Toward a fast and consistent approach to model solar magnetic fields in multiple layers
Xiaoshuai Zhu, Thomas Wiegelmann

TL;DR
This paper introduces a novel combined extrapolation method that efficiently models magnetic fields across multiple layers of the solar atmosphere, improving accuracy over existing methods.
Contribution
The paper presents a new combined magnetohydrostatic and nonlinear force-free field extrapolation approach for multi-layer solar magnetic field modeling, optimized for speed and accuracy.
Findings
The combined method achieves accuracy comparable to MHS extrapolation.
It outperforms NLFFF extrapolation in multi-layer magnetic field reconstruction.
The approach is moderately efficient for high-resolution magnetograms.
Abstract
Aims. We aim to develop a fast and consistent extrapolation method to model multiple layers of the solar atmosphere. Methods. The new approach combines the magnetohydrostatic (MHS) extrapolation which models the solar low atmosphere in a flat box and the nonlinear force-free field (NLFFF) extrapolation which models the solar corona with a chromospheric vector magnetogram deduced from the MHS extrapolation. We test our code with a snapshot of a radiative magnetohydrodynamic simulation of a solar flare. Comparisons are conducted by several metrics quantitatively. Results. Based on a number of test runs, we find out the optimized configuration for the combination of two extrapolations with a 5.8-Mm-high box for the MHS extrapolation and a magnetogram at a height of 1 Mm for the NLFFF extrapolation. The new approach under this configuration is able to reconstruct the magnetic fields in…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Geophysics and Gravity Measurements
