Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Key Laboratory of Solar Activity, National Astronomical Observatoires of Chinese Academy of Sciences
Chinese Academy of Sciences, Beijing, China
Beijing Astronomical Observatory, Chinese Academy of Sciences
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, P.R. China Astronomical Observatoires, Chinese Academy of Sciences
National Astronomical Observatoires, Datun Rd. No. 20A, Chaoyang District, Beijing 100012, China
National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588; and it Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
National Astronomical Observatoires, 20A Datun Road, Chaoyang District, Beijing 100012, China
Beijing Astronomical Observatory, Datun Rd. No. 20A, Chaoyang District, Beijing 100012, China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China
W. W. Hansen Experimental Physics Lab., Stanford University, Stanford, CA 94305-4085, USA
National Astronomical Observatories, Chinese Academy of Sciences
Key Laboratory of Solar Activity, National Astronomical Observatoires, Chinese Academy of Sciences, Beijing, China
National Astronomical Observatoires, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China. s.
National Astronomical Observatoires, 20A Datun Road, Chaoyang District, Beijing, China
A survey of the size-flux relation for pores and spots
A Synthesized Method for Solving the 1800 Ambiguity of Solar Transverse Magnetic Field
Application of support vector machine combined with K-nearest neighbors in solar flare and solar proton events forecasting
Correlation Between Solar Flare Productivity and Photospheric Magnetic Field Properties. 1. Maximum Horizontal Gradient, Length of Neutral Line, Number of Singular Points
Correlation between solar flare productivity and photospheric vector magnetic fields
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