PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "2009-02-04 D. Humm (APL) v5 to go with v5 AT CDRs; 2009-05-20 D. Humm (APL) still v5 but new filename format" DATA_SET_ID = "MRO-M-CRISM-6-ADR-V1.0" PRODUCT_ID = "ADR50924300802_094B5_VS30L_6" /*( ADRptttttttttt_xxxxx_VSbwn_v )*/ /*( p = partition at start of validity )*/ /*( tttttttttt = sclk at start of validity )*/ /*( xxxxx = obs. ID of volcano scan TRDR )*/ /*( r = frame rate identifier, 0-4 )*/ /*( b = binning identifier, 0-3 )*/ /*( eee = exposure time parameter, 0-480 )*/ /*( w = wavelength filter, 0-3 )*/ /*( s = side: 1 or 2, or 0 if N/A )*/ /*( n = sensor ID: S, L, or J )*/ /*( v = version )*/ PRODUCT_TYPE = ADR INSTRUMENT_HOST_NAME = "MARS RECONNAISSANCE ORBITER" SPACECRAFT_ID = MRO INSTRUMENT_NAME = "COMPACT RECONNAISSANCE IMAGING SPECTROMETER FOR MARS" INSTRUMENT_ID = CRISM TARGET_NAME = MARS START_TIME = 2009-04-15T22:13:00 STOP_TIME = NULL SPACECRAFT_CLOCK_START_COUNT = "5/0924300802" SPACECRAFT_CLOCK_STOP_COUNT = NULL OBSERVATION_TIME = NULL PRODUCT_CREATION_TIME = 2009-10-09T20:00:00 MRO:SENSOR_ID = "L" PRODUCT_VERSION_ID = "6" SAMPLING_MODE_ID = "HYPERSPEC" MRO:WAVELENGTH_FILE_NAME = "CDR450924300802_WA0300000L_3.IMG" PIXEL_AVERAGING_WIDTH = 10 /*( pixel bin size, across track ) */ MRO:WAVELENGTH_FILTER = "0" /* This ADR label describes one calibration data file. The file */ /* is a mutiple-band, multiple-frame image file derived from flight data. */ /* It consists of a binary image followed by a list of row numbers */ /* corresponding to the wavelength filter. */ /* The VS or volcano scan ADR was calculated by Frank Morgan */ /* of JHU/APL from CRISM observations of Olympus Mons. */ SOURCE_PRODUCT_ID = { "FFC000094B5_00_IF254L_TRR2", "FFC000094B5_02_IF254L_TRR2" } /* This VS ADR gives atmospheric tranmission derived from volcano scan */ /* observation ID 094B5. */ /* It includes a spectral fit-based adjustment to correct an aerosol-like */ /* slope at wavelengths shortward of approximately 2.7 microns. */ /* The raw AT transmission is fit at wavelengths outside gas absorptions */ /* with an aerosol model with optical depth quadratic in log wavelength. */ /* The raw AT is divided by the fit to correct variable short wavelength */ /* slopes. */ OBJECT = FILE ^IMAGE = "ADR50924300802_094B5_VS30L_6.IMG" /* offset is in file records, which is just (imgbands*imglines) + 1 */ ^ROWNUM_TABLE = ("ADR50924300802_094B5_VS30L_6.IMG",439 ) RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 256 /* one row now, not one frame to save space in table */ FILE_RECORDS = 442 /* compute by ROUND ((imgbands * imglines * */ /* line_samples * samplebits/8 + */ /* tablerows * tablerowbytes) / */ /* record_bytes + 0.5 ) */ OBJECT = IMAGE LINES = 1 LINE_SAMPLES = 64 SAMPLE_TYPE = PC_REAL SAMPLE_BITS = 32 BANDS = 438 BAND_NAME = NULL BAND_STORAGE_TYPE = LINE_INTERLEAVED DESCRIPTION = "Atmospheric transmission" END_OBJECT = IMAGE /* be sure to pad this object to a full record (2560/bin bytes here) */ OBJECT = ROWNUM_TABLE NAME = "SELECTED ROWS FROM DETECTOR" INTERCHANGE_FORMAT = "BINARY" ROWS = 438 COLUMNS = 1 ROW_BYTES = 2 DESCRIPTION = "The detector is subsampled in the spectral direction by selecting specific rows to be downlinked. This table provides a list of the rows selected for all frames in this multidimensional image cube." OBJECT = COLUMN NAME = DETECTOR_ROW_NUMBER DATA_TYPE = MSB_UNSIGNED_INTEGER BIT_MASK = 2#0000000111111111# START_BYTE = 1 BYTES = 2 DESCRIPTION = "Detector row number from which the data was taken." END_OBJECT = COLUMN END_OBJECT = ROWNUM_TABLE END_OBJECT = FILE END