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Автор Delitsky, Mona L.
Автор Eviatar, Aharon
Автор Richardson, John D.
Дата выпуска 1989
dc.description We investigate the possibility of the formation of a plasma torus generated by the satellite Triton in the magnetosphere of Neptune. We solve a set of coupled differential equations that describe the evolution of material sputtered from the surface or atmosphere of Triton in the conditions likely to exist in an assumed Neptunian magnetosphere for various combinations of nitrogen and methane that may exist on Triton. The model assumes a mechanism for transport that gives upper limits for predicted torus concentrations. Our conclusion is that a successful detection of plasma by the Voyager Plasma Science instrument may be possible and could be an important source of information about the composition of Triton's surface and atmosphere.
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Копирайт Copyright 1989 by the American Geophysical Union.
Тема Magnetospheric Physics
Тема Magnetospheric Physics: Energetic particles, precipitating
Тема Magnetospheric Physics: Magnetosphere interactions with satellites and rings
Тема Magnetospheric Physics: Magnetospheric configuration and dynamics
Тема Magnetospheric Physics: Planetary magnetospheres
Тема Planetary Sciences: Fluid Planets
Тема Planetology: Fluid Planets: Interactions with particles and fields
Название A predicted Triton plasma torus in Neptune's magnetosphere
Тип article
DOI 10.1029/GL016i002p00215
Electronic ISSN 1944-8007
Print ISSN 0094-8276
Журнал Geophysical Research Letters
Том 16
Первая страница 215
Последняя страница 218
Аффилиация Delitsky, Mona L.; Jet Propulsion Laboratory‐California Institute of Technology
Аффилиация Eviatar, Aharon; Department of Atmospheric Science, University of California, Los Angeles
Аффилиация Richardson, John D.; Center for Space Research, Massachusetts Institute of Technology
Выпуск 2
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