AbstractA brief review of the numerical methods implemented in the widely used ZEUS code for astrophysical magnetohydrodynamics (MHD) is given. Extensions of the numerical methods to treat problems in nonideal MHD in a variety of regimes are discussed. In particular, methods for treating Ohmic dissipation, and methods for studying partially ionized plasmas in which the ion and neutral components are weakly coupled through a collisional drag term are considered. Recent application of the methods to the study of the dynamics of accretion disks is described
The large-scale dynamics of plasma flows can often be described within a fluidistic approximation kn...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
We assess the suitability of various numerical MHD algorithms for astrophysical accretion disk simu...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
We describe numerical methods for solving the equations of radiation magnetohydrodynamics (MHD) for ...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
We present a multidimensional numerical code to solve isothermal magnetohydrodynamic (IMHD) equation...
Due to the prevalence of magnetic fields in astrophysical environments, magnetohydrodynamic (MHD) si...
With ninety per cent of visible matter in the universe existing in the plasma state, an understandin...
With ninety per cent of visible matter in the universe existing in the plasma state, an understandin...
In certain astrophysical systems, the commonly employed ideal magnetohydrodynamics (MHD) approximati...
In this era of precision cosmology, a detailed physical understanding on the evolution of cosmic bar...
This thesis presents an algorithm for simulating the equations of ideal magnetohydrodynamics and oth...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
The large-scale dynamics of plasma flows can often be described within a fluidistic approximation kn...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
We assess the suitability of various numerical MHD algorithms for astrophysical accretion disk simu...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
We describe numerical methods for solving the equations of radiation magnetohydrodynamics (MHD) for ...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
We present a multidimensional numerical code to solve isothermal magnetohydrodynamic (IMHD) equation...
Due to the prevalence of magnetic fields in astrophysical environments, magnetohydrodynamic (MHD) si...
With ninety per cent of visible matter in the universe existing in the plasma state, an understandin...
With ninety per cent of visible matter in the universe existing in the plasma state, an understandin...
In certain astrophysical systems, the commonly employed ideal magnetohydrodynamics (MHD) approximati...
In this era of precision cosmology, a detailed physical understanding on the evolution of cosmic bar...
This thesis presents an algorithm for simulating the equations of ideal magnetohydrodynamics and oth...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
The large-scale dynamics of plasma flows can often be described within a fluidistic approximation kn...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
We assess the suitability of various numerical MHD algorithms for astrophysical accretion disk simu...