-Jul-11,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S69 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2011-184T11:53:00,000T00:07:00,3-Jul-11,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-184T12:00:00,000T00:05:00,3-Jul-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-184T12:05:00,000T00:33:00,3-Jul-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-184T12:38:00,000T00:30:00,3-Jul-11,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2011-184T13:00:00,000T01:30:00,3-Jul-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 70.6 requested range 3.4 Mkm",,,,,, 2011-184T13:00:00,000T01:30:00,3-Jul-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-184T13:00:00,000T01:30:00,3-Jul-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 71 deg, range = 3.4 Mkm.",,,,,, 2011-184T13:08:00,003T22:52:00,3-Jul-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-184T14:30:00,000T01:00:00,3-Jul-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-184T15:30:00,000T18:00:00,3-Jul-11,VIMS,Prime,rings(general),EG60PHASE,,E/G Ring phase observation,"Target 167,500 km on the LEFT ansa and stare for the entire time.",,,,,, 2011-184T15:30:00,000T18:00:00,3-Jul-11,CIRS,SPASS Rider,rings(general),EG60PHASE,,,null,,,,,, 2011-184T15:30:00,000T18:00:00,3-Jul-11,ISS,Non-SPASS,rings(general),EG60PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2011-185T09:30:00,000T23:30:00,4-Jul-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-186T12:10:00,000T09:00:00,5-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-186T13:10:00,000T08:00:00,5-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11186_SP,rider,,,,,, 2011-186T23:00:00,000T01:00:00,5-Jul-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-187T00:00:00,000T23:00:00,6-Jul-11,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-188T01:55:00,000T09:00:00,7-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-188T02:55:00,000T08:00:00,7-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11188_SP,rider,,,,,, 2011-188T12:00:00,000T00:34:00,7-Jul-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-188T12:34:00,001T08:56:00,7-Jul-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-188T22:00:00,000T12:00:00,7-Jul-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-189T10:00:00,000T11:00:00,8-Jul-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-189T19:00:00,000T03:00:00,8-Jul-11,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2011-189T19:01:20,000T00:00:01,8-Jul-11,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2011-189T21:30:00,000T02:00:00,8-Jul-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-189T22:00:00,000T02:24:00,8-Jul-11,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2011-189T23:30:00,000T11:24:00,8-Jul-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-190T00:00:00,000T01:08:00,9-Jul-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-190T01:54:00,000T09:00:00,9-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-190T02:54:00,000T08:00:00,9-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11190_SP,rider,,,,,, 2011-190T10:54:00,003T23:44:59,9-Jul-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-190T10:54:00,000T01:54:11,9-Jul-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-190T10:54:00,001T02:46:00,9-Jul-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-190T10:54:00,003T23:45:00,9-Jul-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_150",,,,,, 2011-190T10:54:00,002T09:13:00,9-Jul-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-190T11:34:00,000T11:55:00,9-Jul-11,VIMS,Prime,Saturn,EQUATMAP,,Saturn Equatorial Mosaic,"2 (rows)x3(columns) Regional mosaics, one collected each 57 minutes throughout the 12-hrs duration. Mosaic is centered at the equator. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 9.5-minute intervals between frame centers (7 mins for science, 2.5 for repositioning). Each of these mosaics should take 57 minutes",,,,,, 2011-190T11:34:00,000T11:55:00,9-Jul-11,CIRS,SPASS Rider,Saturn,EQUATMAP,,Rider,VIMS rider,,,,,, 2011-190T11:34:00,000T11:55:00,9-Jul-11,ISS,Non-SPASS,Saturn,EQUATMAP,,Night NAC lightning search,Rider on VIMS to search for lightning spectrum at the night side with NAC and to monitor clouds illuminated by rings with WAC.,,,,,, 2011-190T12:48:11,000T23:00:00,9-Jul-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-190T14:32:58,002T02:54:00,9-Jul-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.994705 Rs exit= 13.997132 Range altitude= 5297.9182 km ... -1272.2958 Info: provides the necessary rate for the Dust Shadow PIE,,,,,, 2011-190T23:39:00,000T11:00:00,9-Jul-11,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev151 Saturn atmospheric occultation on 2011/213. DSS-34 required for X- and Ka-band support.",,,,,, 2011-191T01:39:00,000T09:00:00,10-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-191T02:39:00,000T08:00:00,10-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11191_SP,rider,,,,,, 2011-191T08:00:00,000T03:48:00,10-Jul-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-191T11:02:00,000T03:18:00,10-Jul-11,CDA,Prime,Other,RINGSHAD,,CDA Ring Shadow Crossing1_5Rs,CDA Ring Shadow Crossing @ 5Rs; objective code RC1a,,,,,, 2011-191T11:48:00,000T02:00:00,10-Jul-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-191T11:48:11,000T00:30:00,10-Jul-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-191T11:49:58,000T02:00:00,10-Jul-11,CDA,SPASS Rider,DustRAM direction,RPX0150,,CDA RPXing 2011-191T12:49:58,RPXing at 4.5795861 Rs,,,,,, 2011-191T12:18:11,000T01:30:00,10-Jul-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-191T13:40:00,000T04:45:00,10-Jul-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-191T13:48:00,000T10:12:00,10-Jul-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-191T13:48:11,000T23:00:00,10-Jul-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-191T14:58:00,000T01:58:00,10-Jul-11,VIMS,Prime,Saturn,EQUATMAP,,Saturn Equatorial Mosaic,"2 (rows)x3(columns) Regional mosaics, one collected each 57 minutes throughout the 2-hrs duration. Mosaic centered at the Equator at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 9 mi 30 sec intervals between frame centers (7 mins for science, 2 min 30 secs for repositioning). Each of these mosaics should take 57 min",,,,,, 2011-191T14:58:00,000T01:58:00,10-Jul-11,CIRS,SPASS Rider,Saturn,EQUATMAP,,Rider,VIMS rider,,,,,, 2011-191T14:58:00,000T01:58:00,10-Jul-11,ISS,Non-SPASS,Saturn,EQUATMAP,,Night NAC lightning search,Rider on VIMS to search for lightning spectrum at the night side with NAC and to monitor clouds illuminated by rings with WAC.,,,,,, 2011-191T15:59:41,000T00:00:01,10-Jul-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.039 Rs, lat = -0 deg, phase = 135 deg",,,,,, 2011-191T16:56:00,000T02:12:00,10-Jul-11,VIMS,Prime,Saturn,ALPORIOCC,Alpha Orion occultation,alpOri Saturn occultation,"alpOri atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. After the occ, at time 17:59, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation occurred (latitude 60.4N).",,,,,, 2011-191T16:56:00,000T02:12:00,10-Jul-11,CIRS,,Saturn,ALPORIOCC,Alpha Orion occultation,CIRS_150SA_ALPORIOCC001_VIMS,"PIE Collaboration with VIMS. Stellar Occ Saturn ingress T17:39 60N dark limb, T1759 integrate on limb at 60N",,,,,, 2011-191T18:25:00,002T16:14:00,10-Jul-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-191T19:08:00,000T02:10:00,10-Jul-11,VIMS,Prime,Saturn,ALPCMIOCC,Alpha CMI occultation,alpCMi Saturn occultation,"alpCMi atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Point at star until 20:08 and then do CIRS limb stare.",,,,,, 2011-191T19:08:00,000T02:10:00,10-Jul-11,CIRS,,Saturn,ALPCMIOCC,Alpha CMI occultation,CIRS_150SA_ALPCMIOCC001_VIMS,Collab with VIMS. Stellar Occ Saturn ingress T19:26 35N dark limb at T20:08 do limb integration 1 hr 3 latitudes,,,,,, 2011-191T21:18:00,000T02:11:00,10-Jul-11,VIMS,Prime,Saturn,EQUATMAP,,Saturn Equatorial Mosaic,"2 (rows)x3(columns) Regional mosaics, one collected each 57 minutes throughout the 2-hrs duration. MOsaic centered at the equator at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 9 mi 30 sec intervals between frame centers (7 mins for science, 2 min 30 secs for repositioning). Each of these mosaics should take 57 min",,,,,, 2011-191T21:18:00,000T02:11:00,10-Jul-11,CIRS,SPASS Rider,Saturn,EQUATMAP,,Rider,VIMS rider,,,,,, 2011-191T21:18:00,000T02:11:00,10-Jul-11,ISS,Non-SPASS,Saturn,EQUATMAP,,Night NAC lightning search,Rider on VIMS to search for lightning spectrum at the night side with NAC and to monitor clouds illuminated by rings with WAC.,,,,,, 2011-192T01:39:00,000T09:00:00,11-Jul-11,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev151 Saturn atmospheric occultation on 2011/213. DSS-43 required for X- and S-band support.",,,,,, 2011-192T01:39:00,000T09:00:00,11-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-192T02:39:00,000T08:00:00,11-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11192_SP,rider,,,,,, 2011-192T11:19:00,000T01:30:00,11-Jul-11,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 54.7 requested range 1.8 Mkm",,,,,, 2011-192T11:19:00,000T01:30:00,11-Jul-11,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-192T11:19:00,000T01:30:00,11-Jul-11,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 55 deg, range = 1.8 Mkm.",,,,,, 2011-192T12:48:11,001T21:50:49,11-Jul-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-192T12:49:00,000T11:40:00,11-Jul-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere. Here is a high spatial res observation 12.2-16.3Rs. Target 1N. Rings are ~edge-on. FP1 offset (left) for H2O. Low phase, with ORS riders, including UVIS slit.",,,,,, 2011-192T12:49:00,000T11:40:00,11-Jul-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn CIRS COMPSIT Ridealong,Ridealong with CIRS,,,,,, 2011-192T12:49:00,000T11:40:00,11-Jul-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-192T17:26:58,009T18:43:02,11-Jul-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.009839 Rs exit= 14.011002 Range altitude= -1269.8391 km ... 5325.1842,,,,,, 2011-192T20:07:00,001T14:32:00,11-Jul-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-193T00:29:00,000T23:00:00,12-Jul-11,VIMS,Prime,Saturn,NHEMMOVIE,,Saturn Equatorial Mosaic,"3 (rows)x3(columns) Regional mosaics, one collected each 85.5 minutes throughout the 23:40-hrs duration. Lowest row (tier) of the mosaic is centered at the equator at the sub-S/C Saturn longitude. Each mosaic comprised of 3 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 9 mi 30 sec intervals between frame centers (7 mins for science, 2 min 30 secs for repositioning). Each of these mosaics should take 85.5 min",,,,,, 2011-193T00:29:00,000T23:00:00,12-Jul-11,ISS,SPASS Rider,Saturn,NHEMMOVIE,,Day WAC at the corners of 3x3,Rider on VIMS to monitor day side clouds in WAC every hour copied from ISS_140SA_REGMAP003_VIMS,,,,,, 2011-194T01:39:00,000T09:00:00,13-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-194T02:39:00,000T08:00:00,13-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11194_SP,rider,,,,,, 2011-194T10:39:00,016T16:27:59,13-Jul-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-194T10:39:00,008T01:31:00,13-Jul-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-194T10:39:00,000T23:21:00,13-Jul-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-194T10:39:00,008T01:31:00,13-Jul-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_150_151",,,,,, 2011-194T10:39:00,008T01:31:00,13-Jul-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-194T11:18:00,000T00:02:00,13-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-194T11:20:00,000T14:40:00,13-Jul-11,ISS,Prime,RingE,ERNGVRLP,,Low-Phase Edge-on obs E-ring observation after Eq,Low elevation observation of E ring at low phase.,,,,,, 2011-194T11:20:00,000T14:40:00,13-Jul-11,CIRS,SPASS Rider,rings(general),ERNGVRLP,,,null,,,,,, 2011-194T11:20:00,000T14:40:00,13-Jul-11,VIMS,SPASS Rider,RingE,ERNGVRLP,,E Ring observation,"E Ring observation, 1 second integration time",,,,,, 2011-195T01:58:00,000T00:02:00,14-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-195T02:00:00,000T05:00:00,14-Jul-11,ISS,Prime,Other,RHEAL4,,Rhea L4 satellite search,Satellite search around Rhea L4 Lagrange point.,,,,,, 2011-195T06:58:00,000T00:02:00,14-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-195T07:00:00,000T03:00:00,14-Jul-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2011-195T09:58:00,000T00:02:00,14-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-195T10:00:00,000T08:00:00,14-Jul-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-195T17:58:00,000T00:02:00,14-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-195T18:00:00,000T01:30:00,14-Jul-11,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 11.4 requested range 2.7 Mkm",,,,,, 2011-195T18:00:00,000T01:30:00,14-Jul-11,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-195T18:00:00,000T01:30:00,14-Jul-11,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 11 deg, range = 2.7 Mkm.",,,,,, 2011-195T18:00:00,015T09:07:00,14-Jul-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-195T19:28:00,000T00:02:00,14-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-195T19:30:00,000T02:30:00,14-Jul-11,ISS,Prime,Tethys,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Tethys across Titan","Images of mutual event, transit of Tethys across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-195T21:58:00,000T00:02:00,14-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-196T01:24:00,000T09:00:00,15-Jul-11,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev151 Saturn atmospheric occultation on 2011/213. DSS-34 required for X- and Ka-band support.",,,,,, 2011-196T01:24:00,000T09:00:00,15-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-196T02:24:00,000T08:00:00,15-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11196_SP,rider,,,,,, 2011-196T10:24:00,001T23:29:00,15-Jul-11,CDA,Prime,DustRAM direction,RETROGRAD,,CDA Apoapse Retrograde,Retrograde observation outbound to apoapse,,,,,, 2011-198T11:23:00,000T09:00:00,17-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-198T12:23:00,000T08:00:00,17-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11198_SP,rider,,,,,, 2011-198T20:58:00,000T00:02:00,17-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-198T21:00:00,000T01:30:00,17-Jul-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 45.7 requested range 3.6 Mkm",,,,,, 2011-198T21:00:00,000T01:30:00,17-Jul-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-198T21:00:00,000T01:30:00,17-Jul-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 46 deg, range = 3.6 Mkm.",,,,,, 2011-198T22:28:00,000T00:02:00,17-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-198T22:30:00,000T02:00:00,17-Jul-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-199T00:28:00,000T00:02:00,18-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-199T00:30:00,000T01:30:00,18-Jul-11,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Rhea","Images of mutual event, transit of Dione across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-199T01:58:00,000T00:02:00,18-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-199T02:00:00,001T08:00:00,18-Jul-11,UVIS,Prime,Saturn,MOS150APO,,,"System scan of Saturn magnetosphere to image hydrogen and oxygen, day 1. One 32.0-hr block of time. Combined day 1 and day 2 scan patterns form three swaths from +/- 4 Rs E-W which extend out to ~+/-4 Rs N-S. Note: data to be taken only when slit is stationary. 0) Start at Saturn center. EUV and FUV low resolution slits on. Align slit with Saturn spin axis. Start data capture, stare 541.0 s, stop data capture. 1) Repeat PATTERN A 61 times. 2) Slew +64 mrad about x axis. Start data capture, stare 541.0 s, stop data capture. 3) Repeat PATTERN B 122 times. PATTERN A: Slew +1.5 mrad about z-axis. Start data capture, stare 541.0 s, stop data capture. PATTERN B: Slew -1.5 mrad about z-axis. Start data capture, stare 541.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (2238.09337 bps, from Alain's spreadsheet)x(541.0s per stare)x(185 stares) ~ 224x10^6 bits",,,,,, 2011-199T12:10:00,000T20:00:00,18-Jul-11,CDA,SPASS Rider,DustRAM direction,ISD0031,,CDA ISD 2011-202T12:10:00,ISD observation around apoapse 2011-202T12:10:00 45.706274 Rs,,,,,, 2011-200T09:58:00,000T00:02:00,19-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-200T18:53:00,000T09:00:00,19-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-200T19:53:00,000T08:00:00,19-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_150IC_DSCAL11200_SP,rider,,,,,, 2011-201T04:28:00,000T00:02:00,20-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-201T04:30:00,000T00:30:00,20-Jul-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-201T04:58:00,000T00:02:00,20-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-201T05:00:00,001T08:00:00,20-Jul-11,UVIS,Prime,Saturn,MOS150APO,,,"System scan of Saturn magnetosphere to image hydrogen and oxygen, day 2. One 32.0-hr block of time. Combined day 1 and day 2 scan patterns form three swaths from +/- 4 Rs E-W which extend out to ~+/-4 Rs N-S. Note: data to be taken only when slit is stationary. 0) Start at Saturn center. EUV and FUV low resolution slits on. Align slit with Saturn spin axis. Start data capture, stare 571.0 s, stop data capture. 1) Repeat PATTERN A 58 times. 2) Slew -64 mrad about x axis. Start data capture, stare 571.0 s, stop data capture. 3) Repeat PATTERN B 116 times. PATTERN A: Slew -1.5 mrad about z-axis. Start data capture, stare 571.0 s, stop data capture. PATTERN B: Slew +1.5 mrad about z-axis. Start data capture, stare 571.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (2120.50528 bps, from Alain's spreadsheet)x(571.0s per stare)x(176 stares) ~ 213.1x10^6 bits",,,,,, 2011-201T06:10:00,000T20:00:00,20-Jul-11,CDA,SPASS Rider,DustRAM direction,ISD0031,,CDA ISD 2011-202T12:10:00,ISD observation around apoapse 2011-202T12:10:00 45.706274 Rs,,,,,, 2011-202T12:10:00,009T18:34:58,21-Jul-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.009839 Rs exit= 14.011002 Range altitude= -1269.8391 km ... 5325.1842,,,,,, 2011-202T12:10:00,000T02:00:00,21-Jul-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-202T12:10:00,008T14:57:00,21-Jul-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_150_151",,,,,, 2011-202T12:10:00,008T14:57:00,21-Jul-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-202T12:10:21,000T00:00:01,21-Jul-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 21.7 d, inc = 0.4 deg, r = 45.664 Rs, phase = 45 deg",,,,,, 2011-202T12:58:00,000T00:02:00,21-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-202T14:10:00,008T12:57:00,21-Jul-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-202T14:38:00,000T13:00:00,21-Jul-11,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,"RSS USO characterization plus PIM. Pointing=XBAND to Earth. No rolling during 3-hour USO from 2011-202T18:38:00 till 2011-202T21:38:00, to be tracked at DSS-25 in 1-way mode. Keep Ka-band ON till end of downlink to satisfy PIM requirement.",,,,,, 2011-202T18:38:00,000T09:00:00,21-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-202T19:38:00,000T08:00:00,21-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11202_SP,rider,,,,,, 2011-203T03:38:00,001T02:22:00,22-Jul-11,CDA,Prime,DustRAM direction,ISD0031,,CDA ISD 2011-202T12:10:00,ISD observation around apoapse 2011-202T12:10:00 45.706274 Rs,,,,,, 2011-204T06:00:00,000T11:08:00,23-Jul-11,VIMS,Prime,Star,TRANSIT,,Exoplanet transit observation,"Stare at RA/Dec, acquire transit of stellar disk using occultation and/or imaging modes",,,,,, 2011-204T06:00:00,000T11:08:00,23-Jul-11,ISS,SPASS Rider,Star,TRANSIT,,EXOPLANET TRANSIT,ISS rider on a VIMS exo-planet transit observation of HD189733. BOTSIMS to provide starfield,,,,,, 2011-204T16:10:00,000T20:00:00,23-Jul-11,CDA,SPASS Rider,DustRAM direction,ISD0031,,CDA ISD 2011-202T12:10:00,ISD observation around apoapse 2011-202T12:10:00 45.706274 Rs,,,,,, 2011-204T17:08:00,000T10:30:00,23-Jul-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-204T18:38:00,000T09:00:00,23-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-204T19:38:00,000T08:00:00,23-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11204_SP,rider,,,,,, 2011-205T00:00:00,000T01:08:00,24-Jul-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-205T03:38:00,000T11:22:00,24-Jul-11,VIMS,Prime,Star,TRANSIT,,Exoplanet transit observation,"Stare at RA/Dec, acquire transit of stellar disk using occultation and/or imaging modes",,,,,, 2011-205T03:38:00,000T11:22:00,24-Jul-11,ISS,SPASS Rider,Star,TRANSIT,,EXOPLANET TRANSIT,ISS rider on a VIMS exo-planet transit observation of HD189733. BOTSIMS to provide starfield,,,,,, 2011-205T15:58:00,000T00:02:00,24-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-205T16:00:00,000T01:30:00,24-Jul-11,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 63.6 requested range 1.5 Mkm",,,,,, 2011-205T16:00:00,000T01:30:00,24-Jul-11,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-205T16:00:00,000T01:30:00,24-Jul-11,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 64 deg, range = 1.5 Mkm.",,,,,, 2011-205T17:28:00,000T00:02:00,24-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-205T17:30:00,000T04:00:00,24-Jul-11,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2011-205T17:30:00,000T04:00:00,24-Jul-11,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2011-205T21:28:00,000T00:02:00,24-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-205T21:30:00,000T18:30:00,24-Jul-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-206T15:58:00,000T00:02:00,25-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-206T18:22:00,000T09:00:00,25-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-206T19:22:00,000T08:00:00,25-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11206_SP,rider,,,,,, 2011-206T20:00:00,002T00:00:00,25-Jul-11,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Apoapse Retrograde,Retrograde observation inbound towards Hyperion,,,,,, 2011-207T03:58:00,000T00:02:00,26-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-207T04:00:00,000T01:00:00,26-Jul-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-207T04:58:00,000T00:02:00,26-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-207T05:00:00,000T23:00:00,26-Jul-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-208T03:58:00,000T00:02:00,27-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-208T05:00:00,000T11:52:00,27-Jul-11,VIMS,Prime,Star,STARCAL,Star calibration,6-star calibration,"Stare at RA/Dec for selected stars to acquire spectra, at tau_IR between 40 and 640 msec. Valid targets: alp CMa (101.2871/-16.7161), L2Pup (108.3846/-44.6397), alp Car(95.9883/-52.6956), R Aql(286.5921/8.2300), X Oph (279.5871/8.8339), and R Lyr (283.8333/43.9461).",,,,,, 2011-208T18:22:00,000T09:00:00,27-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-208T19:22:00,000T08:00:00,27-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11208_SP,rider,,,,,, 2011-209T11:28:00,000T00:02:00,28-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-209T11:30:00,000T12:00:00,28-Jul-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-209T11:30:00,000T12:00:00,28-Jul-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-209T23:28:00,000T00:02:00,28-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-209T23:30:00,000T11:00:00,28-Jul-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-210T10:28:00,000T00:02:00,29-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-210T12:00:00,000T02:00:00,29-Jul-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-210T13:58:00,000T00:02:00,29-Jul-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-210T18:07:00,000T09:00:00,29-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-210T19:07:00,000T08:00:00,29-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11210_SP,rider,,,,,, 2011-211T03:07:00,008T05:59:00,30-Jul-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-211T03:07:00,001T01:52:56,30-Jul-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-211T03:07:00,002T02:48:00,30-Jul-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-211T03:07:00,013T02:55:00,30-Jul-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_151_152",,,,,, 2011-211T03:07:00,008T05:59:00,30-Jul-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 250 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-211T03:07:00,001T00:58:00,30-Jul-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-211T03:47:00,000T16:30:00,30-Jul-11,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-211T20:17:00,000T16:00:00,30-Jul-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-211T20:17:00,000T16:00:00,30-Jul-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-211T20:17:00,000T16:00:00,30-Jul-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-212T04:05:00,000T22:58:00,31-Jul-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-212T04:59:56,000T23:00:00,31-Jul-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-212T06:44:58,000T20:17:00,31-Jul-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.998297 Rs exit= 13.993331 Range altitude= 5319.8381 km ... -1246.8114,,,,,, 2011-212T12:26:00,000T04:00:00,31-Jul-11,CIRS,Prime,Saturn,NADIROCC,Occultation,NADIROCC egress,"Helium abundance measurement at the RSS egress occultation point. If RSS request deleted, this can be, too. IF RSS observes both ingress & egress, the NADIROCC that best fits the timeline can be chosen Ingress 56.6N graphic Egress 48.3N graphic",,,,,, 2011-212T16:00:00,000T11:03:00,31-Jul-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-212T18:06:00,000T09:00:00,31-Jul-11,RSS,SPASS Rider,Saturn,KADOWN,RSS Ka-Band downlink,Gravity Science Enhancement (GSE),"Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-25 (or DSS-26) required for X- and Ka-band support.",,,,,, 2011-212T18:06:00,000T09:00:00,31-Jul-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-212T19:06:00,000T08:00:00,31-Jul-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11212_SP,rider,,,,,, 2011-213T01:01:00,000T02:05:00,1-Aug-11,RSS,SPASS Rider,Saturn,THERMAL,Thermal stabilization period,RSS Thermal Stabilization 151 pre-Occ,null,,,,,, 2011-213T03:01:58,000T04:00:00,1-Aug-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.998297 Rs exit= 13.993331 Range altitude= 5319.8381 km ... -1246.8114,,,,,, 2011-213T03:03:00,001T09:16:00,1-Aug-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-213T03:26:00,000T02:25:00,1-Aug-11,RSS,Prime,Saturn,OCCSIANDE,,RSS SA Atmospheric Occultation Ingress &Egress,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2011-213T03:59:00,000T02:00:00,1-Aug-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-213T03:59:56,000T00:30:00,1-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-213T04:01:58,000T02:00:00,1-Aug-11,CDA,SPASS Rider,DustRAM direction,RPX0160,,CDA RPXing 2011-213T05:01:58,RPXing at 4.5880786 Rs,,,,,, 2011-213T04:29:56,000T01:30:00,1-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-213T05:55:00,000T04:40:00,1-Aug-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-213T05:59:56,000T23:00:00,1-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-213T06:51:00,000T02:20:00,1-Aug-11,VIMS,Prime,Saturn,HRESPLUME,,Saturn Hi Res equatorial Plume Imag,"A single 2 (rows)x7(columns) of the equatorial region, centered on the equator. Mosaic comprised of 2 rows of 7 frames each, oriented with the 7 frames in the east-west direction. 10-minute intervals between frame centers (7 mins for science, 3.0 for repositioning).",,,,,, 2011-213T06:51:00,000T02:20:00,1-Aug-11,CIRS,SPASS Rider,Saturn,HRESPLUME,,Rider,VIMS rider,,,,,, 2011-213T07:01:58,001T02:37:00,1-Aug-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.998297 Rs exit= 13.993331 Range altitude= 5319.8381 km ... -1246.8114,,,,,, 2011-213T08:12:28,000T00:00:01,1-Aug-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.045 Rs, lat = -0 deg, phase = 135 deg",,,,,, 2011-213T09:11:00,000T02:09:00,1-Aug-11,VIMS,Prime,Saturn,ALPORIOCC,Alpha Orion occultation,alpOri Saturn occultation,"alpOri atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. DO occultation first, turn to limb ingress point (60N) at time 10:04.",,,,,, 2011-213T09:11:00,000T02:09:00,1-Aug-11,CIRS,,Saturn,ALPORIOCC,Alpha Orion occultation,CIRS_151SA_ALPORIOCC001_VIMS,Collab with VIMS. Stellar Occ Saturn Do CIRS limb stare first then go to star at 09:10 ingress T09:51 58N dark limb,,,,,, 2011-213T10:35:00,002T10:26:00,1-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-213T11:20:00,000T02:10:00,1-Aug-11,VIMS,Prime,Saturn,ALPCMIOCC,Alpha CMI occultation,alpCMi Saturn occultation,"alpCMi atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. Do occultation first, turn to limb ingress point (32.7N) at time 11:58.",,,,,, 2011-213T11:20:00,000T02:10:00,1-Aug-11,CIRS,,Saturn,ALPCMIOCC,Alpha CMI occultation,CIRS_151SA_ALPCMIOCC001_VIMS,Collab with VIMS. Stellar Occ Saturn ingress T11:38 33N dark limb T11:59 go to limb for CIRS integration,,,,,, 2011-213T13:30:00,000T07:04:00,1-Aug-11,VIMS,Prime,Saturn,HRESPLUME,,Saturn Hi Res equatorial Plume Imag,"7 mosaics, each 2 (rows)x3(columns) of the equatorial region, centered on the equator. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 10-minute intervals between frame centers (7 mins for science, 3.0 for repositioning).",,,,,, 2011-213T13:30:00,000T07:04:00,1-Aug-11,CIRS,SPASS Rider,Saturn,HRESPLUME,,Rider,VIMS rider,,,,,, 2011-213T13:30:00,000T07:04:00,1-Aug-11,ISS,Non-SPASS,Saturn,HRESPLUME,,Day WAC VIMS rider,"VIMS day WAC rider. 7 mosaics, each 2 (rows)x3(columns) of the equatorial region, centered on the equator. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 10-minute intervals between frame centers",,,,,, 2011-213T20:34:00,000T01:04:00,1-Aug-11,UVIS,Prime,Rhea,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to eps Ori to look for volatiles.,,,,,, 2011-213T20:34:00,000T01:04:00,1-Aug-11,CIRS,SPASS Rider,Rhea,ICYEX,,,null,,,,,, 2011-213T20:34:00,000T01:04:00,1-Aug-11,ISS,SPASS Rider,Rhea,ICYEXO,Icy satellite exosphere,Rhea stellar occ. (Orion Belt stars),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-213T20:34:00,000T01:04:00,1-Aug-11,VIMS,SPASS Rider,Rhea,ICYEXO,Icy satellite exosphere,Rhea occultation,Rhea occultation,,,,,, 2011-213T21:38:00,000T18:00:00,1-Aug-11,VIMS,Prime,Saturn,HRESPEARL,,Saturn Hi Res String of Pearls Imag,"18 mosaics, each 2 (rows)x3(columns) of the String of Pearls region, centered at 33.5 degrees latitude (planetocentric). Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 10-minute intervals between frame centers (7 mins for science, 3.0 for repositioning).",,,,,, 2011-213T21:38:00,000T18:00:00,1-Aug-11,CIRS,SPASS Rider,Saturn,HRESPEARL,,Rider,VIMS rider,,,,,, 2011-213T21:38:00,000T18:00:00,1-Aug-11,ISS,Non-SPASS,Saturn,HRESPEARL,,Day WAC VIMS rider,"VIMS day WAC rider. 18 mosaics, each 2 (rows)x3(columns) of the String of Pearls region, centered at 33.5 degrees latitude (planetocentric). Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 10-minute",,,,,, 2011-214T04:59:56,000T21:30:04,2-Aug-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-214T09:38:58,009T20:22:02,2-Aug-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.006049 Rs exit= 14.003014 Range altitude= -1244.2693 km ... 5385.9661,,,,,, 2011-214T12:19:00,009T17:42:00,2-Aug-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-214T17:51:00,000T09:00:00,2-Aug-11,RSS,SPASS Rider,Saturn,KADOWN,RSS Ka-Band downlink,Gravity Science Enhancement (GSE),"Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-25 (or DSS-26) required for X- and Ka-band support.",,,,,, 2011-214T17:51:00,000T09:00:00,2-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-214T18:51:00,000T08:00:00,2-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11214_SP,rider,,,,,, 2011-215T02:30:00,000T02:00:00,3-Aug-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-215T03:31:00,000T17:30:00,3-Aug-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-215T03:31:00,000T17:30:00,3-Aug-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-215T03:31:00,000T17:30:00,3-Aug-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-215T04:30:00,009T01:32:00,3-Aug-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-215T21:01:00,000T09:59:00,3-Aug-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-216T07:00:00,006T19:20:00,4-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-216T08:30:00,000T13:26:00,4-Aug-11,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-217T00:06:00,000T09:00:00,5-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-217T01:06:00,000T08:00:00,5-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11216_SP,rider,,,,,, 2011-217T09:46:00,000T02:00:00,5-Aug-11,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-217T09:46:00,000T02:00:00,5-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-217T11:46:00,000T09:00:00,5-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-217T20:46:00,000T02:00:00,5-Aug-11,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 2-9-2 template + polarimetry, 2-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-217T20:46:00,000T02:00:00,5-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-217T22:46:00,000T23:10:00,5-Aug-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-217T22:46:00,000T23:10:00,5-Aug-11,ISS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Saturn appearance monitoring,"Trigger 04040 repeated ~ every 2 hours, or at the beginning and the end of the shorter observation: Trigger description: WAC 1x1 CB2 2x2 BL1,GRN, MT2, 4x4 MT3. Exposures are locked for trigger reuse up to 122 deg phase.",,,,,, 2011-218T00:00:00,000T01:08:00,6-Aug-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-219T00:06:00,000T09:00:00,7-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-219T01:06:00,000T08:00:00,7-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11218_SP,rider,,,,,, 2011-219T09:06:00,011T23:13:00,7-Aug-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-219T09:46:00,000T01:30:00,7-Aug-11,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 55.4 requested range 1.5 Mkm",,,,,, 2011-219T09:46:00,000T01:30:00,7-Aug-11,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 55 deg, range = 1.5 Mkm.",,,,,, 2011-219T11:16:00,000T03:00:00,7-Aug-11,ISS,Prime,Saturn,WIND3HR,,"Wind measuring 3-8-3 template + polarimetry, 3-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-219T11:16:00,000T03:00:00,7-Aug-11,VIMS,SPASS Rider,Saturn,WIND3HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-219T11:16:00,000T03:00:00,7-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-219T14:16:00,000T08:00:00,7-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-219T22:16:00,000T03:00:00,7-Aug-11,ISS,Prime,Saturn,WIND3HR,,"Wind measuring 3-8-3 template + polarimetry, 3-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-219T22:16:00,000T03:00:00,7-Aug-11,VIMS,SPASS Rider,Saturn,WIND3HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-219T22:16:00,000T03:00:00,7-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-220T01:16:00,000T03:00:00,8-Aug-11,ISS,Prime,Saturn,WIND3HR,,"Wind measuring 3-8-3 template + polarimetry, 3-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-220T01:16:00,000T03:00:00,8-Aug-11,VIMS,SPASS Rider,Saturn,WIND3HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-220T01:16:00,000T03:00:00,8-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-220T04:16:00,000T08:00:00,8-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-220T04:16:00,000T08:00:00,8-Aug-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-220T12:16:00,000T03:00:00,8-Aug-11,ISS,Prime,Saturn,WIND3HR,,"Wind measuring 3-8-3 template + polarimetry, 3-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-220T12:16:00,000T03:00:00,8-Aug-11,VIMS,SPASS Rider,Saturn,WIND3HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-220T12:16:00,000T03:00:00,8-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-220T17:36:00,000T09:00:00,8-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-220T18:36:00,000T08:00:00,8-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11220_SP,rider,,,,,, 2011-221T03:16:00,000T01:30:00,9-Aug-11,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 35.3 requested range 1.4 Mkm",,,,,, 2011-221T03:16:00,000T01:30:00,9-Aug-11,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 35 deg, range = 1.4 Mkm.",,,,,, 2011-221T04:46:00,000T16:54:00,9-Aug-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-221T04:46:00,000T16:54:00,9-Aug-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-221T06:01:00,000T20:00:00,9-Aug-11,CDA,SPASS Rider,DustRAM direction,ISD0032,,CDA ISD 2011-224T06:01:00,ISD observation around apoapse 2011-224T06:01:00 45.930701 Rs,,,,,, 2011-221T21:40:00,000T05:00:00,9-Aug-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-221T21:40:00,000T05:00:00,9-Aug-11,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2011-221T21:40:00,000T05:00:00,9-Aug-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-221T21:40:00,000T05:00:00,9-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-222T02:40:00,000T06:00:00,10-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-222T02:40:00,000T06:00:00,10-Aug-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-222T08:40:00,000T05:00:00,10-Aug-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-222T08:40:00,000T05:00:00,10-Aug-11,CIRS,,Saturn,WIND5HR,,low emit COMPSIT near-Equator avoid rings,,,,,,, 2011-222T08:40:00,000T05:00:00,10-Aug-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-222T08:40:00,000T05:00:00,10-Aug-11,UVIS,Non-SPASS,Saturn,WIND,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-222T13:40:00,000T01:30:00,10-Aug-11,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 19.7 requested range 2 Mkm",,,,,, 2011-222T13:40:00,000T01:30:00,10-Aug-11,VIMS,SPASS Rider,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 20 deg, range = 2 Mkm.",,,,,, 2011-222T17:20:00,000T09:00:00,10-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-222T18:20:00,000T08:00:00,10-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_151IC_DSCAL11222_SP,rider,,,,,, 2011-223T00:01:00,000T20:00:00,11-Aug-11,CDA,SPASS Rider,DustRAM direction,ISD0032,,CDA ISD 2011-224T06:01:00,ISD observation around apoapse 2011-224T06:01:00 45.930701 Rs,,,,,, 2011-223T02:20:00,003T14:45:00,11-Aug-11,CAPS,Non-SPASS,Saturn,SURVYXTRA,,MAPS Survey,null,,,,,, 2011-223T02:20:00,003T14:45:00,11-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-223T02:20:00,003T14:45:00,11-Aug-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Sponge Bit Overlay,"Overlay: adding 250 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-223T03:00:00,000T11:00:00,11-Aug-11,ISS,Prime,Saturn,MOVIE,,"Global WAC Saturn movie, one of 2 time steps.","Stare and shoot every 1h 50 min to mosaic in longitude, part of the 2-time-step movie. CB2, MT2, MT3, RED, GRN, BL1, VIO, UV WAC. Cycled while observation lasts.",,,,,, 2011-223T03:00:00,000T11:00:00,11-Aug-11,CIRS,,Saturn,MOVIE,,low emit COMPSIT near-Equator avoid rings,,,,,,, 2011-223T03:00:00,000T11:00:00,11-Aug-11,UVIS,Non-SPASS,Saturn,MOVIE,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-223T06:00:00,000T04:40:00,11-Aug-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-223T06:30:00,000T02:16:32,11-Aug-11,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2011-223T14:00:00,000T14:10:00,11-Aug-11,ISS,Prime,Other,TAQROT,,Tarqeq,Observation of irregular moon of Saturn.,,,,,, 2011-224T04:10:00,000T11:00:00,12-Aug-11,ISS,Prime,Saturn,MOVIE,,"Global WAC Saturn movie, one of the 2 time steps.","Stare and shoot every 1h 50 min to mosaic in longitude, part of the 2-time-step movie. CB2, MT2, MT3, RED, GRN, BL1, VIO, UV WAC. Cycled while observation lasts.",,,,,, 2011-224T04:10:00,000T11:00:00,12-Aug-11,CIRS,,Saturn,MOVIE,,low emit COMPSIT near-Equator avoid rings,,,,,,, 2011-224T04:10:00,000T11:00:00,12-Aug-11,UVIS,Non-SPASS,Saturn,MOVIE,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-224T06:01:00,009T20:31:58,12-Aug-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.006049 Rs exit= 14.003014 Range altitude= -1244.2693 km ... 5385.9661,,,,,, 2011-224T06:01:37,000T00:00:01,12-Aug-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 21.8 d, inc = 0.4 deg, r = 45.884 Rs, phase = 45 deg",,,,,, 2011-224T06:02:00,000T02:00:00,12-Aug-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-224T06:02:00,012T19:32:00,12-Aug-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_151_152",,,,,, 2011-224T06:02:00,009T17:50:00,12-Aug-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-224T08:02:00,009T16:40:21,12-Aug-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-224T16:01:00,000T20:00:00,12-Aug-11,CDA,SPASS Rider,DustRAM direction,ISD0032,,CDA ISD 2011-224T06:01:00,ISD observation around apoapse 2011-224T06:01:00 45.930701 Rs,,,,,, 2011-224T17:20:00,000T09:00:00,12-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-224T18:20:00,000T08:00:00,12-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11224_SP,rider,,,,,, 2011-225T03:00:00,000T01:30:00,13-Aug-11,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 22.4 requested range 2.8 Mkm",,,,,, 2011-225T03:00:00,000T01:30:00,13-Aug-11,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 22 deg, range = 2.8 Mkm.",,,,,, 2011-225T04:30:00,000T05:00:00,13-Aug-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-225T04:30:00,000T05:00:00,13-Aug-11,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2011-225T04:30:00,000T05:00:00,13-Aug-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-225T05:00:00,000T02:16:32,13-Aug-11,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2011-225T09:30:00,000T06:00:00,13-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-225T09:30:00,000T06:00:00,13-Aug-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-225T15:30:00,000T05:00:00,13-Aug-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-225T15:30:00,000T05:00:00,13-Aug-11,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2011-225T15:30:00,000T05:00:00,13-Aug-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-225T15:30:00,000T05:00:00,13-Aug-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-225T20:30:00,000T05:00:00,13-Aug-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-225T20:30:00,000T05:00:00,13-Aug-11,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2011-225T20:30:00,000T05:00:00,13-Aug-11,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-225T20:30:00,000T05:00:00,13-Aug-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-226T01:30:00,000T06:00:00,14-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-226T01:30:00,000T06:00:00,14-Aug-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-226T07:30:00,000T05:00:00,14-Aug-11,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Stare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-226T07:30:00,000T05:00:00,14-Aug-11,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2011-226T07:30:00,000T05:00:00,14-Aug-11,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-226T10:01:00,000T20:00:00,14-Aug-11,CDA,SPASS Rider,DustRAM direction,ISD0032,,CDA ISD 2011-224T06:01:00,ISD observation around apoapse 2011-224T06:01:00 45.930701 Rs,,,,,, 2011-226T12:30:00,000T02:25:00,14-Aug-11,ISS,Prime,Saturn,MONITOR,,Saturn appearance monitoring,"monitoring trigger repeated ~ every 2 hours, or at the beginning and the end of the shorter observation:",,,,,, 2011-226T17:05:00,008T08:35:00,14-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-226T17:05:00,000T09:00:00,14-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-226T18:05:00,000T08:00:00,14-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11226_SP,rider,,,,,, 2011-227T02:45:00,000T16:00:00,15-Aug-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-227T02:45:00,000T16:00:00,15-Aug-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-227T18:45:00,000T09:10:00,15-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-227T18:48:00,000T09:07:00,15-Aug-11,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2011-228T03:55:00,000T11:00:00,16-Aug-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-228T14:55:00,000T11:47:00,16-Aug-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-228T17:05:00,000T09:00:00,16-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-228T18:05:00,000T08:00:00,16-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11228_SP,rider,,,,,, 2011-229T02:42:00,000T01:30:00,17-Aug-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 49.3 requested range 3.5 Mkm",,,,,, 2011-229T02:42:00,000T01:30:00,17-Aug-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 49 deg, range = 3.5 Mkm.",,,,,, 2011-229T04:12:00,000T04:00:00,17-Aug-11,ISS,Prime,Saturn,WIND4HR,,"Wind measuring 4-7-4 template + polarimetry, 4-hr","CHANGED to 3hrs to cut data volumeStare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-229T04:12:00,000T04:00:00,17-Aug-11,VIMS,SPASS Rider,Saturn,WIND4HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-229T04:12:00,000T04:00:00,17-Aug-11,UVIS,Non-SPASS,Saturn,WIND4HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-229T08:12:00,000T07:00:00,17-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-229T15:12:00,000T04:00:00,17-Aug-11,ISS,Prime,Saturn,WIND4HR,,"Wind measuring 4-7-4 template + polarimetry, 4-hr","CHANGED to 3hrs to cut data volumeStare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-229T15:12:00,000T04:00:00,17-Aug-11,VIMS,SPASS Rider,Saturn,WIND4HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-229T15:12:00,000T04:00:00,17-Aug-11,UVIS,Non-SPASS,Saturn,WIND4HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-229T19:12:00,000T04:00:00,17-Aug-11,ISS,Prime,Saturn,WIND4HR,,"Wind measuring 4-7-4 template + polarimetry, 4-hr","CHANGED to 3hrs to cut data volumeStare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-229T19:12:00,000T04:00:00,17-Aug-11,VIMS,SPASS Rider,Saturn,WIND4HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-229T19:12:00,000T04:00:00,17-Aug-11,UVIS,Non-SPASS,Saturn,WIND4HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-229T23:12:00,000T07:00:00,17-Aug-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-230T06:12:00,000T04:00:00,18-Aug-11,ISS,Prime,Saturn,WIND4HR,,"Wind measuring 4-7-4 template + polarimetry, 4-hr","CHANGED to 3hrs to cut data volumeStare and shoot every 10 min to mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2011-230T06:12:00,000T04:00:00,18-Aug-11,VIMS,SPASS Rider,Saturn,WIND4HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2011-230T06:12:00,000T04:00:00,18-Aug-11,UVIS,Non-SPASS,Saturn,WIND4HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2011-230T10:12:00,000T11:00:00,18-Aug-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-230T23:19:00,000T09:00:00,18-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-231T00:19:00,000T08:00:00,19-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11230_SP,rider,,,,,, 2011-231T08:19:00,005T17:14:59,19-Aug-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-231T08:19:00,005T17:15:00,19-Aug-11,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 250 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2011-231T08:59:00,000T01:30:00,19-Aug-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 73.2 requested range 3.1 Mkm",,,,,, 2011-231T08:59:00,000T01:30:00,19-Aug-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-231T08:59:00,000T01:30:00,19-Aug-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 73 deg, range = 3.1 Mkm.",,,,,, 2011-231T10:29:00,000T20:40:00,19-Aug-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-231T10:29:00,000T20:40:00,19-Aug-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-231T10:29:00,000T20:40:00,19-Aug-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-232T09:19:00,000T09:00:00,20-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-232T10:19:00,000T08:00:00,20-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11232_SP,rider,,,,,, 2011-232T18:59:00,000T11:00:00,20-Aug-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-233T05:59:00,000T01:10:00,21-Aug-11,ISS,Prime,Saturn,MONITOR,,Saturn appearance monitoring,"monitoring trigger repeated ~ every 2 hours, or at the beginning and the end of the shorter observation:",,,,,, 2011-233T10:19:00,000T08:00:00,21-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11233_SP,rider,,,,,, 2011-233T18:59:00,000T13:25:00,21-Aug-11,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn Far-IR map,Northern hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude Range=14Rs ~60 mrad from N Pole to Equator,,,,,, 2011-233T23:52:00,002T08:12:00,21-Aug-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-234T00:42:21,000T17:21:39,22-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-234T02:32:58,000T20:11:00,22-Aug-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.990292 Rs exit= 13.998431 Range altitude= 5380.5031 km ... -1234.5231,,,,,, 2011-234T09:04:00,000T09:00:00,22-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-234T10:04:00,000T08:00:00,22-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11234_SP,rider,,,,,, 2011-234T18:04:00,000T05:38:21,22-Aug-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-234T18:44:00,000T05:36:00,22-Aug-11,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2011-234T18:44:00,000T05:36:00,22-Aug-11,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2011-234T18:44:00,000T03:36:00,22-Aug-11,ISS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,WAC polarimetry rider,WAC polarimetry,,,,,, 2011-234T20:00:00,000T03:42:00,22-Aug-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-234T22:43:58,000T04:00:00,22-Aug-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.990292 Rs exit= 13.998431 Range altitude= 5380.5031 km ... -1234.5231,,,,,, 2011-234T23:42:00,000T02:00:00,22-Aug-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-234T23:42:21,000T00:30:00,22-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-234T23:43:58,000T02:00:00,22-Aug-11,CDA,SPASS Rider,DustRAM direction,RPX0170,,CDA RPXing 2011-235T00:43:58,RPXing at 4.6073883 Rs,,,,,, 2011-235T00:00:00,000T01:08:00,23-Aug-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-235T00:12:21,000T01:30:00,23-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-235T00:20:00,000T02:30:00,23-Aug-11,VIMS,Prime,Saturn,OMICETOCC,OmiCet occultation,omiCet Saturn occultation,"omiCet atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. After the occ, at time 01:25, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation occurred (latitude 15.1N).",,,,,, 2011-235T00:20:00,000T02:30:00,23-Aug-11,CIRS,,Saturn,OMICETOCC,OmiCet occultation,CIRS_152SA_OMICETOCC001_VIMS,PIE Collab with VIMS. Stellar Occ Saturn ingress T01:04 15N dark limb at T01:25 go to limb for CIRS integration,,,,,, 2011-235T01:40:00,000T04:40:00,23-Aug-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-235T01:42:00,000T10:18:00,23-Aug-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-235T01:42:21,000T16:21:39,23-Aug-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-235T02:43:58,001T02:41:00,23-Aug-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.990292 Rs exit= 13.998431 Range altitude= 5380.5031 km ... -1234.5231,,,,,, 2011-235T02:50:00,000T06:20:00,23-Aug-11,CIRS,Prime,Saturn,LIMBINT,Limb integration,CIRS_152SA_LIMBINT001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2011-235T02:50:00,000T06:20:00,23-Aug-11,VIMS,,Saturn,ALPORIOCC,Alpha Orion occultation,alpOri Saturn occultation,alpOri atmosphere occultation in the midst of a CIRS limb scan. Target VIMS_IR to 88.793/7.407 between time 05:16 and 05:56.,,,,,, 2011-235T03:58:14,000T00:00:01,23-Aug-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.044 Rs, lat = -0 deg, phase = 136 deg",,,,,, 2011-235T06:20:00,000T12:10:00,23-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-235T09:30:00,000T09:00:00,23-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-235T10:30:00,000T08:00:00,23-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11235_SP,rider,,,,,, 2011-235T18:04:00,001T03:56:00,23-Aug-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-235T18:30:00,000T08:30:00,23-Aug-11,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 13.990292 Rs exit= 13.998431 Range altitude= 5380.5031 km ... -1234.5231,,,,,, 2011-235T18:30:00,003T21:49:00,23-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-235T19:10:00,000T19:14:00,23-Aug-11,VIMS,Prime,Saturn,PEARLMOV,,Saturn Pearl Movie,"2 (rows)x4(columns) Regional mosaics, one collected each 76 minutes throughout the 19-hrs duration. Lowest row (tier) of the mosaic is centered at 33 degrees latitude at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 4 frames each, oriented with the 4 frames in the east-west direction. 9 mi 30 sec intervals between frame centers (7 mins for science, 2 min 30 secs for repositioning). Each of these mosaics should take 76 min. 15 mosaic should fit in the allotted time.",,,,,, 2011-235T19:10:00,000T19:14:00,23-Aug-11,CIRS,SPASS Rider,Saturn,PEARLMOV,,Rider,VIMS rider,,,,,, 2011-235T19:10:00,000T19:14:00,23-Aug-11,ISS,Non-SPASS,Saturn,PEARLMOV,,Day WAC VIMS rider,"VIMS day WAC rider. 2 (rows)x4(columns) Regional mosaics, one collected each 76 minutes throughout the 19-hrs duration. Lowest row (tier) of the mosaic is centered at 33 degrees latitude at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of",,,,,, 2011-235T19:30:00,000T02:44:00,23-Aug-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-236T05:24:58,009T20:22:02,24-Aug-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.011150 Rs exit= 14.010960 Range altitude= -1231.9544 km ... 5511.3929,,,,,, 2011-236T08:04:00,000T17:30:00,24-Aug-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-236T16:34:00,000T09:00:00,24-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-236T17:34:00,000T08:00:00,24-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11236_SP,rider,,,,,, 2011-236T21:20:00,000T02:16:32,24-Aug-11,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2011-236T22:00:00,000T02:00:00,24-Aug-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-237T00:00:00,000T01:34:00,25-Aug-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-237T01:34:00,012T23:13:59,25-Aug-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-237T01:34:00,007T23:29:00,25-Aug-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-237T01:34:00,009T00:14:00,25-Aug-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_152_153",,,,,, 2011-237T01:34:00,002T23:45:00,25-Aug-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-237T02:13:00,000T00:02:00,25-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-237T02:15:00,000T11:00:00,25-Aug-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-237T02:15:00,000T11:00:00,25-Aug-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-237T02:34:00,000T02:44:00,25-Aug-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-237T13:13:00,000T00:02:00,25-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-237T13:15:00,000T02:15:00,25-Aug-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2011-237T15:28:00,000T00:02:00,25-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-237T15:30:00,000T05:00:00,25-Aug-11,ISS,Prime,Hyperion,HYPERION,Hyperion,Hyperion ORS observation,ORS observation,,,,,, 2011-237T15:30:00,000T05:00:00,25-Aug-11,CIRS,,Hyperion,HYPERION,Hyperion,,null,,,,,, 2011-237T15:30:00,000T05:00:00,25-Aug-11,UVIS,,Hyperion,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2011-237T15:30:00,000T05:00:00,25-Aug-11,VIMS,SPASS Rider,Hyperion,HYPERION,Hyperion,,"Hyperion start=165 deg phase, 4.5 mrad at end",,,,,, 2011-237T20:00:00,002T00:00:00,25-Aug-11,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Apoapse Retrograde,Hyperion OrX - Retrograde observation outbound to apoapse,,,,,, 2011-237T20:28:00,000T00:02:00,25-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-237T22:49:00,000T09:00:00,25-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-237T23:49:00,000T08:00:00,25-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11237_SP,rider,,,,,, 2011-238T00:00:00,000T06:49:36,26-Aug-11,CAPS,Non-SPASS,Saturn,BURST16K,16 kbps burst,Burst of 16kbps data,Burst of 16 kbps data (which gives uncollapsed ELS data). 32 B cycles duration. Data is in addition to 1000 bps from SWSKR.,,,,,, 2011-238T08:28:00,000T00:02:00,26-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-238T08:30:00,000T15:00:00,26-Aug-11,VIMS,Prime,rings(general),EG30PHASE,,E/G Ring phase observation,"Target VIMS to 240,000 km on the LEFT ansa stare for the first 7.5 hours, then target the same radius on the RIGHT ansa for the remainder of the time",,,,,, 2011-238T08:30:00,000T15:00:00,26-Aug-11,CIRS,SPASS Rider,rings(general),EG30PHASE,,,null,,,,,, 2011-238T08:30:00,000T15:00:00,26-Aug-11,ISS,Non-SPASS,rings(general),EG30PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2011-238T23:28:00,000T00:02:00,26-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-238T23:30:00,000T14:30:00,26-Aug-11,ISS,Prime,rings(general),ARCLELR,,Faint Ring Low Phase Observation,Observation of faint rings at low elevation angles and low phase,,,,,, 2011-238T23:30:00,000T14:30:00,26-Aug-11,CIRS,SPASS Rider,rings(general),ARCLELR,,,null,,,,,, 2011-238T23:30:00,000T14:30:00,26-Aug-11,VIMS,SPASS Rider,rings(general),ARCLELR,,Faint ring observation,"Faint ring observation, 1 second integration time",,,,,, 2011-239T13:58:00,000T00:02:00,27-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-239T16:19:00,000T09:00:00,27-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-239T16:19:00,000T09:00:00,27-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-239T17:19:00,000T08:00:00,27-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11239_SP,rider,,,,,, 2011-240T01:19:00,000T08:00:00,28-Aug-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-240T01:19:00,006T00:28:00,28-Aug-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-240T09:19:00,000T22:00:00,28-Aug-11,CDA,Prime,DustRAM direction,ISD0033,,CDA ISD,ISD observation around apoapse 2011-246T01:47:00 45.911332 Rs,,,,,, 2011-240T09:19:00,009T15:29:00,28-Aug-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-241T08:49:00,000T09:00:00,29-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-241T09:49:00,000T08:00:00,29-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11241_SP,rider,,,,,, 2011-241T18:28:00,000T00:02:00,29-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-241T18:30:00,000T01:30:00,29-Aug-11,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 13.6 requested range 3.1 Mkm",,,,,, 2011-241T18:30:00,000T01:30:00,29-Aug-11,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-241T18:30:00,000T01:30:00,29-Aug-11,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 14 deg, range = 3.1 Mkm.",,,,,, 2011-241T19:58:00,000T00:02:00,29-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-241T20:00:00,000T01:00:00,29-Aug-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-241T20:58:00,000T00:02:00,29-Aug-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-242T16:03:00,000T09:00:00,30-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-242T17:03:00,000T08:00:00,30-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11242_SP,rider,,,,,, 2011-243T01:03:00,000T13:30:00,31-Aug-11,CDA,Prime,DustRAM direction,ISD0033,,CDA ISD 2011-246T01:47:00,ISD observation around apoapse 2011-246T01:47:00 45.911332 Rs,,,,,, 2011-243T16:03:00,000T09:00:00,31-Aug-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-243T17:03:00,000T08:00:00,31-Aug-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11243_SP,rider,,,,,, 2011-244T01:58:00,000T00:02:00,1-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-244T02:00:00,000T01:30:00,1-Sep-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 30.4 requested range 3.8 Mkm",,,,,, 2011-244T02:00:00,000T01:30:00,1-Sep-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-244T02:00:00,000T01:30:00,1-Sep-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 30 deg, range = 3.8 Mkm.",,,,,, 2011-244T03:28:00,000T00:02:00,1-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-244T03:30:00,000T01:00:00,1-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-244T04:28:00,000T00:02:00,1-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-244T16:03:00,000T09:00:00,1-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-244T17:03:00,000T08:00:00,1-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11244_SP,rider,,,,,, 2011-245T01:03:00,000T15:00:00,2-Sep-11,CDA,Prime,DustRAM direction,ISD0033,,CDA ISD 2011-246T01:47:00,ISD observation around apoapse 2011-246T01:47:00 45.911332 Rs,,,,,, 2011-245T01:03:00,001T00:00:00,2-Sep-11,INMS,Non-SPASS,Saturn,SURVPOTMA,,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-245T16:03:00,000T09:00:00,2-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-245T17:03:00,000T08:00:00,2-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_152IC_DSCAL11245_SP,rider,,,,,, 2011-246T01:03:00,001T13:15:00,3-Sep-11,CDA,Prime,DustRAM direction,ISD0033,,CDA ISD,ISD observation around apoapse 2011-246T01:47:00 45.911332 Rs,,,,,, 2011-246T01:03:00,000T00:45:00,3-Sep-11,INMS,Non-SPASS,Saturn,SURVBOTMA,,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-246T01:47:00,003T23:01:00,3-Sep-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S70,Range enter= 14.011150 Rs exit= 14.010960 Range altitude= -1231.9544 km ... 5511.3929,,,,,, 2011-246T01:47:53,000T00:00:01,3-Sep-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 21.8 d, inc = 0.4 deg, r = 45.867 Rs, phase = 44 deg",,,,,, 2011-246T01:48:00,000T02:00:00,3-Sep-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-246T01:48:00,003T23:00:00,3-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_152_153",,,,,, 2011-246T01:48:00,003T23:00:00,3-Sep-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-246T03:48:00,003T21:00:00,3-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-247T15:48:00,000T09:00:00,4-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-247T16:48:00,000T08:00:00,4-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11247_SP,rider,,,,,, 2011-248T00:48:00,000T13:30:00,5-Sep-11,ISS,Prime,Other,L5IAPE,,Iapetus L5 satellite search,Satellite search around Iapetus L5 Lagrange point.,,,,,, 2011-248T05:47:00,000T20:00:00,5-Sep-11,CDA,SPASS Rider,DustRAM direction,ISD0033,,CDA ISD 2011-246T01:47:00,ISD observation around apoapse 2011-246T01:47:00 45.911332 Rs,,,,,, 2011-248T14:18:00,000T11:42:00,5-Sep-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-248T15:48:00,000T09:00:00,5-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-248T16:48:00,000T08:00:00,5-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11248_SP,rider,,,,,, 2011-249T01:58:00,000T00:02:00,6-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-249T02:00:00,000T01:30:00,6-Sep-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 71.9 requested range 3.2 Mkm",,,,,, 2011-249T02:00:00,000T01:30:00,6-Sep-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-249T02:00:00,000T01:30:00,6-Sep-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 22 deg, range = 2.8 Mkm.",,,,,, 2011-249T03:28:00,000T00:02:00,6-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-249T03:30:00,000T01:00:00,6-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-249T04:28:00,000T00:02:00,6-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-249T04:30:00,000T09:00:00,6-Sep-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-249T13:28:00,000T00:02:00,6-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-249T15:48:00,000T09:00:00,6-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-249T16:48:00,000T08:00:00,6-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11249_SP,rider,,,,,, 2011-249T21:00:00,000T01:08:00,6-Sep-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-250T00:48:00,004T05:58:59,7-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-250T00:48:00,005T21:26:58,7-Sep-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S70,Range enter= 14.011150 Rs exit= 14.010960 Range altitude= -1231.9544 km ... 5511.3929,,,,,, 2011-250T00:48:00,000T00:43:00,7-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-250T00:48:00,001T00:00:00,7-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-250T00:48:00,004T05:59:00,7-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_152_153",,,,,, 2011-250T00:48:00,004T05:59:00,7-Sep-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-250T00:53:00,000T00:02:00,7-Sep-11,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S70 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2011-250T01:31:00,000T00:07:00,7-Sep-11,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-250T01:38:00,000T00:05:00,7-Sep-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-250T01:43:00,000T00:33:00,7-Sep-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-250T01:45:00,000T01:30:00,7-Sep-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 80 requested range 2.8 Mkm",,,,,, 2011-250T01:45:00,000T01:30:00,7-Sep-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-250T01:45:00,000T01:30:00,7-Sep-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 80 deg, range = 2.2 Mkm.",,,,,, 2011-250T02:16:00,000T00:30:00,7-Sep-11,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2011-250T02:46:00,002T04:02:00,7-Sep-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-250T03:15:00,000T01:00:00,7-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-250T04:15:00,000T05:15:00,7-Sep-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-250T09:30:00,000T04:00:00,7-Sep-11,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2011-250T09:30:00,000T04:00:00,7-Sep-11,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2011-250T13:48:00,000T11:00:00,7-Sep-11,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,"HGA Boresight Calibration. Pointing=XBAND to Earth + crosshair maneuver. Telemetry OFF, TWNC ON for 1-hr calibration from 2011-250T17:48:00 to 2011-250T18:48:00. Required to be tracked by DSS-25 (or DSS-26). Keep Ka-band ON until EOT at 2011-251T00:48:00. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2011-250T15:48:00,000T09:00:00,7-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-250T16:48:00,000T08:00:00,7-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11250_SP,rider,,,,,, 2011-250T17:48:00,000T01:00:00,7-Sep-11,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,"HGA Boresight Calibration. Pointing=XBAND to Earth + crosshair maneuver. Telemetry OFF, TWNC ON for 1-hr calibration from 2011-250T17:48:00 to 2011-250T18:48:00. Required to be tracked by DSS-25 (or DSS-26). Keep Ka-band ON until EOT at 2011-251T00:48:00. