Physics
Scientist
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing, P.R. China
Chinese Academy of Sciences, Beijing, China
Beijing Observatory, People's Republic of China
National Research Council of Canada, Herzberg Institute of Astrophysics, Ottawa
A solar flare in the Fe I 5324 line on 24 June, 1993.
A Synthesized Method for Solving the 1800 Ambiguity of Solar Transverse Magnetic Field
Characteristics of intranetwork magnetic fields in a solar coronal hole.
Characteristics of small scale magnetic fields in a solar coronal hole.
Coincidence between H-alpha flare kernels and peaks of observed longitudinal electric current densities
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