MOCCT: A numerical technique for astrophysical MHD

DOI10.1016/0010-4655(95)00190-QzbMath0923.76152OpenAlexW2060791159MaRDI QIDQ1378224

James M. Stone, John F. Hawley

Publication date: 8 February 1998

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0010-4655(95)00190-q

zbMATH Keywords

Lorentz forceelectromagnetic forcesAlfvén characteristicstime-explicit operator split nonconservative technique

Mathematics Subject Classification ID

Finite difference methods applied to problems in fluid mechanics (76M20) Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items

A constrained transport divergence-free finite element method for incompressible MHD equations, Hybrid DG/FV schemes for magnetohydrodynamics and relativistic hydrodynamics, Divergence-free magnetohydrodynamics on conformally moving, adaptive meshes using a vector potential method, A \(4^{\mathrm{th}}\)-order accurate finite volume method for ideal classical and special relativistic MHD based on pointwise reconstructions, EFFICIENT COMPUTATION OF MAGNETO-HYDRODYNAMIC PHENOMENA IN ASTROPHYSICS BY CCUP-MOCCT METHOD, General relativistic MHD simulations of black hole accretion disks and jets, Implementation of the CIP algorithm to magnetohydrodynamic simulations, Disk planet interactions and early evolution in young planetary systems, The ZEUS code for astrophysical magnetohydrodynamics: New extensions and applications, MOCCT, Meshless methods for magnetohydrodynamics with vector potential

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