Mesoscale Simulation of Atmospheric Response to Chaos Terrain Formation

Details Mesoscale Simulation of Atmospheric Response to Chaos Terrain Formation Mesoscale Simulation of Atmospheric Response to Chaos Terrain Formation

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1171k&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1171

Physics

Scientific paper

We report preliminary results from MRAMS (Mars Regional Atmospheric
Modeling System) simulations intended to test the hypothesis that
localized precipitation during chaos terrain formation formed inverted
channel networks on the plateau adjacent to Juventae Chasma.

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