PDS_VERSION_ID = "PDS3" DATA_SET_ID = "MEX-M-MRS-1/2/3-EXT1-0786-V1.0" DATA_SET_NAME = "MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 1 0786 V1.0" MISSION_ID = "MEX" MISSION_NAME = "MARS EXPRESS" ORBIT_NUMBER = 2627 PROCESSING_LEVEL_ID = 3 PRODUCT_TYPE = "RDR" TARGET_NAME = "MARS" TARGET_TYPE = "PLANET" OBSERVATION_TYPE = "Global Gravity" INSTRUMENT_HOST_NAME = "MARS EXPRESS" INSTRUMENT_HOST_ID = "MEX" INSTRUMENT_NAME = "MARS EXPRESS ORBITER RADIO SCIENCE" INSTRUMENT_TYPE = "RADIO SCIENCE" INSTRUMENT_ID = "MRS" PRODUCER_ID = "RIU_COLOGNE" PRODUCER_FULL_NAME = "MARTIN PAETZOLD" PRODUCER_INSTITUTION_NAME= "RHEINISCHES INSTITUT FUER UMWELTFORSCHUNG, PLANETENFORSCHUNG" DSN_STATION_NUMBER = 32 PRODUCT_CREATION_TIME = 2008-08-13T14:08:55.000 SPACECRAFT_CLOCK_START_COUNT = "N/A" SPACECRAFT_CLOCK_STOP_COUNT = "N/A" 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 = "TWOD_X" INSTRUMENT_MODE_DESC = "TWO-WAY DUAL-FREQUENCY X-BAND U/L X&S-Band D/L" RECORD_TYPE = STREAM PRODUCT_ID = "M32ICL3L02_B2S_060280853_00.JPG" SOURCE_PRODUCT_ID = "M32ICL3L02_D2S_060280853_00.TAB" ^BROWSE_IMAGE = "M32ICL3L02_B2S_060280853_00.JPG" OBJECT = BROWSE_IMAGE ENCODING_TYPE = JPEG LINES = 3730 LINE_SAMPLES = 2294 SAMPLE_BITS = 24 SAMPLE_TYPE = UNSIGNED_INTEGER DESCRIPTION = "JPEG files contain several figures generated from level 2 Doppler data after processing and calibration. These may be useful in identifying data which deserve more detailed inspection. For example, by looking at the JPEG file, the user can determine whether a signal was easily detectable or whether the data were corrupted. Certain data anomalies can be readily seen in the plots. The panels are arranged in the following way and can be easily identified by the titel on top of it. First row: left: Auto Gain Control in dBm vs UTC time in (DOYs) right: Calibration in Hz vs UTC time in (DOYs) Second row: left: Complete Residual of observed and predicted Doppler shift [Hz] vs UTC time in (DOYs) right: Complete Differential Doppler [Hz] vs UTC time in (DOYs) (only available if both X- and S-Band was recorded) Third row and following: The complete residual (above) was subdivided into several plots. Every 3600 data points a new plot was generated in order to better identify smaller fluctuations which would otherwise not be seen in the complete plot. After the Residual plots: The complete differential Doppler (above) was subdivided into several plots. Every 3600 data points a new plot was generated in order to better identify smaller fluctuations which would otherwise not be seen in the complete plot. (only available if both X- and S-Band was recorded)." END_OBJECT = BROWSE_IMAGE END