Implementation of thermal conduction energy transfer models in the Bifrost Solar atmosphere MHD code
George Cherry, Boris Gudiksen, Mikolaj Szydlarski

TL;DR
This paper evaluates various numerical methods for modeling thermal conduction in the solar atmosphere within the Bifrost MHD code, highlighting their accuracy, efficiency, and limitations to guide future simulations.
Contribution
It provides a comprehensive comparison of explicit, implicit, and hyperbolic methods for thermal conduction modeling in solar atmosphere simulations, including new analytical benchmarks.
Findings
Hyperbolic approximation is most accurate and fastest for long simulations.
No single method is optimal for all accuracy and efficiency needs.
Hyper-diffusivity improves method performance and convergence.
Abstract
Context: Thermal conductivity provides important contributions to the energy evolution of the upper solar atmosphere, behaving as a non-linear concentration-dependent diffusion equation. Recently, different methods have been offered as best-fit solutions to these problems in specific situations, but their effectiveness and limitations are rarely discussed. Aims. We rigorously test the different implementations of solving the conductivity flux, in the massively-parallel magnetohydrodynamics code, Bifrost, with the aim of specifying the best scenarios for the use of each method. Methods: We compare the differences and limitations of explicit versus implicit methods, and analyse the convergence of a hyperbolic approximation. Among the tests, we use a newly derived 1st-order self-similar approximation to compare the efficacy of each method analytically in a 1D pure-thermal test scenario.…
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Taxonomy
TopicsSpacecraft and Cryogenic Technologies · Solar and Space Plasma Dynamics · Geophysics and Gravity Measurements
