DATA_SET_ID                    = "GO-E-PWS-4-SUMM-E2SA60S-V1.0"

    DATA_SET_NAME                  = "
      GO E PWS RESAMP SUMMARY EARTH 2 SPECTRUM ANALYZER 60S V1.0"
    START_TIME                     = 1992-11-06T21:00:00.000Z
    STOP_TIME                      = 1992-12-17T06:21:00.000Z
    DATA_SET_RELEASE_DATE          = 1995-06-19
    PRODUCER_FULL_NAME             = "DR. WILLIAM S. KURTH"
    TARGET_NAME                    = EARTH
    INSTRUMENT_HOST_ID             = GO
    INSTRUMENT_ID                  = PWS

    DESCRIPTION:

    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 second flyby of Earth.  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.  During the time interval spanned by this data
    set, Galileo approached Earth from the local late evening sector, made a
    close approach to Earth by passing through the magnetosphere, plasmasphere,
    ionosphere, and finally exited the Earth system near local dawn."

                                 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."