CCSD3ZF0000100000001NJPL3IF0PDS200000001 = SFDU_LABEL /* File Structure */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 512 FILE_RECORDS = 301 LABEL_RECORDS = 27 CHECKSUM = 4048258 /* Unsigned 32-bit checksum of all bytes after label records */ FILE_STATE = CLEAN ^HISTORY = 28 OBJECT = HISTORY END_OBJECT = HISTORY ^HISTOGRAM_IMAGE = 52 OBJECT = HISTOGRAM_IMAGE /* Two dim histogram image structure */ LINES = 256 LINE_SAMPLES = 408 SAMPLE_TYPE = UNSIGNED_INTEGER SAMPLE_BITS = 8 SAMPLE_NAME = BAND LINE_NAME = INTENSITY NOTE = "This is an unannotated two-dimensional histogram 'image' showing frequency of measured 'Intensity' versus band number. The 'Intensity' may be DN, Radiance, or BDRF (Bi-Directional Reflectance), or a combination of BDRF with Radiance, with BDRF below a cutoff band number and radiance above. The cutoff is defined by: BDRF_RAD_TRANSITION_BAND_NUMBER. The 'Intensity' is DN only if CORE_NAME in the QUBE object is RAW_DATA_NUMBER." BDRF_RAD_TRANSITION_BAND_NUMBER = 1 END_OBJECT = HISTOGRAM_IMAGE ^QUBE = 256 OBJECT = QUBE /* Qube structure */ AXES = 3 AXIS_NAME = (SAMPLE,LINE,BAND) /* Core description */ CORE_ITEMS = (20,6,48) CORE_ITEM_BYTES = 4 CORE_ITEM_TYPE = VAX_REAL CORE_BASE = 0.0 CORE_MULTIPLIER = 1.0 /* Core scaling is: True_value = base + (multiplier * stored_value) */ CORE_VALID_MINIMUM = 16#FFEFFFFF# CORE_HIGH_REPR_SATURATION = 16#FFFBFFFF# CORE_HIGH_INSTR_SATURATION = 16#FFFCFFFF# CORE_LOW_INSTR_SATURATION = 16#FFFDFFFF# CORE_LOW_REPR_SATURATION = 16#FFFEFFFF# CORE_NULL = 16#FFFFFFFF# CORE_NAME = RADIANCE_FACTOR CORE_UNIT = DIMENSIONLESS /* 'Radiance factor' = ( PI * Radiance) / Solar_Flux */ SPATIAL_BINNING_TYPE = FOOTPRINT_AVERAGE THRESHOLD_WEIGHT = 0.10000 FOOTPRINT_GRID_SIZE = 10 /* SPATIAL_BINNING_TYPE, FOOTPRINT_GRID_SIZE, THRESHOLD_WEIGHT, and */ /* (for certain projections) MAXIMUM_PIXEL_DISTORTION, are parameters */ /* that are not relevant to the Tube core data, but can be used in */ /* subsequent ISIS processing to generate a projected cube from a */ /* tube file with program NIMSGEOMF. Note that the value: */ /* SPATIAL_BINNING_TYPE = FOOTPRINT_AVERAGE */ /* does trigger the addition of two extra backplanes per grating */ /* position: the RIGHT_EDGE_PROJ_LINE/SAMPLE backplanes. */ EXPANDED_RADIUS = 85790.40 DARK_UPDATE_TYPE = NOUPDAT FILL_BOX_SIZE = 0 FILL_MIN_VALID_PIXELS = 0 PHOTOMETRIC_CORRECTION_TYPE = NONE /* Suffix description */ SUFFIX_BYTES = 4 SUFFIX_ITEMS = (0,0,1) BAND_SUFFIX_NAME = NATIVE_TIME BAND_SUFFIX_UNIT = SECOND BAND_SUFFIX_ITEM_BYTES = 4 BAND_SUFFIX_ITEM_TYPE = VAX_REAL BAND_SUFFIX_BASE = 0.000000 BAND_SUFFIX_MULTIPLIER = 63.000000 BAND_SUFFIX_VALID_MINIMUM = (16#FFEFFFFF#) BAND_SUFFIX_NULL = (16#FFFFFFFF#) BAND_SUFFIX_LOW_REPR_SAT = (16#FFFEFFFF#) BAND_SUFFIX_LOW_INSTR_SAT = (16#FFFDFFFF#) BAND_SUFFIX_HIGH_INSTR_SAT = (16#FFFCFFFF#) BAND_SUFFIX_HIGH_REPR_SAT = (16#FFFBFFFF#) /* The NATIVE TIME band of the suffix is the time in "chops" of */ /* the first grating position at the corresponding line and sample */ /* after the NATIVE START TIME, where 63 chops = 1 second. */" /* Data description: general */ DATA_SET_ID = 'GO-J-NIMS-3-TUBE-V1.0' SPACECRAFT_NAME = GALILEO_ORBITER MISSION_PHASE_NAME = CALLISTO_20_ENCOUNTER INSTRUMENT_NAME = 'NEAR INFRARED MAPPING SPECTROMETER' INSTRUMENT_ID = NIMS ^INSTRUMENT_DESCRIPTION = "NIMSINST.TXT" TARGET_NAME = CAL START_TIME = 1999-05-05T20:21:24Z STOP_TIME = 1999-05-05T20:22:10Z NATIVE_START_TIME = "4982425.00.0" NATIVE_STOP_TIME = "4982425.69" OBSERVATION_NAME = '20NNOPCAL_03A' NOTE = "Optical calibration of the NIMS grating // OPCAL // MIPL Systematic Processing Product" PRODUCT_ID = "20NNOPCAL_03A_MSY01.VIOF" PRODUCT_CREATION_DATE = 2000-06-14 IMAGE_ID = NULL MIN_SPACECRAFT_SOLAR_DISTANCE = 7.40644e+08 MAX_SPACECRAFT_SOLAR_DISTANCE = 7.40644e+08 MINIMUM_CENTRAL_BODY_DISTANCE = 2063620.00 MAXIMUM_CENTRAL_BODY_DISTANCE = 2063620.00 /* Data description: instrument status */ INSTRUMENT_MODE_ID = LONG_MAP GAIN_MODE_ID = 4 CHOPPER_MODE_ID = REFERENCE START_GRATING_POSITION = 00 OFFSET_GRATING_POSITION = 04 GRATING_POSITION_INCREMENT = 01 GRATING_POSITIONS = 24 MEAN_FOCAL_PLANE_TEMPERATURE = 65.00 MEAN_RAD_SHIELD_TEMPERATURE = 0.00 MEAN_TELESCOPE_TEMPERATURE = 0.00 MEAN_GRATING_TEMPERATURE = 130.00 MEAN_CHOPPER_TEMPERATURE = 0.00 MEAN_ELECTRONICS_TEMPERATURE = 0.00 MEAN_DARK_DATA_NUMBER = (27.66,27.27,29.67,26.02,24.92,22.31, 26.22,26.85,25.36,8.95,33.32,34.82,32.42,30.88,29.36,28.34, 26.65) /* The "mean dark data numbers" are the DN value of dark sky for each of the */ /* 17 NIMS detectors, averaged over the mirror-position-specific values used */ /* in the computation of radiance. The original dark values were obtained */ /* from either off-limb portions of the observation or special "heaven dark" */ /* observations for an encounter. */ THERMAL_DETECTOR_OFFSET = (515.50,516.03,514.03) THERMAL_DETECTOR_SENS_RATIO = (47.56,47.34,48.29) GROUP = BAND_BIN /* Spectral axis description */ BAND_BIN_CENTER = (0.6869,0.6948,0.7027,0.7106,0.7185,0.7264, 0.7344,0.7423,0.7502,0.7581,0.7660,0.7739,0.7818,0.7897, 0.7976,0.8055,0.8134,0.8213,0.8292,0.8371,0.8450,0.8529, 0.8608,0.8688,0.8258,0.8338,0.8417,0.8496,0.8575,0.8654, 0.8734,0.8813,0.8892,0.8971,0.9050,0.9129,0.9209,0.9288, 0.9367,0.9446,0.9525,0.9604,0.9684,0.9763,0.9842,0.9921, 1.0000,1.0079) BAND_BIN_UNIT = MICROMETER BAND_BIN_ORIGINAL_BAND = (1,2,3,4,5,6,7,8,9,10,11,12,13,14, 15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33, 34,35,36,37,38,39,40,41,42,43,44,45,46,47,48) BAND_BIN_GRATING_POSITION = (0,1,2,3,4,5,6,7,8,9,10,11,12,13, 14,15,16,17,18,19,20,21,22,23,0,1,2,3,4,5,6,7,8,9,10,11, 12,13,14,15,16,17,18,19,20,21,22,23) BAND_BIN_DETECTOR = (1,1,1,1,1,1,1,1,1,1,1,1,1,1,1,1,1,1,1, 1,1,1,1,1,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2,2, 2) BAND_BIN_SOLAR_FLUX = (6318.7402,6183.9702,6050.6299,5918.8501, 5788.7202,5660.3501,5533.8301,5409.2202,5287.0200,5186.8101, 5087.8101,4990.0698,4893.6299,4798.5498,4704.8301,4616.1401, 4530.2798,4445.6699,4362.3301,4280.2900,4199.5498,4120.1201, 4042.0100,3965.2100,4397.8198,4315.0898,4233.6602,4153.5400, 4074.7400,3997.2600,3921.1101,3846.2800,3772.7700,3700.5701, 3637.7200,3580.4099,3523.9700,3468.3899,3413.6599,3359.7800, 3306.7700,3254.5901,3203.2600,3152.7700,3103.1001,3054.2600, 3006.2300,2957.4500) BAND_BIN_SENSITIVITY = (0.6491,0.7183,0.7998,0.8976,0.9833, 1.0609,1.1409,1.2210,1.3000,1.3082,1.2907,1.2520,1.2388, 1.2314,1.2708,1.2991,1.3129,1.2737,1.2083,1.1252,1.0373, 0.9774,0.9678,0.9754,1.1770,1.0750,1.0468,1.0368,1.0178, 0.9611,0.8911,0.8660,0.8814,0.8980,0.8703,0.7835,0.6542, 