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Fig. 12.

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GOES 1−8 Å peak flux (FSXR) as function of the mean flare-related changes of the (a) free magnetic energy and (b) total helicity, for 220 flares of sample SM1+. The horizontal dashed lines indicate a SXR flux of 5 × 10−5 W m−2, i.e., GOES class M5. Numbers in brackets indicate the ratio of confined to eruptive flares within the tested sample. Flares for which a helicity reversal is detected were excluded. Blue and red color indicates confined and eruptive flare type, respectively. X-class and M-class flares are shown as stars and circles, respectively.

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