Physics – Plasma Physics
Scientist
Physics
Plasma Physics
Scientist
Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190
Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080
Center for Space Science and Applied Research, Chinese Academy of Sciences, P.O. Box 8701, Beijing 100080, People's Republic of China
Chinese Academy of Sciences, Institute of Space Physics, Beijing, People's Republic of China; Maryland, University, College Park, MD
Key Laboratory for Space Weather / CSSAR, Beijing, China
Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080, China
Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080, China.
Center for Space Science and Applied Research, Chinese Academy of Sciences, State Key Laboratory of Space Weather, Beijing, China
University of Maryland, College Park, MD, US
Center for Space Science and Applied Research, Chinese Academy of Science, Beijing, China
Key Laboratory of Space Weather, CSSAR / CAS, Beijing, China
Maryland, University, College Park
State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
Chinese Academy of Sciences, Institute of Space Physics, Beijing, People's Republic of China
Centre d'Étude Spatiale des Rayonnement, Bp 4346, 31029, Toulouse, France
Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
Chinese Academy of Sciences, Center for Space Science and Applied Research, Beijing, People's Republic of China
Institute of Physics, Chinese Academy of Sciences, Beijing 100080, China
A beam-maser instability: Direct amplification of radiation
Altitude-dependent Emission of Type III Solar Radio Bursts
Beam-density gradient drift instabilities and heating in the plasma sheet boundary layer
Characteristics of middle- to low-latitude Pi2 excited by bursty bulk flows
Cluster observations of waves in the whistler frequency range associated with magnetic reconnection in the Earth's magnetotail
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