A time dependent relation between EUV solar flare light-curves from lines with differing formation temperatures | Journal of Space Weather and Space Climate

Developing New Space Weather Tools: Transitioning fundamental science to operational prediction systems

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Fig. 4

Histograms of the LETM time constant, , for the L(FeXXIII) model for flares grouped according to GOES XRS magnitude range shown at the top of each panel. is the LETM time constant, and taken to be the measured time difference between the time of peak intensity of the indicated line and the Fe XXIII line.

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