Computer Science – Computer Vision and Pattern Recognition
Scientist
Computer Science
Computer Vision and Pattern Recognition
Scientist
California Institute of Technology, Pasadena, California, USA
Institute of High Energy Physics, Beijing, P. R. China
University of Michigan, Department of Atmospheric, Oceanic, and Space Sciences, Ann Arbor, MI 48109-2143, USA for Space Environment Modeling, The University of Michigan, Ann Arbor, MI 48109-2143, USA Physics Research Laboratory, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48105, USA Los Angeles, CA, USA;
University of California Los Angeles, Los Angeles, CA, USA;
IGPP, UCLA, Los Angeles, CA, USA;
Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, USA;
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, CA, USA;
Institute for Geophysics and Planetary Physics, University of California, Los Angeles, CA, USA
University of Michigan, Department of Atmospheric, Oceanic and Space Sciences, Ann Arbor, MI 48109, USA Atmospheric, Oceanica and Space Science, University of Michigan, Ann Arbor, MI 48109, USA of Michigan, AOSS Department 2455 Hayward St., Ann Arbor, MI 48109-2143, USA of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA Astronomical Observatoires / Yunnan Observatory, CAS
University of Michigan, 2455 Hayward #1421, Ann arbor, MI 48109, USA of Michigan, Atmospheric, Oceanic, and Space Sciences Dept, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA for Space Environment Modeling, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, USA
Space Physics Research Laboratory, University of Michigan, Ann Arbor, MI 48109-2143, USA; N
3-D, 3-species MHD model of the interaction of the solar wind with Mars, in the presence of crustal magnetic fields.
3-D, 3-species, MHD studies of the Interaction of the Solar Wind with Mars.
3-D, MHD Studies of the Effects of the Crustal Magnetic Field and Corona on the Solar Wind Interaction with Mars.
3D global MHD simulation of the interaction between Saturn's magnetosphere and Titan's atmosphere/ionosphere
3D Global MHD Simulation of Titan's interaction with its surrounding plasma
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