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Peking Observatory, Peking, Communist China
Beijing Observatory, People's Republic of China
Astronomical Observatory, Peking, Communist China
Astronomical Observatory, Beijing, People's Republic of China
Paris, Observatoire, Meudon, France
Bern, Universität, Switzerland
Academia Sinica, Beijing, China
Beijing Observatory, Beijing, China
Beijing Observatory, China
Center for Space Science & Applied Research China
Beijing Observatory, Academia Sinica, China
Beijing Observatory, Academia Sinica
Beijing Observatory, Academia Sinica, R.O.C.
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Observatoire de Paris, Meudon, France
Beijing Astronomical Observatory, People's Republic of China
Beijing Observatory, Academia Sinica, Beijing, China
Beijing Astronomical Observatory, Chinese Academy of Sciences China
Beijing Astronomical Observatory, Academia Sinica China
Beijing Observatory, Academia Sinica China2Department of Astronomy, Nanjing University China3Yunnan Observatory, Academia Sinica China
A magnetic loop model for the slowly varying radio source observed during the solar eclipse of 1980 February 16
A model of radiation for solar radio SVC
A Model of Solar (Radio) Active Regions
A model of SVC radiation in magnetic dipole field and radiation varying with magnetic field. I - Active region model and SVC radiation source model
A model of SVC radiation in magnetic dipole field and radiation varying with magnetic field. II - SVC radiation mechanism and radiation variation with magnetic field
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