Computer Science
Scientist
Department of Earth and Planetary Sciences, McGill University, Montreal, PQ, Canada, H3A 2A7 and Planetary Sciences, McGill University, Montreal, Canada
Department of Earth and Planetary Sciences, McGill University, Montreal, Canada
Earth and Planetary Sciences, McGill University, Montreal, Quebec, Canada
Department of Physics, University of Toronto, Toronto, ON M5S 1A7, Canada; Department of Earth and Planetary Sciences, McGill University, Montreal, QC H3A 2A7, Canada
Department of Earth and Planetary Sciences, McGill University, 3450 University St., Montreal, H3A 2A7, Quebec, Canada
Physics, University of Toronto, Toronto, ON, Canada M5S 1A7; Earth and Planetary Sciences, McGill University, Montreal, QC, Canada H3A 2A7
Department of Physics, University of Toronto, Toronto, Ontario, Canada
Earth and Planetary Sciences, McGill University, Que., H3A 2A7, Montréal, Canada
Arizona Univ., Tucson.
Lunar Science Institute
McGill University
Department of Geological Sciences, McGill University, Montreal, Que. H3A 2A7, Canada
Earth and Planetary Sciences, McGill University, 3450 University Street, Montreal, Quebec, H3A 2A7, Canada.
Department of Geological Sciences, McGill University, 3450 University Street, Montreal, Que. H3A 2A7, Canada
Department of Physics, University of Toronto, Toronto, Ontario, Canada; Department of Earth and Planetary Sciences, McGill University, Montreal, Quebec, Canada
Earth and Planetary Sciences, McGill University, Montreal, Quebec, Canada H3A 2A7
Department of Physics, University of Toronto, 60 St. George St., Toronto, ON, Canada M5S 1A7
The Lunar Science Institute
Department of Physics, University of Toronto, Toronto, Canada
Department of Physics, University of Toronto, Toronto, ON, Canada M5S 1A7
Arya Mehr University of Technology, Teheran, Iran
Department of
A 50-degree spherical harmonic model of the magnetic field of Mars
A Coherent Magnetic Field Model of the Martian Crust
A coherent model of the crustal magnetic field of Mars
A study of lunar impact crater size-distributions
An improved 50-degree spherical harmonic model of the magnetic field of Mars derived from both high-altitude and low-altitude data
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