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Isolation of major Venus thermospheric cooling mechanism and implications for earth and MarsThe additional cooling mechanism responsible for the unexpectedly cold dayside Venus thermosphere is isolated. Consideration is given not only to the condition that the calculated temperatures must be reduced to the observed dayside temperatures but also that the theoretical temperature variations must be in accord with the observed low amplitude of temperature variations associated with the 27-d variations of the sun. It is found that the low amplitude of the 27-d oscillations, combined with the cooling necessary for observed 300-K dayside temperatures, cannot be explained by eddy conduction cooling and can only be explained by very strong 15-micron cooling. Implications of the decrease in amplitude of the 11-yr Venus thermospheric variability due to the 15-micron thermostat effect are examined.
Document ID
19920050949
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Keating, Gerald M.
(NASA Langley Research Center Hampton, VA, United States)
Bougher, Stephen W.
(Arizona, University Tucson, United States)
Date Acquired
August 15, 2013
Publication Date
April 1, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: A4, A
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
92A33573
Distribution Limits
Public
Copyright
Other

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