Volcanic Eruption Styles on Mars Due to Shallow Interactions Between Magma and Volatiles

Details Volcanic Eruption Styles on Mars Due to Shallow Interactions Between Magma and Volatiles Volcanic Eruption Styles on Mars Due to Shallow Interactions Between Magma and Volatiles

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1275w&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1275

Computer Science

3

Scientific paper

Martian dikes commonly penetrate within ~5 km of the surface and inject
shallow sills into the cryosphere. We review the consequences of
magma-cryosphere interactions taking account of dike and sill geometries
and cryosphere volatile compositions.

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