A New Code for Nonlinear Force-Free Field Extrapolation of the Global Corona
Chaowei Jiang, Xueshang Feng, and Changqing Xiang

TL;DR
This paper introduces a high-performance, parallelized global NLFFF extrapolation code for the solar corona, utilizing a magnetohydrodynamics relaxation approach and Yin-Yang grid to improve accuracy and efficiency in modeling the coronal magnetic field.
Contribution
It presents a novel parallelized global NLFFF extrapolation code based on MHD relaxation and Yin-Yang grid, suitable for high-resolution full-sphere magnetogram data.
Findings
Code validated with semi-analytic solutions showing high accuracy.
Demonstrates fast convergence and readiness for practical applications.
Potential for integration with adaptive mesh refinement techniques.
Abstract
Reliable measurements of the solar magnetic field are still restricted to the photosphere, and our present knowledge of the three-dimensional coronal magnetic field is largely based on extrapolation from photospheric magnetogram using physical models, e.g., the nonlinear force-free field (NLFFF) model as usually adopted. Most of the currently available NLFFF codes have been developed with computational volume like Cartesian box or spherical wedge while a global full-sphere extrapolation is still under developing. A high-performance global extrapolation code is in particular urgently needed considering that Solar Dynamics Observatory (SDO) can provide full-disk magnetogram with resolution up to . In this work, we present a new parallelized code for global NLFFF extrapolation with the photosphere magnetogram as input. The method is based on magnetohydrodynamics relaxation…
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