NuSTAR observations of 113 faint solar X-ray transients show they are cooler and dimmer than RHESSI microflares, with quiet-Sun events having lower energies and no cases above 3x10^27 erg.
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New X-ray flare detections from M dwarfs combined with literature data yield flare frequency constraints and an upper limit of 0.5-30 Myr on atmospheric loss times for habitable planets orbiting them.
citing papers explorer
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A Statistical Survey of Faint Solar X-ray Transients Observed by NuSTAR
NuSTAR observations of 113 faint solar X-ray transients show they are cooler and dimmer than RHESSI microflares, with quiet-Sun events having lower energies and no cases above 3x10^27 erg.
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Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context
New X-ray flare detections from M dwarfs combined with literature data yield flare frequency constraints and an upper limit of 0.5-30 Myr on atmospheric loss times for habitable planets orbiting them.