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PDS_VERSION_ID                 = PDS3                                         
LABEL_REVISION_NOTE            = "Initiated        JMAFI, 2004-03-01"         
                                                                              
OBJECT                         = INSTRUMENT                                   
  INSTRUMENT_HOST_ID           = P10                                          
  INSTRUMENT_ID                = UV                                           
                                                                              
  OBJECT                       = INSTRUMENT_INFORMATION                       
    INSTRUMENT_NAME            = "ULTRAVIOLET PHOTOMETER"                     
    INSTRUMENT_TYPE            = "ULTRAVIOLET SPECTROMETER"                   
    INSTRUMENT_DESC            = "                                            
                                                                              
  Instrument Overview                                                         
  ===================                                                         
    The ultraviolet photometer investigated the ultraviolet reflective        
    properties or emission from interplanetary hydrogen, helium and           
    dust, and from Jupiter's atmosphere and satellites. It was hoped to       
    provide data to resolve the origin of interplanetary neutral              
    hydrogen and establish the boundaries of the heliosphere. From            
    measurements of the interplanetary helium, experimenters hoped to         
    determine the percentage of this gas in the interstellar medium.          
                                                                              
    The ultraviolet photometer had a fixed viewing angle and uses the         
    spin of the spacecraft to scan around the celestial sphere. When          
    close to Jupiter, the photometer scaned the medium above the cloud        
    tops. By measuring the changes in the intensity of ultraviolet light      
    reflected into two photocathodes of the instrument -- one measuring       
    radiation at 1216 Angstroms, the other at 584 Angstroms -- the            
    photometer detected light from hydrogen and helium respectively.          
                                                                              
    Within the Jovian system the photometer measured the scattering of        
    solar ultraviolet light by the atmosphere of Jupiter. This                
    scattering provided information on the amount of atomic hydrogen in       
    Jupiter's upper atmosphere, the mixing rate of Jupiter's atmosphere,      
    the amount of helium there, and therefore the ratio of helium to          
    hydrogen at Jupiter. Prior to Pioneer 10's mission helium had not         
    been identified at the planet.                                            
                                                                              
    By measuring changes in the ultraviolet light glow the instrument         
    checked to see if Jupiter has polar auroras.                              
                                                                              
  ['Instrument Overview' was adapted from FIMMELETAL pp. 56-57.]"             
                                                                              
  END_OBJECT                   = INSTRUMENT_INFORMATION                       
                                                                              
  OBJECT                       = INSTRUMENT_REFERENCE_INFO                    
    REFERENCE_KEY_ID           = "FIMMELETAL1977"                             
  END_OBJECT                   = INSTRUMENT_REFERENCE_INFO                    
                                                                              
  OBJECT                       = INSTRUMENT_REFERENCE_INFO                    
    REFERENCE_KEY_ID           = "JUDGEETAL1976"                              
  END_OBJECT                   = INSTRUMENT_REFERENCE_INFO                    
                                                                              
END_OBJECT                     = INSTRUMENT                                   
END