English

FastQSL: A Fast Computation Method for Quasi-separatrix Layers

Solar and Stellar Astrophysics 2022-09-28 v4 Instrumentation and Methods for Astrophysics

Abstract

Magnetic reconnection preferentially takes place at the intersection of two separatrices or two quasi-separatrix layers, which can be quantified by the squashing factor Q, whose calculation is computationally expensive due to the need to trace as many field lines as possible. We developed a method (FastQSL) optimized for obtaining Q and the twist number in a 3D data cube. FastQSL utilizes the hardware acceleration of the graphic process unit (GPU) and adopts a step-size adaptive scheme for the most computationally intensive part: tracing magnetic field lines. As a result, it achieves a computational efficiency of 4.53 million Q values per second. FastQSL is open source, and user-friendly for data import, export, and visualization.

Keywords

Cite

@article{arxiv.2208.12569,
  title  = {FastQSL: A Fast Computation Method for Quasi-separatrix Layers},
  author = {Peijin Zhang and Jun Chen and Rui Liu and Chuanbing Wang},
  journal= {arXiv preprint arXiv:2208.12569},
  year   = {2022}
}
R2 v1 2026-06-25T01:59:58.541Z