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The Variability of Transverse Aeolian Ripples in Troughs on MarsA precursory glance at MGS images of the surface of Mars show an abundance of aeolian transverse ridges. These ridges are located in a variety of geological terrains. Zimbelman and Wilson have separated the small-scale aeolian features of Syrtis Major into six categories: ripples associated with obstacles, ripple bands, ripple fields, ripple patches, isolated ripple patches and ripples associated with dunes. This paper focuses on one of these categories, that of ripple bands which tend to accumulate within linear troughs. As the origin of these features is still being studied (i.e. ripples versus dunes), we refer to them simply as transverse aeolian ridges.
Document ID
20030111360
Document Type
Conference Paper
Authors
Bourke, M. C. (Oxford Univ. Oxford, United Kingdom)
Wilson, S.A. (Smithsonian Institution Washington, DC, United States)
Zimbelman, J. R. (Smithsonian Institution Washington, DC, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Lunar and Planetary Science XXXIV
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
CONTRACT_GRANT: NAG1-1075
Distribution Limits
Public
Copyright
Public Use Permitted.

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