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PDS_VERSION_ID                     = PDS3                                    
LABEL_REVISION_NOTE                = "J. MAFI (PPI), 1998-05-18"             
RECORD_TYPE                        = STREAM                                  
                                                                             
OBJECT                             = INSTRUMENT                              
  INSTRUMENT_HOST_ID               = ULY                                     
  INSTRUMENT_ID                    = SWICS                                   
                                                                             
  OBJECT                           = INSTRUMENT_INFORMATION                  
    INSTRUMENT_NAME              = "SOLAR WIND ION COMPOSITION SPECTROMETER" 
    INSTRUMENT_TYPE                = "ENERGETIC PARTICLE DETECTOR"           
    INSTRUMENT_DESC                = "                                       
                                                                             
  Instrument Overview                                                        
  ===================                                                        
    (excerpted from [GLOECKLERETAL1992])                                     
                                                                             
    Abstract.  -- The Solar Wind Ion Composition Spectrometer                
    (SWICS) on Ulysses is designed to determine uniquely the                 
    elemental and ionic-charge composition, and the temperatures             
    and mean speeds of all major solar-wind ions, from H through             
    Fe, at solar wind speeds ranging from 175 km/s (protons) to              
    1280 km/s (Fe^8+).  The instrument, which covers an energy per           
    charge range from 0.16 to 59.6 keV/e in ~ 13 min, combines an            
    electrostatic analyzer with post-acceleration, followed by a             
    time-of-flight and energy measurement.  The measurements made            
    by SWICS will have an impact on many areas of solar and                  
    heliospheric physics, in particular providing essential and              
    unique information on: (i) conditions and processes in the               
    region of the corona where the solar wind is accelerated, (ii)           
    the location of the source regions of the solar wind in the              
    corona; (iii) coronal heating processes; (iv) the extent and             
    causes of variations in the composition of the solar                     
    atmosphere; (v)plasma processes in the solar wind; (vi) the              
    acceleration of energetic particles in the solar wind; (vii)             
    the thermalization and acceleration of interstellar ions in the          
    solar wind, and their composition; and (viii) the composition,           
    charge states and behavior of the plasma in various regions of           
    the Jovian magnetosphere."                                               
  END_OBJECT                       = INSTRUMENT_INFORMATION                  
                                                                             
  OBJECT                           = INSTRUMENT_REFERENCE_INFO               
    REFERENCE_KEY_ID               = "GLOECKLERETAL1992"                     
  END_OBJECT                       = INSTRUMENT_REFERENCE_INFO               
                                                                             
END_OBJECT                         = INSTRUMENT                              
END