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2011-251T00:48:00,000T21:00:00,8-Sep-11,ISS,Prime,Other,PAAROT,,Paaliaq,Observation of irregular moon of Saturn.,,,,,, 2011-251T00:48:00,000T21:00:00,8-Sep-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-251T00:48:00,003T05:59:00,8-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-251T01:30:00,000T20:00:00,8-Sep-11,CDA,Non-SPASS,Other,DECON,Decontamination,Decon in S70,SSR-Load (6Ext_Mem_Load) planned to be at exactly 2011-251T02:00:00. Roughly one hour apart from the preceeding D/L (SP_153EA_G34B262ND250_PRIME) having a carryover with 442 MB. Expectations is that a SSR-Ping-Pong disable might not be necessary. No additional DV necessary,,,,,, 2011-251T04:00:00,000T08:40:00,8-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-251T20:00:00,002T00:00:00,8-Sep-11,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Apoapse Retrograde,Retrograde observation inbound towards Hyperion,,,,,, 2011-251T21:48:00,000T09:00:00,8-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-251T22:48:00,000T08:00:00,8-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11251_SP,rider,,,,,, 2011-252T06:48:00,000T23:59:00,9-Sep-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-252T07:30:00,000T01:30:00,9-Sep-11,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 96.1 requested range 1.5 Mkm",,,,,, 2011-252T07:30:00,000T01:30:00,9-Sep-11,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-252T07:30:00,000T01:30:00,9-Sep-11,VIMS,SPASS Rider,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 96 deg, range = 1.5 Mkm.",,,,,, 2011-252T09:00:00,000T01:00:00,9-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-252T10:00:00,000T11:00:00,9-Sep-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-252T21:47:00,000T09:00:00,9-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-252T22:47:00,000T08:00:00,9-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11252_SP,rider,,,,,, 2011-253T06:47:00,000T17:13:00,10-Sep-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-253T07:00:00,000T14:40:00,10-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-253T07:30:00,000T12:00:00,10-Sep-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-253T21:47:00,000T09:00:00,10-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-253T22:47:00,000T08:00:00,10-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11253_SP,rider,,,,,, 2011-254T00:00:00,000T00:34:00,11-Sep-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-254T00:34:00,000T06:13:00,11-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-254T06:47:00,000T18:03:06,11-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-254T06:47:00,000T08:03:06,11-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-254T06:47:00,000T16:03:06,11-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-254T06:47:00,002T00:45:00,11-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_153_T78",,,,,, 2011-254T06:47:00,001T12:50:00,11-Sep-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-254T07:42:00,000T06:08:06,11-Sep-11,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template M4: CIRS only.,,,,,, 2011-254T07:42:00,000T06:08:06,11-Sep-11,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-254T07:42:00,000T06:08:06,11-Sep-11,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan Scan,"VIMS ridealong with CIRS while scanning across Titan. Phase = 106 deg, SSC Lat/Lon = 0.001S/133.876 deg, SS Lat/Lon = 11.120N/240.244 deg. Alt = 389822.08 km, range = 392397.08 km. Resolution = 195 km/px. Temp. M4. Obtain cubes while scanning across Titan.",,,,,, 2011-254T13:50:06,000T04:00:00,11-Sep-11,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2011-254T13:50:06,000T04:00:00,11-Sep-11,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-254T13:50:06,000T04:00:00,11-Sep-11,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS. Phase = 107 deg, SSC Lat/Lon = 0.003S/138.541 deg, SS Lat/Lon = 11.122N/246.039 deg. Alt = 261219.6 km, range = 263794.6 km. Resolution = 131 km/px. Temp. N1. Obtain cubes of Titan of 160 and 640 msec.",,,,,, 2011-254T13:50:06,000T04:00:00,11-Sep-11,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS FIRNADCMP,Rider to CIRS FIRNADCMP,,,,,, 2011-254T14:50:06,000T11:00:00,11-Sep-11,INMS,Non-SPASS,Saturn,T78INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-254T17:50:06,000T04:00:00,11-Sep-11,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,"Obtain vertical profiles of temperature and abundances of trace gases in Titan's stratosphere. The arrays are positioned on the limb (-/+ Z perp to limb) at two altitudes, about 100 km and 350 km at center.",,,,,, 2011-254T17:50:06,000T04:00:00,11-Sep-11,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-254T17:50:06,000T04:00:00,11-Sep-11,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan Limb mapping.,"VIMS ridealong with CIRS for Titan limb mapping. Phase = 108 deg, SSC Lat/Lon = 0.006S/141.168 deg, SS Lat/Lon = 11.124N/249.719 deg. Alt = 180787.6 km, range = 183362.6 km. Resolution = 90 km/px. Temp. R. Obtain cubes for Titan limb mapping.",,,,,, 2011-254T21:50:06,000T02:45:00,11-Sep-11,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2011-254T21:50:06,000T02:45:00,11-Sep-11,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-254T21:50:06,000T02:45:00,11-Sep-11,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan Scan,"VIMS ridealong with CIRS while scanning across Titan. Phase = 110 deg, SSC Lat/Lon = 0.013S/142.614 deg, SS Lat/Lon = 11.126N/253.478 deg. Alt = 99450.3 km, range = 102025.3 km. Resolution = 50 km/px. Temp. T. Obtain cubes while scanning across Titan.",,,,,, 2011-254T22:50:06,000T08:00:00,11-Sep-11,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T78 flyby,"T78 is a dusk, equatorial flyby across Titan's mid range magnetic tail (5941 km altitude). During this flyby, Cassini will have another opportunity to observe the structure of the magnetic tail, formed by draped fields, this time in the dusk region of Saturn's magnetosphere. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2011-255T00:35:06,000T01:00:00,12-Sep-11,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2011-255T00:35:06,000T01:00:00,12-Sep-11,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-255T00:35:06,000T00:32:00,12-Sep-11,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,"VIMS ridealong for regional mapping. Phase = 117 deg, SSC Lat/Lon = 0.033S/139.002 deg, SS Lat/Lon = 11.127N/256.140 deg. Alt = 42387.0 km, range = 44962.0 km. Resolution = 21 km/px. Obtain cubes for regional mapping of Titan.",,,,,, 2011-255T00:50:06,000T01:00:00,12-Sep-11,CAPS,SPASS Rider,Titan,T78INBND,,Inbound 153TI (T78),null,,,,,, 2011-255T00:50:06,000T01:00:00,12-Sep-11,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-255T00:50:06,000T01:15:00,12-Sep-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-255T01:35:06,000T00:32:00,12-Sep-11,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2011-255T01:35:06,000T00:32:00,12-Sep-11,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-255T01:50:06,000T02:00:00,12-Sep-11,CAPS,,Titan,T78CLOSE,,Closest Approach 153TI (T78),Collaborative rider only applies to UVIS USUNOCC,,,,,, 2011-255T01:50:06,000T02:00:00,12-Sep-11,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-255T01:50:06,000T02:00:00,12-Sep-11,INMS,Non-SPASS,Titan,TITAN78,,Titan Flyby,Titan observation,,,,,, 2011-255T02:05:06,000T01:30:00,12-Sep-11,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2011-255T02:07:06,000T00:16:00,12-Sep-11,VIMS,Prime,Titan,OCCHIAQ,,Titan Stellar Occ.,Titan Stellar Occ of chiAqr starting at C/A -00:35:45,,,,,, 2011-255T02:07:06,000T00:16:00,12-Sep-11,CIRS,SPASS Rider,Titan,OCCRAQR,,ISS rider Titan low phase,Rider along with VIMS occ.,,,,,, 2011-255T02:23:06,000T00:56:00,12-Sep-11,UVIS,Prime,Sun,USUNOCC,Solar occultation,Solar Occ Titan,This is a solar occultation by Titan. Slit aligned tangent to limb. Record data during occultation. Turn back occurs after this period.,,,,,, 2011-255T02:23:06,000T00:56:00,12-Sep-11,CIRS,SPASS Rider,Sun,USUNOCC,Solar occultation,,Ride along with UVIS.,,,,,, 2011-255T02:23:06,000T00:56:00,12-Sep-11,ISS,,Sun,USUNOCC,Solar occultation,UVIS SOlar Occ Rider,Long exposures on high altitude haze while in eclipse,,,,,, 2011-255T02:23:06,000T00:56:00,12-Sep-11,VIMS,SPASS Rider,Titan,SOLOCC,Solar occultation,Solar Occ.,"VIMS ridealong with UVIS during solar occ. from -00:03 to +00:24. Phase = 156 deg, SSC Lat/Lon = 0.144S/99.7362 deg, SS Lat/Lon = 11.128N/257.863 deg. Alt = 8252.8 km, range = 10827.8 km. Resolution = 4.1 km/px.",,,,,, 2011-255T03:19:06,000T03:31:00,12-Sep-11,CAPS,Prime,Titan,T78PTG,,Titan Encounter,null,,,,,, 2011-255T03:19:06,000T03:31:00,12-Sep-11,CIRS,SPASS Rider,Titan,T78PTG,,ISS rider Titan low phase,Rider on CAPS PRIME.,,,,,, 2011-255T03:35:06,000T01:15:00,12-Sep-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-255T03:50:06,000T01:00:00,12-Sep-11,CAPS,SPASS Rider,Titan,T78OUTBND,,Outbound 153TI (T78),null,,,,,, 2011-255T03:50:06,000T01:00:00,12-Sep-11,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-255T03:50:06,000T11:00:00,12-Sep-11,INMS,Non-SPASS,Saturn,T78OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-255T04:50:06,000T15:56:54,12-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-255T06:50:06,000T06:09:54,12-Sep-11,UVIS,Prime,Titan,HDACSTARE,,HDAC observation of Titan (stare),HDAC observation of Titan (stare). EUV and FUV will also be taking data with the setup like the setup for EUVFUV,,,,,, 2011-255T06:50:06,000T06:09:54,12-Sep-11,CIRS,SPASS Rider,Titan,HDACSTARE,,,Ride along with UVIS.,,,,,, 2011-255T06:50:06,000T06:09:54,12-Sep-11,ISS,SPASS Rider,Titan,HDACSTARE,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-255T06:50:06,000T06:09:54,12-Sep-11,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan,"VIMS ridealong with UVIS while scanning across Titan. Phase = 77 deg, SSC Lat/Lon = 0.010S/338.182 deg, SS Lat/Lon = 11.129N/262.012 deg. Alt = 80979.0 km, range = 83554.0 km. Resolution = 40 km/px. Temp. X, modified. Obtain cubes while scanning across Titan.",,,,,, 2011-255T06:50:06,001T00:56:54,12-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-255T14:50:06,000T05:37:42,12-Sep-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-255T15:00:00,000T15:00:00,12-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-255T17:47:00,000T13:00:00,12-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11255_SP,rider,,,,,, 2011-255T19:37:00,000T11:55:00,12-Sep-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-255T20:27:48,000T11:19:12,12-Sep-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-255T20:47:00,000T10:45:00,12-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-255T22:14:58,000T09:32:02,12-Sep-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.998093 Rs exit= 13.992206 Range altitude= 5506.1023 km ... -118.37048,,,,,, 2011-256T07:32:00,002T09:14:59,13-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-256T07:32:00,002T09:15:00,13-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_153",,,,,, 2011-256T07:32:00,001T18:54:00,13-Sep-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-256T07:47:00,001T15:59:58,13-Sep-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.998093 Rs exit= 13.992206 Range altitude= 5506.1023 km ... -118.37048,,,,,, 2011-256T07:47:00,000T11:40:48,13-Sep-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-256T07:47:00,000T04:13:00,13-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-256T08:37:00,000T03:23:00,13-Sep-11,ISS,Prime,Enceladus,PLMMPMR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-256T08:37:00,000T03:23:00,13-Sep-11,CIRS,SPASS Rider,Enceladus,PLMMHPHR,,,null,,,,,, 2011-256T08:37:00,000T03:23:00,13-Sep-11,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2011-256T12:00:00,000T06:00:00,13-Sep-11,UVIS,Prime,Saturn,ENAURFOOT,,Search for Enceladus Auroral Footprint,"Slow repeated slews across Saturn's auroral zone, emphasizing Enceladus-related auroras This means slews should cover 55-90 latitude. They should also cover the sub-Enceladus longitude between 60-70 latitude.",,,,,, 2011-256T12:00:00,000T06:00:00,13-Sep-11,MAG,Non-SPASS,Enceladus,ENAURFOOT,,EnAurFoot PIE,MAPS EnAurFoot PIE observation,,,,,, 2011-256T18:00:00,000T01:10:00,13-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-256T18:27:00,000T04:00:00,13-Sep-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-256T18:35:01,000T03:24:59,13-Sep-11,CDA,Prime,Other,RINGSHAD,,CDA Ring Shadow Crossing1_4Rs,CDA Ring Shadow Crossing @ 4Rs; objective code RC1a,,,,,, 2011-256T19:10:00,000T07:50:00,13-Sep-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-256T19:27:48,000T02:00:00,13-Sep-11,INMS,Non-SPASS,Saturn,ENCELRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-256T21:27:48,000T23:00:00,13-Sep-11,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-256T22:00:00,000T03:00:00,13-Sep-11,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2011-256T22:00:00,000T03:00:00,13-Sep-11,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2011-256T22:00:00,000T03:00:00,13-Sep-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-256T22:00:00,000T03:00:00,13-Sep-11,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2011-256T23:01:16,000T00:00:01,13-Sep-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.231 Rs, lat = -0 deg, phase = 129 deg",,,,,, 2011-257T01:00:00,000T01:30:00,14-Sep-11,ISS,Prime,Pallene,PALLENE,,Pallene flyby,ORS observation,,,,,, 2011-257T01:00:00,000T01:30:00,14-Sep-11,CIRS,SPASS Rider,Pallene,PALLENE,,,null,,,,,, 2011-257T01:00:00,000T01:30:00,14-Sep-11,UVIS,SPASS Rider,Pallene,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-257T01:00:00,000T01:30:00,14-Sep-11,VIMS,SPASS Rider,Pallene,PALLENE,,Pallene,Pallene,,,,,, 2011-257T02:30:00,000T03:07:00,14-Sep-11,CIRS,Prime,Tethys,PACMAN,,153TE_PACMAN001,"02:50 - 03:20 FP3/4 Mapping @ 6 mu rad/s 03:31 - 03:25 FP1 stare @ center of target 03:26 - 03:56 FP3/4 Mapping @ 6 mu rad/s 03:57 - 04:27 FP3/4 Mapping @ 6 mu rad/s 04:27 - 04:32 FP1 Stare @ center of target 04:33 - 05:03 FP3/4 Mapping @ 6 mu rad/s 05:04 - 05:22 FP3/4 Mapping @ 6 mu 05:22 - 05:37 Turn Low-phase distant FP3 search for ""Pac Man"" phenomenon on Tethys leading side Placeholder only- subject to negotiation",,,,,, 2011-257T02:30:00,000T03:07:00,14-Sep-11,ISS,SPASS Rider,Tethys,PACMAN,,CIRS Tethys rider,CIRS rider,,,,,, 2011-257T02:30:00,000T03:07:00,14-Sep-11,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-257T02:30:00,000T03:07:00,14-Sep-11,VIMS,SPASS Rider,Tethys,PACMAN,,Tethys,Tethys,,,,,, 2011-257T03:00:00,001T13:47:00,14-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-257T07:47:00,000T09:00:00,14-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-257T08:47:00,000T08:00:00,14-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11257_SP,rider,,,,,, 2011-257T16:47:00,000T04:00:00,14-Sep-11,CIRS,Prime,Tethys,PACMAN,,153TE_PACMAN002,"16:47 - 17:07 Turn (15.5 mins/168.4 deg iDigit estimate + padding) 17:07 - 17:31 Two FP3/4 scans (1 swath will cover disk) @ 6 mu rad/s 17:31 - 17:36 FP1 stare @ center 17:36 - 18:46 FP3/4 Scans (? number, maybe 5, do as many as possible) @ 6 mu rad/s 18:46 - 19:01 FP1 stare @ center 19:01 - 20:22 FP3/4 Scans (probably time for ~ 7) @ 6 mu rad/s 20:22 - 20:27 FP1 stare @ center 20:27 - 20:47 Turn (15.4 mins/166.3 deg iDigit estimate + padding) Placeholder only- subject to negotiation",,,,,, 2011-257T16:47:00,000T04:00:00,14-Sep-11,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-257T20:27:48,000T20:19:12,14-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-257T20:47:00,000T01:30:00,14-Sep-11,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 31.6 requested range 1.9 Mkm",,,,,, 2011-257T20:47:00,000T01:30:00,14-Sep-11,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-257T20:47:00,000T01:30:00,14-Sep-11,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 31.6 deg, range = 1.9 Mkm.",,,,,, 2011-257T23:46:58,007T20:11:02,14-Sep-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.005072 Rs exit= 14.012565 Range altitude= -115.03122 km ... 3434.1980,,,,,, 2011-258T02:26:00,000T14:21:00,15-Sep-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-258T07:47:00,000T09:00:00,15-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-258T08:47:00,000T08:00:00,15-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11258_SP,rider,,,,,, 2011-258T16:47:00,015T06:29:59,15-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-258T16:47:00,000T00:51:00,15-Sep-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-258T16:47:00,000T23:45:00,15-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-258T16:47:00,007T03:12:00,15-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_153_154",,,,,, 2011-258T16:47:00,007T03:11:00,15-Sep-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-258T17:28:00,000T00:02:00,15-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-258T17:30:00,000T07:00:00,15-Sep-11,ISS,Prime,RingE,ERNGVRLP,,Low-Phase Edge-on obs E-ring observation after Eq,Low elevation observation of E ring at low phase.,,,,,, 2011-258T17:30:00,000T07:00:00,15-Sep-11,CIRS,SPASS Rider,rings(general),ERNGVRLP,,,null,,,,,, 2011-258T17:30:00,000T06:58:00,15-Sep-11,VIMS,SPASS Rider,RingE,ERNGVRLP,,E Ring observation,ISS rider; 1 second IR integration time,,,,,, 2011-258T17:38:00,000T02:00:00,15-Sep-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-258T19:38:00,000T20:54:00,15-Sep-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-259T00:28:00,000T00:02:00,16-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-259T00:28:00,000T00:02:00,16-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-259T00:30:00,000T06:30:00,16-Sep-11,ISS,Prime,rings(general),ARCLELR,,Faint Ring Low Phase Observation,Observation of faint rings at low elevation angles and low phase,,,,,, 2011-259T00:30:00,000T06:30:00,16-Sep-11,CIRS,SPASS Rider,rings(general),ARCLELR,,,null,,,,,, 2011-259T06:58:00,000T00:02:00,16-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-259T06:58:00,000T00:02:00,16-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-259T07:32:00,000T09:00:00,16-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-259T08:32:00,000T08:00:00,16-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11259_SP,rider,,,,,, 2011-259T16:32:00,003T13:45:00,16-Sep-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-259T16:32:00,000T09:30:00,16-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-259T16:56:00,000T00:02:00,16-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-259T16:56:00,000T00:02:00,16-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-259T16:58:00,000T00:30:00,16-Sep-11,ISS,Prime,Hyperion,SFAD,,Scientist for a Day,Outreach images for Scientist for a Day. 12-bit NACs of Hyperion.,,,,,, 2011-259T16:58:00,000T04:54:00,16-Sep-11,UVIS,SPASS Rider,Hyperion,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-259T17:28:00,000T04:24:00,16-Sep-11,ISS,Prime,Hyperion,HYPERION,Hyperion,Hyperion ORS observation,ORS observation,,,,,, 2011-259T21:50:00,000T00:02:00,16-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-259T21:50:00,000T00:02:00,16-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-259T21:52:00,000T01:30:00,16-Sep-11,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 17.8 requested range 2.8 Mkm",,,,,, 2011-259T21:52:00,000T01:30:00,16-Sep-11,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-259T21:52:00,000T01:28:00,16-Sep-11,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 17.6 deg, range = 2.8 Mkm.",,,,,, 2011-259T23:20:00,000T00:02:00,16-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-259T23:20:00,000T00:02:00,16-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-259T23:22:00,000T01:00:00,16-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-260T00:20:00,000T00:02:00,17-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-260T00:20:00,000T00:02:00,17-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-260T00:22:00,000T01:40:00,17-Sep-11,ISS,Prime,Tethys,SFAD,,Scientist for a Day,Outreach images for Scientist for a Day,,,,,, 2011-260T00:22:00,000T01:40:00,17-Sep-11,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-260T02:00:00,000T00:02:00,17-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-260T02:00:00,000T00:02:00,17-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-260T02:02:00,000T08:00:00,17-Sep-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-260T10:00:00,000T00:02:00,17-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-260T10:00:00,000T00:02:00,17-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-260T10:02:00,000T01:18:00,17-Sep-11,ISS,Prime,Enceladus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Enceladus across Titan","Images of mutual event, transit of Enceladus across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-260T10:02:00,002T20:15:00,17-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-260T11:18:00,000T00:02:00,17-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-260T11:18:00,000T00:02:00,17-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-260T11:20:00,000T01:14:00,17-Sep-11,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Titan","Images of mutual event, transit of Dione across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-260T12:32:00,000T00:02:00,17-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-260T12:32:00,000T00:02:00,17-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-260T15:02:00,000T09:00:00,17-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-260T16:02:00,000T08:00:00,17-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11260_SP,rider,,,,,, 2011-261T00:02:00,000T13:30:00,18-Sep-11,CDA,Prime,DustRAM direction,ISD0034,,CDA ISD 2011-265T19:58:00,ISD observation around apoapse 2011-265T19:58:00 40.293290 Rs,,,,,, 2011-261T15:02:00,000T09:00:00,18-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-261T16:02:00,000T08:00:00,18-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11261_SP,rider,,,,,, 2011-262T00:58:00,000T00:02:00,19-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-262T00:58:00,000T00:02:00,19-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-262T01:00:00,000T01:30:00,19-Sep-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 43.4 requested range 3.3 Mkm",,,,,, 2011-262T01:00:00,000T01:30:00,19-Sep-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-262T01:00:00,000T01:28:00,19-Sep-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 40.4 deg, range = 3.3 Mkm.",,,,,, 2011-262T02:28:00,000T00:02:00,19-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-262T02:28:00,000T00:02:00,19-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-262T02:30:00,000T02:00:00,19-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-262T04:28:00,000T00:02:00,19-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-262T04:28:00,000T00:02:00,19-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-262T04:30:00,000T16:00:00,19-Sep-11,UVIS,Prime,Saturn,MOS153APO,,,"Mosaic scan of Saturn magnetosphere, day 1. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances of 20 minutes observation margin at start and end, and 30 minutes for turn back to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew -111.1 mrad about z axis and +32 mrad about x axis. Start data capture, stare 294.5 s, stop data capture. Repeat PATTERN 148 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 294.5 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (4111.40412 bps, from Alain's spreadsheet)x(294.5s per stare)x(149 stares) = 180.4105x10^6 bits. Additional 1% added to effective data rate per Alain because of data packet filling issues.",,,,,, 2011-262T20:28:00,000T00:02:00,19-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-262T20:28:00,000T00:02:00,19-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-262T21:17:00,000T09:00:00,19-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-262T22:17:00,000T08:00:00,19-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11262_SP,rider,,,,,, 2011-263T06:17:00,000T15:00:00,20-Sep-11,CDA,Prime,DustRAM direction,ISD0034,,CDA ISD 2011-265T19:58:00,ISD observation around apoapse 2011-265T19:58:00 40.293290 Rs,,,,,, 2011-263T06:17:00,001T00:00:00,20-Sep-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-263T06:17:00,001T00:00:00,20-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-263T21:17:00,000T09:00:00,20-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-263T22:17:00,000T08:00:00,20-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11263_SP,rider,,,,,, 2011-264T06:17:00,001T13:42:00,21-Sep-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-264T06:17:00,001T11:12:00,21-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-264T06:58:00,000T00:02:00,21-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-264T06:58:00,000T00:02:00,21-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-264T07:00:00,000T05:00:00,21-Sep-11,ISS,Prime,Other,L5RHEA,,Rhea L5 satellite search,Satellite search around Rhea L5 Lagrange point.,,,,,, 2011-264T11:58:00,000T00:02:00,21-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-264T11:58:00,000T00:02:00,21-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-264T12:00:00,000T01:00:00,21-Sep-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-264T12:58:00,000T00:02:00,21-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-264T12:58:00,000T00:02:00,21-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-264T13:00:00,000T16:00:00,21-Sep-11,UVIS,Prime,Saturn,MOS153APO,,,"Mosaic scan of Saturn magnetosphere, day 2. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances of 20 minutes observation margin at start and end, and 30 minutes for turn back to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew -100.0 mrad about z axis and +96 mrad about x axis. Start data capture, stare 328.0 s, stop data capture. Repeat PATTERN 134 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 328.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (3691.48937 bps, from Alain's spreadsheet)x(328.0s per stare)x(135 stares) = 163.4592x10^6 bits. Additional 1% added to effective data rate per Alain because of data packet filling issues.",,,,,, 2011-265T00:00:00,000T01:08:00,22-Sep-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-265T04:58:00,000T00:02:00,22-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-265T04:58:00,000T00:02:00,22-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-265T07:17:00,000T09:00:00,22-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-265T08:17:00,000T08:00:00,22-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_153IC_DSCAL11265_SP,rider,,,,,, 2011-265T16:58:00,000T00:02:00,22-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-265T16:58:00,000T00:02:00,22-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-265T17:00:00,000T01:00:00,22-Sep-11,ISS,Prime,Saturn,SFAD,,Scientist for a Day,Outreach images for Scientist for a Day,,,,,, 2011-265T17:29:00,000T05:00:00,22-Sep-11,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2011-265T17:58:00,000T00:02:00,22-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-265T17:58:00,000T00:02:00,22-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-265T18:00:00,000T08:00:00,22-Sep-11,ISS,Prime,Other,L5DIONE,,Dione L5 satellite search,Satellite search around Dione L5 Lagrange point.,,,,,, 2011-265T19:58:00,007T20:06:58,22-Sep-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.005072 Rs exit= 14.012565 Range altitude= -115.03122 km ... 3434.1980,,,,,, 2011-265T19:58:00,007T17:29:00,22-Sep-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-265T19:58:51,000T00:00:01,22-Sep-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.7 d, inc = 0.3 deg, r = 40.259 Rs, phase = 50 deg",,,,,, 2011-265T19:59:00,000T02:00:00,22-Sep-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-265T19:59:00,008T03:18:00,22-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_153_154",,,,,, 2011-265T21:59:00,005T18:03:00,22-Sep-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-265T22:29:00,002T01:03:00,22-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-266T01:58:00,000T00:02:00,23-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-266T01:58:00,000T00:02:00,23-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-266T02:00:00,001T08:00:00,23-Sep-11,UVIS,Prime,Saturn,MOS153APO,,,"Mosaic scan of Saturn magnetosphere, day 3. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances of 20 minutes observation margin at start and end, and 30 minutes for turn back to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew -100.0 mrad about z axis and -32 mrad about x axis. Start data capture, stare 353.0 s, stop data capture. Repeat PATTERN A 134 times. Slew -64 mrad about x axis. Start data capture, stare 353.0 s, stop data capture. Repeat PATTERN B 134 times. PATTERN A: Slew +1.5 mrad about z-axis. Start data capture, stare 353.0 s, stop data capture. PATTERN B: Slew -1.5 mrad about z-axis. Start data capture, stare 353.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (3430.05245 bps, from Alain's spreadsheet)x(353.0 s per stare)x(270 stares) = 326.9183x10^6 bits. Additional 1% added to effective data rate per Alain because of data packet filling issues.",,,,,, 2011-267T09:58:00,000T00:02:00,24-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-267T09:58:00,000T00:02:00,24-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-267T14:32:00,000T09:00:00,24-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-267T15:32:00,000T08:00:00,24-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11267_SP,rider,,,,,, 2011-267T23:32:00,000T13:30:00,24-Sep-11,CDA,Prime,DustRAM direction,ISD0034,,CDA ISD 2011-265T19:58:00,ISD observation around apoapse 2011-265T19:58:00 40.293290 Rs,,,,,, 2011-267T23:32:00,004T16:30:00,24-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-268T03:00:00,000T03:07:00,25-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-268T14:32:00,000T09:00:00,25-Sep-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-268T14:32:00,000T09:00:00,25-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-268T15:32:00,000T08:00:00,25-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11268_SP,rider,,,,,, 2011-268T16:00:00,000T03:07:00,25-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-268T23:32:00,000T06:00:00,25-Sep-11,CDA,Prime,DustRAM direction,ISD0034,,CDA ISD 2011-265T19:58:00,ISD observation around apoapse 2011-265T19:58:00 40.293290 Rs,,,,,, 2011-269T01:00:00,000T03:07:00,26-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-269T07:02:00,000T09:00:00,26-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-269T08:02:00,000T08:00:00,26-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11269_SP,rider,,,,,, 2011-269T09:00:00,000T03:07:00,26-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-269T16:50:00,000T06:00:00,26-Sep-11,ISS,Prime,Titan,LRMONITOR,Long range monitor,LRM (Long Range Monitoring),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-269T18:00:00,000T03:07:00,26-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-269T22:50:00,000T06:00:00,26-Sep-11,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2011-270T07:02:00,000T09:00:00,27-Sep-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-270T07:02:00,000T09:00:00,27-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-270T08:02:00,000T08:00:00,27-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11270_SP,rider,,,,,, 2011-270T09:00:00,000T03:07:00,27-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-270T16:02:00,000T15:00:00,27-Sep-11,ISS,Prime,Other,SKOROT,,Skoll,Observation of irregular moon of Saturn.,,,,,, 2011-270T16:02:00,000T15:00:00,27-Sep-11,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2011-270T18:00:00,000T02:55:00,27-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-271T07:02:00,000T09:00:00,28-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-271T08:02:00,000T08:00:00,28-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11271_SP,rider,,,,,, 2011-271T16:02:00,000T15:00:00,28-Sep-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-271T16:02:00,001T00:00:00,28-Sep-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-271T18:00:00,000T02:55:00,28-Sep-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-272T07:02:00,000T09:00:00,29-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-272T08:02:00,000T08:00:00,29-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11272_SP,rider,,,,,, 2011-272T16:02:00,000T06:11:00,29-Sep-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-272T16:02:00,001T07:15:00,29-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-272T16:41:00,000T00:02:00,29-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-272T16:41:00,000T00:02:00,29-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-272T16:43:00,000T10:17:00,29-Sep-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-272T22:13:00,000T02:00:00,29-Sep-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-273T00:13:00,000T23:04:00,30-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-273T02:58:00,000T00:02:00,30-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-273T02:58:00,000T00:02:00,30-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-273T03:00:00,000T08:52:00,30-Sep-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-273T03:00:00,000T08:52:00,30-Sep-11,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2011-273T03:00:00,000T08:50:00,30-Sep-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-273T11:50:00,000T00:02:00,30-Sep-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-273T11:50:00,000T00:02:00,30-Sep-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-273T13:27:00,000T09:50:00,30-Sep-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-273T14:17:00,000T09:00:00,30-Sep-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-273T14:17:00,000T09:00:00,30-Sep-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-273T15:17:00,000T08:00:00,30-Sep-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11273_SP,rider,,,,,, 2011-273T16:04:58,002T01:36:00,30-Sep-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.999708 Rs exit= 13.999159 Range altitude= 3429.9258 km ... 1434.3619,,,,,, 2011-273T23:17:00,000T13:35:26,30-Sep-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-273T23:17:00,000T02:35:26,30-Sep-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-273T23:17:00,000T12:35:26,30-Sep-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-273T23:17:00,002T23:45:00,30-Sep-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_154_E14",,,,,, 2011-273T23:17:00,001T21:02:00,30-Sep-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-274T00:02:00,000T06:18:00,1-Oct-11,ISS,Prime,Dione,WISPYMOVI,,Dione movie,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-274T00:02:00,000T06:18:00,1-Oct-11,CIRS,SPASS Rider,Dione,WISPYMOVI,,,null,,,,,, 2011-274T00:02:00,000T06:18:00,1-Oct-11,UVIS,SPASS Rider,Dione,ICYSTARE,,ICYSTARE: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of satellite.,,,,,, 2011-274T00:02:00,000T06:18:00,1-Oct-11,VIMS,SPASS Rider,Dione,WISPYMOV,,Dione,Dione,,,,,, 2011-274T01:52:26,000T10:00:00,1-Oct-11,INMS,Non-SPASS,Enceladus,E14INBND,,Enceladus flyby,Enceladus observation,,,,,, 2011-274T07:15:00,000T04:45:00,1-Oct-11,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-274T07:15:00,000T04:45:00,1-Oct-11,CIRS,SPASS Rider,Enceladus,PLUMHPHR,,,null,,,,,, 2011-274T07:15:00,000T04:45:00,1-Oct-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-274T07:15:00,000T04:45:00,1-Oct-11,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume,Enceladus Plume,,,,,, 2011-274T11:21:00,000T02:00:00,1-Oct-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-274T11:21:58,000T02:00:00,1-Oct-11,CDA,SPASS Rider,DustRAM direction,RPX0200,,CDA RPXing 2011-274T12:21:58,RPXing at 4.6601740 Rs,,,,,, 2011-274T11:52:26,000T00:07:34,1-Oct-11,INMS,Non-SPASS,Enceladus,ENCEL14,,Enceladus encounter,Enceladus observation,,,,,, 2011-274T11:52:26,000T04:00:00,1-Oct-11,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2011-274T12:00:00,000T02:19:26,1-Oct-11,INMS,Prime,Enceladus,ENCEL14,,Enceladus encounter,Enceladus observation,,,,,, 2011-274T12:52:26,000T02:00:00,1-Oct-11,CAPS,SPASS Rider,Titan,EN14CLOSE,,Closest Approach 154EN (14),null,,,,,, 2011-274T12:52:26,000T02:00:00,1-Oct-11,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2011-274T13:22:26,000T01:00:00,1-Oct-11,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 142,BIT_OVERLAY_300,,,,,, 2011-274T13:46:26,000T00:08:00,1-Oct-11,CIRS,,Enceladus,EN14CLOSE,,CIRS_154EN_EN14CLOSE001_CAPS,"Enceladus south polar drag at closest approach. 15.5 cm-1, shutter closed first three minutes.",,,,,, 2011-274T14:19:26,000T03:40:34,1-Oct-11,CIRS,Prime,Enceladus,FP1SECLX,,CIRS Enceladus PIE,Will accommodate 20 minute stare for SID unsuspend.,,,,,, 2011-274T14:19:26,000T03:40:34,1-Oct-11,CIRS,SPASS Rider,Enceladus,FP1SECLX,,CIRS_154EN_FP1SECLX001 eclipse support images,"Five clear WAC images (at 50 second intervals centered on nominal eclipse exit at 2011-274T14:49:51) at 2011-274T14:48:11, T14:49:01, T14:49:51, T14:50:41, and T14:51:31. CLR1-CLR2; 2x2 summation mode.",,,,,, 2011-274T14:19:26,000T03:40:34,1-Oct-11,ISS,,Enceladus,FP1SECLX,,CIRS Enceladus rider,ORS observation,,,,,, 2011-274T14:19:26,000T03:40:34,1-Oct-11,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,Enceladus eclips. Framing for cirs eclipse per John Pearl email 3/17/2011 and 4/12/2011,,,,,, 2011-274T14:19:26,000T01:53:00,1-Oct-11,INMS,Non-SPASS,Enceladus,ENCEL14,,Enceladus encounter,Enceladus observation,,,,,, 2011-274T14:22:00,000T03:38:00,1-Oct-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-274T14:52:26,002T08:09:34,1-Oct-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-274T15:52:26,000T04:57:34,1-Oct-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-274T16:00:00,000T02:15:00,1-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-274T16:12:26,000T09:40:00,1-Oct-11,INMS,Non-SPASS,Enceladus,E14OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2011-274T16:52:54,000T00:00:01,1-Oct-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.250 Rs, lat = -0 deg, phase = 130 deg",,,,,, 2011-274T18:00:00,000T02:00:00,1-Oct-11,ISS,Prime,Enceladus,ENCELADUS,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2011-274T18:00:00,000T02:00:00,1-Oct-11,CIRS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,,null,,,,,, 2011-274T18:00:00,000T02:00:00,1-Oct-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-274T18:00:00,000T02:00:00,1-Oct-11,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus,Enceladus,,,,,, 2011-274T20:50:00,001T03:27:00,1-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-274T20:55:00,000T14:52:00,1-Oct-11,ISS,Prime,Dione,GLOCOL,Global coverage mapping,Dione global color,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-274T20:55:00,000T14:52:00,1-Oct-11,CIRS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,,null,,,,,, 2011-274T20:55:00,000T14:52:00,1-Oct-11,UVIS,SPASS Rider,Dione,ICYSTARE,,ICYSTARE: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of satellite.,,,,,, 2011-274T20:55:00,000T14:52:00,1-Oct-11,VIMS,SPASS Rider,Dione,GLOCOL,Global coverage mapping,Dione,Dione,,,,,, 2011-275T01:52:26,000T06:07:34,2-Oct-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-275T03:29:58,000T02:00:00,2-Oct-11,CDA,SPASS Rider,DustRAM direction,RPX0210,,CDA RPXing 2011-275T04:29:58,RPXing at 8.2431491 Rs,,,,,, 2011-275T08:00:00,000T02:00:00,2-Oct-11,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2011-275T10:00:00,001T13:02:00,2-Oct-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-275T14:17:00,000T10:00:00,2-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-275T14:17:00,000T09:00:00,2-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-275T15:17:00,000T09:00:00,2-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11275_SP,rider,,,,,, 2011-275T17:40:58,007T20:59:02,2-Oct-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.012016 Rs exit= 14.012778 Range altitude= 1437.7342 km ... 3137.7187,,,,,, 2011-275T20:19:00,001T02:43:00,2-Oct-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-276T00:17:00,000T05:30:00,3-Oct-11,ISS,Prime,Other,ENCEL4,,Enceladus L4 satellite search,Satellite search around Enceladus L4 Lagrange point.,,,,,, 2011-276T00:17:00,000T05:30:00,3-Oct-11,CIRS,SPASS Rider,Other,ENCEL4,,,null,,,,,, 2011-276T00:17:00,000T05:30:00,3-Oct-11,VIMS,SPASS Rider,Other,ENCEL4,,ISS_NAC to Rocks,ISS_NAC to Rocks,,,,,, 2011-276T00:17:00,000T22:45:00,3-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-276T02:00:00,000T01:24:00,3-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-276T05:47:00,000T06:05:00,3-Oct-11,ISS,Prime,Other,TITANL4,,Titan L4 satellite search,Satellite search around Titan L4 Lagrange point.,,,,,, 2011-276T05:47:00,000T06:05:00,3-Oct-11,VIMS,SPASS Rider,Other,TITANL4,,ISS_NAC to Rocks,ISS_NAC to Rocks,,,,,, 2011-276T14:02:00,000T09:00:00,3-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-276T15:02:00,000T08:00:00,3-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11276_SP,rider,,,,,, 2011-276T16:00:00,000T01:24:00,3-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-276T23:02:00,014T15:44:00,3-Oct-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-276T23:02:00,001T06:15:00,3-Oct-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-276T23:02:00,001T06:15:00,3-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-276T23:02:00,006T15:39:00,3-Oct-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_154_155",,,,,, 2011-276T23:02:00,006T15:38:00,3-Oct-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-276T23:58:00,000T00:02:00,3-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-276T23:58:00,000T00:02:00,3-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-277T00:00:00,000T01:30:00,4-Oct-11,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 26.7 requested range 2.6 Mkm",,,,,, 2011-277T00:00:00,000T01:30:00,4-Oct-11,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-277T00:00:00,000T01:30:00,4-Oct-11,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 14 range = 2.2 Mkm.,,,,,, 2011-277T00:00:00,000T01:24:00,4-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-277T01:28:00,000T00:02:00,4-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-277T01:28:00,000T00:02:00,4-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-277T01:30:00,000T01:00:00,4-Oct-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-277T02:28:00,000T00:02:00,4-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-277T02:28:00,000T00:02:00,4-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-277T02:30:00,000T12:00:00,4-Oct-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-277T14:28:00,000T00:02:00,4-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-277T14:28:00,000T00:02:00,4-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-277T14:30:00,000T03:00:00,4-Oct-11,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2011-277T14:31:20,000T00:00:01,4-Oct-11,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2011-277T15:36:00,000T01:03:00,4-Oct-11,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Titan","Images of mutual event, transit of Rhea across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-277T16:37:00,000T00:02:00,4-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-277T16:37:00,000T00:02:00,4-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-277T17:30:00,000T02:00:00,4-Oct-11,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2011-277T19:28:00,000T00:02:00,4-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-277T19:28:00,000T00:02:00,4-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-277T20:17:00,000T09:00:00,4-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-277T21:17:00,000T08:00:00,4-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11277_SP,rider,,,,,, 2011-277T22:00:00,000T01:24:00,4-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-278T05:17:00,000T08:00:00,5-Oct-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-278T05:17:00,000T23:59:00,5-Oct-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-278T13:17:00,006T15:44:00,5-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-278T20:16:00,000T09:00:00,5-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-278T21:16:00,000T08:00:00,5-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11278_SP,rider,,,,,, 2011-279T05:16:00,003T23:45:00,6-Oct-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-279T05:58:00,000T00:02:00,6-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-279T05:58:00,000T00:02:00,6-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-279T06:00:00,000T12:00:00,6-Oct-11,UVIS,Prime,Saturn,MOS154APO,,,"Mosaic scan of Saturn magnetosphere, day 1. Scan will focus on vicinity of Saturn disk to image oxygen. Overall extent of scan: +/- 2.5 Rs E-W and N-S (one quadrant covered in each of the first four observation periods; fifth period covers Saturn disk). EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances for 20 minutes of observation margin at start and end, and 30 minutes for turn to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew +32 mrad about x axis. Start data capture, stare 691.0 s, stop data capture. Repeat PATTERN 49 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 691.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1752.25545 bps, from Alain's spreadsheet)x(691.0s per stare)x(50 stares) = 60.5404x10^6 bits. Data rate multiplier includes an extra 1% per Alain because of data packet filling issues.",,,,,, 2011-279T07:00:00,000T01:50:00,6-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-279T17:58:00,000T00:02:00,6-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-279T17:58:00,000T00:02:00,6-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-279T20:16:00,000T09:00:00,6-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-279T20:16:00,000T09:00:00,6-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-279T21:16:00,000T08:00:00,6-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11279_SP,rider,,,,,, 2011-279T22:00:00,000T01:50:00,6-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-280T00:00:00,000T01:08:00,7-Oct-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-280T05:58:00,000T00:02:00,7-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-280T05:58:00,000T00:02:00,7-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-280T06:00:00,000T12:00:00,7-Oct-11,UVIS,Prime,Saturn,MOS154APO,,,"Mosaic scan of Saturn magnetosphere, day 2. Scan will focus on vicinity of Saturn disk to image oxygen. Overall extent of scan: +/- 2.5 Rs E-W and N-S (one quadrant covered in each of the first four observation periods; fifth period covers Saturn disk). EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances for 20 minutes of observation margin at start and end, and 30 minutes for turn to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew +32 mrad about x axis. Start data capture, stare 755.0 s, stop data capture. Repeat PATTERN 45 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 755.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1603.71989 bps, from Alain's spreadsheet)x(755.0s per stare)x(46 stares) = 55.6972x10^6 bits. Data rate multiplier includes an extra 1% per Alain because of data packet filling issues.",,,,,, 2011-280T07:00:00,000T01:50:00,7-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-280T14:40:00,000T20:00:00,7-Oct-11,CDA,SPASS Rider,DustRAM direction,ISD0035,,CDA ISD 2011-283T14:40:00,ISD observation around apoapse 2011-283T14:40:00 40.397222 Rs,,,,,, 2011-280T17:58:00,000T00:02:00,7-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-280T17:58:00,000T00:02:00,7-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-280T20:16:00,000T09:00:00,7-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-280T20:16:00,000T09:00:00,7-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-280T21:16:00,000T08:00:00,7-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11280_SP,rider,,,,,, 2011-280T22:00:00,000T01:50:00,7-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-281T05:58:00,000T00:02:00,8-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-281T05:58:00,000T00:02:00,8-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-281T06:00:00,000T12:00:00,8-Oct-11,UVIS,Prime,Saturn,MOS154APO,,,"Mosaic scan of Saturn magnetosphere, day 3. Scan will focus on vicinity of Saturn disk to image oxygen. Overall extent of scan: +/- 2.5 Rs E-W and N-S (one quadrant covered in each of the first four observation periods; fifth period covers Saturn disk). EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances for 20 minutes of observation margin at start and end, and 30 minutes for turn to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew -32 mrad about x axis. Start data capture, stare 791.0 s, stop data capture. Repeat PATTERN 43 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 791.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1530.73137 bps, from Alain's spreadsheet)x(791.0s per stare)x(44 stares) = 53.2756x10^6 bits. Data rate multiplier includes an extra 1% per Alain because of data packet filling issues.",,,,,, 2011-281T07:00:00,000T01:50:00,8-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-281T17:58:00,000T00:02:00,8-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-281T17:58:00,000T00:02:00,8-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-281T20:16:00,000T09:00:00,8-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-281T20:16:00,000T09:00:00,8-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-281T21:16:00,000T08:00:00,8-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11281_SP,rider,,,,,, 2011-281T22:00:00,000T01:50:00,8-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-282T05:58:00,000T00:02:00,9-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-282T05:58:00,000T00:02:00,9-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-282T06:00:00,000T01:00:00,9-Oct-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-282T06:58:00,000T00:02:00,9-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-282T06:58:00,000T00:02:00,9-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-282T07:00:00,000T12:00:00,9-Oct-11,UVIS,Prime,Saturn,MOS154APO,,,"Mosaic scan of Saturn magnetosphere, day 4. Scan will focus on vicinity of Saturn disk to image oxygen. Overall extent of scan: +/- 2.5 Rs E-W and N-S (one quadrant covered in each of the first four observation periods; fifth period covers Saturn disk). EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances for 20 minutes of observation margin at start and end, and 30 minutes for turn to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew -32 mrad about x axis. Start data capture, stare 811.0 s, stop data capture. Repeat PATTERN 42 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 811.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1492.98214 bps, from Alain's spreadsheet)x(811.0s per stare)x(43 stares) = 52.065x10^6 bits. Data rate multiplier includes an extra 1% per Alain because of data packet filling issues.",,,,,, 2011-282T07:00:00,000T04:50:00,9-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-282T08:40:00,000T20:00:00,9-Oct-11,CDA,SPASS Rider,DustRAM direction,ISD0035,,CDA ISD 2011-283T14:40:00,ISD observation around apoapse 2011-283T14:40:00 40.397222 Rs,,,,,, 2011-282T18:58:00,000T00:02:00,9-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-282T18:58:00,000T00:02:00,9-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-282T20:01:00,000T09:00:00,9-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-282T21:01:00,000T08:00:00,9-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_154IC_DSCAL11282_SP,rider,,,,,, 2011-282T22:00:00,000T04:50:00,9-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-283T05:01:00,000T09:40:00,10-Oct-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-283T05:58:00,000T00:02:00,10-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-283T05:58:00,000T00:02:00,10-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-283T06:00:00,000T01:00:00,10-Oct-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-283T06:58:00,000T00:02:00,10-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-283T06:58:00,000T00:02:00,10-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-283T07:00:00,000T12:00:00,10-Oct-11,UVIS,Prime,Saturn,MOS154APO,,,"Mosaic scan of Saturn magnetosphere, day 5. Scan will focus on vicinity of Saturn disk to image oxygen. Overall extent of scan: +/- 2.5 Rs E-W and N-S (one quadrant covered in each of the first four observation periods; fifth period covers Saturn disk). EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances for 20 minutes of observation margin at start and end, and 30 minutes for turn to waypoint at end, have been made. Start at WAYPOINT (Saturn center). Align slit with Saturn spin axis. Slew +37.5 mrad about z axis. Start data capture, stare 679.0 s, stop data capture. Repeat PATTERN 50 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 679.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1783.22314 bps, from Alain's spreadsheet)x(679.0s per stare)x(51 stares) = 61.751234x10^6 bits. Data rate multiplier includes an extra 1% per Alain because of data packet filling issues.",,,,,, 2011-283T14:40:00,007T20:54:58,10-Oct-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.012016 Rs exit= 14.012778 Range altitude= 1437.7342 km ... 3137.7187,,,,,, 2011-283T14:40:00,007T18:17:00,10-Oct-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-283T14:40:34,000T00:00:01,10-Oct-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.8 d, inc = 0.2 deg, r = 40.357 Rs, phase = 50 deg",,,,,, 2011-283T14:41:00,000T02:00:00,10-Oct-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-283T14:41:00,008T00:05:00,10-Oct-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_154_155",,,,,, 2011-283T16:41:00,000T12:20:00,10-Oct-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-283T18:58:00,000T00:02:00,10-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-283T18:58:00,000T00:02:00,10-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-283T20:01:00,000T09:00:00,10-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-283T21:01:00,000T08:00:00,10-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11283_SP,rider,,,,,, 2011-284T00:40:00,000T20:00:00,11-Oct-11,CDA,SPASS Rider,DustRAM direction,ISD0035,,CDA ISD 2011-283T14:40:00,ISD observation around apoapse 2011-283T14:40:00 40.397222 Rs,,,,,, 2011-284T05:01:00,006T12:47:00,11-Oct-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-284T07:00:00,000T04:55:00,11-Oct-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,"MAPS MB,A Campaign","Part of MB,A MAPS Campaign. Observe plasma waves on dawn-side magnetospheric boundaries at a variety of radial distances",,,,,, 2011-284T20:01:00,000T09:00:00,11-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-284T20:01:00,000T09:00:00,11-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-284T21:01:00,000T08:00:00,11-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11284_SP,rider,,,,,, 2011-285T05:01:00,006T09:45:00,12-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-285T18:40:00,000T20:00:00,12-Oct-11,CDA,SPASS Rider,DustRAM direction,ISD0035,,CDA ISD 2011-283T14:40:00,ISD observation around apoapse 2011-283T14:40:00 40.397222 Rs,,,,,, 2011-285T20:01:00,000T09:00:00,12-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-285T20:01:00,000T09:00:00,12-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-285T21:01:00,000T08:00:00,12-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11285_SP,rider,,,,,, 2011-287T06:31:00,000T08:15:00,14-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-287T06:31:00,000T08:15:00,14-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-287T07:31:00,000T07:15:00,14-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11287_SP,rider,,,,,, 2011-288T06:01:00,000T09:00:00,15-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-288T06:01:00,000T09:00:00,15-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-288T07:01:00,000T08:00:00,15-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11288_SP,rider,,,,,, 2011-289T06:01:00,000T09:00:00,16-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-289T06:01:00,000T09:00:00,16-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-289T07:01:00,000T08:00:00,16-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11289_SP,rider,,,,,, 2011-289T15:01:00,000T13:15:00,16-Oct-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-290T05:46:00,000T09:00:00,17-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-290T05:46:00,000T09:00:00,17-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-290T06:46:00,000T08:00:00,17-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11290_SP,rider,,,,,, 2011-290T15:28:00,000T00:02:00,17-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-290T15:28:00,000T00:02:00,17-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-290T15:30:00,000T11:55:00,17-Oct-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-290T15:30:00,000T11:55:00,17-Oct-11,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2011-290T15:30:00,000T11:53:00,17-Oct-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-290T17:48:00,000T02:00:00,17-Oct-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-290T19:48:00,000T18:58:00,17-Oct-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-291T03:23:00,000T00:02:00,18-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-291T03:23:00,000T00:02:00,18-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-291T05:46:00,000T09:00:00,18-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-291T05:46:00,000T09:00:00,18-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-291T06:46:00,000T08:00:00,18-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11291_SP,rider,,,,,, 2011-291T08:57:00,000T05:49:00,18-Oct-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-291T11:34:58,002T01:36:00,18-Oct-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.999923 Rs exit= 13.990475 Range altitude= 3133.7401 km ... 1438.9036,,,,,, 2011-291T14:46:00,000T17:36:12,18-Oct-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-291T14:46:00,000T06:36:12,18-Oct-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-291T14:46:00,000T16:36:12,18-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-291T14:46:00,001T13:45:00,18-Oct-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_155_E15",,,,,, 2011-291T14:46:00,001T13:45:00,18-Oct-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-291T15:26:00,000T01:30:00,18-Oct-11,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 36.7 requested range 1.4 Mkm",,,,,, 2011-291T15:26:00,000T01:30:00,18-Oct-11,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-291T15:26:00,000T01:30:00,18-Oct-11,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase =37 range =1.4 Mkm.,,,,,, 2011-291T21:22:12,000T10:00:00,18-Oct-11,INMS,Non-SPASS,Enceladus,E15INBND,,Enceladus flyby,Enceladus observation,,,,,, 2011-291T23:50:00,000T02:00:00,18-Oct-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-291T23:50:00,000T02:00:00,18-Oct-11,CIRS,SPASS Rider,Titan,CLOUD,,,null,,,,,, 2011-291T23:50:00,000T02:00:00,18-Oct-11,VIMS,SPASS Rider,Titan,CLOUD,,titan clouds,follow iss,,,,,, 2011-292T02:30:00,000T04:10:00,19-Oct-11,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-292T02:30:00,000T04:10:00,19-Oct-11,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2011-292T02:30:00,000T04:10:00,19-Oct-11,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2011-292T02:30:00,000T04:10:00,19-Oct-11,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,enceladus,follow iss,,,,,, 2011-292T06:40:00,000T02:00:00,19-Oct-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-292T06:41:58,000T02:00:00,19-Oct-11,CDA,SPASS Rider,DustRAM direction,RPX0220,,CDA RPXing 2011-292T07:41:58,RPXing at 4.7495649 Rs,,,,,, 2011-292T06:45:00,000T02:03:00,19-Oct-11,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2011-292T06:45:00,000T02:03:00,19-Oct-11,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2011-292T06:45:00,000T02:03:00,19-Oct-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-292T06:45:00,000T02:03:00,19-Oct-11,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,enceladus,null,,,,,, 2011-292T07:22:12,000T04:00:00,19-Oct-11,INMS,Non-SPASS,Enceladus,ENCEL15,,Enceladus encounter,Enceladus observation,,,,,, 2011-292T07:22:12,000T04:00:00,19-Oct-11,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2011-292T08:22:12,000T02:00:00,19-Oct-11,CAPS,SPASS Rider,Titan,EN15CLOSE,,Closest Approach 155EN (15),null,,,,,, 2011-292T08:22:12,000T02:00:00,19-Oct-11,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2011-292T08:48:00,000T00:42:00,19-Oct-11,UVIS,Prime,Enceladus,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,"Target to epsilon Ori to observe plume occultation. Orient slit to get 2 stars in Orion's belt (eps Ori and zeta Ori). This will give us vertical structure in the plume, and pin down collimation of gas in the jets.",,,,,, 2011-292T08:48:00,000T00:42:00,19-Oct-11,CIRS,SPASS Rider,Enceladus,ICYEX,,,null,,,,,, 2011-292T08:48:00,000T00:42:00,19-Oct-11,ISS,SPASS Rider,Enceladus,ICYEX,,UVIS Enceladus rider,ORS observation,,,,,, 2011-292T08:52:12,000T01:00:00,19-Oct-11,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 142,BIT_OVERLAY_300,,,,,, 2011-292T09:30:00,000T02:20:00,19-Oct-11,CIRS,Prime,Enceladus,ENCELADUS,Enceladus,CIRS Enceladus PIE,"09:30 - 09:40 Pick up turn (67 deg/8 mins iDigit) 09:40 - 10:00 FP1 N/S diametric scan @ 300 mu rad/s, followed by a L/R equatorial scan, then parallel scans along roughly the +30 and -30 merdians if time permits. 10:00 - 10:15 Full FP1 raster scan, without overlap between scans if necesscery to get full disk coverage 10:15 - 10:50 Baseline for eclipse and eclipse-emergence. Series of equatorial limb-to-limb scans @ 300 mu rad/s during emergence 10:50 - 11:45 FP3 map of subsolar region, consisting of two abutting 8-mrad long swaths at 6 murad/sec. Brief FP1 stare at the end to provide one more point on the warming curve. 11:45 - 11:50 Turn. 15.5 cm-1; FP1+FP3; Blink. CLR1-CLR2, 2x2 summation mode for SI. Timing TBD (but see above).",,,,,, 2011-292T09:30:00,000T02:20:00,19-Oct-11,CIRS,SPASS Rider,Enceladus,FP1SECLX,,CIRS_155EN_FP1SECLX001 eclipse support images,"Five clear WAC images (at 50 second intervals centered on nominal eclipse exit at 2011-292T10:20:33) at 2011-292T10:18:53. T10:19:43, T10:20:33, T10:21:23, and T10:22:13. Clear; 2x2 summation mode.",,,,,, 2011-292T09:30:00,000T02:20:00,19-Oct-11,ISS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,CIRS Enceladus rider,ORS observation,,,,,, 2011-292T09:30:00,000T02:20:00,19-Oct-11,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,ICYMAP: UV Surface Map,Map surface albedo in UV. Limb drifts to determine atmospheric scattering.,,,,,, 2011-292T09:30:00,000T02:20:00,19-Oct-11,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,enceladus,follow cirs,,,,,, 2011-292T10:22:12,000T09:23:48,19-Oct-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-292T11:22:12,000T10:00:00,19-Oct-11,INMS,Non-SPASS,Enceladus,E15OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2011-292T11:22:12,000T04:57:48,19-Oct-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-292T12:23:30,000T00:00:01,19-Oct-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.259 Rs, lat = -0 deg, phase = 130 deg",,,,,, 2011-292T14:06:00,000T14:25:00,19-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-292T14:06:00,000T05:25:00,19-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-292T16:20:00,000T12:11:00,19-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-292T18:31:00,000T10:00:00,19-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11292_SP,rider,,,,,, 2011-292T19:31:00,000T09:00:00,19-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-292T19:46:00,000T08:45:00,19-Oct-11,CAPS,Non-SPASS,Saturn,8KBURST,,8k burst,null,,,,,, 2011-292T20:31:00,000T07:00:00,19-Oct-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-292T21:22:12,000T03:37:48,19-Oct-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-292T22:57:58,000T02:00:00,19-Oct-11,CDA,SPASS Rider,DustRAM direction,RPX0230,,CDA RPXing 2011-292T23:57:58,RPXing at 8.2194446 Rs,,,,,, 2011-293T01:00:00,000T02:00:00,20-Oct-11,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2011-293T03:00:00,000T01:31:00,20-Oct-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-293T04:31:00,016T16:46:00,20-Oct-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-293T04:31:00,001T00:00:00,20-Oct-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-293T04:31:00,002T02:59:00,20-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-293T04:31:00,008T05:40:00,20-Oct-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_155_156",,,,,, 2011-293T04:31:00,000T11:19:00,20-Oct-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-293T05:28:00,000T00:02:00,20-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-293T05:28:00,000T00:02:00,20-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-293T05:30:00,000T10:00:00,20-Oct-11,ISS,Prime,rings(general),ARCLELR,,Faint Ring Low Phase Observation,Observation of faint rings at low elevation angles and low phase,,,,,, 2011-293T05:30:00,000T10:00:00,20-Oct-11,CIRS,SPASS Rider,rings(general),ARCLELR,,,null,,,,,, 2011-293T05:30:00,000T09:58:00,20-Oct-11,VIMS,SPASS Rider,rings(general),ARCLELR,,Faint ring observation,ISS rider; 1 second IR integration time,,,,,, 2011-293T13:10:58,007T20:59:02,20-Oct-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.003331 Rs exit= 14.003404 Range altitude= 1442.2792 km ... 