The primary objective of this project is to develop an advanced algorithm for parallel supercomputers to model time-dependent magnetohydrodynamics (MHD) in all three dimensions. This will provide a valuable tool for the design and testing of plasma related technologies that are important to the Air Force and industry. Implementing the algorithm on parallel supercomputers will allow the detailed modeling of realistic plasmas in complex three-dimensional geometries. We have developed a time-dependent, two-dimensional, arbitrary-geometry version of the algorithm, placed it into a testbed code, added the modifications necessary for viscous and resistive effects, and tested the code against known analytical problems. We have implemented the algo...
We developed a data parallel code written in High Performance Fortran for simulating magnetized flui...
Magnetohydrodynamics (MHD) is the study of flow under the effects of an electromagnetic field. MHD a...
Context. The numerical simulation of turbulence and flows in almost ideal astrophysical plasmas with...
The equations of magnetohydrodynamics (MHD) are discussed in the framework of parallel computing. Bo...
A three-dimensional MHD solver is described in the paper. The solver simulates reacting flows with n...
The set of eight nonlinear partial differential equations of magnetohydrodynamics (MHD) is used for ...
The impressive progress of the kinetic schemes in the solution of gas dynamics problems and the deve...
The impressive progress of the kinetic consistent schemes in the solution of the gas dynamics probl...
We present GRADSPMHD, a completely Lagrangian parallel magnetohydrodynamics code based on the SPH fo...
© 1994, Springer Verlag. All rights reserved. The equations of magnetohydrodynamics (MHD) describe t...
Numerical calculations have had an important role in fusion research since its beginning, but the ap...
The impressive progress of the kinetic schemes in the solution of gas dy- namics problems and th...
This is the final report of our NASA AISRP grant entitled 'High Performance Parallel Methods for Spa...
Extended magnetohydrodynamic (MHD) codes are used to model the large, slow-growing instabilities tha...
We report progress for the development of MH4D for the first and second quarters of FY2004, December...
We developed a data parallel code written in High Performance Fortran for simulating magnetized flui...
Magnetohydrodynamics (MHD) is the study of flow under the effects of an electromagnetic field. MHD a...
Context. The numerical simulation of turbulence and flows in almost ideal astrophysical plasmas with...
The equations of magnetohydrodynamics (MHD) are discussed in the framework of parallel computing. Bo...
A three-dimensional MHD solver is described in the paper. The solver simulates reacting flows with n...
The set of eight nonlinear partial differential equations of magnetohydrodynamics (MHD) is used for ...
The impressive progress of the kinetic schemes in the solution of gas dynamics problems and the deve...
The impressive progress of the kinetic consistent schemes in the solution of the gas dynamics probl...
We present GRADSPMHD, a completely Lagrangian parallel magnetohydrodynamics code based on the SPH fo...
© 1994, Springer Verlag. All rights reserved. The equations of magnetohydrodynamics (MHD) describe t...
Numerical calculations have had an important role in fusion research since its beginning, but the ap...
The impressive progress of the kinetic schemes in the solution of gas dy- namics problems and th...
This is the final report of our NASA AISRP grant entitled 'High Performance Parallel Methods for Spa...
Extended magnetohydrodynamic (MHD) codes are used to model the large, slow-growing instabilities tha...
We report progress for the development of MH4D for the first and second quarters of FY2004, December...
We developed a data parallel code written in High Performance Fortran for simulating magnetized flui...
Magnetohydrodynamics (MHD) is the study of flow under the effects of an electromagnetic field. MHD a...
Context. The numerical simulation of turbulence and flows in almost ideal astrophysical plasmas with...