Ice Accumulation and Flow on Mars: Orientation Trends and Implications for Climate in the Late Amazonian

Details Ice Accumulation and Flow on Mars: Orientation Trends and Implications for Climate in the Late Amazonian Ice Accumulation and Flow on Mars: Orientation Trends and Implications for Climate in the Late Amazonian

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1324d&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1324

Physics

3

Scientific paper

Preliminary results of a mid-latitude survey of glacial-like features
show a latitude-dependent orientation trend, suggesting micro-climate
driven accumulation of ice in the Late Amazonian. This trend is
identical to that of young martian gullies.

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