Studies of Lava Flows in Mars' Tharsis Region Using SHARAD Radar

Details Studies of Lava Flows in Mars' Tharsis Region Using SHARAD Radar Studies of Lava Flows in Mars' Tharsis Region Using SHARAD Radar

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1595s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1595

Computer Science

Scientific paper

Models show that Tharsis area lavas, including long flows near Ascraeus
and Pavonis Montes, had viscosities consistent with basaltic flows. We
surveyed SHARAD radar data across the area to understand the composition
and stratigraphy of these flows.

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