Data-driven simulation of AR 11158 produces an X-flare triggered by torus instability after MFR formation above a cPIL, with energy release and photospheric changes matching some observed trends.
2012a, ApJL
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Confined flares exhibit total Lorentz force change below 1.8 × 10^22 dyne along the PIL, separating them from eruptive flares in a sample of 37 major events observed 2011-2017.
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Data-inspired simulation of AR 11158
Data-driven simulation of AR 11158 produces an X-flare triggered by torus instability after MFR formation above a cPIL, with energy release and photospheric changes matching some observed trends.
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Photospheric Lorentz force changes in eruptive and confined solar flares
Confined flares exhibit total Lorentz force change below 1.8 × 10^22 dyne along the PIL, separating them from eruptive flares in a sample of 37 major events observed 2011-2017.