Non-force-free initial magnetic fields in solar flare simulations release about twice the magnetic energy and yield EUV emission closer to observations than conventional NLFF extrapolations.
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2 Pith papers cite this work. Polarity classification is still indexing.
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FastQSL 2 extends prior magnetic connectivity software with spherical coordinate support that eliminates polar singularities, arbitrary output meshes, and direct computation of field lines plus current density for solar applications.
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Energetics and Emission in a Simulated Solar Flare Initialised by a Non-Force Free Magnetic Field
Non-force-free initial magnetic fields in solar flare simulations release about twice the magnetic energy and yield EUV emission closer to observations than conventional NLFF extrapolations.
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FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis
FastQSL 2 extends prior magnetic connectivity software with spherical coordinate support that eliminates polar singularities, arbitrary output meshes, and direct computation of field lines plus current density for solar applications.