Pre-flare flux ropes appear in 90% of major flares, and thresholds of twist (|T_w| = 2) and decay index (n = 1.3) separate eruptive from confined flares with over 70% accuracy.
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A Study of Pre-Flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes
Pre-flare flux ropes appear in 90% of major flares, and thresholds of twist (|T_w| = 2) and decay index (n = 1.3) separate eruptive from confined flares with over 70% accuracy.