This paper describes ZEUS-MP, a multi-physics, massively parallel, message- passing implementation of the ZEUS code. ZEUS-MP differs significantly from the ZEUS-2D code, the ZEUS-3D code, and an early "version 1" of ZEUS-MP distributed publicly in 1999. ZEUS-MP offers an MHD algorithm better suited for multidimensional flows than the ZEUS-2D module by virtue of modifications to the Method of Characteristics scheme first suggested by Hawley and Stone (1995), and is shown to compare quite favorably to the TVD scheme described by Ryu et. al (1998). ZEUS-MP is the first publicly-available ZEUS code to allow the advection of multiple chemical (or nuclear) species. Radiation hydrodynamic simulations are enabled via an implicit flux-limited radiat...
The primary objective of this project is to develop an advanced algorithm for parallel supercomputer...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
A number of physics problems can be modeled by a set of N elements, which have pair-wise interaction...
In this, the third of a series of three papers, we conclude a detailed description of ZEUS-2D, a num...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
AbstractWe describe a scalable parallel algorithm for numerical simulations of turbulent, radiative,...
Aims. The transport of energy through radiation is very important in many astrophysical phenomena. I...
We present a numerical algorithm for the incorporation of the active cosmic ray transport into the Z...
Aims. The transport of energy through radiation is very important in many astrophysical ph...
Abstract: The paper presents the new application software (code) MARPLE 3D designed in KIA...
In a Priority Program on Massively Parallel Computing, eight Dutch research groups (http://www.phys....
A number of physics problems can be modeled by a set of N elements, which have pair-wise interaction...
It is now generally agreed that multidimensional, multigroup, radiation hydrodynamics is an indispen...
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
We present a new multi-fluid, grid-based magnetohydrodynamics (MHD) code PIERNIK, which is based on ...
The primary objective of this project is to develop an advanced algorithm for parallel supercomputer...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
A number of physics problems can be modeled by a set of N elements, which have pair-wise interaction...
In this, the third of a series of three papers, we conclude a detailed description of ZEUS-2D, a num...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
AbstractWe describe a scalable parallel algorithm for numerical simulations of turbulent, radiative,...
Aims. The transport of energy through radiation is very important in many astrophysical phenomena. I...
We present a numerical algorithm for the incorporation of the active cosmic ray transport into the Z...
Aims. The transport of energy through radiation is very important in many astrophysical ph...
Abstract: The paper presents the new application software (code) MARPLE 3D designed in KIA...
In a Priority Program on Massively Parallel Computing, eight Dutch research groups (http://www.phys....
A number of physics problems can be modeled by a set of N elements, which have pair-wise interaction...
It is now generally agreed that multidimensional, multigroup, radiation hydrodynamics is an indispen...
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
We present a new multi-fluid, grid-based magnetohydrodynamics (MHD) code PIERNIK, which is based on ...
The primary objective of this project is to develop an advanced algorithm for parallel supercomputer...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
A number of physics problems can be modeled by a set of N elements, which have pair-wise interaction...