PDS_VERSION_ID                   = PDS3
LABEL_REVISION_NOTE              = "
             2012-06-06, D. Kazden, minor updates for version 3 standards;
             2020-02-05, D. Kazden, updated cITATION_DESC;"

OBJECT                       = DATA_SET
  DATA_SET_ID                    = "GO-A-PWS-4-SUMM-GSA60S-V1.0"

  OBJECT                         = DATA_SET_INFORMATION
    DATA_SET_NAME                  = "
      GO A PWS RESAMP SUMMARY GASPRA SPECTRUM ANALYZER 60S V1.0"
    DATA_SET_COLLECTION_MEMBER_FLG = N
    DATA_OBJECT_TYPE               = "TIME_SERIES"
    ARCHIVE_STATUS = ARCHIVED 
    START_TIME                     = 1991-10-29T06:39:00.000
    STOP_TIME                      = 1991-10-30T08:47:00.000
    DATA_SET_RELEASE_DATE          = 1995-06-19
    PRODUCER_FULL_NAME             = "DR. WILLIAM S. KURTH"
    DETAILED_CATALOG_FLAG          = "N"
    DATA_SET_TERSE_DESC            = " This data set includes 1-minute
    averages of the electric and magnetic wave spectra obtained during
    the period that the Galileo plasma wave receiver was operated during
    the flyby of Gaspra."
    ABSTRACT_DESC                  = " This data set includes 1-minute
    averages of the electric and magnetic wave spectra obtained during
    the period that the Galileo plasma wave receiver was operated during
    the electric field spectrum is the electric field spectral density in
    units of V^2/m^2/Hz. The magnetic field spectrum is provided in units
    of magnetic field spectral density, nT^2/Hz.  The spectral information
    is averaged and binned into 49 logarithmically-spaced channels from about
    6 Hz to 5.6 MHz for the electric measurements and 34 channels from about
    6 Hz to 75 kHz for the magnetic.  Note that these 'channels' do not
    generally correspond to the 158 specific channels described in the
    instrument description document. The reduction in spectral resolution for
    this data set was performed in order to make the set more conducive to use
    as a browse data set.   The sources of this browse data set are the High
    Frequency Receiver, Sweep Frequency Receiver, and Spectrum Analyzer which
    make up the Low Rate Science portion of the PWS."
    CITATION_DESC                  = "Kurth, W.S., GO-A-PWS-4-SUMM-GSA60S-V1.0,
                                     GO A PWS RESAMP SUMMARY GASPRA SPECTRUM
                                     ANALYZER 60S V1.0, NASA Planetary Data
                                     System, 1995."
    DATA_SET_DESC                  = "This data set includes 1-minute averages
    of the electric and magnetic wave spectra obtained during the period that
    the Galileo plasma wave receiver was operated during the flyby of Gaspra.
    The parameter provided for the electric field spectrum is the electric
    field spectral density in units of V^2/m^2/Hz. The magnetic field spectrum
    is provided in units of magnetic field spectral density, nT^2/Hz.  The
    spectral information is averaged and binned into 49 logarithmically-spaced
    channels from about 6 Hz to 5.6 MHz for the electric measurements and 34
    channels from about 6 Hz to 75 kHz for the magnetic.  Note that these
    'channels' do not generally correspond to the 158 specific channels
    described in the instrument description document. The reduction in
    spectral resolution for this data set was performed in order to make the
    set more conducive to use as a browse data set.   The sources of this
    browse data set are the High Frequency Receiver, Sweep Frequency
    Receiver, and Spectrum Analyzer which make up the Low Rate
    Science portion of the PWS."

    CONFIDENCE_LEVEL_NOTE          = "
    This data set includes all available Low Rate Science spectrum analyzer
    data within the interval of time covered. The data included in this set
    have been checked for accuracy by including only those words from the
    telemetry stream which did not have parity errors based on parity bits
    included with the data as part of the PWS data processing unit functions.
    The magnetic spectra contain narrowband interference lines at 2.4 kHz and
    harmonics.  Missing data are indicated by zero."

  END_OBJECT                     = DATA_SET_INFORMATION

  OBJECT                           = DATA_SET_MISSION
    MISSION_NAME                   = "GALILEO"
  END_OBJECT                       = DATA_SET_MISSION

  OBJECT                         = DATA_SET_TARGET
    TARGET_NAME                    = GASPRA
  END_OBJECT                     = DATA_SET_TARGET

  OBJECT                         = DATA_SET_HOST
    INSTRUMENT_HOST_ID             = GO
    INSTRUMENT_ID                  = PWS
  END_OBJECT                     = DATA_SET_HOST

  OBJECT                         = DATA_SET_REFERENCE_INFORMATION
    REFERENCE_KEY_ID               = "N/A"
  END_OBJECT                     = DATA_SET_REFERENCE_INFORMATION

END_OBJECT                     = DATA_SET
END