3119.1998,,,,,, 2011-293T15:28:00,000T00:02:00,20-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-293T15:28:00,000T00:02:00,20-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-293T15:30:00,000T03:00:00,20-Oct-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2011-293T15:50:00,007T18:20:00,20-Oct-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-293T18:28:00,000T00:02:00,20-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-293T18:28:00,000T00:02:00,20-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-293T19:31:00,000T09:00:00,20-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-293T20:31:00,000T08:00:00,20-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11293_SP,rider,,,,,, 2011-294T04:31:00,000T14:45:00,21-Oct-11,ISS,Prime,Other,LOGROT,,Loge,Observation of irregular moon of Saturn.,,,,,, 2011-294T04:31:00,000T23:45:00,21-Oct-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-294T19:16:00,000T09:00:00,21-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-294T20:16:00,000T08:00:00,21-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11294_SP,rider,,,,,, 2011-295T00:00:00,000T01:08:00,22-Oct-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-295T04:16:00,006T05:55:00,22-Oct-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-295T04:58:00,000T00:02:00,22-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-295T04:58:00,000T00:02:00,22-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-295T05:00:00,000T01:30:00,22-Oct-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 48.9 requested range 2.4 Mkm",,,,,, 2011-295T05:00:00,000T01:30:00,22-Oct-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-295T05:00:00,000T01:26:00,22-Oct-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase =50 range =2.4 Mkm.,,,,,, 2011-295T06:28:00,000T00:02:00,22-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-295T06:28:00,000T00:02:00,22-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-295T06:30:00,000T01:00:00,22-Oct-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-295T07:28:00,000T00:02:00,22-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-295T07:28:00,000T00:02:00,22-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-295T07:30:00,000T07:00:00,22-Oct-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-295T14:28:00,000T00:02:00,22-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-295T14:28:00,000T00:02:00,22-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-295T14:30:00,000T03:30:00,22-Oct-11,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2011-295T14:30:00,000T03:30:00,22-Oct-11,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2011-295T14:30:00,014T06:47:00,22-Oct-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-295T17:58:00,000T00:02:00,22-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-295T17:58:00,000T00:02:00,22-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-295T18:00:00,000T23:00:00,22-Oct-11,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2011-296T16:58:00,000T00:02:00,23-Oct-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-296T16:58:00,000T00:02:00,23-Oct-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-296T19:17:00,000T09:00:00,23-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-296T19:17:00,000T09:00:00,23-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-296T20:17:00,000T08:00:00,23-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11296_SP,rider,,,,,, 2011-297T05:00:00,000T19:00:00,24-Oct-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-297T05:00:00,000T19:00:00,24-Oct-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-297T05:00:00,000T19:00:00,24-Oct-11,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=2.3 to 2.1 Phase=65,,,,,, 2011-298T01:30:00,000T01:30:00,25-Oct-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-298T05:32:00,000T09:00:00,25-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-298T05:32:00,000T09:00:00,25-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-298T06:32:00,000T08:00:00,25-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11298_SP,rider,,,,,, 2011-298T10:10:00,000T20:00:00,25-Oct-11,CDA,SPASS Rider,DustRAM direction,ISD0036,,CDA ISD 2011-301T10:10:00,ISD observation around apoapse 2011-301T10:10:00 40.398870 Rs,,,,,, 2011-298T14:32:00,000T13:15:00,25-Oct-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-298T14:32:00,000T13:15:00,25-Oct-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-298T14:32:00,000T13:15:00,25-Oct-11,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=2.3 to 2.1 Phase=65,,,,,, 2011-299T05:17:00,000T09:00:00,26-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-299T06:17:00,000T08:00:00,26-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11299_SP,rider,,,,,, 2011-299T14:17:00,000T13:30:00,26-Oct-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-299T14:17:00,000T13:30:00,26-Oct-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-299T14:17:00,000T13:30:00,26-Oct-11,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=2.3 to 2.1 Phase=65,,,,,, 2011-300T05:17:00,000T09:00:00,27-Oct-11,RSS,SPASS Rider,Earth,SCE8,,Solar Conjunction Experiment (SCE) #8,"Characterize the solar corona at 2 frequency bands (X and Ka1 or X and S, depending on DSN antenna requested by SP), and assess the electron content and possible Faraday rotation, during the solar conjunction period.",,,,,, 2011-300T05:17:00,000T09:00:00,27-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-300T06:17:00,000T08:00:00,27-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11300_SP,rider,,,,,, 2011-300T14:17:00,000T15:00:00,27-Oct-11,CDA,Prime,DustRAM direction,ISD0036,,CDA ISD 2011-301T10:10:00,ISD observation around apoapse 2011-301T10:10:00 40.398870 Rs,,,,,, 2011-301T05:17:00,000T09:00:00,28-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-301T06:17:00,000T08:00:00,28-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_155IC_DSCAL11301_SP,rider,,,,,, 2011-301T10:10:00,007T21:00:57,28-Oct-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.003331 Rs exit= 14.003404 Range altitude= 1442.2792 km ... 3119.1998,,,,,, 2011-301T10:10:00,007T18:21:00,28-Oct-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-301T10:10:57,000T00:00:01,28-Oct-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.8 d, inc = 0.2 deg, r = 40.358 Rs, phase = 50 deg",,,,,, 2011-301T10:11:00,000T04:06:00,28-Oct-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Orbit Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-301T10:11:00,008T11:06:00,28-Oct-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_155_156",,,,,, 2011-301T14:17:00,000T15:00:00,28-Oct-11,CDA,Prime,DustRAM direction,ISD0036,,CDA ISD 2011-301T10:10:00,ISD observation around apoapse 2011-301T10:10:00 40.398870 Rs,,,,,, 2011-301T14:17:00,001T00:00:00,28-Oct-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-302T05:17:00,000T09:00:00,29-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-302T06:17:00,000T08:00:00,29-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11302_SP,rider,,,,,, 2011-302T14:17:00,000T13:15:00,29-Oct-11,CDA,Prime,DustRAM direction,ISD0036,,CDA ISD 2011-301T10:10:00,ISD observation around apoapse 2011-301T10:10:00 40.398870 Rs,,,,,, 2011-302T14:17:00,004T13:30:00,29-Oct-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-303T05:02:00,000T04:00:00,30-Oct-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-303T05:02:00,000T09:00:00,30-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-303T06:02:00,000T08:00:00,30-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11303_SP,rider,,,,,, 2011-303T14:02:00,000T13:30:00,30-Oct-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-303T14:02:00,000T13:30:00,30-Oct-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-303T14:02:00,000T13:30:00,30-Oct-11,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=2.3 to 2.1 Phase=65,,,,,, 2011-304T05:02:00,000T09:00:00,31-Oct-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-304T06:02:00,000T08:00:00,31-Oct-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11304_SP,rider,,,,,, 2011-304T14:02:00,000T13:30:00,31-Oct-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-304T14:02:00,000T13:30:00,31-Oct-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-304T14:02:00,000T13:30:00,31-Oct-11,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=2.3 to 2.1 Phase=65,,,,,, 2011-305T05:02:00,000T09:00:00,1-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-305T06:02:00,000T08:00:00,1-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11305_SP,rider,,,,,, 2011-305T14:02:00,001T04:45:00,1-Nov-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-305T14:02:00,001T04:45:00,1-Nov-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-306T18:47:00,000T09:00:00,2-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-306T19:47:00,000T08:00:00,2-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11306_SP,rider,,,,,, 2011-307T03:47:00,000T15:00:00,3-Nov-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-307T03:47:00,000T15:00:00,3-Nov-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-307T03:47:00,000T15:00:00,3-Nov-11,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=2.3 to 2.1 Phase=65,,,,,, 2011-307T03:47:00,001T00:00:00,3-Nov-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-307T18:47:00,000T09:00:00,3-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-307T19:47:00,000T08:00:00,3-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11307_SP,rider,,,,,, 2011-308T03:47:00,000T09:36:00,4-Nov-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-308T04:28:00,000T00:02:00,4-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-308T04:28:00,000T00:02:00,4-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-308T10:00:00,000T01:00:00,4-Nov-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-308T10:58:00,000T00:02:00,4-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-308T10:58:00,000T00:02:00,4-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-308T11:00:00,000T12:00:00,4-Nov-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-308T13:23:00,000T02:00:00,4-Nov-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-308T15:23:00,001T01:35:53,4-Nov-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-308T22:58:00,000T00:02:00,4-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-308T22:58:00,000T00:02:00,4-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-308T23:00:00,000T11:00:00,4-Nov-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-308T23:00:00,000T11:00:00,4-Nov-11,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2011-308T23:00:00,000T10:58:00,4-Nov-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-309T00:00:00,000T01:08:00,5-Nov-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-309T04:31:00,000T16:46:00,5-Nov-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-309T07:10:57,000T14:06:03,5-Nov-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.990548 Rs exit= 13.988640 Range altitude= 3115.2254 km ... 1446.4904,,,,,, 2011-309T09:58:00,000T00:02:00,5-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-309T09:58:00,000T00:02:00,5-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-309T12:17:00,000T09:00:00,5-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-309T13:17:00,000T08:00:00,5-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11309_SP,rider,,,,,, 2011-309T16:58:53,000T04:18:07,5-Nov-11,INMS,Non-SPASS,Enceladus,SURVENCEL,,Enceladus flyby,Enceladus observation,,,,,, 2011-309T21:17:00,000T06:41:53,5-Nov-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-309T21:17:00,001T11:27:57,5-Nov-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.990548 Rs exit= 13.988640 Range altitude= 3115.2254 km ... 1446.4904,,,,,, 2011-309T21:17:00,000T05:41:53,5-Nov-11,INMS,Non-SPASS,Enceladus,E16INBND,,Enceladus flyby,Enceladus observation,,,,,, 2011-309T21:17:00,000T05:41:53,5-Nov-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-309T21:17:00,002T06:15:00,5-Nov-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_156_E16",,,,,, 2011-309T21:17:00,001T14:08:00,5-Nov-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-309T22:15:00,000T02:00:00,5-Nov-11,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2011-309T22:15:00,000T02:00:00,5-Nov-11,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2011-309T22:15:00,000T02:00:00,5-Nov-11,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2011-309T22:15:00,000T02:00:00,5-Nov-11,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,Enceladus Plume,Enceladus,,,,,, 2011-309T22:15:00,000T04:42:00,5-Nov-11,RADAR,Non-SPASS,Enceladus,E16WARMUP,,Warmup for E16,,,,,,, 2011-310T00:15:00,000T02:42:00,6-Nov-11,CIRS,Prime,Enceladus,ENCELADUS,Enceladus,,"00:15 - 00:18 Turn 00:18 - 02:27 3 FP3 global scans of Enceladus, each scan has 2 swaths. 02:27 - 02:57 Turn",,,,,, 2011-310T00:15:00,000T02:42:00,6-Nov-11,ISS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,CIRS Enceladus rider,ORS observation,,,,,, 2011-310T00:15:00,000T02:42:00,6-Nov-11,VIMS,SPASS Rider,Enceladus,SCAN,System scan,Enceladus,Enceladus,,,,,, 2011-310T02:13:00,000T01:45:53,6-Nov-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-310T02:57:00,000T01:22:10,6-Nov-11,RADAR,Prime,Enceladus,ENCELINB,,E16 Inbound RAD/SCATT/HiSAR,SOST E16 PIE.,,,,,, 2011-310T02:58:53,000T04:00:00,6-Nov-11,INMS,Non-SPASS,Enceladus,ENCEL16,,Enceladus encounter,Enceladus observation,,,,,, 2011-310T02:58:53,000T04:00:00,6-Nov-11,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2011-310T03:58:53,000T02:00:00,6-Nov-11,CAPS,SPASS Rider,Titan,EN16CLOSE,,Closest Approach 156EN (16),null,,,,,, 2011-310T03:58:53,000T02:00:00,6-Nov-11,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2011-310T04:19:10,000T00:31:19,6-Nov-11,RADAR,Prime,Enceladus,ENCELINB,,E16 Inbound RAD/SCATT/HiSAR,SOST E16 PIE.,,,,,, 2011-310T04:28:53,000T01:00:00,6-Nov-11,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 142,BIT_OVERLAY_300,,,,,, 2011-310T04:51:29,000T00:44:24,6-Nov-11,RADAR,Prime,Enceladus,ENCELCA,,E16 Inb/outb Imaging Near C/A,SOST E16 PIE.,,,,,, 2011-310T05:56:58,000T01:24:07,6-Nov-11,RADAR,Prime,Enceladus,ENCELOUTB,,E16 Outbound HiSAR/SCATT/RAD,SOST E16 PIE.,,,,,, 2011-310T05:58:53,001T21:33:07,6-Nov-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-310T06:58:53,000T10:00:00,6-Nov-11,INMS,Non-SPASS,Enceladus,E16OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2011-310T06:58:53,000T04:56:07,6-Nov-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-310T07:21:09,000T03:29:56,6-Nov-11,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2011-310T07:21:09,000T03:29:56,6-Nov-11,CIRS,SPASS Rider,Enceladus,ENCEL,Enceladus,,null,,,,,, 2011-310T07:21:09,000T03:29:56,6-Nov-11,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-310T07:21:09,000T03:29:56,6-Nov-11,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus Plume,Enceladus,,,,,, 2011-310T07:58:12,000T00:00:01,6-Nov-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.260 Rs, lat = -0 deg, phase = 130 deg",,,,,, 2011-310T10:53:00,000T05:14:00,6-Nov-11,UVIS,Prime,Dione,ICYSTARE,,ICYSTARE: Satellite/System Volatile Map,Map volatiles in system in immediate neighborhood of satellite.,,,,,, 2011-310T10:53:00,000T05:14:00,6-Nov-11,CIRS,SPASS Rider,Dione,ICYSTARE,,,null,,,,,, 2011-310T10:53:00,000T05:14:00,6-Nov-11,ISS,SPASS Rider,Dione,ICYSTARE,,Dione,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-310T10:53:00,000T05:14:00,6-Nov-11,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,Dione stare,,,,,, 2011-310T11:55:00,001T15:37:00,6-Nov-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-310T16:07:00,000T03:00:00,6-Nov-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2011-310T16:07:00,000T03:00:00,6-Nov-11,VIMS,SPASS Rider,Dione,SPICACAL,,Spica,Spica calibration,,,,,, 2011-310T16:58:53,000T04:01:07,6-Nov-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-310T19:47:00,000T09:00:00,6-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-310T20:47:00,000T09:30:00,6-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11310_SP,rider,,,,,, 2011-310T21:00:00,000T02:00:00,6-Nov-11,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2011-310T23:00:00,001T04:32:00,6-Nov-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-311T07:47:00,000T04:23:00,7-Nov-11,ISS,Prime,Other,L5ENCE,,Enceladus L5 satellite search,Satellite search around Enceladus L5 Lagrange point.,,,,,, 2011-311T07:47:00,000T04:23:00,7-Nov-11,VIMS,SPASS Rider,Other,L5ENC,,L5 Rocks,L5 Rocks,,,,,, 2011-311T08:44:57,007T21:27:03,7-Nov-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.001504 Rs exit= 14.003424 Range altitude= 1449.8337 km ... 2469.7022,,,,,, 2011-311T11:25:00,000T16:07:00,7-Nov-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-311T12:10:00,000T04:52:00,7-Nov-11,ISS,Prime,Other,L5RHEA,,Rhea L5 satellite search,Satellite search around Rhea L5 Lagrange point.,,,,,, 2011-311T12:10:00,000T04:52:00,7-Nov-11,VIMS,SPASS Rider,Other,L5ENCA,,L5 Rocks,L5 Rocks,,,,,, 2011-311T18:32:00,000T09:00:00,7-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-311T19:32:00,000T08:00:00,7-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11311_SP,rider,,,,,, 2011-312T03:32:00,007T23:30:00,8-Nov-11,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2011-312T03:32:00,000T23:45:00,8-Nov-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-312T03:32:00,003T17:30:00,8-Nov-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-312T03:32:00,007T02:41:00,8-Nov-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_156_157",,,,,, 2011-312T03:32:00,007T02:40:00,8-Nov-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-312T04:10:00,000T00:02:00,8-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-312T04:12:00,000T09:55:00,8-Nov-11,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2011-312T04:12:00,000T09:55:00,8-Nov-11,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2011-312T14:05:00,000T00:02:00,8-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-312T14:47:00,000T03:30:00,8-Nov-11,ISS,Prime,Other,TITANL4,,Titan L4 satellite search,Satellite search around Titan L4 Lagrange point.,,,,,, 2011-312T18:17:00,000T09:00:00,8-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-312T19:17:00,000T08:00:00,8-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11312_SP,rider,,,,,, 2011-313T03:17:00,000T15:00:00,9-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-313T03:17:00,001T00:00:00,9-Nov-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-313T18:17:00,000T09:00:00,9-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-313T19:17:00,000T08:00:00,9-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11313_SP,rider,,,,,, 2011-314T03:17:00,001T07:15:00,10-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-314T03:17:00,005T02:56:00,10-Nov-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-315T12:02:00,000T09:00:00,11-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-315T13:02:00,000T08:00:00,11-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11315_SP,rider,,,,,, 2011-315T21:02:00,000T07:00:00,11-Nov-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-316T04:02:00,001T12:30:00,12-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-316T04:02:00,003T23:00:00,12-Nov-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-316T06:12:00,000T20:00:00,12-Nov-11,CDA,SPASS Rider,DustRAM direction,ISD0037,,CDA ISD 2011-319T06:12:00,ISD observation around apoapse 2011-319T06:12:00 40.460618 Rs,,,,,, 2011-317T18:02:00,000T04:00:00,13-Nov-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-317T18:02:00,000T09:00:00,13-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-317T19:02:00,000T08:00:00,13-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_156IC_DSCAL11317_SP,rider,,,,,, 2011-318T00:12:00,000T20:00:00,14-Nov-11,CDA,SPASS Rider,DustRAM direction,ISD0037,,CDA ISD 2011-319T06:12:00,ISD observation around apoapse 2011-319T06:12:00 40.460618 Rs,,,,,, 2011-318T03:02:00,001T13:30:00,14-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-319T06:12:00,000T20:50:00,15-Nov-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S71,Range enter= 14.001504 Rs exit= 14.003424 Range altitude= 1449.8337 km ... 2469.7022,,,,,, 2011-319T06:12:00,000T20:50:00,15-Nov-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-319T06:12:47,000T00:00:01,15-Nov-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.9 d, inc = 0.2 deg, r = 40.424 Rs, phase = 50 deg",,,,,, 2011-319T06:13:00,000T02:00:00,15-Nov-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-319T06:13:00,000T20:49:00,15-Nov-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_156_157",,,,,, 2011-319T08:13:00,000T18:49:00,15-Nov-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-319T16:12:00,000T10:50:00,15-Nov-11,CDA,SPASS Rider,DustRAM direction,ISD0037,,CDA ISD 2011-319T06:12:00 End: S71,ISD observation around apoapse 2011-319T06:12:00 40.460618 Rs,,,,,, 2011-319T18:02:00,000T09:00:00,15-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-319T19:02:00,000T08:00:00,15-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11319_SP,rider,,,,,, 2011-320T03:02:00,006T20:58:00,16-Nov-11,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2011-320T03:02:00,000T09:10:00,16-Nov-11,CDA,SPASS Rider,DustRAM direction,ISD0037,,CDA ISD 2011-319T06:12:00 Enter: S71,ISD observation around apoapse 2011-319T06:12:00 40.460618 Rs,,,,,, 2011-320T03:02:00,007T00:42:57,16-Nov-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S71,Range enter= 14.001504 Rs exit= 14.003424 Range altitude= 1449.8337 km ... 2469.7022,,,,,, 2011-320T03:02:00,000T00:43:00,16-Nov-11,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-320T03:02:00,006T23:31:00,16-Nov-11,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2011-320T03:02:00,009T09:31:00,16-Nov-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_157",,,,,, 2011-320T03:02:00,006T22:03:00,16-Nov-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-320T03:07:00,000T00:02:00,16-Nov-11,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S71 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2011-320T03:08:00,001T13:10:00,16-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-320T03:45:00,000T00:07:00,16-Nov-11,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-320T03:52:00,000T00:05:00,16-Nov-11,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-320T03:57:00,000T00:33:00,16-Nov-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2011-320T04:00:00,000T12:00:00,16-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-320T04:30:00,000T00:30:00,16-Nov-11,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2011-320T05:00:00,002T19:00:00,16-Nov-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-321T10:12:00,000T20:00:00,17-Nov-11,CDA,SPASS Rider,DustRAM direction,ISD0037,,CDA ISD 2011-319T06:12:00,ISD observation around apoapse 2011-319T06:12:00 40.460618 Rs,,,,,, 2011-321T17:48:00,000T09:00:00,17-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-321T18:48:00,000T08:00:00,17-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11321_SP,rider,,,,,, 2011-322T02:48:00,001T13:30:00,18-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-322T04:00:00,000T12:00:00,18-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-323T00:00:00,000T00:34:00,19-Nov-11,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2011-323T00:34:00,003T22:12:37,19-Nov-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-323T17:48:00,000T09:00:00,19-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-323T18:48:00,000T08:00:00,19-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11323_SP,rider,,,,,, 2011-324T02:48:00,000T13:15:00,20-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-324T03:00:00,000T14:00:00,20-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-324T17:33:00,000T09:00:00,20-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-324T18:33:00,000T08:00:00,20-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11324_SP,rider,,,,,, 2011-324T19:00:00,000T05:00:00,20-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-325T00:00:00,000T01:08:00,21-Nov-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-325T02:33:00,000T08:00:00,21-Nov-11,ISS,Prime,Other,SUTPHA,,Suttungr,Observation of irregular moon of Saturn.,,,,,, 2011-325T03:00:00,000T09:00:00,21-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-325T10:33:00,000T05:30:00,21-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-325T13:33:00,000T13:00:00,21-Nov-11,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,"RSS USO characterization plus PIM. Pointing=XBAND to Earth. No rolling during 3-hour USO from 2011-325T17:33:00 till 2011-325T20:33:00, to be tracked at DSS-34 in 1-way mode. Keep Ka-band ON till end of downlink to satisfy PIM requirement.",,,,,, 2011-325T17:33:00,000T03:25:00,21-Nov-11,RSS,SPASS Rider,Dione,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev158 Dione gravity observation on 2011/346. DSS-25 required for X- and Ka-band support.",,,,,, 2011-325T17:33:00,000T09:00:00,21-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-325T21:18:00,000T05:15:00,21-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11325_SP,rider,,,,,, 2011-326T02:33:00,000T13:30:00,22-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-326T03:00:00,000T14:00:00,22-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-326T17:33:00,000T09:00:00,22-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-326T18:33:00,000T08:00:00,22-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11326_SP,rider,,,,,, 2011-326T18:35:00,000T05:00:00,22-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-326T22:46:37,000T23:00:00,22-Nov-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-327T00:00:00,001T07:30:00,23-Nov-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-327T01:05:00,002T06:51:00,23-Nov-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-327T02:33:00,000T00:40:00,23-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-327T02:33:00,000T00:40:00,23-Nov-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-327T03:11:00,000T00:02:00,23-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-327T03:13:00,000T01:30:00,23-Nov-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 86.6 requested range 2.1 Mkm",,,,,, 2011-327T03:13:00,000T01:30:00,23-Nov-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-327T03:13:00,000T01:30:00,23-Nov-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 87 range =2.1 Mkm. Also contains Stormwatch cube.,,,,,, 2011-327T03:13:00,000T16:31:00,23-Nov-11,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2011-327T03:44:57,002T01:32:00,23-Nov-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.990559 Rs exit= 13.988915 Range altitude= 2466.2198 km ... 1687.1107,,,,,, 2011-327T04:41:00,000T00:02:00,23-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-327T04:43:00,000T10:41:00,23-Nov-11,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2011-327T04:43:00,000T10:41:00,23-Nov-11,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Stare Ridealong.,Auroral Stare Ridealong and Stormwatch cube,,,,,, 2011-327T15:22:00,000T00:02:00,23-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-327T16:00:00,001T00:00:00,23-Nov-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-327T16:33:00,000T07:46:00,23-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-327T19:44:00,000T04:56:00,23-Nov-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-327T21:24:00,000T10:54:00,23-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11327_SP,rider,,,,,, 2011-327T21:46:00,000T02:00:00,23-Nov-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-327T21:46:37,000T02:00:00,23-Nov-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-327T21:47:57,000T02:00:00,23-Nov-11,CDA,SPASS Rider,DustRAM direction,RPX0260,,CDA RPXing 2011-327T22:47:57,RPXing at 5.2688865 Rs,,,,,, 2011-327T23:46:37,000T08:31:23,23-Nov-11,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2011-328T00:40:00,000T08:08:00,24-Nov-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-328T03:13:00,000T05:05:00,24-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-328T04:13:00,000T03:00:00,24-Nov-11,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2011-328T04:31:31,000T00:00:01,24-Nov-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.255 Rs, lat = -0 deg, phase = 130 deg",,,,,, 2011-328T07:30:00,000T20:03:00,24-Nov-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-328T08:18:00,001T04:15:00,24-Nov-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-328T08:43:00,000T03:57:00,24-Nov-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-328T08:48:00,000T18:05:00,24-Nov-11,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2011-328T12:40:00,000T02:00:00,24-Nov-11,CDA,Prime,DustRAM direction,RPX0270,,CDA RPXing 2011-328T13:39:57,RPXing at 6.9988158 Rs,,,,,, 2011-328T14:40:00,000T12:53:00,24-Nov-11,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-329T02:53:00,000T09:40:00,25-Nov-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-329T03:33:00,000T09:00:00,25-Nov-11,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2011-329T03:33:00,000T09:00:00,25-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-329T04:33:00,000T08:00:00,25-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11329_SP,rider,,,,,, 2011-329T05:16:57,007T21:56:03,25-Nov-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.001796 Rs exit= 14.007734 Range altitude= 1690.3222 km ... 2469.6904,,,,,, 2011-329T07:56:00,000T04:37:00,25-Nov-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-329T12:33:00,014T23:17:00,25-Nov-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-329T12:33:00,000T09:27:00,25-Nov-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-329T12:33:00,009T13:16:00,25-Nov-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-329T12:33:00,007T14:40:00,25-Nov-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_157_158",,,,,, 2011-329T12:33:00,007T14:40:00,25-Nov-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-329T12:40:00,000T00:40:00,25-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-329T13:18:00,000T00:02:00,25-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-329T13:20:00,000T03:00:00,25-Nov-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration,"Typical slew rate for calibrations is 0.02mrad/s, and for this observation we request 5x slower (0.004mrad/s). The integration time is typically 45sec, and we request a decreased integration time of nominally 2x lower (i.e. 20sec), but may be adjusted to accommodate data volume constraints.",,,,,, 2011-329T13:20:00,000T03:00:00,25-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-329T16:18:00,000T00:02:00,25-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-329T16:20:00,000T18:00:00,25-Nov-11,ISS,Prime,rings(general),ARCLELR,,Faint Ring Low Phase Observation,Observation of faint rings at low elevation angles and low phase,,,,,, 2011-329T16:20:00,000T18:00:00,25-Nov-11,CIRS,SPASS Rider,rings(general),ARCLELR,,,null,,,,,, 2011-329T16:20:00,000T18:00:00,25-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-329T22:00:00,000T02:00:00,25-Nov-11,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2011-330T00:00:00,006T02:04:00,26-Nov-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-330T08:00:00,002T00:00:00,26-Nov-11,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde Hyperion,Retrograde observation around Hyperion - outbound leg,,,,,, 2011-330T10:18:00,000T00:02:00,26-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-330T10:20:00,000T14:40:00,26-Nov-11,ISS,Prime,Other,THRROT,,Thrymr,Observation of irregular moon of Saturn.,,,,,, 2011-330T10:20:00,000T14:40:00,26-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-331T00:58:00,000T00:02:00,27-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-331T03:33:00,000T09:00:00,27-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-331T04:33:00,000T08:00:00,27-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11331_SP,rider,,,,,, 2011-331T11:00:00,000T08:45:00,27-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-331T18:00:00,000T15:34:00,27-Nov-11,CIRS,Prime,Titan,COMPMAP,Composition map,Titan Composition,Titan composition,,,,,, 2011-331T18:00:00,000T15:34:00,27-Nov-11,ISS,SPASS Rider,Titan,COMPMAP,Composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-331T18:00:00,000T15:34:00,27-Nov-11,VIMS,SPASS Rider,Titan,COMPMAP,Composition map,Titan Monitoring Campaign,Titan Monitoring Campaign; phase =?? range =?? Mkm - one cube per hour.,,,,,, 2011-332T11:04:00,000T09:00:00,28-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-332T12:04:00,000T08:00:00,28-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11332_SP,rider,,,,,, 2011-332T20:04:00,000T13:15:00,28-Nov-11,CDA,Prime,DustRAM direction,ISD0038,,CDA ISD 2011-337T03:13:00,ISD observation around apoapse 2011-337T03:13:00 40.537579 Rs,,,,,, 2011-333T10:49:00,000T09:00:00,29-Nov-11,RSS,SPASS Rider,Dione,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev158 Dione gravity observation on 2011/346. DSS-25 and DSS-55 required for X- and Ka-band support.",,,,,, 2011-333T10:49:00,000T09:00:00,29-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-333T11:49:00,000T08:00:00,29-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11333_SP,rider,,,,,, 2011-333T19:49:00,000T00:41:00,29-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-333T20:00:00,000T16:30:00,29-Nov-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-333T20:28:00,000T00:02:00,29-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-333T20:30:00,000T01:00:00,29-Nov-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-333T20:30:00,000T01:00:00,29-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-333T21:28:00,000T00:02:00,29-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-333T21:30:00,000T13:30:00,29-Nov-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-333T21:30:00,000T13:30:00,29-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-334T10:58:00,000T00:02:00,30-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-334T11:00:00,000T04:00:00,30-Nov-11,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2011-334T11:00:00,000T04:00:00,30-Nov-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-334T11:00:00,000T04:00:00,30-Nov-11,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2011-334T14:58:00,000T00:02:00,30-Nov-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-334T15:34:00,000T06:00:00,30-Nov-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-334T17:04:00,000T09:00:00,30-Nov-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-334T18:04:00,000T08:00:00,30-Nov-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11334_SP,rider,,,,,, 2011-335T02:04:00,000T15:00:00,1-Dec-11,CDA,Prime,DustRAM direction,ISD0038,,CDA ISD 2011-337T03:13:00,ISD observation around apoapse 2011-337T03:13:00 40.537579 Rs,,,,,, 2011-335T02:30:00,000T14:30:00,1-Dec-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-335T17:04:00,000T09:00:00,1-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-335T18:04:00,000T08:00:00,1-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11335_SP,rider,,,,,, 2011-335T18:30:00,000T04:00:00,1-Dec-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-336T02:04:00,000T14:45:00,2-Dec-11,CDA,Prime,DustRAM direction,ISD0038,,CDA ISD 2011-337T03:13:00,ISD observation around apoapse 2011-337T03:13:00 40.537579 Rs,,,,,, 2011-336T02:04:00,000T23:45:00,2-Dec-11,INMS,Non-SPASS,Saturn,SURVPOTMA,,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-336T02:05:00,000T14:30:00,2-Dec-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-336T16:49:00,000T09:00:00,2-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-336T17:49:00,000T08:00:00,2-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_157IC_DSCAL11336_SP,rider,,,,,, 2011-336T17:49:00,000T07:00:00,2-Dec-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-337T01:49:00,000T01:24:00,3-Dec-11,INMS,Non-SPASS,Saturn,SURVBOTMA,,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-337T03:13:00,007T22:01:57,3-Dec-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.001796 Rs exit= 14.007734 Range altitude= 1690.3222 km ... 2469.6904,,,,,, 2011-337T03:13:00,000T02:00:00,3-Dec-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-337T03:13:00,007T08:37:00,3-Dec-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_157_158",,,,,, 2011-337T03:13:00,003T22:21:00,3-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-337T03:13:14,000T00:00:01,3-Dec-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.9 d, inc = 0.2 deg, r = 40.497 Rs, phase = 49 deg",,,,,, 2011-337T05:13:00,006T06:36:00,3-Dec-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-337T10:50:00,000T00:40:00,3-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-337T11:28:00,000T00:02:00,3-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-337T11:30:00,000T01:09:00,3-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-337T11:30:00,000T01:09:00,3-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-337T12:37:00,000T00:02:00,3-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-337T14:09:00,000T23:00:00,3-Dec-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-337T14:09:00,000T23:00:00,3-Dec-11,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Saturn CIRS MIRMAP ridealong,CIRS MIRMAP Ridealong for 23 hrs and Stormwatch cube,,,,,, 2011-338T00:00:00,000T07:00:00,4-Dec-11,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2011-338T13:07:00,000T00:02:00,4-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-338T16:49:00,000T09:00:00,4-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-338T17:49:00,000T08:00:00,4-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11338_SP,rider,,,,,, 2011-339T01:49:00,000T08:00:00,5-Dec-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-339T09:49:00,005T02:01:00,5-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-339T16:49:00,000T09:00:00,5-Dec-11,RSS,SPASS Rider,Dione,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev158 Dione gravity observation on 2011/346. DSS-34 required for X- and Ka-band support.",,,,,, 2011-339T16:49:00,000T09:00:00,5-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-339T17:49:00,000T08:00:00,5-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11339_SP,rider,,,,,, 2011-340T00:00:00,000T01:08:00,6-Dec-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-340T01:49:00,000T13:15:00,6-Dec-11,CDA,Prime,DustRAM direction,ISD0038,,CDA ISD 2011-337T03:13:00,ISD observation around apoapse 2011-337T03:13:00 40.537579 Rs,,,,,, 2011-340T16:34:00,000T09:00:00,6-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-340T17:34:00,000T08:00:00,6-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11340_SP,rider,,,,,, 2011-341T01:34:00,000T00:40:00,7-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-341T01:34:00,003T10:16:00,7-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-341T02:12:00,000T00:02:00,7-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-341T02:14:00,000T01:30:00,7-Dec-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 52.7 requested range 3.3 Mkm",,,,,, 2011-341T02:14:00,000T01:30:00,7-Dec-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-341T02:14:00,000T01:30:00,7-Dec-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 53 range =3.3 Mkm.,,,,,, 2011-341T03:42:00,000T00:02:00,7-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-341T03:44:00,000T00:58:00,7-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-341T03:44:00,000T00:58:00,7-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-341T04:40:00,000T00:02:00,7-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-341T04:42:00,000T01:02:00,7-Dec-11,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Dione","Images of mutual event, transit of Rhea across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-341T04:42:00,000T01:02:00,7-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-341T05:42:00,000T00:02:00,7-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-341T20:24:00,000T02:00:00,7-Dec-11,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Titan","Images of mutual event, transit of Dione across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-341T20:24:00,000T02:00:00,7-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-341T22:22:00,000T00:02:00,7-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-341T23:29:00,000T01:10:00,7-Dec-11,ISS,Prime,Tethys,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Tethys across Titan","Images of mutual event, transit of Tethys across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2011-341T23:29:00,000T01:10:00,7-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-342T00:00:00,002T00:00:00,8-Dec-11,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde Hyperion,Retrograde observation around Hyperion - inbound leg,,,,,, 2011-342T00:37:00,000T00:02:00,8-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-342T02:49:00,000T09:00:00,8-Dec-11,RSS,SPASS Rider,Dione,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev158 Dione gravity observation on 2011/346. DSS-55 required for X- and Ka-band support.",,,,,, 2011-342T02:49:00,000T09:00:00,8-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-342T03:49:00,000T08:00:00,8-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11342_SP,rider,,,,,, 2011-342T11:49:00,000T14:40:00,8-Dec-11,CDA,Prime,DustRAM direction,ISD0038,,CDA ISD 2011-337T03:13:00,ISD observation around apoapse 2011-337T03:13:00 40.537579 Rs,,,,,, 2011-343T02:49:00,000T09:00:00,9-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-343T03:49:00,000T08:00:00,9-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11343_SP,rider,,,,,, 2011-343T11:49:00,001T00:01:00,9-Dec-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-343T11:50:45,000T00:38:15,9-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-343T12:27:00,000T00:02:00,9-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-343T12:29:00,000T01:30:00,9-Dec-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 81.7 requested range 2.7 Mkm",,,,,, 2011-343T12:29:00,000T01:30:00,9-Dec-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-343T12:29:00,000T01:30:00,9-Dec-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 82 range =2.7 Mkm. Also a Stormwatch cube,,,,,, 2011-343T13:57:00,000T00:02:00,9-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-343T14:10:00,000T12:00:00,9-Dec-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-343T14:10:00,000T12:00:00,9-Dec-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn CIRS COMPSIT ridealong,Ridealong with CIRS COMPSIT,,,,,, 2011-344T02:08:00,000T00:02:00,10-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-344T02:50:00,000T09:00:00,10-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-344T03:50:00,000T08:00:00,10-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11344_SP,rider,,,,,, 2011-344T11:50:00,001T20:49:22,10-Dec-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-344T11:50:00,000T08:26:01,10-Dec-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-344T11:50:00,001T01:45:00,10-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-344T11:50:00,002T16:15:00,10-Dec-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_158_D3",,,,,, 2011-344T11:50:00,000T10:46:00,10-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-344T12:00:00,000T03:00:00,10-Dec-11,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration,Instance of USTRCAL01 & 02,,,,,, 2011-344T12:00:00,000T03:00:00,10-Dec-11,VIMS,SPASS Rider,Star,SPICACAL,,Spica calibration,Spica calibration,,,,,, 2011-344T19:00:00,000T03:00:00,10-Dec-11,ISS,Prime,Titan,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, Tethys-Rhea-Titan","Images of mutual event, transit of Titan across Tethys follwed by transit of Rhea across Titan",,,,,, 2011-344T19:00:00,000T03:00:00,10-Dec-11,VIMS,SPASS Rider,Titan,MUTUALEV,,Titan high phase,Titan high phase,,,,,, 2011-344T20:16:01,000T23:00:00,10-Dec-11,INMS,Non-SPASS,Dione,DIONERPD,,Dione Ring Plane Observation,Observe neutral molecules in the Dione equatorial plane,,,,,, 2011-344T22:00:00,000T02:00:00,10-Dec-11,ISS,Prime,Titan,M150R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 128 requested range 1.7 Mkm",,,,,, 2011-344T22:00:00,000T01:30:00,10-Dec-11,CIRS,SPASS Rider,Titan,M150R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-344T22:00:00,000T02:00:00,10-Dec-11,VIMS,SPASS Rider,Titan,M150R2HZ,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 128 range =1.7 Mkm.,,,,,, 2011-344T22:36:00,002T06:52:00,10-Dec-11,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-345T01:14:57,002T01:34:00,11-Dec-11,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.994854 Rs exit= 13.997219 Range altitude= 2466.2053 km ... 1591.0476,,,,,, 2011-345T02:35:00,000T09:00:00,11-Dec-11,RSS,SPASS Rider,Dione,KADOWN,RSS Ka-Band downlink,Gravity Science Enhancement (GSE),"Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-55 (or DSS-54) required for X- and Ka-band support.",,,,,, 2011-345T02:35:00,000T09:00:00,11-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-345T03:35:00,000T08:00:00,11-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11345_SP,rider,,,,,, 2011-345T11:35:00,000T10:10:00,11-Dec-11,UVIS,Prime,Saturn,ENAURFOOT,,Search for Enceladus Auroral Footprint,"Slow repeated slews across Saturn's auroral zone, emphasizing Enceladus-related auroras This means slews should cover 55-90 latitude. They should also cover the sub-Enceladus longitude between 60-70 latitude.",,,,,, 2011-345T11:35:00,000T10:10:00,11-Dec-11,VIMS,SPASS Rider,Saturn,ENAURFOOT,,Saturn movie,Saturn movie,,,,,, 2011-345T13:35:00,000T08:10:00,11-Dec-11,MAG,Non-SPASS,Enceladus,ENAURFOOT,,EnAurFoot PIE,MAPS EnAurFoot PIE observation,,,,,, 2011-345T19:15:00,000T02:00:00,11-Dec-11,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2011-345T19:15:57,000T02:00:00,11-Dec-11,CDA,SPASS Rider,DustRAM direction,RPX0280,,CDA RPXing 2011-345T20:15:57,RPXing at 5.2736229 Rs,,,,,, 2011-345T19:16:01,000T00:30:00,11-Dec-11,INMS,Non-SPASS,Dione,DIONERPD,,Dione Ring Plane Observation,Observe neutral molecules in the Dione equatorial plane,,,,,, 2011-345T19:46:01,000T01:30:00,11-Dec-11,INMS,Non-SPASS,Dione,DIONERPD,,Dione Ring Plane Observation,Observe neutral molecules in the Dione equatorial plane,,,,,, 2011-345T21:16:01,000T00:23:21,11-Dec-11,INMS,Non-SPASS,Dione,DIONERPD,,Dione Ring Plane Observation,Observe neutral molecules in the Dione equatorial plane,,,,,, 2011-345T21:39:22,000T10:00:00,11-Dec-11,INMS,Non-SPASS,Dione,D3INBND,,Dione flyby,Dione observation,,,,,, 2011-345T21:45:00,000T03:15:00,11-Dec-11,CDA,Prime,Other,RINGSHAD,,CDA Ring Shadow Crossing1_4Rs,CDA Ring Shadow Crossing @ 4Rs; objective code RC1a,,,,,, 2011-345T21:45:00,000T00:25:00,11-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-345T22:10:00,000T07:50:00,11-Dec-11,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2011-345T23:00:00,000T02:09:22,11-Dec-11,RSS,SPASS Rider,Dione,THERMAL,Thermal stabilization period,RSS thermal stabilization,"A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance. CDA can articulate during warm-up, but not during the science observation.",,,,,, 2011-346T01:09:22,000T03:00:00,12-Dec-11,RSS,SPASS Rider,Dione,GRAVITY,RSS gravity science experiment,RSS Dione' Gravity Field Experiment,Experiment to determine Dione's gravity field,,,,,, 2011-346T02:00:19,000T00:00:01,12-Dec-11,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.241 Rs, lat = -0 deg, phase = 131 deg",,,,,, 2011-346T04:09:22,000T02:30:00,12-Dec-11,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2011-346T04:09:22,000T02:30:00,12-Dec-11,CIRS,,Enceladus,ENCEL,Enceladus,,null,,,,,, 2011-346T04:09:22,000T02:30:00,12-Dec-11,UVIS,,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-346T04:09:22,000T02:30:00,12-Dec-11,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,ENCELADUS,Enceladus,,,,,, 2011-346T06:00:00,000T01:39:22,12-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-346T06:39:22,000T01:30:00,12-Dec-11,CIRS,Prime,Dione,DIONE,Dione,,"Fractures are ~ 210 -> 360 W and 30 S -> 60 N. 06:39 - 7:26 FP3/4 scan @ 6 mu rad/s ~equator to ~ 60 N centered at ~270 W (far enough W to observe the fractures but not so far that we're wasting FP3 off the limb) then from this latitude as far south as we have time for centered at ~300 W (or whereever it needs to be to have the scans close to overlapping) Phase is 137.3 deg 07:26 - 07:40 FP1 raster scan 07:40 - 08:09 Turn, SID suspend likely, okayed by INMS & RSS",,,,,, 2011-346T06:39:22,000T01:30:00,12-Dec-11,ISS,SPASS Rider,Dione,DIONE,Dione,Dione,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-346T06:39:22,000T01:30:00,12-Dec-11,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-346T06:39:22,000T01:30:00,12-Dec-11,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,Dione,,,,,, 2011-346T07:39:22,000T01:30:00,12-Dec-11,INMS,,Dione,DIONE3,,Dione encounter,Dione observation,,,,,, 2011-346T07:39:22,000T04:00:00,12-Dec-11,MAG,Non-SPASS,Dione,DITAR,Dione targeted flyby,Dione targeted flyby,Monitor the interaction of Dione with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2011-346T08:09:22,000T03:00:00,12-Dec-11,RSS,Prime,Dione,GRAVITY,RSS gravity science experiment,RSS Dione' Gravity Field Experiment,Experiment to determine Dione's gravity field,,,,,, 2011-346T08:39:22,000T02:00:00,12-Dec-11,CAPS,SPASS Rider,Titan,DI3CLOSE,,Closest Approach 158DI (3),null,,,,,, 2011-346T08:39:22,000T02:00:00,12-Dec-11,RPWS,Non-SPASS,Dione,DICA,,RPWS Dione closest approach observations,"Make high resolution RPWS observations of the magnetosphere - Dione interaction using WBR, WFR, and LP.",,,,,, 2011-346T09:09:22,000T02:30:00,12-Dec-11,INMS,,Dione,DIONE3,,Dione encounter,Dione observation,,,,,, 2011-346T09:09:22,000T01:00:00,12-Dec-11,MIMI,Non-SPASS,Dione,ENCNTROV,,MIMI Dione 158,BIT_OVERLAY_950,,,,,, 2011-346T10:09:57,000T02:00:00,12-Dec-11,CDA,SPASS Rider,DustRAM direction,RPX0290,,CDA RPXing 2011-346T11:09:57,RPXing at 7.0102459 Rs,,,,,, 2011-346T10:39:22,000T17:25:38,12-Dec-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-346T11:09:22,000T03:30:00,12-Dec-11,ISS,Prime,Dione,REGMAP,Regional mapping,Dione regional mapping,ISS mosaic plus CIRS scan plus VIMS sit'n'stare,,,,,, 2011-346T11:09:22,000T03:30:00,12-Dec-11,CIRS,SPASS Rider,Dione,REGMAP,Regional mapping,,null,,,,,, 2011-346T11:09:22,000T03:30:00,12-Dec-11,UVIS,,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2011-346T11:09:22,000T03:30:00,12-Dec-11,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,Dione,,,,,, 2011-346T11:39:22,000T10:00:00,12-Dec-11,INMS,Non-SPASS,Dione,D3OUTBND,,Dione flyby,Dione observation,,,,,, 2011-346T11:39:22,000T16:25:38,12-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-346T14:39:22,000T03:00:00,12-Dec-11,RSS,SPASS Rider,Dione,GRAVITY,RSS gravity science experiment,RSS Dione' Gravity Field Experiment,Experiment to determine Dione's gravity field,,,,,, 2011-346T15:20:00,000T11:15:00,12-Dec-11,RSS,SPASS Rider,Dione,KADOWN,RSS Ka-Band downlink,Gravity Science Enhancement (GSE),"Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-34 required for X- and Ka-band support.",,,,,, 2011-346T17:40:00,000T08:55:00,12-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-346T18:25:00,000T08:10:00,12-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11346_SP,rider,,,,,, 2011-346T21:39:22,000T06:25:38,12-Dec-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-347T02:48:57,010T16:25:03,13-Dec-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.010039 Rs exit= 14.010615 Range altitude= 1594.0656 km ... -7510.6888,,,,,, 2011-347T04:05:00,000T00:55:00,13-Dec-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-347T04:05:00,000T04:06:24,13-Dec-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-347T04:05:00,000T12:06:24,13-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-347T04:05:00,003T07:15:00,13-Dec-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_158_T79",,,,,, 2011-347T04:20:00,001T00:11:24,13-Dec-11,CAPS,Prime,Titan,T79PTG,,Titan Encounter,null,,,,,, 2011-347T04:20:00,000T06:51:24,13-Dec-11,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2011-347T04:20:00,001T00:11:24,13-Dec-11,CIRS,SPASS Rider,Titan,T79PTG,,,Rider along with CAPS flyby.,,,,,, 2011-347T04:20:00,000T06:51:24,13-Dec-11,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T04:20:00,000T06:51:24,13-Dec-11,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,Rider to CIRS NADCMP,Rider to CIRS.,,,,,, 2011-347T05:00:00,000T14:11:24,13-Dec-11,CAPS,SPASS Rider,Titan,T79INBND,,Inbound 158TI (T79),null,,,,,, 2011-347T05:28:00,001T20:52:00,13-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-347T08:11:24,000T11:00:00,13-Dec-11,INMS,Non-SPASS,Titan,T79INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-347T11:11:24,000T04:00:00,13-Dec-11,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,"Obtain vertical profiles of temperature and abundances of trace gases in Titan's stratosphere. The arrays are positioned on the limb (-/+ Z perp to limb) at two altitudes, about 100 km and 350 km at center.",,,,,, 2011-347T11:11:24,000T04:00:00,13-Dec-11,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T11:11:24,000T04:00:00,13-Dec-11,UVIS,Non-SPASS,Titan,MIRLMBINT,Mid infrared limb integration,Rider to CIRS NADCMP,Rider to CIRS.,,,,,, 2011-347T12:11:24,000T07:00:00,13-Dec-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-347T15:11:24,000T02:45:00,13-Dec-11,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2011-347T15:11:24,000T02:45:00,13-Dec-11,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T15:11:24,000T02:45:00,13-Dec-11,UVIS,Non-SPASS,Titan,FIRNADMAP,Far infrared nadir composition map,Rider to CIRS,Rider to CIRS.,,,,,, 2011-347T16:11:24,000T08:00:00,13-Dec-11,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T79 flyby,"T79 is a noon, equatorial, upstream flyby. Although the CA altitude is above the upper boundary of the induced magnetosphere, observations indicate that MAG could cross it under low ambient upstream pressure period. We assign grade two priority. Data rate: 988bps (16vps).",,,,,, 2011-347T17:56:24,000T01:00:00,13-Dec-11,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2011-347T17:56:24,000T01:00:00,13-Dec-11,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T17:56:24,000T01:00:00,13-Dec-11,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2011-347T18:11:24,000T01:00:00,13-Dec-11,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-347T18:11:24,000T01:00:00,13-Dec-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-347T18:56:24,000T00:30:00,13-Dec-11,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2011-347T18:56:24,000T00:30:00,13-Dec-11,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T19:11:24,000T02:00:00,13-Dec-11,CAPS,SPASS Rider,Titan,T79CLOSE,,Closest Approach 158TI (T79),null,,,,,, 2011-347T19:11:24,000T02:00:00,13-Dec-11,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-347T19:11:24,000T02:00:00,13-Dec-11,INMS,Non-SPASS,Titan,TITAN79,,Titan Flyby,Titan observation,,,,,, 2011-347T19:11:24,000T02:00:00,13-Dec-11,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2011-347T19:26:24,000T00:45:00,13-Dec-11,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2011-347T19:26:24,000T00:45:00,13-Dec-11,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T20:11:24,000T08:20:00,13-Dec-11,VIMS,Prime,Titan,CLOSAPP,,Scan and Mosaics,VIMS scan of Belet where ISS saw variations - then mosaics of Belet and Adiri - then global mosaics,,,,,, 2011-347T20:11:24,000T14:00:00,13-Dec-11,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,ISS rider Titan low phase,Rider to VIMS Titan cloud monitor,,,,,, 2011-347T20:11:24,000T08:20:00,13-Dec-11,ISS,SPASS Rider,Titan,CLOSAPP,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-347T21:11:24,000T08:00:00,13-Dec-11,CAPS,SPASS Rider,Titan,T79OUTBND,,Outbound 158TI (T79),null,,,,,, 2011-347T21:11:24,000T01:00:00,13-Dec-11,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2011-347T21:11:24,000T11:00:00,13-Dec-11,INMS,Non-SPASS,Titan,T79OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-347T21:11:24,000T06:00:00,13-Dec-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-347T21:11:24,000T01:00:00,13-Dec-11,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2011-348T00:11:24,002T11:08:36,14-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-348T05:11:24,000T05:00:00,14-Dec-11,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,GLObal mapping of Titan.,"VIMS global mapping of Titan. Phase = 17 deg. SSC Lat/Lon = 0.511S/208.593 deg, SS Lat/Lon = 12.356N/197.195 deg. Alt = 177252.995 and range = 179827.995 km. Resolution = 89 km/px. Temp. V. Obtain cubes of 160 and 640 msec for global mapping of Titan.",,,,,, 2011-348T05:11:24,000T05:00:00,14-Dec-11,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,ISS rider Titan low phase,Rider to VIMS Titan cloud monitor,,,,,, 2011-348T05:11:24,000T05:00:00,14-Dec-11,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-348T05:11:24,002T06:08:36,14-Dec-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-348T08:11:24,002T03:08:36,14-Dec-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-348T10:11:24,000T02:28:36,14-Dec-11,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template A4: No ISS dwells.,,,,,, 2011-348T10:11:24,000T02:28:36,14-Dec-11,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-348T10:11:24,000T02:28:36,14-Dec-11,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 16 deg. SSC Lat/Lon = 0.603S/212.230 deg, SS Lat/Lon = 12.358N/201.896 deg. Alt = 278235.240 and range = 280810.240 km. Resolution = 139 km/px. Temp. A. Obtain cubes while scanning across Titan.",,,,,, 2011-348T15:05:00,000T11:30:00,14-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-348T16:05:00,000T10:30:00,14-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11348_SP,rider,,,,,, 2011-349T02:20:00,001T09:00:00,15-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-349T03:15:00,000T03:00:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T03:15:00,000T03:00:00,15-Dec-11,CIRS,,Titan,CLOUD,,,null,,,,,, 2011-349T03:15:00,000T03:00:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 15, SSC Lat/Lon = 0.670S/225.504 deg, SS Lat/Lon = 12.366N/217.956 deg. Alt = 636422.0 km, range = 638997.0 km. Resolution = 318 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-349T06:15:00,000T03:00:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T06:15:00,000T03:00:00,15-Dec-11,CIRS,,Titan,CLOUD,,,null,,,,,, 2011-349T06:15:00,000T03:00:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 15 deg, SSC Lat/Lon = 0.671S/227 deg, SS Lat/Lon = 12N/220 deg. Alt = 710563 km, range = 704138 km. Resolution = 351 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-349T09:15:00,000T03:00:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T09:15:00,000T03:00:00,15-Dec-11,CIRS,,Titan,CLOUD,,,,,,,,, 2011-349T09:15:00,000T03:00:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 15 deg, SSC Lat/Lon = 0.670S/230 deg, SS Lat/Lon = 12N/223 deg. Alt = 769175 km, range = 771750 km. Resolution = 385 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-349T12:15:00,000T03:00:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T12:15:00,000T03:00:00,15-Dec-11,CIRS,,Titan,CLOUD,,,,,,,,, 2011-349T12:15:00,000T03:00:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 14 deg, SSC Lat/Lon = 0.67S/232 deg, SS Lat/Lon = 12N/226 deg. Alt = 833721 km, range = 836296 km. Resolution = 417 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-349T15:15:00,000T03:00:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T15:15:00,000T03:00:00,15-Dec-11,CIRS,,Titan,CLOUD,,,,,,,,, 2011-349T15:15:00,000T03:00:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 14 deg, SSC Lat/Lon = 0.67S/234 deg, SS Lat/Lon = 12N/229 deg. Alt = 898806 km, range = 901381 km. Resolution = 449 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-349T18:15:00,000T03:00:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T18:15:00,000T03:00:00,15-Dec-11,CIRS,,Titan,CLOUD,,,,,,,,, 2011-349T18:15:00,000T03:00:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 14 deg, SSC Lat/Lon = 0.66S/237 deg, SS Lat/Lon = 12N/232 deg. Alt = 968156 km, range = 970731 km. Resolution = 484 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-349T18:15:00,000T03:00:00,15-Dec-11,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2011-349T18:16:20,000T00:00:01,15-Dec-11,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2011-349T21:15:00,000T02:00:00,15-Dec-11,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2011-349T23:15:00,000T00:55:00,15-Dec-11,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2011-349T23:15:00,000T00:55:00,15-Dec-11,CIRS,,Titan,CLOUD,,,,,,,,, 2011-349T23:17:54,000T00:55:00,15-Dec-11,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Titan Cloud monitoring,"VIMS ridealong with ISS for cloud monitoring. Phase = 14 deg, SSC Lat/Lon = 0.66S/240 deg, SS Lat/Lon = 12N/236 deg. Alt = 1077884 km, range = 1080459 km. Resolution = 539 km/px. Obtain 160 and 640 ms cubes for cloud mapping during caboose segment.",,,,,, 2011-350T02:20:00,000T09:00:00,16-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-350T03:20:00,000T08:00:00,16-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11350_SP,rider,,,,,, 2011-350T11:20:00,000T15:00:00,16-Dec-11,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2011-350T11:20:00,000T15:00:00,16-Dec-11,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2011-350T11:20:00,000T15:00:00,16-Dec-11,VIMS,SPASS Rider,Titan,TEA,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase =?? range =?? Mkm - one cube per hour.,,,,,, 2011-350T11:20:00,016T13:02:00,16-Dec-11,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2011-350T11:20:00,001T00:00:00,16-Dec-11,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-350T11:20:00,006T23:01:00,16-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-350T11:20:00,007T07:54:00,16-Dec-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_158_159",,,,,, 2011-350T11:20:00,007T07:54:00,16-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-351T02:20:00,000T09:00:00,17-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-351T03:20:00,000T08:00:00,17-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11351_SP,rider,,,,,, 2011-351T11:20:00,000T15:01:00,17-Dec-11,CDA,Prime,DustRAM direction,RETROGRAD,,CDA Retrograde Apo,Retrograde observation outbound leg,,,,,, 2011-351T11:20:00,001T00:01:00,17-Dec-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-352T02:21:00,000T09:00:00,18-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-352T03:21:00,000T08:00:00,18-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11352_SP,rider,,,,,, 2011-352T11:21:00,000T13:30:00,18-Dec-11,CDA,Prime,DustRAM direction,ISD0039,,CDA ISD 2011-357T19:14:00,ISD observation around apoapse 2011-357T19:14:00 48.172998 Rs,,,,,, 2011-352T11:21:00,004T13:30:00,18-Dec-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-353T02:21:00,000T09:00:00,19-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-353T03:21:00,000T08:00:00,19-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11353_SP,rider,,,,,, 2011-353T11:21:00,000T13:15:00,19-Dec-11,CDA,Prime,DustRAM direction,ISD0039,,CDA ISD 2011-357T19:14:00,ISD observation around apoapse 2011-357T19:14:00 48.172998 Rs,,,,,, 2011-354T00:36:00,000T06:00:00,20-Dec-11,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2011-354T02:06:00,000T09:00:00,20-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-354T03:06:00,000T08:00:00,20-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11354_SP,rider,,,,,, 2011-354T11:06:00,000T00:54:00,20-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-354T11:58:00,000T00:02:00,20-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-354T12:00:00,000T01:00:00,20-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-354T12:00:00,000T01:00:00,20-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-354T12:58:00,000T00:02:00,20-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-354T15:00:00,000T16:00:00,20-Dec-11,UVIS,Prime,Saturn,MOS158APO,,,"System scan of Saturn magnetosphere hydrogen, day 1. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances made for 20 minutes observation margin at start and end, and 30 minutes for turn to waypoint at end. Align slit with Saturn spin axis. Slew -32 mrad about x-axis. Start data capture, stare 808.0 s, stop data capture. Repeat PATTERN 59 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 808.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1498.52539 bps, from Alain's spreadsheet)x(808.0s per stare)x(60 stares) = 72.65x10^6 bits. Multiplier includes adjustment factor of 1.01 for data packet filling issues.",,,,,, 2011-354T15:00:00,000T16:00:00,20-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-355T00:00:00,000T01:08:00,21-Dec-11,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2011-355T06:58:00,000T00:02:00,21-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-355T09:36:00,000T09:00:00,21-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-355T10:36:00,000T08:00:00,21-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11355_SP,rider,,,,,, 2011-355T18:36:00,000T00:40:00,21-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-355T19:14:00,000T00:02:00,21-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-355T19:16:00,000T01:30:00,21-Dec-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 40.3 requested range 3.8 Mkm",,,,,, 2011-355T19:16:00,000T01:30:00,21-Dec-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-355T19:16:00,000T01:30:00,21-Dec-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 40 range =3.8 Mkm. Also Stormwatch Cube,,,,,, 2011-355T20:44:00,000T00:02:00,21-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-355T20:46:00,000T01:00:00,21-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-355T20:46:00,000T01:00:00,21-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-355T21:44:00,000T00:02:00,21-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-355T23:00:00,000T16:00:00,21-Dec-11,UVIS,Prime,Saturn,MOS158APO,,,"System scan of Saturn magnetosphere hydrogen, day 2. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances made for 20 minutes observation margin at start and end, and 30 minutes for turn to waypoint at end. Align slit with Saturn spin axis. Slew -32 mrad about x-axis. Start data capture, stare 853.0 s, stop data capture. Repeat PATTERN 56 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 853.