Physics
Scientist
Center for Space Environment Modeling, University of Michigan 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
University of Michigan, Ann Arbor, USA
Atmospheric, Oceanic, and Space Sciences Department, University of Michigan, Ann Arbor, MI, USA
Space Physics Research Laboratory, University of Michigan, Ann Arbor, Michigan, USA
University of Michigan, Space Physics Research Laboratory, 2455 Hayward St SRB Rm 1432A, Ann Arbor, MI 48109-2143, USA
Department of Atmospheric, Oceanic and Space Sciences, The University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA
University of Michigan, Departmen of Atmospheric, Oceanic and Space Sciences, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA
AOSS, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA
Center for Space Environment Modeling, Space Research Building University of Michigan, Ann Arbor, MI 48109-2143, USA
University of Michigan, Department of Atmospheric, Oceanic and Space Sciences, 2455 Hayward, Ann Arbor, MI 48109-2143, USA
University of Michigan, AOSS Dept., 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
University of Michigan, Space Research Building, 2455 Hayward str., Ann Arbor, MI 48109, USA
Space Physics Research Laboratory, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 49109, USA
University of Michigan, Space Research Building 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
Space Physics Research Laboratory, The University of Michigan, Ann Arbor, MI 48109-2, USA
University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
University of Michigan Department of Atmospheric, Oceanic and Space Sciences, University of Michigan 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
University of Michi
A comparison of global models for the solar wind interaction with Mars
Data-Model Comparisons of Photoelectron Flux Intensities on the Strong Crustal Field Lines at Mars
Development of Magnetospheric Current Systems During Storms: MHD and Event-Oriented Magnetic Field Modeling Approaches
Distortions of the Inner Magnetosphere Magnetic Field during storms, saw-tooth oscillations and Steady Magnetospheric Convection events
Evolution of the proton ring current energy distribution during 21-25 April 2001 storm
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