Hostname: page-component-54dcc4c588-trf7k Total loading time: 0 Render date: 2025-10-01T01:35:46.850Z Has data issue: false hasContentIssue false
  • English
  • Français

The Evolutional Characteristics of Magnetic and Velocity Fields of Large Flares in AR 6659

Published online by Cambridge University Press:  12 April 2016

Luo Baorong ,
Hou Shuming ,
Luan Ti  and
Cao Ying
Luo Baorong
Affiliation:
Yunnan Observatory, Chinese Academy of Sciences
Hou Shuming
Affiliation:
Yunnan Observatory, Chinese Academy of Sciences
Luan Ti
Affiliation:
Yunnan Observatory, Chinese Academy of Sciences
Cao Ying
Affiliation:
Yunnan Observatory, Chinese Academy of Sciences

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The evolutional characteristics of magnetic and velocity fields of four large flares in AR 6659 are analysed in this paper.

Information

Type
Session 6. Flares and Transients
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 362 - 365
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Hou, S. and Luo, B. 1992, The Flares at AR6659 Workshop, Ottawa.Google Scholar
Li, J. et al. 1988, Acta Astrophysica Sinica, 8(4), 301.Google Scholar
Luo, B. 1992, Acta Astronomica Sinica, 33(3), 277.Google Scholar
Takashi, Sakurai et al. 1992, Pub. Astro. Soc. Japan, 44, 7–13.Google Scholar
SESC PRF of SGD, 1976, 822-825.Google Scholar
Zhang, H. et al. 1989, Acta Astrophysica Sinica, 9(3), 271.Google Scholar