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Fig. 8


Total (bolometric) radiated energies, Ebol, in solar flares as a function of peak GOES flux FG, as given by Emslie et al. (2012, diamonds) and Kretzschmar (2011, crosses). A power-law fit (dotted line) to the values of Kretzschmar (2011), its slope α and intercept b, and the rank correlation coefficient, R, are also shown.

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