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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

Serge Koutchmy
Affiliation:
IAP UMR 7095, INSU-CNRS and UPMC, 98 bis Bd Arago 75014 Paris, France email: koutchmy@iap.fr, bazin@iap.fr, sweiller@free.fr
Boris Filippov
Affiliation:
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow Region 142190, Russia email: boris_filippov@mail.ru
Ehsan Tavabi
Affiliation:
Payame Noor University of Tehran, 14155-6466, I.R. of Iran email: etavabi@gmail.com
Cyrille Bazin
Affiliation:
IAP UMR 7095, INSU-CNRS and UPMC, 98 bis Bd Arago 75014 Paris, France email: koutchmy@iap.fr, bazin@iap.fr, sweiller@free.fr
Sylvain Weiller
Affiliation:
IAP UMR 7095, INSU-CNRS and UPMC, 98 bis Bd Arago 75014 Paris, France email: koutchmy@iap.fr, bazin@iap.fr, sweiller@free.fr
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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
Copyright
Copyright © International Astronomical Union 2013 

References

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