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Earth, Planets and Space
Fig. 10 | Earth, Planets and Space

Fig. 10

From: Validation of computed extreme ultraviolet emission spectra during solar flares

Fig. 10

Comparison results of EUV flare line time-integrated irradiance. Relationship between the SDO/EVE MEGS-A observations and the proposed model estimations of the EUV flare time-integrated irradiance for a Fe VIII, b Fe XV, c Fe XVI, d Fe XVIII, e Fe XX, and f He II. In each panel, the solid line indicates the regression of each plot; the dashed line indicates the straight line with slope of “1”. The slope of the regression and correlation coefficient (CC) are shown at the bottom right

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