Effects of mesh topology on MHD solution features in coronal simulations

Effects of mesh topology on MHD solution features in coronal simulations

Magnetohydrodynamic (MHD) simulations of the solar corona have become more popular with the increased availability of computational power. Modern computational plasma codes, relying upon computational fluid dynamics (CFD) methods, allow the coronal features to be resolved using solar surface magneto...

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Bibliographic Details
Main Authors: Brchnelova, M. (Author), Lani, A. (Author), Leitner, P. (Author), Perri, B. (Author), Poedts, S. (Author), Zhang, F. (Author)
Format: Article
Language:English
Published: Cambridge University Press 2022
Subjects:
Astrophysical plasma
astrophysical plasmas
Computational fluid dynamics
Computational fluid dynamics methods
Computational power
Economic and social effects
Geodesy
Magnetograms
Magnetohydrodynamic simulations
Magnetohydrodynamics
Magnetoplasma
Mesh generation
Mesh topologies
Plasma diagnostics
plasma dynamics
Plasma dynamics
plasma simulation
Plasma simulation
Plasma-Simulation
Simulation platform
Solar corona
Solar surfaces
Topology
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