Theoretical researches into planetary atmospheres and their influence upon surface features

The interface between certain geological and atmospheric phenomena on Mars was studied by examining those geological features which are associated with the presence of water in the liquid or solid phases. Several classes of Martian surface features thought to have had their origins in flow processes...

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Bibliographic Details
Main Author: Goody, R.
Format: Other/Unknown Material
Language:unknown
Published: 1974
Subjects:
SPACE SCIENCES
Ice Shelves
Online Access:http://hdl.handle.net/2060/19740027141
id ftnasantrs:oai:casi.ntrs.nasa.gov:19740027141
record_format openpolar
spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19740027141 2023-05-15T16:41:58+02:00 Theoretical researches into planetary atmospheres and their influence upon surface features Goody, R. Unclassified, Unlimited, Publicly available Oct 1, 1974 application/pdf http://hdl.handle.net/2060/19740027141 unknown Document ID: 19740027141 Accession ID: 74N35254 http://hdl.handle.net/2060/19740027141 No Copyright CASI SPACE SCIENCES NASA-CR-140188 1974 ftnasantrs 2019-07-21T05:29:58Z The interface between certain geological and atmospheric phenomena on Mars was studied by examining those geological features which are associated with the presence of water in the liquid or solid phases. Several classes of Martian surface features thought to have had their origins in flow processes were studied in order to determine the role ice may have played in their creations. Preliminary studies concerning the behavior of Martian ice shelves were conducted, with the conclusion that flow rates of Martian and earth ice sheets are similar. Withdrawal of subsurface ice was found to be among the explanations for the origins of the chaotic terrains and drifted blocks. Other/Unknown Material Ice Shelves NASA Technical Reports Server (NTRS)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic SPACE SCIENCES
spellingShingle SPACE SCIENCES
Goody, R.
Theoretical researches into planetary atmospheres and their influence upon surface features
topic_facet SPACE SCIENCES
description The interface between certain geological and atmospheric phenomena on Mars was studied by examining those geological features which are associated with the presence of water in the liquid or solid phases. Several classes of Martian surface features thought to have had their origins in flow processes were studied in order to determine the role ice may have played in their creations. Preliminary studies concerning the behavior of Martian ice shelves were conducted, with the conclusion that flow rates of Martian and earth ice sheets are similar. Withdrawal of subsurface ice was found to be among the explanations for the origins of the chaotic terrains and drifted blocks.
format Other/Unknown Material
author Goody, R.
author_facet Goody, R.
author_sort Goody, R.
title Theoretical researches into planetary atmospheres and their influence upon surface features
title_short Theoretical researches into planetary atmospheres and their influence upon surface features
title_full Theoretical researches into planetary atmospheres and their influence upon surface features
title_fullStr Theoretical researches into planetary atmospheres and their influence upon surface features
title_full_unstemmed Theoretical researches into planetary atmospheres and their influence upon surface features
title_sort theoretical researches into planetary atmospheres and their influence upon surface features
publishDate 1974
url http://hdl.handle.net/2060/19740027141
op_coverage Unclassified, Unlimited, Publicly available
genre Ice Shelves
genre_facet Ice Shelves
op_source CASI
op_relation Document ID: 19740027141
Accession ID: 74N35254
http://hdl.handle.net/2060/19740027141
op_rights No Copyright
_version_ 1766032439282499584

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