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.
Author details: | Yingna Su, Bernhard KliemORCiDGND, Adriaan van Ballegooijen, Edward Deluca |
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URN: | urn:nbn:de:kobv:517-opus4-414887 |
DOI: | https://doi.org/10.25932/publishup-41488 |
ISSN: | 1866-8372 |
Title of parent work (English): | Solar and Astrophysical Dynamos and Magnetic Activity |
Publication series (Volume number): | Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe (674) |
Publication type: | Postprint |
Language: | English |
Date of first publication: | 2019/03/07 |
Publication year: | 2012 |
Publishing institution: | Universität Potsdam |
Release date: | 2019/03/07 |
Tag: | Sun: coronal mass ejections (CMEs); Sun: flares; Sun: magnetic fields |
Issue: | 674 |
Number of pages: | 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 |
DDC classification: | 5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften |
Peer review: | Referiert |
Publishing method: | Open Access |
Grantor: | Cambridge University Press (CUP) |
License (German): | Keine öffentliche Lizenz: Unter Urheberrechtsschutz |