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Numerical simulations of the CME on 2010 April 8

  • We present 3D zero-beta ideal MHD simulations of the solar flare/CME event that occurred in Active Region 11060 on 2010 April 8. The initial magnetic configurations of the two simulations are stable nonlinear force-free field and unstable magnetic field models constructed by Su et al. (2011) using the flux rope insertion method. The MHD simulations confirm that the stable model relaxes to a stable equilibrium, while the unstable model erupts as a CME. Comparisons between observations and MHD simulations of the CME are also presented.

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Metadaten
Author:Yingna Su, Bernhard KliemORCiD, Adriaan van Ballegooijen, Edward Deluca
URN:urn:nbn:de:kobv:517-opus4-414887
DOI:https://doi.org/10.25932/publishup-41488
ISSN:1866-8372
Parent Title (English):Solar and Astrophysical Dynamos and Magnetic Activity
Series (Serial Number):Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe (674)
Document Type:Postprint
Language:English
Date of first Publication:2019/03/07
Year of Completion:2012
Publishing Institution:Universität Potsdam
Release Date:2019/03/07
Tag:Sun: coronal mass ejections (CMEs); Sun: flares; Sun: magnetic fields
Issue:674
Pagenumber:2
First Page:575
Last Page:576
Source:Proceedings of the International Astronomical Union 8 (2012) 2 pp. 575–576 Symposium 294 (Solar and Astrophysical Dynamos and Magnetic Activity)
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften
Peer Review:Referiert
Publication Way:Open Access
Grantor:Cambridge University Press (CUP)
Licence (German):License LogoKeine Nutzungslizenz vergeben - es gilt das deutsche Urheberrecht