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The thermal balance of the atmosphere of Venus

Tomasko, M. G. and Boese, R. and Ingersoll, A. P. and Lacis, A. A. and Limaye, S. S. and Pollack, J. B. and Seiff, A. and Stewart, A. I. and Suomi, V. E. and Taylor, F. W. (1977) The thermal balance of the atmosphere of Venus. Space Science Reviews, 20 (4). pp. 389-412. ISSN 0038-6308. http://resolver.caltech.edu/CaltechAUTHORS:20130312-075926587

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Abstract

Current knowledge of the temperature structure of the atmosphere of Venus is briefly summarized. The principal features to be explained are the high surface temperature, the small horizontal temperature contrasts near the cloud tops in the presence of strong apparent motions, and the low value of the exospheric temperature. In order to understand the role of radiative and dynamical processes in maintaining the thermal balance of the atmosphere, a great deal of additional data on the global temperature structure, solar and thermal radiation fields, structure and optical properties of the clouds, and circulation of the atmosphere are needed. The ability of the Pioneer Venus Orbiter and Multiprobe Missions to provide these data is indicated.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/BF02186460DOIArticle
http://link.springer.com/article/10.1007%2FBF02186460PublisherArticle
ORCID:
AuthorORCID
Ingersoll, A. P.0000-0002-2035-9198
Additional Information:© 1977 by D. Reidel Publishing Company, Dordrecht-Holland.
Record Number:CaltechAUTHORS:20130312-075926587
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20130312-075926587
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:37453
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:12 Mar 2013 15:37
Last Modified:13 Feb 2019 18:05

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