Physics – Plasma Physics
Scientist
Physics
Plasma Physics
Scientist
Space Physics Research Laboratory, University of Michigan, Ann Arbor, Michigan, USA
Center for Planetary Sciences, AOSS Department, University of Michigan
Center for Space Environment Modeling, University of Michigan, Ann Arbor, Michigan, USA
Center for Space Environment Modeling, Atmospheric, Oceanic, and Space Sciences Department, University of Michigan, Ann Arbor, Michigan, USA
Department of Atmospheric, Oceanic and Space Sciences, College of Engineering, University of Michigan, Ann Arbor, Michigan, USA
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
Atmospheric, Oceanic, and Space Sciences Laboratory, University of Michigan, 2455 Hayward St. Ann Arbor, MI 48109-2143, USA
University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
Department of Oceanic and Atmospheric Sciences, University of Michigan, Ann Arbor, MI 48109, USA
Department of Atmospheric and Oceanic Sciences, University of Michigan, Ann Arbor, MI 48109, USA Physics Research Laboratory, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA of Michigan, Space Research Bldg, 2455 Hayward, Ann Arbor, MI 48109-2143, USA of Michigan, Space Research Building 2455 Hayward St., Ann Arbor, MI 48109-2143, USA for Space Environment Modeling, University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109, USA
Michigan, University, Ann Arbor
University of Michigan, Ann Arbor, MI, US
Michigan, University, Ann Arbor, MI
Space Physics Research Laboratory, University of Michigan, Ann Arbor, MI 48109-2143, USA
Atmospheric, Oceanic, and Space Sciences Department, University of Michigan, Ann Arbor, Michigan, USA
Space Physics Research Laboratory, University of Michigan, Ann Arbor, Michigan
A bounce-averaged kinetic model of the ring current ion population
A Perspective on Geomagnetic Storms and Substorms based upon an Analysis of Midlatitude Magnetic Observations and Model Simulations
A possible energy source to power stable auroral red arcs - Precipitating electrons
A statistical comparison of hot-ion properties at geosynchronous orbit during intense and moderate geomagnetic storms at solar maximum and minimum
A statistical comparison of ion bulk properties at geosynchronous orbit during moderate and intense geomagnetic storms at solar minimum and maximum
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