High Mantle Viscosity Controls the Enormous Size of Martian Volcanoes: A Hypothesis Based on Inferences from Rayleigh-Taylor Instability Theory

Details High Mantle Viscosity Controls the Enormous Size of Martian Volcanoes: A Hypothesis Based on Inferences from Rayleigh-Taylor Instability Theory High Mantle Viscosity Controls the Enormous Size of Martian Volcanoes: A Hypothesis Based on Inferences from Rayleigh-Taylor Instability Theory

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1309y&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1309

Physics

Scientific paper

The size and spacing of Tharsis volcanoes increase with time. This is
explained by an increase in mantle viscosity with time that controls
volcano spacing assuming eruption centers were initiated by
Rayleigh-Taylor instability.

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