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Fig. 12 | Earth, Planets and Space

Fig. 12

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

Fig. 12

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

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