Fig. 11
From: Validation of computed extreme ultraviolet emission spectra during solar flares
Comparison results of EUV flare band time-integrated irradiance. The relationship between the SDO/EVE MEGS-A observations and proposed model estimations of the EUV flare energies of two wavelength bands for a 55–355 Å and b 55–135 Å. The results of the proposed model are plotted in red, and the FISM results are plotted in blue. In each panel, the solid line indicates the regression of each plot; the dashed line indicates the straight line with slope of “1” and the slope of regression is shown at the upper left and bottom right