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Simulating the Coronal Evolution of AR 11437 using SDO/HMI Magnetograms

By Stephanie Yardley and others
The coronal magnetic field evolution of AR 11437 is simulated by applying the magnetofrictional relaxation technique of Mackay et al. (2011). A sequence of photospheric line-of-sight magnetograms produced by SDO/HMI are used to drive the simulation and continuously evolve the coronal magnetic field of the active region through a series... Show more
December 1, 2017
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Simulating the Coronal Evolution of AR 11437 using SDO/HMI Magnetograms
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