Mathematics – Logic
Scientist
Mathematics
Logic
Scientist
Center for Space Environment Modeling, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA
Center for Space Environment Modeling, The University of Michigan, Ann Arbor, MI 48109-2143, USA
Center for Space Environment Modeling, University of Michigan, Ann Arbor, Michigan, USA
University of Michigan, SRB Hayward, Ann Arbor, MI 48109-2143, USA
University of Michigan, SRB, Hayward, Ann Arbor, MI 48109-2143, USA
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
University of Michigan, 1411D Space Research Building, Ann Arbor, MI 48109-2143, USA
University of Michigan, Space Research Building 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA
College of Engineering, University of Michigan, Ann Arbor, MI 48109, USA
University of Michigan, Space Physics Res. Lab 2455 Hayward, Ann Arbor, MI 48109-2143, USA
University of Michigan, Space Research Building 2455 Hayward Rd. Rm. 1411, Ann Arbor, MI 48105, USA
Space Physics Research Laboratory, Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, USA
Space Physics Research Lab, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA
University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143
University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA
University of Michigan, Space Research Building, Ann Arbor, MI 48109-2143, USA
University of Michigan, 2455 Hayward Ave. 1411 SRB, Ann Arbor, MI 48109, USA
Space Physics Research Laboratory, University of Michigan, Space Research Building 2455 Hayward Ave, Ann Arbor, MI 48109-2143, USA
Center for Space Environment Modeling, University of Michigan, Ann Arbor, MI 48109-2143, USA
University of Michigan, 1411D Space Research Building 2455 Hayward St., Ann Arb
3D Global MHD Simulations of Flux-Rope-Driven CMEs
3D MHD Simulation of a Coronal Arcade Eruption by Self-Induced Shearing
A Parallel Adaptive 3D MHD Scheme for Modeling Coronal and Solar Wind Plasma Flows
A three-dimensional MHD study of solar wind mass loading processes at Venus: Effects of photoionization, electron impact ionization, and charge exchange
About the Inflow Boundary Condition for Forecasting Simulations of Magnetospheric Dynamics.
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