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Models of planetary ringsThe Voyager occultations provide several uniform and high quality data sets for Saturn, Uranus, and Neptune. These data are intercompared, and theoretical models for the particle sizes and the particle transport are developed. The major topics covered include: ring size distribution, torques and resonances, and satellite wakes.
Document ID
19920001716
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Esposito, L. W. (Colorado Univ. Boulder., United States)
Brophy, T. G. (Colorado Univ. Boulder., United States)
Stewart, Glen R. (Colorado Univ. Boulder., United States)
Yanamandra-Fisher, P. A. (Jet Propulsion Lab. California Inst. of Tech., Pasadena., United States)
Date Acquired
September 6, 2013
Publication Date
June 1, 1991
Publication Information
Publication: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990
Subject Category
Lunar And Planetary Exploration
Accession Number
92N10934
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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