Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Center for Space Environment Modeling, University of Michigan
Space Research Bldg, Univ Michigan, Ann Arbor, MI, USA;
Ctr Space Env Modeling, Univ of Michigan, Ann Arbor, MI, USA;
Michigan University, Ann Arbor, MI, USA;
AOSS, University of Michigan, Ann Arbor, MI, USA;
University of Michigan, Ann Arbor, MI, USA;
Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA;
Atmospheric Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA;
CPA / K.U.Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium
Centrum voor Plasma-Astrofysica, Celestijnenlaan 200B, 3001 Leuven, Belgium
Centrum voor Plasma-Astrofysica, K.U.Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
Centre for Plasma Astrophysics, K.U.LEUVEN, Belgium
Centrum voor Plasma Astrofysica, K. U. Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium
Centre for Plasma Astrophysics, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
Centrum voor Plasma-Astrofysica, K.U. Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium; Center for Space Environment Modeling, University of Michigan, Ann Arbor, MI 48109-2143, USA
University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA
Centre for Plasma Astrophysics, K.U. Leuven, Belgium
Center for Space Environment Modeling, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA
University of Michigan, Ann Arbor, MI, USA
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI, USA
Department of Atmos & Space Sciences, University of Michigan, Ann Arbor, MI, USA
AOSS, University of Michigan, Ann Arbor, MI, USA
Atmospheric Oceanic & Space Science, University of Michigan, Ann Arbor, MI, USA
Centre for Plasma Astrophysics, Leuven Mathematical Modelin
3D Evolution of a "Density-Driven" CME Event
3D simulation of flux emergence from convective zone to corona with BATSRUS
4D Model for the Solar Environment
A 3D Self-consistent Solar Model from the Chromosphere to 1AU
A 3D Two-Temperature Solar Wind Model with Alfven Wave Heating
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