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Progress in Earth and Planetary Science
Fig. 12 | Progress in Earth and Planetary Science

Fig. 12

From: Magnetohydrodynamics modeling of coronal magnetic field and solar eruptions based on the photospheric magnetic field

Fig. 12

Enhancement of B t during an X2.2-class flare. a The observations of B t enhancement in the photosphere during an X2.2-class flare, reported by Wang et al. (2012). b The B z distribution for which the B t enhancement was measured in the MHD simulation by Inoue et al. (2015). The white contour line corresponds to the PIL. c B t enhancements as observed in the MHD simulation by Inoue et al. (2015). All images are copyright AAS and are reproduced by permission

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