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...

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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:
Ice Sheet
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
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Summary: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

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