Evolution of Coronal Magnetic Field Parameters During X5.4 Solar Flare

Seth H Garland, PhD student at the Air Force Institute of Technology, authored a paper including part of his dissertation research on modeling the evolution of 3D coronal magnetic fields during a solar flare.  This paper was accepted on 2/22/23 for publication in Frontiers in Astronomy and Space Sciences, section Space Physics; at https://www.frontiersin.org/articles/10.3389/fspas.2023.1148293/full.

Garland article graphic
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