Convective Gas Flow in Terrestrial and Martian Volcanic Soils: Implications for the Interpretation of THEMIS-IR Data

Details Convective Gas Flow in Terrestrial and Martian Volcanic Soils: Implications for the Interpretation of THEMIS-IR Data Convective Gas Flow in Terrestrial and Martian Volcanic Soils: Implications for the Interpretation of THEMIS-IR Data

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3097a&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3097

Physics

Scientific paper

We report on the detection of convective air flow in the soil of a
terrestrial volcano. Similar processes may operate on Mars as suggested
by observations (THEMIS) at Cerberus fractures, motivating the search
for subsurface heat source on Mars.

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