Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
National Astronomical Observatoires / Yunnan Observatory, CAS, Kunming 650011, China
National Astronomical Observatoires / Yunnan Observatory, CAS, Kunming 650011, China.
Yunnan Observatory, CAS, Kunming 650011, National Astronomical Observatoires, PR China; United Laboratory of Optical Astronomy, CAS, PR China
Yunnan Observatory, Yunnan, China
United Laboratory of Optical Astronomy, CAS, China
Yunnan Observatory, Chinese Academy of Sciences, YN650011, People's Republic of China; and National Astronomical Observatoires, People's Republic of China; United Laboratory of Optical Astronomy, Chinese Academy of Sciences, People's Republic of China. Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China
Yunnan Observatory, CAS, Kunming 650011 and National Astronomical Observatoires, CAS, Beijing 100012, PR China; United Laboratory of Optical Astronomy, CAS, Shanghai 200030, PR China
Yunnan Observatory, CAS, Kunming 650011, P.R. China; United Laboratory of Optical Astronomy, CAS, P.R. China
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China and National Astronomical Observatoires, Chinese Academy of Sciences Beijing 100012, China
Yunnan Observatory, Kunming, China
Yunnan Observatory, CAS, 650011 Kunming, P.R. China; United Laboratory of Optical Astronomy, CAS
Astronomical Observatory, Kunming, People's Republic of China
Yunnan Observatory, Chinese Academy of Sciences, YN650011, National Astronomical Observatoires, China; United Laboratory of Optical Astronomy, Chinese Astronomical Society, China.
Institute of Plasma Physics, Academic Sinica, P.O. Box 1126 Hefei, Anlui 230031, People's Republic of China
Yunnan Observatory, Kunming 650011, PR China; National Astronomical Observatoires, Beijing 100012, PR China; United Laboratory of Optical Astronomy, CAS, PR China
Yunnan Observatory, Kunming, People's Republic of China
Astronomic
'Multi-cloud model` (MCM) method and its applications to the study on asymmetric spectral profiles
A Method for Measurements of Solar Vector Magnetic Fields
A Solar Stokes Spectrum Telescope
Asymmetrical Distribution of Sunspot Groups in the Solar Hemispheres
Can Asymmetry of Solar Activity be Extended into Extended Cycle?
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