Hostname: page-component-745bb68f8f-kw2vx Total loading time: 0 Render date: 2025-01-11T11:46:30.957Z Has data issue: false hasContentIssue false
  • English
  • Français

Study of ribbon separation and magnetic reconnection rates

Published online by Cambridge University Press:  18 July 2013

Wenbin Xie ,
Hongqi Zhang ,
Jun Lin  and
Haimin Wang
Wenbin Xie
Affiliation:
Department of Physics, Jilin Normal University, Postbus 136000, Jilin, China email: [email protected] National Astronomical Observatories Chinese Academy of Sciences, Postbus 100012 Beijing, China email: [email protected]
Hongqi Zhang
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Postbus 100012 Beijing, China email: [email protected]
Jun Lin
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Postbus 650011, Yunnan, China email: [email protected]
Haimin Wang
Affiliation:
New Jersey Institute of Technology, Postbus NJ07102, Newark email: [email protected]
Rights & Permissions [Opens in a new window]

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 study the correlation between the speed of two-ribbon separation and the magnetic flux density during the 2001 April 10 solar flare. A weak negative correlation is found between the ribbon separation speed (Vr) and the longitudinal magnetic flux density (Bz). In addition, we estimate the magnetic reconnection rate (Erec). Along the flare ribbons, Erec fluctuates in the small range except near the HXR source. The localized enhancement of the reconnection rate corresponds to the position of the HXR source.

Keywords

Solar activitySolar flaresSolar magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 585 - 586
Copyright
Copyright © International Astronomical Union 2013 

References

Asai, A., Yokoyama, T., Shimojo, M., Masuda, S., Kurokawa, H., & Shibata, K. 2004, ApJ, 611, 557 Google Scholar
Kitahara, T. & Kurokawa, H. 1990, SolPhys, 125, 321 Google Scholar
Lin, J. 2004, SolPhys, 222, 115 Google Scholar
Miklenic, C. H., Veronig, A. M., Vršnak, B., & Hanslmeier, A. 2007, Astron. Astrophys., 461, 697 Google Scholar