Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation
Several lines of evidence concerning the vertical abundance profile of water in the atmosphere of Venus lead to strikingly unusual distributions (the water vapor abundance decreases sharply in the immediate vicinity of the surface) or to serious conflicts in the profiles (different IR bands suggest...
Main Authors: | , |
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Format: | Other/Unknown Material |
Language: | unknown |
Published: |
1990
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Online Access: | http://ntrs.nasa.gov/search.jsp?R=19900062894 |