Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
Scientist
University of Michigan, Space Physics Research Laboratory Ann Arbor, MI 48105
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109
University of Michigan
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
2417B Space Research Bldg, Univ Michigan, Ann Arbor, MI, USA;
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA;
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI, USA;
Atmospheric, Oceanic and Space Sciences, U. of Michigan, Ann Arbor, MI, USA;
Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI, USA;
Dept Atmos Ocean Space, Univ Michigan, Ann Arbor, MI, USA;
AOSS, University of Michigan, Ann Arbor, MI, USA;
Atmospheric, Oceanic & Space Sciences, University of Michigan, Ann Arbor, MI, USA;
University of Michigan College of Engineering, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA
Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, USA
University of Michigan, Atmospheric, Oceanic & Space Sciences 2455 Hayward St., Ann Arbor, MI 48109, USA
University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA
University of Michigan, Space Research Building 2455 Hayward, Ann Arbor, MI 48109, USA Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Mic, USA
Department of Atmospheric, Oceanic and Space Sciences,
A solar wind coronal origin study from SOHO/UVCS and ACE/SWICS joint analysis
ACE/SWICS observations of heavy ion dropouts near fast-slow stream interfaces
Active Region and Coronal Holes Sources of Solar Wind at Solar Activity Maximum
Active-Region Sources of Solar Wind near Solar Maximum
Algorithm for Tracing Radio Rays in Solar Corona and Chromosphere
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