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3D dynamical structuring of a high latitude erupting prominence: II- Analysis of the coronal context and eruption
Published online by Cambridge University Press: 06 January 2014
Abstract
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Both the origin of the quiescent prominences and their eruption related to CMEs event are still a matter of extended studies. The case of high latitudes quiescent prominences producing slow CMEs can be considered as a potential component of the slow wind. A high latitude prominence was observed on November 13 - 14, 2011. A schematic representation of flux rope is proposed to describe the magnetic structure of the prominence prior to its eruption.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 433 - 434
- Copyright
- Copyright © International Astronomical Union 2013
References
Koutchmy, S., Filippov, B.Tavabi, E.Weiller, S., & Bazin, C. 2013, IAUS-300 Proc. Poster IGoogle Scholar
Regnier, S., Walsh, R. N., & Alexander, C. E. 2011, Astron. Astrophys., 533, L1CrossRefGoogle Scholar
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