Numerical solution of shallow water magnetohydrodynamic equations with non-flat bottom topography
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Publication:5071751
DOI10.1080/10618562.2014.891019OpenAlexW2028800647MaRDI QIDQ5071751
Munshoor Ahmed, Shamsul Qamar, Saqib Zia
Publication date: 22 April 2022
Published in: International Journal of Computational Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/10618562.2014.891019
conservation lawsprojection methoddiscontinuous solutionskinetic flux vector splitting schemebottom topographycentral-upwind schemeshallow water magnetohydrodynamic equations
Related Items (5)
High-order accurate entropy stable finite difference schemes for the shallow water magnetohydrodynamics ⋮ On the well-posedness of strong solution to ideal magnetohydrodynamic equations ⋮ A new S-M limiter entropy stable scheme based on moving mesh method for ideal MHD and SWMHD equations ⋮ A Well-Balanced FVC Scheme for 2D Shallow Water Flows on Unstructured Triangular Meshes ⋮ Asymptotic shallow models arising in magnetohydrodynamics
Cites Work
- Unnamed Item
- A kinetic flux-vector splitting method for the shallow water magnetohydrodynamics
- A gas-kinetic scheme for shallow-water equations with source terms
- The effect of nonzero \(\bigtriangledown\cdot B\) on the numerical solution of the magnetohydrodynamic equations
- Balancing source terms and flux gradients in high-resolution Godunov methods: The quasi-steady wave-propagation algorithm
- Kinetic flux vector splitting for Euler equations
- The \(\nabla \cdot B=0\) constraint in shock-capturing magnetohydrodynamics codes
- A well-balanced gas-kinetic scheme for the shallow-water equations with source terms
- An evolution Galerkin scheme for the shallow water magnetohydrodynamic equations in two space dimensions
- A high-order kinetic flux-splitting method for the relativistic magnetohydrodynamics
- Gas-kinetic theory-based flux splitting method for ideal magnetohydrodynamics
- A solution-adaptive upwind scheme for ideal magnetohydrodynamics
- Numerical simulation of the MHD equations by a kinetic-type method
- New high-resolution central schemes for nonlinear conservation laws and convection-diffusion equations
- A second-order well-balanced positivity preserving central-upwind scheme for the Saint-Venant system
- High order finite difference WENO schemes with the exact conservation property for the shallow water equations
- Well-balanced finite volume schemes of arbitrary order of accuracy for shallow water flows
- A steady-state capturing method for hyperbolic systems with geometrical source terms
- Adaptive multi-resolution central-upwind schemes for systems of conservation laws
- Non-oscillatory central-upwind scheme for hyperbolic conservation laws
- Rossby waves in “shallow water” magnetohydrodynamics
- Genuinely multidimensional evolution Galerkin schemes for the shallow water equations
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