Aeolian Dunes from Volcaniclastic Sediments: The Medusae Fossae Formation, Mars, and Andean Ignimbrites, Earth

Details Aeolian Dunes from Volcaniclastic Sediments: The Medusae Fossae Formation, Mars, and Andean Ignimbrites, Earth Aeolian Dunes from Volcaniclastic Sediments: The Medusae Fossae Formation, Mars, and Andean Ignimbrites, Earth

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1692b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1692

Computer Science

Scientific paper

One hypothesis for the source of dark dune sediments on Mars is
volcaniclastic sediments. Comparison between dark dunes in the western
Medusae Fossae Formation and dark dunes derived from an Andean
ignimbrite supports this hypothesis.

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