How Lateral Density Gradients Affect the Distribution of Multiple Magma Chambers Within Martian Shield Volcanoes

Details How Lateral Density Gradients Affect the Distribution of Multiple Magma Chambers Within Martian Shield Volcanoes How Lateral Density Gradients Affect the Distribution of Multiple Magma Chambers Within Martian Shield Volcanoes

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1536s&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1536

Physics

Scientific paper

We propose that the reason why certain martian volcanoes produce
multiple summit calderas is that the locations of successive underlying
magma chambers migrate under the influence of lateral density gradients
that form within the edifice.

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