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Ionospheric Models of Saturn, Uranus, and Neptune

TCARUS 24, 358--:~62 (1975) Ionospheric Models of saturn , uranus , and Neptune S. K. ATREYA t AND T. M. DONAHUE ~ Department of Physics, University of Pittsburgh, Pittsburgh, Pennsylvania 15260 Received September 6, 1974; revised November 4, 1974 model ionospheres are calculated for saturn , uranus , and Neptune . Protons are the maj or ions above 150 km altitude measured from a reference levelwhere the hydrogen density is 1 1016 molecules cm-a, while below 150 km quick conversion of protons to Ha + ions by a three-body association mechanism leads to a rapid removal of ionization in dissociative recombination of Ha +. Electron density maxima are found at about 260 km for saturn and uranus and 200 km for Neptune .

IONOSPHERIC MODELS OF SATURN, URANUS AND NEPTUNE TABLE I IMPORTANT REACTIONS I1,,1 THE IOI~OSPHERE OF THE OUTER PLANETS a 359 Reaction number Reaction Rate constant Reference

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