Fig. 7
From: Validation of computed extreme ultraviolet emission spectra during solar flares
Observed and reproduced light curves of GOES/XRS-A and GOES/XRS-B. The dashed and solid lines indicate the reproduced and observed light curves of GOES/XRS during the M9.9-class flare on January 1, 2014, respectively. The red and blue lines represent GOES/XRS-B and GOES/XRS-A, respectively