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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.SR 3verdicts
UNVERDICTED 3representative citing papers
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.
Persistent same-polarity flux emergences drove collisional shearing and cancellations at a PIL, accumulating free energy and forming MFRs that produced multiple large flares including X9.0, with a pre-flare drop in photospheric free-energy area as a possible precursor.
citing papers explorer
-
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.
-
Magnetic Evolution of Highly-Sheared Region in Active Region 13842 Producing Large X9.0 Flare
Persistent same-polarity flux emergences drove collisional shearing and cancellations at a PIL, accumulating free energy and forming MFRs that produced multiple large flares including X9.0, with a pre-flare drop in photospheric free-energy area as a possible precursor.