Fig. 9
From: Validation of computed extreme ultraviolet emission spectra during solar flares
Example of EUV flare line light curves. The EUV flare line light curves for the M9.9-class flare on January 1, 2014. The wavelength resolution of the light curves was 10 Å, which is the same as that of FISM. The panels indicate the light curves of Fe VIII and Fe XX 130 Å (red), Fe XV 280 Å (cyan), Fe XVI 330 Å (purple), Fe XVIII 90 Å (orange), and He II 300 Å (blue) obtained by the SDO/EVE MEGS-A observation (top panel: solid line), the proposed model estimation (middle panel: dashed line), and FISM estimations (bottom panel: dotted line), respectively. The slope of the regression and correlation coefficient (CC) for each model are shown at the upper left and bottom right