0.5419,0.4667,0.4224,0.3954,0.3680,0.3281,0.2801,0.2316, 0.1773,0.1329,0.0922) /* "Band Bin Sensitivity" is the sensitivity for each band, in units of */ /* DN/radiance_unit (see CORE UNIT). These values are functions of */ /* reported focal plane assembly temperature during the observation and */ /* of ground and flight calibration data. They may be used to construct */ /* "idealized data numbers" (DNs which would have been measured by an */ /* anomaly-free instrument) by the formula: */ /* DN = dark_value + sensitivity * radiance, */ /* where 'dark_value' is approximated by the MEAN_DARK_DATA_NUMBER array, */ /* preceding the BAND_BIN group. */ /* Note that actually measured raw DNs are not obtainable in this way, */ /* due to corrections for instrument anomalies (see the referenced */ /* INSTRUMENT_DESCRIPTION for details) and possible resampling of the */ /* data. The above formula for DN also does not hold for the higher */ /* intensity regime in the thermal detectors (15-17), for which the */ /* following formula applies: */ /* DN = thermal_offset + sensitivity * radiance / sens_ratio */ /* where 'thermal_offset' and 'sens_ratio' for detectors 15, 16, and 17 are */ /* given by the THERMAL_DETECTOR_OFFSET and THERMAL_DETECTOR_SENS_RATIO */ /* arrays, preceding the BAND_BIN group. */ /* The radiances for which the above formula applies, are those lying above: */ /* Cutoff_radiance = thermal_offset / sensitivity */ END_GROUP = BAND_BIN END_OBJECT = QUBE END GROUP = VISIS2 VERSION_DATE = 2000-01-26 DATE_TIME = 2000-06-14T11:47:00 NODE_NAME = "MIPL" USER_NAME = "FrankLeader/43214" SOFTWARE_DESC = "ISIS cube file with PDS label has been generated as systematic product by MIPL using the following programs: NIMSMERGE2 to create EDRs; NIMSCMM2 to create the merged mosaic & geometry cube; HIST2D to create a two-dimensional histogram; NIMSR2IOF to convert Radiance to BDRF; VISIS2 to create the ISIS cube." USERNOTE = "MIPL Systematic Processing Product" GROUP = PARAMETERS EDR_FILE_NAME = "NE:20NNOPCAL_03A.4" PLATFORM_CKERNEL_NAME = " " ROTOR_CKERNEL_NAME = " " SP_KERNEL_FILE_NAME = "SPICEKER:S980928A.BSP" I_KERNEL_FILE_NAME = "NDAT:NIMS_IKERNEL_MAB5.DAT" SPIKE_FILE_NAME = "DUMMY_DSPK.DAT" BOOM_FILE_NAME = "GLL:[NIMS.CAL]BOOM_OBSCURATION.NIM" DARK_VALUE_FILE_NAME = "NCAL:16HNDARKCL04A_FEL02.DRK" CALIBRATION_FILE_NAME = "NCAL:N1999A_GS4_06_C20.CAL" SOLAR_FLUX_FILE_NAME = "NCAL:NIMS_SOLAR.DAT" MERGED_MOSAIC_FILE_NAME = "GLLNIMS:20NNOPCAL_03A_MSY01.TIOF" GRATING_POSITION_CORRECTION = 1.7400 GRATING_STEP_INFLATION = 0.2145 /* The "Grating Position Correction" and "Grating Step Inflation" are */ /* adjustments to the nominal grating positions, based on flight calibrations */ /* and known sharp spectral features of the target, used in determination of */ /* wavelengths. GRATING_POSITION_CORRECTION is an additive term to the */ /* grating position and (1.0 + GRATING_STEP_INFLATION) is a multiplicative */ /* term modifying the grating stepsize. */ SUMMARY_IMAGE_RED_ID = 0 SUMMARY_IMAGE_GREEN_ID = 0 SUMMARY_IMAGE_BLUE_ID = 0 ADAPT_STRETCH_SAT_FRAC = 0.0000 ADAPT_STRETCH_SAMP_FRAC = -999.0000 RED_STRETCH_RANGE = ( -999, 0) GREEN_STRETCH_RANGE = ( -999, 0) BLUE_STRETCH_RANGE = ( -999, 0) END_GROUP = PARAMETERS END_GROUP = VISIS2 END 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