PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "2016-02-04, SONC, initial release" RECORD_TYPE = STREAM OBJECT = DATA_SET DATA_SET_ID = "RL-C-PTOLEMY-5-FSS-V1.0" OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "ROSETTA-LANDER 67P PTOLEMY 5 FSS V1.0" DATA_SET_TERSE_DESC = "This data set contains the data referred to FSS Mission Phase" DATA_SET_COLLECTION_MEMBER_FLG = "N" DATA_OBJECT_TYPE = TABLE START_TIME = 2014-11-12T15:54:00.000 STOP_TIME = 2014-11-14T23:18:50.596 DATA_SET_RELEASE_DATE = 2016-02-04 PRODUCER_FULL_NAME = "SCIENCE OPERATIONS AND NAVIGATION CENTER" DETAILED_CATALOG_FLAG = "N" ABSTRACT_DESC = "This archive contains derived data from the PTOLEMY instrument onboard ROSETTA Lander, acquired during the FSS mission phase. The primary target is the comet 67P/CHURYUMOV-GERASIMENKO. It also contains documentation which describes the PTOLEMY experiment. The data archived in this data set conform to the Planetary Data System (PDS) Standards, Version 3.6." ARCHIVE_STATUS = "IN QUEUE" CITATION_DESC = "I. Wright, S. Barber, A. Morse, D. Andrews, ROSETTA-LANDER 67P PTOLEMY 5 FSS V1.0, RL-C-PTOLEMY-5-FSS-V1.0, ESA Planetary Science Archive and NASA Planetary Data System, 2017." CONFIDENCE_LEVEL_NOTE = "Data confidence is nominal, meaning that all data have been validated by the scientific team and found as expected. Any exceptions are noted by the DATA_QUALITY_ID. Moreover the data set underwent a successful external review" DATA_SET_DESC = " Data Set Overview ================= This data set contains derived data combining calibrated mass spectra referred to FSS Mission Phase. Data ==== Both data, scientific and housekeeping, are collected in this data set. They referred to CODMAC Level 5. The level 5 data product contains ion counts for mass spectra at each observation site and ion counts for each of the main compounds obtained from Ptolemy sniff operations made during the Philae first-science sequence. Processing ========== Only CODMAC Level 5 data are present in this data set. Mass spectra with the same mass range (using the same scan function) are summed to produce a single mass spectrum with calibrated mass range. In addition integer masses are assigned for the channel closest to the integer mass. Ion counts were determined for each mass by using a rolling sum (n = 11 for WGA 3, n = 7 for WGA 4) of the ion counts centered on the assigned mass (using the data set above). A single combined spectrum was produced for each observation by summing WGA3 and WGA4, with values extrapolated for the missing ranges using the ratio of total ion counts in the overlapping range. Coordinate System ================= The geometry items SC_SUN_POSITION_VECTOR, SC_TARGET_POSITION_VECTOR and SC_TARGET_VELOCITY_VECTOR provided in the label of the data product are relative to the Earth Mean Equator and Equinox reference frame of J2000. SUB_SPACECRAFT_LATITUDE, SUB_SPACECRAFT_LONGITUDE are given in the PLANETOCENTRIC coordinate system. These parameters are computed at time t=START_TIME. Distances are given in km, angles in degrees. " END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = "67P/CHURYUMOV-GERASIMENKO 1 (1969 R1)" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_MISSION MISSION_NAME = "INTERNATIONAL ROSETTA MISSION" END_OBJECT = DATA_SET_MISSION OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = "RL" INSTRUMENT_ID = "PTOLEMY" END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "WRIGHTETAL2007" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END