Rarefaction Shocks, Shock Errors and Low Order of Accuracy in ZEUS
arXiv:astro-ph/0207419 · doi:10.1086/344336
Abstract
We show that there are simple one dimensional problems for which the MHD code, ZEUS, generates significant errors, whereas upwind conservative schemes perform very well on these problems.
11 pages, accepted in ApJ Letters
Cited by in corpus (29)
- PLUTO: a Numerical Code for Computational Astrophysics
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- A High Order Godunov Scheme with Constrained Transport and Adaptive Mesh Refinement for Astrophysical MHD
- Simulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP
- Second Order Accurate Schemes for Magnetohydrodynamics With Divergence-Free Reconstruction
- Simulating the formation of molecular clouds. I. Slow formation by gravitational collapse from static initial conditions
- Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: II. The Effects of Field-Aligned Rotation
- MHD simulations of the magnetorotational instability in a shearing box with zero net flux. I. The issue of convergence
- Simulating Magnetohydrodynamical Flow with Constrained Transport and Adaptive Mesh Refinement; Algorithms & Tests of the AstroBEAR Code
- Magnetohydrodynamic Simulations of Shock Interactions with Radiative Clouds
- A divergence-free semi-implicit finite volume scheme for ideal, viscous and resistive magnetohydrodynamics
- A pseudo-planar, periodic-box formalism for modelling the outer evolution of structure in spherically expanding stellar winds
- MHD simulations of the magnetorotational instability in a shearing box with zero net flux: the case Pm=4
- Three-Dimensional Simulations of Magnetized Superbubbles: New Insights into the Importance of MHD Effects on Observed Quantities
- The Interaction of Asymptotic Giant Branch Stars with the Interstellar Medium
- Local Turbulence Simulations for the Multiphase ISM
- A high-order Godunov scheme for global 3D MHD accretion disks simulations. I. The linear growth regime of the magneto-rotational instability
- Exact shering box solutions of MHD flows with resistivity, viscosity and cooling
- A novel structure preserving semi-implicit finite volume method for viscous and resistive magnetohydrodynamics
- A new thermodynamically compatible finite volume scheme for magnetohydrodynamics
- Simulations of Evolving or Outbursting Molecular Protostellar Jets
- Molecular Clouds as Ensembles of Transient Cores
- A well-balanced and exactly divergence-free staggered semi-implicit hybrid finite volume/finite element scheme for the incompressible MHD equations
- Phurbas: An Adaptive, Lagrangian, Meshless, Magnetohydrodynamics Code. II. Implementation and Tests
- AZEuS: An Adaptive Zone Eulerian Scheme for Computational MHD
- Mass loss and magnetospheres of massive stars
- Multidimensional upwind hydrodynamics on unstructured meshes using Graphics Processing Units I. Two-dimensional uniform meshes
- Initial Ionization of Compressible Turbulence
- Numerical Methods for Simulating Star Formation