Physics – Plasma Physics
Scientist
Physics
Plasma Physics
Scientist
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA
New Hampshire University
New Hampshire Univ., Durham.
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, 2455 Hayward, Ann Arbor, MI 48109-2143, USA
University of Michigan, Atmospheric, Oceanic, and Space Sciences 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
Michigan University
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
New Hampshire, University, Durham, N.H.
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143
AOSS, University of Michigan, Ann Arbor, MI, USA;
AOSS, Univ Michigan, Ann Arbor, MI, USA;
University of Michigan, Ann Arbor, MI, USA;
NASA / Goddard Space Flight Center
Department of Atmospheric, Oceanic, and Space Science, University of Michigan, Ann Arbor, MI 48109 Office of Space Science and Applications, Washington, DC
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, USA
Department of AOSS, University of Michigan, Ann Arbor, MI 48109, USA
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109-2143 ggloatumich.edu
New Hampshire, University, Durham, NH
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143 of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109
A model describing CME reconnection by diffusion of open magnetic field lines
A Model Describing the Reconnection of Magnetic Field Lines Behind Coronal Mass Ejections.
A New Technique for Mapping Open Magnetic Flux from the Solar Surface into the Heliosphere
A survey of approximately 1 MeV/nucleon solar flare particle abundances, in the Z 1-26 range, during the 1973-1977 solar minimum period
Acceleration and Composition of Solar Wind Suprathermal Tails
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