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Ionospheres of the terrestrial planetsThe theory and observations relating to the ionospheres of the terrestrial planets Venus, the earth, and Mars are reviewed. Emphasis is placed on comparing the basic differences and similarities between the planetary ionospheres. The review covers the plasma and electric-magnetic field environments that surround the planets, the theory leading to the creation and transport of ionization in the ionospheres, the relevant observations, and the most recent model calculations. The theory section includes a discussion of ambipolar diffusion in a partially ionized plasma, diffusion in a fully ionized plasma, supersonic plasma flow, photochemistry, and heating and cooling processes. The sections on observations and model calculations cover the neutral atmosphere composition, the ion composition, the electron density, and the electron, ion, and neutral temperatures.
Document ID
19810031217
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schunk, R. W.
(Michigan, University Ann Arbor, Mich.; Utah State University of Agriculture and Applied Science, Logan, Utah, United States)
Nagy, A. F.
(Michigan, University Ann Arbor, Mich., United States)
Date Acquired
August 11, 2013
Publication Date
November 1, 1980
Publication Information
Publication: Reviews of Geophysics and Space Physics
Volume: 18
Subject Category
Lunar And Planetary Exploration
Accession Number
81A15621
Funding Number(s)
CONTRACT_GRANT: NSF ATM-78-10501
CONTRACT_GRANT: NSF ATM-78-21768
CONTRACT_GRANT: NGR-23-005-015
Distribution Limits
Public
Copyright
Other

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