Fig. 13From: Magnetohydrodynamics modeling of coronal magnetic field and solar eruptions based on the photospheric magnetic fieldSummary of the dynamics of the magnetic field during an X2.2-class solar flare. Summary of the magnetic field dynamics during an X2.2-class solar flare, obtained from Inoue et al. (2014a) and Inoue et al. (2015) Back to article page