Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
V. A. Fock Physics Institute, St.-Petersburg, Russia
Physics Institute, St. Petersburg University, Russia
Department of AOSS, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA
CSEM, Department of AOSS University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143
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
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
Space Physics Research Lab, University of Michigan
Space Research Laboratory, University of Michigan, Ann Arbor, MI 48109-2143
Laboratory for Plasma Astrophysics, Faculty of Engineering, Toyama University, 3190 Gofuku, Toyama 930-8555, Japan
Center for Space Environment Modeling, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109-2143, USA
Center for Space Environment Modeling, University of Michigan, Ann Arbor, Michigan, USA
Center for Space Environment Modeling, University of Michigan, Ann Arbor., 2455 Hayward, Ann Arbor, MI 48109-2143, USA
Laboratory for Plasma Astrophysics, Faculty of Engineering, Toyama University, 3190, Gofuku, Toyama 930-8555, Japan
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109 of Atmospheric, Oceanic and Space Sciences, University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
Center for Space Environment Modeling-University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA
University of Michigan, Space Res Bldg 2455 Hayward St, Ann Arbor, MI 48109, USA
Center for Space Environment Modeling, University of Michigan at Ann Arbor, 2455 Hayward Street, Ann Arbor, MI 48109-2143
3-D global MHD model prediction for the first close flyby of Titan by Cassini
3-D, MHD Studies of the Effects of the Crustal Magnetic Field and Corona on the Solar Wind Interaction with Mars.
3D MHD studies of the effects of the crustal magnetic field and the corona on the solar wind interaction with Mars
4D Model for MHD Wave Turbulence in the Solar Corona and Solar Wind
4D Model for the Solar Environment
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