MOCCT: A numerical technique for astrophysical MHD
- 2 August 1995
- journal article
- Published by Elsevier in Computer Physics Communications
- Vol. 89 (1-3) , 127-148
- https://doi.org/10.1016/0010-4655(95)00190-q
Abstract
No abstract availableKeywords
This publication has 32 references indexed in Scilit:
- The Piecewise Parabolic Method (PPM) for gas-dynamical simulationsPublished by Elsevier ,2004
- Extension of the Piecewise Parabolic Method to Multidimensional Ideal MagnetohydrodynamicsJournal of Computational Physics, 1994
- An Approximate Riemann Solver for Ideal MagnetohydrodynamicsJournal of Computational Physics, 1994
- A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolutionThe Astrophysical Journal, 1991
- A Powerful Local Shear Instability in Weakly Magnetized Disks. II. Nonlinear EvolutionThe Astrophysical Journal, 1991
- Simulation of magnetohydrodynamic flows - A constrained transport methodThe Astrophysical Journal, 1988
- An upwind differencing scheme for the equations of ideal magnetohydrodynamicsJournal of Computational Physics, 1988
- The solar wind‐magnetosphere‐ionosphere current‐voltage relationshipGeophysical Research Letters, 1987
- The Effect of Nonzero ∇ · B on the numerical solution of the magnetohydrodynamic equationsJournal of Computational Physics, 1980
- Strang-Type Difference Schemes for Multidimensional ProblemsSIAM Journal on Numerical Analysis, 1972