Fig. 1From: Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flaresExample of the observed and modeled soft X-ray fluxes of GOES/XRS-B. The soft X-ray fluxes of GOES/XRS-B during the X1.1-class flare on November 8, 2013. The solid red, blue, and black lines indicate the light curves obtained from the SFEM, the flare component of FISM2 (FISM2 flare), and the GOES/XRS observation, respectively. The dotted blue line indicates the daily component of FISM2 (FISM2 daily)Back to article page