Two variants of the advection upstream splitting method are modified to solve the equations of ideal magnetohydrodynamics. Discontinuity-sensing functions used in AUSMPW and M-AUSMPW for the magnetohydrodynamics equations are newly defined in consideration of a magnetic field. The new pressure-based weight functions are shown to effectively remove the oscillations behind a strong shock wave as well as provide a highly accurate solution for a stationary contact discontinuity. To satisfy the divergence-free constraint of a magnetic field, the hyperbolic divergence cleaning method is chosen and applied for all the test cases. Ryu and Jones onedimensional magnetohydrodynamics shock-tube problem and Orszag and Tangs two-dimensional magne...
In order to overcome some difficulties observed in the computation of hypersonic flows, a robust, ac...
A shock capturing strategy for high-order accurate Discontinuous Galerkin (DG) approximations of the...
A description is given for preserving del . B = 0 in a magnetohydrodynamic (MHD) code that employs t...
This paper presents how the equations of magnetohydrodynamics (MHD) in primitive form should be writ...
This paper presents an adaptive moving mesh algorithm for two-dimensional (2D) ideal magnetohydrodyn...
Artículo de publicación ISIIn this paper we explore flux vector splittings for the MHD system of equ...
In this article we propose different splitting procedures for the transient incompressible MHD syste...
During the simulations of the magnetohydrodynamic equations, numerical errors might cause the format...
We propose and analyze an effective decoupling algorithm for unsteady thermally coupled magneto-hydr...
We modify an existing magnetohydrodynamics algorithm to make it more compatible with a dimensionally...
We describe a high-order numerical magnetohydrodynamics (MHD) solver built upon a novel non-linear e...
The ideal MagnetoHydroDynamic (MHD) equations accurately describe the macroscopic dynamics of a perf...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
In simulations of magnetohydrodynamic (MHD) processes the violation of the divergence constraint cau...
A description is given for preserving ${\bmsy\nabla}\cdot{\vec B}=0$ in a magnetohydrodynamic (MHD) ...
In order to overcome some difficulties observed in the computation of hypersonic flows, a robust, ac...
A shock capturing strategy for high-order accurate Discontinuous Galerkin (DG) approximations of the...
A description is given for preserving del . B = 0 in a magnetohydrodynamic (MHD) code that employs t...
This paper presents how the equations of magnetohydrodynamics (MHD) in primitive form should be writ...
This paper presents an adaptive moving mesh algorithm for two-dimensional (2D) ideal magnetohydrodyn...
Artículo de publicación ISIIn this paper we explore flux vector splittings for the MHD system of equ...
In this article we propose different splitting procedures for the transient incompressible MHD syste...
During the simulations of the magnetohydrodynamic equations, numerical errors might cause the format...
We propose and analyze an effective decoupling algorithm for unsteady thermally coupled magneto-hydr...
We modify an existing magnetohydrodynamics algorithm to make it more compatible with a dimensionally...
We describe a high-order numerical magnetohydrodynamics (MHD) solver built upon a novel non-linear e...
The ideal MagnetoHydroDynamic (MHD) equations accurately describe the macroscopic dynamics of a perf...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
In simulations of magnetohydrodynamic (MHD) processes the violation of the divergence constraint cau...
A description is given for preserving ${\bmsy\nabla}\cdot{\vec B}=0$ in a magnetohydrodynamic (MHD) ...
In order to overcome some difficulties observed in the computation of hypersonic flows, a robust, ac...
A shock capturing strategy for high-order accurate Discontinuous Galerkin (DG) approximations of the...
A description is given for preserving del . B = 0 in a magnetohydrodynamic (MHD) code that employs t...