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Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes

By Stephanie Yardley and others
The coronal magnetic field evolution of 20 bipolar active regions (ARs) is simulated from their emergence to decay using the time-dependent nonlinear force-free field method of Mackay et al. A time sequence of cleaned photospheric line-of-sight magnetograms, that covers the entire evolution of each AR, is used to drive the... Show more
December 14, 2020
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Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes
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