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1419.47071 bps, from Alain's spreadsheet)x(853.0s per stare)x(57 stares) = 69.02x10^6 bits. Multiplier includes adjustment factor of 1.01 for data packet filling issues.",,,,,, 2011-355T23:00:00,000T16:00:00,21-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-356T14:58:00,000T00:02:00,22-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-356T15:51:00,000T09:00:00,22-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-356T16:51:00,000T08:00:00,22-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11356_SP,rider,,,,,, 2011-357T00:51:00,000T15:00:00,23-Dec-11,ISS,Prime,Other,SUTROT,,Suttungr,Observation of irregular moon of Saturn.,,,,,, 2011-357T00:51:00,000T18:23:00,23-Dec-11,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-357T10:21:00,000T05:00:00,23-Dec-11,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2011-357T15:21:00,002T09:55:00,23-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-357T15:51:00,000T09:00:00,23-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-357T16:51:00,000T08:00:00,23-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_158IC_DSCAL11357_SP,rider,,,,,, 2011-357T19:14:00,010T16:08:57,23-Dec-11,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.010039 Rs exit= 14.010615 Range altitude= 1594.0656 km ... -7510.6888,,,,,, 2011-357T19:14:00,000T05:37:00,23-Dec-11,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-357T19:14:00,009T05:08:00,23-Dec-11,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_158_159",,,,,, 2011-357T19:14:00,009T05:08:00,23-Dec-11,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2011-357T19:14:07,000T00:00:01,23-Dec-11,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 23.5 d, inc = 0.9 deg, r = 48.124 Rs, phase = 58 deg",,,,,, 2011-358T00:51:00,000T00:09:00,24-Dec-11,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2011-358T00:52:45,000T01:37:15,24-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-358T01:00:00,000T02:00:00,24-Dec-11,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2011-358T02:28:00,000T00:02:00,24-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-358T02:30:00,000T01:00:00,24-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-358T02:30:00,000T01:00:00,24-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-358T03:00:00,008T21:22:00,24-Dec-11,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2011-358T03:28:00,000T00:02:00,24-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-358T03:30:00,001T08:00:00,24-Dec-11,UVIS,Prime,Saturn,MOS158APO,,,"System scan of Saturn magnetosphere hydrogen, day 3. EUV and FUV low resolution slits on. Note: data to be taken only when slit is stationary. Allowances made for 20 minutes observation margin at start and end, and 30 minutes for turn to waypoint at end. Align slit with Saturn spin axis. Slew +32 mrad about x-axis and -167 mrad about z-axis. Start data capture, stare 922.0 s, stop data capture. Repeat PATTERN 111 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 922.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1313.24134 bps, from Alain's spreadsheet)x(922.0s per stare)x(112 stares) = 135.611x10^6 bits. Multiplier includes adjustment factor of 1.01 for data packet filling issues.",,,,,, 2011-358T03:30:00,001T08:00:00,24-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-359T11:28:00,000T00:02:00,25-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-359T11:30:00,000T01:30:00,25-Dec-11,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 58.3 requested range 4.1 Mkm",,,,,, 2011-359T11:30:00,000T01:30:00,25-Dec-11,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-359T11:30:00,000T01:30:00,25-Dec-11,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 58 range =4.1Mkm. Also Stormwatch cube.,,,,,, 2011-359T12:58:00,000T00:02:00,25-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-359T15:36:00,000T09:00:00,25-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-359T16:36:00,000T08:00:00,25-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_159IC_DSCAL11359_SP,rider,,,,,, 2011-359T23:14:00,000T20:00:00,25-Dec-11,CDA,SPASS Rider,DustRAM direction,ISD0039,,CDA ISD 2011-357T19:14:00,ISD observation around apoapse 2011-357T19:14:00 48.172998 Rs,,,,,, 2011-360T00:36:00,000T00:40:00,26-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-360T01:14:00,000T00:02:00,26-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-360T01:16:00,000T07:00:00,26-Dec-11,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2011-360T01:16:00,000T07:00:00,26-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-360T08:14:00,000T00:02:00,26-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-360T08:16:00,000T01:30:00,26-Dec-11,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 74.7 requested range 3.8 Mkm",,,,,, 2011-360T08:16:00,000T01:30:00,26-Dec-11,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-360T08:16:00,000T01:30:00,26-Dec-11,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 75 range =3.8 Mkm. Also Stormwatch cube,,,,,, 2011-360T08:16:00,006T16:06:00,26-Dec-11,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2011-360T09:44:00,000T00:02:00,26-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-360T09:46:00,000T01:00:00,26-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-360T09:46:00,000T01:00:00,26-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-360T10:44:00,000T00:02:00,26-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-360T10:46:00,000T23:00:00,26-Dec-11,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2011-360T10:46:00,000T23:00:00,26-Dec-11,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ride-along,MIRMAP ridelong with CIRS. Also Stormwatch Cube,,,,,, 2011-361T09:44:00,000T00:02:00,27-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-361T15:37:00,000T09:00:00,27-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-361T16:37:00,000T08:00:00,27-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_159IC_DSCAL11361_SP,rider,,,,,, 2011-362T00:00:00,002T00:00:00,28-Dec-11,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde APO,Retrograde observation inbound leg,,,,,, 2011-362T00:37:00,001T13:15:00,28-Dec-11,CDA,Prime,DustRAM direction,ISD0039,,CDA ISD 2011-357T19:14:00,ISD observation around apoapse 2011-357T19:14:00 48.172998 Rs,,,,,, 2011-363T15:22:00,000T09:00:00,29-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-363T16:22:00,000T08:00:00,29-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_159IC_DSCAL11363_SP,rider,,,,,, 2011-364T07:20:00,000T00:40:00,30-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-364T07:58:00,000T00:02:00,30-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-364T08:30:00,000T01:30:00,30-Dec-11,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 105.5 requested range 1.9 Mkm",,,,,, 2011-364T08:30:00,000T01:30:00,30-Dec-11,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2011-364T08:30:00,000T01:30:00,30-Dec-11,VIMS,SPASS Rider,Titan,M120R2HZ,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 106 range =1.9 Mkm. Also Stormwatch cube,,,,,, 2011-364T09:58:00,000T00:02:00,30-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-364T10:00:00,000T00:56:00,30-Dec-11,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 004 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2011-364T10:00:00,000T00:56:00,30-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-364T10:54:00,000T00:02:00,30-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-364T12:26:00,000T12:34:00,30-Dec-11,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2011-364T12:26:00,000T12:34:00,30-Dec-11,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2011-365T00:58:00,000T00:02:00,31-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-365T01:00:00,000T12:00:00,31-Dec-11,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2011-365T01:00:00,000T12:00:00,31-Dec-11,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn CIRS COMPSIT ridealong,Ridealong with CIRS COMPSIT. Also Stormwatch Cube,,,,,, 2011-365T12:58:00,000T00:02:00,31-Dec-11,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2011-365T15:22:00,000T09:00:00,31-Dec-11,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2011-365T16:22:00,000T08:00:00,31-Dec-11,CIRS,SPASS Rider,InstrumentCalibration,DSCAL11,,CIRS_159IC_DSCAL11365_SP,rider,,,,,, 2012-001T00:22:00,000T00:43:00,1-Jan-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-001T01:03:00,000T00:02:00,1-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-001T01:05:00,000T01:00:00,1-Jan-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 15","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-001T01:05:00,000T01:00:00,1-Jan-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-001T02:03:00,000T00:02:00,1-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-001T02:05:00,000T11:00:00,1-Jan-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-001T02:05:00,000T11:00:00,1-Jan-12,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2012-001T02:05:00,000T11:00:00,1-Jan-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong and Stormwatch cube,,,,,, 2012-001T13:03:00,000T00:02:00,1-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-001T15:22:00,000T09:00:00,1-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-001T16:22:00,000T08:00:00,1-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12001_SP,rider,,,,,, 2012-002T00:22:00,000T12:51:37,2-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-002T00:22:00,000T02:51:37,2-Jan-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-002T00:22:00,000T10:51:37,2-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-002T00:22:00,001T18:01:00,2-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_159_T80",,,,,, 2012-002T00:22:00,001T08:21:00,2-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-002T01:16:59,000T04:56:38,2-Jan-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-002T01:16:59,000T04:56:38,2-Jan-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-002T01:16:59,000T00:56:38,2-Jan-12,VIMS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,Stare at Titan.,"VIMS ridealong with CIRS while staring at Titan. Phase = 117.8 deg, SSC Lat/Lon = 6.714S/144.932 deg, SS Lat/Lon = 12.590N/261.968 deg. Alt =275675.692 km, range = 278250.692 km. Resolution = 137 km/px. Temp. M4. Obtain cubes while staring at Titan.",,,,,, 2012-002T01:16:59,000T04:56:38,2-Jan-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-002T02:13:37,000T04:00:00,2-Jan-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS while staring at Titan. Phase = 118 deg, SSC Lat/Lon = 7.130S/145.975 deg, SS Lat/Lon = 12.590N/262.829 deg. Alt =257297.6 km, range = 259872.6 km. Resolution = 129 km/px. Temp. N1. Obtain cubes of 160 and 640 msec.",,,,,, 2012-002T03:13:37,000T11:00:00,2-Jan-12,INMS,Non-SPASS,Titan,T80INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-002T06:13:37,000T04:00:00,2-Jan-12,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2012-002T06:13:37,000T04:00:00,2-Jan-12,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-002T06:13:37,000T04:00:00,2-Jan-12,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Stare at Titan.,"VIMS ridealong with CIRS for Titan limb mapping. Phase = 117 deg, SSC Lat/Lon = 9.890S/151.142 deg, SS Lat/Lon = 12.591N/266.587 deg. Alt =178040.4 km, range = 180615.4 km. Resolution = 89 km/px. Temp. R. Obtain cubes of Titan's limb.",,,,,, 2012-002T10:13:37,000T02:45:00,2-Jan-12,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2012-002T10:13:37,000T02:30:00,2-Jan-12,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-002T10:13:37,000T02:45:00,2-Jan-12,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 114 deg, SSC Lat/Lon = 16.662S/158.933 deg, SS Lat/Lon = 12.593N/270.344 deg. Alt =100963.1 km, range = 103538.1 km. Resolution = 50 km/px. Temp. T. Obtain cubes while scanning across Titan.",,,,,, 2012-002T11:13:37,000T08:00:00,2-Jan-12,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T80 flyby,T80 is a flyby at extremely high altitude over the south pole. It is highly unlikely that MAG will detect any signs of Titan's induced magnetosphere. We assign grade two priority. Data rate: 988bps (16vps).,,,,,, 2012-002T12:43:37,000T04:45:00,2-Jan-12,RADAR,Non-SPASS,Titan,T80WARMUP,,Warmup for T80 iRAD,,,,,,, 2012-002T12:58:37,000T04:30:00,2-Jan-12,ISS,Prime,Titan,HIGHRES,High resolution observartion,HRM (High Resolution Mosaic),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-002T12:58:37,000T04:30:00,2-Jan-12,CIRS,SPASS Rider,Titan,HIGHRES,High resolution observartion,,Ride along with ISS.,,,,,, 2012-002T12:58:37,000T04:30:00,2-Jan-12,VIMS,,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,"VIMS ridealong with ISS for regional mapping during C/A. At C/A, phase = 75.9 deg, SSC Lat/Lon = 59.9S/247.171 deg, SS Lat/Lon = 12.595N/275.041 deg. Alt =29415.9 km, range = 31990.9 km. Resolution = 14.7 km/px. Obtain mosaics and cubes for regional mapping of Titan during C/A.",,,,,, 2012-002T12:58:37,000T04:30:00,2-Jan-12,UVIS,Non-SPASS,Titan,HIRES,High resolution image,HDAC and FUV and EUV on Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-002T13:13:37,000T01:30:00,2-Jan-12,CAPS,SPASS Rider,Titan,T80INBND,,Inbound 159TI (T80),null,,,,,, 2012-002T13:13:37,000T01:00:00,2-Jan-12,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-002T13:13:37,000T01:10:00,2-Jan-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-002T14:13:37,000T02:00:00,2-Jan-12,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-002T14:13:37,000T02:00:00,2-Jan-12,INMS,Non-SPASS,Titan,TITAN80,,Titan Flyby,Titan observation,,,,,, 2012-002T14:23:38,000T01:40:00,2-Jan-12,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2012-002T14:43:37,000T01:00:00,2-Jan-12,CAPS,SPASS Rider,Titan,T80CLOSE,,Closest Approach 159TI (T80),null,,,,,, 2012-002T15:43:37,000T01:30:00,2-Jan-12,CAPS,SPASS Rider,Titan,T80OUTBND,,Outbound 159TI (T80),null,,,,,, 2012-002T16:03:38,000T01:09:59,2-Jan-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-002T16:13:37,000T01:00:00,2-Jan-12,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-002T16:13:37,000T11:00:00,2-Jan-12,INMS,Non-SPASS,Titan,T80OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-002T17:13:37,001T01:09:22,2-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-002T17:28:37,000T02:45:00,2-Jan-12,RADAR,Prime,Titan,T80OUTRAD,,T80 Outbound Radiometry,,,,,,, 2012-002T19:13:37,000T23:09:23,2-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-002T20:13:37,000T04:00:00,2-Jan-12,VIMS,Prime,Titan,STELLOCC,,Stellar Occ.,"Titan stellar occs of CW Leo (RA/Dec = 146.9862/13.2786) at +05:31 to +05:56 and R Leo (146.8892/11.4286) at +06:15 to +06:34. Phase = 56 deg, SSC Lat/Lon = 13.606S/330.293 deg, SS Lat/Lon = 12.597N/279.738 deg. Alt =100868.74 km, range = 103443.74 km. Resolution = 50 km/px.",,,,,, 2012-002T20:13:37,000T04:00:00,2-Jan-12,CIRS,SPASS Rider,Titan,STELLOCC,,,Ride along with VIMS.,,,,,, 2012-002T20:13:37,000T04:00:00,2-Jan-12,ISS,SPASS Rider,Titan,STELLOCC,,VIMS Occs Riders,Point and stare; cycle camera commands.,,,,,, 2012-003T00:13:37,000T05:44:22,3-Jan-12,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan.,"VIMS global mapping of Titan. Phase = 58 deg, SSC Lat/Lon = 6.80S/338.277 deg, SS Lat/Lon = 12.598N/283.495 deg. Alt =177958.175 km, range = 180533.175 km. Resolution = 89 km/px. Obtain 160 and 640 msec cubes for global mapping of Titan.",,,,,, 2012-003T00:13:37,000T05:44:22,3-Jan-12,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2012-003T00:13:37,000T05:44:22,3-Jan-12,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-003T03:13:37,000T15:09:22,3-Jan-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-003T08:23:00,000T10:00:00,3-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-003T08:43:00,000T09:40:00,3-Jan-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-003T09:23:00,000T09:00:00,3-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12003_SP,rider,,,,,, 2012-003T11:22:57,000T07:00:03,3-Jan-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997969 Rs exit= 13.989544 Range altitude= -7488.2246 km ... -15158.577,,,,,, 2012-003T18:23:00,000T18:22:00,3-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-003T18:23:00,000T01:40:57,3-Jan-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997969 Rs exit= 13.989544 Range altitude= -7488.2246 km ... -15158.577,,,,,, 2012-003T18:23:00,000T03:27:12,3-Jan-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-003T18:23:00,001T20:45:00,3-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-003T18:23:00,012T21:24:00,3-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_159_160",,,,,, 2012-003T18:23:00,002T05:45:00,3-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 350 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2012-003T18:23:00,001T22:59:00,3-Jan-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-003T20:03:57,000T04:00:00,3-Jan-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997969 Rs exit= 13.989544 Range altitude= -7488.2246 km ... -15158.577,,,,,, 2012-003T21:03:57,000T02:00:00,3-Jan-12,CDA,SPASS Rider,DustRAM direction,RPX0300,,CDA RPXing 2012-003T22:03:57,RPXing at 9.6843061 Rs,,,,,, 2012-003T21:04:00,000T02:00:00,3-Jan-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-003T21:50:12,000T23:00:00,3-Jan-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-004T00:00:00,000T03:00:00,4-Jan-12,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2012-004T00:00:00,000T03:00:00,4-Jan-12,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2012-004T00:00:00,000T03:00:00,4-Jan-12,CIRS,Non-SPASS,Enceladus,PLMHPMR,Observe Enceladus' plumes,,null,,,,,, 2012-004T00:03:57,000T19:48:00,4-Jan-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997969 Rs exit= 13.989544 Range altitude= -7488.2246 km ... -15158.577,,,,,, 2012-004T05:00:00,000T12:00:00,4-Jan-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-004T06:30:00,000T07:30:00,4-Jan-12,CIRS,Prime,Saturn,LIMBMAP,Limb map,CIRS_159SA_LIMBMAP001,"obtain stratospheric thermal structure by means of limb sounding in the mid-IR, longitude coverage. POINTING: -y to Saturn, z to limb Within +/- 45 degrees latitude",,,,,, 2012-004T06:30:00,000T03:30:00,4-Jan-12,VIMS,SPASS Rider,Saturn,LIMBMAP,Limb map,Saturn CIRS LIMBMAP ridealong,CIRS LIMBMAPMAP Ridealong for 3.5 hrs,,,,,, 2012-004T10:00:00,000T01:20:00,4-Jan-12,VIMS,,Saturn,GAMERIOCC,,gam Eri occultation,gam Eri occultation; use tau_IR of 80 msec,,,,,, 2012-004T11:20:00,000T02:40:00,4-Jan-12,VIMS,SPASS Rider,Saturn,LIMBMAP,Limb map,Saturn CIRS LIMBMAP ridealong,CIRS LIMBMAPMAP Ridealong for 2.7 hrs,,,,,, 2012-004T12:45:00,003T11:08:00,4-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-004T13:02:30,000T00:00:01,4-Jan-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.419 Rs, lat = 2 deg, phase = 123 deg",,,,,, 2012-004T14:06:00,000T02:34:00,4-Jan-12,UVIS,Prime,Star,URIOTORI,,URSTAR,,,,,,, 2012-004T16:40:00,000T11:00:00,4-Jan-12,VIMS,Prime,Saturn,HIRESMAP,High resolution map,Saturn Hi Res Regional Map of Northern Mid-latitud,"Large, single-tier, high-spatial resolution mosaic built up by just repeatedly imaging the sub-spacecraft longitude centered at 35 degrees North Latitude. 7 mins for science. Image acquisition repeated at 10 minute intervals for 11 hours.",,,,,, 2012-004T19:51:57,000T04:00:00,4-Jan-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997969 Rs exit= 13.989544 Range altitude= -7488.2246 km ... -15158.577,,,,,, 2012-004T20:50:00,000T02:00:00,4-Jan-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-004T20:50:12,000T02:00:00,4-Jan-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-004T20:51:57,000T02:00:00,4-Jan-12,CDA,SPASS Rider,DustRAM direction,RPX0310,,CDA RPXing 2012-004T21:51:57,RPXing at 6.9705853 Rs,,,,,, 2012-004T22:50:12,000T23:00:00,4-Jan-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-004T23:51:57,000T14:49:00,4-Jan-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997969 Rs exit= 13.989544 Range altitude= -7488.2246 km ... -15158.577,,,,,, 2012-005T03:00:00,000T09:58:00,5-Jan-12,CIRS,SPASS Rider,Saturn,EMASCAN,,Center to Limb study,,,,,,, 2012-005T03:40:00,000T09:18:00,5-Jan-12,ISS,Prime,Saturn,EMASCAN,,Saturn Emission Angle Scan,"For each latitude image at a low emission angle, medium emission angle and high emission angle as the planet rotates. Move to other latitudes as time and data volume permit. Collaborative with VIMS.",,,,,, 2012-005T03:40:00,000T09:18:00,5-Jan-12,VIMS,SPASS Rider,Saturn,EMASCAN,,Saturn ISS center-to-limb imaging ridealong,CIRS EMASCAN center-to-limb Ridealong. Three images per hour for ~ 9 hrs,,,,,, 2012-005T14:40:57,000T22:19:03,5-Jan-12,CDA,Non-SPASS,Other,RATE010A,,Data rate End:SApo,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-005T15:08:00,000T02:30:00,5-Jan-12,CDA,Non-SPASS,Other,RATE010B,,Data rate End:SApo,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-005T15:08:00,002T08:45:00,5-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-005T15:08:00,000T09:00:00,5-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-005T16:08:00,000T08:00:00,5-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12005_SP,rider,,,,,, 2012-005T17:22:00,010T22:25:00,5-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-005T21:50:12,000T09:24:48,5-Jan-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-006T00:46:00,000T00:02:00,6-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-006T00:48:00,000T08:00:00,6-Jan-12,ISS,Prime,Other,YMIPHA,,Ymir,Observation of irregular moon of Saturn.,,,,,, 2012-006T00:48:00,000T08:00:00,6-Jan-12,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2012-006T02:00:00,000T01:08:00,6-Jan-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-006T07:15:00,010T02:24:00,6-Jan-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-006T08:46:00,000T00:02:00,6-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-006T08:48:00,000T13:00:00,6-Jan-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-006T08:48:00,000T13:00:00,6-Jan-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-006T10:00:00,000T01:28:00,6-Jan-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-006T13:00:00,010T02:47:00,6-Jan-12,CDA,Non-SPASS,Other,RATE010B,,Data rate End:SApo,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-006T21:46:00,000T00:02:00,6-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-006T21:48:00,000T10:00:00,6-Jan-12,VIMS,Prime,Saturn,REGMAP,Regional mapping,Saturn Hi Res Regional Map of Northern Mid-latitud,"2*3 mosaic (2 rows of 3 frames)centrered at 40 degrees North Latitude. Mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction. 10-minute intervals between frame centers (7 mins for science, 3.0 for repositioning). Repeated 11 times to cover 11 hours",,,,,, 2012-007T07:46:00,000T00:02:00,7-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-007T07:48:00,000T04:55:00,7-Jan-12,ISS,Prime,Saturn,EMASCAN,,Saturn Emission Angle Scan,"For each latitude image at a low emission angle, medium emission angle and high emission angle as the planet rotates. Move to other latitudes as time and data volume permit. Collaborative with VIMS.",,,,,, 2012-007T07:48:00,000T04:55:00,7-Jan-12,CIRS,SPASS Rider,Saturn,EMASCAN,,Center to Limb study,,,,,,, 2012-007T07:48:00,000T04:55:00,7-Jan-12,VIMS,SPASS Rider,Saturn,EMASCAN,,Saturn ISS center-to-limb imaging ridealong,CIRS EMASCAN center-to-limb Ridealong. Three images per hour for ~ 5 hrs,,,,,, 2012-007T12:41:00,000T00:02:00,7-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-007T14:53:00,000T09:00:00,7-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-007T15:53:00,000T08:00:00,7-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12007_SP,rider,,,,,, 2012-007T23:53:00,003T08:31:00,7-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-007T23:53:00,003T15:15:00,7-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-008T00:31:00,000T00:02:00,8-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-008T00:33:00,000T01:30:00,8-Jan-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 32.5 requested range 3 Mkm",,,,,, 2012-008T02:01:00,000T00:02:00,8-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-008T02:03:00,000T22:00:00,8-Jan-12,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2012-008T02:03:00,000T22:00:00,8-Jan-12,ISS,SPASS Rider,Saturn,MIRTMAP,,Day WAC,Rider on CIRS to monitor day side clouds in WAC every ~2 hours,,,,,, 2012-008T02:03:00,000T22:00:00,8-Jan-12,VIMS,SPASS Rider,Saturn,MIRTMAP,,Saturn CIRS MIRTMAP ridealong,CIRS MIRTMAP Ridealong for 23 hrs,,,,,, 2012-009T00:01:00,000T00:02:00,9-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-009T06:23:00,000T11:00:00,9-Jan-12,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2012-009T08:23:00,000T09:00:00,9-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-009T09:23:00,000T08:00:00,9-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12009_SP,rider,,,,,, 2012-009T18:01:00,000T00:02:00,9-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-009T18:03:00,000T01:30:00,9-Jan-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 50 requested range 3.3 Mkm",,,,,, 2012-009T18:03:00,000T01:30:00,9-Jan-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-009T18:03:00,000T01:30:00,9-Jan-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 50 range =3.3 Mkm.,,,,,, 2012-009T19:31:00,000T00:02:00,9-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-009T19:33:00,000T05:00:00,9-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-009T19:33:00,000T05:00:00,9-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-009T19:33:00,000T05:00:00,9-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-010T00:31:00,000T00:02:00,10-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-010T00:33:00,000T06:00:00,10-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-010T00:33:00,000T06:00:00,10-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-010T06:31:00,000T00:02:00,10-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-010T06:33:00,000T05:00:00,10-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-010T06:33:00,000T05:00:00,10-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-010T06:33:00,000T05:00:00,10-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-010T11:31:00,000T00:02:00,10-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-010T11:33:00,000T05:00:00,10-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-010T11:33:00,000T05:00:00,10-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-010T11:33:00,000T05:00:00,10-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-010T16:31:00,000T00:02:00,10-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-010T16:33:00,000T06:00:00,10-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-010T16:33:00,000T06:00:00,10-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-010T22:31:00,000T00:02:00,10-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-010T22:33:00,000T05:00:00,10-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-010T22:33:00,000T05:00:00,10-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-010T22:33:00,000T05:00:00,10-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-011T03:31:00,000T00:02:00,11-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-011T08:24:00,006T01:01:00,11-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-011T08:24:00,006T01:01:00,11-Jan-12,CDA,Non-SPASS,Other,RATE010C,,Data rate End:SApo,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-011T08:24:00,000T04:30:00,11-Jan-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-011T08:24:00,005T07:23:00,11-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 150 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2012-011T08:24:00,000T09:00:00,11-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-011T09:24:00,000T08:00:00,11-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12011_SP,rider,,,,,, 2012-011T15:08:00,004T18:31:00,11-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-011T18:02:00,000T00:02:00,11-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-011T18:04:00,000T01:30:00,11-Jan-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 65.5 requested range 3.1 Mkm",,,,,, 2012-011T18:04:00,000T01:30:00,11-Jan-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-011T18:04:00,000T01:30:00,11-Jan-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 66 range =3.1 Mkm.,,,,,, 2012-011T18:45:00,000T05:34:00,11-Jan-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-011T19:32:00,000T00:02:00,11-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-011T19:34:00,000T02:55:00,11-Jan-12,ISS,Prime,Saturn,MONITOR,,Saturn storm watch,"monitoring trigger repeated ~ every 2 hours, or at the beginning and the end of the shorter observation:",,,,,, 2012-011T22:27:00,000T00:02:00,11-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-012T00:39:00,000T09:00:00,12-Jan-12,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2012-012T00:39:00,000T09:00:00,12-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-012T01:39:00,000T08:00:00,12-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12012_SP,rider,,,,,, 2012-012T10:17:00,000T00:02:00,12-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-012T10:19:00,000T01:30:00,12-Jan-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 69.3 requested range 2.9 Mkm",,,,,, 2012-012T10:19:00,000T01:30:00,12-Jan-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-012T10:19:00,000T01:30:00,12-Jan-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 69 range =2.9 Mkm.,,,,,, 2012-012T11:47:00,000T00:02:00,12-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-012T11:49:00,000T10:40:00,12-Jan-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-012T11:49:00,000T10:40:00,12-Jan-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-012T22:27:00,000T00:02:00,12-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-013T00:39:00,000T09:00:00,13-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-013T01:39:00,000T08:00:00,13-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12013_SP,rider,,,,,, 2012-013T10:17:00,000T00:02:00,13-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-013T10:19:00,000T01:30:00,13-Jan-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 72.9 requested range 2.6 Mkm",,,,,, 2012-013T10:19:00,000T01:30:00,13-Jan-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-013T10:19:00,000T01:30:00,13-Jan-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 73 range =2.6 Mkm.,,,,,, 2012-013T11:47:00,000T00:02:00,13-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-013T11:49:00,000T10:40:00,13-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-013T11:49:00,000T10:40:00,13-Jan-12,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT,COMPSIT ridelong with CIRS,,,,,, 2012-013T11:49:00,000T10:40:00,13-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-013T15:46:00,000T20:00:00,13-Jan-12,CDA,SPASS Rider,DustRAM direction,ISD0040,,CDA ISD 2012-016T15:46:00,ISD observation around apoapse 2012-016T15:46:00 49.163222 Rs,,,,,, 2012-013T22:27:00,000T00:02:00,13-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-014T00:39:00,000T09:00:00,14-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-014T01:39:00,000T08:00:00,14-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12014_SP,rider,,,,,, 2012-014T10:17:00,000T00:02:00,14-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-014T10:19:00,000T01:30:00,14-Jan-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 73.1 requested range 2.2 Mkm",,,,,, 2012-014T10:19:00,000T01:30:00,14-Jan-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-014T10:19:00,000T01:30:00,14-Jan-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 73 range =2.1 Mkm.,,,,,, 2012-014T11:47:00,000T00:02:00,14-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-014T11:49:00,000T10:40:00,14-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-014T11:49:00,000T10:40:00,14-Jan-12,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT,COMPSIT ridelong with CIRS,,,,,, 2012-014T11:49:00,000T10:40:00,14-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-014T22:27:00,000T00:02:00,14-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-015T00:39:00,000T09:00:00,15-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-015T01:39:00,000T08:00:00,15-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12015_SP,rider,,,,,, 2012-015T09:46:00,000T20:00:00,15-Jan-12,CDA,SPASS Rider,DustRAM direction,ISD0040,,CDA ISD 2012-016T15:46:00,ISD observation around apoapse 2012-016T15:46:00 49.163222 Rs,,,,,, 2012-015T10:17:00,000T00:02:00,15-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-015T10:19:00,000T01:30:00,15-Jan-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 68.4 requested range 1.9 Mkm",,,,,, 2012-015T10:19:00,000T01:30:00,15-Jan-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-015T10:19:00,000T01:30:00,15-Jan-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,Titan Monitoring Campaign; phase = 68 range =1.9 Mkm.,,,,,, 2012-015T11:47:00,000T00:02:00,15-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-015T11:49:00,000T12:10:00,15-Jan-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-015T11:49:00,000T12:10:00,15-Jan-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-015T23:57:00,000T00:02:00,15-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-016T00:39:00,000T09:00:00,16-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-016T01:39:00,000T08:00:00,16-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_159IC_DSCAL12016_SP,rider,,,,,, 2012-016T09:39:00,000T07:00:00,16-Jan-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-016T09:39:00,000T06:08:00,16-Jan-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-016T15:46:37,000T00:00:01,16-Jan-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 24.2 d, inc = 1.6 deg, r = 49.116 Rs, phase = 57 deg",,,,,, 2012-016T15:47:00,008T07:08:00,16-Jan-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S72,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-016T15:47:00,000T17:38:00,16-Jan-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-016T15:47:00,008T07:08:00,16-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_159_160",,,,,, 2012-016T15:47:00,000T17:38:00,16-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 150 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2012-016T15:47:00,008T07:08:00,16-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-016T16:39:00,000T16:46:00,16-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-017T00:25:00,000T09:00:00,17-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-017T01:25:00,000T08:00:00,17-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12017_SP,rider,,,,,, 2012-017T01:46:00,000T20:00:00,17-Jan-12,CDA,SPASS Rider,DustRAM direction,ISD0040,,CDA ISD 2012-016T15:46:00,ISD observation around apoapse 2012-016T15:46:00 49.163222 Rs,,,,,, 2012-017T09:25:00,001T07:03:00,17-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-017T09:25:00,003T13:45:00,17-Jan-12,CDA,Non-SPASS,Other,RATE010A,,Data rate Enter:SApo End: S72,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-017T09:25:00,007T13:30:00,17-Jan-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-017T09:25:00,000T16:02:00,17-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-017T09:25:00,007T13:30:00,17-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MAPS SURVEY Campaign Overlay,"Overlay: adding 100 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane.",,,,,, 2012-017T10:03:00,000T00:02:00,17-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-017T10:05:00,000T01:30:00,17-Jan-12,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 48.4 requested range 1.8 Mkm",,,,,, 2012-017T10:05:00,000T01:30:00,17-Jan-12,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-017T10:05:00,000T01:30:00,17-Jan-12,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 48, range =1.8 Mkm.",,,,,, 2012-017T11:33:00,000T00:02:00,17-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-017T11:35:00,000T02:00:00,17-Jan-12,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-017T11:35:00,000T02:00:00,17-Jan-12,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-017T13:33:00,000T00:02:00,17-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-017T13:35:00,000T09:00:00,17-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-017T13:35:00,000T09:00:00,17-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-017T22:33:00,000T00:02:00,17-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-017T22:35:00,000T02:00:00,17-Jan-12,ISS,Prime,Saturn,WIND2HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-017T22:35:00,000T02:00:00,17-Jan-12,UVIS,Non-SPASS,Saturn,WIND2HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-018T00:00:00,000T00:42:00,18-Jan-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-018T00:33:00,000T00:02:00,18-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-018T00:35:00,000T11:00:00,18-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-018T00:35:00,000T11:00:00,18-Jan-12,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS COMPSIT,COMPSIT ridelong with CIRS,,,,,, 2012-018T00:35:00,000T11:00:00,18-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-018T01:27:00,004T22:04:00,18-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-018T11:33:00,000T00:02:00,18-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-018T14:10:00,000T09:00:00,18-Jan-12,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2012-018T14:10:00,000T09:00:00,18-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-018T15:10:00,000T08:00:00,18-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12018_SP,rider,,,,,, 2012-018T16:28:00,004T06:50:00,18-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-018T19:46:00,000T20:00:00,18-Jan-12,CDA,SPASS Rider,DustRAM direction,ISD0040,,CDA ISD 2012-016T15:46:00,ISD observation around apoapse 2012-016T15:46:00 49.163222 Rs,,,,,, 2012-018T23:48:00,000T00:02:00,18-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-018T23:50:00,000T01:30:00,18-Jan-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 39.5 requested range 2.2 Mkm",,,,,, 2012-018T23:50:00,000T01:30:00,18-Jan-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-018T23:50:00,000T01:30:00,18-Jan-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 40 deg, range =2.2 Mkm.",,,,,, 2012-019T01:18:00,000T00:02:00,19-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-019T01:20:00,000T05:00:00,19-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-019T01:20:00,000T05:00:00,19-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-019T01:20:00,000T05:00:00,19-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-019T06:18:00,000T00:02:00,19-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-019T06:20:00,000T06:00:00,19-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-019T06:20:00,000T06:00:00,19-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-019T12:18:00,000T00:02:00,19-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-019T12:20:00,000T05:00:00,19-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-019T12:20:00,000T05:00:00,19-Jan-12,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2012-019T12:20:00,000T05:00:00,19-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-019T12:20:00,000T05:00:00,19-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-019T17:18:00,000T00:02:00,19-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-019T17:20:00,000T05:00:00,19-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-019T17:20:00,000T05:00:00,19-Jan-12,CIRS,,Saturn,WIND5HR,,low emit COMPSIT avoid rings,,,,,,, 2012-019T17:20:00,000T05:00:00,19-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-019T17:20:00,000T05:00:00,19-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-019T22:18:00,000T00:02:00,19-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-019T22:20:00,000T06:00:00,19-Jan-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-019T22:20:00,000T06:00:00,19-Jan-12,UVIS,Non-SPASS,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-020T04:18:00,000T00:02:00,20-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-020T04:20:00,000T05:00:00,20-Jan-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","Track features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-020T04:20:00,000T05:00:00,20-Jan-12,VIMS,SPASS Rider,Saturn,WIND5HR,,ISS Wind Map,Wind movie ride-along with ISS,,,,,, 2012-020T04:20:00,000T05:00:00,20-Jan-12,UVIS,Non-SPASS,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-020T09:18:00,000T00:02:00,20-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-020T14:10:00,000T09:00:00,20-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-020T15:10:00,000T08:00:00,20-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12020_SP,rider,,,,,, 2012-020T23:10:00,003T23:45:00,20-Jan-12,CDA,Non-SPASS,Other,RATE010B,,Data rate Enter:SApo End: S72,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-020T23:48:00,000T00:02:00,20-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-020T23:50:00,000T01:30:00,20-Jan-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 42.4 requested range 2.9 Mkm",,,,,, 2012-020T23:50:00,000T01:30:00,20-Jan-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-020T23:50:00,000T01:30:00,20-Jan-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 42 deg, range =2.9 Mkm.",,,,,, 2012-021T00:00:00,000T00:30:00,21-Jan-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-021T01:18:00,000T00:02:00,21-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-021T01:20:00,000T16:00:00,21-Jan-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-021T01:20:00,000T16:00:00,21-Jan-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-021T17:18:00,000T00:02:00,21-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-021T17:20:00,000T10:00:00,21-Jan-12,ISS,Prime,Saturn,EMASCAN,,Saturn Emission Angle Scan,"For each latitude image at a low emission angle, medium emission angle and high emission angle as the planet rotates. Move to other latitudes as time and data volume permit. Collaborative with VIMS.",,,,,, 2012-021T17:20:00,000T10:00:00,21-Jan-12,CIRS,SPASS Rider,Saturn,EMASCAN,,Center to Limb study,,,,,,, 2012-021T17:20:00,000T10:00:00,21-Jan-12,VIMS,SPASS Rider,Saturn,EMASCAN,,Saturn ISS center-to-limb imaging ridealong,CIRS EMASCAN center-to-limb Ridealong. Three images per hour for ~ 9 hrs,,,,,, 2012-022T03:18:00,000T00:02:00,22-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-022T13:55:00,000T09:00:00,22-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-022T14:55:00,000T08:00:00,22-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12022_SP,rider,,,,,, 2012-022T23:18:00,001T23:37:00,22-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-022T23:31:00,001T23:24:00,22-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-022T23:33:00,000T00:02:00,22-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-022T23:35:00,000T01:30:00,22-Jan-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 54.3 requested range 3.2 Mkm",,,,,, 2012-022T23:35:00,000T01:30:00,22-Jan-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-022T23:35:00,000T01:30:00,22-Jan-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 54 deg, range =3.2 Mkm.",,,,,, 2012-023T01:03:00,000T00:02:00,23-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-023T01:05:00,000T22:00:00,23-Jan-12,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2012-023T01:05:00,000T22:00:00,23-Jan-12,ISS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Day WAC,Rider on CIRS to monitor day side clouds in WAC every ~2 hours,,,,,, 2012-023T01:05:00,000T22:00:00,23-Jan-12,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP Ride-along,MIRMAP ridelong with CIRS,,,,,, 2012-023T23:03:00,000T00:02:00,23-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-023T23:45:00,000T12:40:00,23-Jan-12,ISS,Prime,Other,SIAPOL,,Siarnaq,Observation of irregular moon of Saturn.,,,,,, 2012-023T23:45:00,000T12:40:00,23-Jan-12,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2012-024T12:23:00,000T00:02:00,24-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-024T13:55:00,000T09:00:00,24-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-024T14:55:00,000T08:00:00,24-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12024_SP,rider,,,,,, 2012-024T22:55:00,001T10:01:00,24-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-024T22:55:00,000T20:00:00,24-Jan-12,CDA,Non-SPASS,Other,DECON,Decontamination,Decon in S72,SSR-Load (6Ext_Mem_Load) planned to be at exactly 2012-024T23:55:00. One hour apart from the preceeding D/L (SP_160EA_C70METSEQ024_PRIME) having a carryover with 0 MB. Expectations is that a SSR-Ping-Pong disable might not be necessary. No additional DV necessary,,,,,, 2012-024T22:55:00,002T17:10:00,24-Jan-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S72,Range enter= 14.002192 Rs exit= 14.007424 Range altitude= -15184.727 km ... -7342.4240,,,,,, 2012-024T22:55:00,000T00:43:00,24-Jan-12,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-024T22:55:00,002T23:46:00,24-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-024T22:55:00,004T23:46:00,24-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SAT_160",,,,,, 2012-024T22:55:00,002T15:15:00,24-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-024T23:00:00,000T00:02:00,24-Jan-12,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S72 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2012-024T23:38:00,000T00:07:00,24-Jan-12,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-024T23:39:00,000T00:02:00,24-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-024T23:41:00,000T01:30:00,24-Jan-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 72.8 requested range 3.1 Mkm",,,,,, 2012-024T23:41:00,000T01:30:00,24-Jan-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-024T23:41:00,000T01:30:00,24-Jan-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 73 deg, range =3.1 Mkm.",,,,,, 2012-024T23:45:00,000T00:05:00,24-Jan-12,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-024T23:50:00,000T00:33:00,24-Jan-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-025T00:23:00,000T00:30:00,25-Jan-12,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2012-025T00:53:00,001T22:22:00,25-Jan-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-025T01:09:00,000T00:02:00,25-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-025T02:41:00,000T16:00:00,25-Jan-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-025T02:41:00,000T16:00:00,25-Jan-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-025T18:39:00,000T00:02:00,25-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-025T18:41:00,000T03:05:00,25-Jan-12,VIMS,Prime,Saturn,REGMAP,Regional mapping,Regional Map,"Two 3*3 mosaics of Saturn, centered on the equator. Each frame takes 7 minutes of data, 3 minutes to move to next frame.",,,,,, 2012-025T21:44:00,000T00:02:00,25-Jan-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-025T23:56:00,000T09:00:00,25-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-026T00:56:00,000T08:00:00,26-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12025_SP,rider,,,,,, 2012-026T08:56:00,003T13:45:00,26-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-026T09:36:00,000T14:55:00,26-Jan-12,ISS,Prime,Saturn,EMASCAN,,Saturn Emission Angle Scan,"For each latitude image at a low emission angle, medium emission angle and high emission angle as the planet rotates. Move to other latitudes as time and data volume permit. Collaborative with VIMS.",,,,,, 2012-026T09:36:00,000T14:55:00,26-Jan-12,CIRS,SPASS Rider,Saturn,EMASCAN,,Center to Limb study,,,,,,, 2012-026T09:36:00,000T14:55:00,26-Jan-12,VIMS,SPASS Rider,Saturn,EMASCAN,,Feature Track (Emission Angle Scan),Follow several features from limb to center-of disk and from center-of -disk to limb. Ridealong with ISS.,,,,,, 2012-026T23:15:00,000T02:00:00,26-Jan-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-027T00:31:00,000T11:00:00,27-Jan-12,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn Far-IR map,Northern hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude Range=14Rs ~60 mrad from N Pole to Equator,,,,,, 2012-027T01:15:00,000T00:34:00,27-Jan-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2012-027T01:49:00,001T01:23:09,27-Jan-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-027T13:41:00,000T09:00:00,27-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-027T14:10:00,000T08:31:00,27-Jan-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-027T14:41:00,000T08:00:00,27-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12027_SP,rider,,,,,, 2012-027T16:05:00,000T07:16:00,27-Jan-12,CDA,Non-SPASS,Other,RATE080A,,Data rate,Range enter= 13.994778 Rs exit= 13.994147 Range altitude= -7320.0579 km ... -15306.985,,,,,, 2012-027T22:41:00,002T00:00:00,27-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-027T22:41:00,002T00:00:00,27-Jan-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-027T23:21:00,000T11:00:00,27-Jan-12,VIMS,Prime,Saturn,DEEPDYN,,Deep dynamics mosaic for Deep Atmopsheres Campaign,"11 2x3 Global mosaics, one collected each hour throughout the 11-hrs duration. Mosaic is centered on the equator at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction, with border between them along the equator. 10-minute intervals between frame centers (7 mins for science, 3 for repositioning). Each of these mosaics should take an hour.",,,,,, 2012-027T23:21:00,000T11:00:00,27-Jan-12,CIRS,SPASS Rider,Saturn,DEEPDYN,,VIMS rider for good spatial res obs,rider,,,,,, 2012-027T23:21:00,000T21:39:00,27-Jan-12,CDA,Non-SPASS,Other,RATE080B,,Data rate,Range enter= 13.994778 Rs exit= 13.994147 Range altitude= -7320.0579 km ... -15306.985,,,,,, 2012-028T02:21:00,000T02:00:00,28-Jan-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-028T02:21:57,000T02:00:00,28-Jan-12,CDA,SPASS Rider,DustRAM direction,RPX0320,,CDA RPXing 2012-028T03:21:57,RPXing at 9.7523021 Rs,,,,,, 2012-028T03:12:09,000T13:58:31,28-Jan-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-028T07:51:00,000T03:00:00,28-Jan-12,RADAR,Non-SPASS,Other,WU4SAGM,,Warmup for Saturn V/R/V Deep Atmosphere.,Warmup for global map-2 in SWG PIEs.,,,,,, 2012-028T10:51:00,000T14:00:00,28-Jan-12,RADAR,Prime,Saturn,GLOBALMAP,Global coverage mapping,Saturn V/R/V Deep Atmosphere.,Saturn global map-2 in EQ-PIEs. peri=2012-028T18:29:55; 266523 km.,,,,,, 2012-028T12:00:00,000T12:00:00,28-Jan-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-028T17:10:40,000T02:34:00,28-Jan-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-028T18:29:57,000T00:00:01,28-Jan-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 4.418 Rs, lat = 2 deg, phase = 124 deg",,,,,, 2012-028T19:44:40,000T17:55:07,28-Jan-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-028T21:00:00,000T03:51:00,28-Jan-12,CDA,Non-SPASS,Other,RATE080C,,Data rate,Range enter= 13.994778 Rs exit= 13.994147 Range altitude= -7320.0579 km ... -15306.985,,,,,, 2012-029T00:51:00,000T19:17:57,29-Jan-12,CDA,Non-SPASS,Other,RATE080D,,Data rate,Range enter= 13.994778 Rs exit= 13.994147 Range altitude= -7320.0579 km ... -15306.985,,,,,, 2012-029T01:21:00,000T11:00:00,29-Jan-12,VIMS,Prime,Saturn,DEEPDYN,,Deep dynamics mosaic for Deep Atmopsheres Campaign,"11 2x3 Global mosaics, one collected each hour throughout the 11-hrs duration. Mosaic is centered on the equator at the sub-S/C Saturn longitude. Each mosaic comprised of 2 rows of 3 frames each, oriented with the 3 frames in the east-west direction, with border between them along the equator. 10-minute intervals between frame centers (7 mins for science, 3 for repositioning). Each of these mosaics should take an hour.",,,,,, 2012-029T01:21:00,000T11:00:00,29-Jan-12,ISS,Non-SPASS,Saturn,DEEPDYN,,Night NAC at each frame of 3x2,Rider on 2x3 VIMS mosaic to monitor day side clouds in WAC every hour,,,,,, 2012-029T02:11:00,000T02:00:00,29-Jan-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-029T02:13:57,000T02:00:00,29-Jan-12,CDA,SPASS Rider,DustRAM direction,RPX0330,,CDA RPXing 2012-029T03:13:57,RPXing at 6.9313774 Rs,,,,,, 2012-029T13:39:47,000T12:00:01,29-Jan-12,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-029T13:41:00,000T09:00:00,29-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-029T14:41:00,000T08:00:00,29-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12029_SP,rider,,,,,, 2012-029T20:08:57,010T16:07:03,29-Jan-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.006797 Rs exit= 14.001835 Range altitude= -15333.168 km ... 5862.8843,,,,,, 2012-029T22:41:00,000T12:58:48,29-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-029T22:41:00,000T10:58:48,29-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-029T22:41:00,000T12:58:47,29-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_160_T81",,,,,, 2012-029T22:41:00,001T18:00:00,29-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-029T23:36:01,000T05:03:47,29-Jan-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-029T23:36:01,000T05:03:47,29-Jan-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-029T23:36:01,000T05:03:47,29-Jan-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS while staring at Titan. Phase = 162 deg. SSC Lat/Lon = 4.263S/8.601 deg, SS Lat/Lon = 12.957N/172.610 deg. Alt = 255975.8 km, range = 258550.8 km. Resolution = 128 km/px. Temp. N1. Obtain cubes while staring at Titan.",,,,,, 2012-029T23:36:01,000T05:03:47,29-Jan-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-030T01:39:48,000T11:00:00,30-Jan-12,INMS,Non-SPASS,Saturn,T81INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-030T04:39:48,000T06:45:00,30-Jan-12,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-030T04:39:48,000T06:45:00,30-Jan-12,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2012-030T04:39:48,000T06:45:00,30-Jan-12,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 161 deg. SSC Lat/Lon = 7.221S/14.318 deg, SS Lat/Lon = 12.959N/176.371 deg. Alt = 176614.6 km, range = 179189.6 km. Resolution = 88 km/px. Temp. X. Obtain cubes while scanning across Titan.",,,,,, 2012-030T09:39:48,000T08:00:00,30-Jan-12,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T81 flyby,T81 is a flyby at extremely high altitude over the south pole. It is highly unlikely that MAG will detect any signs of Titan's induced magnetosphere. We assign grade two priority. Data rate: 988bps (16vps).,,,,,, 2012-030T11:24:48,000T05:00:00,30-Jan-12,ISS,Prime,Titan,HIRES,High resolution image,HRI (High Resolution Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-030T11:24:48,000T05:15:00,30-Jan-12,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with ISS.,,,,,, 2012-030T11:24:48,000T05:00:00,30-Jan-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping of Titan.,"VIMS ridealong with ISS during C/A. At C/A, phase = 96.3 deg. SSC Lat/Lon = 59.98S/104.91 deg, SS Lat/Lon = 12.964N/184.833 deg. Alt = 31130.2 km, range = 33705.2 km. Resolution = 15.6 km/px. Obtain mosaics and cubes for regional mapping.",,,,,, 2012-030T11:24:48,000T05:00:00,30-Jan-12,UVIS,Non-SPASS,Titan,HIRES,High resolution image,HDAC and FUV and EUV on Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-030T11:39:47,000T04:30:00,30-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_160_T81",,,,,, 2012-030T11:39:48,000T01:00:00,30-Jan-12,CAPS,SPASS Rider,Titan,T81INBND,,Inbound 160TI (T81),null,,,,,, 2012-030T11:39:48,000T01:00:00,30-Jan-12,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-030T11:39:48,000T01:00:00,30-Jan-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-030T12:39:48,000T02:00:00,30-Jan-12,CAPS,SPASS Rider,Titan,T81CLOSE,,Closest Approach 160TI (T81),null,,,,,, 2012-030T12:39:48,000T02:00:00,30-Jan-12,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-030T12:39:48,000T02:00:00,30-Jan-12,INMS,Non-SPASS,Titan,TITAN81,,Titan Flyby,Titan observation,,,,,, 2012-030T12:39:48,000T02:00:00,30-Jan-12,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2012-030T14:39:48,000T01:00:00,30-Jan-12,CAPS,SPASS Rider,Titan,T81OUTBND,,Outbound 160TI (T81),null,,,,,, 2012-030T14:39:48,000T01:00:00,30-Jan-12,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-030T14:39:48,000T11:00:00,30-Jan-12,INMS,Non-SPASS,Saturn,T81OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-030T14:39:48,000T01:00:00,30-Jan-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-030T15:39:48,001T06:01:13,30-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-030T16:09:47,001T00:31:13,30-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_160_T81",,,,,, 2012-030T16:24:48,000T06:15:00,30-Jan-12,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-030T16:24:48,000T06:15:00,30-Jan-12,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan Scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 40 deg. SSC Lat/Lon = 26.977S/184.530 deg, SS Lat/Lon = 12.965N/184.530 deg. Alt = 64903.9 km, range = 67478.9 km. Resolution = 32 km/px. Temp. modified X. Obtain cubes while scanning across Titan.",,,,,, 2012-030T16:39:48,000T06:00:00,30-Jan-12,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS.,,,,,, 2012-030T17:39:48,000T23:01:12,30-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-030T22:39:48,000T05:36:13,30-Jan-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-030T22:39:48,000T05:36:13,30-Jan-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-030T22:39:48,000T05:36:13,30-Jan-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS while staring at Titan. Phase = 25 deg. SSC Lat/Lon = 10.576S/200.823 deg, SS Lat/Lon = 12.968N/193.296 deg. Alt = 176715.6 km, range = 179290.6 km. Resolution = 88 km/px. Temp. C. Obtain cubes while staring at Titan.",,,,,, 2012-030T22:39:48,000T05:36:13,30-Jan-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-031T01:39:48,000T15:01:12,31-Jan-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-031T06:41:00,000T10:00:00,31-Jan-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-031T07:41:00,000T10:00:00,31-Jan-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12031_SP,rider,,,,,, 2012-031T16:41:00,002T15:46:00,31-Jan-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-031T16:41:00,009T05:47:00,31-Jan-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-031T16:41:00,008T19:35:00,31-Jan-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_160_161",,,,,, 2012-031T16:41:00,000T04:00:00,31-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-031T20:41:00,008T15:35:00,31-Jan-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-031T21:41:00,017T17:18:00,31-Jan-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-031T22:00:00,002T00:00:00,31-Jan-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - outbound leg - Apo region,,,,,, 2012-031T22:20:00,000T03:00:00,31-Jan-12,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2012-032T01:20:00,000T02:37:00,1-Feb-12,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2012-032T06:57:00,000T09:00:00,1-Feb-12,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing).",,,,,, 2012-032T06:57:00,000T09:00:00,1-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-032T07:57:00,000T08:00:00,1-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12032_SP,rider,,,,,, 2012-032T15:57:00,001T07:30:00,1-Feb-12,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2012-032T15:57:00,001T07:30:00,1-Feb-12,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-032T15:57:00,001T07:30:00,1-Feb-12,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- Range=1.1 to 1.8 Phase=17 to 15,,,,,, 2012-033T23:27:00,000T09:00:00,2-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-034T00:27:00,000T08:00:00,3-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12033_SP,rider,,,,,, 2012-034T08:27:00,000T15:00:00,3-Feb-12,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2012-034T08:27:00,000T15:00:00,3-Feb-12,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-034T08:27:00,000T15:00:00,3-Feb-12,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,"TEA-1cube every hour-Range=2,0 to 2.4 Phase=15 to 16",,,,,, 2012-034T08:27:00,001T00:00:00,3-Feb-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-034T23:27:00,000T09:00:00,3-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-035T00:00:00,000T01:08:00,4-Feb-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-035T00:27:00,000T08:00:00,4-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12034_SP,rider,,,,,, 2012-035T08:27:00,000T20:45:00,4-Feb-12,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2012-035T08:27:00,000T20:45:00,4-Feb-12,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-035T08:27:00,000T20:45:00,4-Feb-12,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour-Range=2.5 to 3.0 Phase=23 to 18,,,,,, 2012-035T08:27:00,005T03:49:00,4-Feb-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-036T06:42:00,000T09:00:00,5-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-036T07:42:00,000T08:00:00,5-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12036_SP,rider,,,,,, 2012-036T15:42:00,000T13:30:00,5-Feb-12,CDA,Prime,DustRAM direction,ISD0041,,CDA ISD 2012-040T12:16:00,ISD observation around apoapse 2012-040T12:16:00 48.160571 Rs,,,,,, 2012-037T06:42:00,000T09:00:00,6-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-037T07:42:00,000T08:00:00,6-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12037_SP,rider,,,,,, 2012-037T16:20:00,000T00:02:00,6-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-037T16:22:00,000T01:30:00,6-Feb-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 31.4 requested range 3.6 Mkm",,,,,, 2012-037T16:22:00,000T01:30:00,6-Feb-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-037T16:22:00,000T01:30:00,6-Feb-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 31 deg, range =3.6 Mkm. Also Stormwatch cube",,,,,, 2012-037T17:50:00,000T00:02:00,6-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-037T17:52:00,000T01:00:00,6-Feb-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-037T17:52:00,000T01:00:00,6-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-037T18:50:00,000T00:02:00,6-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-037T18:52:00,000T09:40:00,6-Feb-12,ISS,Prime,Other,L5TITAN,,Titan L5 satellite search,Satellite search around Titan L5 Lagrange point.,,,,,, 2012-037T18:52:00,000T09:40:00,6-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-038T02:32:00,000T13:00:00,7-Feb-12,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,"RSS USO characterization plus PIM. Pointing=XBAND to Earth. No rolling during 3-hour USO from 2012-038T06:32:00 till 2012-038T09:32:00, to be tracked at DSS-25 in 1-way mode. Keep Ka-band ON till end of downlink at 2012-038T15:32:00 to satisfy PIM requirement.",,,,,, 2012-038T04:30:00,000T00:02:00,7-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-038T06:42:00,000T09:00:00,7-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-038T07:42:00,000T08:00:00,7-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12038_SP,rider,,,,,, 2012-038T12:00:00,002T00:00:00,7-Feb-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - Apo leg,,,,,, 2012-038T16:20:00,000T00:02:00,7-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-038T16:22:00,000T01:00:00,7-Feb-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 007 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-038T16:22:00,000T01:00:00,7-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-038T17:20:00,000T00:02:00,7-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-038T17:22:00,000T11:10:00,7-Feb-12,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2012-038T17:22:00,000T11:10:00,7-Feb-12,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-038T17:22:00,000T11:10:00,7-Feb-12,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- TBChecked Range=0.55 to 0.83 Phase=19 to 18. Also Stormwatch Cube,,,,,, 2012-039T04:30:00,000T00:02:00,8-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-039T04:32:00,000T06:40:00,8-Feb-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-039T06:42:00,000T09:00:00,8-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-039T07:42:00,000T08:00:00,8-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12039_SP,rider,,,,,, 2012-039T19:42:00,000T09:16:00,8-Feb-12,CDA,Prime,DustRAM direction,ISD0041,,CDA ISD 2012-040T12:16:00,ISD observation around apoapse 2012-040T12:16:00 48.160571 Rs,,,,,, 2012-040T06:28:00,000T09:00:00,9-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-040T07:28:00,000T08:00:00,9-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_160IC_DSCAL12040_SP,rider,,,,,, 2012-040T12:16:00,010T16:22:57,9-Feb-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.006797 Rs exit= 14.001835 Range altitude= -15333.168 km ... 