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Photochemistry of planetary ionospheresThe dominant photochemical reactions taking place in the ionospheres of Venus, Saturn, and Comet P/Halley are presented. It is shown that the differences in the ionospheres of these celestial bodies result from the different chemistry, energetics, and dynamics of the respective atmospheres. The role of photochemistry in the formation of the individual ionospheres is discussed.
Document ID
19880041959
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(87)90205-5
Authors
Nagy, Andrew F. (Michigan, University Ann Arbor, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1987
Publication Information
Publication: Advances in Space Research
Volume: 7
Issue: 12 1
ISSN: 0273-1177
Subject Category
Lunar And Planetary Exploration
Accession Number
88A29186
Funding Number(s)
CONTRACT_GRANT: NGR-23-005-015
CONTRACT_GRANT: NAS2-12315
Distribution Limits
Public
Copyright
Other

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