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The clouds of VenusThe physical and chemical properties of the clouds of Venus are reviewed with special emphasis on data that are related to cloud dynamics. None of the currently popular interpretations of cloud phenomena on Venus is consistent with all the data. Either a considerable fraction of the observational evidence is faulty or has been misinterpreted, or the clouds of Venus are much more complex than the current simplistic models. Several lines of attack are suggested to resolve some of the contradictions.
Document ID
19750059050
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Young, A. T.
(Texas A & M University College Station, Tex., United States)
Date Acquired
August 8, 2013
Publication Date
June 1, 1975
Subject Category
Lunar And Planetary Exploration
Accession Number
75A43122
Funding Number(s)
CONTRACT_GRANT: NGR-44-001-117
Distribution Limits
Public
Copyright
Other

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