Megafans and Paleo-Megafans in Amazonis and Northwest Tharsis: Implications for Fluvial Processes, Surface Geology, and Spreading of the Olympus Mons Volcano

Details Megafans and Paleo-Megafans in Amazonis and Northwest Tharsis: Implications for Fluvial Processes, Surface Geology, and Spreading of the Olympus Mons Volcano Megafans and Paleo-Megafans in Amazonis and Northwest Tharsis: Implications for Fluvial Processes, Surface Geology, and Spreading of the Olympus Mons Volcano

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2253w&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2253

Physics

Scientific paper

Megafan sediments of Amazonis may have repeatedly provided decollement
conditions that have produced the distinctive shape and tectonism of
both the Olympus Mons edifice and its flanking landslides (aureole
deposits).

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