PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 1024 FILE_RECORDS = 300 ^IMAGE = "9132S00A.SRI" INSTRUMENT_HOST_NAME = "MARS GLOBAL SURVEYOR" TARGET_NAME = "MARS" INSTRUMENT_NAME = "RADIO SCIENCE SUBSYSTEM" DATA_SET_ID = "MGS-M-RSS-5-SDP-V1.0" PRODUCT_ID = "9132S00A.SRI" PRODUCT_RELEASE_DATE = 2001-01-28 DESCRIPTION = "This file contains a 2-D array in image format showing power vs frequency and time near a Mars Global Surveyor radio occultation. A nominal image is made from 300 512-point power spectra where the spacing between spectra is 0.2048 s and the frequency spanned is 2500 Hz (4.88 Hz resolution). Images show the spacecraft carrier emerging from occultation (egress) or disappearing as the spacecraft goes behind the limb (ingress). Near the occultation time there may be a weak surface echo racing away from the carrier to lower frequencies (egress) or coming in from higher frequencies to merge with the carrier at occultation (ingress). The keywords for start and stop time give the beginning and ending of data recording for the occultation. For exact times of each spectrum see the Surface Reflection Table file that corresponds to this image (same file name except for suffix .SRT). This image was produced by Dick Simpson of the MGS Radio Science Team." START_TIME = 1999-05-12T18:00:00 STOP_TIME = 1999-05-12T18:10:00 SOFTWARE_NAME = "SURF2PDS;2000-06-26" PRODUCT_CREATION_TIME = 2000-07-26T19:48:07 PRODUCER_ID = "MGS RST" OBJECT = IMAGE LINES = 300 LINE_SAMPLES = 512 SAMPLE_TYPE = MSB_INTEGER SAMPLE_BITS = 16 UNIT = "DECIBEL" OFFSET = 0.0 SCALING_FACTOR = 0.01 DESCRIPTION = "This image contains values of received signal power versus frequency and time in units of decibels relative to one watt. Values can be obtained by multiplying the sample in the image by SCALING_FACTOR and then adding OFFSET. Each line in the image corresponds to one power spectrum. The first line in the file is the LAST spectrum. The first point in a line corresponds to the lowest frequency (0 Hz)." END_OBJECT = IMAGE END