EFFICIENT COMPUTATION OF MAGNETO-HYDRODYNAMIC PHENOMENA IN ASTROPHYSICS BY CCUP-MOCCT METHOD

DOI10.1142/S021987620400006XzbMath1089.76047OpenAlexW2135863789MaRDI QIDQ5695029

Youichi Ogata, Takahiro Kudoh, Kazunari Shibata, Takashi Yabe

Publication date: 11 October 2005

Published in: International Journal of Computational Methods (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s021987620400006x

zbMATH Keywords

Poisson equationParker instability

Mathematics Subject Classification ID

Cites Work

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• MOCCT: A numerical technique for astrophysical MHD
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• Shock capturing with improved numerical viscosity in primitive Euler representation
• Towards the ultimate conservative difference scheme. V. A second-order sequel to Godunov's method
• A Method for the Numerical Calculation of Hydrodynamic Shocks
• The constrained interpolation profile method for multiphase analysis.
• Exactly conservative semi-Lagrangian scheme for multi-dimensional hyperbolic equations with directional splitting technique

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