Lava Tube Flow: Constraints on Maximum Sustained Eruption Rates for Major Martian Volcanic Edifices

Details Lava Tube Flow: Constraints on Maximum Sustained Eruption Rates for Major Martian Volcanic Edifices Lava Tube Flow: Constraints on Maximum Sustained Eruption Rates for Major Martian Volcanic Edifices

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1992w&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1992

Physics

Scientific paper

Modeling maximum volcanic flow rates of large martian volcanoes yields
an inverse relationship between edifice size and flow rate . . . low
rates (often lava tubes) yield the largest edifice volumes; higher rates
(usually channels) produce the smallest.

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