PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "B.TRANTHAM 2017-05-11 B.TRANTHAM 2018-11-01, updated DATA_SET_DESC based on review comments, B.TRANTHAM 2019-03-28, updated dataset based on review comments; 20200120 RChen/EN not sure if ingest software would get the date" RECORD_TYPE = STREAM OBJECT = DATA_SET DATA_SET_ID = " RO-C-RPCIES-3-EXT3-V2.0" OBJECT = DATA_SET_MISSION MISSION_NAME = "INTERNATIONAL ROSETTA MISSION" END_OBJECT = DATA_SET_MISSION OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = BURCHETAL2007 END_OBJECT = DATA_SET_REFERENCE_INFORMATION OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = " ROSETTA-ORBITER 67P RPCIES 3 EXT3 V2.0" DATA_SET_COLLECTION_MEMBER_FLG = "N" DATA_OBJECT_TYPE = {TABLE, HEADER} START_TIME = 2016-07-01T00:02:57.965 STOP_TIME = 2016-09-30T10:34:28.545 DATA_SET_RELEASE_DATE = 2017-03-20 PRODUCER_FULL_NAME = "BRAD TRANTHAM" DETAILED_CATALOG_FLAG = "N" ABSTRACT_DESC = " This dataset contains CALIBRATED DATA of the Rosetta RPCIES instrument taken during the extended mission 3 phase (EXT3). The target of this phase was comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). Included are the data taken between 01 Jul 2016 and 30 Sep 2016. This version of the data has been reprocessed to remove an error introduced in the previous version." DATA_SET_DESC = " Data Set Overview ================= The following describes the nature of instrument operation during the various periods for which IES data are available in this submission. In all cases the data are calibrated differential electron and ion energy flux as function of energy, azimuth (direction in the instrument symmetry plane) and elevation (angle above or below the symmetry plane). During this phase Rosetta traversed distances between approximately 0 (at impact) to 26 km to the comet, performing terminator and other trajectories. IES observed solar wind ions and electrons as well as the low energy (~20 eV) ions attracted to the S/C when it was at a negative potential. Very few other cometary ions were observed. Nor could cometary electrons be distinguished from solar wind electrons. IES operated continuously during this period. Processing ========== All Rosetta Plasma Consortium (RPC) data packets are transmitted together during downlinks with Rosetta. RPC data are retrieved from the Data Distribution System (DDS) at European Space Operations Centre (ESOC) to a central RPC data server at Imperial College London. Data for IES is copied from the RPC central data server by IESGS at Southwest Research Institute. The pipeline processing software is the IES Ground System (IESGS). IESGS extracts IES CCSDS packets from the RPC collective data files stored on the RPC central data server at Imperial College. These packets are used to build ion and electron data products. The data products are grouped by date and written out to PDS compliant archive data files. One data file is created for each day. IESGS also generates the labels for the archive data files. IES science products, archive and label files, and limited spectrograms are available to team scientists on the IESGS website. For information on how the calibrated data files are created from edited data files, please see DOCUMENT\FLUX_CALCULATION\ FLUX_CALCULATION.PDF. Coordinate System ================= In order to determine IES pointing, attitude data for the Rosetta spacecraft is obtained through SPICE kernels. Level 5 files use Comet-centered Solar EQuatorial (CSEQ) as the reference frame to specify the velocity direction components. This is a common frame used in many other data sets and is referenced as '67P/C-G_CSEQ' in SPICE. SUB_SPACECRAFT_LATITUDE, SUB_SPACECRAFT_LONGITUDE are given in the Cheops reference frame. These parameters are computed at time t=START_TIME. Distances are given in km, angles in degrees. Version History ================= Version 1 - Initial release Version 2 - Reprocessed to remove an error in the data" CONFIDENCE_LEVEL_NOTE = " Confidence Level Overview ========================= This dataset is used by the IES science team after processing. This is done to ensure that the archived data contains good, valid products. Caveat about using IES Level 3 Differential Energy Flux data: The background subtraction technique used in the production of the Level 3 Differential Energy Flux data does not work well for certain modes and as a result, the flux values may be slightly different from nominal. Please contact the IES team before using the data. Once the background subtraction issue is resolved, the IES team will deliver updated data. Review ====== This archival data set was examined by the IES science team prior to submission to the NASA Planetary Data System (PDS) and ESA Plantetary Science Archive (PSA). It was reviewed by PDS, PSA, and the Rosetta data archive working group. Limitations =========== None." ARCHIVE_STATUS = "LOCALLY ARCHIVED" CITATION_DESC = " Trantham, B., ROSETTA-ORBITER 67P RPCIES 3 EXT3 V2.0, RO-C-RPCIES-3-EXT3-V2.0, ESA Planetary Science Archive and NASA Planetary Data System, 2019" DATA_SET_TERSE_DESC = " This dataset contains CALIBRATED DATA of the extended mission phase 3 (EXT3). Included are the data taken between 01 Jul 2016 and 30 Sep 2016." 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_HOST INSTRUMENT_HOST_ID = RO INSTRUMENT_ID = "RPCIES" END_OBJECT = DATA_SET_HOST END_OBJECT = DATA_SET END