The Role of Eolian Processes in Forming Martian Polar Topography

Details The Role of Eolian Processes in Forming Martian Polar Topography The Role of Eolian Processes in Forming Martian Polar Topography

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998lpico.953...19h&link_type=abstract

The First International Conference on Mars Polar Science and Exploration, Proceedings of the Conference held at Camp Allen, TX.

Physics

Mars Surface, Planetary Geology, Topography, Polar Regions, Contours, Geomorphology, Troughs, Escarpments, Dunes, Valleys

Scientific paper

The major topographic features of the martian polar layered deposits
include the conspicuous spiral troughs, subtle undulations, broad
reentrants (chasma) and steep, arcuate scarps, and dune fields. A
prominent role for eolian processes in formation of all these features
is suggested here.

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