Hostname: page-component-76fb5796d-9pm4c Total loading time: 0 Render date: 2024-04-25T11:42:20.931Z Has data issue: false hasContentIssue false
  • English
  • Français

Parametric Survey of Emerging Flux for Triggering CMEs

Published online by Cambridge University Press:  03 June 2005

X. Y. Xu ,
P. F. Chen ,
C. Fang  and
M. D. Ding
X. Y. Xu
Affiliation:
Department of Astronomy, Nanjing University, Nanjing, 210093, China email: xyxu@nju.edu.cn
P. F. Chen
Affiliation:
Department of Astronomy, Nanjing University, Nanjing, 210093, China email: xyxu@nju.edu.cn
C. Fang
Affiliation:
Department of Astronomy, Nanjing University, Nanjing, 210093, China email: xyxu@nju.edu.cn
M. D. Ding
Affiliation:
Department of Astronomy, Nanjing University, Nanjing, 210093, China email: xyxu@nju.edu.cn
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.

Observations suggest that solar coronal mass ejections (CMEs) are closely associated with reconnection-favored flux emergence, which was explained as the emerging flux trigger mechanism for CMEs by Chen and Shibata (2000) based on numerical simulations. This paper presents a parametric survey of the CME-triggering environment. Our numerical results show that whether the CMEs can be triggered depends on both the amount and the location of the emerging flux. The results are useful for space weather forecast.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Magnetohydrodynamics (MHD)Sun: coronal mass ejections
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 217 - 218
Copyright
© 2005 International Astronomical Union