PDS_VERSION_ID                    = PDS3
LABEL_REVISION_NOTE               = "B.TRANTHAM  2019-02-25;
  20200120 RChen/EN not sure if ingest software would get the date"
RECORD_TYPE                       = STREAM

OBJECT                            = DATA_SET
 DATA_SET_ID                      = "
   RO-C-RPCIES-5-ESC2-V1.0"

 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 5 ESC2 V1.0"
  DATA_SET_COLLECTION_MEMBER_FLG  = "N"
  DATA_OBJECT_TYPE                = {TABLE, HEADER}
  START_TIME                      = 2015-03-11T00:02:45.505
  STOP_TIME                       = 2015-06-30T23:59:28.672
  DATA_SET_RELEASE_DATE           = 2018-09-13
  PRODUCER_FULL_NAME              = "BRAD TRANTHAM"
  DETAILED_CATALOG_FLAG           = "N"
  ABSTRACT_DESC = "
  This dataset contains DERIVED DATA of the Rosetta RPCIES
  instrument taken during the comet escort 2 phase (ESC2). The target of this phase
  was comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). Included are the
  data taken between 11 Mar 2015 and 30 Jun 2015."
  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 derived ion and electron
      moments.

      Rosetta Comet Escort 2 (ESC 2) covers the period from 2015-March-11 to
      2015-June-30. IES measured electrons generally below 500 eV. There are
      brief moments in which the electron detection is at all energies.
      IES electron detector observed ICA interference as a repetitive
      Morse code pattern.

      IES measured solar wind plasma continuously throughout this phase except
      for the occasional periods in which S/C pointing was not optimal.
      There are periods in this phase when we are unable to separate solar
      wind protons from the picked-up ions. During these intervals, no solar
      wind proton moments are reported. IES detected solar wind alpha
      particles during this phase. There are some intervals where proton
      moments are not reported, but alpha moments are reported. This is due
      to the fact that the alpha population is at higher energies than
      picked up ions, which are mixed with the proton population.
      Throughout this phase, there are intervals with strong cometary pick
      up activity and energization.

    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 derived data files are created
      from calibrated data files, please see DOCUMENT\MOMENTS_CALCULATION\
      MOMENTS_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."

  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.

    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 5 ESC2 V1.0,
    RO-C-RPCIES-5-ESC2-V1.0, ESA Planetary Science Archive and
    NASA Planetary Data System,  2019"
  DATA_SET_TERSE_DESC = "
  This dataset contains DERIVED DATA of the comet escort phase 2 (ESC2).
  Included are the data taken between 11 Mar 2015 and 30 Jun 2015."


 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