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Saturn ionosphere - Theoretical interpretationVoyager 1 high latitude and Pioneer 11 equatorial ionospheric structure indicate a solar EUV-controlled ionosphere with a possible molecular ion in the topside. Vibrationally excited H2 in the high latitudes may be an important loss mechanism. Dynamical effects are expected to be important for determining the peak density and its location.
Document ID
19810060800
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Atreya, S. K.
(Michigan, University Ann Arbor, MI, United States)
Waite, J. H., Jr.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 11, 2013
Publication Date
August 20, 1981
Publication Information
Publication: Nature
Volume: 292
Subject Category
Lunar And Planetary Exploration
Accession Number
81A45204
Distribution Limits
Public
Copyright
Other

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