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Modelling Mass Movements for Planetary StudiesUse of an empirical model in conjunction with data from the Chaos Jumbles rock avalanches constrain to first order their flow behavior, and provide a method to interpret rock/debris avalanche emplacement on Mars. Additional information is contained in the original extended abstract.
Document ID
20020046065
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Bulmer, M. H. (Maryland Univ. Baltimore County Catonsville, MD United States)
Glaze, L. (Proxemy Research, Inc. Laytonsville, MD United States)
Barnouin-Jha, O. (Johns Hopkins Univ. Laurel, MD United States)
Murphy, W. (Leeds Univ. United Kingdom)
Neumann, G. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20020045549Collected WorksLunar and Planetary Science XXXIII
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