Physics
Plasma Physics
Scientist
Institute of Space Physics and Applied Technology, School of Earth and Space Sciences, Peking University, Beijing, China
Beijing University, People's Republic of China
Institute of Space Physics and Applied Technology, Peking University, Beijing, China
Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
Department of Geophysics, Peking University, Beijing, China
Department of Geophysics, Peking University Beijing 100871, China
Department of Geophysics, Peking University, Beijing 100871, People's Republic of China, CNMax-Planck-Institute for Aeronomy, Katlenburg-Lindau, Germany, DESpace Weather Laboratory, Center for Space Science and Application Research, Chinese Academy of Science, Beijing, People's Republic of China, CNInstitute of Geophysics, Chinese Academy of Science, Beijing, People's Republic of China, CNInstitute of Space Medico-Engineering, Beijing, People's Republic of China, CN
School of Earth and Space Science, Peking University, Beijing, China
State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
Max-Planck-Inst. für Aeronomie, Katlenburg-Lindau, Germany
Beijing Univ., China
SESS, Peking University, Beijing, China
School of Earth and Space Sciences, Peking University, Beijing, China
School of Earth and Space Sciences, Peking University, Beijing 100871, China; Center for Space Science and Applied Research, Chinese Academy of Science, Beijing 100080, China
Peking University, Beijing 100871, China
California, University, Los Angeles, CA; Beijing, University, Beijing, People's Republic of China
Beijing University, Beijing, People's Republic of China; California, University, Los Angeles, CA
Beijing University, Beijing, People's R
A Cluster measurement of fast magnetic reconnection in the magnetotail
A global synthesis model of dipolarization at substorm expansion onset
A magnetic null geometry reconstructed from Cluster spacecraft observations
A series of plasma flow vortices in the tail plasma sheet associated with solar wind pressure enhancement
Ballooning instability in the presence of a plasma flow: A synthesis of tail reconnection and current disruption models for the initiation of substorms
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