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wind-related modification of the meteorite crater morphology as key to wind regime history on marsThe results of high resolution imaging of the Martian surface by MOC, show that wind activity is a dominant process in the current environment, forming and modifying the surface from the equator to the poles.
Document ID
20000081525
Document Type
Conference Paper
Authors
Kuzmin, R. O.
(Academy of Sciences (USSR) Moscow, USSR)
Greeley, R.
(Arizona State Univ. Tempe, AZ United States)
Rafkin, S.
(San Jose State Univ. CA United States)
Haberle, R.
(NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Analytic PrimaryLunar and Planetary Science XXXI