Numerical Modeling of Titan Fluvial Channels

Details Numerical Modeling of Titan Fluvial Channels Numerical Modeling of Titan Fluvial Channels

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2348m&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2348

Physics

Scientific paper

Model for brines flowing in martian gullies will be modified under Titan
conditions. It will place minimum constrains on the fluid properties
within Titan’s large channels in order to identify the maximum
boulder sizes the channel could support.

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