Physics – Condensed Matter – Strongly Correlated Electrons
Scientist
Physics
Condensed Matter
Strongly Correlated Electrons
Scientist
Minnesota University
5. Space Physics Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
Space Sciences Laboratory, UC Berkeley, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, Berkeley, California 94720, USA
School of Physics and Astronomy, University of Minnesota Minneapolis MN 55455, USA
University of California, Berkeley, CA, USA;
Space Sciences Laboratory, University of California, Berkeley, California, USA
Space Science Laboratory, UC Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
Chinese Academy of Sciences, Geophysics Institute, Beijing, People's Republic of China
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California, 7 Gauss way, Berkeley, CA 94720, USA
Space Sciences Laboratory University of California, Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, at Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
University of Minnesota, Minneapolis, Minnesota 55455
California, University, Los Angeles
Minnesota, University, Minneapolis
University of Minnesota, Minneapolis, MN, US
Augsburg College, Minneapolis, MN
School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 of Minnesota, School of Physics and Astronomy 116 Church St. SE, Minneapolis, MN 55455, USA of Minnesota, 116 Church Street S.E., Minneapolis, MN 55455, USA Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California at Berkely, Berkeley, CA 94720, USA
Sp
A comparison of Pi2 pulsations in the inner magnetosphere and magnetic pulsations at geosynchronous orbit
A comparison of ULF fluctuations in the solar wind, magnetosheath, and dayside magnetosphere. 2. Field and plasma conditions in the magnetosheath
A comparison of ULF fluctuations in the solar wind, magnetosheath, and dayside magnetosphere. I - Magnetosheath morphology. II - Field and plasma conditions in the magnetosheath
A comprehensive statistical study of foreshock density holes
A study of geomagnetic storms at Beijing in terms of solar wind
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