International audienceA description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code for ideal magnetohydrodynamics. The code provides several high-resolution shock-capturing schemes which are constructed to maintain conserved quantities of the flow in a finite-volume sense. Divergence-free magnetic field topologies are maintained to machine precision by collating the components of the magnetic field on a cell-interface staggered grid and utilizing the constrained transport approach for integrating the induction equations. The maintenance of magnetic field topologies on adaptive grids is achieved using prolongation and restriction operators which preserve the divergence and curl of the magnetic field acr...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
International audienceA description is given of the algorithms implemented in the AstroBEAR adaptive...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
We present the implementation of a three-dimensional, second-order accurate Godunov-type algorithm f...
We present a constrained transport (CT) algorithm for solving the 3D ideal magnetohydrodynamic (MHD)...
This paper presents an adaptive moving mesh algorithm for two-dimensional (2D) ideal magnetohydrodyn...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
International audienceAims. In this paper, we present a new method to perform numerical simulations ...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
We present the implementation of a three-dimensional, second order accurate Godunov-type algorithm f...
Aims. In this paper, we present a new method to perform numerical simulations of astrophysical MHD ...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
International audienceA description is given of the algorithms implemented in the AstroBEAR adaptive...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
We present the implementation of a three-dimensional, second-order accurate Godunov-type algorithm f...
We present a constrained transport (CT) algorithm for solving the 3D ideal magnetohydrodynamic (MHD)...
This paper presents an adaptive moving mesh algorithm for two-dimensional (2D) ideal magnetohydrodyn...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
International audienceAims. In this paper, we present a new method to perform numerical simulations ...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
We present the implementation of a three-dimensional, second order accurate Godunov-type algorithm f...
Aims. In this paper, we present a new method to perform numerical simulations of astrophysical MHD ...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...