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A model for the formation of spokes in Saturn's ringsEvidence is mounting which implies that the generation, evolution, and motion of spokes require a dense plasma near the Saturn ring plane. It is presently suggested that spokes consist of charged, micron-sized dust particles which are elevated from the rings by radially moving, dense plasma columns due to meteor impacts on the ring. Electrostatic wall sheaths at the ring, and ring charging by electric fields sufficiently strong to overcome the gravitational force on small dust particles, arise from the dense plasma, which also increases the probability of dust particle excess electronic charge. The radial motion of the plasma column is due to an azimuthal polarization electric field due to the relative motion between the corotating plasma and the negatively charged dust particles moving at Keplerian speeds.
Document ID
19830046137
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Goertz, C. K.
(Max-Planck-Institut fuer Aeronomie, Katlenburg, West Germany; Iowa, University Iowa City, IA, United States)
Morfill, G.
(Max-Planck-Institut fuer extraterrestrische Physik Garching, Germany)
Date Acquired
August 11, 2013
Publication Date
February 1, 1983
Subject Category
Lunar And Planetary Exploration
Accession Number
83A27355
Funding Number(s)
CONTRACT_GRANT: NSF ATM-76-82739
CONTRACT_GRANT: NAS2-6553
Distribution Limits
Public
Copyright
Other

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