PDS_VERSION_ID = PDS3 PRODUCT_ID = GLLUVS2:[GLL_RAW.EUV_P2]EUV_G08A.IDLSAVE;2 PRODUCT_NAME = "EUV OBSERVATION DATA" OBSERVATION_ID = "ALL EUV OBSERVATIONS FOR G08A" PRODUCT_CREATION_DATE = 4-JUN-1997 FILE_RECORDS = 14 SPACECRAFT_NAME = "GALILEO ORBITER" INSTRUMENT_NAME = "EXTREME ULTRAVIOLET SPECTROMETER" MISSION_PHASE_NAME = "JUPITER ORBIT OPERATIONS" SPACECRAFT_CLOCK_START_TIME = 3942462:00:0 SPACECRAFT_CLOCK_STOP_TIME = 3943748:00:0 ^TABLE = "EUV_IDLSAVE.FMT" DESCRIPTION = " This file was produced by the Galileo UVS/EUV team at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado at Boulder. Refer to the Galileo UVS/EUV instrument paper 'Galileo Ultraviolet Spectrometer Experiment', Vol 60, Space Science Reviews, pages 503-530, by C.W. Hord et al, for hardware and calibration information. Also see the EUV instrument template and catalog files for additional instrument information. This file, written in the IDL 'save file' format, contains data records for all EUV observations during the listed orbit. The data records are contained in an array of anonymous IDL strucures. Each data record includes the following parameters: spacecraft start time, spacecraft stop time, and EUV observation data. There is one record for each RTS summation buffer during the orbit. The following is an example of an array with thirty observation data records: EUV_DAT STRUCT = -> Array[30] Within the array 'EUV_DAT,' the structures have the following form: ** Structure <7132ac>, 3 tags, length=24584, refs=1: START LONG 3893922 FIN LONG 3893981 DATA DOUBLE Array[24, 128] The spacecraft start and stop time, labeled as START and FIN in the IDL structure, are the start and end times, in RIMS, of the orbital observations included in the DATA array. The DATA array is a double- precision, floating point matrix consisting of 24 sky-sectors by 128 wavelengths. The 'superpixel' bins have been deconvolved into the standard 128 pixel EUV detector locations. Note that that values for the last two wavelengths are zero. The (IDL) 0th sky-sector is the first sampled. Notice that the early (Nominal mission) orbits sampled the torus before encounters so the 0th word is North-Poleward while orbits C9 and E14 (and after) observe the torus after encounter so the 0th sky-sector is South-Poleward. " END