A Structural Solution for the Formation of Dunes in the Martian Polar Region

Details A Structural Solution for the Formation of Dunes in the Martian Polar Region A Structural Solution for the Formation of Dunes in the Martian Polar Region

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2050z&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Geometry and location of linear and rhombus dunes at the polar regions
of Mars are controlled by en echelon and conjugate fractures,
respectively. The processes of the formation and evolution of dunes
provide information of climate change on Mars.

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