PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "2006-08-31 GEO:shs Created; 2007-03-07 EN:bjs shortened dsname and created two dshost objects; 2009-05 GEO: added reference" RECORD_TYPE = STREAM OBJECT = DATA_SET DATA_SET_ID = "MER1/MER2-M-APXS-5-OXIDE-SCI-V1.0" OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "MER ALPHA PARTICLE X-RAY SPECTROMETER 5 OXIDE ABUNDANCE V1.0" DATA_SET_COLLECTION_MEMBER_FLG = N ARCHIVE_STATUS = "IN QUEUE" DATA_OBJECT_TYPE = SPREADSHEET START_TIME = 2004-01-04 STOP_TIME = NULL DATA_SET_RELEASE_DATE = 2006-08-31 PRODUCER_FULL_NAME = "RALF GELLERT" DETAILED_CATALOG_FLAG = Y DATA_SET_TERSE_DESC = "Mars Exploration Rover Alpha Particle X-ray Spectrometer Oxide Abundance Data" CITATION_DESC = "Gellert, Ralf, MER 1 Alpha Particle X-Ray Spectrometer 2 X-Ray Spectra V1.0, NASA Planetary Data System, MER1-M-APXS-2-XRAYSPEC-SCI-V1.0, 2004." ABSTRACT_DESC = "This archive contains oxide abundance data derived from the APXS Reduced Data Record (RDR) products on the Mars Exploration Rovers. The data consist of one file for each rover. When new APXS RDR data appear in a MER release, the oxide abundance data are revised in the following release approximately three months later. Hence the oxide data lag behind the EDR and RDR data by one release." DATA_SET_DESC = " Data Set Overview ================= This archive contains oxide abundance data derived from X-ray analyses of the MER APXS (Alpha Particle X-Ray Spectrometer) Reduced Data Record (RDR) products. A description of the data analysis procedure and interpretation of the results can be found in Gellert, R., et al. (2006), Alpha Particle X-Ray Spectrometer (APXS): Results from Gusev crater and calibration report, J. Geophys. Res., 111, E02S05, doi:10.1029/2005JE002555 [GELLERTETAL2006], and in Ming, D.W. et al. (2008), Results of the Alpha Particle X-Ray Spectrometer from Cumberland Ridge to Home Plate, J. Geophys. Res., 113, E12S39, doi:10.1029/2008JE003195 [MINGETAL2008]. Processing ========== The Committee On Data Management and Computation (CODMAC) data level numbering system is used to describe the processing level of the oxide abundance data product. The products are considered CODMAC Level 5, Derived Data equivalent to NASA level 3. The APXS oxide abundance data products were generated by the MER APXS Team. A nonlinear least squares algorithm was used to derive peak areas of characteristic element lines from APXS summed spectra. Peak areas were converted into element or oxide concentration using instrument calibration tables. Details of data processing and calibration are given in Gellert et al. 2006. The data were derived from APXS reduced data records (RDRs) from both rovers. Data ==== Each APXS oxide abundance data file is a table. Columns are variable length and are delimited with commas. Each row is terminated with a carriage return and line feed character. " CONFIDENCE_LEVEL_NOTE = "NULL" END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = MARS END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_MISSION MISSION_NAME = "MARS EXPLORATION ROVER" END_OBJECT = DATA_SET_MISSION OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = "MER1" INSTRUMENT_ID = "APXS" END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = "MER2" INSTRUMENT_ID = "APXS" END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "GELLERTETAL2006" END_OBJECT = DATA_SET_REFERENCE_INFORMATION OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "MINGETAL2008" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END