PDS_VERSION_ID                  = PDS3
RECORD_TYPE                     = FIXED_LENGTH
RECORD_BYTES                    = 2
FILE_RECORDS                    = 498960
PRODUCT_ID                      = "HSP2004_088_03_54_23"
SPACECRAFT_CLOCK_START_COUNT    = "1/1459138664.160"
SPACECRAFT_CLOCK_STOP_COUNT     = "UNK"
START_TIME                      = 2004-088T03:54:22.856
STOP_TIME                       = 2004-088T04:27:38.696
DATA_SET_ID                     = "CO-S-UVIS-2-SSB-V1.2"
TARGET_NAME                     = "STAR"
INSTRUMENT_HOST_NAME            = "CASSINI_ORBITER"
INSTRUMENT_NAME                 = "ULTRAVIOLET IMAGING SPECTROGRAPH"
INSTRUMENT_ID                   = "UVIS"
OBSERVATION_ID                  = 41935
MISSION_PHASE_NAME              = CRUISE
PRODUCT_CREATION_TIME           = 2012-024
INTEGRATION_DURATION            = 8 <MILLISECOND>
COMPRESSION_TYPE                = "SQRT_9"
HI_VOLTAGE_POWER_SUPPLY_STATE   = ON
ODC_ID                          = 103 /* INDEX INTO PLANNING PRODUCTS */
DESCRIPTION                     = "
  This file was produced by the Cassini UVIS team at the Laboratory
  for Atmospheric and Space Physics (LASP) at the University of Colorado
  at Boulder.  For a description of hardware and scientific objectives,
  refer to the Cassini UVIS instrument paper The Cassini Ultraviolet
  Imaging Spectrograph Investigation, Space Science Reviews, 115, 299-361,
  by L. W. Esposito et. al."
 
^TIME_SERIES                  = "HSP2004_088_03_54_23.DAT"
RIGHT_ASCENSION           = "N/A" /* interplanetary Hydrogen survey */
DECLINATION               = "N/A" /* interplanetary Hydrogen survey */
SUB_SOLAR_LATITUDE        = "N/A" /* interplanetary Hydrogen survey */
SUB_SOLAR_LONGITUDE       = "N/A" /* interplanetary Hydrogen survey */
SUB_SPACECRAFT_LATITUDE   = "N/A" /* interplanetary Hydrogen survey */
SUB_SPACECRAFT_LONGITUDE  = "N/A" /* interplanetary Hydrogen survey */
PHASE_ANGLE               = "N/A" /* interplanetary Hydrogen survey */
EMISSION_ANGLE            = "N/A" /* interplanetary Hydrogen survey */
INCIDENCE_ANGLE           = "N/A" /* interplanetary Hydrogen survey */
CENTRAL_BODY_DISTANCE     = "N/A" /* interplanetary Hydrogen survey */
SC_PLANET_POSITION_VECTOR =   
(37600272.0<KM>, 27511849.0<KM>, 8110278.6<KM>)
SC_PLANET_VELOCITY_VECTOR =   
(-4.2976668<KM/S>, -3.0938243<KM/S>, -0.92193596<KM/S>)
SC_SUN_POSITION_VECTOR    =   
(-3.4078052e+08<KM>, 1.1855051e+09<KM>, 5.0595924e+08<KM>)
SC_SUN_VELOCITY_VECTOR    =   
(-5.6374915<KM/S>, 0.90707970<KM/S>, 0.44562608<KM/S>)
SC_TARGET_POSITION_VECTOR =   
"N/A" /* interplanetary Hydrogen survey */
SC_TARGET_VELOCITY_VECTOR =   
"N/A" /* interplanetary Hydrogen survey */
PLANET_CENTER_POSITION_VECTOR =   
"N/A" /* interplanetary Hydrogen survey */
PLANET_CENTER_VELOCITY_VECTOR =   
"N/A" /* interplanetary Hydrogen survey */
/* UVIS HSP Channel Time Series Object Definition */
OBJECT                          = TIME_SERIES
  INTERCHANGE_FORMAT            = BINARY
  ROWS                          = 498960
  COLUMNS                       = 1
  ROW_BYTES                     = 2
  SAMPLING_PARAMETER_NAME       = TIME
  SAMPLING_PARAMETER_UNIT       = MILLISECONDS
  SAMPLING_PARAMETER_INTERVAL   = 8.000
  DESCRIPTION                   = "Sequence of counts from UVIS HSP.
        The purpose of this observation is to measure the HeI 584A and HI
    Lyman Series emissions from the interplanetary/local interstellar
    medium, while the S/C rotates about the Z-axis."
  OBJECT                        = COLUMN
    NAME                        = PHOTOMETER_COUNTS
    DATA_TYPE                   = MSB_UNSIGNED_INTEGER
    START_BYTE                  = 1
    BYTES                       = 2
  END_OBJECT                    = COLUMN
END_OBJECT                      = TIME_SERIES
END