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to calculate magnetic topology, length and twist number of field lines

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FastQSL

CC BY-NC-SA 4.0

This module is licensed under a CC BY-NC-SA 4.0 License.

Since the server of http://staff.ustc.edu.cn/~rliu/qfactor.html will stop, those codes will be updated on this site from July 2022.

A GPU version is also provided https://github.com/peijin94/FastQSL.


Dependencies

For *.pro

  • IDL https://www.nv5geospatialsoftware.com/Products/IDL or
  • GDL https://gnudatalanguage.github.io
    • note: setting an environmental variable of GDL_PATH is necessary for write_png. If you used one of the binary packages available for Linux, then it depends on the distribution:
      -Ubuntu & Fedora: /usr/share/gnudatalanguage/lib
      -ArchLinux: /usr/lib/gdl
      -Gentoo: /usr/local/share/gdl
      -MacOS: /opt/local/share/gnudatalanguage/lib
      Please append such line to ~/.bashrc (e.g. for Ubuntu)
      export GDL_PATH=/usr/share/gnudatalanguage/lib

For *.f90

Usage

Please see the beginning of qfactor.pro

  • Demos (the compilation described at the beginning of qfactor.pro should be done first):
IDL> .r demo_charge4.pro

Cite as

@ARTICLE{2022ApJ...937...26Z,
       author = {{Zhang}, PeiJin and {Chen}, Jun and {Liu}, Rui and {Wang}, ChuanBing},
        title = "{FastQSL: A Fast Computation Method for Quasi-separatrix Layers}",
      journal = {\apj},
     keywords = {Solar magnetic fields, GPU computing, 1503, 1969},
         year = 2022,
        month = sep,
       volume = {937},
       number = {1},
          eid = {26},
        pages = {26},
          doi = {10.3847/1538-4357/ac8d61},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...937...26Z},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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