Abstract
This paper describes an MHD simulation of an observed Sigmoid in AR 11283 from its formation to eruption. The Non-linear Force Free MHD model (Jiang and Feng, 2012) and the data-driven active region evolution model (Wu et al., 2006; Jiang et al. 2013) together with the SDO/HMI magnetograms are used. We show the successful simulation results of the eruption of a flux-rope structure. © 2013 International Astronomical Union.
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CITATION STYLE
Wu, S. T., Jiang, C., Feng, X., Hu, Q., & Liu, Y. (2013). Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. In Proceedings of the International Astronomical Union (Vol. 8, pp. 466–467). Cambridge University Press. https://doi.org/10.1017/S1743921313011587
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