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...

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Bibliographic Details
Main Authors: Lewis, John S., Grinspoon, David H.
Format: Other/Unknown Material
Language:unknown
Published: 1990
Subjects:
91
Online Access:http://ntrs.nasa.gov/search.jsp?R=19900062894