Physics
Scientist
SIGMA Weather Group, State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences
SIGMA Weather Group, State Key Laboratory for Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
Beijing Observatory, Chinese Academy of Sciences, Beijing, PR China
National Astronomical Observatoires / Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China; Graduate School of Chinese Academy of Sciences, Beijing 100049, China
Differential Rotation of Strong Magnetic Flux During Solar Cycles 21 - 23
Effects of α-Enhancement on Stellar Evolution
Pulsational frequencies in the delta Scuti stars V624 Tauri and HD 23194. Results of the STEPHI X campaign on the Pleiades cluster
Three-dimensional MHD simulation of two coronal mass ejections' propagation and interaction using a successive magnetized plasma blobs model
Variations of Solar Electron and Proton Flux in Magnetic Cloud Boundary Layers and Comparisons with Those across the Shocks and in the Reconnection Exhausts
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