Mathematics – Logic
Scientist
Mathematics
Logic
Scientist
Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
Department of Earth and Planetary Sciences, Campus Box 1169, Washington University in Saint Louis, St. Louis, MO 63130, USA
Department of Earth and Planetary Sciences, Washington University, St. Louis, Missouri, USA
Washington University in Saint Louis, 1 Brookings Drive, Saint Louis, MO 63130, USA of Physics, New Mexico State University, P.O. Box 30001, 88003, Las Cruces, NM, USA
Department of Physics, New Mexico State University, Las Cruces, New Mexico, USA
AN SSSR, Institut Fiziki Zemli, Moscow, USSR
California Institute of Technology, Pasadena.
Department of Physics, New Mexico State University, Las Cruces, NM 88003
Department of Earth and Planetary Sciences, Washington University, Campus Box 1169, Saint Louis, MO 63130-4899, USA
AN SSR, Institut Fiziki Zemli, Moscow, USSR
Washington University in St. Louis, Department of Earth and Planetary Sciences, St. Louis, MO 63130, USA of Earth and Planetary Science, Washington University, Saint Louis, MO 63130 University, Campus Box 1169, 1 Brookings Drive, St. Louis, MO 63130, USA of Physics, New Mexico State University, 88003, Las Cruces, NM, USA
Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, MO 63130, USA
Department of Physics, New Mexico State University, Las Cruces, NM, USA
Mail Stop 252-21, Seimological Laboratory, California Inst. of Technology, Pasadena, CA 91125
New Mexico State University, Department of Physics, Las Cruces, NM 88003, USA
Department of Physics, New Mexico State University, Las Cruces, NM 88003, USA
California Institute of Technology, Pasadena, CA, US
California Inst. of Technology, Pasadena
A Simple Cooling Model for the Cessation and Distribution of Volcanism on Venus
A simple cooling model for the evolution of volcanism on Venus
Can sharp seismic discontinuities be caused by non-equilibrium phase transformations?
Comparison of Lunar and Terrestrial Magma Oceans
Constraints on the Global Lithospheric Thickness of Venus in the Isostatic Stagnant Lid Approximation
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