2025/09/17 by Zhenhua Liu, Liu, Zhenhua, Chaowei Jiang +1
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #FOS: Physical sciences #Geomagnetism and Paleomagnetism Studies #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #Solar and Stellar Astrophysics (astro-ph.SR)
paper · pdf · doi:10.48550/arxiv.2509.13811
openalex publication_date 2025/09/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Magnetic field extrapolation from the solar photosphere to the corona plays an important role in solar physics research. In this work, we present a fully-implicit viscous-relaxation nonlinear force-free field (FIVR-NLFFF) extrapolation code based on a viscous magnetohydrodynamic relaxation model. The method solves the magnetic induction equation alongside a simplified momentum equation, which assumes a balance between the Lorentz force and the viscous force. Under this assumption, the velocity field driving the magnetic field evolution is determined instantaneously by the Lorentz force distribution. Through viscous dissipation, the system relaxes toward a minimum-energy state, consistent with the vector magnetogram prescribed at the lower boundary. To enhance numerical stability, we adopt a fully implicit time integration scheme and employ central finite differences for spatial discretization. The resulting system of nonlinear algebraic equations is solved using the Jacobian-free Newton-Krylov method, as implemented in the Portable, Extensible Toolkit for Scientific Computation (PETSc). We validate the code using three benchmark models: the Low and Lou force-free solution, the Titov-Démoulin magnetic flux rope model, and a strongly sheared arcade configuration containing a current sheet. Quantitative comparisons demonstrate good agreement with the reference solutions. Notably, the code's ability to handle discontinuities and reconstruct coronal current sheets makes it a promising tool for studying magnetic fields that may directly trigger solar eruptions.