The BADPIT method finds substantially more EUV transient brightenings in a flare-productive solar active region than in a quiescent one, potentially serving as an early indicator for major flares.
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Brightenings AnD Polarity Inversion Tracking (BADPIT) method for studying solar active region evolution before major solar flares
The BADPIT method finds substantially more EUV transient brightenings in a flare-productive solar active region than in a quiescent one, potentially serving as an early indicator for major flares.