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Jovian sodium plasmaThe nature of the sodium plasma created by ionization of the sodium emitted into the environment of Jupiter by Io is discussed. It is shown that the ions form a three-component plasma: cold, thermal, and energetic. Observational evidence for the effect of the plasma on the neutral sodium cloud is presented. The energetic component is predicted to generate ion cyclotron turbulence near the sodium gyrofrequency.
Document ID
19760050328
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Eviatar, A.
(Lunar Science Inst. Houston, TX, United States)
Mekler, Y.
(Tel Aviv University Tel Aviv, Israel)
Coroniti, F. V.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
April 15, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 205
Subject Category
Lunar And Planetary Exploration
Accession Number
76A33294
Funding Number(s)
CONTRACT_GRANT: NGL-05-007-190
Distribution Limits
Public
Copyright
Other

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