ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO

Introduction: Deposits on the flanks of the large Tharsis Montes volcanoes have been recognized to be of glacial origin [1,2,3]. These Amazonian-aged deposits display three distinct facies, ridged, knobby, and smooth [4], each of which can be associated with different glacial processes [1]. We use t...

Full description

Bibliographic Details
Main Authors: Tharsis Montes, Tropical Mountain, Glaciation J. L. Fastook, D. E. Shean, J. W. Head
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.174.6157
http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf
id ftciteseerx:oai:CiteSeerX.psu:10.1.1.174.6157
record_format openpolar
spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.174.6157 2023-05-15T16:40:20+02:00 ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO Tharsis Montes Tropical Mountain Glaciation J. L. Fastook D. E. Shean J. W. Head The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.174.6157 http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.174.6157 http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf text ftciteseerx 2016-01-07T16:10:26Z Introduction: Deposits on the flanks of the large Tharsis Montes volcanoes have been recognized to be of glacial origin [1,2,3]. These Amazonian-aged deposits display three distinct facies, ridged, knobby, and smooth [4], each of which can be associated with different glacial processes [1]. We use the fundamental differences between the atmospheric Text Ice Sheet Unknown
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
description Introduction: Deposits on the flanks of the large Tharsis Montes volcanoes have been recognized to be of glacial origin [1,2,3]. These Amazonian-aged deposits display three distinct facies, ridged, knobby, and smooth [4], each of which can be associated with different glacial processes [1]. We use the fundamental differences between the atmospheric
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author Tharsis Montes
Tropical Mountain
Glaciation J. L. Fastook
D. E. Shean
J. W. Head
spellingShingle Tharsis Montes
Tropical Mountain
Glaciation J. L. Fastook
D. E. Shean
J. W. Head
ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO
author_facet Tharsis Montes
Tropical Mountain
Glaciation J. L. Fastook
D. E. Shean
J. W. Head
author_sort Tharsis Montes
title ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO
title_short ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO
title_full ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO
title_fullStr ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO
title_full_unstemmed ICE SHEET MODELING DURING HIGH-OBLIQUITY CLIMATES ON MARS: APPLICATION TO
title_sort ice sheet modeling during high-obliquity climates on mars: application to
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.174.6157
http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf
genre Ice Sheet
genre_facet Ice Sheet
op_source http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.174.6157
http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1794.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
_version_ 1766030730297606144