Rayleigh-Taylor Instability-driven Plume Tectonics and the Rheology of the Archean, Venusian, and Martian Crusts

Details Rayleigh-Taylor Instability-driven Plume Tectonics and the Rheology of the Archean, Venusian, and Martian Crusts Rayleigh-Taylor Instability-driven Plume Tectonics and the Rheology of the Archean, Venusian, and Martian Crusts

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000lpi....31.1998m&link_type=article

31st Annual Lunar and Planetary Science Conference, March 13-17, 2000, Houston, Texas, abstract no. 1998

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