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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ftnasantrs:oai:casi.ntrs.nasa.gov:19900062894 2023-05-15T15:52:38+02:00 Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation Lewis, John S. Grinspoon, David H. Unclassified, Unlimited, Publicly available Sep 14, 1990 http://ntrs.nasa.gov/search.jsp?R=19900062894 unknown http://ntrs.nasa.gov/search.jsp?R=19900062894 Accession ID: 90A49949 Copyright Other Sources 91 Science; 249; 1273-127 1990 ftnasantrs 2012-02-15T18:35:22Z 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 water abundances that are discrepant by a factor of 2.5 to 10). These data sets can be reconciled if (1) water molecules associate with carbon dioxide and sulfur trioxide to make gaseous carbonic acid and sulfuric acid in the lower atmosphere, and (2) the discrepant 0.94-micrometer water measurements are due to gaseous sulfuric acid, requiring it to be a somewhat stronger absorber than water vapor in this wavelength region. A mean total water abundance of 50 + or - 20 parts/million and a near-surface free water vapor abundance of 10 + or - 4 parts/million are derived. Other/Unknown Material Carbonic acid NASA Technical Reports Server (NTRS) Venus ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
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NASA Technical Reports Server (NTRS) |
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ftnasantrs |
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91 |
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91 Lewis, John S. Grinspoon, David H. Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation |
topic_facet |
91 |
description |
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 water abundances that are discrepant by a factor of 2.5 to 10). These data sets can be reconciled if (1) water molecules associate with carbon dioxide and sulfur trioxide to make gaseous carbonic acid and sulfuric acid in the lower atmosphere, and (2) the discrepant 0.94-micrometer water measurements are due to gaseous sulfuric acid, requiring it to be a somewhat stronger absorber than water vapor in this wavelength region. A mean total water abundance of 50 + or - 20 parts/million and a near-surface free water vapor abundance of 10 + or - 4 parts/million are derived. |
format |
Other/Unknown Material |
author |
Lewis, John S. Grinspoon, David H. |
author_facet |
Lewis, John S. Grinspoon, David H. |
author_sort |
Lewis, John S. |
title |
Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation |
title_short |
Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation |
title_full |
Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation |
title_fullStr |
Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation |
title_full_unstemmed |
Vertical distribution of water in the atmosphere of Venus - A simple thermochemical explanation |
title_sort |
vertical distribution of water in the atmosphere of venus - a simple thermochemical explanation |
publishDate |
1990 |
url |
http://ntrs.nasa.gov/search.jsp?R=19900062894 |
op_coverage |
Unclassified, Unlimited, Publicly available |
long_lat |
ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
geographic |
Venus |
geographic_facet |
Venus |
genre |
Carbonic acid |
genre_facet |
Carbonic acid |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19900062894 Accession ID: 90A49949 |
op_rights |
Copyright |
_version_ |
1766387761286217728 |