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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3D MHD simulation of successive flux-rope eruptions shows reconnection flux accumulating linearly with CME velocity, consistent with HMI/AIA observations of one event.
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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.
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Evolution of reconnection flux during eruption of magnetic flux ropes
3D MHD simulation of successive flux-rope eruptions shows reconnection flux accumulating linearly with CME velocity, consistent with HMI/AIA observations of one event.