The space-time CE/SE method for solving one-dimensional special relativistic magnetohydrodynamics equations
From MaRDI portal
Publication:743354
DOI10.1016/j.cpc.2012.11.020zbMath1296.76184OpenAlexW2048937797MaRDI QIDQ743354
Publication date: 24 September 2014
Published in: Computer Physics Communications (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/j.cpc.2012.11.020
discontinuous solutionshyperbolic systemCE/SE methodspecial relativistic magnetohydrodynamics equations
Lua error in Module:PublicationMSCList at line 37: attempt to index local 'msc_result' (a nil value).
Cites Work
- Unnamed Item
- Unnamed Item
- Flux-corrected transport techniques for multidimensional compressible magnetohydrodynamics
- Non-oscillatory central differencing for hyperbolic conservation laws
- On the application of a variant CE/SE method for solving two-dimensional ideal MHD equations
- New algorithms for ultra-relativistic numerical hydrodynamics
- A high-order kinetic flux-splitting method for the relativistic magnetohydrodynamics
- Kinetic schemes for the ultra-relativistic Euler equations.
- The method of space-time conservation element and solution element -- a new approach for solving the Navier-Stokes and Euler equations
- Extension of the piecewise parabolic method to one-dimensional relativistic hydrodynamics
- Capturing shock reflections: An improved flux formula
- The space-time conservation element and solution element method: A new high-resolution and genuinely multidimensional paradigm for solving conservation laws
- Solving the Euler and Navier-Stokes equations by the AMR-CESE method
- Application of space-time CE/SE method to shallow water magnetohydrodynamic equations
- A BGK-Type Flux-Vector Splitting Scheme for the Ultrarelativistic Euler Equations
- An efficient shock-capturing central-type scheme for multidimensional relativistic flows
- Relativistic Fluids and Magneto-fluids
- An efficient shock-capturing central-type scheme for multidimensional relativistic flows
- Numerical hydrodynamics in special relativity
- Application of the space-time conservation element and solution element method to one-dimensional convection-diffusion problems
- Divergence-free adaptive mesh refinement for magnetohydrodynamics.
- A space-time conservation element and solution element method for solving the two- and three-dimensional unsteady Euler equations using quadilateral and hexahedral meshes.
This page was built for publication: The space-time CE/SE method for solving one-dimensional special relativistic magnetohydrodynamics equations