5862.8843,,,,,, 2012-040T12:16:00,000T02:00:00,9-Feb-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-040T12:16:00,009T02:43:00,9-Feb-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_160_161",,,,,, 2012-040T12:16:00,009T02:43:00,9-Feb-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-040T12:16:15,000T00:00:01,9-Feb-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 23.5 d, inc = 1.4 deg, r = 48.111 Rs, phase = 55 deg",,,,,, 2012-040T14:16:00,001T01:12:00,9-Feb-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-040T15:28:00,000T07:00:00,9-Feb-12,CDA,Prime,DustRAM direction,ISD0041,,CDA ISD 2012-040T12:16:00,ISD observation around apoapse 2012-040T12:16:00 48.160571 Rs,,,,,, 2012-040T22:28:00,000T08:00:00,9-Feb-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-041T06:28:00,008T08:31:00,10-Feb-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-041T06:28:00,000T09:00:00,10-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-041T07:28:00,000T08:00:00,10-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12041_SP,rider,,,,,, 2012-041T15:28:00,000T15:00:00,10-Feb-12,CDA,Prime,DustRAM direction,ISD0041,,CDA ISD 2012-040T12:16:00,ISD observation around apoapse 2012-040T12:16:00 48.160571 Rs,,,,,, 2012-041T15:28:00,001T00:00:00,10-Feb-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-041T18:00:00,002T00:00:00,10-Feb-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - Apo leg,,,,,, 2012-042T06:28:00,000T09:00:00,11-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-042T07:28:00,000T08:00:00,11-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12042_SP,rider,,,,,, 2012-042T15:28:00,004T16:15:00,11-Feb-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-042T16:06:00,000T00:02:00,11-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-042T16:08:00,000T01:00:00,11-Feb-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-042T16:08:00,000T01:00:00,11-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-042T17:06:00,000T00:02:00,11-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-042T17:08:00,000T11:10:00,11-Feb-12,CIRS,Prime,Titan,TEA,,Titan Composition,Titan composition,,,,,, 2012-042T17:08:00,000T11:10:00,11-Feb-12,ISS,,Titan,TEA,,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-042T17:08:00,000T11:10:00,11-Feb-12,VIMS,SPASS Rider,Titan,TEA,,TEA-TMC-Clouds,TEA-1cube every hour- TBChecked Range=0.55 to 0.83 Phase=19 to 18. Also Stormwatch cube,,,,,, 2012-043T04:16:00,000T00:02:00,12-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-043T06:28:00,000T09:00:00,12-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-043T07:28:00,000T08:00:00,12-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12043_SP,rider,,,,,, 2012-043T15:28:00,000T13:15:00,12-Feb-12,CDA,Prime,DustRAM direction,ISD0041,,CDA ISD 2012-040T12:16:00,ISD observation around apoapse 2012-040T12:16:00 48.160571 Rs,,,,,, 2012-044T06:13:00,000T09:00:00,13-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-044T07:13:00,000T08:00:00,13-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12044_SP,rider,,,,,, 2012-044T22:52:00,000T00:02:00,13-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-044T22:54:00,000T01:30:00,13-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-045T00:22:00,000T00:02:00,14-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-045T00:24:00,000T01:30:00,14-Feb-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 86.8 requested range 3.1 Mkm",,,,,, 2012-045T00:24:00,000T01:30:00,14-Feb-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-045T00:24:00,000T01:28:00,14-Feb-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 87 deg, range =3.1 Mkm.",,,,,, 2012-045T01:52:00,000T00:02:00,14-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-045T01:54:00,000T02:06:00,14-Feb-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-045T01:54:00,000T02:06:00,14-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-045T03:58:00,000T00:02:00,14-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-045T06:13:00,000T09:00:00,14-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-045T07:13:00,000T08:00:00,14-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12045_SP,rider,,,,,, 2012-045T15:13:00,000T06:00:00,14-Feb-12,CDA,Prime,DustRAM direction,ISD0041,,CDA ISD 2012-040T12:16:00,ISD observation around apoapse 2012-040T12:16:00 48.160571 Rs,,,,,, 2012-045T22:43:00,000T09:00:00,14-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-046T07:43:00,000T04:00:00,15-Feb-12,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2012-046T07:43:00,000T04:00:00,15-Feb-12,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2012-046T11:43:00,000T11:00:00,15-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-046T22:43:00,000T09:00:00,15-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-046T23:43:00,000T08:00:00,15-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12046_SP,rider,,,,,, 2012-047T06:00:00,002T00:00:00,16-Feb-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - inbound leg - Apo region,,,,,, 2012-047T07:43:00,000T23:46:00,16-Feb-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-047T08:21:00,000T00:02:00,16-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-047T08:23:00,000T01:30:00,16-Feb-12,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 106.1 requested range 1.6 Mkm",,,,,, 2012-047T08:23:00,000T01:30:00,16-Feb-12,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-047T08:23:00,000T01:30:00,16-Feb-12,VIMS,SPASS Rider,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 106 deg, range =1.6 Mkm. Also Stormwatch cube",,,,,, 2012-047T09:51:00,000T00:02:00,16-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-047T09:53:00,000T12:00:00,16-Feb-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-047T21:51:00,000T00:02:00,16-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-047T22:29:00,000T09:00:00,16-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-047T23:29:00,000T08:00:00,16-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12047_SP,rider,,,,,, 2012-048T07:29:00,001T01:14:17,17-Feb-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-048T08:08:00,000T00:02:00,17-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-048T08:10:00,000T06:00:00,17-Feb-12,ISS,Prime,RingE,ERNGVERT,,Edge-on obs E-ring observation after Equinox.,Low elevation observation of E ring at moderate phase.,,,,,, 2012-048T08:10:00,000T06:00:00,17-Feb-12,CIRS,SPASS Rider,rings(general),ERNGVERT,,,null,,,,,, 2012-048T08:10:00,000T06:00:00,17-Feb-12,VIMS,SPASS Rider,RingE,ERNGVERT,,E Ring observation,"E Ring observation, 1 second integration time. Also Stormwatch cube",,,,,, 2012-048T14:08:00,000T00:02:00,17-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-048T14:20:00,000T13:20:00,17-Feb-12,ISS,Prime,RingE,ERNGVERT,,Edge-on obs E-ring observation after Equinox.,Low elevation observation of E ring at moderate phase.,,,,,, 2012-048T14:20:00,000T13:20:00,17-Feb-12,CIRS,SPASS Rider,rings(general),ERNGVERT,,,null,,,,,, 2012-048T14:20:00,000T13:20:00,17-Feb-12,VIMS,SPASS Rider,RingE,ERNGVERT,,E Ring observation,"E Ring observation, 1 second integration time. Also Stormwatch cube",,,,,, 2012-049T03:38:00,000T00:02:00,18-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-049T05:59:00,000T09:00:00,18-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-049T06:59:00,000T08:00:00,18-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12049_SP,rider,,,,,, 2012-049T08:43:17,000T12:00:00,18-Feb-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-049T14:59:00,000T15:44:17,18-Feb-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-049T14:59:00,000T13:44:17,18-Feb-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-049T14:59:00,001T16:45:00,18-Feb-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_161_T82",,,,,, 2012-049T14:59:00,001T11:01:00,18-Feb-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-049T15:54:00,000T04:49:17,18-Feb-12,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s. Template A4: No ISS dwells.,,,,,, 2012-049T15:54:00,000T04:49:17,18-Feb-12,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-049T15:54:00,000T04:49:17,18-Feb-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS. Phase = 117 deg. SSC Lat/Lon = 0.617S/137.639 deg, SS Lat/Lon = 13.197N/255.349 deg. Alt = 339151.9 km, range =341726.9 km. Resolution = 170 km/px. Temp. M4. Obtain cubes of Titan for global mapping.",,,,,, 2012-049T20:43:17,000T02:00:00,18-Feb-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-049T20:43:17,000T02:00:00,18-Feb-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-049T20:43:17,000T02:00:00,18-Feb-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS. Phase = 118 deg. SSC Lat/Lon = 0.565S/140.626 deg, SS Lat/Lon = 13.199N/258.951 deg. Alt = 260248.5 km, range =262823.5 km. Resolution = 130 km/px. Temp. N. Obtain cubes of Titan for global mapping.",,,,,, 2012-049T20:43:17,000T11:00:00,18-Feb-12,INMS,Non-SPASS,Saturn,T82INBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-049T20:43:17,000T02:00:00,18-Feb-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-049T22:43:17,000T01:00:00,18-Feb-12,ISS,Prime,Titan,MONITORNA,Monitoring of surface and atmosphere,LRM (Long Range Monitoring),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-049T22:43:17,000T01:00:00,18-Feb-12,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride along with VIMS.,,,,,, 2012-049T22:43:17,000T01:00:00,18-Feb-12,VIMS,,Titan,PHOTOMWAC,Photometry map,Stare at Titan.,"VIMS ridealong with ISS. Phase = 118 deg. SSC Lat/Lon = 0.494S/142.839 deg, SS Lat/Lon = 13.200N/261.770 deg. Alt = 199145.7 km, range =201720.7 km. Resolution = 100 km/px. Temp. N. Obtain cubes of Titan for global mapping.",,,,,, 2012-049T23:43:17,000T04:00:00,18-Feb-12,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2012-049T23:43:17,000T04:00:00,18-Feb-12,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-049T23:43:17,000T04:00:00,18-Feb-12,UVIS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,UVIS Rider to CIRS MIRLMBINT,UVIS Rider to CIRS Mid IR Limb INT,,,,,, 2012-049T23:43:17,000T04:00:00,18-Feb-12,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan Limb Mapping.,"VIMS ridealong with CIRS for limb mapping. Phase = 118 deg. SSC Lat/Lon = 0.459S/143.522 deg, SS Lat/Lon = 13.200N/262.709 deg. Alt = 178888.9 km, range =181463.9 km. Resolution = 89 km/px. Temp. R. Obtain cubes of Titan's limb.",,,,,, 2012-050T00:00:00,000T01:08:00,19-Feb-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-050T03:43:17,000T02:45:00,19-Feb-12,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2012-050T03:43:17,000T02:45:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T03:43:17,000T02:45:00,19-Feb-12,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 120 deg. SSC Lat/Lon = 0.177S/145.485 deg, SS Lat/Lon = 13.201N/266.467 deg. Alt = 98320.3 km, range =100895.3 km. Resolution = 49 km/px. Temp. T. Obtain cubes while scanning across Titan.",,,,,, 2012-050T04:43:17,000T08:00:00,19-Feb-12,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T82 flyby,"T82 is a dusk sector equatorial flyby across Titan's magnetic tail. Similar in geometry, but at a lower altitude (3844 km) than T78, Cassini will be able to provide a better characterization of the magnetotail by providing samples at different radial distances from the moon at a fixed local time. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2012-050T06:28:17,000T01:00:00,19-Feb-12,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2012-050T06:28:17,000T01:00:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T06:28:17,000T01:00:00,19-Feb-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,"VIMS ridealong with CIRS during C/A. At C/A, Phase = 142.6 deg. SSC Lat/Lon = 9.779N/61.442 deg, SS Lat/Lon = 13.203N/271.164 deg. Alt = 3803.3 km, range = 6378.3 km. Resolution = 1.9 km/px. Obtain mosaics and cubes of Titan during C/A.",,,,,, 2012-050T06:28:17,000T01:00:00,19-Feb-12,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2012-050T06:43:17,000T01:00:00,19-Feb-12,CAPS,SPASS Rider,Titan,T82INBND,,Inbound 161TI (T82),null,,,,,, 2012-050T06:43:17,000T01:00:00,19-Feb-12,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-050T06:43:17,000T01:00:00,19-Feb-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-050T07:28:17,000T00:30:00,19-Feb-12,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2012-050T07:28:17,000T00:30:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T07:28:17,000T00:30:00,19-Feb-12,UVIS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,Rider to CIRS,Rider to CIRS.,,,,,, 2012-050T07:28:17,000T00:30:00,19-Feb-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,"VIMS ridealong with CIRS during C/A. At C/A, Phase = 142.6 deg. SSC Lat/Lon = 9.779N/61.442 deg, SS Lat/Lon = 13.203N/271.164 deg. Alt = 3803.3 km, range = 6378.3 km. Resolution = 1.9 km/px. Obtain mosaics and cubes of Titan during C/A.",,,,,, 2012-050T07:43:17,000T02:00:00,19-Feb-12,CAPS,SPASS Rider,Titan,T82CLOSE,,Closest Approach 161TI (T82),null,,,,,, 2012-050T07:43:17,000T02:00:00,19-Feb-12,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-050T07:43:17,000T02:00:00,19-Feb-12,INMS,Non-SPASS,Titan,TITAN82,,Titan Flyby,Titan observation,,,,,, 2012-050T07:43:17,000T02:00:00,19-Feb-12,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2012-050T07:58:17,000T00:45:00,19-Feb-12,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2012-050T07:58:17,000T00:45:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T07:58:17,000T00:45:00,19-Feb-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,"VIMS ridealong with CIRS during C/A. At C/A, Phase = 142.6 deg. SSC Lat/Lon = 9.779N/61.442 deg, SS Lat/Lon = 13.203N/271.164 deg. Alt = 3803.3 km, range = 6378.3 km. Resolution = 1.9 km/px. Obtain mosaics and cubes of Titan during C/A.",,,,,, 2012-050T07:58:17,000T00:45:00,19-Feb-12,UVIS,Non-SPASS,Titan,FIRLMBT,Far Infrared limb tracking,Rider to CIRS,Rider to CIRS.,,,,,, 2012-050T08:43:17,000T00:45:00,19-Feb-12,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2012-050T08:43:17,000T00:45:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T08:43:17,000T00:45:00,19-Feb-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,"VIMS ridealong with CIRS during C/A. At C/A, Phase = 142.6 deg. SSC Lat/Lon = 9.779N/61.442 deg, SS Lat/Lon = 13.203N/271.164 deg. Alt = 3803.3 km, range = 6378.3 km. Resolution = 1.9 km/px. Obtain mosaics and cubes of Titan during C/A.",,,,,, 2012-050T08:43:17,000T00:45:00,19-Feb-12,UVIS,Non-SPASS,Titan,FIRLMBT,Far Infrared limb tracking,Rider to CIRS,Rider to CIRS.,,,,,, 2012-050T09:28:17,000T00:30:00,19-Feb-12,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2012-050T09:28:17,000T00:30:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T09:28:17,000T00:30:00,19-Feb-12,UVIS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,Rider to CIRS,Rider to CIRS.,,,,,, 2012-050T09:28:17,000T00:30:00,19-Feb-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,"VIMS ridealong with CIRS during C/A. At C/A, Phase = 142.6 deg. SSC Lat/Lon = 9.779N/61.442 deg, SS Lat/Lon = 13.203N/271.164 deg. Alt = 3803.3 km, range = 6378.3 km. Resolution = 1.9 km/px. Obtain mosaics and cubes of Titan during C/A.",,,,,, 2012-050T09:43:17,000T01:00:00,19-Feb-12,CAPS,SPASS Rider,Titan,T82OUTBND,,Outbound 161TI (T82),null,,,,,, 2012-050T09:43:17,000T01:00:00,19-Feb-12,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-050T09:43:17,000T11:00:00,19-Feb-12,INMS,Non-SPASS,Saturn,T82OUTBND,,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-050T09:43:17,000T01:00:00,19-Feb-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-050T09:58:17,000T01:00:00,19-Feb-12,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2012-050T09:58:17,000T01:00:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T09:58:17,000T01:00:00,19-Feb-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional mapping.,"VIMS ridealong with CIRS during C/A. At C/A, Phase = 142.6 deg. SSC Lat/Lon = 9.779N/61.442 deg, SS Lat/Lon = 13.203N/271.164 deg. Alt = 3803.3 km, range = 6378.3 km. Resolution = 1.9 km/px. Obtain mosaics and cubes of Titan during C/A.",,,,,, 2012-050T09:58:17,000T01:00:00,19-Feb-12,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider to CIRS,Rider to CIRS.,,,,,, 2012-050T10:43:17,000T21:00:43,19-Feb-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-050T10:58:17,000T02:45:00,19-Feb-12,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2012-050T10:58:17,000T02:45:00,19-Feb-12,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T10:58:17,000T02:45:00,19-Feb-12,VIMS,,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 66 deg. SSC Lat/Lon = 1.376N/339.233 deg, SS Lat/Lon = 13.204N/273.278 deg. Alt = 43334.3 km, range = 45909.3 km. Resolution = 22 km/px. Temp. E. Obtain cubes while scanning across Titan.",,,,,, 2012-050T12:43:17,000T19:00:43,19-Feb-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-050T13:43:17,000T04:00:00,19-Feb-12,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2012-050T13:43:17,000T04:00:00,19-Feb-12,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T13:43:17,000T04:00:00,19-Feb-12,UVIS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,UVIS Rider to CIRS MIRLMBMAP,UVIS Rider to CIRS Mid IR Limb observation,,,,,, 2012-050T13:43:17,000T04:00:00,19-Feb-12,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Titan Limb Mapping.,"VIMS ridealong with CIRS for limb mapping. Phase = 62 deg. SSC Lat/Lon = 0.607N/337.399 deg, SS Lat/Lon = 13.205N/275.861 deg. Alt = 98394.0 km, range = 100969.0 km. Resolution = 49 km/px. Temp. F. Obtain cubes of Titan's limb.",,,,,, 2012-050T17:43:17,000T02:05:43,19-Feb-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-050T17:43:17,000T02:05:43,19-Feb-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-050T17:43:17,000T02:05:43,19-Feb-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS. Phase = 61 deg. SSC Lat/Lon = 0.320N/339.664 deg, SS Lat/Lon = 13.206N/279.618 deg. Alt = 179309.9 km, range = 181884.9 km. Resolution = 90 km/px. Temp. C modified. Obtain cubes of Titan for global mapping.",,,,,, 2012-050T17:43:17,000T02:05:43,19-Feb-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-050T20:43:17,000T04:53:20,19-Feb-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-050T22:14:00,000T09:00:00,19-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-050T23:14:00,000T08:30:00,19-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12050_SP,rider,,,,,, 2012-051T01:36:37,000T06:07:23,20-Feb-12,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-051T02:00:00,000T05:44:00,20-Feb-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-051T04:38:57,002T01:28:00,20-Feb-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.988945 Rs exit= 13.992453 Range altitude= 5856.1711 km ... 1564.9085,,,,,, 2012-051T07:44:00,000T21:36:00,20-Feb-12,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2012-051T07:44:00,000T16:52:37,20-Feb-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-051T07:44:00,000T17:46:00,20-Feb-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-051T07:44:00,001T04:30:00,20-Feb-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_161_162",,,,,, 2012-051T07:44:00,002T01:02:00,20-Feb-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-051T08:35:00,000T09:10:00,20-Feb-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2012-051T08:35:00,000T09:10:00,20-Feb-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,"Range=12.5 to 8 Rs, phase=114-134",,,,,, 2012-051T08:35:00,000T09:10:00,20-Feb-12,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC aurora stare,CL1 NAC 4x4 images. 10 Mbits/hr,,,,,, 2012-051T17:45:00,000T07:50:00,20-Feb-12,ISS,Prime,Enceladus,PLMHPMR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2012-051T17:45:00,000T07:50:00,20-Feb-12,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2012-051T18:00:00,001T00:00:00,20-Feb-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-052T00:36:00,000T02:00:00,21-Feb-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-052T00:36:37,000T00:58:23,21-Feb-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-052T00:37:57,000T02:00:00,21-Feb-12,CDA,SPASS Rider,DustRAM direction,RPX0340,,CDA RPXing 2012-052T01:37:57,RPXing at 4.2853048 Rs,,,,,, 2012-052T01:30:00,000T07:50:00,21-Feb-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-052T01:35:00,000T02:02:00,21-Feb-12,INMS,Prime,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-052T03:37:00,000T03:44:00,21-Feb-12,VIMS,Prime,Saturn,ALPCMAOCC,,alpCMa Saturn occultation,"alpCMa atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. After the occ, at time 05:57, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation occurred (latitude 49.9S).",,,,,, 2012-052T03:37:00,000T03:44:00,21-Feb-12,CIRS,,Saturn,ALPCMAOCC,,CIRS_161SA_ALPCMAOCC001_VIMS,PIE Collaboration with VIMS. Stellar Occ Saturn ingress T05:36 50S dark limb at T05:57 go to limb for CIRS integration,,,,,, 2012-052T03:37:00,000T21:59:37,21-Feb-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-052T05:20:00,001T06:40:00,21-Feb-12,CAPS,SPASS Rider,Saturn,EQINMAG,,MAPS equatorial inner magnetosphere,null,,,,,, 2012-052T05:22:34,000T00:00:01,21-Feb-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.231 Rs, lat = -0 deg, phase = 117 deg",,,,,, 2012-052T07:21:00,000T02:43:00,21-Feb-12,VIMS,Prime,Saturn,ALPHYAOCC,,alpHya Saturn occultation,"alpHya atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. After the occ, at time 08:11, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation occurred (latitude 41.3S).",,,,,, 2012-052T07:21:00,000T02:43:00,21-Feb-12,CIRS,,Saturn,ALPHYAOCC,,CIRS_161SA_ALPHYAOCC001_VIMS,Collaboration with VIMS. Stellar Occ Saturn ingress T07:50 41S dark limb at T08:11 go to limb for CIRS integration,,,,,, 2012-052T09:20:00,001T21:54:00,21-Feb-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-052T12:14:00,008T15:37:00,21-Feb-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_161_162",,,,,, 2012-052T12:14:00,000T09:00:00,21-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-052T13:14:00,000T08:00:00,21-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12052_SP,rider,,,,,, 2012-052T19:25:00,000T02:00:00,21-Feb-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-052T19:25:57,000T02:00:00,21-Feb-12,CDA,SPASS Rider,DustRAM direction,RPX0350,,CDA RPXing 2012-052T20:25:57,RPXing at 9.8949844 Rs,,,,,, 2012-052T21:54:00,000T10:51:00,21-Feb-12,CAPS,Prime,Saturn,EQIMAGPTG,,MAPS equatorial inner magnetosphere,null,,,,,, 2012-053T01:36:37,001T05:37:23,22-Feb-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-053T06:06:57,007T21:44:03,22-Feb-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.005339 Rs exit= 14.001168 Range altitude= 1570.1147 km ... 5853.5762,,,,,, 2012-053T08:45:00,000T12:49:00,22-Feb-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2012-053T08:45:00,000T12:49:00,22-Feb-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,"Range=15-19Rs phase=21, sub s/c lat=0",,,,,, 2012-053T08:45:00,000T12:49:00,22-Feb-12,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Ridealong,Auroral UVIS Ridealong,,,,,, 2012-053T08:46:00,007T19:05:00,22-Feb-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-053T12:00:00,015T08:01:00,22-Feb-12,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2012-053T22:14:00,000T09:00:00,22-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-053T23:14:00,000T08:00:00,22-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12053_SP,rider,,,,,, 2012-054T07:14:00,000T23:45:00,23-Feb-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-054T07:14:00,009T02:31:00,23-Feb-12,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2012-054T07:54:00,000T13:25:00,23-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-054T21:59:00,000T09:00:00,23-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-054T22:59:00,000T08:00:00,23-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12054_SP,rider,,,,,, 2012-055T06:59:00,000T00:40:00,24-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-055T06:59:00,005T20:52:00,24-Feb-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-055T07:37:00,000T00:02:00,24-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-055T07:39:00,000T01:30:00,24-Feb-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 33.9 requested range 2.9 Mkm",,,,,, 2012-055T07:39:00,000T01:30:00,24-Feb-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-055T07:39:00,000T01:30:00,24-Feb-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 34 deg, range =2.9 Mkm. Also Stormwatch cube",,,,,, 2012-055T09:07:00,000T00:02:00,24-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-055T09:09:00,000T10:35:00,24-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-055T09:09:00,000T10:35:00,24-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-055T19:42:00,000T00:02:00,24-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-055T21:14:00,000T22:36:00,24-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-055T21:14:00,000T22:36:00,24-Feb-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-056T19:48:00,000T00:02:00,25-Feb-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-056T22:00:00,000T09:00:00,25-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-056T23:00:00,000T08:00:00,25-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12056_SP,rider,,,,,, 2012-057T07:00:00,000T21:00:00,26-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-058T03:51:00,000T20:00:00,27-Feb-12,CDA,SPASS Rider,DustRAM direction,ISD0042,,CDA ISD 2012-061T03:51:00,ISD observation around apoapse 2012-061T03:51:00 40.505944 Rs,,,,,, 2012-058T05:30:00,000T09:00:00,27-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-058T06:30:00,000T08:00:00,27-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12058_SP,rider,,,,,, 2012-058T14:30:00,001T13:15:00,27-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-059T21:51:00,000T20:00:00,28-Feb-12,CDA,SPASS Rider,DustRAM direction,ISD0042,,CDA ISD 2012-061T03:51:00,ISD observation around apoapse 2012-061T03:51:00 40.505944 Rs,,,,,, 2012-060T05:15:00,000T09:00:00,29-Feb-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-060T06:15:00,000T08:00:00,29-Feb-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_161IC_DSCAL12060_SP,rider,,,,,, 2012-060T14:15:00,000T01:30:00,29-Feb-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 85.1 requested range 2.8 Mkm",,,,,, 2012-060T14:15:00,000T01:30:00,29-Feb-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-060T14:15:00,000T01:30:00,29-Feb-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 85 deg, range =2.8 Mkm.",,,,,, 2012-060T15:45:00,001T12:00:00,29-Feb-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-061T03:51:00,007T21:37:57,1-Mar-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.005339 Rs exit= 14.001168 Range altitude= 1570.1147 km ... 5853.5762,,,,,, 2012-061T03:51:00,000T02:00:00,1-Mar-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-061T03:51:00,007T16:10:00,1-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_161_162",,,,,, 2012-061T03:51:00,007T16:10:00,1-Mar-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-061T03:51:09,000T00:00:01,1-Mar-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.9 d, inc = 0.4 deg, r = 40.464 Rs, phase = 63 deg",,,,,, 2012-061T05:51:00,007T01:49:00,1-Mar-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-061T13:51:00,000T20:00:00,1-Mar-12,CDA,SPASS Rider,DustRAM direction,ISD0042,,CDA ISD 2012-061T03:51:00,ISD observation around apoapse 2012-061T03:51:00 40.505944 Rs,,,,,, 2012-062T05:15:00,000T09:00:00,2-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-062T06:15:00,000T08:00:00,2-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12062_SP,rider,,,,,, 2012-062T14:15:00,000T01:30:00,2-Mar-12,ISS,Prime,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 96.1 requested range 2 Mkm",,,,,, 2012-062T14:15:00,000T01:30:00,2-Mar-12,CIRS,SPASS Rider,Titan,M120R2HZ,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-062T14:15:00,000T01:30:00,2-Mar-12,VIMS,SPASS Rider,Titan,M120R2HZ,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 96 deg, range =2.0 Mkm.",,,,,, 2012-062T15:45:00,000T18:00:00,2-Mar-12,ISS,Prime,Other,THRROT,,Thrymr,Observation of irregular moon of Saturn.,,,,,, 2012-063T07:51:00,000T20:00:00,3-Mar-12,CDA,SPASS Rider,DustRAM direction,ISD0042,,CDA ISD 2012-061T03:51:00,ISD observation around apoapse 2012-061T03:51:00 40.505944 Rs,,,,,, 2012-063T09:45:00,000T07:00:00,3-Mar-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-063T16:45:00,000T10:45:00,3-Mar-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-063T16:45:00,004T21:01:00,3-Mar-12,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2012-064T03:30:00,000T06:00:00,4-Mar-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-064T05:00:00,000T09:00:00,4-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-064T06:00:00,000T08:00:00,4-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12064_SP,rider,,,,,, 2012-064T14:00:00,000T22:00:00,4-Mar-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-065T00:00:00,000T01:08:00,5-Mar-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-065T12:00:00,000T04:00:00,5-Mar-12,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2012-065T12:00:00,000T04:00:00,5-Mar-12,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2012-065T16:00:00,000T11:16:00,5-Mar-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2012-065T16:00:00,000T11:16:00,5-Mar-12,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC aurora stare,CL1 NAC 4x4 images. 10 Mbits/hr,,,,,, 2012-066T04:46:00,000T09:00:00,6-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-066T05:46:00,000T08:00:00,6-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12066_SP,rider,,,,,, 2012-066T13:46:00,000T11:15:00,6-Mar-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2012-066T13:46:00,000T11:15:00,6-Mar-12,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC aurora stare,CL1 NAC 4x4 images. 10 Mbits/hr,,,,,, 2012-067T01:01:00,000T02:15:00,7-Mar-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-067T04:46:00,000T09:00:00,7-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-067T05:46:00,000T08:00:00,7-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12067_SP,rider,,,,,, 2012-067T13:46:00,000T11:15:00,7-Mar-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Fixed pointing at the auroral oval,,,,,, 2012-067T13:46:00,000T11:15:00,7-Mar-12,ISS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,NAC aurora stare,CL1 NAC 4x4 images. 10 Mbits/hr,,,,,, 2012-068T01:01:00,000T08:30:00,8-Mar-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-068T07:40:00,000T02:00:00,8-Mar-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-068T09:40:00,000T10:21:00,8-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-068T12:01:00,000T08:00:00,8-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12068_SP,rider,,,,,, 2012-068T13:46:00,000T06:15:00,8-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-068T20:01:00,002T10:00:00,8-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-068T20:01:00,000T02:23:08,8-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-068T20:01:00,001T02:19:00,8-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-068T20:01:00,002T10:00:00,8-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_162",,,,,, 2012-068T20:01:00,002T10:00:00,8-Mar-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-068T20:41:00,000T09:35:00,8-Mar-12,ISS,Prime,Other,JARROT,,Jarnsaxa,Observation of irregular moon of Saturn.,,,,,, 2012-068T20:41:00,000T09:35:00,8-Mar-12,VIMS,SPASS Rider,Other,JARROT,,UVIS_FUV to Rocks,UVIS_FUV to Rocks,,,,,, 2012-068T22:24:08,000T23:00:00,8-Mar-12,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-069T01:28:57,000T02:30:00,9-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.988282 Rs exit= 13.999801 Range altitude= 5846.8374 km ... 1591.6608,,,,,, 2012-069T03:58:57,001T23:02:00,9-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.988282 Rs exit= 13.999801 Range altitude= 5846.8374 km ... 1591.6608,,,,,, 2012-069T06:16:00,000T09:35:00,9-Mar-12,ISS,Prime,Other,MUNROT,,Mundilfari,Observation of irregular moon of Saturn.,,,,,, 2012-069T06:16:00,000T09:35:00,9-Mar-12,VIMS,SPASS Rider,Other,MUNROT,,UVIS_FUV to Rocks,UVIS_FUV to Rocks,,,,,, 2012-069T15:51:00,000T02:00:00,9-Mar-12,ISS,Prime,Titan,M30R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 23.1 requested range 0.9 Mkm",,,,,, 2012-069T15:51:00,000T02:00:00,9-Mar-12,CIRS,SPASS Rider,Titan,M30R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-069T18:00:00,000T03:42:00,9-Mar-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-069T21:24:08,000T00:30:00,9-Mar-12,INMS,Non-SPASS,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-069T21:25:57,000T02:00:00,9-Mar-12,CDA,SPASS Rider,DustRAM direction,RPX0360,,CDA RPXing 2012-069T22:25:57,RPXing at 4.3139193 Rs,,,,,, 2012-069T21:42:00,000T02:00:00,9-Mar-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-069T21:54:08,000T01:30:00,9-Mar-12,INMS,SPASS Rider,Saturn,RINGPLND,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-069T22:01:00,000T08:00:00,9-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12069_SP,rider,,,,,, 2012-069T22:20:00,000T07:50:00,9-Mar-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-069T23:24:08,000T06:36:52,9-Mar-12,INMS,Non-SPASS,Saturn,SURVEYRPD,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-069T23:42:00,000T12:18:00,9-Mar-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-070T02:13:20,000T00:00:01,10-Mar-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.245 Rs, lat = -0 deg, phase = 117 deg",,,,,, 2012-070T06:01:00,000T16:23:08,10-Mar-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-070T06:10:00,000T23:51:00,10-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-070T06:35:00,000T01:40:00,10-Mar-12,ISS,Prime,Enceladus,ENCEL,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2012-070T06:35:00,000T01:40:00,10-Mar-12,CIRS,,Enceladus,ENCEL,Enceladus,,null,,,,,, 2012-070T06:35:00,000T01:40:00,10-Mar-12,UVIS,,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-070T06:35:00,000T01:40:00,10-Mar-12,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,ISS_NAC to Enceladus,ISS_NAC to Enceladus,,,,,, 2012-070T08:15:00,000T01:30:00,10-Mar-12,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 16.4 requested range 1.4 Mkm",,,,,, 2012-070T08:15:00,000T01:30:00,10-Mar-12,CIRS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-070T08:15:00,000T01:30:00,10-Mar-12,VIMS,SPASS Rider,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 16 deg, range =1.4 Mkm.",,,,,, 2012-070T10:25:00,000T04:35:00,10-Mar-12,CIRS,Prime,Rhea,RHEA,Rhea,,10:50 - 10:55 Turn 10:55 - 11:40 FP1 raster scans @ nyquist sampling (probably time for 5 full scans) 11:40 - 12:00 Quiescent Period 12:00 - 12:15 Single FP1 raster scan @ nyquist sampling 12:15 - 13:00 Single FP3 swath along lit crescent @ 6 mu rad/s 13:00 - 13:20 Single FP1 raster scan @ nyquist sampling 13:20 - 14:55 Two FP3 swarchs along (now fatter) sun lit cresecent @ 6 mu rad/s 14:55 - 15:00 Turn,,,,,, 2012-070T10:25:00,000T04:35:00,10-Mar-12,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-070T10:25:00,000T04:35:00,10-Mar-12,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-070T10:25:00,000T04:35:00,10-Mar-12,VIMS,SPASS Rider,Rhea,RHEA,Rhea,CIRS Rhea,CIRS Rhea,,,,,, 2012-070T15:00:00,000T01:30:00,10-Mar-12,ISS,Prime,Rhea,REGMAP,Regional mapping,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-070T15:00:00,000T01:30:00,10-Mar-12,CIRS,SPASS Rider,Rhea,REGMAP,Regional mapping,,null,,,,,, 2012-070T15:00:00,000T01:30:00,10-Mar-12,UVIS,,Rhea,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Rhea, ORS Rider",UV albedo map of Rhea's surface plus limb drifts,,,,,, 2012-070T15:00:00,000T01:30:00,10-Mar-12,VIMS,SPASS Rider,Rhea,REGMAP,Regional mapping,ISS_NAC to Rhea,ISS_NAC to Rhea,,,,,, 2012-070T16:13:57,000T02:00:00,10-Mar-12,CDA,SPASS Rider,DustRAM direction,RPX0370,,CDA RPXing 2012-070T17:13:57,RPXing at 9.8652064 Rs,,,,,, 2012-070T16:30:00,000T01:50:00,10-Mar-12,ISS,Prime,Rhea,RHEARINGS,,Rhea ring search,Sit'n'stare over one ansa,,,,,, 2012-070T16:30:00,000T01:50:00,10-Mar-12,CIRS,SPASS Rider,Rhea,RHEARINGS,,,null,,,,,, 2012-070T16:30:00,000T01:50:00,10-Mar-12,UVIS,SPASS Rider,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-070T16:30:00,000T01:50:00,10-Mar-12,VIMS,SPASS Rider,Rhea,RHEARINGS,,ISS_NAC to Rhea,ISS_NAC to Rhea,,,,,, 2012-070T18:51:00,000T08:00:00,10-Mar-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-070T21:01:00,000T09:00:00,10-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-070T22:01:00,000T08:00:00,10-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12070_SP,rider,,,,,, 2012-070T22:24:08,000T07:36:52,10-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-071T03:00:57,007T20:53:03,11-Mar-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.012661 Rs exit= 14.004410 Range altitude= 1596.8968 km ... 5854.2896,,,,,, 2012-071T06:01:00,015T12:46:00,11-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-071T06:01:00,004T23:45:00,11-Mar-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-071T06:01:00,002T10:40:00,11-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-071T06:01:00,007T17:54:00,11-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_162_163",,,,,, 2012-071T06:01:00,007T17:54:00,11-Mar-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-071T06:58:00,000T00:02:00,11-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-071T07:00:00,000T03:00:00,11-Mar-12,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2012-071T07:00:00,000T03:00:00,11-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-071T09:58:00,000T00:02:00,11-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-071T10:00:00,000T12:00:00,11-Mar-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-071T10:00:00,000T12:00:00,11-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-071T21:58:00,000T00:02:00,11-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-071T22:00:00,000T01:30:00,11-Mar-12,ISS,Prime,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 23.4 requested range 2.1 Mkm",,,,,, 2012-071T22:00:00,000T01:30:00,11-Mar-12,CIRS,SPASS Rider,Titan,M30R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-071T22:00:00,000T01:30:00,11-Mar-12,VIMS,SPASS Rider,Titan,M30R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 23 deg, range =2.1 Mkm.",,,,,, 2012-071T23:28:00,000T00:02:00,11-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-071T23:30:00,000T01:30:00,11-Mar-12,ISS,Prime,Enceladus,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Enceladus across Titan","Images of mutual event, transit of Enceladus across Titan for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2012-071T23:30:00,000T01:30:00,11-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-072T00:58:00,000T00:02:00,12-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-072T01:00:00,000T01:00:00,12-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-072T01:00:00,000T01:00:00,12-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-072T01:58:00,000T00:02:00,12-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-072T04:31:00,000T09:00:00,12-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-072T05:31:00,000T08:00:00,12-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12072_SP,rider,,,,,, 2012-072T13:31:00,000T13:30:00,12-Mar-12,CDA,Prime,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - outbound leg - Peri->Apo transition,,,,,, 2012-073T04:31:00,000T09:00:00,13-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-073T05:31:00,000T08:00:00,13-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12073_SP,rider,,,,,, 2012-073T14:09:00,000T00:02:00,13-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-073T14:11:00,000T01:30:00,13-Mar-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 55.1 requested range 2.9 Mkm",,,,,, 2012-073T14:11:00,000T01:30:00,13-Mar-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-073T14:11:00,000T01:30:00,13-Mar-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 56 deg, range =2.9 Mkm. Also Stormatch Cube",,,,,, 2012-073T15:39:00,000T00:02:00,13-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-073T15:41:00,000T01:00:00,13-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-073T15:41:00,000T01:00:00,13-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-073T16:39:00,000T00:02:00,13-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-073T16:41:00,000T08:00:00,13-Mar-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-073T16:41:00,000T08:00:00,13-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-074T00:39:00,000T00:02:00,14-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-074T00:41:00,000T01:49:00,14-Mar-12,ISS,Prime,Tethys,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Tethys across Dione","Images of mutual event, transit of Tethys across Dione for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2012-074T00:41:00,000T01:49:00,14-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-074T00:41:00,004T14:21:00,14-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-074T02:28:00,000T00:02:00,14-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-074T10:46:00,000T09:00:00,14-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-074T11:46:00,000T08:00:00,14-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12074_SP,rider,,,,,, 2012-074T20:14:00,000T00:02:00,14-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-074T20:16:00,000T23:00:00,14-Mar-12,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2012-074T20:16:00,000T23:00:00,14-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-075T19:14:00,000T00:02:00,15-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-075T19:16:00,000T01:00:00,15-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-075T19:16:00,000T01:00:00,15-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-075T20:14:00,000T00:02:00,15-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-075T20:46:00,000T09:00:00,15-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-075T21:46:00,000T08:00:00,15-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12075_SP,rider,,,,,, 2012-076T05:46:00,000T14:45:00,16-Mar-12,CDA,Prime,DustRAM direction,ISD0043,,CDA ISD 2012-078T23:54:00,ISD observation around apoapse 2012-078T23:54:00 40.386116 Rs,,,,,, 2012-076T05:46:00,000T23:45:00,16-Mar-12,INMS,Non-SPASS,Saturn,SURVPOTMA,,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-076T20:31:00,000T09:00:00,16-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-076T21:31:00,000T08:00:00,16-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12076_SP,rider,,,,,, 2012-076T23:30:00,002T00:00:00,16-Mar-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - Apo leg,,,,,, 2012-077T05:31:00,001T18:24:00,17-Mar-12,INMS,Non-SPASS,Saturn,SURVBOTMA,,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-077T05:58:00,000T00:02:00,17-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-077T06:00:00,000T01:00:00,17-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-077T06:00:00,000T01:00:00,17-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-077T06:58:00,000T00:02:00,17-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-077T07:00:00,001T08:00:00,17-Mar-12,UVIS,Prime,Saturn,MOS162APO,,,"Mosaic scan of Saturn magnetosphere, day 1. One 32.0-hr block of time assumed. EUV and FUV low resolution slits on. Align slit with Saturn spin axis. Waypoint is assumed to be Saturn center. Allowances have been made for 0) 20 minutes observation margin at start and end; and 1) 30 minutes for turn back to waypoint at end. Note: data to be taken only when slit is stationary. 1) Start at Saturn center. Slew +32 mrad about x-axis and -100 mrad about z-axis. Start data capture, stare 367.0 s, stop data capture. 2) Repeat PATTERN A 132 times. 3) Slew +64 mrad about x-axis. Start data capture, stare 367.0 s, stop data capture. 4) Repeat PATTERN B 132 times. 5) Turn back to waypoint. PATTERN A: Slew +1.5 mrad about z-axis. Start data capture, stare 367.0 s, stop data capture. PATTERN B: Slew -1.5 mrad about z-axis. Start data capture, stare 367.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (3299.20576 bps, from Alain's spreadsheet)x(367.0s per stare)x(266 stares)x(data packet filling factor of 1.01) = 325.296x10^6 bits",,,,,, 2012-077T07:00:00,001T08:00:00,17-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-077T17:54:00,000T20:00:00,17-Mar-12,CDA,SPASS Rider,DustRAM direction,ISD0043,,CDA ISD 2012-078T23:54:00,ISD observation around apoapse 2012-078T23:54:00 40.386116 Rs,,,,,, 2012-078T14:58:00,000T00:02:00,18-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-078T15:02:00,000T05:00:00,18-Mar-12,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2012-078T20:02:00,007T22:45:00,18-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-078T20:32:00,000T09:00:00,18-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-078T21:32:00,000T08:00:00,18-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_162IC_DSCAL12078_SP,rider,,,,,, 2012-078T23:54:00,007T20:50:57,18-Mar-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.012661 Rs exit= 14.004410 Range altitude= 1596.8968 km ... 5854.2896,,,,,, 2012-078T23:54:47,000T00:00:01,18-Mar-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.8 d, inc = 0.4 deg, r = 40.349 Rs, phase = 62 deg",,,,,, 2012-078T23:55:00,000T02:00:00,18-Mar-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-078T23:55:00,007T18:52:00,18-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_162_163",,,,,, 2012-078T23:55:00,007T18:52:00,18-Mar-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-079T01:00:00,002T00:00:00,19-Mar-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - Apo leg,,,,,, 2012-079T01:55:00,005T17:07:00,19-Mar-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-079T05:58:00,000T00:02:00,19-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-079T06:00:00,000T16:00:00,19-Mar-12,UVIS,Prime,Saturn,MOS162APO,,,"Mosaic scan of Saturn magnetosphere, day 2. One 16.0-hr block of time assumed. EUV and FUV low resolution slits on. Align slit with Saturn spin axis. Waypoint is assumed to be Saturn center. Allowances have been made for 0) 20 minutes observation margin at start and end; and 1) 30 minutes for turn back to waypoint at end. Note: data to be taken only when slit is stationary. 1) Start at Saturn center. Slew -96 mrad about x-axis and -100 mrad about z-axis. Start data capture, stare 350.0 s, stop data capture. 2) Repeat PATTERN 132 times. 3) Turn back to waypoint. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 350.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (3459.45289 bps, from Alain's spreadsheet)x(350.0s per stare)x(133 stares)x(data packet filling factor of 1.01) = 162.6479x10^6 bits",,,,,, 2012-079T06:00:00,000T16:00:00,19-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-079T21:58:00,000T00:02:00,19-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-079T22:00:00,000T01:00:00,19-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-079T22:00:00,000T01:00:00,19-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-079T22:58:00,000T00:02:00,19-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-080T00:00:00,000T01:08:00,20-Mar-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-080T00:30:00,000T01:30:00,20-Mar-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 88.2 requested range 1.6 Mkm",,,,,, 2012-080T00:30:00,000T01:30:00,20-Mar-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-080T00:30:00,000T01:30:00,20-Mar-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 88 deg, range =1.6 Mkm. Also Stormwatch cube",,,,,, 2012-080T01:58:00,000T00:02:00,20-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-080T04:02:00,000T09:00:00,20-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-080T05:02:00,000T08:00:00,20-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12080_SP,rider,,,,,, 2012-080T13:02:00,000T13:15:00,20-Mar-12,CDA,Prime,DustRAM direction,ISD0043,,CDA ISD 2012-078T23:54:00,ISD observation around apoapse 2012-078T23:54:00 40.386116 Rs,,,,,, 2012-081T01:47:00,000T11:00:00,21-Mar-12,RSS,SPASS Rider,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,"HGA Boresight Calibration. Pointing=XBAND to Earth + crosshair maneuver. Telemetry OFF, TWNC ON for 1-hr calibration from 2012-081T05:47:00 to 2012-081T06:47:00. Required to be tracked by DSS-25 (or DSS-26). Keep Ka-band ON until EOT at 2012-081T06:47:00. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2012-081T03:47:00,000T09:00:00,21-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-081T04:47:00,000T08:00:00,21-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12081_SP,rider,,,,,, 2012-081T05:47:00,000T01:00:00,21-Mar-12,RSS,Prime,Earth,BORESIGHT,HGA boresight calibration,HGA Boresight Calibration,"HGA Boresight Calibration. Pointing=XBAND to Earth + crosshair maneuver. Telemetry OFF, TWNC ON for 1-hr calibration from 2012-081T05:47:00 to 2012-081T06:47:00. Required to be tracked by DSS-25 (or DSS-26). Keep Ka-band ON until EOT at 2012-081T06:47:00. Playback of telemetry required afterwards for C-Kernel generation.",,,,,, 2012-081T13:25:00,000T00:02:00,21-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-081T13:27:00,000T12:10:00,21-Mar-12,ISS,Prime,Other,TITANL4,,Titan L4 satellite search,Satellite search around Titan L4 Lagrange point.,,,,,, 2012-081T13:27:00,000T12:10:00,21-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-082T01:35:00,000T00:02:00,22-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-082T03:47:00,000T09:00:00,22-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-082T04:47:00,000T08:00:00,22-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12082_SP,rider,,,,,, 2012-082T12:47:00,000T13:30:00,22-Mar-12,CDA,Prime,DustRAM direction,ISD0043,,CDA ISD 2012-078T23:54:00,ISD observation around apoapse 2012-078T23:54:00 40.386116 Rs,,,,,, 2012-083T03:47:00,000T09:00:00,23-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-083T04:47:00,000T08:00:00,23-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12083_SP,rider,,,,,, 2012-083T13:28:00,000T00:02:00,23-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-083T13:30:00,000T02:00:00,23-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-083T13:30:00,000T02:00:00,23-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-083T15:28:00,000T00:02:00,23-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-083T15:30:00,000T01:30:00,23-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-083T16:58:00,000T00:02:00,23-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-083T17:00:00,000T16:00:00,23-Mar-12,UVIS,Prime,Saturn,MOS162APO,,,"Mosaic scan of Saturn magnetosphere, day 3. One 16.0-hr block of time assumed. EUV and FUV low resolution slits on. Align slit with Saturn spin axis. Waypoint is assumed to be Saturn center. Allowances have been made for 0) 20 minutes observation margin at start and end; and 1) 30 minutes for turn back to waypoint at end. Note: data to be taken only when slit is stationary. 1) Start at Saturn center. Slew -32 mrad about x-axis and -133 mrad about z-axis. Start data capture, stare 252.0 s, stop data capture. 2) Repeat PATTERN 176 times. 3) Turn back to waypoint. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 252.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (4804.79569 bps, from Alain's spreadsheet)x(252.0s per stare)x(177 stares)x(data packet filling factor of 1.01) = 216.45624x10^6 bits",,,,,, 2012-083T17:00:00,000T16:00:00,23-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-084T08:58:00,000T00:02:00,24-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-084T10:02:00,000T09:00:00,24-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-084T11:02:00,000T08:00:00,24-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12084_SP,rider,,,,,, 2012-084T18:00:00,002T00:00:00,24-Mar-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - inbound leg - Apo->Peri transition,,,,,, 2012-084T19:02:00,000T23:45:00,24-Mar-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-084T19:58:00,000T00:02:00,24-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-084T20:00:00,000T02:00:00,24-Mar-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-084T20:00:00,000T02:00:00,24-Mar-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-084T21:58:00,000T00:02:00,24-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-084T22:00:00,000T11:00:00,24-Mar-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-084T22:00:00,000T11:00:00,24-Mar-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2012-085T08:58:00,000T00:02:00,25-Mar-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-085T09:47:00,000T09:00:00,25-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-085T10:47:00,000T08:00:00,25-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12085_SP,rider,,,,,, 2012-085T18:47:00,000T13:00:00,25-Mar-12,ISS,Prime,rings(general),PHOEBEHOL,,Observation of Saturn's shadow on the Phoebe ring,Stare at edge of Saturn's Shadow on the Phoebe Ring,,,,,, 2012-085T18:47:00,000T08:08:00,25-Mar-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-086T02:55:00,000T02:00:00,26-Mar-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-086T04:55:00,000T13:52:00,26-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-086T09:47:00,000T09:00:00,26-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-086T10:47:00,000T08:00:00,26-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12086_SP,rider,,,,,, 2012-086T18:47:00,000T14:20:00,26-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-086T18:47:00,000T11:43:09,26-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-086T18:47:00,000T21:43:09,26-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-086T18:47:00,002T23:45:00,26-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_163_E17",,,,,, 2012-086T18:47:00,001T15:45:00,26-Mar-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-086T19:27:00,000T01:30:00,26-Mar-12,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 50.4 requested range 1.5 Mkm",,,,,, 2012-086T19:27:00,000T01:30:00,26-Mar-12,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-086T19:27:00,000T01:30:00,26-Mar-12,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 50 deg, range =1.5 Mkm.",,,,,, 2012-086T20:44:57,000T04:55:03,26-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-086T20:57:00,000T04:00:00,26-Mar-12,ISS,Prime,Other,L5TITAN,,Titan L5 satellite search,Satellite search around Titan L5 Lagrange point.,,,,,, 2012-086T20:57:00,000T04:00:00,26-Mar-12,VIMS,SPASS Rider,Other,L5TITAN,,Rock spectra,"ISS NAC to Rocks 160, 640ms IR",,,,,, 2012-087T01:40:00,000T05:00:00,27-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-087T06:30:09,000T10:00:00,27-Mar-12,INMS,Non-SPASS,Enceladus,E17INBND,,Enceladus flyby,Enceladus observation,,,,,, 2012-087T06:40:00,000T03:05:00,27-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-087T09:07:00,000T08:23:09,27-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-087T09:45:00,000T05:10:00,27-Mar-12,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2012-087T09:45:00,000T05:10:00,27-Mar-12,CIRS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,,null,,,,,, 2012-087T09:45:00,000T05:10:00,27-Mar-12,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2012-087T09:45:00,000T05:10:00,27-Mar-12,VIMS,SPASS Rider,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus plume,ISS NAC to Enceladus plume,,,,,, 2012-087T09:45:00,000T03:00:00,27-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-087T12:45:00,000T08:25:00,27-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-087T15:00:09,000T03:00:00,27-Mar-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-087T15:05:00,000T02:25:00,27-Mar-12,CIRS,Prime,Enceladus,ENCEL,Enceladus,,"Shutter closed details: This observation starts with FP3 maps, so we need to perform irregularly timed shutter closed observations. Shutter closed times: 15:05:00 - 15:07:00 (which will lose 1 min of 1st FP3 map, but since we're on approach this is at lowest spatial and we'll get a complete map in the following scan) 17:10:00 - 17:14:00 (during FP1 scan). Shutter closed specs: Wavenumber resolution: 15.67 cm-1, NoAdd, blink mode, data to be obtained for all focal planes. Observation detail from Port 1 SFOF 15:05 - 15:06 Turn 15:06 - 16:20 Global FP3 scan (taking ~ 2 to 3 swaths) @ 6 mu rad/s 16:20 - 16:54 Global FP3 scan of the SPT 16:54 - 17:10 FP3 scan of SPT @ limb @ 6 mu rad/s of SPT, up to ~ 50 S 17:11 - 17:28 FP1 raster scan 17:28 - 17:30 Turn",,,,,, 2012-087T15:05:00,000T02:25:00,27-Mar-12,VIMS,SPASS Rider,Enceladus,ENCEL,Enceladus,Enceladus,Enceladus,,,,,, 2012-087T16:30:09,000T00:59:51,27-Mar-12,INMS,Non-SPASS,Enceladus,ENCEL17,,Enceladus encounter,Enceladus observation,,,,,, 2012-087T16:30:09,000T04:00:00,27-Mar-12,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2012-087T16:41:57,000T02:00:00,27-Mar-12,CDA,SPASS Rider,DustRAM direction,RPX0380,,CDA RPXing 2012-087T17:41:57,RPXing at 4.3344952 Rs,,,,,, 2012-087T17:30:00,000T02:00:00,27-Mar-12,INMS,Prime,Enceladus,ENCEL17,,Enceladus encounter,Enceladus observation,,,,,, 2012-087T17:30:00,000T02:00:00,27-Mar-12,CIRS,SPASS Rider,Enceladus,ENCEL17,,,null,,,,,, 2012-087T17:30:09,000T02:00:00,27-Mar-12,CAPS,SPASS Rider,Titan,EN17CLOSE,,Closest Approach 163EN (17),null,,,,,, 2012-087T18:00:09,000T01:00:00,27-Mar-12,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 163,BIT_OVERLAY_950,,,,,, 2012-087T18:00:09,000T01:00:00,27-Mar-12,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2012-087T19:30:00,000T01:30:00,27-Mar-12,ISS,Prime,Enceladus,ENCELADUS,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2012-087T19:30:00,000T01:30:00,27-Mar-12,CIRS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,,null,,,,,, 2012-087T19:30:00,000T01:30:00,27-Mar-12,UVIS,,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus's surface plus limb drifts,,,,,, 2012-087T19:30:00,000T01:30:00,27-Mar-12,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus 20 deg phase,ISS NAC to Enceladus,,,,,, 2012-087T19:30:00,000T01:00:09,27-Mar-12,INMS,Non-SPASS,Enceladus,ENCEL17,,Enceladus encounter,Enceladus observation,,,,,, 2012-087T19:30:09,000T15:01:51,27-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-087T20:30:09,000T10:00:00,27-Mar-12,INMS,Non-SPASS,Enceladus,E17OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2012-087T20:30:09,000T04:59:51,27-Mar-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-087T21:10:00,000T03:40:00,27-Mar-12,ISS,Prime,Janus,JANUS,Janus,Janus ORS observation,ORS observation,,,,,, 2012-087T21:10:00,000T03:40:00,27-Mar-12,CIRS,SPASS Rider,Janus,JANUS,Janus,,null,,,,,, 2012-087T21:10:00,000T03:40:00,27-Mar-12,VIMS,SPASS Rider,Janus,JANUS,Janus,Janus,ISS NAC to Janus,,,,,, 2012-087T21:10:00,000T00:15:00,27-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-087T21:10:00,000T04:20:00,27-Mar-12,RADAR,Non-SPASS,Other,WU4DISCAT,,Warm Up for Rev 163 Dione.,Warmup for scatterometry/radiometry of Dione in rev 163.,,,,,, 2012-087T21:11:20,000T00:00:01,27-Mar-12,RADAR,Non-SPASS,NotApplicable,PINPONDIS,,Disable SSR PingPong for RADAR FSW Load,The RADAR FSW load time is exact. Disable ping-pong commands are inserted around this time.,,,,,, 2012-087T21:25:00,000T04:05:00,27-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-087T21:31:39,000T00:00:01,27-Mar-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.253 Rs, lat = -0 deg, phase = 118 deg",,,,,, 2012-088T01:30:00,000T02:50:00,28-Mar-12,RADAR,Prime,Dione,SCATTRAD,RADAR Scatterometry / Radiometry,Rev163 Dione SCATT/RAD,Scatterometry/Radiometry of Dione in Rev 163.,,,,,, 2012-088T01:30:00,000T03:00:00,28-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-088T01:30:00,001T17:02:00,28-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-088T04:30:00,000T03:44:00,28-Mar-12,CIRS,SPASS Rider,Dione,REGMAP,Regional mapping,,null,,,,,, 2012-088T04:30:00,000T03:44:00,28-Mar-12,UVIS,,Dione,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Dione, ORS Rider",UV albedo map of Dione's surface plus limb drifts,,,,,, 2012-088T04:30:00,000T03:44:00,28-Mar-12,VIMS,SPASS Rider,Dione,REGMAP,Regional mapping,Dione 80 to 1 deg phase,"Dione 80 to 1 deg phase, 24 to 12 mrad 160, 640 ms, 80ms at low phase",,,,,, 2012-088T04:30:00,000T12:50:00,28-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-088T04:40:00,000T03:34:00,28-Mar-12,ISS,Prime,Dione,REGMAP,Regional mapping,Dione regional mapping,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-088T06:30:09,000T03:29:51,28-Mar-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-088T10:00:00,000T02:00:00,28-Mar-12,INMS,Non-SPASS,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Mag Survey,Inner magnetospheric survey,,,,,, 2012-088T10:32:00,001T08:00:00,28-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-088T10:32:00,001T08:00:00,28-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEYOV,,MIMI SOST segment Overlay,"Overlay: adding 250 bps Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_163_E17",,,,,, 2012-088T10:32:00,000T14:26:00,28-Mar-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-088T10:32:00,000T09:00:00,28-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-088T11:09:00,000T02:00:00,28-Mar-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-088T11:09:57,000T02:00:00,28-Mar-12,CDA,SPASS Rider,DustRAM direction,RPX0390,,CDA RPXing 2012-088T12:09:57,RPXing at 9.6897685 Rs,,,,,, 2012-088T11:32:00,000T09:00:00,28-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12088_SP,rider,,,,,, 2012-088T12:00:00,001T06:32:00,28-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-088T17:20:00,000T03:12:00,28-Mar-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.991547 Rs exit= 13.993759 Range altitude= 5847.5359 km ... 1595.2226,,,,,, 2012-088T20:32:00,007T22:45:00,28-Mar-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.006619 Rs exit= 14.000931 Range altitude= 1600.2676 km ... 5554.0959,,,,,, 2012-088T20:32:00,000T07:28:00,28-Mar-12,RADAR,Non-SPASS,Other,WU4ENGTST,RADAR engineering test warm up,RADAR Engineering Test Warm Up,Warmup for calibration and science data collection.,,,,,, 2012-088T21:12:00,000T01:30:00,28-Mar-12,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 41.5 requested range 1.9 Mkm",,,,,, 2012-088T21:12:00,000T01:30:00,28-Mar-12,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-088T21:12:00,000T01:30:00,28-Mar-12,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 42 deg, range =1.9 Mkm.",,,,,, 2012-088T22:42:00,000T03:33:00,28-Mar-12,ISS,Prime,Other,L5RHEA,,Rhea L5 satellite search,Satellite search around Rhea L5 Lagrange point.,,,,,, 2012-088T22:42:00,000T03:33:00,28-Mar-12,VIMS,SPASS Rider,Other,L5RHEA,,Rock spectra,"ISS NAC to Rocks 160, 640ms IR",,,,,, 2012-089T00:58:00,000T17:34:00,29-Mar-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-089T02:15:00,000T00:45:00,29-Mar-12,CIRS,Prime,Rhea,RHEA,Rhea,,"FP3/4 Shutter Closed Special Table Requirements: Shutter closed from 02:54 -> 02:58 (FP3 scan is early in the design and there is negligible turn time so we want to do shutter closed towards the end). Data will be taken for all focal planes, 15.67 cm-1 spectral resolution, Blink mode for FP3/4. Thanks! Observation Design (updated from the SFAF) 02:15 - 02:16 Turn (including 20 s stare at the start tracking Rhea with the ISS NAC) 02:16 - 02:46 Global FP3 scan of Rhea (probably 2 swaths) at 6 mu rad/s 02:47 - 02:51 ISS NAC Stare at Rhea's center to observe the Rhea/Janus/Mimas mutual event 02:51 - 02:53 FP1 Stare at Rhea with 2 mins dark sky 02:53 - 03:00 Turn",,,,,, 2012-089T02:15:00,000T00:45:00,29-Mar-12,ISS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-089T02:15:00,000T00:45:00,29-Mar-12,UVIS,,Rhea,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Rhea, ORS Rider",UV albedo map of Rhea's surface plus limb drifts,,,,,, 2012-089T02:15:00,000T00:45:00,29-Mar-12,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea 20 deg phase,Rhea 20 deg phase 3.5 mrad,,,,,, 2012-089T03:00:00,000T01:00:00,29-Mar-12,ISS,Prime,Rhea,SATCAL,,ISS Photometric Calibration Star 1,Photometric Calibration on Rhea,,,,,, 2012-089T03:00:00,000T01:00:00,29-Mar-12,CIRS,SPASS Rider,Rhea,SATCAL,,,null,,,,,, 2012-089T03:00:00,000T01:00:00,29-Mar-12,UVIS,,Rhea,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-089T03:00:00,000T01:00:00,29-Mar-12,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea 17 deg phase 3.5 mrad,"Rhea 17 deg phase 3.5 mrad 120, 640 ms",,,,,, 2012-089T04:00:00,000T03:22:00,29-Mar-12,RADAR,Prime,Saturn,ENGTEST,Engineering test,Engineering Test of Diagnostic Modes,Engineering test of diagnostic modes on the flight unit.,,,,,, 2012-089T07:22:00,000T06:40:00,29-Mar-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-089T09:32:00,000T09:00:00,29-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-089T10:17:00,000T08:00:00,29-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12089_SP,rider,,,,,, 2012-089T18:32:00,007T17:15:00,29-Mar-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-089T18:32:00,001T10:00:00,29-Mar-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-089T18:32:00,007T17:15:00,29-Mar-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-089T18:32:00,007T00:45:00,29-Mar-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_163_164",,,,,, 2012-089T18:32:00,007T00:45:00,29-Mar-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-089T19:12:00,000T07:00:00,29-Mar-12,VIMS,Prime,Star,ALPCENCAL,,Alpha Centauri calibration,Alpha Centauri calibration,,,,,, 2012-090T07:32:00,000T07:00:00,30-Mar-12,VIMS,Prime,Star,FOMALHAUT,Fomalhaut,Fomalhaut calibration,Fomalhaut calibration,,,,,, 2012-090T19:32:00,000T09:00:00,30-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-090T20:32:00,000T08:00:00,30-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12090_SP,rider,,,,,, 2012-091T04:32:00,000T11:00:00,31-Mar-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-091T04:32:00,001T00:00:00,31-Mar-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-091T15:32:00,000T04:00:00,31-Mar-12,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2012-091T15:32:00,000T04:00:00,31-Mar-12,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2012-091T18:00:00,002T00:00:00,31-Mar-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - outbound leg - Apo region,,,,,, 2012-091T19:32:00,000T09:00:00,31-Mar-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-091T20:32:00,000T08:00:00,31-Mar-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12091_SP,rider,,,,,, 2012-092T04:32:00,004T07:15:00,1-Apr-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-092T04:53:00,000T00:02:00,1-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-092T04:55:00,000T20:10:00,1-Apr-12,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2012-092T04:55:00,000T20:10:00,1-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-093T01:03:00,000T00:02:00,2-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-093T03:02:00,000T09:00:00,2-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-093T04:02:00,000T08:00:00,2-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12093_SP,rider,,,,,, 2012-093T12:02:00,000T13:30:00,2-Apr-12,CDA,Prime,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-094T03:02:00,000T09:00:00,3-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-094T04:02:00,000T08:00:00,3-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12094_SP,rider,,,,,, 2012-094T12:40:00,000T00:02:00,3-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-094T12:42:00,000T01:30:00,3-Apr-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 83.7 requested range 1.7 Mkm",,,,,, 2012-094T12:42:00,000T01:30:00,3-Apr-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-094T12:42:00,000T01:30:00,3-Apr-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 84 deg, range =1.7 Mkm. Also Stormwatch cube",,,,,, 2012-094T14:10:00,000T00:02:00,3-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-094T14:12:00,000T01:00:00,3-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 012 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-094T15:10:00,000T00:02:00,3-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-094T15:52:00,000T09:40:00,3-Apr-12,ISS,Prime,Other,THRPHA,,Thrymr,Observation of irregular moon of Saturn.,,,,,, 2012-095T00:00:00,000T01:08:00,4-Apr-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-095T03:02:00,000T09:00:00,4-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-095T04:02:00,000T08:00:00,4-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12095_SP,rider,,,,,, 2012-095T12:02:00,000T14:45:00,4-Apr-12,CDA,Prime,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-096T02:47:00,000T09:00:00,5-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-096T03:47:00,000T08:00:00,5-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_163IC_DSCAL12096_SP,rider,,,,,, 2012-096T11:47:00,000T15:00:00,5-Apr-12,VIMS,Prime,rings(general),EG60PHASE,,E/G Ring phase observation,"Stare at E or G ring ansa, 1 second integration.",,,,,, 2012-096T11:47:00,000T15:00:00,5-Apr-12,CIRS,SPASS Rider,rings(general),EG60PHASE,,,null,,,,,, 2012-096T11:47:00,000T07:30:00,5-Apr-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-096T11:47:00,000T15:00:00,5-Apr-12,ISS,Non-SPASS,rings(general),EG60PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2012-096T19:17:00,000T16:30:00,5-Apr-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S73,Range enter= 14.006619 Rs exit= 14.000931 Range altitude= 1600.2676 km ... 5554.0959,,,,,, 2012-096T19:17:00,000T02:00:00,5-Apr-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-096T19:17:00,000T16:30:00,5-Apr-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_163_164",,,,,, 2012-096T19:17:00,000T16:30:00,5-Apr-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-096T19:17:27,000T00:00:01,5-Apr-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.8 d, inc = 0.4 deg, r = 40.361 Rs, phase = 62 deg",,,,,, 2012-096T21:17:00,000T14:30:00,5-Apr-12,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-097T02:47:00,000T09:00:00,6-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-097T03:47:00,000T08:00:00,6-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12097_SP,rider,,,,,, 2012-097T05:17:00,000T06:30:00,6-Apr-12,CDA,SPASS Rider,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00 End: S73,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-097T11:47:00,007T05:45:59,6-Apr-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-097T11:47:00,007T04:29:57,6-Apr-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S73,Range enter= 14.006619 Rs exit= 14.000931 Range altitude= 1600.2676 km ... 5554.0959,,,,,, 2012-097T11:47:00,000T00:43:00,6-Apr-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-097T11:47:00,001T00:00:00,6-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-097T11:47:00,007T05:46:00,6-Apr-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_164",,,,,, 2012-097T11:47:00,007T01:50:00,6-Apr-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-097T11:52:00,000T00:02:00,6-Apr-12,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S73 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2012-097T11:53:00,000T13:24:00,6-Apr-12,CDA,Prime,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00 Enter: S73,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-097T12:30:00,000T00:07:00,6-Apr-12,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-097T12:37:00,000T00:05:00,6-Apr-12,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-097T12:42:00,000T00:33:00,6-Apr-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-097T13:15:00,000T00:30:00,6-Apr-12,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2012-097T13:45:00,003T10:15:00,6-Apr-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-098T02:47:00,000T09:00:00,7-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-098T03:47:00,000T08:00:00,7-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12098_SP,rider,,,,,, 2012-098T11:47:00,000T08:00:00,7-Apr-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-098T19:47:00,000T05:16:00,7-Apr-12,CDA,Prime,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-098T19:47:00,005T12:46:00,7-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-099T02:33:00,000T09:00:00,8-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-099T03:33:00,000T08:00:00,8-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12099_SP,rider,,,,,, 2012-099T12:11:00,000T00:02:00,8-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-099T12:13:00,000T01:30:00,8-Apr-12,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 38.9 requested range 1.8 Mkm",,,,,, 2012-099T12:13:00,000T01:30:00,8-Apr-12,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-099T12:13:00,000T01:30:00,8-Apr-12,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 39 deg, range =1.8 Mkm.",,,,,, 2012-099T13:41:00,000T00:02:00,8-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-099T13:43:00,000T01:00:00,8-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 003 RD OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-099T14:41:00,000T00:02:00,8-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-099T14:41:00,000T00:02:00,8-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-100T02:33:00,000T09:00:00,9-Apr-12,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing). DSS-25 required for X- and Ka-band support.",,,,,, 2012-100T02:33:00,000T01:54:00,9-Apr-12,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev165 Enceladus gravity observation on 2012/123. DSS-55 required for X- and Ka-band support.",,,,,, 2012-100T02:33:00,000T09:00:00,9-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-100T03:33:00,000T08:00:00,9-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12100_SP,rider,,,,,, 2012-100T11:33:00,000T13:30:00,9-Apr-12,CDA,Prime,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-101T00:00:00,000T00:34:00,10-Apr-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2012-101T00:34:00,001T17:14:00,10-Apr-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-101T02:33:00,000T09:00:00,10-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-101T03:33:00,000T08:00:00,10-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12101_SP,rider,,,,,, 2012-101T11:33:00,000T20:35:00,10-Apr-12,CDA,Prime,DustRAM direction,ISD0044,,CDA ISD 2012-096T19:17:00,ISD observation around apoapse 2012-096T19:17:00 40.400826 Rs,,,,,, 2012-101T13:00:00,000T09:00:00,10-Apr-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-102T08:48:00,000T09:00:00,11-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-102T09:48:00,000T08:00:00,11-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12102_SP,rider,,,,,, 2012-102T17:00:00,002T00:00:00,11-Apr-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - inbound leg - Apo->Peri transition,,,,,, 2012-102T17:48:00,000T23:45:00,11-Apr-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-102T18:00:00,000T14:00:00,11-Apr-12,CDA,Non-SPASS,Other,DECON,Decontamination,Decon in S73,SSR-Load (6Ext_Mem_Load) planned to be at exactly 2012-102T19:00:00. This 1h:12m apart from the preceeding end of the OTP (SP_164EA_C34BWGOTP102_PRIME) having a carryover of 0 MB. Expectation is that a SSR-Ping-Pong disable might not be necessary. No additional DV necessary,,,,,, 2012-102T18:26:00,000T00:02:00,11-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-102T18:28:00,000T01:30:00,11-Apr-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 55.2 requested range 2.3 Mkm",,,,,, 2012-102T18:28:00,000T01:30:00,11-Apr-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-102T18:28:00,000T01:30:00,11-Apr-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 55 deg, range =2.3 Mkm.",,,,,, 2012-102T19:56:00,000T00:02:00,11-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-102T19:58:00,000T01:00:00,11-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-102T20:56:00,000T00:02:00,11-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-102T20:56:00,000T00:02:00,11-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-103T02:09:00,000T00:02:00,12-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-103T08:33:00,000T09:00:00,12-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-103T09:33:00,000T08:00:00,12-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12103_SP,rider,,,,,, 2012-103T17:33:00,000T13:00:00,12-Apr-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-103T17:33:00,000T13:00:00,12-Apr-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2012-103T17:33:00,000T03:57:00,12-Apr-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-103T19:00:00,000T11:00:00,12-Apr-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-103T21:30:00,000T02:00:00,12-Apr-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-103T23:30:00,000T18:03:00,12-Apr-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-104T08:33:00,000T09:00:00,13-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-104T08:33:00,000T09:00:00,13-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-104T09:33:00,000T08:00:00,13-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12104_SP,rider,,,,,, 2012-104T13:37:00,000T03:56:00,13-Apr-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-104T16:16:57,002T01:34:00,13-Apr-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.988068 Rs exit= 13.997712 Range altitude= 5547.6408 km ... 1620.6955,,,,,, 2012-104T17:33:00,000T19:28:38,13-Apr-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-104T17:33:00,000T08:28:38,13-Apr-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-104T17:33:00,000T18:28:38,13-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-104T17:33:00,001T15:45:00,13-Apr-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_164_E18 part 1",,,,,, 2012-104T17:33:00,001T15:45:00,13-Apr-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-104T18:13:00,000T01:30:00,13-Apr-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 77.6 requested range 1.8 Mkm",,,,,, 2012-104T18:13:00,000T01:30:00,13-Apr-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-104T18:13:00,000T01:30:00,13-Apr-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 78 deg, range =1.8 Mkm.",,,,,, 2012-104T19:43:00,000T04:00:00,13-Apr-12,ISS,Prime,Other,L5RHEA,,Rhea L5 satellite search,Satellite search around Rhea L5 Lagrange point.,,,,,, 2012-104T23:48:00,000T05:27:00,13-Apr-12,VIMS,Prime,Enceladus,ENCELPLUM,,Enceladus Plume,Enceladus plume,,,,,, 2012-104T23:48:00,000T05:27:00,13-Apr-12,CIRS,SPASS Rider,Enceladus,PLMSTARE,,,"FP1, FP3 only",,,,,, 2012-105T02:01:38,000T10:00:00,14-Apr-12,INMS,Non-SPASS,Enceladus,E18INBND,,Enceladus flyby,Enceladus observation,,,,,, 2012-105T05:15:00,000T05:20:00,14-Apr-12,ISS,Prime,Enceladus,PLMHPMR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2012-105T05:15:00,000T05:20:00,14-Apr-12,CIRS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,,"FP1, FP3 only",,,,,, 2012-105T05:15:00,000T05:20:00,14-Apr-12,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2012-105T05:15:00,000T05:20:00,14-Apr-12,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,Enceladus Plume,Enceladus plume,,,,,, 2012-105T10:35:00,000T02:25:00,14-Apr-12,CIRS,Prime,Enceladus,ENCEL,Enceladus,,"Shutter closed details: 15.67 cm-1 resolution No Add, FP1 Data, FP3 Data, FP3 Blink, FP4 Data, FP4 Blink. Requested shutter closed times: 2012-105T11:19:00->11:24:00 2012-105T12:42:00->12:47:00 This observation time is on approach, nightside observation of Enceladus' equatorial anti-Saturn hemisphere, with dark sky behind. Pick up and hand off at the waypoint, which is ISS_NAC to Enceladus / NEG_X to 92.9/36.6 deg. So the turns are minimal. Preliminary Observation Design: 10:35 - 10:37 Turn 10:37 - 11:16 FP3 6 mu rad/s global scan (2 swaths) [We'd like the FP3/4 shutter closed observations to start during this first FP1 raster scan using table 405:2] 11:16 - 11:21 FP1 raster scan at Nyquist sampling 11:21 - 12:33 FP3 6 mu rad/s global scan (3 swaths) 12:33 - 12:41 FP3 6 mu rad/s SPT scan 12:41 - 12:58 FP1 raster scan at Nyquist sampling 12:58 - 13:00 Turn",,,,,, 2012-105T10:35:00,000T02:25:00,14-Apr-12,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-105T10:35:00,000T02:25:00,14-Apr-12,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus ORS,Enceladus ORS,,,,,, 2012-105T12:01:38,000T00:58:22,14-Apr-12,INMS,Non-SPASS,Enceladus,ENCEL18,,Enceladus encounter,Enceladus observation,,,,,, 2012-105T12:01:38,000T04:00:00,14-Apr-12,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2012-105T12:01:38,000T01:15:00,14-Apr-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-105T12:09:57,000T02:00:00,14-Apr-12,CDA,SPASS Rider,DustRAM direction,RPX0400,,CDA RPXing 2012-105T13:09:57,RPXing at 4.3617851 Rs,,,,,, 2012-105T13:00:00,000T02:00:00,14-Apr-12,INMS,Prime,Enceladus,ENCEL18,,Enceladus encounter,Enceladus observation,,,,,, 2012-105T13:00:00,000T02:00:00,14-Apr-12,ISS,SPASS Rider,Enceladus,ENCEL18,,ISS Rider on INMS Enceladus Prime,ISS rider on an INMS prime close flyby of Enceladus,,,,,, 2012-105T13:00:00,000T02:00:00,14-Apr-12,VIMS,SPASS Rider,Enceladus,ENCEL18,,Enceladus ORS,"Follow INMS, ORS drag across south polar region",,,,,, 2012-105T13:01:38,000T02:00:00,14-Apr-12,CAPS,SPASS Rider,Titan,EN18CLOSE,,Closest Approach 164EN (18),null,,,,,, 2012-105T13:16:38,000T01:30:00,14-Apr-12,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2012-105T13:31:38,000T01:00:00,14-Apr-12,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 164,BIT_OVERLAY_1200,,,,,, 2012-105T13:56:38,000T00:20:00,14-Apr-12,CIRS,SPASS Rider,Enceladus,ENCEL18,,CIRS_164EN_ENCEL18001_INMS,"Shutter closed details: 15.67 cm-1 resolution, Data from FP1, FP3 and FP4. Use Pairs for FP3 and FP4. Would like shutter closed at the start of the observation, for as long as possible but that so that CIRS is back looking at sky by 14:00. Ride with INMS- secondary chosen to drag the ORS fields of view along Baghdad Sulcus. Close range means useful data will require dissecting individual interferograms",,,,,, 2012-105T13:59:38,000T00:04:00,14-Apr-12,UVIS,SPASS Rider,Enceladus,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus's surface plus limb drifts,,,,,, 2012-105T15:00:00,000T01:55:00,14-Apr-12,CIRS,Prime,Enceladus,ENCEL,Enceladus,,"This is a dayside observation of Enceladus equatorial Saturn-facing hemisphere on departure. We pick up and hand off from the waypoint (ISS_NAC to Enceladus / NEG_X to 92.9 / 36.6) , so turn times will be small. Note from John Spencer on design plan: Start with hi-res FP3 map of subsolar region or nearby (c.f. the one planned for Rev. 155 at 10:50 UT - this one will be higher resolution but should maybe also cover different territory- the subsolar point is at a similar location in each case). Preliminary Design: 15:00 - 15:02 Turn [Note shutter closed will be taken between 15:00:00 and 15:01:53] 15:02 - 16:38 FP3 scans a 6 mu rad/s, focusing initially at sub-solar region (where the highest temps and thus S/N will be), building to a global map, with good SPT coverage? 16:38 - 16:53 FP1 raster scan at Nyquist sampling 16:53 - 16:55 Turn",,,,,, 2012-105T15:00:00,000T01:55:00,14-Apr-12,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-105T15:00:00,000T01:55:00,14-Apr-12,VIMS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus ORS,Enceladus ORS,,,,,, 2012-105T15:00:00,000T01:01:38,14-Apr-12,INMS,Non-SPASS,Enceladus,ENCEL18,,Enceladus encounter,Enceladus observation,,,,,, 2012-105T15:01:38,000T18:16:22,14-Apr-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-105T16:01:38,000T10:00:00,14-Apr-12,INMS,Non-SPASS,Enceladus,E18OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2012-105T16:01:38,000T04:58:22,14-Apr-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-105T17:00:00,000T02:40:00,14-Apr-12,VIMS,Prime,Saturn,ALPCMIOCC,Alpha CMI occultation,alpCMi Saturn occultation,"alpCMi atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec. After the occ, at time 18:04, turn to point CIRS_FP3 to the point on Saturn's limb where the occultation occurred (latitude 21.3N).",,,,,, 2012-105T17:00:00,000T02:30:00,14-Apr-12,CIRS,,Saturn,ALPCMIOCC,Alpha CMI occultation,CIRS_164SA_ALPCMIOCC001_VIMS,Collab with VIMS. Stellar Occ Saturn ingress T17:43 21N dark limb at T18:04 go to limb for CIRS integration,,,,,, 2012-105T17:03:11,000T00:00:01,14-Apr-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.253 Rs, lat = -0 deg, phase = 118 deg",,,,,, 2012-105T19:40:00,000T00:50:00,14-Apr-12,CIRS,Prime,Tethys,TETHYS,Tethys,,"On nightside approach of Tethys' equatorial Saturn facing hemisphere. In a custom period, pick up and hand off at ISS_NAC to Tethys / POS_X to 264.0/68.0. Note: FP3, FP1 only 19:40 - 19:42 Turn [Note FP3 shutter closed between 19:40:00 and 19:41:53] 19:42 - 19:55 1st FP1 raster scan at Nyquist sampling 19:55 - 20:08 2nd FP1 raster scan at Nyquist sampling 20:08 - 20:28 3rd FP1 raster scan at Nyquist sampling 20:28 - 20:30 Turn",,,,,, 2012-105T19:40:00,000T00:50:00,14-Apr-12,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-105T19:40:00,000T00:50:00,14-Apr-12,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys ORS,Tethys ORS,,,,,, 2012-105T20:30:00,000T04:00:00,14-Apr-12,ISS,Prime,Tethys,TETHYS,Tethys,Tethys ORS observation,ORS observation,,,,,, 2012-105T20:30:00,000T04:00:00,14-Apr-12,CIRS,,Tethys,TETHYS,Tethys,,"FP1, FP3 only CIRS can probably use most of the time from 20:30 to 21:30, and from 21:52 to 22:15, and whatever gaps occur between mosaics in the subsequent ISS coverage.",,,,,, 2012-105T20:30:00,000T04:00:00,14-Apr-12,UVIS,,Tethys,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus's surface plus limb drifts,,,,,, 2012-105T20:30:00,000T04:00:00,14-Apr-12,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys ORS,Tethys ORS,,,,,, 2012-105T21:00:00,000T22:58:00,14-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-106T00:30:00,000T02:00:00,15-Apr-12,CIRS,Prime,Tethys,TETHYS,Tethys,,"This is dayside departure, viewing over equatorial latitudes of Tethys' trailing hemisphere. In custom period, pick up and hand off at the waypoint (ISS_NAC to Tethys, POS_X to 264.0/68.0), so we have short turns. Notes from John Spencer: FP1, FP3 only Focus on likely location of daytime color/thermal anomaly 00:30 - 00:32 Turn [FP3 shutter closed from 00:30:00 to 00:31:53] 00:32 - 00:42 FP1 raster scan at Nyquist sampling 00:42 - 01:30 1st FP3 swath at 6 mu rad/s, N-> S centered on longitude ~145 deg W 01:30 - 02:00 2nd FP3 swath at 6 mu rad/s, S->N centered on longitude ~180 deg W 02:00 - 02:28 3rd FP3 swath at 6 mu rad/s, N->S centered on longitude ~220 deg W. 02:28 - 02:30 Turn",,,,,, 2012-106T00:30:00,000T02:00:00,15-Apr-12,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-106T00:30:00,000T02:00:00,15-Apr-12,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys ORS,Tethys ORS,,,,,, 2012-106T02:01:38,001T15:16:22,15-Apr-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-106T02:30:00,000T04:30:00,15-Apr-12,VIMS,Prime,Tethys,TETHYS,Tethys,Tethys composition,"not a pie. Pick up & leave off at ISS_NAC to Tethys, POS_X to 264.0/68.0",,,,,, 2012-106T02:30:00,000T04:30:00,15-Apr-12,CIRS,,Tethys,TETHYS,Tethys,,"FP1, FP3 only",,,,,, 2012-106T02:30:00,000T04:30:00,15-Apr-12,ISS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys ORS observation,ORS observation,,,,,, 2012-106T02:30:00,000T04:30:00,15-Apr-12,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-106T06:15:57,000T02:00:00,15-Apr-12,CDA,SPASS Rider,DustRAM direction,RPX0410,,CDA RPXing 2012-106T07:15:57,RPXing at 9.4912160 Rs,,,,,, 2012-106T09:18:00,001T08:00:00,15-Apr-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-106T09:18:00,001T08:00:00,15-Apr-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_164_E18 part 2",,,,,, 2012-106T09:18:00,000T11:11:00,15-Apr-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-106T09:18:00,000T09:00:00,15-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-106T10:18:00,000T09:00:00,15-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12106_SP,rider,,,,,, 2012-106T17:50:57,007T20:55:03,15-Apr-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.010572 Rs exit= 14.009308 Range altitude= 1625.5878 km ... 5358.8271,,,,,, 2012-106T19:58:00,005T05:50:00,15-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-106T20:00:00,000T12:00:00,15-Apr-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-106T20:29:00,000T20:49:00,15-Apr-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-106T20:38:00,000T01:30:00,15-Apr-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 68.5 requested range 1.5 Mkm",,,,,, 2012-106T20:38:00,000T01:30:00,15-Apr-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-106T20:38:00,000T01:30:00,15-Apr-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 68 deg, range =1.5 Mkm.",,,,,, 2012-106T22:08:00,000T01:30:00,15-Apr-12,CIRS,Prime,Rhea,RHEA,Rhea,,"Old shutter closed request (subsequently changed to Lego table): Shutter closed details: 15.67 cm-1 resolution No Add, FP1 Data, FP3 Data, FP3 Blink, FP4 Data, FP4 Blink. Requested shutter closed time: 2012-106T22:36:10-22:40:10 This is a daytime observation (small dark crescent - phase is <40 deg) with dark sky behind. Rhea is only slightly larger than the FP3/4 FOV and Rhea is smaller than the FP1 fov. Preliminary Plan: 22:08 - 22:10 Turn 22:10 - 22:36 Global FP3/4 coverage (2 swaths) at 6 mu rad/s [Please schedule the first FP3/4 shutter closed observation to take place during this FP1 stare using table number 355:1] 22:36 - 22:41 FP1 stare, centered on Rhea's center 22:41 - 23:26 2 x Global FP3/4 coverage (2 swaths each) at 6 mu rad/s 23:26 - 23:38 Turn",,,,,, 2012-106T22:08:00,000T01:30:00,15-Apr-12,UVIS,,Rhea,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Rhea's surface,,,,,, 2012-106T22:08:00,000T01:30:00,15-Apr-12,VIMS,SPASS Rider,Rhea,RHEA,Rhea,Rhea,Rhea,,,,,, 2012-106T23:38:00,000T06:30:00,15-Apr-12,ISS,Prime,Other,RHEAL4,,Rhea L4 satellite search,Satellite search around Rhea L4 Lagrange point.,,,,,, 2012-106T23:38:00,000T06:30:00,15-Apr-12,VIMS,SPASS Rider,Rhea,RHEAL4,,Rhea,Rhea L4 search,,,,,, 2012-107T06:42:30,000T06:05:30,16-Apr-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-107T08:18:00,000T09:00:00,16-Apr-12,RSS,SPASS Rider,Earth,DSNMONCAL,,DSN Monopulse Calibration,"An opportunity for the DSN station to perform an on-point phase cal (using Cassini Ka-band signal) to update the monopulse TAU value, which is needed for monopulse to work correctly. The cals should be conducted when the s/c is in 1-way mode and again when the s/c is 2-way or 3-way mode. The new TAU is the average of these two values. The mono cal can be conducted during the prime tracking pass with minimal impact to X-band (0.23 dB down in gain on X-band, 7 mdeg offset in pointing). DSS-34 required for X- and Ka-band support.",,,,,, 2012-107T08:18:00,000T09:00:00,16-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-107T09:18:00,000T08:00:00,16-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12107_SP,rider,,,,,, 2012-107T17:18:00,014T16:43:59,16-Apr-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-107T17:18:00,001T10:00:00,16-Apr-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-107T17:18:00,006T21:28:00,16-Apr-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_164_165",,,,,, 2012-107T17:18:00,006T21:28:00,16-Apr-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-107T17:58:00,000T00:02:00,16-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-107T18:00:00,000T01:00:00,16-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 008 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-107T18:00:00,002T00:00:00,16-Apr-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - outbound leg,,,,,, 2012-107T18:58:00,000T00:02:00,16-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-107T18:58:00,000T00:02:00,16-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-107T19:00:00,000T12:00:00,16-Apr-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-108T06:58:00,000T00:02:00,17-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-108T06:58:00,000T00:02:00,17-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-108T18:18:00,000T09:00:00,17-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-108T19:18:00,000T08:00:00,17-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12108_SP,rider,,,,,, 2012-109T03:18:00,001T00:00:00,18-Apr-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-109T18:18:00,000T09:00:00,18-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-109T19:18:00,000T08:00:00,18-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12109_SP,rider,,,,,, 2012-110T00:00:00,000T01:08:00,19-Apr-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-110T03:18:00,004T11:28:00,19-Apr-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-110T06:28:00,000T00:02:00,19-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-110T06:30:00,000T01:00:00,19-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 010 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-110T07:28:00,000T00:02:00,19-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-110T07:28:00,000T00:02:00,19-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-110T07:30:00,000T01:30:00,19-Apr-12,ISS,Prime,Dione,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Dione across Rhea","Images of mutual event, transit of Dione across Rhea for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2012-110T08:58:00,000T00:02:00,19-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-110T08:58:00,000T00:02:00,19-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-110T09:00:00,000T09:00:00,19-Apr-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-110T17:58:00,000T00:02:00,19-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-110T17:58:00,000T00:02:00,19-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-110T18:00:00,000T04:00:00,19-Apr-12,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2012-110T18:00:00,000T04:00:00,19-Apr-12,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2012-110T21:58:00,000T00:02:00,19-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-110T21:58:00,000T00:02:00,19-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-110T22:00:00,000T01:30:00,19-Apr-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 81.3 requested range 1.4 Mkm",,,,,, 2012-110T22:00:00,000T01:30:00,19-Apr-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-110T22:00:00,000T01:30:00,19-Apr-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 81 deg, range =1.4 Mkm.",,,,,, 2012-110T23:28:00,000T00:02:00,19-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T01:48:00,000T09:00:00,20-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-111T02:48:00,000T08:00:00,20-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12111_SP,rider,,,,,, 2012-111T04:48:00,000T07:00:00,20-Apr-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-111T11:26:00,000T00:02:00,20-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T11:28:00,000T02:00:00,20-Apr-12,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 69.8 requested range 1.1 Mkm",,,,,, 2012-111T11:28:00,000T02:00:00,20-Apr-12,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-111T11:28:00,000T01:30:00,20-Apr-12,VIMS,SPASS Rider,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 70 deg, range =1.1 Mkm.",,,,,, 2012-111T13:26:00,000T00:02:00,20-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T13:26:00,000T00:02:00,20-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-111T13:28:00,000T01:00:00,20-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-111T14:26:00,000T00:02:00,20-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T14:26:00,000T00:02:00,20-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-111T14:28:00,000T04:02:00,20-Apr-12,ISS,Prime,Other,L5TITANA,,Titan L5 satellite search (part 1),Satellite search around Titan L5 Lagrange point.,,,,,, 2012-111T14:46:00,000T20:00:00,20-Apr-12,CDA,SPASS Rider,DustRAM direction,ISD0045,,CDA ISD 2012-114T14:46:00,ISD observation around apoapse 2012-114T14:46:00 40.404374 Rs,,,,,, 2012-111T18:28:00,000T00:02:00,20-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T18:28:00,000T00:02:00,20-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-111T18:30:00,000T01:30:00,20-Apr-12,ISS,Prime,Rhea,MUTUALEVE,Mutual event satellite transit observation,"Mutual Event, transit of Rhea across Tethys","Images of mutual event, transit of Rhea across Tethys for orbit determination purposes. This observation CANNOT take place earlier or later",,,,,, 2012-111T19:58:00,000T00:02:00,20-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T19:58:00,000T00:02:00,20-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-111T20:00:00,000T03:30:00,20-Apr-12,ISS,Prime,Other,L5TITANB,,Titan L5 satellite search (part 2),Satellite search around Titan L5 Lagrange point.,,,,,, 2012-111T23:28:00,000T00:02:00,20-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-111T23:28:00,000T00:02:00,20-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-112T01:48:00,001T09:00:00,21-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-112T01:48:00,000T09:00:00,21-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-112T02:48:00,000T08:00:00,21-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12112_SP,rider,,,,,, 2012-113T01:48:00,000T09:00:00,22-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-113T02:48:00,000T08:00:00,22-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12113_SP,rider,,,,,, 2012-113T08:46:00,000T20:00:00,22-Apr-12,CDA,SPASS Rider,DustRAM direction,ISD0045,,CDA ISD 2012-114T14:46:00,ISD observation around apoapse 2012-114T14:46:00 40.404374 Rs,,,,,, 2012-113T10:48:00,000T07:00:00,22-Apr-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-113T17:48:00,008T16:14:00,22-Apr-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-114T01:33:00,000T09:00:00,23-Apr-12,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev165 Enceladus gravity observation on 2012/123. DSS-25 and DSS-55 required for X- and Ka-band support.",,,,,, 2012-114T01:33:00,000T09:00:00,23-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-114T02:33:00,000T08:00:00,23-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_164IC_DSCAL12114_SP,rider,,,,,, 2012-114T11:11:00,000T00:02:00,23-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-114T11:13:00,000T01:30:00,23-Apr-12,ISS,Prime,Titan,M60R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 34.7 requested range 1.7 Mkm",,,,,, 2012-114T11:13:00,000T01:30:00,23-Apr-12,CIRS,SPASS Rider,Titan,M60R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-114T11:13:00,000T01:30:00,23-Apr-12,VIMS,SPASS Rider,Titan,M60R2CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch; phase = 35 deg, range =1.7 Mkm.",,,,,, 2012-114T12:41:00,000T00:02:00,23-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-114T12:43:00,000T01:00:00,23-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 014 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-114T13:41:00,000T00:02:00,23-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-114T13:41:00,000T00:02:00,23-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-114T13:43:00,000T11:07:00,23-Apr-12,VIMS,Prime,rings(general),EG60PHASE,,E/G Ring phase observation,"Stare at E or G ring ansa, 1 second integration.",,,,,, 2012-114T13:43:00,000T11:07:00,23-Apr-12,CIRS,SPASS Rider,rings(general),EG60PHASE,,,null,,,,,, 2012-114T13:43:00,000T11:07:00,23-Apr-12,UVIS,SPASS Rider,rings(general),EG60PHASE,,,VIMS rider,,,,,, 2012-114T13:43:00,000T11:07:00,23-Apr-12,ISS,Non-SPASS,rings(general),EG60PHASE,,Phase Curve and color measurements of faint rings,"VIMS rider, Low res, low elev., medium-phase of G or E ring",,,,,, 2012-114T14:46:00,007T21:00:57,23-Apr-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.010572 Rs exit= 14.009308 Range altitude= 1625.5878 km ... 5358.8271,,,,,, 2012-114T14:46:00,000T02:00:00,23-Apr-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-114T14:46:00,007T19:16:00,23-Apr-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_164_165",,,,,, 2012-114T14:46:00,007T18:22:00,23-Apr-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-114T14:46:17,000T00:00:01,23-Apr-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.8 d, inc = 0.4 deg, r = 40.363 Rs, phase = 62 deg",,,,,, 2012-114T15:00:00,002T00:00:00,23-Apr-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - APO leg,,,,,, 2012-114T16:46:00,000T17:47:00,23-Apr-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-115T00:48:00,000T00:02:00,24-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-115T01:33:00,000T09:00:00,24-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-115T02:33:00,000T08:00:00,24-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12115_SP,rider,,,,,, 2012-115T10:33:00,000T14:59:00,24-Apr-12,ISS,Prime,Other,ERRRES,,Erriapus,Observation of irregular moon of Saturn.,,,,,, 2012-115T10:33:00,000T23:59:00,24-Apr-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-116T01:32:00,000T09:00:00,25-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-116T02:32:00,000T08:00:00,25-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12116_SP,rider,,,,,, 2012-116T10:32:00,003T23:45:00,25-Apr-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-116T13:30:00,000T07:00:00,25-Apr-12,VIMS,Prime,Star,TRANSIT,,Exoplanet transit observation,"Stare at RA/Dec, acquire transit of stellar disk using occultation and/or imaging modes",,,,,, 2012-116T13:30:00,000T07:00:00,25-Apr-12,ISS,SPASS Rider,Star,TRANSIT,,EXOPLANET TRANSIT,ISS rider on a VIMS exo-planet transit observation of HD189733. BOTSIMS to provide starfield,,,,,, 2012-117T07:32:00,000T09:00:00,26-Apr-12,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev165 Enceladus gravity observation on 2012/123. DSS-34 required for X- and Ka-band support.",,,,,, 2012-117T07:32:00,000T09:00:00,26-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-117T08:32:00,000T08:00:00,26-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12117_SP,rider,,,,,, 2012-117T16:32:00,000T13:20:00,26-Apr-12,CDA,Prime,DustRAM direction,ISD0045,,CDA ISD 2012-114T14:46:00,ISD observation around apoapse 2012-114T14:46:00 40.404374 Rs,,,,,, 2012-118T07:32:00,000T09:00:00,27-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-118T08:32:00,000T08:00:00,27-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12118_SP,rider,,,,,, 2012-119T01:17:00,000T09:00:00,28-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-119T02:17:00,000T08:00:00,28-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12119_SP,rider,,,,,, 2012-119T10:55:00,000T00:02:00,28-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-119T10:57:00,000T01:30:00,28-Apr-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 59.7 requested range 2.9 Mkm",,,,,, 2012-119T10:57:00,000T01:30:00,28-Apr-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-119T10:57:00,000T01:30:00,28-Apr-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch; phase = 60 deg, range =2.9 Mkm.",,,,,, 2012-119T12:25:00,000T00:02:00,28-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-119T12:27:00,000T01:00:00,28-Apr-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-119T13:25:00,000T00:02:00,28-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-119T13:25:00,000T00:02:00,28-Apr-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-120T01:17:00,000T09:00:00,29-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-120T02:17:00,000T08:00:00,29-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12120_SP,rider,,,,,, 2012-120T09:30:00,002T00:00:00,29-Apr-12,CDA,SPASS Rider,DustRAM direction,RETROGRAD,,CDA Retrograde campaign,Retrograde observation - Inbound leg,,,,,, 2012-120T10:17:00,000T14:45:00,29-Apr-12,CDA,Prime,DustRAM direction,ISD0045,,CDA ISD 2012-114T14:46:00,ISD observation around apoapse 2012-114T14:46:00 40.404374 Rs,,,,,, 2012-120T10:17:00,000T23:45:00,29-Apr-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-121T01:02:00,000T09:00:00,30-Apr-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-121T02:02:00,000T08:00:00,30-Apr-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12121_SP,rider,,,,,, 2012-121T10:02:00,000T06:58:00,30-Apr-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-121T10:40:00,000T00:02:00,30-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-121T10:42:00,000T01:30:00,30-Apr-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 82.7 requested range 2.5 Mkm",,,,,, 2012-121T10:42:00,000T01:30:00,30-Apr-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-121T10:42:00,000T01:30:00,30-Apr-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stirmwatch,"Titan Monitoring Campaign and Stormwatch; phase = 83 deg, range =2.5 Mkm.",,,,,, 2012-121T12:10:00,000T00:02:00,30-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-121T12:12:00,000T10:20:00,30-Apr-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-121T12:12:00,000T10:20:00,30-Apr-12,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2012-121T12:12:00,000T10:20:00,30-Apr-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stormwatch,Auroral Slew UVIS Ridealong and Stormwatch cube,,,,,, 2012-121T17:00:00,000T02:00:00,30-Apr-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-121T19:00:00,000T15:02:00,30-Apr-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-121T22:30:00,000T00:02:00,30-Apr-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-122T01:02:00,000T09:00:00,1-May-12,RSS,SPASS Rider,Enceladus,GSE,,Gravity Science Enhancement (GSE),"Enceladus inbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-25 required for X- and Ka-band support.",,,,,, 2012-122T01:02:00,000T09:00:00,1-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-122T02:02:00,000T08:00:00,1-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12122_SP,rider,,,,,, 2012-122T06:07:00,000T03:55:00,1-May-12,RSS,SPASS Rider,Enceladus,GRAVORT,RSS gravity science Operational Readiness Test,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev165 Enceladus gravity observation on 2012/123. DSS-34 required for X- and Ka-band support.",,,,,, 2012-122T09:08:00,000T00:54:00,1-May-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-122T10:02:00,000T09:45:00,1-May-12,ISS,Prime,Other,YMIROTA,,Ymir,Observation of irregular moon of Saturn.,,,,,, 2012-122T10:02:00,000T22:29:29,1-May-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-122T10:02:00,000T11:29:29,1-May-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-122T10:02:00,000T21:29:29,1-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-122T10:02:00,002T23:45:00,1-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_165_E19",,,,,, 2012-122T10:02:00,002T05:57:00,1-May-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-122T11:46:57,000T05:00:00,1-May-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.996445 Rs exit= 13.998747 Range altitude= 5352.5920 km ... 1572.1676,,,,,, 2012-122T16:46:57,001T17:00:03,1-May-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.996445 Rs exit= 13.998747 Range altitude= 5352.5920 km ... 1572.1676,,,,,, 2012-122T19:47:00,000T03:00:00,1-May-12,VIMS,Prime,Sun,SOLARPORT,Solar port observation,Solar port calibration,"turn from xband to earth, neg X to nsp",,,,,, 2012-122T21:31:29,000T10:00:00,1-May-12,INMS,Non-SPASS,Enceladus,E19INBND,,Enceladus flyby,Enceladus observation,,,,,, 2012-122T23:01:29,000T02:30:00,1-May-12,ISS,Prime,Enceladus,PLMHPMR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2012-122T23:01:29,000T02:30:00,1-May-12,CIRS,SPASS Rider,Enceladus,PLMHPMR,Observe Enceladus' plumes,,null,,,,,, 2012-122T23:01:29,000T02:30:00,1-May-12,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2012-122T23:01:29,000T02:30:00,1-May-12,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,Enceladus plume,"plume, follow iss",,,,,, 2012-122T23:26:29,000T02:05:00,1-May-12,RSS,SPASS Rider,Enceladus,THERMAL,Thermal stabilization period,RSS thermal stabilization,"A period of thermal stabilization of the RFIS bay is required immediately prior to any radio science experiment using Ka-band. It must be preceeded by 5 minutes Ka-band TWTA maintenance. CDA can articulate during warm-up, but not during the science observation.",,,,,, 2012-123T01:31:29,000T03:00:00,2-May-12,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2012-123T04:31:29,000T01:33:31,2-May-12,ISS,Prime,Enceladus,PLMHPHR,Observe Enceladus' plumes,Enceladus Plume PIE,Enceladus plume PIE,,,,,, 2012-123T04:31:29,000T01:33:31,2-May-12,CIRS,SPASS Rider,Enceladus,PLMHPMR,Observe Enceladus' plumes,,null,,,,,, 2012-123T04:31:29,000T01:33:31,2-May-12,UVIS,SPASS Rider,Enceladus,ICYPLU,Observe Enceladus plumes,ICYPLU: Enceladus Plume Observation,"Observe Enceladus' plume, usually at very high phase angles",,,,,, 2012-123T04:31:29,000T01:33:31,2-May-12,VIMS,SPASS Rider,Enceladus,PLUME,Observe Enceladus' plumes,Enceladus plume,"plume, follow iss",,,,,, 2012-123T06:05:00,000T01:56:29,2-May-12,CIRS,Prime,Enceladus,ENCELADUS,Enceladus,,"Shutter closed details: 15.67 cm-1 resolution No Add, FP1 Data, FP3 Data, FP3 Blink, FP4 Data, FP4 Blink. Shutter closed request times: 2012-123T07:19:30 -> 07:24:30 Nightside approach of Enceladus' anti-Saturn hemisphere at equatorial latitudes. Spatial resolution is good at end (12.2 mrad), increasing from 5.0 mrad at start. No turn at pick up, longish turn at end. 06:05 - 06:07 Turn (Marginal turn times, pick up from Enceladus) [Note shutter closed is being taken between 06:05:00 and 06:06:53, so don't scan until complete (shutter closed needed at the start since the FP3 observation period is long)] 06:07 - 07:20 FP3 global scans at 6 mu rad/s, concentrating the highest spatial resolution observation over the SPT 07:20 - 07:30 FP1 raster at Nyquist sampling 07:30 - 08:01 Turn (Primary and Secondary turn required)",,,,,, 2012-123T07:31:29,000T01:50:00,2-May-12,INMS,Non-SPASS,Enceladus,ENCEL19,,Enceladus encounter,Enceladus observation,,,,,, 2012-123T07:31:29,000T04:00:00,2-May-12,MAG,Non-SPASS,Enceladus,ENTAR,Enceladus,Enceladus targeted flyby,Monitor the interaction of Enceladus with the Saturnian magnetospheric plasma and determine whether it generates an internal magnetic field.,,,,,, 2012-123T07:37:00,000T02:00:00,2-May-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-123T07:39:57,000T02:00:00,2-May-12,CDA,SPASS Rider,DustRAM direction,RPX0420,,CDA RPXing 2012-123T08:39:57,RPXing at 4.3625436 Rs,,,,,, 2012-123T08:01:29,000T03:00:00,2-May-12,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2012-123T08:31:29,000T02:00:00,2-May-12,CAPS,SPASS Rider,Titan,EN19CLOSE,,Closest Approach 165EN (19),null,,,,,, 2012-123T08:31:29,000T02:00:00,2-May-12,RPWS,Non-SPASS,Enceladus,ENCA,Enceladus closest approach observation,Enceladus closest approach observations,"RPWS observations in the immediate vicinity of Enceladus, including the characterization of the plasma wave spectrum and search for evidence of pickup ions. Pointing: prefer RPWS Langmuir Probe within 90 degrees of plasma ram.",,,,,, 2012-123T09:01:29,000T01:00:00,2-May-12,MIMI,Non-SPASS,Enceladus,ENCNTROV,,MIMI Enceladus 165,BIT_OVERLAY_950,,,,,, 2012-123T09:21:29,000T00:20:00,2-May-12,INMS,Non-SPASS,Enceladus,ENCEL19,,Enceladus encounter,Enceladus observation,,,,,, 2012-123T09:41:29,000T01:50:00,2-May-12,INMS,Non-SPASS,Enceladus,ENCEL19,,Enceladus encounter,Enceladus observation,,,,,, 2012-123T10:31:29,001T23:15:31,2-May-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-123T11:01:29,000T03:00:00,2-May-12,CIRS,Prime,Enceladus,ENCELADUS,Enceladus,,"Shutter closed details: 15.67 cm-1 resolution No Add, FP1 Data, FP3 Data, FP3 Blink, FP4 Data, FP4 Blink. Requested shutter closed times: 2012-123T11:35:00-11:40:00 and 2012-123T13:39:00-13:44:00. Daytime after c/a equatorial observation, with little subscft longitude variation (Saturn-facing/leading hemisphere coverage). Spatial resolution is decent at the start (12.65 mrad, decreasing to 4.08 mrad at end), low phase (<20 deg throughout). Annoying turns at start and end. 11:01 - 11:24 Turn (Primary and possibly Secondary Changes) [FYI Shutter closed between 01:01:00 and 01:02:53] 11:24 - 11:39 ISS mosaic, details below 11:39 - 12:10 1st FP3 Scan at 6 mu rad/s 12:10 - 12:35 2nd FP3 Scan at 6 mu rad/s 12:35 - 12:55 3rd FP3 Scan at 6 mu rad/s [Note Shutter closed between 13:01:00 and 13:02:53, can we make this time away from disk - not in the center of a scan? ] 12:55 - 13:15 4th FP3 Scan at 6 mu rad/s 13:15 - 13:28 5th FP3 Scan (incomplete) at 6 mu rad/s 13:28 - 14:01 Turn (Primary and possibly Secondary change) ISS would like a 4 panel mosaic (with 3 min dwell times) at the start of the observation period",,,,,, 2012-123T11:01:29,000T03:00:00,2-May-12,ISS,SPASS Rider,Enceladus,ENCELADUS,Enceladus,Enceladus ORS observation,ORS observation,,,,,, 2012-123T11:01:29,000T03:00:00,2-May-12,UVIS,SPASS Rider,Enceladus,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-123T11:31:29,000T10:00:00,2-May-12,INMS,Non-SPASS,Enceladus,E19OUTBND,,Enceladus flyby,Enceladus observation,,,,,, 2012-123T11:31:29,000T05:03:31,2-May-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-123T12:33:44,000T00:00:01,2-May-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.245 Rs, lat = -0 deg, phase = 118 deg",,,,,, 2012-123T14:01:29,000T03:00:00,2-May-12,RSS,SPASS Rider,Enceladus,GRAVITY,RSS gravity science experiment,RSS Enceladus Gravity Field Experiment,"Experiment to determine Enceladus's gravity field, possibly detecting a diapir under the south pole, and infer constraints on its internal structure.",,,,,, 2012-123T16:35:00,001T17:12:00,2-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-123T17:49:00,000T02:13:00,2-May-12,CIRS,Prime,Dione,DIONE,Dione,,"17:49 - 17:50 Turn [FP3/4 shutter closed between 17:49:00 and 17:50:53] 17:50 - 18:10 1st FP1 raster scan at Nyquist sampling 18:10 - 18:30 2nd FP1 raster scan at Nyquist sampling 18:30 - 18:35 ISS mosaic, details below FP3/4 shutter closed between 18:49:00 and 18:50:53] 18:35 - 19:10 3rd FP1 raster scan at Nyquist sampling FP3/4 shutter closed between 19:49:00 and 19:50:53] 19:10 - 20:01 4th FP1 raster scan probably not at Nyquist sampling to achieve global coverage 20:01 - 20:02 Turn Nightside approach over equatorial latitudes of the leading hemisphere. Will be able to see fractured region, especially early in observation time. ISS request a 5-panel mosaic with 30 sec dwell times of the sunlit crescent in the ~ middle of this observation period.",,,,,, 2012-123T17:49:00,000T02:13:00,2-May-12,ISS,,Dione,DIONE,Dione,Dione high phase,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-123T17:49:00,000T02:13:00,2-May-12,UVIS,SPASS Rider,Dione,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-123T17:49:00,000T02:13:00,2-May-12,VIMS,SPASS Rider,Dione,DIONE,Dione,Dione,follow cirs,,,,,, 2012-123T20:02:00,000T04:09:00,2-May-12,ISS,Prime,Dione,REGMAP,Regional mapping,Dione regional mapping,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-123T20:02:00,000T04:09:00,2-May-12,CIRS,SPASS Rider,Dione,DIONE,Dione,,null,,,,,, 2012-123T20:02:00,000T04:09:00,2-May-12,UVIS,,Dione,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Enceladus, ORS Rider",UV albedo map of Enceladus's surface plus limb drifts,,,,,, 2012-123T20:02:00,000T04:09:00,2-May-12,VIMS,SPASS Rider,Dione,REGMAP,Regional mapping,Dione,"plume, follow iss",,,,,, 2012-123T21:31:29,001T12:15:31,2-May-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-124T00:47:00,000T09:00:00,3-May-12,RSS,SPASS Rider,Enceladus,GSE,,Gravity Science Enhancement (GSE),"Enceladus inbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-25 required for X- and Ka-band support.",,,,,, 2012-124T00:47:00,000T09:00:00,3-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-124T01:41:00,000T02:00:00,3-May-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-124T01:41:57,000T02:00:00,3-May-12,CDA,SPASS Rider,DustRAM direction,RPX0430,,CDA RPXing 2012-124T02:41:57,RPXing at 9.4592188 Rs,,,,,, 2012-124T01:47:00,000T09:00:00,3-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12124_SP,rider,,,,,, 2012-124T09:47:57,000T03:33:00,3-May-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.996445 Rs exit= 13.998747 Range altitude= 5352.5920 km ... 1572.1676,,,,,, 2012-124T11:17:00,000T03:00:00,3-May-12,UVIS,Prime,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration USTRCAL01 & USTRCAL02,Instance of USTRCAL01 & 02,,,,,, 2012-124T12:59:00,000T20:48:00,3-May-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-124T13:20:57,007T20:07:03,3-May-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.011610 Rs exit= 14.010733 Range altitude= 1576.8851 km ... 2485.2715,,,,,, 2012-124T14:17:00,000T09:00:00,3-May-12,ISS,Prime,Other,YMIROTB,,Ymir,Observation of irregular moon of Saturn.,,,,,, 2012-125T00:47:00,000T09:00:00,4-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-125T01:47:00,000T08:00:00,4-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12125_SP,rider,,,,,, 2012-125T09:47:00,015T15:28:59,4-May-12,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2012-125T09:47:00,002T00:00:38,4-May-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-125T09:47:00,009T23:14:00,4-May-12,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2012-125T09:47:00,006T23:41:00,4-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_165_166",,,,,, 2012-125T09:47:00,006T23:41:00,4-May-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-125T10:27:00,000T12:50:00,4-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-126T00:00:00,000T01:08:00,5-May-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-126T00:47:00,000T09:00:00,5-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-126T01:47:00,000T08:00:00,5-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12126_SP,rider,,,,,, 2012-126T09:47:00,000T02:00:00,5-May-12,ISS,Prime,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 81.5 requested range 0.7 Mkm",,,,,, 2012-126T09:47:00,000T02:00:00,5-May-12,CIRS,SPASS Rider,Titan,M90R1CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-126T09:47:00,000T02:00:00,5-May-12,VIMS,SPASS Rider,Titan,M90R1CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 82 deg, range =0.7 Mkm.",,,,,, 2012-126T11:47:00,000T13:00:00,5-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-127T00:47:00,000T09:00:00,6-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-127T01:47:00,000T08:00:00,6-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12127_SP,rider,,,,,, 2012-127T09:47:00,000T14:45:00,6-May-12,ISS,Prime,Titan,LRMONITOR,Long range monitor,LRM (Long Range Monitoring),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-127T09:47:00,000T14:45:00,6-May-12,CIRS,SPASS Rider,Titan,LRMONITOR,Long range monitor,Long Range Monitor,,,,,,, 2012-127T09:47:00,000T23:45:00,6-May-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-128T00:32:00,000T04:30:00,7-May-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-128T00:32:00,000T09:00:00,7-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-128T01:32:00,000T08:00:00,7-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12128_SP,rider,,,,,, 2012-128T09:32:00,000T02:00:00,7-May-12,ISS,Prime,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 37.3 requested range 0.9 Mkm",,,,,, 2012-128T09:32:00,000T02:00:00,7-May-12,CIRS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-128T09:32:00,000T02:00:00,7-May-12,VIMS,SPASS Rider,Titan,M60R1CLD,Titan cloud monitor campaign,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 37 deg, range =0.9 Mkm.",,,,,, 2012-128T09:32:00,003T23:56:00,7-May-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-128T11:32:00,001T17:45:00,7-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-129T09:28:00,000T20:00:00,8-May-12,CDA,SPASS Rider,DustRAM direction,ISD0046,,CDA ISD 2012-132T09:28:00,ISD observation around apoapse 2012-132T09:28:00 40.303042 Rs,,,,,, 2012-130T06:47:00,000T09:00:00,9-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-130T07:47:00,000T08:00:00,9-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12130_SP,rider,,,,,, 2012-130T08:00:00,000T03:30:00,9-May-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-130T15:47:00,000T07:00:00,9-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-131T00:17:00,000T09:00:00,10-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-131T03:28:00,000T20:00:00,10-May-12,CDA,SPASS Rider,DustRAM direction,ISD0046,,CDA ISD 2012-132T09:28:00,ISD observation around apoapse 2012-132T09:28:00 40.303042 Rs,,,,,, 2012-131T09:17:00,000T13:30:00,10-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-132T00:17:00,000T09:00:00,11-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-132T01:17:00,000T08:00:00,11-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_165IC_DSCAL12131_SP,rider,,,,,, 2012-132T09:17:00,000T01:30:00,11-May-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 34.4 requested range 2.6 Mkm",,,,,, 2012-132T09:17:00,000T01:30:00,11-May-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-132T09:17:00,000T01:30:00,11-May-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 34 deg, range =2.6 Mkm.",,,,,, 2012-132T09:28:00,007T20:12:56,11-May-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.011610 Rs exit= 14.010733 Range altitude= 1576.8851 km ... 2485.2715,,,,,, 2012-132T09:28:00,000T00:05:00,11-May-12,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,Load IEBs,,,,,, 2012-132T09:28:00,008T15:48:00,11-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAG_165_166",,,,,, 2012-132T09:28:00,007T17:34:32,11-May-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-132T09:28:15,000T00:00:01,11-May-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 17.8 d, inc = 0.4 deg, r = 40.266 Rs, phase = 62 deg",,,,,, 2012-132T09:33:00,000T00:33:00,11-May-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,MRO,,,,,, 2012-132T10:06:00,000T01:22:00,11-May-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-132T10:47:00,000T08:00:00,11-May-12,ISS,Prime,Other,ERRPHA,,Erriapus,Observation of irregular moon of Saturn.,,,,,, 2012-132T11:28:00,002T21:33:00,11-May-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-132T18:47:00,000T04:00:00,11-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-132T19:28:00,000T20:00:00,11-May-12,CDA,SPASS Rider,DustRAM direction,ISD0046,,CDA ISD 2012-132T09:28:00,ISD observation around apoapse 2012-132T09:28:00 40.303042 Rs,,,,,, 2012-133T00:17:00,000T09:00:00,12-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-133T01:17:00,000T08:00:00,12-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12132_SP,rider,,,,,, 2012-133T09:17:00,000T01:30:00,12-May-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 40.6 requested range 2.9 Mkm",,,,,, 2012-133T09:17:00,000T01:30:00,12-May-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-133T09:17:00,000T01:30:00,12-May-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 41 deg, range =2.9 Mkm.",,,,,, 2012-133T10:47:00,000T12:00:00,12-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-134T00:17:00,000T09:00:00,13-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-134T01:17:00,000T08:00:00,13-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12133_SP,rider,,,,,, 2012-134T09:17:00,000T01:30:00,13-May-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 48 requested range 3.1 Mkm",,,,,, 2012-134T09:17:00,000T01:30:00,13-May-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-134T09:17:00,000T01:30:00,13-May-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 48 deg, range =3.1 Mkm.",,,,,, 2012-134T12:17:00,000T11:04:00,13-May-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-134T13:28:00,000T20:00:00,13-May-12,CDA,SPASS Rider,DustRAM direction,ISD0046,,CDA ISD 2012-132T09:28:00,ISD observation around apoapse 2012-132T09:28:00 40.303042 Rs,,,,,, 2012-135T00:01:00,000T09:00:00,14-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-135T01:01:00,000T08:00:00,14-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12134_SP,rider,,,,,, 2012-135T09:01:00,000T07:00:00,14-May-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-135T09:01:00,001T00:00:00,14-May-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-135T16:01:00,000T08:00:00,14-May-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-135T16:01:00,000T08:00:00,14-May-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-135T16:01:00,000T08:00:00,14-May-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare greyscale,"CL1 NAC 4x4 images. 10 Mbits/hr, only half of the time expected to be a stare",,,,,, 2012-135T16:01:00,000T08:00:00,14-May-12,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Stare Ridealong.,Auroral Stare Ridealong,,,,,, 2012-135T16:01:00,004T16:45:00,14-May-12,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2012-136T00:01:00,000T09:00:00,15-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-136T01:01:00,000T08:00:00,15-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12135_SP,rider,,,,,, 2012-136T09:01:00,000T13:30:00,15-May-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-136T09:01:00,000T13:30:00,15-May-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-136T09:01:00,000T13:30:00,15-May-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare greyscale,"CL1 NAC 4x4 images. 10 Mbits/hr, only half of the time expected to be a stare",,,,,, 2012-136T09:01:00,000T13:30:00,15-May-12,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Stare Ridealong.,Auroral Stare Ridealong,,,,,, 2012-136T09:01:00,003T01:59:00,15-May-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-136T10:00:00,000T07:00:00,15-May-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-137T00:01:00,000T09:00:00,16-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-137T01:01:00,000T08:00:00,16-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12136_SP,rider,,,,,, 2012-137T02:00:00,000T02:00:00,16-May-12,RPWS,Non-SPASS,co-rotation,HIRATE,High rate mode,RPWS High Rate Campaign,RPWS high rate observations when we have extra bits,,,,,, 2012-137T09:01:00,000T01:30:00,16-May-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 76.5 requested range 3.1 Mkm",,,,,, 2012-137T09:01:00,000T01:30:00,16-May-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-137T09:01:00,000T01:30:00,16-May-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 76 deg, range =3.1 Mkm.",,,,,, 2012-137T10:31:00,000T11:45:00,16-May-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-137T10:31:00,000T11:45:00,16-May-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-137T10:31:00,000T11:45:00,16-May-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare greyscale,"CL1 NAC 4x4 images. 10 Mbits/hr, only half of the time expected to be a stare",,,,,, 2012-137T10:31:00,000T11:45:00,16-May-12,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Stare Ridealong.,Auroral Stare Ridealong,,,,,, 2012-137T19:46:00,000T13:00:00,16-May-12,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,"RSS USO characterization plus PIM. Pointing=XBAND to Earth. No rolling during 3-hour USO from 2012-137T23:46:00 till 2012-138T02:46:00, to be tracked at DSS-25 in 1-way mode. Keep Ka-band ON till end of downlink at 2012-138T08:46:00 to satisfy PIM requirement.",,,,,, 2012-137T23:46:00,000T09:00:00,16-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-138T00:46:00,000T08:00:00,17-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12137_SP,rider,,,,,, 2012-138T08:46:00,000T12:00:00,17-May-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-138T08:46:00,000T12:00:00,17-May-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-138T08:46:00,000T12:00:00,17-May-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare greyscale,"CL1 NAC 4x4 images. 10 Mbits/hr, only half of the time expected to be a stare",,,,,, 2012-138T08:46:00,000T12:00:00,17-May-12,VIMS,,Saturn,AURSTARE,Saturn aurora,UVIS Auroral Stare Ridealong.,Auroral Stare Ridealong,,,,,, 2012-138T20:46:00,000T01:30:00,17-May-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 89.1 requested range 2.8 Mkm",,,,,, 2012-138T20:46:00,000T01:30:00,17-May-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-138T20:46:00,000T01:30:00,17-May-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 89 deg, range =2.8 Mkm.",,,,,, 2012-138T23:46:00,000T09:00:00,17-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-139T00:46:00,000T08:00:00,18-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12138_SP,rider,,,,,, 2012-139T08:46:00,000T15:00:00,18-May-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-139T08:46:00,000T15:00:00,18-May-12,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,null,,,,,, 2012-139T08:46:00,000T15:00:00,18-May-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong,Auroral Slew UVIS Ridealong,,,,,, 2012-139T11:00:00,000T00:34:00,18-May-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,MRO,,,,,, 2012-139T11:34:00,000T01:26:00,18-May-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-139T13:00:00,000T19:46:00,18-May-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-139T23:46:00,000T09:00:00,18-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-140T00:00:00,000T01:08:00,19-May-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-140T00:46:00,000T08:00:00,19-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12139_SP,rider,,,,,, 2012-140T03:02:32,000T22:13:28,19-May-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-140T05:40:56,002T01:30:00,19-May-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 13.997863 Rs exit= 13.991282 Range altitude= 2479.6701 km ... 5091.5760,,,,,, 2012-140T08:46:00,000T07:30:00,19-May-12,CAPS,Prime,Saturn,EQIMAGPTG,,Equatorial Inner Magnetosphere pointing,null,,,,,, 2012-140T08:46:00,000T02:24:51,19-May-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-140T08:46:00,000T00:40:00,19-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-140T09:26:00,000T06:10:00,19-May-12,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2012-140T11:10:51,000T04:56:46,19-May-12,INMS,Non-SPASS,Methone,M1RPA,,Methone Ring Plane Observation,Observe neutral molecules in the Methone equatorial plane,,,,,, 2012-140T15:36:00,000T09:40:00,19-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-140T16:07:37,000T09:08:23,19-May-12,INMS,Non-SPASS,Methone,M1INBND,,Methone flyby,Enceladus observation,,,,,, 2012-140T16:16:00,000T09:00:00,19-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-140T17:16:00,000T08:00:00,19-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12140_SP,rider,,,,,, 2012-140T18:20:56,000T02:00:00,19-May-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-140T18:21:56,000T02:00:00,19-May-12,CDA,SPASS Rider,DustRAM direction,RPX0440,,CDA RPXing 2012-140T19:21:56,RPXing at 8.0155113 Rs,,,,,, 2012-140T20:42:00,000T04:34:00,19-May-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-141T01:16:00,001T07:14:59,20-May-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-141T01:16:00,000T00:56:00,20-May-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-141T01:16:00,000T01:14:00,20-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-141T01:16:00,001T07:15:00,20-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SOST_166",,,,,, 2012-141T01:16:00,000T08:55:00,20-May-12,RPWS,Non-SPASS,Saturn,CHORUS,,RPWS CHORUS Campaign,"Part of RPWS Chorus campaign, attempt to get high rate data from within L Shell of 8",,,,,, 2012-141T01:16:00,001T08:33:55,20-May-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-141T01:17:00,000T05:17:00,20-May-12,CIRS,Prime,Tethys,TETHYS,Tethys,,"Shutter closed details: 15.67 cm-1 resolution No Add, FP1 Data, FP3 Data, FP3 Blink, FP4 Data, FP4 Blink. Requested shutter closed times: 2012-141T01:17:00-01:21:00 and 2012-141T02:47:00-02:52:00 and 2012-141T04:28:00-04:33:00 This is a high spatial resolution observation of Tethys' leading hemisphere at low phase. 01:16 - 01:36 Turn 01:36 - 02:00 FP1 raster scan at Nyquist sampling 02:00 - 02:45 ISS mosaic 02:45 - 03:50 Single FP3/4 N/S swath centered on 360W longitude at 6 mu rad /s 03:50 - 04:10 FP1 raster scan at Nyquist sampling 04:10 - 04:30 Quiescent Period perhaps including secondary turn? 04:30 - 05:30 Single FP3/4 N/S swath 6 mu rad /s, centered on Tethys' leading hemisphere so that there's 1 to 2 FP3 detector overlap with previous FP3 observation. 05:30 - 05:40 FP1 raster scan at Nyquist sampling 05:40 - 06:34 Cover remainder of disk with FP3, up to 12 murad/sec, whatever it takes to get a global map (or perhaps just the longitudes not covered previously). 