Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
U. Chicago
University of Chicago and Center for Magnetic Self Organization in Laboratory and Astrophysical Plasmas
Department of Astronomy and Astrophysics, University of Chicago, Chicago, USA
Joint Institute for Laboratory Astrophysics; Colorado, University, Boulder
Department of Mathematics, University of Chicago, Chicago, IL 60637, USA
Joint Inst. for Lab. Astrophysics, Boulder, CO
Chicago, University, IL
Department of Mathematics, University of Chicago
Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Ave, Chicago, IL 60637, USA
Department of Mathematics, University of Chicago, 5734 S. University Ave, Chicago, IL 60637
Department of Mathematics, University of Chicago, 5734 South University Avenue, Chicago, IL 60637 and Astrophysics Center, University of Chicago, 5640 South Ellis Avenue, Chicago Illinois 60637
Department of Astronomy and Astrophysics and the Computation Institute, University of Chicago, Chicago, IL 60637 of Astronomy and Astrophysics and The Computation Institute, University of Chicago, Chicago, Illinois 60637, USA
Chicago Univ., IL
Department of Mathematics, University of Chicago, 5734 South University Avenue, Chicago, IL 60637
Joint Institute for Laboratory Astrophysics, Boulder, CO
Assistant Professor in the Department of Mathematics, University of Chicago.
The University of Chicago, Department of Mathematics
University of Chicago, Chicago, IL
Department of Mathematics, University of Chicago, 5734 South University Avenue, Chicago, IL 60637, USA
School of Mathematics, University of Newcastle-upon-Tyne, England NE1 7RU
University of Chicago, Chicago, IL, US
Department of Mathematics, University of Chicago, Chicago, IL
A Dynamo Driven by Turbulent Thermal Convection.
A new twist to the solar cycle
An Experimental Plasma Dynamo Program for Investigations of Fundamental Processes in Heliophysics
Aspect ratio dependence in magnetorotational instability shearing box simulations
Challenges to the theory of solar convection
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