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On the evolution of Saturn's 'Spokes' - TheoryStarting with the assumption that negatively charged micron-sized dust grains may be elevated above Saturn's ring plane by plasma interactions, the subsequent evolution of the system is discussed. The discharge of the fine dust by solar UV radiation produces a cloud of electrons which moves adiabatically in Saturn's dipolar magnetic field. The electron cloud is absorbed by the ring after one bounce, alters the local ring potential significantly, and reduces the local Debye length. As a result, more micron-sized dust particles may be elevated above the ring plane and the spoke grows. This process continues until the electron cloud has dissipated.
Document ID
19830046138
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Morfill, G. E.
(Max-Planck-Institut fuer extraterrestrische Physik Garching, Germany)
Gruen, E.
(Max-Planck Institut fuer Kernphysik Heidelberg, Germany)
Goertz, C. K.
(Max-Planck-Institut fuer Aeronomie Katlenburg, Germany)
Johnson, T. V.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Date Acquired
August 11, 2013
Publication Date
February 1, 1983
Publication Information
Publication: Icarus
Volume: 53
Subject Category
Lunar And Planetary Exploration
Accession Number
83A27356
Distribution Limits
Public
Copyright
Other

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