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Solar Flare Prediction and Magnetic Field Evolution in Solar Active Region

Published online by Cambridge University Press:  30 March 2016

H.N. Wang ,
G.Q. Zhang ,
C.L. Zhu  and
J.L. Sun
H.N. Wang
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100012, China and National Astronomical Observatories, CAS, Beijing 100012, China
G.Q. Zhang
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100012, China and National Astronomical Observatories, CAS, Beijing 100012, China
C.L. Zhu
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100012, China and National Astronomical Observatories, CAS, Beijing 100012, China
J.L. Sun
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100012, China and National Astronomical Observatories, CAS, Beijing 100012, China

Abstract

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The authors propose a number of empirical criteria for prediction of solar flares based on many years of observations at Huairou Solar Observing Station of Beijing Astronomical Observatory.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 396 - 397
Copyright
Copyright © Astronomical Society of Pacific 2002