PDS_VERSION_ID                  = PDS3
RECORD_TYPE                     = FIXED_LENGTH
RECORD_BYTES                    = 2
FILE_RECORDS                    = 6011145
PRODUCT_ID                      = "HSP2012_004_15_29"
SPACECRAFT_CLOCK_START_COUNT    = "1/1704381628.96"
SPACECRAFT_CLOCK_STOP_COUNT     = "UNK"
START_TIME                      = 2012-004T14:29:49.491
STOP_TIME                       = 2012-004T16:10:00.636
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                  = 144798
MISSION_PHASE_NAME              = XXM
PRODUCT_CREATION_TIME           = 2012-362
INTEGRATION_DURATION            = 1 <MILLISECOND>
COMPRESSION_TYPE                = "SQRT_9"
HI_VOLTAGE_POWER_SUPPLY_STATE   = ON
ODC_ID                          = 1120 /* 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                  = "HSP2012_004_15_29.DAT"
RIGHT_ASCENSION           = 83.858
DECLINATION               = -5.91
SUB_SOLAR_LATITUDE        = "UNK"  /* insufficient ephemeris data. */
SUB_SOLAR_LONGITUDE       = "UNK"  /* insufficient ephemeris data. */
SUB_SPACECRAFT_LATITUDE   = "UNK"  /* insufficient ephemeris data. */
SUB_SPACECRAFT_LONGITUDE  = "UNK"  /* insufficient ephemeris data. */
PHASE_ANGLE               = "UNK"  /* insufficient ephemeris data. */
EMISSION_ANGLE            = "UNK"  /* insufficient ephemeris data. */
INCIDENCE_ANGLE           = "UNK"  /* insufficient ephemeris data. */
CENTRAL_BODY_DISTANCE     = "UNK"  /* insufficient ephemeris data. */
SC_PLANET_POSITION_VECTOR =   
"UNK"  /* insufficient ephemeris data. */
SC_PLANET_VELOCITY_VECTOR =   
"UNK"  /* insufficient ephemeris data. */
SC_SUN_POSITION_VECTOR    =   
(-1.3365178e+09<KM>, -5.3830593e+08<KM>, -1.6464897e+08<KM>)
SC_SUN_VELOCITY_VECTOR    =   
(18.940011<KM/S>, -11.660971<KM/S>, -4.7143653<KM/S>)
SC_TARGET_POSITION_VECTOR =   
"UNK"  /* insufficient ephemeris data. */
SC_TARGET_VELOCITY_VECTOR =   
"UNK"  /* insufficient ephemeris data. */
PLANET_CENTER_POSITION_VECTOR =   
"UNK"  /* insufficient ephemeris data. */
PLANET_CENTER_VELOCITY_VECTOR =   
"UNK"  /* insufficient ephemeris data. */
/* UVIS HSP Channel Time Series Object Definition */
OBJECT                          = TIME_SERIES
  INTERCHANGE_FORMAT            = BINARY
  ROWS                          = 6011145
  COLUMNS                       = 1
  ROW_BYTES                     = 2
  SAMPLING_PARAMETER_NAME       = TIME
  SAMPLING_PARAMETER_UNIT       = MILLISECONDS
  SAMPLING_PARAMETER_INTERVAL   = 1.000
  DESCRIPTION                   = "Sequence of counts from UVIS HSP.
        The purpose of this observation is to observe a stellar
    occultation by Saturn's main rings, making high spatial resolution
    measurements of ring structure with the HSP.  Usually, the FUV
    measures the ring reflectance for spatial-spectral mapping of the
    rings and background measurements."
  OBJECT                        = COLUMN
    NAME                        = PHOTOMETER_COUNTS
    DATA_TYPE                   = MSB_UNSIGNED_INTEGER
    START_BYTE                  = 1
    BYTES                       = 2
  END_OBJECT                    = COLUMN
END_OBJECT                      = TIME_SERIES
END