Hostname: page-component-7bb8b95d7b-dvmhs Total loading time: 0 Render date: 2024-10-07T08:35:52.397Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Neutral Line Rotations in Flare-Productive Regions

Published online by Cambridge University Press:  30 March 2016

Takako T. Ishii ,
Ayumi Asai ,
Hiroki Kurokawa  and
Tsutomu T. Takeuchi
Takako T. Ishii
Affiliation:
Kwasan and Hida Observatories, Kyoto-U., Yamashina-ku, Kyoto, JAPAN 607-8471
Ayumi Asai
Affiliation:
Kwasan and Hida Observatories, Kyoto-U., Yamashina-ku, Kyoto, JAPAN 607-8471
Hiroki Kurokawa
Affiliation:
Kwasan and Hida Observatories, Kyoto-U., Yamashina-ku, Kyoto, JAPAN 607-8471
Tsutomu T. Takeuchi
Affiliation:
NAOJ, Mitaka, Tokyo, JAPAN 181-8588

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.

We examined the evolution of active regions and found that rotational motions of the neutral line in the δ-type magnetic configuration are common in the flare-productive active regions.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 138
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Kurokawa, H., Wang, T.J., & Ishii, T.T. 2002, ApJ, 572, 598 Google Scholar