PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM START_TIME = 2008-01-25T01:25:00 STOP_TIME = 2008-01-25T01:45:00 PRODUCT_CREATION_TIME = 2011-04-12T17:18:32.000 SPACECRAFT_CLOCK_START_COUNT = "N/A" SPACECRAFT_CLOCK_STOP_COUNT = "N/A" PROCESSING_LEVEL_ID = 1 PRODUCT_TYPE = "UDR" OBSERVATION_TYPE = "Bistatic Radar" DATA_SET_ID = "MEX-M-MRS-1/2/3-EXT2-1421-V1.0" DATA_SET_NAME = "MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 2 1421 V1.0" MISSION_ID = "MEX" ORBIT_NUMBER = 5219 MISSION_NAME = "MARS EXPRESS" INSTRUMENT_HOST_NAME = "MARS EXPRESS" INSTRUMENT_NAME = "MARS EXPRESS ORBITER RADIO SCIENCE" INSTRUMENT_TYPE = "RADIO SCIENCE" TARGET_NAME = MARS TARGET_TYPE = "PLANET" INSTRUMENT_HOST_ID = "MEX" STANDARD_DATA_PRODUCT_ID = BRO DATA_QUALITY_ID = "N/A" DATA_QUALITY_DESC = "See the DATASET.CAT for further information on the quality of this data set." SPACECRAFT_POINTING_MODE = "EARTH" ^SPACECRAFT_POINTING_MODE_DESC= "MEX_POINTING_MODE_DESC.TXT" INSTRUMENT_MODE_ID = "ONED" INSTRUMENT_MODE_DESC = "ONE-WAY DUAL-FREQUENCY X&S-Band D/L" PRODUCER_ID = "SUE" PRODUCER_FULL_NAME = "MARTIN PAETZOLD" PRODUCER_INSTITUTION_NAME= "RHEINISCHES INSTITUT FUER UMWELTFORSCHUNG, PLANETENFORSCHUNG" PRODUCT_ID = "M63R2A4L1A_BRO_080252230_01" SOURCE_PRODUCT_ID = "M63R2A4L1A_RSR_080252230_01.DAT" ^PS_DOCUMENT = "M63R2A4L1A_BRO_080252230_01.AUX" ^BROWSE_IMAGE = "M63R2A4L1A_BRO_080252230_01.JPG" OBJECT = PS_DOCUMENT DOCUMENT_NAME = "MEX RADIO SCIENCE QUICK LOOK PLOT SET" PUBLICATION_DATE = 2008-01-30 DOCUMENT_TOPIC_TYPE = "N/A" INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = "POSTSCRIPT" FILES = 1 DESCRIPTION = " PostScript files contain one figure each showing quick look views after early processing of raw data. These may be useful in identifying data which deserve more detailed inspection. For example, by printing the PostScript file, the user can determine whether a signal was easily detectable or whether the data were corrupted. Certain data anomalies (saturation in the analog-to-digital converters, clipping in amplifiers ahead of the ADCs, receiver tuning errors, poor choices of receiver gain, etc.) can be readily seen in the plots. Each PostScript file is sized to fit on a single 8-1/2 x 11 inch page. Each landscape format page includes four panels showing: upper left: a histogram of raw data samples (for high sample resolutions -- e.g., 16 bits -- the histogram plot is usually compressed by aggregating adjacent bins); upper right: a sequence of average power spectra derived from the raw samples (each spectrum typically represents 60 s); lower left: averaged raw sample power versus time (typically sample power is averaged over 1 s); and lower right: an extract of the first few lines of the source RSR PDS label PostScript file names have the form ydddhhmm.PS1 where y is the one-digit year (0-9) ddd is the three-digit day-of-year (001-366) hh is the two-digit hour (00-23) mm is the two-digit minute (00-59) The file names are chosen so that they match the RSR file names ydddhhmm.RSR. Note that, in cases when there were multiple recordings of the same event starting at the same time, the mm component may be modified in one of the files so that file names are unique. Each panel was generated by MATLAB as a Level 1 PostScript file for color printers. The panels were then assembled into single page PostScript files using the psmulti utility, a PERL script written by D. Murray Laing. The computing platform was a Sun Ultra running Solaris 2.8. MATLAB is a technical computing environment for computation and visualization distributed by The Math Works, Inc., Natick MA. MATLAB is a trademark of The Math Works, Inc. PostScript is a trademark of Adobe Systems, Inc. The files were later converted to 300 dpi JPEG files with corrected MaRS compliant file names." END_OBJECT = PS_DOCUMENT OBJECT = BROWSE_IMAGE ENCODING_TYPE = JPEG LINES = 3300 LINE_SAMPLES = 2550 SAMPLE_BITS = 24 SAMPLE_TYPE = UNSIGNED_INTEGER END_OBJECT = BROWSE_IMAGE END