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• W1985104375 startingPage "5" @default.
• W1985104375 abstract "The plasma environments of the outer planets are a study in contrasts. The magnetosphere of Jupiter is dominated by the prodigious plasma output of Io, with losses due to diffusion driven by mass loading. At Saturn, the small icy satellites are the major sources of plasma for the inner magnetosphere. The low mass loading rates there imply that the densities of the plasma tori are limited by dissociative recombination, rather than diffusive transport. At Uranus, the icy satellites are negligible plasma sources compared to the input from the extended neutral hydrogen cloud and the ionosphere. Convection driven by the solar wind penetrates deep into the inner magnetosphere because of the unique orientation of the rotation axis of Uranus. The expected magnetosphere of Neptune is similar to that of Saturn and Jupiter, with Triton, the ring arcs, and the planet as possible plasma sources. The Voyager 2 encounter with Neptune holds out the hope of a passage through a non-terrestrial auroral region, a unique event in planetary exploration." @default.
• W1985104375 created "2016-06-24" @default.
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• W1985104375 creator A5015356657 @default.
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• W1985104375 date "1990-01-01" @default.
• W1985104375 modified "2023-09-26" @default.
• W1985104375 title "Thermal plasma in outer planet magnetospheres" @default.
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• W1985104375 doi "https://doi.org/10.1016/0273-1177(90)90081-a" @default.
• W1985104375 hasPublicationYear "1990" @default.
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