Physics
Scientist
Department of Physics, University of Toronto, 60 St. George Street, Toronto, ON, Canada M5S 1A7
University of Toronto, Department of Physics, 60 St. George St., Toronto, ON M5S1A7 Canada of Physics, University of Toronto, Toronto, Ontario, Canada
Department of Earth and Planetary Sciences, Harvard University, 20 Oxford St., Cambridge, MA 02138, USA of Physics, University of Toronto, 60 St. George St., Toronto, ON M5S1A7, Canada of Physics, University of Toronto, Toronto, ON, Canada University, Department of Earth and Planetary Sciences, 20 Oxford St., Cambridge, MA 02138, USA of Physics, University of Toronto, 60 St. George Street, Toronto, ON M5S 1A7, Canada
University of Toronto, Toronto, ON, Canada University of Toronto, Toronto, ON, Canada University, 20 Oxford St., Cambridge, MA 02138, USA
Department of Earth and Planetary Sciences, Harvard University, Cambridge, Massachusetts 02138, USA
Department of Physics, University of Toronto
Department of Physics, University of Toronto, 60 St. George Street, Toronto, ON M5S 1A7, Canada.
Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138, USA Now at: Department of Physics, University of Toronto, 60 St. George St., Toronto, ON, Canada.
Department of Physics, University of Toronto, Toronto, ON M5S1A7, Canada.
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology; Department of Physics, University of Toronto
A Dynamo Model for Axisymmetrizing Saturn's Internal Magnetic Field Using Thermal Winds in Stably Stratified Layers (Invited)
A dynamo model for axisymmetrizing Saturn's magnetic field
A Dynamo Model of Saturn's Extremely Axisymmetric Internal Magnetic Field
Can Mercury's Weak Surface Magnetic Field be Generated by a Dynamo?
Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields
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Profile ID: LFWR-SCP-P-426467