Exchange of water vapor between the atmosphere and surface of Mars.
A model for exchange of water from the atmosphere to condensing CO2 caps is developed. The rate of water condensation in the caps is assumed to be proportional to the meridional heat flux. It follows that the amount of water condensed in the caps varies inversely with the amount of CO2 condensed. Th...
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1973
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ftnasantrs:oai:casi.ntrs.nasa.gov:19730037468 2023-05-15T17:57:28+02:00 Exchange of water vapor between the atmosphere and surface of Mars. Leovy, C. B. Unclassified, Unlimited, Publicly available Jan 1, 1973 http://ntrs.nasa.gov/search.jsp?R=19730037468 unknown http://ntrs.nasa.gov/search.jsp?R=19730037468 Accession ID: 73A22270 Copyright Other Sources 30 Icarus; 18; Jan. 197 1973 ftnasantrs 2012-02-15T11:25:52Z A model for exchange of water from the atmosphere to condensing CO2 caps is developed. The rate of water condensation in the caps is assumed to be proportional to the meridional heat flux. It follows that the amount of water condensed in the caps varies inversely with the amount of CO2 condensed. The seasonal phase of the release of water from the caps is not consistent with observed variations in the abundance of atmospheric water. Seasonal variations of atmospheric water abundance are most consistent with vapor exchange between the atmosphere and permafrost in the subtropics. Other/Unknown Material permafrost NASA Technical Reports Server (NTRS) |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
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ftnasantrs |
language |
unknown |
topic |
30 |
spellingShingle |
30 Leovy, C. B. Exchange of water vapor between the atmosphere and surface of Mars. |
topic_facet |
30 |
description |
A model for exchange of water from the atmosphere to condensing CO2 caps is developed. The rate of water condensation in the caps is assumed to be proportional to the meridional heat flux. It follows that the amount of water condensed in the caps varies inversely with the amount of CO2 condensed. The seasonal phase of the release of water from the caps is not consistent with observed variations in the abundance of atmospheric water. Seasonal variations of atmospheric water abundance are most consistent with vapor exchange between the atmosphere and permafrost in the subtropics. |
format |
Other/Unknown Material |
author |
Leovy, C. B. |
author_facet |
Leovy, C. B. |
author_sort |
Leovy, C. B. |
title |
Exchange of water vapor between the atmosphere and surface of Mars. |
title_short |
Exchange of water vapor between the atmosphere and surface of Mars. |
title_full |
Exchange of water vapor between the atmosphere and surface of Mars. |
title_fullStr |
Exchange of water vapor between the atmosphere and surface of Mars. |
title_full_unstemmed |
Exchange of water vapor between the atmosphere and surface of Mars. |
title_sort |
exchange of water vapor between the atmosphere and surface of mars. |
publishDate |
1973 |
url |
http://ntrs.nasa.gov/search.jsp?R=19730037468 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
permafrost |
genre_facet |
permafrost |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19730037468 Accession ID: 73A22270 |
op_rights |
Copyright |
_version_ |
1766165913158025216 |