Magnetohydrodynamic Modeling of the Solar Corona with an Effective Implicit Strategy

نویسندگان

چکیده

Abstract In this paper, we design an effective and robust model to solve the 3D single-fluid solar wind plasma magnetohydrodynamics (MHD) problem of low β . This MHD is formulated on a six-component composite grid system free polar singularities. The computational domain ranges from surface super-Alfvénic region. As common all codes, code must handle physical positivity-preserving property, time-step enlargement, magnetic field divergence-free maintenance. To maintain positivity, employ Harten–Lax–van Leer Riemann solver take self-adjusting method for variable reconstruction. loosen limitation, resort implicit lower–upper symmetric Gauss–Seidel keep sparse Jacobian matrix diagonally dominant improve convergence rate. deal with constant theme that divergence-free, adopt globally solenoidality-preserving approach. After establishing model, use its explicit versions numerically investigate steady-state in Carrington rotations (CRs) 2172 2210. Both simulations achieve almost same results two CRs are basically consistent coronal observations mapped situ interplanetary measurements. Furthermore, conduct ad hoc simulation by multiplying initial CR factor 6. shows can robustly efficiently as about 5 × 10 −7 Therefore, established very promising simulating complex strong environments.

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ژورنال

عنوان ژورنال: Astrophysical Journal Supplement Series

سال: 2021

ISSN: ['1538-4365', '0067-0049']

DOI: https://doi.org/10.3847/1538-4365/ac1f8b