CCSD3ZF0000100000001NJPL3IF0PDSX00000001
PDS_VERSION_ID                     = PDS3

RECORD_TYPE                        = STREAM
OBJECT                             = INSTRUMENT
  INSTRUMENT_HOST_ID               = ULY
  INSTRUMENT_ID                    = SCE
  OBJECT                           = INSTRUMENT_INFORMATION
    INSTRUMENT_NAME                = "SOLAR CORONA EXPERIMENT"
    INSTRUMENT_TYPE                = "RADIO SCIENCE"
    INSTRUMENT_DESC                = "

      Instrument Overview
      ===================

      (excerpted from [BIRDETAL1992A])

      Abstract. -- The main science objective of the Ulysses Solar
      Corona Experiment is to derive the plasma parameters of the
      solar atmosphere using established coronal-sounding
      techniques. Applying appropriate model assumptions, the 3-D
      electron density distribution will be determined from
      dual-frequency ranging and Doppler measurements recorded at
      the NASA Deep Space Network during the solar conjunctions.
      Multi-station observations will be used to derive the plasma
      bulk velocity at solar distances where the solar wind is
      expected to undergo its greatest acceleration. As a secondary
      objective profiting from the favorable geometry during Jupiter
      encounter, radio-sounding measurements will yield a unique
      cross-scan of the electron density in the Io Plasma Torus."

  END_OBJECT                       = INSTRUMENT_INFORMATION

  OBJECT                           = INSTRUMENT_REFERENCE_INFO
    REFERENCE_KEY_ID               = "BIRDETAL1992A"
  END_OBJECT                       = INSTRUMENT_REFERENCE_INFO

END_OBJECT                         = INSTRUMENT
END