Factors controlling the depths and sizes of magma reservoirs in Martian volcanoes

Details Factors controlling the depths and sizes of magma reservoirs in Martian volcanoes Factors controlling the depths and sizes of magma reservoirs in Martian volcanoes

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1565w&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 565.

Physics

Mars Surface, Volcanoes, Magma, Density Measurement, Basalt, Pressure Measurement, Depth, Planetary Crusts, Rocks, Geophysical Fluids, Fluid Pressure

Scientific paper

We investigate how the variation of density with depth controls the
locations of magma reservoirs in basaltic volcanoes on Mars, finding
that reservoir centers should typically lie at depths of 9 to 13 km, and
discuss stress controls on the vertical extents of reservoirs.

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