Fig. 10
Flare EM(T) distributions used to modify solar coronal EMD, normalized to unit surface. Black distribution: time-averaged flares presented in Reale et al. (2001) generated according to Orlando et al. (2017); blue distribution: contribution of flares at soft and hard energies; green distributions: contribution of flares in the decay phase; red distribution: contribution of flares at the lowest temperatures.
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