Fig. 1.
Magnetic flux ropes formed during the X2.2 flare just prior to the 9.3 flare derived from NLFFF magnetic field reconstruction by Inoue et al. (2018) (panel a), which established the magnetic topology derived by the MHD simulations just prior to the X9.3 flare (panel b) with the loop footpoints being linked to the sunquake locations detected for this flare.
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