Computer Science
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..243w&link_type=abstract
Advances in Space Research, vol. 20, p. 243
Computer Science
6
Jupiter Atmosphere, Planetary Ionospheres, Emission Spectra, Saturn Atmosphere, Neptune Atmosphere, Particle Precipitation, Planetary Magnetospheres, Auroral Spectroscopy, Heavy Ions, Galileo Probe, Voyager 1 Spacecraft
Scientific paper
Analyses of Jovian IR, UV, and X-ray wavelength auroral emissions bear on the nature of the magnetosphere-ionosphere interaction, and have indicated heavy-ion precipitations into the Jupiter equatorial region. The ionospheric structure indicated by Voyager 1 radio science data is reproduced by a model of the low-latitude ionosphere that incorporates ion precipitation effects. Additional current models encompass Jovian atmospheric hydrocarbon atoms, a 1D time-dependent model of the Saturn ionosphere, and a photochemical model of the upper atmosphere of Neptune.
Connerney Jack E. P.
Cravens Thomas E.
Drossart Pierre
Gladstone Randall G.
Lam Hoanh An
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