BADPIT detects up to five times more transient brightenings in a flaring active region than a comparable non-flaring one, with power-law events nearly absent in the quiescent region, over 24-hour periods before X-class flares.
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Brightenings AnD Polarity Inversion Tracking (BADPIT) method for studying solar active region evolution before major solar flares
BADPIT detects up to five times more transient brightenings in a flaring active region than a comparable non-flaring one, with power-law events nearly absent in the quiescent region, over 24-hour periods before X-class flares.