06:34 Hand off. ISS request info from Tilmann: An ISS mosaic is desired. (DOY 2012-141T2.00-2.45) It should start on the eastern side (terminator) and then go ""up and down"", with each ""stripe"" shifted to the west. I guess the first stripe (near the terminator) should be a 1x5 or 1x6 mosaic, and the next ones (toward west) also 1x5, maybe 1x4 later. I guess it should be ~4 such stripes, but we have to see in pdt what is actually needed to get an as complete as possible coverage. Dwell should be 2 minutes for VIMS.",,,,,, 2012-141T01:17:00,000T05:17:00,20-May-12,ISS,,Tethys,TETHYS,Tethys,Tethys ORS observation,ORS observation,,,,,, 2012-141T01:17:00,000T05:17:00,20-May-12,UVIS,SPASS Rider,Tethys,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-141T01:17:00,000T05:16:00,20-May-12,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys composition,"Tethys composition, follow cirs",,,,,, 2012-141T02:12:00,000T01:05:00,20-May-12,INMS,Non-SPASS,Methone,M1RPA,,Methone Ring Plane Observation,Observe neutral molecules in the Methone equatorial plane,,,,,, 2012-141T02:30:00,000T07:55:00,20-May-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-141T03:17:00,000T01:40:37,20-May-12,INMS,Non-SPASS,Methone,M1INBND,,Methone flyby,Enceladus observation,,,,,, 2012-141T04:57:37,000T04:00:00,20-May-12,INMS,Non-SPASS,Methone,METHONE1,,Methone encounter,Methone observation,,,,,, 2012-141T06:26:25,000T00:00:01,20-May-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.222 Rs, lat = -0 deg, phase = 119 deg",,,,,, 2012-141T06:34:00,000T01:52:00,20-May-12,ISS,Prime,Methone,METHONE,,Methone ORS observation,ORS observation,,,,,, 2012-141T06:34:00,000T01:52:00,20-May-12,CIRS,,Methone,METHONE,,,null,,,,,, 2012-141T06:34:00,000T01:52:00,20-May-12,UVIS,,Methone,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-141T06:34:00,000T01:52:00,20-May-12,VIMS,SPASS Rider,Methone,METHONE,,Methone composition,"Methone composition, follow iss",,,,,, 2012-141T08:26:00,000T03:00:00,20-May-12,CAPS,Prime,Saturn,EINMAGPTG,,Equatorial Inner Magnetosphere pointing,null,,,,,, 2012-141T08:26:00,000T04:00:00,20-May-12,UVIS,,InstrumentCalibration,ALPVIR,Alpha Virginis occultation,UVIS calibration,"Typical slew rate for calibrations is 0.02mrad/s, and for this observation we request 5x slower (0.004mrad/s). The integration time is typically 45sec, and we request a decreased integration time of nominally 2x lower (i.e. 20sec), but may be adjusted to accommodate data volume constraints.",,,,,, 2012-141T08:57:37,000T00:37:23,20-May-12,INMS,Non-SPASS,Methone,M1OUTBND,,Methone flyby,Methone observation,,,,,, 2012-141T09:35:00,000T01:06:00,20-May-12,INMS,Non-SPASS,Methone,M1RPA,,Methone Ring Plane Observation,Observe neutral molecules in the Methone equatorial plane,,,,,, 2012-141T10:10:46,000T02:00:00,20-May-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-141T10:11:56,000T02:00:00,20-May-12,CDA,SPASS Rider,DustRAM direction,RPX0450,,CDA RPXing 2012-141T11:11:56,RPXing at 4.7357587 Rs,,,,,, 2012-141T10:25:00,000T10:56:00,20-May-12,MAG,Non-SPASS,Other,EQINMAG,,EqInMAG PIE,MAPS Eq_In_MAG PIE observation,,,,,, 2012-141T10:41:00,000T08:16:37,20-May-12,INMS,Non-SPASS,Methone,M1RPA,,Methone Ring Plane Observation,Observe neutral molecules in the Methone equatorial plane,,,,,, 2012-141T11:26:00,000T10:35:00,20-May-12,CAPS,Prime,Saturn,EINMAGPTG,,Equatorial Inner Magnetosphere pointing,null,,,,,, 2012-141T18:57:37,000T13:33:23,20-May-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-141T21:21:00,000T11:10:00,20-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-141T23:31:00,000T09:00:00,20-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-142T00:31:00,000T08:00:00,21-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12141_SP,rider,,,,,, 2012-142T07:10:56,006T22:04:04,21-May-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 14.004159 Rs exit= 4.2471232 Range altitude= 5098.0882 km ... -40023.636,,,,,, 2012-142T08:31:00,000T14:39:11,21-May-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-142T08:31:00,000T02:39:51,21-May-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-142T08:31:00,000T12:39:11,21-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-142T08:31:00,001T17:30:00,21-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_166_T83",,,,,, 2012-142T09:26:00,000T06:44:11,21-May-12,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan,"VIMS global mapping of Titan and specular reflection observations. Phase = 164.985 deg, SSC Lat/Lon = 0.581N/7.561 deg. SS Lat/Lon = 14.359N/186.051 deg. Alt = 313770.8 km, range = 316345.8 km. Resolution = 157 km/px. Temp. O extended. Obtain cubes for global mapping of Titan and specular reflection.",,,,,, 2012-142T09:26:00,000T06:44:11,21-May-12,ISS,,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-142T09:49:55,001T16:11:05,21-May-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-142T11:10:11,000T05:00:00,21-May-12,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride along with VIMS.,,,,,, 2012-142T11:10:51,000T01:59:20,21-May-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-142T13:10:11,000T11:00:00,21-May-12,INMS,Non-SPASS,Titan,T83INBND,,Titan flyby,Titan observation,,,,,, 2012-142T16:10:11,000T04:00:00,21-May-12,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2012-142T16:10:11,000T04:00:00,21-May-12,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-142T16:10:11,000T04:00:00,21-May-12,VIMS,,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping.,"VIMS ridealong with CIRS for mapping of Titan's limb. Phase = 164.375 deg, SSC Lat/Lon = 1.107N/14.621 deg. SS Lat/Lon = 14.363N/192.397 deg. Alt = 175644.913 km, range = 178219.913 km. Resolution = 88 km/px. Temp. R. Obtain cubes of Titan's limb.",,,,,, 2012-142T16:10:11,000T04:00:00,21-May-12,UVIS,Non-SPASS,Titan,MIRLMBINT,Mid infrared limb integration,Rider with CIRS MIRLMBINT,Rider with CIRS MIRLMBINT,,,,,, 2012-142T19:43:11,000T03:00:00,21-May-12,RADAR,Non-SPASS,Titan,T83WARMUP,,Warmup for T83,,,,,,, 2012-142T20:10:11,000T02:33:00,21-May-12,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2012-142T20:10:11,000T02:33:00,21-May-12,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-142T20:10:11,000T02:33:00,21-May-12,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 163.365 deg, SSC Lat/Lon = 2.053N/18.863 deg. SS Lat/Lon = 14.364N/196.158 deg. Alt = 96348.2 km, range = 98923.2 km. Resolution = 48 km/px. Temp. T. Obtain cubes while scanning across Titan.",,,,,, 2012-142T21:10:11,000T08:00:00,21-May-12,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T83 flyby,"T83 is a low altitude (990 km) north polar flyby in the post noon sector of Saturn's magnetosphere. With closest approach slightly in the dayside ionosphere, Cassini will be able to study the diffusion of the external magnetic field at low altitudes and high solar zenith angles. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2012-142T22:43:11,000T01:15:00,21-May-12,RADAR,Prime,Titan,T83INSCAT,,T83 Inbound Scatterometry,,,,,,, 2012-142T23:10:11,000T01:00:00,21-May-12,CAPS,SPASS Rider,Titan,T83INBND,,Inbound 166TI (T83),null,,,,,, 2012-142T23:10:11,000T01:00:00,21-May-12,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-142T23:10:11,000T01:00:00,21-May-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-142T23:58:11,000T00:41:00,21-May-12,RADAR,Prime,Titan,T83IHISAR,,T83 Inbound HiSAR,,,,,,, 2012-143T00:10:11,000T02:00:00,22-May-12,CAPS,SPASS Rider,Titan,T83CLOSE,,Closest Approach 166TI (T83),null,,,,,, 2012-143T00:10:11,000T02:00:00,22-May-12,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-143T00:10:11,000T00:45:00,22-May-12,INMS,Non-SPASS,Titan,TITAN83,,Titan Flyby,Titan observation,,,,,, 2012-143T00:10:11,000T02:00:00,22-May-12,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2012-143T00:40:11,000T00:15:00,22-May-12,RADAR,Prime,Titan,T83INALT,,T83 Inbound Altimetry,,,,,,, 2012-143T00:55:11,000T00:10:00,22-May-12,RADAR,Prime,Titan,T83IRASAR,,T83 Inbound Ride-along SAR,,,,,,, 2012-143T00:55:11,000T00:10:30,22-May-12,INMS,SPASS Rider,Titan,TITAN83,,Titan Flyby,Titan observation,,,,,, 2012-143T01:05:11,000T00:05:00,22-May-12,RADAR,Prime,Titan,T83IRASAR,,T83 Inbound Ride-along SAR,,,,,,, 2012-143T01:05:41,000T00:08:40,22-May-12,INMS,Non-SPASS,Titan,TITAN83,,Titan Flyby,Titan observation,,,,,, 2012-143T01:10:11,000T00:18:00,22-May-12,RADAR,Prime,Titan,T83OUTSAR,,T83 Outbound SAR,,,,,,, 2012-143T01:14:21,000T00:55:50,22-May-12,INMS,Non-SPASS,Titan,TITAN83,,Titan Flyby,Titan observation,,,,,, 2012-143T01:28:11,000T00:12:00,22-May-12,RADAR,Prime,Titan,T83OUTALT,,T83 Outbound Altimetry,,,,,,, 2012-143T01:40:11,000T00:20:00,22-May-12,RADAR,Prime,Titan,T83OHISAR,,T83 Outbound HiSAR,,,,,,, 2012-143T02:10:11,000T01:00:00,22-May-12,CAPS,SPASS Rider,Titan,T83OUTBND,,Outbound 166TI (T83),null,,,,,, 2012-143T02:10:11,000T01:00:00,22-May-12,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-143T02:10:11,000T11:00:00,22-May-12,INMS,Non-SPASS,Titan,T83OUTBND,,Titan flyby,Titan observation,,,,,, 2012-143T02:10:11,000T01:00:00,22-May-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-143T02:22:11,000T01:03:00,22-May-12,RADAR,Prime,Titan,T83OUTSCT,,T83 Outbound Scatterometry,,,,,,, 2012-143T03:10:11,000T22:50:49,22-May-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-143T03:25:11,000T03:45:00,22-May-12,RADAR,Prime,Titan,T83OUTRAD,,T83 Outbound Radiometry,,,,,,, 2012-143T05:10:11,000T20:50:49,22-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-143T07:10:11,000T03:00:00,22-May-12,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan.,"VIMS global mapping of Titan. Phase = 21.6 deg, SSC Lat/Lon = 6.861S/210.665 deg. SS Lat/Lon = 14.369N/206.500 deg. Alt = 115998.6 km, range = 118573.6 km. Resolution = 58 km/px. Temp. I1. Obtain 2x2 mosaics and cubes for global mapping of Titan at medium resolution.",,,,,, 2012-143T07:10:11,000T03:00:00,22-May-12,CIRS,SPASS Rider,Titan,CLOUDMAP,Cloud map,,Ride along with VIMS.,,,,,, 2012-143T07:10:11,000T03:00:00,22-May-12,ISS,,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-143T10:10:11,000T05:35:49,22-May-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-143T10:10:11,000T02:00:00,22-May-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-143T10:10:11,000T04:55:49,22-May-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan.,"VIMS ridealong with CIRS while staring at Titan. Phase = 22.2 deg, SSC Lat/Lon = 7.42S/213.521 deg. SS Lat/Lon = 14.370N/209.320 deg. Alt = 175218.9 km, range = 177793.9 km. Resolution = 88 km/px. Temp. C. Obtain 160 and 640 ms cubes of Titan.",,,,,, 2012-143T10:10:11,000T03:00:00,22-May-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-143T13:10:11,000T12:50:49,22-May-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-143T16:01:00,000T10:00:00,22-May-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev167 Saturn rings occultation on 2012/156. DSS-63 and DSS-14 required for X- and S-band support.",,,,,, 2012-143T16:01:00,000T09:00:00,22-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-143T17:01:00,000T09:00:00,22-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12143_SP,rider,,,,,, 2012-144T02:01:00,012T11:44:00,23-May-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-144T02:01:00,002T06:15:00,23-May-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-144T02:01:00,007T05:59:00,23-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-144T02:01:00,005T03:15:00,23-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_166_167",,,,,, 2012-144T02:01:00,005T03:15:00,23-May-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-144T02:38:00,000T00:02:00,23-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-144T02:40:00,000T01:50:00,23-May-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 001 ST OB SET IN REV 166","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-144T04:28:00,000T00:02:00,23-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-144T04:28:00,000T00:02:00,23-May-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Stiorm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-144T06:00:00,000T14:50:00,23-May-12,ISS,Prime,rings(general),FNTLPMOV,,Faint Ring observation at low phase,Faint Ring Observation at low phase,,,,,, 2012-144T06:00:00,000T14:50:00,23-May-12,CIRS,SPASS Rider,rings(general),FNTLPMOV,,,null,,,,,, 2012-144T06:00:00,000T14:50:00,23-May-12,UVIS,SPASS Rider,rings(general),FNTLPMOV,,,ISS rider,,,,,, 2012-144T06:00:00,000T14:50:00,23-May-12,VIMS,SPASS Rider,rings(general),FNTLPMOV,,Faint ring movie and Strmwatch,Low phase arc or D-Ring observation and Saturn Stormwatch,,,,,, 2012-144T20:48:00,000T00:02:00,23-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-144T23:16:00,000T09:00:00,23-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-145T00:16:00,000T08:00:00,24-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12144_SP,rider,,,,,, 2012-145T08:16:00,000T15:00:00,24-May-12,CDA,Prime,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._); outound-leg",,,,,, 2012-145T23:16:00,000T09:00:00,24-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-146T00:16:00,000T08:00:00,25-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12145_SP,rider,,,,,, 2012-146T05:15:00,000T20:00:00,25-May-12,CDA,SPASS Rider,DustRAM direction,ISD0047,,CDA ISD 2012-149T05:15:00,ISD observation around apoapse 2012-149T05:15:00 37.467580 Rs,,,,,, 2012-146T08:16:00,000T15:00:00,25-May-12,ISS,Prime,Star,CALSTAR1,Stellar Calibration,ISS Photometric Calibration Star 1,Photometric Calibration Star 1 (Vega),,,,,, 2012-146T08:16:00,001T00:00:00,25-May-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-146T23:16:00,000T09:00:00,25-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-147T00:16:00,000T08:00:00,26-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12146_SP,rider,,,,,, 2012-147T08:16:00,000T13:30:00,26-May-12,CDA,Prime,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._); APO-Leg",,,,,, 2012-147T08:16:00,001T21:00:00,26-May-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-147T23:15:00,000T20:00:00,26-May-12,CDA,SPASS Rider,DustRAM direction,ISD0047,,CDA ISD 2012-149T05:15:00,ISD observation around apoapse 2012-149T05:15:00 37.467580 Rs,,,,,, 2012-147T23:16:00,000T09:00:00,26-May-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev167 Saturn rings occultation on 2012/156. DSS-25 required for X- and Ka-band support.",,,,,, 2012-147T23:16:00,000T09:00:00,26-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-148T00:16:00,000T08:00:00,27-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12147_SP,rider,,,,,, 2012-148T08:54:00,000T00:02:00,27-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-148T08:56:00,000T01:30:00,27-May-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 32 requested range 2.5 Mkm",,,,,, 2012-148T08:56:00,000T01:30:00,27-May-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-148T08:56:00,000T01:30:00,27-May-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch; phase = 32 deg, range =2.5 Mkm.",,,,,, 2012-148T10:24:00,000T00:02:00,27-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-148T10:26:00,000T01:00:00,27-May-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-148T11:24:00,000T00:02:00,27-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-148T11:24:00,000T00:02:00,27-May-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-148T21:30:00,000T06:00:00,27-May-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-148T23:00:00,000T09:00:00,27-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-149T00:00:00,000T08:00:00,28-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_166IC_DSCAL12148_SP,rider,,,,,, 2012-149T05:15:00,007T19:47:56,28-May-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 14.004159 Rs exit= 4.2471232 Range altitude= 5098.0882 km ... -40023.636,,,,,, 2012-149T05:15:50,000T00:00:01,28-May-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 16.0 d, inc = 15.8 deg, r = 37.437 Rs, phase = 61 deg",,,,,, 2012-149T05:16:00,000T02:00:00,28-May-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-149T05:16:00,007T08:29:00,28-May-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_166_167",,,,,, 2012-149T05:16:00,006T20:04:00,28-May-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-149T07:16:00,002T00:44:00,28-May-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-149T08:00:00,000T13:30:00,28-May-12,CDA,Prime,DustRAM direction,ISD0047,,CDA ISD 2012-149T05:15:00,ISD observation around apoapse 2012-149T05:15:00 37.467580 Rs,,,,,, 2012-149T23:00:00,000T09:00:00,28-May-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev167 Saturn rings occultation on 2012/156. DSS-25 required for X- and Ka-band support.",,,,,, 2012-149T23:00:00,000T09:00:00,28-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-150T00:00:00,000T08:00:00,29-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12149_SP,rider,,,,,, 2012-150T08:38:00,000T00:02:00,29-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-150T08:40:00,000T01:30:00,29-May-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 46.1 requested range 3.1 Mkm",,,,,, 2012-150T08:40:00,000T01:30:00,29-May-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-150T08:40:00,000T01:30:00,29-May-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch; phase = 46 deg, range =3.09 Mkm.",,,,,, 2012-150T10:08:00,000T00:02:00,29-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-150T10:10:00,000T01:00:00,29-May-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OB SET IN REV 167","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-150T11:08:00,000T00:02:00,29-May-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-150T11:08:00,000T00:02:00,29-May-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-150T11:50:00,000T11:10:00,29-May-12,ISS,Prime,Other,YMIROT,,Ymir,Observation of irregular moon of Saturn.,,,,,, 2012-150T23:00:00,000T09:00:00,29-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-151T00:00:00,000T08:00:00,30-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12150_SP,rider,,,,,, 2012-151T08:00:00,000T08:00:00,30-May-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-151T08:00:00,001T00:00:00,30-May-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-151T09:15:00,000T20:00:00,30-May-12,CDA,SPASS Rider,DustRAM direction,ISD0047,,CDA ISD 2012-149T05:15:00,ISD observation around apoapse 2012-149T05:15:00 37.467580 Rs,,,,,, 2012-151T16:00:00,004T21:45:00,30-May-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-151T23:00:00,000T09:00:00,30-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-152T00:00:00,000T08:00:00,31-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12151_SP,rider,,,,,, 2012-152T08:00:00,003T16:15:00,31-May-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-152T15:15:00,000T09:00:00,31-May-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev167 Saturn rings occultation on 2012/156. DSS-55 required for X- and Ka-band support.",,,,,, 2012-152T15:15:00,000T09:00:00,31-May-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-152T16:15:00,000T08:00:00,31-May-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12152_SP,rider,,,,,, 2012-153T00:53:00,000T00:02:00,1-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-153T00:55:00,000T01:30:00,1-Jun-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 71.6 requested range 3.1 Mkm",,,,,, 2012-153T00:55:00,000T01:30:00,1-Jun-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-153T00:55:00,000T01:30:00,1-Jun-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stirmwatch,"Titan Monitoring Campaign and Stormwatch; phase = 72 deg, range =3.09 Mkm.",,,,,, 2012-153T02:17:00,000T01:08:00,1-Jun-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-153T02:23:00,000T00:02:00,1-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-153T02:25:00,000T01:00:00,1-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 005 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-153T03:23:00,000T00:02:00,1-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-153T03:23:00,000T00:02:00,1-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-153T03:25:00,000T04:00:00,1-Jun-12,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2012-153T03:25:00,000T04:00:00,1-Jun-12,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2012-153T07:23:00,000T00:02:00,1-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-153T07:23:00,000T00:02:00,1-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-153T15:00:00,000T09:00:00,1-Jun-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev167 Saturn rings occultation on 2012/156. DSS-55 required for X- and Ka-band support.",,,,,, 2012-153T15:00:00,000T09:00:00,1-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-153T16:00:00,000T08:00:00,1-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12153_SP,rider,,,,,, 2012-154T00:38:00,000T00:02:00,2-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-154T00:40:00,000T01:30:00,2-Jun-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 83.8 requested range 2.8 Mkm",,,,,, 2012-154T00:40:00,000T01:30:00,2-Jun-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-154T00:40:00,000T01:30:00,2-Jun-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch; phase = 84 deg, range =2.85 Mkm.",,,,,, 2012-154T02:08:00,000T00:02:00,2-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-154T02:10:00,000T01:00:00,2-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-154T03:08:00,000T00:02:00,2-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-154T03:08:00,000T00:02:00,2-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-154T12:00:00,002T00:00:00,2-Jun-12,CDA,SPASS Rider,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._); inbound leg",,,,,, 2012-154T15:15:00,000T09:00:00,2-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-154T16:15:00,000T08:00:00,2-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12154_SP,rider,,,,,, 2012-155T00:58:00,000T00:02:00,3-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-155T01:00:00,000T13:00:00,3-Jun-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-155T01:00:00,000T13:00:00,3-Jun-12,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,South pole rider FP1 may be off planet. UVIS slews to track auroral oval.,,,,,, 2012-155T01:00:00,000T13:00:00,3-Jun-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stormwatch,Auroral Slew UVIS Ridealong and Stormwatch,,,,,, 2012-155T13:58:00,000T00:02:00,3-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-155T15:15:00,000T09:00:00,3-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-155T16:15:00,000T08:00:00,3-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12155_SP,rider,,,,,, 2012-156T00:15:00,000T03:06:35,4-Jun-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-156T01:20:00,000T12:25:00,4-Jun-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-156T03:21:35,000T10:23:25,4-Jun-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-156T04:45:00,000T09:00:00,4-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-156T05:45:00,000T08:00:00,4-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12156_SP,rider,,,,,, 2012-156T13:45:00,000T06:15:00,4-Jun-12,ISS,Prime,rings(general),PROPSURVY,,Azimuthal survey of the propeller region,Aim for full longitudinal coverage of the trans-Encke region to reacquire giant propellers. Part 1 of a two-part survey.,,,,,, 2012-156T13:45:00,000T06:15:00,4-Jun-12,CIRS,SPASS Rider,rings(general),PROPSURVY,,CIRS_167IRI_PROPSURVY001_ISS,rider,,,,,, 2012-156T13:45:00,000T06:15:00,4-Jun-12,UVIS,SPASS Rider,rings(general),PROPSURVY,,,ISS rider,,,,,, 2012-156T13:45:00,001T17:44:00,4-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-156T13:45:00,000T12:36:35,4-Jun-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-156T13:45:00,000T10:55:00,4-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-156T13:45:00,001T17:44:00,4-Jun-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. RINGS_167",,,,,, 2012-156T13:45:00,001T17:44:00,4-Jun-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-156T19:37:00,000T01:25:00,4-Jun-12,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 167 RI OCC Thermal Stabilization,"A thermal stabilization period of 2 hrs and 5 min is required immediately prior to any radio science experiment which uses Ka-band or S-band. Note that the observation period of the corresponding science request includes a budgeted 40 min waypoint turn that can be considered as part of the warmup time. Hence, the total duration of this warmup request is shorter than the required 2 hrs and 5 min by those 40 min (that is, only 1 hr and 25 min). The duration should be increased back to the original 2 hrs 5 min if a waypoint turn proves unnecessary.",,,,,, 2012-156T20:00:00,000T01:02:00,4-Jun-12,VIMS,Prime,rings(general),COMPDARK,,"Ring composition, dark face",160/640 msec tau_IR,,,,,, 2012-156T20:00:00,000T01:02:00,4-Jun-12,CIRS,SPASS Rider,rings(general),COMPDARK,,CIRS_167RI_COMPDARK001_VIMS,rider,,,,,, 2012-156T20:00:00,000T01:02:00,4-Jun-12,UVIS,SPASS Rider,rings(general),COMPDARK,,,VIMS rider,,,,,, 2012-156T21:02:00,000T04:15:00,4-Jun-12,RSS,Prime,rings(general),OCC,Occultation,RSS XXM Ring Occ - Ingress,Ingress ring occultation conducted using TBD bands (TBD Op-mode). The op-mode is selected based on power constraints. Observations will commence after a 2 hrs 5 min period of thermal stabilization (in RSS WARMUP op-mode).,,,,,, 2012-157T00:40:00,000T08:40:00,5-Jun-12,MAG,Non-SPASS,Other,INTFLD,MAG Internal field observation,MAG_Internal_Field_Measurements,This request will yield unique observations of Saturns internal magnetic field over a unique orbit track in latitude and longitude space.,,,,,, 2012-157T01:02:56,000T04:42:00,5-Jun-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 4.2310368 Rs exit= 3.1710234 Range altitude= -39488.338 km ... 39573.232,,,,,, 2012-157T01:20:00,000T04:00:00,5-Jun-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-157T01:50:00,000T01:57:00,5-Jun-12,UVIS,Prime,Sun,USUNOCC,Solar occultation,Saturn solar occ,"This is an egress solar occ by Saturn. Egress start time is 2011-157T02:24:55 and the line-of-sight impact parameter reaches the desired end distance of 2 Rs around the observation's end time, 2011-157T03:47:00. Unfortunately, the observation margin and allowance for waypoint turn at the end cut into the egress. I have compromised by keeping the observation margin at the requested 20 minutes and shortening the time for the waypoint turn from the usual 30 minutes to 10 minutes. The final LOS impact parameter then ends up at ~1.6 Rs which is smaller than ideal but better than the 1.36 Rs provided by the 30 minute waypoint turn. EUV occultation port centered on the Sun. 1) 20 minutes observation margin. 2) Record data from 2012-157T02:10:00 until 2012-157T03:17:00. 3) 20 minutes observation margin and 10 minutes for turn to waypoint. Note: Egress start and end times are based on the 091005 kernel. If the timing allows a later end for data collection, we will gladly shift the start of data collection closer to the start of the actual egress in exchange. Total data collection time: 000T01:07:00. Total observation request duration: 000T01:57:00. bps = 18918.883 bps (from Alain's spreadsheet). Total data volume = 76.054e+6 bits.",,,,,, 2012-157T01:50:00,000T01:57:00,5-Jun-12,VIMS,SPASS Rider,Saturn,USUNOCC,Solar occultation,Saturn Solar Occultation egress,Saturn Solar Occultation egress. UVIS ridealong. +36 Lat.,,,,,, 2012-157T02:21:35,000T00:50:25,5-Jun-12,INMS,SPASS Rider,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Magnetosphere Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-157T02:21:56,000T02:00:00,5-Jun-12,CDA,SPASS Rider,DustRAM direction,RPX0460,,CDA RPXing 2012-157T03:21:56,RPXing at 3.3261222 Rs,,,,,, 2012-157T03:12:00,000T01:09:35,5-Jun-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-157T03:47:00,000T05:13:00,5-Jun-12,CIRS,Prime,Mimas,MIMAS,Mimas,,"Shutter closed details: 15.67 cm-1 resolution No Add, FP1 Data, FP3 Data, FP3 Blink, FP4 Data, FP4 Blink. Requested shutter closed times: 2012-157T04:11:00-04:16:00 2012-157T06:04:00-06:09:00 2012-157T07:49:00-07:54:00 2012-157T08:41:00-08:46:00 Time",,,,,, 2012-157T03:47:00,000T05:13:00,5-Jun-12,ISS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas ORS observation,ORS observation,,,,,, 2012-157T03:47:00,000T05:13:00,5-Jun-12,VIMS,SPASS Rider,Mimas,MIMAS,Mimas,Mimas,follow CIRS,,,,,, 2012-157T04:00:00,000T03:30:00,5-Jun-12,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Region Campaign,Part of RPWS campaign to obtain high resolution WBR data in the narrow band emission source region,,,,,, 2012-157T04:15:00,000T01:47:00,5-Jun-12,UVIS,,Mimas,ICYLON,Icy satellite longitudinal coverage,ICYLON: Longitude / Phase Space Coverage,Target to icy satellite. Measure uv albedo across longitude / phase space. Opportunities selected by SOST-ORS consortium. Slit orientation is flexible.,,,,,, 2012-157T04:21:35,000T23:00:00,5-Jun-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-157T04:52:47,000T00:00:01,5-Jun-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 3.097 Rs, lat = 8 deg, phase = 119 deg",,,,,, 2012-157T05:44:56,001T01:44:04,5-Jun-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.1765580 Rs exit= 6.6706246 Range altitude= 40048.612 km ... -40205.640,,,,,, 2012-157T07:00:00,000T01:41:00,5-Jun-12,UVIS,,Mimas,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Mimas, ORS Rider",UV albedo map of Mimas's surface,,,,,, 2012-157T09:00:00,000T03:00:00,5-Jun-12,VIMS,Prime,rings(general),COMPLIT,,"Ring composition, lit face",160/640 msec tau_IR,,,,,, 2012-157T09:00:00,000T03:00:00,5-Jun-12,CIRS,SPASS Rider,rings(general),COMPLIT,,CIRS_167RI_COMPLIT001_VIMS,rider,,,,,, 2012-157T09:00:00,000T03:00:00,5-Jun-12,UVIS,SPASS Rider,rings(general),COMPLIT,,,VIMS rider,,,,,, 2012-157T09:20:00,000T22:09:00,5-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-157T12:00:00,000T08:19:00,5-Jun-12,ISS,Prime,rings(general),PROPSURVY,,Azimuthal survey of the propeller region,Aim for full longitudinal coverage of the trans-Encke region to reacquire giant propellers. Part 2 of a two-part survey.,,,,,, 2012-157T12:00:00,000T08:19:00,5-Jun-12,CIRS,SPASS Rider,rings(general),PROPSURVY,,CIRS_167RI_PROPSURVY002_ISS,rider,,,,,, 2012-157T12:00:00,000T08:19:00,5-Jun-12,UVIS,SPASS Rider,rings(general),PROPSURVY,,,ISS rider,,,,,, 2012-157T22:29:00,000T09:00:00,5-Jun-12,RSS,SPASS Rider,rings(general),GSE,,Gravity Science Enhancement (GSE),"Rings Occultation inbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-25 required for X- and Ka-band support.",,,,,, 2012-157T22:29:00,000T09:00:00,5-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-157T23:29:00,000T08:00:00,5-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12157_SP,rider,,,,,, 2012-158T03:21:35,000T04:07:25,6-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-158T07:29:00,000T14:38:21,6-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-158T07:29:00,002T23:45:00,6-Jun-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.1765580 Rs exit= 6.6706246 Range altitude= 40048.612 km ... -40205.640,,,,,, 2012-158T07:29:00,000T04:38:21,6-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-158T07:29:00,000T12:38:21,6-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-158T07:29:00,002T23:45:00,6-Jun-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_167_T84",,,,,, 2012-158T07:29:00,000T00:56:00,6-Jun-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-158T08:24:00,000T02:43:21,6-Jun-12,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2012-158T08:24:00,000T02:43:21,6-Jun-12,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-158T08:24:00,000T02:43:21,6-Jun-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS staring at Titan. Phase = 156.356 deg, SSC Lat/Lon = 8.823N/9.382 deg. SS Lat/Lon = 14.554N/185.808 deg. Alt = 314219.04 km, range = 316794.04 km. Resolution = 157 km/px. Temp. M4. Obtain cubes of 160 and 640 ms while staring at Titan. Look for specular reflection.",,,,,, 2012-158T08:25:00,001T13:49:00,6-Jun-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-158T11:07:21,000T04:00:00,6-Jun-12,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global mapping of Titan,"VIMS global mapping of Titan and specular reflection observations. Phase = 156.109 deg, SSC Lat/Lon = 9.046N/12.134 deg. SS Lat/Lon = 14.555N/188.394 deg. Alt = 257115.556 km, range = 259690.556 km. Resolution = 129 km/px. Temp. O. Obtain cubes for global mapping of Titan and specular reflection.",,,,,, 2012-158T11:07:21,000T04:00:00,6-Jun-12,CIRS,SPASS Rider,Titan,CLOUD,,,Ride along with VIMS.,,,,,, 2012-158T11:07:21,000T04:00:00,6-Jun-12,ISS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-158T12:07:21,000T11:00:00,6-Jun-12,INMS,Non-SPASS,Titan,T84INBND,,Titan flyby,Titan observation,,,,,, 2012-158T15:07:21,000T04:00:00,6-Jun-12,CIRS,Prime,Titan,MIRLMBINT,Mid infrared limb integration,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2012-158T15:07:21,000T04:00:00,6-Jun-12,ISS,SPASS Rider,Titan,MIRLMBINT,Mid infrared limb integration,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-158T15:07:21,000T04:00:00,6-Jun-12,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb mapping.,"VIMS ridealong with CIRS for limb mapping. Phase = 155.736 deg, SSC Lat/Lon = 9.418N/15.920 deg. SS Lat/Lon = 14.557N/192.155 deg. Alt = 176161.7 km, range = 178736.7 km. Resolution = 88 km/px. Temp. R. Obtain cubes of for limb mapping and specular reflection.",,,,,, 2012-158T15:07:21,000T04:00:00,6-Jun-12,UVIS,Non-SPASS,Titan,MIRLMBINT,Mid infrared limb integration,Rider with CIRS MIRLMBINT,Rider with CIRS MIRLMBINT,,,,,, 2012-158T18:52:21,000T03:00:00,6-Jun-12,RADAR,Non-SPASS,Titan,T84WARMUP,,Warmup for T84,,,,,,, 2012-158T19:07:21,000T02:45:00,6-Jun-12,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2012-158T19:07:21,000T02:45:00,6-Jun-12,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-158T19:07:21,000T02:45:00,6-Jun-12,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 155.112 deg, SSC Lat/Lon = 10.125N/19.126 deg. SS Lat/Lon = 14.559N/195.916 deg. Alt = 96666.8 km, range = 99241,8 km. Resolution = 48 km/px. Temp. T. Obtain cubes scanning across Titan. Possible specular reflection..",,,,,, 2012-158T20:07:21,000T08:00:00,6-Jun-12,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T84 flyby,"T84 is another low altitude (990 km) north polar flyby in the post noon sector of Saturn's magnetosphere. With closest approach slightly in the dayside ionosphere, Cassini will be able to study the diffusion of the external magnetic field at low altitudes and high solar zenith angles. A comparison with T83 will be useful. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2012-158T21:52:21,000T01:03:00,6-Jun-12,RADAR,Prime,Titan,T84INSCAT,,T84 Inbound Scatterometry,,,,,,, 2012-158T22:07:21,000T01:00:00,6-Jun-12,CAPS,SPASS Rider,Titan,T84INBND,,Inbound 167TI (T84),null,,,,,, 2012-158T22:07:21,000T01:00:00,6-Jun-12,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-158T22:07:21,000T01:00:00,6-Jun-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-158T22:55:21,000T00:41:00,6-Jun-12,RADAR,Prime,Titan,T84IHISAR,,T84 Inbound HiSAR,,,,,,, 2012-158T23:07:21,000T02:00:00,6-Jun-12,CAPS,SPASS Rider,Titan,T84CLOSE,,Closest Approach 167TI (T84),null,,,,,, 2012-158T23:07:21,000T02:00:00,6-Jun-12,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-158T23:07:21,000T00:52:27,6-Jun-12,INMS,Non-SPASS,Titan,TITAN84,,Titan Flyby,Titan observation,,,,,, 2012-158T23:07:21,000T02:00:00,6-Jun-12,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2012-158T23:37:21,000T00:12:00,6-Jun-12,RADAR,Prime,Titan,T84INALT,,T84 Inbound Altimetry,,,,,,, 2012-158T23:49:21,000T00:36:00,6-Jun-12,RADAR,Prime,Titan,T84INOSAR,,T84 Inbound and Outbound SAR,,,,,,, 2012-158T23:59:48,000T00:03:03,6-Jun-12,INMS,Non-SPASS,Titan,T84PHDIN,,Titan Flyby,Titan observation,,,,,, 2012-159T00:02:51,000T00:08:40,7-Jun-12,INMS,SPASS Rider,Titan,TITAN84,,Titan Flyby,Titan observation,,,,,, 2012-159T00:11:31,000T00:00:12,7-Jun-12,INMS,Non-SPASS,Titan,TITAN84,,Titan Flyby,Titan observation,,,,,, 2012-159T00:11:43,000T00:55:38,7-Jun-12,INMS,Non-SPASS,Titan,T84PHDOUT,,Titan Flyby,Titan observation,,,,,, 2012-159T00:25:21,000T00:12:00,7-Jun-12,RADAR,Prime,Titan,T84OUTALT,,T84 Outbound Altimetry,,,,,,, 2012-159T00:37:21,000T00:20:00,7-Jun-12,RADAR,Prime,Titan,T84OHISAR,,T84 Outbound HiSAR,,,,,,, 2012-159T01:07:21,000T01:00:00,7-Jun-12,CAPS,SPASS Rider,Titan,T84OUTBND,,Outbound 167TI (T84),null,,,,,, 2012-159T01:07:21,000T01:00:00,7-Jun-12,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-159T01:07:21,000T11:00:00,7-Jun-12,INMS,Non-SPASS,Titan,T84OUTBND,,Titan flyby,Titan observation,,,,,, 2012-159T01:07:21,000T01:00:00,7-Jun-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-159T01:19:21,000T01:03:00,7-Jun-12,RADAR,Prime,Titan,T84OUTSCT,,T84 Outbound Scatterometry,,,,,,, 2012-159T02:07:21,002T05:06:39,7-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-159T02:22:21,000T06:45:00,7-Jun-12,UVIS,Prime,Titan,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Titan,Several slow scans across Titan's visible hemisphere to form spectral images,,,,,, 2012-159T02:22:21,000T06:45:00,7-Jun-12,CIRS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,,Ride along with UVIS EUV-FUV scan,,,,,, 2012-159T02:22:21,000T06:45:00,7-Jun-12,ISS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-159T02:22:21,000T06:45:00,7-Jun-12,VIMS,SPASS Rider,Titan,EUVFUV,UVIS EUV / FUV imaging,Titan scan.,"VIMS ridealong with UVIS while scanning across Titan. Phase = 26.045 deg, SSC Lat/Lon = 11.425S/204.487 deg. SS Lat/Lon = 14.562N/202.732 deg. Alt = 42402.2 km, range = 44977.2 km. Resolution = 21 km/px. Temp. X. Obtain cubes scanning across Titan.",,,,,, 2012-159T04:07:21,002T03:06:39,7-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-159T09:07:21,000T05:00:00,7-Jun-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-159T09:07:21,000T05:00:00,7-Jun-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-159T09:07:21,000T05:00:00,7-Jun-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS while staring at Titan. Phase = 28.255 deg, SSC Lat/Lon = 13.659S/207.750 deg. SS Lat/Lon = 14.569N/209.078 deg. Alt = 178439.8 km, range = 178439.8 km. Resolution = 88 km/px. Temp. C. Obtain cubes of 160 and 640 while staring at Titan.",,,,,, 2012-159T09:07:21,000T05:00:00,7-Jun-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,EUVFUV Imaging of Titan,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-159T12:07:21,001T19:06:39,7-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-159T14:07:21,000T07:11:39,7-Jun-12,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2012-159T14:07:21,000T07:11:39,7-Jun-12,ISS,,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-159T14:07:21,000T07:11:39,7-Jun-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS while staring at Titan. Phase = 28.450 deg, SSC Lat/Lon = 13.814S/211.770 deg. SS Lat/Lon = 14.567N/213.779 deg. Alt = 275884.5 km, range = 278459.5 km. Resolution = 138 km/px. Temp. A2. Obtain cubes of 160 and 640 while staring at Titan.",,,,,, 2012-159T22:14:00,001T09:00:00,7-Jun-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-159T22:14:00,000T09:00:00,7-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-159T23:14:00,000T10:00:00,7-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12159_SP,rider,,,,,, 2012-160T09:39:00,000T07:25:00,8-Jun-12,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2012-160T09:54:00,000T03:00:00,8-Jun-12,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2012-160T09:54:00,000T03:00:00,8-Jun-12,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan,"VIMS ridealong with ISS while staring at Titan. Phase = 28.4 deg, SSC Lat/Lon = 13.783S/210.076 deg. SS Lat/Lon = 14.566N/211.820 deg. Alt = 234053.3 km, range = 236628 km. Resolution = 117 km/px. Obtain cubes of 160 and 640 ms every hour while staring at Titan.",,,,,, 2012-160T12:54:00,000T03:10:00,8-Jun-12,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2012-160T12:54:00,000T03:10:00,8-Jun-12,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan,"VIMS ridealong with ISS while staring at Titan. Phase = 28.4 deg, SSC Lat/Lon = 13.799S/210.752 deg. SS Lat/Lon = 14.566N/212.604 deg. Alt = 250757 km, range = 253332 km. Resolution = 125 km/px. Obtain cubes of 160 and 640 ms every hour while staring at Titan.",,,,,, 2012-160T16:04:00,000T01:00:00,8-Jun-12,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2012-160T16:04:00,000T01:00:00,8-Jun-12,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan,"VIMS ridealong with ISS while staring at Titan. Phase = 28.5 deg, SSC Lat/Lon = 13.818S/213.334 deg. SS Lat/Lon = 14.567N/215.580 deg. Alt = 314587 km, range = 317162 km. Resolution = 157 km/px. Obtain cubes of 160 and 640 ms every hour while staring at Titan.",,,,,, 2012-160T17:04:00,000T02:00:00,8-Jun-12,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2012-160T19:04:00,000T01:00:00,8-Jun-12,ISS,Prime,Titan,CLOUD,,Titan Monitoring Campaign,"Titan Monitoring Campaign,",,,,,, 2012-160T19:04:00,000T01:00:00,8-Jun-12,VIMS,SPASS Rider,Titan,CLOUDMAP,Cloud map,Stare at Titan,"VIMS ridealong with ISS while staring at Titan. Phase = 28.5 deg, SSC Lat/Lon = 13.792S/215.774 deg. SS Lat/Lon = 14.569N/218.401 deg. Alt = 375617 km, range = 378192 km. Resolution = 188 km/px. Obtain cubes of 160 and 640 ms every hour while staring at Titan.",,,,,, 2012-160T22:14:00,000T09:00:00,8-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-160T23:14:00,000T08:00:00,8-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12160_SP,rider,,,,,, 2012-161T07:14:00,009T15:44:00,9-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-161T07:14:00,007T18:32:00,9-Jun-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 3.1765580 Rs exit= 6.6706246 Range altitude= 40048.612 km ... -40205.640,,,,,, 2012-161T07:14:00,001T06:15:00,9-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-161T07:14:00,007T15:44:00,9-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-161T07:14:00,007T18:32:00,9-Jun-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_167_168",,,,,, 2012-161T07:14:00,007T18:32:00,9-Jun-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-161T07:58:00,000T00:02:00,9-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-161T08:00:00,000T12:00:00,9-Jun-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-161T19:58:00,000T00:02:00,9-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-161T19:58:00,000T00:02:00,9-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-161T20:00:00,000T01:00:00,9-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 009 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-161T20:58:00,000T00:02:00,9-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-161T20:58:00,000T00:02:00,9-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-162T04:29:00,000T09:00:00,10-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-162T05:29:00,000T08:00:00,10-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12162_SP,rider,,,,,, 2012-162T13:29:00,000T12:30:00,10-Jun-12,CDA,Prime,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._)",,,,,, 2012-162T13:29:00,001T00:00:00,10-Jun-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-163T04:29:00,000T09:00:00,11-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-163T05:29:00,000T08:00:00,11-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12163_SP,rider,,,,,, 2012-163T13:29:00,005T12:17:00,11-Jun-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-163T14:07:00,000T00:02:00,11-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-163T14:09:00,000T01:30:00,11-Jun-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 35.2 requested range 2.4 Mkm",,,,,, 2012-163T14:09:00,000T01:30:00,11-Jun-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-163T14:09:00,000T01:30:00,11-Jun-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch: Storm Watch: 32*32 pixels with 80 msec integration. phase = 61 deg, range =3.91 Mkm.",,,,,, 2012-163T15:37:00,000T00:02:00,11-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-163T15:39:00,000T01:00:00,11-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 011 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-163T16:37:00,000T00:02:00,11-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-163T16:37:00,000T00:02:00,11-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-163T16:39:00,001T09:30:00,11-Jun-12,CIRS,Prime,Saturn,MIRTMAP,,Saturn Mid-IR T map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude over multiple latitudes POINTING: -y to Saturn, z to pole",,,,,, 2012-165T02:07:00,000T00:02:00,13-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-165T02:07:00,000T00:02:00,13-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-165T04:14:00,000T09:00:00,13-Jun-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev168 Saturn rings occultation on 2012/180. DSS-34 required for X- and Ka-band support.",,,,,, 2012-165T04:14:00,000T09:00:00,13-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-165T05:14:00,000T08:00:00,13-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12165_SP,rider,,,,,, 2012-165T13:14:00,001T13:14:00,13-Jun-12,CDA,Prime,DustRAM direction,ISD0048,,CDA ISD 2012-169T01:46:00,ISD observation around apoapse 2012-169T01:46:00 48.025408 Rs,,,,,, 2012-167T03:58:00,000T09:00:00,15-Jun-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev168 Saturn rings occultation on 2012/180. DSS-43 required for X- and S-band support.",,,,,, 2012-167T03:58:00,000T09:00:00,15-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-167T04:58:00,000T08:00:00,15-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_167IC_DSCAL12167_SP,rider,,,,,, 2012-167T13:36:00,000T00:02:00,15-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-167T13:38:00,000T01:30:00,15-Jun-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 61.2 requested range 3.9 Mkm",,,,,, 2012-167T13:38:00,000T01:30:00,15-Jun-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-167T13:38:00,000T01:30:00,15-Jun-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign and Stormwatch; phase = 61 deg, range =3.91 Mkm.",,,,,, 2012-167T15:06:00,000T00:02:00,15-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-167T15:08:00,000T01:00:00,15-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 013 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-167T16:06:00,000T00:02:00,15-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-167T16:06:00,000T00:02:00,15-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-167T16:08:00,000T23:00:00,15-Jun-12,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2012-167T19:46:00,000T20:00:00,15-Jun-12,CDA,SPASS Rider,DustRAM direction,ISD0048,,CDA ISD 2012-169T01:46:00,ISD observation around apoapse 2012-169T01:46:00 48.025408 Rs,,,,,, 2012-168T15:06:00,000T00:02:00,16-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-168T15:06:00,000T00:02:00,16-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-168T15:08:00,000T10:22:00,16-Jun-12,ISS,Prime,Other,L5TITAN,,Titan L5 satellite search,Satellite search around Titan L5 Lagrange point.,,,,,, 2012-168T22:58:00,000T05:00:00,16-Jun-12,MAG,Non-SPASS,InstrumentCalibration,SCAS,MAG SCAS instrument,MAG/SCAS_Cal,"Boom alignment calibration using SCAS. If moved within scheduling window, KEEP OUTSIDE SCHEDULED MAPS CAMPAIGNS. Note: SCAS operations disturb RSS and RPWS. If OpMode is not ORS, a unique sequence will be required.",,,,,, 2012-169T01:28:00,000T00:02:00,17-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-169T01:28:00,000T00:02:00,17-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-169T01:46:00,001T21:12:00,17-Jun-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S74,Range enter= 3.1765580 Rs exit= 6.6706246 Range altitude= 40048.612 km ... -40205.640,,,,,, 2012-169T01:46:00,000T02:00:00,17-Jun-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-169T01:46:00,001T21:12:00,17-Jun-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_167_168",,,,,, 2012-169T01:46:00,001T21:12:00,17-Jun-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-169T01:46:29,000T00:00:01,17-Jun-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 23.9 d, inc = 21.1 deg, r = 47.979 Rs, phase = 76 deg",,,,,, 2012-169T03:46:00,001T19:12:00,17-Jun-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-169T03:58:00,000T09:00:00,17-Jun-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev168 Saturn rings occultation on 2012/180. DSS-34 required for X- and Ka-band support.",,,,,, 2012-169T03:58:00,001T19:00:00,17-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-169T03:58:00,000T09:00:00,17-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-169T04:58:00,000T08:00:00,17-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12169_SP,rider,,,,,, 2012-169T12:58:00,000T23:30:00,17-Jun-12,CDA,Prime,DustRAM direction,ISD0048,,CDA ISD 2012-169T01:46:00,ISD observation around apoapse 2012-169T01:46:00 48.025408 Rs,,,,,, 2012-170T13:58:00,000T09:00:00,18-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-170T14:58:00,000T08:00:00,18-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12170_SP,rider,,,,,, 2012-170T22:58:00,008T23:57:00,18-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-170T22:58:00,009T18:25:00,18-Jun-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo Enter: S74,Range enter= 3.1765580 Rs exit= 6.6706246 Range altitude= 40048.612 km ... -40205.640,,,,,, 2012-170T22:58:00,000T00:43:00,18-Jun-12,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-170T22:58:00,001T07:30:00,18-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-170T22:58:00,008T23:14:00,18-Jun-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_168",,,,,, 2012-170T22:58:00,008T20:08:00,18-Jun-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-170T23:03:00,000T00:02:00,18-Jun-12,CIRS,Non-SPASS,Other,SEQSETUP,CIRS sequence setup activity,CIRS S74 Sequence Setup,"Enforce CIRS science no-data state, load tables (IEBs) from the SSR, set the focal plane assembly set point",,,,,, 2012-170T23:41:00,000T00:07:00,18-Jun-12,INMS,Non-SPASS,Saturn,RESETLOAD,INMS instrument flight software load,Flight software load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-170T23:48:00,000T00:02:00,18-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-170T23:48:00,000T00:05:00,18-Jun-12,INMS,Non-SPASS,Saturn,IEBLOAD,INMS IEB Load,IEB Load,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-170T23:50:00,000T01:30:00,18-Jun-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 89.7 requested range 3.9 Mkm",,,,,, 2012-170T23:50:00,000T01:30:00,18-Jun-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-170T23:50:00,000T01:30:00,18-Jun-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 90 deg, range =3.85 Mkm.",,,,,, 2012-170T23:53:00,000T00:33:00,18-Jun-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,"Startup sequence. Load FSW, Load IEBs, MRO",,,,,, 2012-171T00:26:00,000T00:30:00,19-Jun-12,INMS,Non-SPASS,Saturn,FLRATESCN,Full rate scan,Full Rate Scan,,,,,,, 2012-171T00:56:00,002T05:32:00,19-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-171T01:18:00,000T00:02:00,19-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-171T01:20:00,000T01:00:00,19-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 002 ND OB SET IN REV 168","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-171T02:18:00,000T00:02:00,19-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-171T02:18:00,000T00:02:00,19-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-171T02:20:00,000T12:00:00,19-Jun-12,VIMS,Prime,rings(general),APOMOSAIC,Apoapsis mosaic,"Ring mosaic, dark side.","Up to 6x4 mosaic, tau_IR = 320 msec",,,,,, 2012-171T02:20:00,000T12:00:00,19-Jun-12,CIRS,SPASS Rider,rings(general),APOMOSAIC,Apoapsis mosaic,,null,,,,,, 2012-171T02:20:00,000T12:00:00,19-Jun-12,UVIS,SPASS Rider,rings(general),APOMOSAIC,Apoapsis mosaic,,VIMS rider,,,,,, 2012-171T14:18:00,000T00:02:00,19-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-171T21:28:00,000T09:00:00,19-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-171T22:28:00,000T08:00:00,19-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12171_SP,rider,,,,,, 2012-172T06:28:00,000T08:00:00,20-Jun-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-172T14:28:00,007T07:44:00,20-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-172T21:28:00,000T09:00:00,20-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-172T22:28:00,000T08:00:00,20-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12172_SP,rider,,,,,, 2012-173T06:28:00,000T14:59:00,21-Jun-12,CDA,Prime,DustRAM direction,ISD0048,,CDA ISD 2012-169T01:46:00,ISD observation around apoapse 2012-169T01:46:00 48.025408 Rs,,,,,, 2012-173T06:28:00,000T23:59:00,21-Jun-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-173T21:27:00,000T09:00:00,21-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-173T22:27:00,000T08:00:00,21-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12173_SP,rider,,,,,, 2012-174T06:27:00,000T15:33:00,22-Jun-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-174T06:40:00,001T13:02:00,22-Jun-12,ISS,Prime,Other,YMIROT,,Ymir,Observation of irregular moon of Saturn.,,,,,, 2012-174T06:40:00,001T13:02:00,22-Jun-12,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2012-174T10:00:00,002T00:00:00,22-Jun-12,CDA,SPASS Rider,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._)",,,,,, 2012-174T22:00:00,000T00:34:00,22-Jun-12,INMS,Non-SPASS,Saturn,MRO,Instrument memory readout,MRO,Backup MRO,,,,,, 2012-174T22:34:00,004T20:48:26,22-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-175T21:12:00,000T09:00:00,23-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-175T22:12:00,000T08:00:00,23-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12175_SP,rider,,,,,, 2012-176T07:13:00,000T00:02:00,24-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-176T07:15:00,000T18:45:00,24-Jun-12,ISS,Prime,rings(general),SPOKEMOV,Ring spoke movie,Lit Face High Phase Spoke Movie,Spoke Movie to search for periodicities,,,,,, 2012-176T07:15:00,000T18:45:00,24-Jun-12,CIRS,SPASS Rider,rings(general),SPOKEMOV,Ring spoke movie,,null,,,,,, 2012-176T07:15:00,000T18:45:00,24-Jun-12,UVIS,SPASS Rider,rings(general),SPOKEMOV,Ring spoke movie,,ISS rider,,,,,, 2012-177T01:58:00,000T00:02:00,25-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-177T01:58:00,000T00:02:00,25-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-177T02:00:00,000T01:00:00,25-Jun-12,ISS,Prime,Other,SATELLORB,Satellite orbit campaign,"SATELLITE ORBIT CAMPAIGN, 006 TH OBS SET IN REV 16","Turn to first satellite, take 1 NAC (CL1,CL2). Turn to second satellite take 1 NAC (CL1,CL2), repeat for up to 10 satellites if visible",,,,,, 2012-177T02:58:00,000T00:02:00,25-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-177T02:58:00,000T00:02:00,25-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-177T03:00:00,000T15:40:00,25-Jun-12,ISS,Prime,RingF,FMOVIE,F ring movie,Long Low Res F Ring Movie,Low Resolution F Ring Movie,,,,,, 2012-177T03:00:00,000T15:40:00,25-Jun-12,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,,null,,,,,, 2012-177T03:00:00,000T15:40:00,25-Jun-12,UVIS,SPASS Rider,rings(general),FMOVIE,F ring movie,,ISS rider,,,,,, 2012-177T18:38:00,000T00:02:00,25-Jun-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-177T18:38:00,000T00:02:00,25-Jun-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-177T21:12:00,000T09:00:00,25-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-177T22:12:00,000T08:00:00,25-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12177_SP,rider,,,,,, 2012-178T21:58:00,000T14:47:00,26-Jun-12,ISS,Prime,Titan,LRMONITOR,Long range monitor,LRM (Long Range Monitoring),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-178T21:58:00,000T14:47:00,26-Jun-12,CIRS,,Titan,LRMONITOR,Long range monitor,long range monitor,Ride along with ISS.,,,,,, 2012-178T21:58:00,000T14:47:00,26-Jun-12,VIMS,SPASS Rider,Titan,LRMONITOR,Long range monitor,PIE-TitanMonitoring,"PIE; phase = ???? deg, range = ???? Mkm.",,,,,, 2012-179T14:15:00,000T08:40:00,27-Jun-12,RSS,SPASS Rider,rings(general),GSE,,Gravity Science Enhancement (GSE),"Rings Occultation inbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-55 required for X- and Ka-band support.",,,,,, 2012-179T15:15:00,000T07:40:00,27-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12179_SP,rider,,,,,, 2012-179T15:55:00,000T04:30:00,27-Jun-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-179T15:55:00,000T07:00:00,27-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-179T19:06:00,000T03:49:00,27-Jun-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-179T19:22:26,000T03:32:34,27-Jun-12,INMS,Non-SPASS,Saturn,SURVEYRPA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-179T22:12:00,003T07:29:00,27-Jun-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-179T22:12:00,003T07:29:00,27-Jun-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. RINGS_168",,,,,, 2012-179T22:55:00,000T04:35:00,27-Jun-12,ISS,Prime,RingF,FMOVIE,F ring movie,Short Med Res F Ring Movie,Medium Resolution F Ring Movie,,,,,, 2012-179T22:55:00,000T04:35:00,27-Jun-12,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Movie,Use 640 or 1000 msec tau_IR,,,,,, 2012-179T22:55:00,001T14:00:00,27-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-179T22:55:00,000T19:27:26,27-Jun-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-179T22:55:00,002T06:51:00,27-Jun-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-180T03:30:00,000T05:21:00,28-Jun-12,ISS,Prime,rings(general),DRCLOSE,,D Ring Close-in observation,D Ring Close-In Observation,,,,,, 2012-180T03:30:00,000T05:21:00,28-Jun-12,VIMS,SPASS Rider,rings(general),DRCLOSE,,D-Ring observation,640 msec tau_IR,,,,,, 2012-180T07:26:00,000T01:25:00,28-Jun-12,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 168 RI OCC Thermal Stabilization,"A thermal stabilization period of 2 hrs and 5 min is required immediately prior to any radio science experiment which uses Ka-band or S-band. Note that the observation period of the corresponding science request includes a budgeted 40 min waypoint turn that can be considered as part of the warmup time. Hence, the total duration of this warmup request is shorter than the required 2 hrs and 5 min by those 40 min (that is, only 1 hr and 25 min). The duration should be increased back to the original 2 hrs 5 min if a waypoint turn proves unnecessary.",,,,,, 2012-180T08:51:00,000T03:55:00,28-Jun-12,RSS,Prime,rings(general),OCC,Occultation,RSS XXM Ring Occ - Ingress,Ingress ring occultation conducted using TBD bands (TBD Op-mode). The op-mode is selected based on power constraints. Observations will commence after a 2 hrs 5 min period of thermal stabilization (in RSS WARMUP op-mode).,,,,,, 2012-180T12:46:00,000T04:19:00,28-Jun-12,ISS,Prime,Saturn,LIMBSCAN,Limb scan,Saturn Limb Scan,Sun behind Saturn limb,,,,,, 2012-180T12:46:00,000T04:19:00,28-Jun-12,VIMS,SPASS Rider,Saturn,SATLIMB,,Saturn Limb in eclipse,Images of Saturn's limb in eclipse. ISS Rider.,,,,,, 2012-180T17:23:00,000T02:52:00,28-Jun-12,CDA,Prime,rings(general),VERT59,,CDA RPXing 2012-180T19:23:56,"RPXing at 5.8881283 Rs, CDA Articulation 90 degrees compatible with INMS",,,,,, 2012-180T17:23:00,000T02:52:00,28-Jun-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 6.6588050 Rs exit= 5.3158804 Range altitude= -39658.170 km ... 39765.492,,,,,, 2012-180T18:22:26,000T00:30:00,28-Jun-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-180T18:52:26,000T01:30:00,28-Jun-12,INMS,SPASS Rider,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Magnetosphere Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-180T20:15:00,000T02:30:00,28-Jun-12,ISS,Prime,Tethys,TETHYS,Tethys,Tethys ORS observation,ORS observation,,,,,, 2012-180T20:15:00,000T02:30:00,28-Jun-12,CIRS,,Tethys,TETHYS,Tethys,,"Could we please have the following tables Marcia? 352:1, 402:1 Scan times from ISS design are confirmed by Todd A (22 Feb 2012) as FP1 raster scan: 2012-180T20:40:51 -> 21:12:20 at 300 urad/s FP3 scans: 22:09:01 -> 22:29:01 at 7 urad/s Adjusted tables so shutter closed is taken from 20:15:00->20:16:53 (355) 21:15:00->21:16:53 (402) FP1 and FP3 only Shutter closed will be taken at: 20:15:00->20:16:53 21:15:00->21:16:53 22:15:00->22:16:53 Note, please ensure the FP3 scan isn't being taken during the shutter closed periods. Design Requests: ~20:45: 20 minutes FP1 full-disk raster scan (timing flexible) ~22:15: 30 minutes for FP3 scan at 6 murad/sec along 90 degree meridian (timing flexible)",,,,,, 2012-180T20:15:00,000T02:30:00,28-Jun-12,UVIS,,Tethys,ICYMAP,Icy satellite surface map,"ICYMAP: UV Surface Map of Tethys, ORS Rider",UV albedo map of Tethys's surface,,,,,, 2012-180T20:15:00,000T02:30:00,28-Jun-12,VIMS,SPASS Rider,Tethys,TETHYS,Tethys,Tethys,follow ISS,,,,,, 2012-180T20:22:26,000T23:00:00,28-Jun-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-180T21:46:56,012T01:58:04,28-Jun-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate End:SApo,Range enter= 5.3099829 Rs exit= 6.6894416 Range altitude= 40304.630 km ... -40522.143,,,,,, 2012-180T22:45:00,000T01:30:00,28-Jun-12,UVIS,Prime,Star,URALPCMA,,URSTAR,,,,,,, 2012-180T22:45:00,000T01:30:00,28-Jun-12,CIRS,SPASS Rider,rings(general),URALPCMA,,CIRS_168RI_URALPCMA001_UVIS,rider,,,,,, 2012-180T22:45:00,000T01:30:00,28-Jun-12,VIMS,SPASS Rider,Saturn,ALPCMAOCC,,Alp CMa Saturn atmosphere occultation,Rider on UVIS_168ST_URALPCMA001_PRIME. Ring occ portion unusable (begins in B ring).,,,,,, 2012-181T00:15:00,000T03:05:00,29-Jun-12,UVIS,Prime,Star,URKAPCMA,,URSTAR,This follows a UVIS PRIME AlpCMa observation directly. Should do direct turn without waypoint turn. Turn directly from AlpCMa to KapCMa.,,,,,, 2012-181T00:15:00,000T03:05:00,29-Jun-12,CIRS,SPASS Rider,rings(general),URKAPCMA,,CIRS_168RI_URKAPCMA001_UVIS,rider,,,,,, 2012-181T00:15:00,000T03:05:00,29-Jun-12,ISS,SPASS Rider,Star,URKAPCMA,,UVIS occultation rider,UVIS occultation rider,,,,,, 2012-181T00:27:21,000T00:00:01,29-Jun-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.063 Rs, lat = 15 deg, phase = 104 deg",,,,,, 2012-181T03:20:00,000T02:10:00,29-Jun-12,VIMS,Prime,rings(general),COMPLIT,,Lit side composition,High-res radial scan across rings. 160 msec IR integration time.,,,,,, 2012-181T03:20:00,000T02:10:00,29-Jun-12,CIRS,SPASS Rider,rings(general),COMPLIT,,CIRS_168RI_COMPLIT001_VIMS,rider,,,,,, 2012-181T03:20:00,000T02:10:00,29-Jun-12,UVIS,SPASS Rider,rings(general),COMPLIT,,,VIMS rider,,,,,, 2012-181T05:30:00,000T05:47:00,29-Jun-12,ISS,Prime,rings(general),MOONLETCD,,Cassini Division moonlet search,Cassini Division moonlet search,,,,,, 2012-181T05:30:00,000T05:47:00,29-Jun-12,CIRS,SPASS Rider,rings(general),MOONLETCD,,CIRS_168RI_MOONLETCD001_ISS,rider,,,,,, 2012-181T12:55:00,001T16:46:00,29-Jun-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-181T13:27:00,000T09:00:00,29-Jun-12,RSS,SPASS Rider,rings(general),GSE,,Gravity Science Enhancement (GSE),"Rings Occultation onbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-55 required for X- and Ka-band support.",,,,,, 2012-181T13:27:00,000T09:00:00,29-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-181T14:27:00,000T06:00:00,29-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12181_SP,rider,,,,,, 2012-181T19:22:26,001T01:50:34,29-Jun-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-181T22:57:00,000T01:30:00,29-Jun-12,ISS,Prime,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 11.6 requested range 2 Mkm",,,,,, 2012-181T22:57:00,000T01:30:00,29-Jun-12,CIRS,SPASS Rider,Titan,M30R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-181T22:57:00,000T01:30:00,29-Jun-12,VIMS,SPASS Rider,Titan,M30R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 12 deg, range =1.98 Mkm.",,,,,, 2012-182T00:27:00,000T10:30:00,30-Jun-12,ISS,Prime,RingB,BMOVIE,B ring movie,B-ring ansa movie,B-ring ansa movie,,,,,, 2012-182T00:27:00,000T10:30:00,30-Jun-12,CIRS,SPASS Rider,rings(general),BMOVIE,B ring movie,CIRS_168RI_BMOVIE001_ISS,rider,,,,,, 2012-182T05:46:00,000T23:55:00,30-Jun-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-182T10:57:00,000T07:34:00,30-Jun-12,ISS,Prime,rings(general),DRLPMOV,,D Ring Close-in observation at low phase,D Ring Close-In Observation at low phase,,,,,, 2012-182T20:41:00,000T09:00:00,30-Jun-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-182T21:13:00,000T02:00:00,30-Jun-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-182T21:41:00,000T08:00:00,30-Jun-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12182_SP,rider,,,,,, 2012-182T23:13:00,000T06:28:00,30-Jun-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-183T05:41:00,004T20:40:00,1-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-183T05:41:00,009T18:04:00,1-Jul-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-183T05:41:00,009T07:54:00,1-Jul-12,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2012-183T05:41:00,009T18:04:00,1-Jul-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAPS_168_169",,,,,, 2012-183T05:41:00,009T18:04:00,1-Jul-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-183T06:19:00,000T00:02:00,1-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-183T06:21:00,000T12:09:00,1-Jul-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-183T06:21:00,000T12:09:00,1-Jul-12,CIRS,SPASS Rider,Saturn,AURSLEW,Saturn aurora,Saturn polar aurorae,South pole rider FP1 may be off planet. UVIS slews to track auroral oval.,,,,,, 2012-183T06:21:00,000T12:09:00,1-Jul-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stormwatch,Auroral Slew UVIS Ridealong and Stormwatch cube,,,,,, 2012-183T07:00:00,000T01:08:00,1-Jul-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-183T18:30:00,000T01:30:00,1-Jul-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 31.4 requested range 2.6 Mkm",,,,,, 2012-183T18:30:00,000T01:30:00,1-Jul-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-183T18:30:00,000T01:30:00,1-Jul-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch,"Titan Monitoring Campaign; phase = 31 deg, range =2.58 Mkm. Stiormwatch cube at end",,,,,, 2012-183T20:00:00,000T14:46:00,1-Jul-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-183T20:00:00,000T14:46:00,1-Jul-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stormwatch Cube,Auroral Slew UVIS Ridealong with Stormwatch cube at the end,,,,,, 2012-184T10:44:00,000T00:02:00,2-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-184T12:56:00,000T09:00:00,2-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev169 Saturn rings and atmospheric occultation on 2012/204. DSS-55 required for X- and Ka-band support.",,,,,, 2012-184T13:56:00,000T08:00:00,2-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12184_SP,rider,,,,,, 2012-184T22:36:00,000T01:30:00,2-Jul-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 53.8 requested range 3.1 Mkm",,,,,, 2012-184T22:36:00,000T01:30:00,2-Jul-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-184T22:36:00,000T01:30:00,2-Jul-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch Cube,"Titan Monitoring Campaign; phase = 54 deg, range =3.06 Mkm. Stormwatch cube at end",,,,,, 2012-185T00:06:00,000T01:00:00,3-Jul-12,ISS,Prime,rings(general),PROPRETRG,Ring propeller targetting observation,Propeller retargetting,Reacquire and track orbits of individual known propellers.,,,,,, 2012-185T00:06:00,000T01:00:00,3-Jul-12,CIRS,SPASS Rider,rings(general),PROPRETRG,Ring propeller targetting observation,CIRS_168RI_PROPRETRG001_ISS,rider,,,,,, 2012-185T01:04:00,000T00:02:00,3-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-185T01:04:00,000T00:02:00,3-Jul-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-185T01:06:00,000T23:25:00,3-Jul-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-185T01:06:00,000T23:25:00,3-Jul-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong an Stormwatch cube,Auroral Slew UVIS Ridealong and Stormwatch Cube,,,,,, 2012-186T03:41:00,000T08:00:00,4-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12186_SP,rider,,,,,, 2012-186T12:21:00,000T01:30:00,4-Jul-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 70 requested range 3.2 Mkm",,,,,, 2012-186T12:21:00,000T01:30:00,4-Jul-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-186T12:21:00,000T01:30:00,4-Jul-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stormwatch Cube,"Titan Monitoring Campaign; phase = 70 deg, range =3.17 Mkm. Stormwatch Cube at end",,,,,, 2012-186T13:49:00,000T00:02:00,4-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-186T13:51:00,001T10:40:00,4-Jul-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-186T13:51:00,001T10:40:00,4-Jul-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stormwatch Cube,Auroral Slew UVIS Ridealong and Stormwatch cube,,,,,, 2012-188T02:21:00,005T14:19:00,6-Jul-12,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2012-188T03:41:00,000T08:00:00,6-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12188_SP,rider,,,,,, 2012-188T12:21:00,000T01:30:00,6-Jul-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 85.7 requested range 2.9 Mkm",,,,,, 2012-188T12:21:00,000T01:30:00,6-Jul-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-188T12:21:00,000T01:30:00,6-Jul-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stormwatch Cube,"Titan Monitoring Campaign; phase = 86 deg, range =2.86 Mkm. Ends with Stormwatch Cube",,,,,, 2012-188T13:49:00,000T00:02:00,6-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-188T13:51:00,001T10:24:00,6-Jul-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-188T13:51:00,001T10:24:00,6-Jul-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stomwatch,Auroral Slew UVIS Ridealong. Ends with Stormwatch Cube,,,,,, 2012-189T23:45:00,000T20:00:00,7-Jul-12,CDA,SPASS Rider,DustRAM direction,ISD0049,,CDA ISD 2012-192T23:45:00,ISD observation around apoapse 2012-192T23:45:00 48.096044 Rs,,,,,, 2012-190T00:13:00,000T00:02:00,8-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-190T03:25:00,000T08:00:00,8-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12190_SP,rider,,,,,, 2012-190T12:03:00,000T00:02:00,8-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-190T12:05:00,001T12:10:00,8-Jul-12,UVIS,Prime,Saturn,AURSLEW,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Repeated slews across the auroral oval,,,,,, 2012-190T12:05:00,001T12:10:00,8-Jul-12,VIMS,,Saturn,AURSLEW,Saturn aurora,UVIS Auroral Slew Ridealong and Stormwatch Cube,Auroral Slew UVIS Ridealong. Ends with Stormwatch cube,,,,,, 2012-191T17:45:00,000T20:00:00,9-Jul-12,CDA,SPASS Rider,DustRAM direction,ISD0049,,CDA ISD 2012-192T23:45:00,ISD observation around apoapse 2012-192T23:45:00 48.096044 Rs,,,,,, 2012-192T00:13:00,000T00:02:00,10-Jul-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-192T03:25:00,000T08:00:00,10-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_168IC_DSCAL12192_SP,rider,,,,,, 2012-192T12:05:00,000T01:30:00,10-Jul-12,ISS,Prime,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 83.9 requested range 1.8 Mkm",,,,,, 2012-192T12:05:00,000T01:30:00,10-Jul-12,CIRS,SPASS Rider,Titan,M90R2CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-192T12:05:00,000T01:30:00,10-Jul-12,VIMS,SPASS Rider,Titan,M90R2CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 84 deg, range =1.76 Mkm.",,,,,, 2012-192T13:35:00,000T08:00:00,10-Jul-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-192T21:35:00,000T04:00:00,10-Jul-12,CAPS,Prime,co-rotation,IONCALPTG,,IMS and IBS calibration,null,,,,,, 2012-192T21:35:00,000T04:00:00,10-Jul-12,CAPS,Non-SPASS,co-rotation,IONCALCOM,,IMS and IBS Calibration Commanding,This request will be used IONCAL commanding. The times are identical to the IONCAL pointing request,,,,,, 2012-192T21:35:00,011T06:48:00,10-Jul-12,MAG,Non-SPASS,Other,MAPSCAKE,,MAPS CAKE,MAPS CAKE observation,,,,,, 2012-192T23:45:00,011T15:45:56,10-Jul-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo,Range enter= 5.3099829 Rs exit= 6.6894416 Range altitude= 40304.630 km ... -40522.143,,,,,, 2012-192T23:45:00,000T02:00:00,10-Jul-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-192T23:45:00,011T04:38:00,10-Jul-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. MAPS_168_169",,,,,, 2012-192T23:45:00,010T17:55:00,10-Jul-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-192T23:45:08,000T00:00:01,10-Jul-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 24.0 d, inc = 21.2 deg, r = 48.049 Rs, phase = 76 deg",,,,,, 2012-193T01:35:00,000T15:05:00,11-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-193T01:45:00,010T08:53:00,11-Jul-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-193T09:45:00,000T20:00:00,11-Jul-12,CDA,SPASS Rider,DustRAM direction,ISD0049,,CDA ISD 2012-192T23:45:00,ISD observation around apoapse 2012-192T23:45:00 48.096044 Rs,,,,,, 2012-193T16:40:00,000T08:00:00,11-Jul-12,ISS,Prime,Other,YMIPHA,,Ymir,Observation of irregular moon of Saturn.,,,,,, 2012-193T16:40:00,000T08:00:00,11-Jul-12,UVIS,SPASS Rider,Other,OUTERSATS,Icy satellite observaton,ICYLON: Icy Satellite Longitude / Phase Coverage,"Measure satellite albedo in ultraviolet light for a good sampling of longitude and phase space. Determine phase function to investigate surface microstructure and frost properties, as a function of location.",,,,,, 2012-193T16:40:00,000T12:00:00,11-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-194T02:10:00,000T09:00:00,12-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev169 Saturn rings and atmospheric occultation on 2012/204. DSS-43 required for X- and S-band support.",,,,,, 2012-194T02:10:00,000T09:00:00,12-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-194T03:10:00,000T06:00:00,12-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12194_SP,rider,,,,,, 2012-194T04:40:00,003T19:20:00,12-Jul-12,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2012-194T11:10:00,000T18:45:00,12-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-195T00:00:00,000T01:08:00,13-Jul-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-195T03:45:00,000T20:00:00,13-Jul-12,CDA,SPASS Rider,DustRAM direction,ISD0049,,CDA ISD 2012-192T23:45:00,ISD observation around apoapse 2012-192T23:45:00 48.096044 Rs,,,,,, 2012-195T07:25:00,000T17:15:00,13-Jul-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-195T07:25:00,000T17:15:00,13-Jul-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-195T07:25:00,000T17:15:00,13-Jul-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare. For rotation timing,"Rider on UVIS PIE. CL1 NAC 4x4 images. 