Abstract
Aims.We study the correlation between the soft (1.6–12.4 keV, mostly thermal) and the hard (20–40 and 60–80 keV, mostly non-thermal) X-ray emission in solar flares up to the most energetic events, spanning about 4 orders of magnitude in peak flux, establishing a general scaling law and extending it to the most intense stellar flaring events observed to date.
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