Physics
Scientist
Center of Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080 China Academy of Sciences, Peking, ZZZZZ China Academy of Sciences, Peking, zzzzz China for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080 China
State Key Laboratory for Space Weather, Chinese Academy of Sciences, Beijing, China
State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing, China
Center for Space Science and Applied Research, Chinese Academy of Sciences, P.O. Box 8701, Beijing 100080, People's Republic of China
Beijing University of Aeronautics and Astronautics, Beijing, China
Key Laboratory for Space Weather, CSSAR, CAS, Beijing, China
Center for Space Science and application Research, Chinese Academy of Science
State Key Laboratory for Space Weather / CSSAR, Beijing, China
Center for Space Science and Applied Research, Chinese Academy of Sciences, State Key Laboratory of Space Weather, Beijing, China
State key laboratory for space weather, China
Space Science Institute, School of Aeronautics, Beihang University, Beijing, China
CSSAR, NO.1 Nanertiao, Zhongguancun, Haidian district, Beijing, 100080, China
Key Laboratory of Space Weather, CSSAR / CAS, Beijing, China
School of Astronautics, Beihang University, Beijing, China
Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Beijing, China
School of Astronautics, Beijing University of Aeronautics and Astronautics, Beijing, China
Centre d'Étude Spatiale des Rayonnements
Lab. of Heliospheric Physics / CSSAR, P.O. Box 8701, 100080, Beijing, China
Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
Center for Space Science and Applied Researc
Alfven waves in regions of magnetic reconnection and the acceleration of newborn ions
Azimuthally small-scale Alfvén waves in magnetosphere excited by the source of finite duration
Behavior of current sheets at directional magnetic discontinuities in the solar wind at 0.72 AU
Characteristic size and shape of the mirror mode structures in the solar wind at 0.72 AU
Chorus intensification in response to interplanetary shock
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