TRAPPIST-1 flares follow a single power law N(≥E_TESS) ∝ E_TESS^{-0.753} from 10^{29} to 10^{33} erg after sensitivity corrections and bandpass conversion.
A new catalogue of solar flare events from soft x-ray goes signal in the period 1986–2020
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Spectral flattening in active-region radio emission at 18-26 GHz signals an 89% probability of a strong solar flare within 30 hours, with only 12% of such flares missed despite weekly observations.
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A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy
TRAPPIST-1 flares follow a single power law N(≥E_TESS) ∝ E_TESS^{-0.753} from 10^{29} to 10^{33} erg after sensitivity corrections and bandpass conversion.
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Correlation between active regions' spectra at high radio frequencies and solar flare occurrences
Spectral flattening in active-region radio emission at 18-26 GHz signals an 89% probability of a strong solar flare within 30 hours, with only 12% of such flares missed despite weekly observations.