The Dynamics of Pyroclastic Density Currents on Mars: Implications for Interpreting Martian Surface Deposits

Details The Dynamics of Pyroclastic Density Currents on Mars: Implications for Interpreting Martian Surface Deposits The Dynamics of Pyroclastic Density Currents on Mars: Implications for Interpreting Martian Surface Deposits

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2140b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2140

Physics

Scientific paper

We’ve developed a model that predicts runout distance,
sedimentation rate and bedform wavelength with distance from source
under Mars conditions. Results show longer runout distances and bedform
wavelengths on Mars due to slower sedimentation rates.

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