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    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1983
    In:  Journal of Geophysical Research: Space Physics Vol. 88, No. A7 ( 1983-07), p. 5573-5579
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 88, No. A7 ( 1983-07), p. 5573-5579
    Abstract: Saturn's broad E ring, the narrow G ring, and the structured and apparently time‐variable F ring(s) contain many micron and submicron‐sized particles, which make up the ‘visible’ component. These rings (or ring systems) are in direct contact with magnetospheric plasma. Fluctuations in the plasma density and/or mean energy, due to magnetospheric and solar wind processes, may induce stochastic charge variations on the dust particles, which in turn lead to an orbit perturbation and spatial diffusion. In addition, Coulomb drag forces may be important, in particular for the E ring. The possibility that electromagnetic effects may play a role in determining the F ring structure, and its possible time variations, is critically examined. Sputtering of micron‐sized dust particles in the E ring by magnetospheric ions yields lifetimes of 10² to 10 4 years. This effect as well as the plasma induced transport processes require an active source for the E ring, probably Enceladus.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1983
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