Simulations of Puu OO lava flows on Mars

Mathematics – Logic

Scientific paper

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Mars Volcanoes, Lava, Flow Distribution, Rheology, Data Simulation, Planetary Gravitation, Scaling Laws, Magma, Mathematical Models

Scientific paper

In this study, longitudinal thickness profiles are simulated for lava flows on Mars, erupted under identical conditions to Phase 2 of the Puu Oo eruption. Data on the thickness, width, slope, and advance rates (Wolfe et al., 1988) are used in two emplacement models to infer the systematic rheologic change along the flow path. The models subsequently provide a basis for scaling the thickness and advance rates to account for the difference in Mars gravity.

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