Add to ORKGThis report consists of two published papers, 'Computation of Magnetohydrodynamic Flows Using an Iterative PNS Algorithm' and 'Numerical Simulation of Turbulent MHD Flows Using an Iterative PNS Algorithm'
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
Numerical simulation for astrophysics phe-nomena has become popular and important in the last decade...
We compare the performances of a pseudospectral and a finite-volume method for the simulation of mag...
A new parabolized Navier-Stokes (PNS) algorithm has been developed to efficiently compute magnetohyd...
Magnetohydrodynamics (MHD) is the study of flow under the effects of an electromagnetic field. MHD a...
This final report summarizes the research accomplished under NASA-Ames Cooperative Agreement NCC2-55...
A general tool for solving MHD and hydrodynamical problems typical of astrophysical applications is ...
The 3-D supersonic viscous flow in an experimental MHD channel has been numerically simulated. The e...
A new forward-backward sweeping parabolized Navier-Stokes algorithm has been developed to efficientl...
The Parabolized Navier-Stokes (PNS) equations form a subset of the Navier-Stokes equations . This re...
The 3-D nonequilibrium seeded air flow in the NASA-Ames experimental MHD channel has been numericall...
The set of eight nonlinear partial differential equations of magnetohydrodynamics (MHD) is used for ...
The capability of computational fluid dynamics (CFD) analysis to predict complex flowfields has been...
AbstractModels for three interesting magnetohydrodynamic (MHD) flows have been considered, whereby p...
The large-scale dynamics of plasma flows can often be described within a fluidistic approximation kn...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
Numerical simulation for astrophysics phe-nomena has become popular and important in the last decade...
We compare the performances of a pseudospectral and a finite-volume method for the simulation of mag...
A new parabolized Navier-Stokes (PNS) algorithm has been developed to efficiently compute magnetohyd...
Magnetohydrodynamics (MHD) is the study of flow under the effects of an electromagnetic field. MHD a...
This final report summarizes the research accomplished under NASA-Ames Cooperative Agreement NCC2-55...
A general tool for solving MHD and hydrodynamical problems typical of astrophysical applications is ...
The 3-D supersonic viscous flow in an experimental MHD channel has been numerically simulated. The e...
A new forward-backward sweeping parabolized Navier-Stokes algorithm has been developed to efficientl...
The Parabolized Navier-Stokes (PNS) equations form a subset of the Navier-Stokes equations . This re...
The 3-D nonequilibrium seeded air flow in the NASA-Ames experimental MHD channel has been numericall...
The set of eight nonlinear partial differential equations of magnetohydrodynamics (MHD) is used for ...
The capability of computational fluid dynamics (CFD) analysis to predict complex flowfields has been...
AbstractModels for three interesting magnetohydrodynamic (MHD) flows have been considered, whereby p...
The large-scale dynamics of plasma flows can often be described within a fluidistic approximation kn...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
Numerical simulation for astrophysics phe-nomena has become popular and important in the last decade...
We compare the performances of a pseudospectral and a finite-volume method for the simulation of mag...