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Автор Cheng, Andrew F.
Автор Waite, J. H.
Дата выпуска 1988
dc.description Eviatar and Richardson [1986] calculated the Pedersen conductance of Saturn's ionosphere and obtained values far smaller than previous estimates. They concluded that the low Pedersen conductance explained the corotation lag in the magnetosphere. We recalculated the Pedersen conductance and confirmed the original estimates. The magnetosphere should corotate with the ionosphere. We suggest that the eddy diffusion coefficient in Saturn's upper atmosphere may be small enough to allow the ionosphere to be significantly despun relative to the interior.
Формат application.pdf
Копирайт Copyright 1988 by the American Geophysical Union.
Тема IONOSPHERE
Тема Planetary ionospheres
Тема Ionosphere/magnetosphere interactions
Тема MAGNETOSPHERIC PHYSICS
Тема Magnetosphere/ionosphere interactions
Тема Magnetospheric configuration and dynamics
Тема Planetary magnetospheres
Тема PLANETARY SCIENCES: SOLID SURFACE PLANETS
Тема Ionospheres
Тема Magnetospheres
Тема PLANETARY SCIENCES: FLUID PLANETS
Тема Ionospheres
Тема Magnetospheres
Тема PLANETARY SCIENCES: COMETS AND SMALL BODIES
Тема Ionospheres
Тема Magnetospheres
Название Corotation lag of Saturn's magnetosphere: Global ionospheric conductivities revisited
Тип shortCommunication
DOI 10.1029/JA093iA05p04107
Electronic ISSN 2156-2202
Print ISSN 0148-0227
Журнал Journal of Geophysical Research: Space Physics
Том 93
Первая страница 4107
Последняя страница 4109
Выпуск A5
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