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Application of a Low-dissipation HLLD Approximate Riemann Solver to Solar Wind Simulations

We investigate the steady-state solar wind in spherical coordinates using a low-dissipation Harten–Lax–van Leer-Discontinuities Riemann solver, in which the magnetic field is decomposed into an initial potential field B _0 and a time-dependent part B _1 . A constrained transport method is employed t...

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Bibliográfalaš dieđut
Váldodahkkit: Caixia Li, Zhenning Shen, Man Zhang, Xueshang Feng
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2025-01-01
Ráidu:The Astrophysical Journal
Fáttát:
Liŋkkat:https://doi.org/10.3847/1538-4357/add018
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