Astronomy & Space

FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis

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MagnetohydrodynamicsComputational phys…Magnetic reconnect…

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FastQSL 2 is an updated software toolkit designed to identify quasi-separatrix layers (QSLs) in magnetic fields, which are regions where magnetic reconnection preferentially occurs. The new version introduces support for spherical coordinate systems that eliminates computational singularities at polar regions, accommodates flexible output mesh shapes, and can calculate both magnetic field and electric current density. The toolkit can quickly trace magnetic field lines and calculate parameters useful for modeling solar wind speed and magnetic connectivity in solar physics applications.


This tool enables more accurate analysis of magnetic reconnection events in the Sun's atmosphere and solar corona, which are crucial for understanding solar flares, coronal mass ejections, and space weather phenomena that can affect satellite operations and power grids on Earth. The improved polar coordinate handling makes it particularly valuable for analyzing global magnetic field structures.


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Magnetohydrodynamics 21 articles Explore Concept → Computational physics Concept coming soon Magnetic reconnection Concept coming soon

⚠️ Preprint – Noch nicht peer-reviewed

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Abstract: We present a new version of FastQSL for locating quasi-separatrix layers (QSLs) — regions characterized by strong magnetic connectivity gradients, preferential current buildup, and subsequent magnetic reconnection. This version now supports spherical coordinates, utilizing a second spherical coordinate system for tracing magnetic field lines around the polar regions. This approach completely resolves the singularity problem at the two poles. Furthermore, our code accommodates arbitrary mesh shapes for output, can provide both magnetic field and electric current density on the mesh, and can save the traced magnetic field lines. We suggest using $Q_mathrm{local}$ calculated through a localized mapping to locate (quasi-)separators. By quickly and accurately outputting the footpoint coordinates of magnetic field lines, FastQSL can be used to derive the two key parameters used for modeling solar wind speed and slip-squashing factors for the case of zero boundary flow. Compared with the first version, FastQSL 2 achieves significant improvements in terms of application scope.

Source: FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis