During two M-class flares, spectrally resolved Lyman-alpha brightening correlated with hard X-ray bursts, with wing asymmetries attributed to chromospheric evaporation and a filament eruption.
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Spectral Irradiance Variability in Lyman-Alpha Emission During Solar Flares
During two M-class flares, spectrally resolved Lyman-alpha brightening correlated with hard X-ray bursts, with wing asymmetries attributed to chromospheric evaporation and a filament eruption.