Physics
Scientist
Beijing Astronomical Observatory, Chinese Academy of Sciences
Beijing Observatory
Beijing Observatory, Beijing, China
A solar flare in the Fe I 5324 line on 24 June, 1993
Relationship between magnetic field evolution and flaring sites in AR 6659 in June 1991
Structures of chromospheric magnetic fields in the solar flare producing active region 5747
Vector magnetogram and dopplergram observation of magnetic flux emergence and its explanation
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