A background-subtracted light-curve technique detects white-light emission in 15 of 23 flares in active region 12887, including 12 C-class events and one C1.0, for an overall occurrence rate of about 65 percent.
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NUV continuum enhancements occur in 80 of 234 solar flares, concentrated on ribbon edges during the impulsive phase, with magnitude rising with flare class.
citing papers explorer
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Detection and analysis of white-light emission in solar flares through light curve diagnostics
A background-subtracted light-curve technique detects white-light emission in 15 of 23 flares in active region 12887, including 12 C-class events and one C1.0, for an overall occurrence rate of about 65 percent.
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Statistical Study of Balmer Continuum Enhancement in Solar Flares
NUV continuum enhancements occur in 80 of 234 solar flares, concentrated on ribbon edges during the impulsive phase, with magnitude rising with flare class.