A Martian global groundwater model
A global groundwater flow model was constructed for Mars to study hydrologic response under a variety of scenarios, improving and extending earlier simple cross sectional models. The model is capable of treating both steady state and transient flow as well as permeability that is anisotropic in the...
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ftnasantrs:oai:casi.ntrs.nasa.gov:19920001551 2023-05-15T17:57:35+02:00 A Martian global groundwater model Howard, Alan D. Unclassified, Unlimited, Publicly available Jun 1, 1991 application/pdf http://hdl.handle.net/2060/19920001551 unknown Document ID: 19920001551 Accession ID: 92N10769 http://hdl.handle.net/2060/19920001551 No Copyright CASI LUNAR AND PLANETARY EXPLORATION NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990; p 114-116 1991 ftnasantrs 2015-03-15T05:02:13Z A global groundwater flow model was constructed for Mars to study hydrologic response under a variety of scenarios, improving and extending earlier simple cross sectional models. The model is capable of treating both steady state and transient flow as well as permeability that is anisotropic in the horizontal dimensions. A single near surface confining layer may be included (representing in these simulations a coherent permafrost layer). Furthermore, in unconfined flow, locations of complete saturation and seepage are determined. The flow model assumes that groundwater gradients are sufficiently low that DuPuit conditions are satisfied and the flow component perpendicular to the ground surface is negligible. The flow equations were solved using a finite difference method employing 10 deg spacing of latitude and longitude. 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 |
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unknown |
topic |
LUNAR AND PLANETARY EXPLORATION |
spellingShingle |
LUNAR AND PLANETARY EXPLORATION Howard, Alan D. A Martian global groundwater model |
topic_facet |
LUNAR AND PLANETARY EXPLORATION |
description |
A global groundwater flow model was constructed for Mars to study hydrologic response under a variety of scenarios, improving and extending earlier simple cross sectional models. The model is capable of treating both steady state and transient flow as well as permeability that is anisotropic in the horizontal dimensions. A single near surface confining layer may be included (representing in these simulations a coherent permafrost layer). Furthermore, in unconfined flow, locations of complete saturation and seepage are determined. The flow model assumes that groundwater gradients are sufficiently low that DuPuit conditions are satisfied and the flow component perpendicular to the ground surface is negligible. The flow equations were solved using a finite difference method employing 10 deg spacing of latitude and longitude. |
format |
Other/Unknown Material |
author |
Howard, Alan D. |
author_facet |
Howard, Alan D. |
author_sort |
Howard, Alan D. |
title |
A Martian global groundwater model |
title_short |
A Martian global groundwater model |
title_full |
A Martian global groundwater model |
title_fullStr |
A Martian global groundwater model |
title_full_unstemmed |
A Martian global groundwater model |
title_sort |
martian global groundwater model |
publishDate |
1991 |
url |
http://hdl.handle.net/2060/19920001551 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
permafrost |
genre_facet |
permafrost |
op_source |
CASI |
op_relation |
Document ID: 19920001551 Accession ID: 92N10769 http://hdl.handle.net/2060/19920001551 |
op_rights |
No Copyright |
_version_ |
1766166044821422080 |