Analog image of an X1.1 class flare in NOAA AR 11429

The data is generated by the DARE-MHD program independently developed within the group, simulated by the photosphere vector magnetogram observed by SDO/HMI, and converted from the original adaptive grid data into a uniform grid using the built-in functions of DARE-MHD. The data of the adaptive grid is used to draw all subgraphs containing magnetic lines of force using Tecplot360. The quasi-separatrix layer (QSL) and twist number (Twist) were calculated using a program developed by Professor Liu Rui of China University of Science and Technology. The equivalent radiation intensity corresponding to the AIA-094 band is obtained by the IDL program within the group. The energy evolution curve is obtained from the data generated by the DARE-MHD program through IDL. The magnetic flux evolution data are obtained from the observed magnetic map and the uniform grid data in the simulation. The remaining images are generated by an IDL program written independently.