Physics
Scientist
Chinese Academy of Sciences, Beijing, China
Beijing Astronomical Observatory, CAS, Beijing 100012, China, and National Astronomical Observatoires, CAS, Beijing 100012, China
Beijing Astronomical Observatory and National Astronomical Observatoires, Datun Rd. 20A, Chaoyang District, Beijing 100012, P.R. China
Distribution of 2-D Magnetic Saddle Points and Morphology of Flare Kernels in Solar Active Regions
Fractal Brownian surface and distribution of longitudinal magnetic fields in two solar active regions
Longitudinal components of highly stressed magnetic fields in the active region NOAA 7640
Prediction of maximum sunspot number in solar cycle 23
Sympathetic flares in two adjacent active regions
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