CCSD3ZF0000100000001NJPL3IF0PDS200000001 = SFDU_LABEL /* Detached PDS label for the PV-ORAD brightness temperature image */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 8192 FILE_RECORDS = 1025 /* Pointers to image file and objects within it */ ^FOREIGN_LABEL = ("PVEN002T.IMG",1) ^IMAGE = ("PVEN002T.IMG",2) /* Image descriptive information */ DATA_SET_ID = "P12-V-ORAD-5-RADAR-IMAGE-V1.0" TARGET_NAME = VENUS SPACECRAFT_NAME = "PIONEER VENUS ORBITER" INSTRUMENT_NAME = "ORBITING RADAR" TRANSMITTED_POLARIZATION = "LINEAR" RECEIVED_POLARIZATION = "SAME SENSE LINEAR" WAVELENGTH = 17. DATA_SET_PARAMETER_NAME = BRIGHTNESS_TEMPERATURE DATA_SET_PARAMETER_UNIT = "DEGREES KELVIN" MAP_PROJECTION_TYPE = "SIMPLE CYLINDRICAL" MAP_SCALE = 5.686 MAXIMUM_LATITUDE = 90.0 MINIMUM_LATITUDE = -90.0 MAXIMUM_LONGITUDE = 240.0 MINIMUM_LONGITUDE = 240.0 PRODUCER_FULL_NAME = "PETER G. FORD" NOTE = "VICAR format image of Venus microwave brightness temperature, in degrees Kelvin, derived from the Pioneer Venus radar altimeter planet and cold-sky calibration measurements, as follows: the dataset was divided into 1 degree latitude intervals. For each interval, the average SC reading was taken to represent a measurement of the 3K cold sky. The average PC values from lowland regions were interpreted as measuring an average temperature of 735K with an emissivity of 88%. The brightness temperature is therefore given by (735*0.88*(PC-)+3*(-PC))/(-). For reference, see Ford, P.G. and G.H. Pettengill, Venus: Global surface radio emissivity, Science, 220, 1379-1381, 1983." /* Object descriptions */ OBJECT = FOREIGN_LABEL TYPE = VICAR2 RECORDS = 1 BYTES = 8192 ^DESCRIPTION = "VICAR2.TXT" END_OBJECT = FOREIGN_LABEL OBJECT = IMAGE LINES = 1024 LINE_SAMPLES = 2048 SAMPLE_BITS = 32 SAMPLE_TYPE = VAX_REAL END_OBJECT = IMAGE END