10 Mbits/hr, expected only half of the time to be usable stare",,,,,, 2012-195T07:25:00,000T17:15:00,13-Jul-12,VIMS,,Saturn,AURSTARE,Saturn aurora,Auroral Stare,Auroral Stare ridealong with UVIS,,,,,, 2012-196T02:10:00,000T09:00:00,14-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev169 Saturn rings and atmospheric occultation on 2012/204. DSS-34 required for X- and Ka-band support.",,,,,, 2012-196T02:10:00,000T09:00:00,14-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-196T03:10:00,000T08:00:00,14-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12196_SP,rider,,,,,, 2012-196T11:10:00,001T11:29:00,14-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-197T22:39:00,000T12:00:00,15-Jul-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-197T22:39:00,000T12:00:00,15-Jul-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-197T22:39:00,000T12:00:00,15-Jul-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare. For rotation timing,"Rider on UVIS PIE. CL1 NAC 4x4 images. 10 Mbits/hr, expected only half of the time to be usable stare",,,,,, 2012-197T22:39:00,000T12:00:00,15-Jul-12,VIMS,,Saturn,AURSTARE,Saturn aurora,Auroral Stare,Auroral Stare ridealong with UVIS,,,,,, 2012-198T00:00:00,000T10:00:00,16-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-198T10:00:00,005T18:23:00,16-Jul-12,CAPS,SPASS Rider,Saturn,LOWLATAPO,,MAPS Low latitude apoapsis,null,,,,,, 2012-198T12:09:00,000T09:00:00,16-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev169 Saturn rings and atmospheric occultation on 2012/204. DSS-63 required for X- and S-band support.",,,,,, 2012-198T12:09:00,000T09:00:00,16-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-198T13:09:00,000T08:00:00,16-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12198_SP,rider,,,,,, 2012-198T21:49:00,000T01:30:00,16-Jul-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 71.2 requested range 3 Mkm",,,,,, 2012-198T21:49:00,000T01:30:00,16-Jul-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-198T21:49:00,000T01:30:00,16-Jul-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 71 deg, range =3.03 Mkm.",,,,,, 2012-198T23:19:00,000T13:05:00,16-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-199T12:24:00,000T12:00:00,17-Jul-12,UVIS,Prime,Saturn,AURSTARE,Saturn aurora,Saturn Aurora,Auroral Observations led by UVIS Mixture of slews for UV imaging and fixed pointings at the auroral oval,,,,,, 2012-199T12:24:00,000T12:00:00,17-Jul-12,CIRS,SPASS Rider,Saturn,AURSTARE,Saturn aurora,Saturn polar aurorae,,,,,,, 2012-199T12:24:00,000T12:00:00,17-Jul-12,ISS,,Saturn,AURSTARE,Saturn aurora,NAC aurora stare. For rotation timing,"Rider on UVIS PIE. CL1 NAC 4x4 images. 10 Mbits/hr, expected only half of the time to be usable stare",,,,,, 2012-199T12:24:00,000T12:00:00,17-Jul-12,VIMS,,Saturn,AURSTARE,Saturn aurora,Auroral Stare,Auroral Stare ridealong with UVIS,,,,,, 2012-200T01:54:00,000T09:00:00,18-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-200T02:54:00,000T08:00:00,18-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12200_SP,rider,,,,,, 2012-200T11:34:00,000T01:30:00,18-Jul-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 84.2 requested range 3 Mkm",,,,,, 2012-200T11:34:00,000T01:30:00,18-Jul-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-200T11:34:00,000T01:30:00,18-Jul-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign; phase = 84 deg, range =3.04 Mkm.",,,,,, 2012-200T13:04:00,000T11:20:00,18-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-201T01:54:00,000T09:00:00,19-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev169 Saturn rings and atmospheric occultation on 2012/204. DSS-34 required for X- and Ka-band support.",,,,,, 2012-201T01:54:00,000T09:00:00,19-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-201T02:54:00,000T08:00:00,19-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12201_SP,rider,,,,,, 2012-201T10:54:00,000T13:15:00,19-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-202T01:39:00,000T09:00:00,20-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-202T02:39:00,000T08:00:00,20-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12202_SP,rider,,,,,, 2012-202T10:39:00,000T14:59:00,20-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-203T01:38:00,000T09:00:00,21-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-203T01:43:00,000T04:00:00,21-Jul-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-203T02:38:00,000T08:00:00,21-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12203_SP,rider,,,,,, 2012-203T10:38:00,000T08:45:00,21-Jul-12,CAPS,Prime,co-rotation,LLACORPTG,,MAPS low latitude apoapsis prime pointing,null,,,,,, 2012-203T10:38:00,000T07:17:48,21-Jul-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-203T17:40:00,000T10:43:00,21-Jul-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-203T17:55:48,000T10:27:12,21-Jul-12,INMS,Non-SPASS,Saturn,SURVEYRPA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-203T19:23:00,000T09:00:00,21-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-204T04:23:00,001T16:15:00,22-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-204T04:23:00,000T12:32:48,22-Jul-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-204T04:23:00,001T16:15:00,22-Jul-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-204T04:23:00,001T16:15:00,22-Jul-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. RINGS_169",,,,,, 2012-204T04:23:00,001T16:15:00,22-Jul-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-204T05:50:00,000T01:25:00,22-Jul-12,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 169 RI OCC Thermal Stabilization,"A thermal stabilization period of 2 hrs and 5 min is required immediately prior to any radio science experiment which uses Ka-band or S-band. Note that the observation period of the corresponding science request includes a budgeted 40 min waypoint turn that can be considered as part of the warmup time. Hence, the total duration of this warmup request is shorter than the required 2 hrs and 5 min by those 40 min (that is, only 1 hr and 25 min). The duration should be increased back to the original 2 hrs 5 min if a waypoint turn proves unnecessary.",,,,,, 2012-204T07:15:11,000T02:55:48,22-Jul-12,RSS,Prime,rings(general),OCC,Occultation,RSS XXM Ring Occ - Ingress,Ingress ring occultation conducted using TBD bands (TBD Op-mode). The op-mode is selected based on power constraints. Observations will commence after a 2 hrs 5 min period of thermal stabilization (in RSS WARMUP op-mode).,,,,,, 2012-204T10:10:59,000T01:32:00,22-Jul-12,RSS,Prime,Saturn,OCCIN,Ingress Occultation,RSS Saturn Ingress Atmospheric Occultation,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2012-204T12:03:00,000T04:17:00,22-Jul-12,VIMS,Prime,rings(general),HIPHASE,High phase observation,High phase ring observation,High phase ring observation. Custom turn period.,,,,,, 2012-204T12:03:00,000T04:17:00,22-Jul-12,CIRS,SPASS Rider,rings(general),HIPHASE,High phase observation,CIRS_169RI_HIPHASE001_VIMS,rider,,,,,, 2012-204T12:03:00,000T04:17:00,22-Jul-12,ISS,,rings(general),HIPHASE,High phase observation,Rider on VIMS Hiphase,"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-204T15:30:56,000T04:50:00,22-Jul-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 6.6775853 Rs exit= 5.3187880 Range altitude= -39975.865 km ... 39848.025,,,,,, 2012-204T16:25:00,000T03:00:00,22-Jul-12,CDA,Prime,rings(general),VERT59,,CDA RPXing 2012-204T17:55:56,"RPXing at 5.9032706 Rs, CDA Articulation 90 degrees, compatible with INMS",,,,,, 2012-204T16:30:00,000T03:00:00,22-Jul-12,RPWS,Non-SPASS,rings(general),RPXING,"Measurements of dust flux, scale height and plasma waves at the magnetic equator during ring plane crossing",RPWS Ring Plane Crossing,Determine the equatorial dust flux and scale height as a function of radial distance. Obtain high resolution of plasma waves at the magnetic equator.,,,,,, 2012-204T16:55:48,000T00:30:00,22-Jul-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-204T17:25:48,000T01:30:00,22-Jul-12,INMS,SPASS Rider,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Magnetosphere Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-204T18:55:48,000T23:00:00,22-Jul-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-204T19:25:00,000T00:55:00,22-Jul-12,CIRS,Prime,rings(general),NP140L30,,,null,,,,,, 2012-204T19:25:00,000T00:55:00,22-Jul-12,CIRS,SPASS Rider,rings(general),NP140L30,,CIRS_169RI_NP140L30001_SI,,,,,,, 2012-204T20:20:00,000T01:56:00,22-Jul-12,VIMS,Prime,Saturn,ALPCMAOCC,,alp Cma atmosphere occultation,"alp Cma atmosphere occultation. Stellar occ mode, no spectral summing, tau_IR = 40 msec.",,,,,, 2012-204T20:20:00,000T01:56:00,22-Jul-12,ISS,SPASS Rider,Saturn,ALPCMAOCC,,VIMS occultation rider,VIMS occultation rider,,,,,, 2012-204T20:20:00,000T01:56:00,22-Jul-12,UVIS,SPASS Rider,Star,URALPCMA,,URSTAR,,,,,,, 2012-204T20:20:56,008T23:46:04,22-Jul-12,CDA,Non-SPASS,Other,RATE010A,,Data rate End:SApo,Range enter= 5.3128487 Rs exit= 7.2761371 Range altitude= 40386.044 km ... -40678.270,,,,,, 2012-204T20:28:00,000T01:48:00,22-Jul-12,CIRS,SPASS Rider,rings(general),URALPCMA,,CIRS_169RI_URALPCMA001_UVIS,rider,,,,,, 2012-204T22:16:00,000T03:44:00,22-Jul-12,UVIS,Prime,Star,URZETCMA,,URSTAR,,,,,,, 2012-204T22:16:00,000T03:18:00,22-Jul-12,CIRS,SPASS Rider,rings(general),URZETCMA,,CIRS_169RI_URZETCMA001_UVIS,rider,,,,,, 2012-204T22:16:00,000T03:44:00,22-Jul-12,ISS,SPASS Rider,Star,URZETCMA,,UVIS occultation rider,UVIS occultation rider,,,,,, 2012-204T23:02:34,000T00:00:01,22-Jul-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.062 Rs, lat = 15 deg, phase = 104 deg",,,,,, 2012-205T02:00:00,000T02:00:00,23-Jul-12,UVIS,Prime,Dione,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to alpha Vir to look for volatiles.,,,,,, 2012-205T02:00:00,000T02:00:00,23-Jul-12,CIRS,,Dione,ICYEX,,,"FP1, FP3 only Shutter closed between: 2012-205T02:00:00 -> 02:01:53 2012-205T03:00:00 -> 03:01:53",,,,,, 2012-205T02:00:00,000T02:00:00,23-Jul-12,ISS,,Dione,ICYEXO,Icy satellite exosphere,Dione,Dione occultation of Alpha Virginis (Spica),,,,,, 2012-205T02:00:00,000T02:00:00,23-Jul-12,VIMS,SPASS Rider,Dione,ICYEX,,occultation,follow UVIS occultation,,,,,, 2012-205T04:00:00,000T05:28:00,23-Jul-12,ISS,Prime,rings(general),MOONLETCD,,Cassini Division moonlet search,Cassini Division moonlet search,,,,,, 2012-205T04:00:00,000T05:28:00,23-Jul-12,CIRS,SPASS Rider,rings(general),MOONLETCD,,CIRS_169RI_MOONLETCD001_ISS,rider,,,,,, 2012-205T11:38:00,000T09:00:00,23-Jul-12,RSS,SPASS Rider,rings(general),GSE,,Gravity Science Enhancement (GSE),"Rings Occultation onbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-55 required for X- and Ka-band support.",,,,,, 2012-205T11:38:00,000T09:00:00,23-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev170 Saturn rings occultation on 2012/225. DSS-55 required for X- and Ka-band support.",,,,,, 2012-205T11:38:00,000T09:00:00,23-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-205T12:38:00,000T08:00:00,23-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12205_SP,rider,,,,,, 2012-205T17:55:48,000T02:42:12,23-Jul-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-205T20:38:00,000T21:25:07,23-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-205T20:38:00,000T11:25:07,23-Jul-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-205T20:38:00,000T19:25:07,23-Jul-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-205T20:38:00,001T22:00:00,23-Jul-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_169_T85",,,,,, 2012-205T20:38:00,000T07:42:00,23-Jul-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-205T21:32:59,000T09:30:08,23-Jul-12,CIRS,Prime,Titan,MIDIRTMAP,Mid infrared thermal map,,Obtain information on the thermal structure of Titan's stratosphere. Slew across disk at 4 microrad/s.,,,,,, 2012-205T21:32:59,000T09:30:08,23-Jul-12,ISS,SPASS Rider,Titan,MIDIRTMAP,Mid infrared thermal map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-205T21:32:59,000T09:30:08,23-Jul-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS while staring at Titan. Phase = 151.178 deg. SSC Lat/Lon = 13.653N/356.284 deg, SS Lat/Lon = 15.127N/177.860 deg. Alt = 461969.7 km, range = 464544.7 km. Resolution = 230 km/px. Temp. M4. Obtain 160 and 640 ms cubes while staring at Titan.",,,,,, 2012-206T04:20:00,001T14:18:00,24-Jul-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-206T07:03:07,000T04:00:00,24-Jul-12,CIRS,Prime,Titan,FIRNADCMP,Far infrared nadir composition map,,"Obtain information on CO, HCN, CH4. Integrate on disk at airmass 1.5--2.0.",,,,,, 2012-206T07:03:07,000T04:00:00,24-Jul-12,ISS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T07:03:07,000T04:00:00,24-Jul-12,VIMS,SPASS Rider,Titan,FIRNADCMP,Far infrared nadir composition map,Stare at Titan,"VIMS ridealong with CIRS while staring at Titan. Phase = 149.808 deg. SSC Lat/Lon = 15.051N/6.052 deg, SS Lat/Lon = 15.131N/186.793 deg. Alt = 256278.3 km, range = 258853.3 km. Resolution = 128 km/px. Temp. N1. Obtain 160 and 640 ms cubes while staring at Titan.",,,,,, 2012-206T07:03:07,000T04:00:00,24-Jul-12,UVIS,Non-SPASS,Titan,FIRNADCMP,Far infrared nadir composition map,FIRNADCMP rider,Several slow wcans across Titan's visible hemisphere to form spectral images,,,,,, 2012-206T08:03:07,000T11:00:00,24-Jul-12,INMS,Non-SPASS,Titan,T85INBND,,Titan flyby,Titan observation,,,,,, 2012-206T11:03:07,000T04:00:00,24-Jul-12,VIMS,Prime,Titan,MEDRES,Medium resolution global mapping,Global Mapping of Titan,"VIMS global mapping of Titan. Phase = 159.237 deg. SSC Lat/Lon = 14.628N/10.194 deg, SS Lat/Lon = 15.133N/190.554 deg. Alt = 175527.2 km, range = 178102.2 km. Resolution = 88 km/px. Temp. Q. Global mapping of Titan at medium resolution. 1 or 2 2x2 mosaics.",,,,,, 2012-206T11:03:07,000T04:00:00,24-Jul-12,CIRS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,,Ride along with VIMS.,,,,,, 2012-206T11:03:07,000T04:00:00,24-Jul-12,ISS,SPASS Rider,Titan,MEDRES,Medium resolution global mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T15:03:07,000T02:30:00,24-Jul-12,VIMS,Prime,Titan,REGMAP,Regional mapping,Regional Mapping of Titan,"VIMS regional mapping of Titan. Phase = 148.185 deg. SSC Lat/Lon = 16.680N/14.492 deg, SS Lat/Lon = 15.135N/194.315 deg. Alt = 96299.7 km, range = 98874.7 km. Resolution = 48 km/px. Temp. Y. Regional mapping of Titan's terminator area.",,,,,, 2012-206T15:03:07,000T02:30:00,24-Jul-12,CIRS,SPASS Rider,Titan,REGMAP,Regional mapping,,Ride along with VIMS.,,,,,, 2012-206T15:03:07,000T02:30:00,24-Jul-12,ISS,SPASS Rider,Titan,REGMAP,Regional mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T16:03:07,000T08:00:00,24-Jul-12,MAG,Non-SPASS,Titan,MAGTITAN,MAG Titan observation,T85 flyby,"T85 is another low altitude (990 km) north polar flyby in the post noon sector of Saturn's magnetosphere. With closest approach in the dayside ionosphere, Cassini will be able to study the diffusion of the external magnetic field at low altitudes and mid solar zenith angles. A comparison with T83 and T84 will be very useful. We assign grade one priority. Data rate: 1976bps (32vps).",,,,,, 2012-206T17:33:07,000T01:15:00,24-Jul-12,CIRS,Prime,Titan,FIRLMBINT,Vertical limb sounding,,"Vertical sounding of stratospheric compounds on Titan, including H2O. Integrations at 2 locations on the limb displaced vertically.",,,,,, 2012-206T17:33:07,000T01:15:00,24-Jul-12,ISS,SPASS Rider,Titan,FIRLMBINT,Vertical limb sounding,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T17:33:07,000T01:15:00,24-Jul-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping of Titan,VIMS ridealong with CIRS - pb with CIRS having 2 observations in the same slot,,,,,, 2012-206T17:33:07,000T01:15:00,24-Jul-12,UVIS,Non-SPASS,Titan,FIRLMBINT,Vertical limb sounding,Rider with CIRS FIRLMBINT,Rider with CIRS MIRLMBINT,,,,,, 2012-206T18:03:07,000T01:00:00,24-Jul-12,CAPS,SPASS Rider,Titan,T85INBND,,Inbound 169TI (T85),null,,,,,, 2012-206T18:03:07,000T01:00:00,24-Jul-12,MIMI,SPASS Rider,Titan,TITINOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-206T18:03:07,000T01:00:00,24-Jul-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-206T18:48:07,000T00:30:00,24-Jul-12,CIRS,Prime,Titan,FIRLMBAER,Ring photometry,,Limb scanning for aerosols.,,,,,, 2012-206T18:48:07,000T00:30:00,24-Jul-12,ISS,SPASS Rider,Titan,FIRLMBAER,Ring photometry,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T18:48:07,000T00:30:00,24-Jul-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping of Titan,"VIMS ridealong with CIRS - Specular reflection on Kivu Lacus at 18:20:08 - pointing on Kivu done by CIRS Phase = 145.606 deg. SSC Lat/Lon = 19.235N/18.180 deg, SS Lat/Lon = 15.136N/196.190 deg. Alt = 42244.6 km, range = 44819.6 km. Resolution = 21 km/px. Limb observations - atmospheric composition",,,,,, 2012-206T19:03:07,000T02:00:00,24-Jul-12,CAPS,SPASS Rider,Titan,T85CLOSE,,Closest Approach 169TI (T85),null,,,,,, 2012-206T19:03:07,000T02:00:00,24-Jul-12,MIMI,SPASS Rider,Titan,TITCAOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-206T19:03:07,000T00:55:30,24-Jul-12,INMS,Non-SPASS,Titan,TITAN85,,Titan Flyby,Titan observation,,,,,, 2012-206T19:03:07,000T02:00:00,24-Jul-12,RPWS,Non-SPASS,Titan,TICA,Titan closest approach,Titan closest approach observations,"RPWS observations in the immediate vicinity of Titan, including thermal plasma density and temperature measurements with the Langmuir probe, search for lightning and other radio emissions, characterization of plasma wave spectrum, search for evidence of pickup ions. Langmuir probe within 90 degrees of spacecraft ram at closest approach, corotational ram outside of +/- 15 minutes.",,,,,, 2012-206T19:19:07,000T00:34:00,24-Jul-12,CIRS,Prime,Titan,FIRLMBT,Far Infrared limb tracking,CIRS_169TI_FIRLMBT001_PRIME,Vertical temperature sounding of Titan's tropopause & stratosphere. Slow radial scans.,,,,,, 2012-206T19:19:07,000T00:34:00,24-Jul-12,ISS,SPASS Rider,Titan,FIRLMBT,Far Infrared limb tracking,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T19:19:07,000T00:34:00,24-Jul-12,VIMS,SPASS Rider,Titan,REGMAP,Regional mapping,Regional Mapping of Titan,"VIMS ridealong with CIRS for regional mapping of Titan. Phase = 136.614 deg. SSC Lat/Lon = 27.954N/23.531 deg, SS Lat/Lon = 15.137N/198.310 deg. Alt = 12903.2 km, range = 15478.2 km. Resolution = 6.5 km/px. Obtain mosaics and cubes of Titan for regional mapping prior to CA.",,,,,, 2012-206T19:53:07,000T00:55:00,24-Jul-12,VIMS,Prime,Titan,HIRES,High resolution image,Hi-resolution regional Mapping of Titan,"VIMS regional mapping of Titan during C/A. At C/A, phase = 58.260 deg. SSC Lat/Lon = 61.630N/149.256 deg, SS Lat/Lon = 15.137N/199.016 deg. Alt = 1012 km, range = 3587 km. Resolution = 0.51 km/px. Obtain mosaics of Titan during C/A.",,,,,, 2012-206T19:53:07,000T00:55:00,24-Jul-12,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with VIMS.,,,,,, 2012-206T19:53:07,000T00:55:00,24-Jul-12,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T19:58:37,000T00:08:40,24-Jul-12,INMS,Non-SPASS,Titan,TITAN85,,Titan Flyby,Titan observation,,,,,, 2012-206T20:07:17,000T00:55:50,24-Jul-12,INMS,Non-SPASS,Titan,TITAN85,,Titan Flyby,Titan observation,,,,,, 2012-206T20:48:07,000T00:22:00,24-Jul-12,CIRS,SPASS Rider,Titan,TRANS,,,Ride along with ENGR.,,,,,, 2012-206T20:48:07,000T00:22:00,24-Jul-12,VIMS,SPASS Rider,Titan,TRANS,,Hi-resolution Mapping during transition,"VIMS cubes during transitionSsegional mapping of Titan during C/A. At C/A, phase = ??? deg. SC Lat/Lon = ??? deg, SS Lat/Lon = 15.N/199. deg. Alt = 20,000km,. Resolution =10 km/px.",,,,,, 2012-206T21:03:07,000T01:00:00,24-Jul-12,CAPS,SPASS Rider,Titan,T85OUTBND,,Outbound 169TI (T85),null,,,,,, 2012-206T21:03:07,000T01:00:00,24-Jul-12,MIMI,SPASS Rider,Titan,TITOUTOV,,MAPS TI Campaign,"Part of TI MAPS Campaign. Investigate micro-scale and near aspects of the Titan interaction by observing during about one hour period around an encounter. With -Y pointed toward Titan, when within 30 minutes of the targeted flyby, optimize secondary axis for corotation flow as close to the S/C -X, +/- Z plane as works with the other constraints on pointing. Also, measure Titan exosphere/magnetosphere interaction by imaging in ENA with INCA (when sun is not in INCA FOV).",,,,,, 2012-206T21:03:07,000T11:00:00,24-Jul-12,INMS,Non-SPASS,Titan,T85OUTBND,,Titan flyby,Titan observation,,,,,, 2012-206T21:03:07,000T01:00:00,24-Jul-12,RPWS,Non-SPASS,Titan,TIINTRMED,Titan magnetosphere interaction,Titan Interaction - Intermediate,"Study the interaction of the magnetosphere with Titan at intermediate distances for evidence of ion pickup, radio emissions, density profiles, and the general wave environment. Prefer Langmuir probe within 90 degrees of plasma ram.",,,,,, 2012-206T21:10:07,000T01:08:00,24-Jul-12,VIMS,Prime,Titan,HIRES,High resolution image,Hi-resolution regional Mapping of Titan,"VIMS regional mapping of Titan. Phase = 28.736 deg. SSC Lat/Lon = 13.581S/199.019 deg, SS Lat/Lon = 15.137N/200.034 deg. Alt = 19384.6 km, range = 21959.6 km. Resolution = 9.7 km/px. Obtain mosaics of Titan for regional mapping.",,,,,, 2012-206T21:10:07,000T01:08:00,24-Jul-12,CIRS,SPASS Rider,Titan,HIRES,High resolution image,,Ride along with VIMS.,,,,,, 2012-206T21:10:07,000T01:08:00,24-Jul-12,ISS,SPASS Rider,Titan,HIRES,High resolution image,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T22:03:07,000T20:29:52,24-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-206T22:18:07,000T02:45:00,24-Jul-12,CIRS,Prime,Titan,FIRNADMAP,Far infrared nadir composition map,CIRS_014TI_FIRNADIRMAP_01,"Obtain information on surface & tropopause temperatures, and on tropospheric CH4. Scan or contiguous steps across disk. POINTING: -y to Titan, x away from sun. Z axis generally aligned N/S or E/W, perpendicular to scan or steps.",,,,,, 2012-206T22:18:07,000T02:45:00,24-Jul-12,ISS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-206T22:18:07,000T02:45:00,24-Jul-12,VIMS,SPASS Rider,Titan,FIRNADMAP,Far infrared nadir composition map,Titan Scan.,"VIMS ridealong with CIRS while scanning across Titan. Phase = 33.528 deg. SSC Lat/Lon = 18.377N/202.052 deg, SS Lat/Lon = 15.138N/201.131 deg. Alt = 42247.8 km, range = 44822.8 km. Resolution = 21 km/px. Temp. E. Obtain cubes while scanning across Titan.",,,,,, 2012-207T00:03:07,001T06:34:53,25-Jul-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-207T01:03:07,000T04:00:00,25-Jul-12,CIRS,Prime,Titan,MIRLMBMAP,Mid infrared limb map,,Obtain vertical profiles of temperatures in Titan's stratosphere. The arrays are stepped along the limb at two altitudes at 5 degree latitude intervals.,,,,,, 2012-207T01:03:07,000T04:00:00,25-Jul-12,ISS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-207T01:03:07,000T04:00:00,25-Jul-12,VIMS,SPASS Rider,Titan,MIRLMBMAP,Mid infrared limb map,Limb Mapping,"VIMS ridealong with CIRS for limb mapping of Titan. Phase = 30.037 deg. SSC Lat/Lon = 20.849N/205.637 deg, SS Lat/Lon = 15.139N/203.717 deg. Alt = 96270.4 km, range = 98845.4 km. Resolution = 48 km/px. Temp. F. Obtain cubes of Titan's limb.",,,,,, 2012-207T05:03:07,000T05:00:00,25-Jul-12,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping of Titan,"VIMS global mapping of Titan. Phase = 36.872 deg. SSC Lat/Lon = 21.672S/209.622 deg, SS Lat/Lon = 15.141N/207.477 deg. Alt = 175115.8 km, range = 177690.8 km. Resolution = 88 km/px. Temp. V. Obtain cubes for global mapping of Titan.",,,,,, 2012-207T05:03:07,000T05:00:00,25-Jul-12,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2012-207T05:03:07,000T05:00:00,25-Jul-12,ISS,,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-207T08:03:07,000T22:34:52,25-Jul-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-207T10:03:07,000T07:39:52,25-Jul-12,VIMS,Prime,Titan,GLOBMAP,Global coverage mapping,Global Mapping of Titan,"VIMS global mapping of Titan. Phase = 37.099 deg. SSC Lat/Lon = 21.906S/214.149 deg, SS Lat/Lon = 15.143N/212.178 deg. Alt = 274416.0 km, range = 276991.0 km. Resolution = 137 km/px. Temp. B. Obtain cubes for global mapping of Titan.",,,,,, 2012-207T10:03:07,000T07:39:52,25-Jul-12,CIRS,SPASS Rider,Titan,GLOBMAP,Global coverage mapping,,Ride along with VIMS.,,,,,, 2012-207T10:03:07,000T07:39:52,25-Jul-12,ISS,,Titan,GLOBMAP,Global coverage mapping,RCI (Ridealong Context Imaging),"ISS on, max data rate = 182.784 kbps, number of frames and bits/frame are input parameters, data volume = number of frames x bits/frame, average data rate = data volume/duration.",,,,,, 2012-207T18:33:00,000T12:05:00,25-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-207T18:38:00,000T12:00:00,25-Jul-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. TOST_169_T85",,,,,, 2012-207T18:38:00,000T12:00:00,25-Jul-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-207T18:38:00,000T10:00:00,25-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-207T19:38:00,000T11:00:00,25-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12207_SP,rider,,,,,, 2012-208T04:38:00,000T02:00:00,26-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-208T06:38:00,017T02:43:00,26-Jul-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-208T06:38:00,002T03:30:00,26-Jul-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-208T06:38:00,001T03:45:00,26-Jul-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-208T06:38:00,007T04:14:00,26-Jul-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_169_170",,,,,, 2012-208T06:38:00,005T13:29:00,26-Jul-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-208T06:53:00,000T17:00:00,26-Jul-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 1. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: 0 mrad about x-axis, -0 mrad about z-axis (z = 0 Rs). Start data capture, stare 757.0 s, stop data capture. Repeat PATTERN 70 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 757.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1599.48284 bps, from Alain's spreadsheet)x(757.0s per stare)x(71 stares) = 85.9674x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-208T08:00:00,002T00:00:00,26-Jul-12,CDA,SPASS Rider,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._)",,,,,, 2012-209T01:23:00,000T09:00:00,27-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-209T02:23:00,000T08:00:00,27-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12209_SP,rider,,,,,, 2012-209T10:23:00,000T08:00:00,27-Jul-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-209T18:23:00,004T01:44:00,27-Jul-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-210T01:08:00,000T09:00:00,28-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-210T02:08:00,000T08:00:00,28-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12210_SP,rider,,,,,, 2012-210T10:08:00,000T15:00:00,28-Jul-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 2. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: 0 mrad about x-axis, -83.8 mrad about z-axis (z ~ -3.1 Rs). Start data capture, stare 765.0 s, stop data capture. Repeat PATTERN 60 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 765.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1582.75623 bps, from Alain's spreadsheet)x(765.0s per stare)x(61 stares) = 73.85932x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-210T10:08:00,000T07:00:00,28-Jul-12,ISS,SPASS Rider,InstrumentCalibration,NACDARK,ISS Narrow Angle Camera dark current calibration,ISS NAC dark current calibration,ISS NAC dark current calibration,,,,,, 2012-210T10:08:00,001T00:00:00,28-Jul-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-210T17:23:00,000T07:00:00,28-Jul-12,ISS,SPASS Rider,InstrumentCalibration,WACDARK,ISS Wide Angle Camera dark current calibration,ISS WAC dark current calibration,ISS WAC dark current calibration,,,,,, 2012-211T01:08:00,000T09:00:00,29-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-211T02:08:00,000T08:00:00,29-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12211_SP,rider,,,,,, 2012-211T10:08:00,001T23:29:00,29-Jul-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 3. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: +50 mrad about x-axis, +142.5 mrad about z-axis (z ~ 5.7 Rs). Start data capture, stare 586.0 s, stop data capture. Repeat PATTERN 261 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 586.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (2066.22613 bps, from Alain's spreadsheet)x(586.0s per stare)x(262 stares) = 317.23183x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-211T10:08:00,004T00:44:00,29-Jul-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-212T10:52:00,000T20:00:00,30-Jul-12,CDA,SPASS Rider,DustRAM direction,ISD0050,,CDA ISD 2012-215T10:52:00,ISD observation around apoapse 2012-215T10:52:00 43.307727 Rs,,,,,, 2012-213T11:07:00,000T09:00:00,31-Jul-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev170 Saturn rings occultation on 2012/225. DSS-55 required for X- and Ka-band support.",,,,,, 2012-213T11:07:00,000T09:00:00,31-Jul-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-213T12:07:00,000T08:00:00,31-Jul-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12213_SP,rider,,,,,, 2012-213T20:07:00,001T03:15:00,31-Jul-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 4. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: -50 mrad about x-axis, +29.4 mrad about z-axis (z ~ +1.25 Rs). Start data capture, stare 633.5 s, stop data capture. Repeat PATTERN 136 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 633.5 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1911.29994 bps, from Alain's spreadsheet)x(633.5 s per stare)x(137 stares) = 165.881x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-213T20:07:00,001T14:45:00,31-Jul-12,CDA,Non-SPASS,Other,RATE010B,,Data rate End:SApo,Range enter= 5.3128487 Rs exit= 7.2761371 Range altitude= 40386.044 km ... -40678.270,,,,,, 2012-213T20:07:00,012T18:38:00,31-Jul-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-213T20:07:00,001T14:45:00,31-Jul-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-214T04:52:00,000T20:00:00,1-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0050,,CDA ISD 2012-215T10:52:00,ISD observation around apoapse 2012-215T10:52:00 43.307727 Rs,,,,,, 2012-215T00:52:00,000T09:00:00,2-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-215T01:52:00,000T08:00:00,2-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_169IC_DSCAL12215_SP,rider,,,,,, 2012-215T10:30:00,000T00:02:00,2-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-215T10:32:00,000T01:30:00,2-Aug-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 64 requested range 3.6 Mkm",,,,,, 2012-215T10:32:00,000T01:30:00,2-Aug-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-215T10:32:00,000T01:30:00,2-Aug-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Stormwatch Cube,"Titan Monitoring Campaign; phase = 64 deg, range =3.60 Mkm. Saturn Stormwatch at end",,,,,, 2012-215T10:52:00,009T09:08:00,2-Aug-12,CDA,Non-SPASS,Other,RATE010A,,Data rate Enter:SApo,Range enter= 5.3128487 Rs exit= 7.2761371 Range altitude= 40386.044 km ... -40678.270,,,,,, 2012-215T10:52:00,000T02:00:00,2-Aug-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-215T10:52:00,009T22:29:00,2-Aug-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. XD_169_170",,,,,, 2012-215T10:52:00,007T13:29:00,2-Aug-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-215T10:52:25,000T00:00:01,2-Aug-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 21.2 d, inc = 32.2 deg, r = 43.265 Rs, phase = 78 deg",,,,,, 2012-215T12:00:00,000T00:02:00,2-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-215T12:02:00,001T10:25:00,2-Aug-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 5. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: -50 mrad about x-axis, +29.1 mrad about z-axis (z ~ +1.25 Rs). Start data capture, stare 633.0 s, stop data capture. Repeat PATTERN 174 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 633.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1912.80966 bps, from Alain's spreadsheet)x(633.0s per stare)x(175 stares) = 211.8915x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-215T12:02:00,001T10:25:00,2-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration during the last two minutes of this observation,,,,,, 2012-215T12:52:00,004T20:44:00,2-Aug-12,INMS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-215T20:52:00,000T20:00:00,2-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0050,,CDA ISD 2012-215T10:52:00,ISD observation around apoapse 2012-215T10:52:00 43.307727 Rs,,,,,, 2012-216T22:25:00,000T00:02:00,3-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-217T00:37:00,000T09:00:00,4-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-217T01:37:00,000T08:00:00,4-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12217_SP,rider,,,,,, 2012-217T09:37:00,000T13:30:00,4-Aug-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 6. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: +50 mrad about x-axis, +135.7 mrad about z-axis (z ~ +5.7 Rs). Start data capture, stare 583.0 s, stop data capture. Repeat PATTERN 68 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 583.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (2076.85851 bps, from Alain's spreadsheet)x(583.0s per stare)x(69 stares) = 83.5458x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-217T14:52:00,000T20:00:00,4-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0050,,CDA ISD 2012-215T10:52:00,ISD observation around apoapse 2012-215T10:52:00 43.307727 Rs,,,,,, 2012-218T00:37:00,000T09:00:00,5-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-218T09:37:00,000T13:29:00,5-Aug-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 7. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: 0 mrad about x-axis, +168.8 mrad about z-axis (z ~ +6.75 Rs Rs). Start data capture, stare 766.0 s, stop data capture. Repeat PATTERN 53 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 766.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1580.68997 bps, from Alain's spreadsheet)x(766.0s per stare)x(54 stares) = 65.3837x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-218T20:36:00,000T13:00:00,5-Aug-12,RSS,SPASS Rider,Earth,USOPIM,RSS Ultra stable oscillator / Periodic Instrument Maintenance,RSS USO Characterization plus PIM,"RSS USO characterization plus PIM. Pointing=XBAND to Earth. No rolling during 3-hour USO from 2012-221T00:21:00 till 2012-221T03:21:00, to be tracked at DSS-34 in 1-way mode. Keep Ka-band ON till end of downlink at 2012-221T09:21:00 to satisfy PIM requirement.",,,,,, 2012-219T00:36:00,000T09:00:00,6-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-219T09:36:00,000T15:00:00,6-Aug-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 8. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: 0 mrad about x-axis, -171.1 mrad about z-axis (z ~ -6.5 Rs Rs). Start data capture, stare 762.0 s, stop data capture. Repeat PATTERN 60 times. PATTERN: Slew -1.5 mrad about z-axis. Start data capture, stare 762.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1588.98755 bps, from Alain's spreadsheet)x(762.0 s per stare)x(61 stares) = 73.8593x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-220T00:36:00,000T09:00:00,7-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-220T01:36:00,000T08:00:00,7-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12220_SP,rider,,,,,, 2012-220T09:36:00,000T14:45:00,7-Aug-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 9. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: 0 mrad about x-axis, +103.6 mrad about z-axis (z ~ +3.625 Rs Rs). Start data capture, stare 762.0 s, stop data capture. Repeat PATTERN 59 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 762.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1588.98755 bps, from Alain's spreadsheet)x(762.0 s per stare)x(60 stares) = 72.6485x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-220T09:36:00,000T23:45:00,7-Aug-12,INMS,Non-SPASS,Saturn,SURVPOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-221T00:21:00,000T09:00:00,8-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-221T01:21:00,000T08:00:00,8-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12221_SP,rider,,,,,, 2012-221T09:21:00,003T09:34:40,8-Aug-12,INMS,Non-SPASS,Saturn,SURVBOTM,MAPS survey,Post OTM Survey,Post-OTM request to resume science mode after NAV OTM.,,,,,, 2012-221T09:58:00,000T00:02:00,8-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-221T10:00:00,000T18:41:00,8-Aug-12,UVIS,Prime,Saturn,MOS169APO,,,"Mosaic scan of Saturn magnetosphere, day 10. EUV and FUV low resolution slits on. Allowances have been made for 20 minutes observation margin at start and end, and 30 minutes for turning back to waypoint at the end. Note: data to be taken only when slit is stationary. Waypoint is assumed to be Saturn center. Align slit with Saturn spin axis. Initial slews: 0 mrad about x-axis, +0 mrad about z-axis (z = 0 Rs). Start data capture, stare 762.0 s, stop data capture. Repeat PATTERN 77 times. PATTERN: Slew +1.5 mrad about z-axis. Start data capture, stare 762.0 s, stop data capture. Note: As no data will be collected while Cassini is slewing, actual data volume = (1588.98755 bps, from Alain's spreadsheet)x(762.0 s per stare)x(78 stares) = 94.4431x10^6 bits. Data rate multiplier includes factor of 1.01 for data packet filling.",,,,,, 2012-221T10:00:00,000T18:41:00,8-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration during the last two minutes of this observation,,,,,, 2012-221T22:00:00,002T00:00:00,8-Aug-12,CDA,SPASS Rider,DustRAM direction,RETROGR,MAPS retrograde campaign,Retrograde campaign,"Retrograde measurement - DV, TLM and power are covered by the background requests (..._RATE..._)",,,,,, 2012-222T04:39:00,000T00:02:00,9-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-222T06:11:00,000T16:00:00,9-Aug-12,ISS,Prime,RingF,FMOVIE,F ring movie,Long Low Res F Ring Movie,Low Resolution F Ring Movie,,,,,, 2012-222T06:11:00,000T16:00:00,9-Aug-12,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,,null,,,,,, 2012-222T06:11:00,000T16:00:00,9-Aug-12,VIMS,SPASS Rider,rings(general),FMOVIE,F ring movie,F Movie,Use 640 or 1000 msec tau_IR,,,,,, 2012-222T22:09:00,000T00:02:00,9-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-223T00:21:00,001T18:26:00,10-Aug-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-223T00:21:00,000T09:00:00,10-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-223T01:21:00,000T08:00:00,10-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12223_SP,rider,,,,,, 2012-223T06:09:00,000T03:12:00,10-Aug-12,MAG,Non-SPASS,Other,R1DLROLL,MAG downlink roll calibration,MAG_R1_DLROLL_CAL,Rider on rolling downlink with MAG FGM in range 1. Used for calibration of range 1. Rides on current MAG activities - no additional power or datavolume used.,,,,,, 2012-223T17:51:00,000T03:00:00,10-Aug-12,RADAR,Non-SPASS,Other,WU4RADCAL,RADAR distant Titan radiometry warm up,Distant Titan Radiometry Warm Up,Warmup for calibration and science data collection.,,,,,, 2012-223T20:51:00,000T02:00:00,10-Aug-12,RADAR,Prime,Titan,RADIOMCAL,RADAR distant Titan radiometry calibration,Distant Titan Radiometry Calibration,Obtain distant Titan radiometer science and calibration data.,,,,,, 2012-224T00:21:00,000T09:00:00,11-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-224T01:21:00,000T08:00:00,11-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12224_SP,rider,,,,,, 2012-224T14:25:00,000T06:25:00,11-Aug-12,VIMS,Prime,rings(general),BETPEGOCC,,betPeg Ring Occultation,Ring stellar occultation; integration time = 40msec; Egress occ.,,,,,, 2012-224T18:47:00,000T14:34:00,11-Aug-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-224T18:55:40,000T14:25:20,11-Aug-12,INMS,Non-SPASS,Saturn,SURVEYRPA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-224T20:00:00,000T21:08:56,11-Aug-12,CDA,Non-SPASS,Other,RATE010B,,Data rate Enter:SApo,Range enter= 5.3128487 Rs exit= 7.2761371 Range altitude= 40386.044 km ... -40678.270,,,,,, 2012-225T00:00:00,000T01:08:00,12-Aug-12,CAPS,Non-SPASS,InstrumentCalibration,ELSCAL,CAPS Electron Spectrometer calibration,ELS Calibration,null,,,,,, 2012-225T00:21:00,000T09:00:00,12-Aug-12,RSS,SPASS Rider,rings(general),GSE,,Gravity Science Enhancement (GSE),"Rings Occultation inbound GSE (Gravity Science Enhancement) Additional downlink pass at Ka-band to improve Saturn's gravity field determination, and for improving Cassini's orbit locally for data analysis of rings and atmosphere occultation. DSS-34 required for X- and Ka-band support.",,,,,, 2012-225T00:21:00,000T09:00:00,12-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-225T01:21:00,000T08:00:00,12-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12225_SP,rider,,,,,, 2012-225T07:56:00,000T01:44:59,12-Aug-12,RSS,SPASS Rider,rings(general),THERMAL,Thermal stabilization period,RSS 170 RI OCC Thermal Stabilization,"A thermal stabilization period of 2 hrs and 5 min is required immediately prior to any radio science experiment which uses Ka-band or S-band. Note that the observation period of the corresponding science request includes a budgeted 40 min waypoint turn that can be considered as part of the warmup time. Hence, the total duration of this warmup request is shorter than the required 2 hrs and 5 min by those 40 min (that is, only 1 hr and 25 min). The duration should be increased back to the original 2 hrs 5 min if a waypoint turn proves unnecessary.",,,,,, 2012-225T09:21:00,002T09:59:00,12-Aug-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-225T09:21:00,000T08:54:00,12-Aug-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-225T09:21:00,002T09:59:00,12-Aug-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. RINGS_170",,,,,, 2012-225T09:21:00,001T22:51:00,12-Aug-12,RPWS,Non-SPASS,Saturn,INSURVEY,Inner magnetosphere survey,RPWS Inner Survey,"Setup RPWS for inner magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-225T09:40:59,000T02:35:00,12-Aug-12,RSS,Prime,Saturn,OCCOUT,Egress Occultation,RSS Saturn Egress Atmospheric Occultation,"This is for the RSS occultation of Saturn's ionosphere and atmosphere, to measure vertical profiles of electron density in the ionosphere, and of density, pressure, and temperature in the neutral atmosphere. X, S, and Ka bands will be used. Prior to this point the RFIS bay will have been thermally stabilized (see thermal stabilisation request).",,,,,, 2012-225T12:15:59,000T03:57:00,12-Aug-12,RSS,Prime,rings(general),OCC,Occultation,RSS XXM Ring Occ - Egress,Ingress ring occultation conducted using TBD bands (TBD Op-mode). The op-mode is selected based on power constraints. Observations will commence after a 2 hrs 5 min period of thermal stabilization (in RSS WARMUP op-mode).,,,,,, 2012-225T16:33:00,000T03:45:00,12-Aug-12,CDA,Prime,DustRAM direction,RPX0490,,CDA RPXing 2012-225T18:55:56,"RPXing at 6.7617841 Rs, CDA articulation 90 degrees, compatible with INMS",,,,,, 2012-225T17:08:56,000T03:32:00,12-Aug-12,CDA,Non-SPASS,Other,RATE080,Dust survey,Data rate,Range enter= 7.2658746 Rs exit= 6.3247734 Range altitude= -39928.740 km ... 39270.128,,,,,, 2012-225T18:15:00,000T00:10:00,12-Aug-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-225T18:25:00,000T01:50:00,12-Aug-12,INMS,SPASS Rider,Saturn,INNERMAG,Observing neutral molecules in the inner magnetosphere,Inner Magnetosphere Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-225T20:15:00,000T22:40:40,12-Aug-12,INMS,Non-SPASS,Saturn,RINGPLNA,,Ring Plane Observation,Observe neutral molecules in the equatorial plane,,,,,, 2012-225T20:40:56,001T22:39:04,12-Aug-12,CDA,Non-SPASS,Other,RATE010A,,Data rate End:SApo,Range enter= 6.3174539 Rs exit= 7.2917467 Range altitude= 40017.515 km ... -40501.884,,,,,, 2012-225T20:45:00,000T02:00:00,12-Aug-12,UVIS,Prime,Dione,ICYEXO,Icy satellite exosphere,ICYEXO: Icy Satellite Exospheres,Target to kappa Ori to look for volatiles.,,,,,, 2012-225T20:45:00,000T02:00:00,12-Aug-12,ISS,SPASS Rider,Dione,ICYEXO,Icy satellite exosphere,Dione,Dione occultation of Kappa Orionis (Saiph),,,,,, 2012-225T20:45:00,000T02:00:00,12-Aug-12,VIMS,SPASS Rider,Dione,ICYEX,,occultation,follow UVIS occultation,,,,,, 2012-225T20:45:00,000T02:00:00,12-Aug-12,CIRS,Non-SPASS,Dione,ICYEX,,,Shutter closed between: 2012-255T20:45:00 -> 20:46:53 2012-255T21:45:00 -> 21:46:53,,,,,, 2012-225T22:45:00,000T02:00:00,12-Aug-12,ISS,Prime,RingF,HIRESFRNG,High resolution F ring image,HIGH RES F RING IMAGING,High resolution imaging of the F ring at ~10RS.,,,,,, 2012-225T22:45:00,000T02:00:00,12-Aug-12,CIRS,SPASS Rider,rings(general),HIRESFRNG,High resolution F ring image,,null,,,,,, 2012-225T22:45:00,000T02:00:00,12-Aug-12,VIMS,SPASS Rider,rings(general),HIRESFRNG,High resolution F ring image,F-Ring observation,320 msec tau_IR,,,,,, 2012-226T00:00:00,000T22:00:00,13-Aug-12,RPWS,Non-SPASS,Saturn,AURXNGOUT,Aurora and Saturn Kilometric Radiation,MAPS AS Campaign,Part of AS MAPS Campaign. Observe the auroral magnetosphere (e.g. the acceleration region) and SKR source regions,,,,,, 2012-226T00:45:00,000T09:00:00,13-Aug-12,ISS,Prime,rings(general),MOONLETC,C ring moonlet search,C-ring moonlet search,C-ring moonlet search,,,,,, 2012-226T00:45:00,000T09:00:00,13-Aug-12,CIRS,SPASS Rider,rings(general),MOONLETC,C ring moonlet search,,null,,,,,, 2012-226T01:31:41,000T00:00:01,13-Aug-12,MP,SPASS Note,Saturn,PERIAPSE,Periapse,,"Periapse R = 5.746 Rs, lat = 24 deg, phase = 103 deg",,,,,, 2012-226T04:00:00,000T04:00:00,13-Aug-12,RPWS,Non-SPASS,Saturn,NBANDLOW,Campaign to obtain high resolution WBR data in the narrow band emission source region,RPWS Narrowband Source Region Campaign,Part of RPWS campaign to obtain high resolution WBR data in the narrow band emission source region,,,,,, 2012-226T09:45:00,000T04:30:00,13-Aug-12,CIRS,Prime,rings(general),NP50L30S,,,null,,,,,, 2012-226T14:45:00,001T04:35:00,13-Aug-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-226T18:55:40,001T00:24:20,13-Aug-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-226T19:30:00,000T01:30:00,13-Aug-12,UVIS,Prime,Mimas,LOPHASE,,ICYLON: Longitude / Phase space coverage,Map uv albedo as a function of longitude and phase angle,,,,,, 2012-226T19:30:00,000T01:30:00,13-Aug-12,ISS,SPASS Rider,Mimas,LOPHASE,,Mimas ORS observation,ORS observation,,,,,, 2012-226T19:30:00,000T01:30:00,13-Aug-12,VIMS,SPASS Rider,Mimas,LOPHASE,,low phase,follow UVIS,,,,,, 2012-226T21:00:00,000T11:10:00,13-Aug-12,ISS,Prime,RingF,FMOVIE,F ring movie,Med/High Res F Ring Movie,Med/High Resolution F Ring Movie,,,,,, 2012-226T21:00:00,000T11:10:00,13-Aug-12,CIRS,SPASS Rider,rings(general),FMOVIE,F ring movie,,null,,,,,, 2012-226T21:00:00,000T11:10:00,13-Aug-12,VIMS,SPASS Rider,RingF,FMOVIE,F ring movie,F Movie,Use 640 or 1000 msec tau_IR,,,,,, 2012-227T08:12:00,009T08:27:00,14-Aug-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-227T10:20:00,000T09:00:00,14-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-227T11:20:00,000T08:00:00,14-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12227_SP,rider,,,,,, 2012-227T19:20:00,010T06:59:00,14-Aug-12,CAPS,Non-SPASS,Saturn,SURVEY,Magnetospheric survey,MAPS Survey,null,,,,,, 2012-227T19:20:00,008T21:19:00,14-Aug-12,CDA,Non-SPASS,Other,RATE010B,,Data rate End:SApo,Range enter= 6.3174539 Rs exit= 7.2917467 Range altitude= 40017.515 km ... -40501.884,,,,,, 2012-227T19:20:00,000T05:33:00,14-Aug-12,INMS,Non-SPASS,Saturn,SURVEYSEG,Campaign to determine atmospheric and ionospheric thermal structure,Segment Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-227T19:20:00,009T11:49:00,14-Aug-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-227T19:20:00,008T21:19:00,14-Aug-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SATURN_170_171",,,,,, 2012-227T20:00:00,000T16:00:00,14-Aug-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-227T20:00:00,000T16:00:00,14-Aug-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-228T00:53:00,000T02:00:00,15-Aug-12,INMS,Non-SPASS,Titan,TTNTORUS,Titan torus observation,Titan Torus observation,Titan Torus observation,,,,,, 2012-228T02:53:00,008T13:46:00,15-Aug-12,INMS,Non-SPASS,Saturn,SURVEYREV,,Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-228T12:00:00,000T11:00:00,15-Aug-12,CIRS,Prime,Saturn,FIRMAP,Far infrared map,Saturn Far-IR map,Northern hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude,,,,,, 2012-228T12:00:00,000T11:00:00,15-Aug-12,VIMS,SPASS Rider,Saturn,FIRMAP,Far infrared map,CIRS FIRMAP ridealong,CIRS FIRMAP Ridealong,,,,,, 2012-228T22:58:00,000T00:02:00,15-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-229T17:35:00,000T09:00:00,16-Aug-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev171 Saturn atmospheric occultation on 2012/246. DSS-25 required for X- and Ka-band support.",,,,,, 2012-229T17:35:00,000T09:00:00,16-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-229T18:35:00,000T08:00:00,16-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12229_SP,rider,,,,,, 2012-230T03:13:00,000T00:02:00,17-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-230T03:15:00,000T22:00:00,17-Aug-12,CIRS,Prime,Saturn,MIRMAP,Mid infrared map,Saturn Mid-IR map,"Either hemisphere Determine upper troposphere and tropopause temperature with spatial resolution of about two degrees of latitude and longitude POINTING: -y to Saturn, z to pole",,,,,, 2012-230T03:15:00,000T22:00:00,17-Aug-12,ISS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,Day WAC,Rider on CIRS to monitor day side clouds in WAC every ~2 hours,,,,,, 2012-230T03:15:00,000T22:00:00,17-Aug-12,VIMS,SPASS Rider,Saturn,MIRMAP,Mid infrared map,CIRS MIRMAP ridealong,CIRS MIRMAP Ridealong,,,,,, 2012-231T01:13:00,000T00:02:00,18-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-231T17:35:00,000T09:00:00,18-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-231T18:35:00,000T08:00:00,18-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12231_SP,rider,,,,,, 2012-232T03:13:00,000T00:02:00,19-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-232T03:15:00,000T01:30:00,19-Aug-12,ISS,Prime,Titan,M60R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 55.8 requested range 3.4 Mkm",,,,,, 2012-232T03:15:00,000T01:30:00,19-Aug-12,CIRS,SPASS Rider,Titan,M60R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-232T03:15:00,000T01:30:00,19-Aug-12,VIMS,SPASS Rider,Titan,M60R3CLD,,Titan Monitoring Campaign and Stormwatch Cube,"Titan Monitoring Campaign; phase = 56 deg, range =3.45 Mkm. Ends with Saturn Stormwatch",,,,,, 2012-232T04:43:00,000T00:02:00,19-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-232T04:45:00,000T05:00:00,19-Aug-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","STrack features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-232T04:45:00,000T05:00:00,19-Aug-12,UVIS,SPASS Rider,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-232T04:45:00,000T05:00:00,19-Aug-12,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2012-232T09:45:00,000T06:00:00,19-Aug-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-232T09:45:00,000T06:00:00,19-Aug-12,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-232T15:43:00,000T00:02:00,19-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-232T15:43:00,000T00:02:00,19-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-232T15:45:00,000T05:00:00,19-Aug-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","STrack features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-232T15:45:00,000T05:00:00,19-Aug-12,UVIS,SPASS Rider,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-232T15:45:00,000T05:00:00,19-Aug-12,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2012-232T20:45:00,000T05:00:00,19-Aug-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","STrack features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-232T20:45:00,000T05:00:00,19-Aug-12,UVIS,SPASS Rider,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-232T20:45:00,000T05:00:00,19-Aug-12,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2012-233T01:45:00,000T06:00:00,20-Aug-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-233T01:45:00,000T06:00:00,20-Aug-12,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-233T07:43:00,000T00:02:00,20-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-233T07:43:00,000T00:02:00,20-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-233T07:45:00,000T05:00:00,20-Aug-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","STrack features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-233T07:45:00,000T05:00:00,20-Aug-12,UVIS,SPASS Rider,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-233T07:45:00,000T05:00:00,20-Aug-12,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2012-233T16:38:00,000T20:00:00,20-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0051,,CDA ISD 2012-236T16:38:00,ISD observation around apoapse 2012-236T16:38:00 43.355822 Rs,,,,,, 2012-233T17:35:00,000T09:00:00,20-Aug-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev171 Saturn atmospheric occultation on 2012/246. DSS-25 required for X- and Ka-band support.",,,,,, 2012-233T17:35:00,000T09:00:00,20-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-233T18:35:00,000T08:00:00,20-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12233_SP,rider,,,,,, 2012-234T03:13:00,000T00:02:00,21-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-234T03:15:00,000T01:30:00,21-Aug-12,ISS,Prime,Titan,M90R3CLD,,Titan Monitoring Campaign,"Titan Monitoring Campaign, requested phase 75.7 requested range 3.5 Mkm",,,,,, 2012-234T03:15:00,000T01:30:00,21-Aug-12,CIRS,SPASS Rider,Titan,M90R3CLD,,Rider for Titan Monitoring Campaign,Rider to ISS Titan cloud monitor,,,,,, 2012-234T03:15:00,000T01:30:00,21-Aug-12,VIMS,SPASS Rider,Titan,M90R3CLD,,Titan Monitoring Campaign and Saturn Stormwatch,"Titan Monitoring Campaign; phase = 76 deg, range =3.51 Mkm. Ends with Saturn Stormwatch cube",,,,,, 2012-234T04:43:00,000T00:02:00,21-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-234T04:45:00,000T16:00:00,21-Aug-12,UVIS,Prime,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV Imaging of Saturn,One slow scans across Saturn's visible hemisphere to form spectral images,,,,,, 2012-234T04:45:00,000T16:00:00,21-Aug-12,CIRS,Non-SPASS,Saturn,EUVFUV,UVIS EUV / FUV imaging,EUVFUV rider,,,,,,, 2012-234T20:43:00,000T00:02:00,21-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-234T20:43:00,000T00:02:00,21-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-234T20:45:00,000T11:00:00,21-Aug-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-234T20:45:00,000T11:00:00,21-Aug-12,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-234T20:45:00,000T11:00:00,21-Aug-12,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS MIRMAP ridealong,CIRS Ridealong,,,,,, 2012-235T07:43:00,000T00:02:00,22-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-235T10:38:00,000T20:00:00,22-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0051,,CDA ISD 2012-236T16:38:00,ISD observation around apoapse 2012-236T16:38:00 43.355822 Rs,,,,,, 2012-235T17:19:00,000T09:00:00,22-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-235T18:19:00,000T08:00:00,22-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_170IC_DSCAL12235_SP,rider,,,,,, 2012-236T02:57:00,000T00:02:00,23-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-236T02:59:00,000T05:00:00,23-Aug-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","STrack features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-236T02:59:00,000T05:00:00,23-Aug-12,UVIS,SPASS Rider,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-236T02:59:00,000T05:00:00,23-Aug-12,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2012-236T07:59:00,000T06:00:00,23-Aug-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-236T07:59:00,000T06:00:00,23-Aug-12,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-236T13:57:00,000T00:02:00,23-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-236T13:57:00,000T00:02:00,23-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-236T13:59:00,000T05:00:00,23-Aug-12,ISS,Prime,Saturn,WIND5HR,,"Wind measuring 5-6-5 template + polarimetry, 5-hr","STrack features for ~2 hours to get the 2-hr time step for winds, mosaic in longitude, part of the windspeed template. CB2, (2x2 MT2, MT3,BL1) NAC Cycled while observation lasts. First 9 minutes is a 13-filter polarmetry block (see the note)",,,,,, 2012-236T13:59:00,000T05:00:00,23-Aug-12,UVIS,SPASS Rider,Saturn,WIND5HR,,UVIS Rider to ISS WIND,UVIS Rider to ISS WIND sit-and-stare,,,,,, 2012-236T13:59:00,000T05:00:00,23-Aug-12,VIMS,Non-SPASS,Saturn,WIND5HR,,5-hr Wind Observation #1,Ride-along with ISS,,,,,, 2012-236T16:38:50,000T00:00:01,23-Aug-12,MP,SPASS Note,Saturn,APOAPSE,Apoapse,,"Apoapse Per = 21.3 d, inc = 32.2 deg, r = 43.311 Rs, phase = 77 deg",,,,,, 2012-236T16:39:00,001T01:55:00,23-Aug-12,CDA,Non-SPASS,Other,RATE010,Dust survey,Data rate Enter:SApo End: S75,Range enter= 6.3174539 Rs exit= 7.2917467 Range altitude= 40017.515 km ... -40501.884,,,,,, 2012-236T16:39:00,000T02:00:00,23-Aug-12,INMS,Non-SPASS,Saturn,ENGBCKGND,,Engineering background observation,Full rate measurement to gather engineering background data,,,,,, 2012-236T16:39:00,001T09:40:00,23-Aug-12,MIMI,Non-SPASS,co-rotation,SURVEY,Magnetospheric survey,MAPS SURVEY Campaign,"Part of SURVEY MAPS Campaign. Pointing: As closely as possible, keep corotation ram in -X, +/-Z half-plane; B field in X, Z plane. SATURN_170_171",,,,,, 2012-236T16:39:00,001T09:40:00,23-Aug-12,RPWS,Non-SPASS,Saturn,OUTSURVEY,Outer magnetospheric survey,RPWS Outer Survey,"Setup RPWS for outer magnetosphere survey observations, attitude N/A, any OPMODE or TLM mode including RPWS.",,,,,, 2012-236T18:39:00,001T07:40:00,23-Aug-12,INMS,Non-SPASS,Saturn,SURVEYSEQ,,Sequence Boundary Survey,Part of the MAPS/TOST Campaign. Determine atmospheric and ionospheric thermal structure.,,,,,, 2012-236T18:59:00,000T11:00:00,23-Aug-12,CIRS,Prime,Saturn,COMPSIT,Sit and stare at one location to derive composition,Saturn COMPSIT,"Measure oxygen compounds (H2O, CO2) in stratosphere as a function of latitude. POINTING: -Y to Saturn, Z to pole Either hemisphere",,,,,, 2012-236T18:59:00,000T11:00:00,23-Aug-12,UVIS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,UVIS Rider to CIRS Compsit,UVIS Rider to CIRS Compsit,,,,,, 2012-236T18:59:00,000T11:00:00,23-Aug-12,VIMS,SPASS Rider,Saturn,COMPSIT,Sit and stare at one location to derive composition,CIRS MIRMAP ridealong and Storm Watch,CIRS Ridealong and Stormwatch,,,,,, 2012-237T02:38:00,000T15:56:00,24-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0051,,CDA ISD 2012-236T16:38:00 End: S75,ISD observation around apoapse 2012-236T16:38:00 43.355822 Rs,,,,,, 2012-237T05:57:00,000T00:02:00,24-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-237T07:09:00,000T08:00:00,24-Aug-12,MAG,Prime,Sun,CALROLL,MAG calibration roll,MAG Calibration Rolls,"Roll about axis other than Z for determination of sensor offsets, actual roll axis is not important - selected axis is usually suitable for MAPS. Preferably calibrations should be made every 15-20 days in areas where field conditions are suitable. Note: periods of suitable data are defined as follows; 1) More distant than 15 RS from Saturn's axis (to try and get into the more uniform part of the internal+sheet field). 2) Inside the magnetopause (more specifically inside a most compressed model MP). 3) More distant than 3 RS from the current sheet. Using a 'hinged' sheet model which departs from Saturn's equatorial plane at about 15 RS and then follows the anti-solar direction on the nightside. This means that, even though its orbit is equatorial, if the spacecraft is situated far enough away from the planet, it should see the nightside current sheet divert northwards away from it (using Saturn axis tilted 17 deg away from Sun). Apart from possible injection events, sheet disruptions etc the resultant periods should have a reasonable probability of seeing a 'quiescent' 'lobe-like' or 'disk-like' field. We would prefer as far downtail as possible so the field has more chance of pointing in a single direction over larger length scales.",,,,,, 2012-237T15:07:00,000T00:02:00,24-Aug-12,ISS,SPASS Rider,Saturn,STORMW,Saturn storm watch,SATURN STORM WATCH,rider on the last 2 minutes of the turn back to the NEG_Y to Saturn waypoint. Taking advantage of the 2 minute margin.,,,,,, 2012-237T15:07:00,000T00:02:00,24-Aug-12,VIMS,SPASS Rider,Saturn,STORMW,Saturn storm watch,Storm Watch Ridealong,Storm Watch: 32*32 pixels with 80 msec integration,,,,,, 2012-237T15:09:00,000T11:10:00,24-Aug-12,MAG,Non-SPASS,Other,SURVEY,Magnetospheric survey,MAG MAPS Survey,Continuous low-rate magnetospheric survey,,,,,, 2012-237T17:19:00,000T09:00:00,24-Aug-12,RSS,SPASS Rider,Saturn,OCCORT,Operations Readiness Test to demonstrate DSN and RSSG preparedness to support upcoming occultations,RSS Operational Readiness Test,"RSS Operations Readiness Test (ORT), to demonstrate DSN and RSSG preparedness to support the Rev171 Saturn atmospheric occultation on 2012/246. DSS-14 and DSS-63 required for X- and S-band support.",,,,,, 2012-237T17:19:00,000T09:00:00,24-Aug-12,UVIS,Non-SPASS,SolarWind,IPHSURVEY,Interplanetary hydrogen survey,UVIS Interplanetary Hydrogen Survey,UVIS is on collecting data at a low rate continuously. No special pointing is required.,,,,,, 2012-237T18:19:00,000T08:00:00,24-Aug-12,CIRS,SPASS Rider,InstrumentCalibration,DSCAL12,,CIRS_171IC_DSCAL12237_SP,rider,,,,,, 2012-237T18:34:00,000T04:04:00,24-Aug-12,CDA,SPASS Rider,DustRAM direction,ISD0051,,CDA ISD 2012-236T16:38:00 Enter: S75,ISD observation around apoapse 2012-236T16:38:00 43.355822 Rs,,,,,, 2012-237T18:34:00,000T07:45:00,24-Aug-12,CDA,Non-SPASS,Other,RATE010A,,Data rate Enter:SApo Enter: S75,Range enter= 6.3174539 Rs exit= 7.2917467 Range altitude= 40017.515 km ... -40501.884,,,,,,