Plasma disturbances affect satellites and spacecraft and can cause serious problems to telecommunications and sensitive sensor systems on Earth. Considering the huge scale of the plasma phenomena, data collection at individual locations is not sufficient to cover this entire relevant environment. Therefore, computational plasma modelling has become a significant issue for space sciences, particularly for the near-Earth magnetosphere. However, the simulations of these disturbances present many physical as well as numerical and computational challenges. In this work, we discuss our recent magnetohydrodynamic solver, realised within the MPI-parallel AMROC (Adaptive Mesh Refinement in Object-oriented C++) framework, in which particular physical...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/77232/1/AIAA-1999-3273-200.pd
In this thesis, we develop an adaptive mesh refinement (AMR) code including magnetic fields, and use...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
Computational magneto-hydrodynamics (MHD) for space physics has become an essential area in understa...
We present an adaptive parallel solver for the numerical simulation of ideal magnetohydrodynamics in...
Abstract—A 3-D parallel adaptive mesh refinement (AMR) scheme is described for solving the partial-d...
The interaction between magnetized space plasmas and obstacles like comets, asteroids or planets is ...
MPI-AMRVAC version 2.0 is an open-source framework for parallel, grid-adaptive simulations of hydrod...
Techniques that have become common in aerodynamics codes have recently begun to be implemented in sp...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
A parallel adaptive mesh refinement (AMR) scheme is described for solving the governing equations of...
International audienceWe report our implementation of the magneto-frictional method in the Message P...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
Relativistic hydro and magnetohydrodynamics provide continuum fluid descriptions for gas and plasma ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/77232/1/AIAA-1999-3273-200.pd
In this thesis, we develop an adaptive mesh refinement (AMR) code including magnetic fields, and use...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
Computational magneto-hydrodynamics (MHD) for space physics has become an essential area in understa...
We present an adaptive parallel solver for the numerical simulation of ideal magnetohydrodynamics in...
Abstract—A 3-D parallel adaptive mesh refinement (AMR) scheme is described for solving the partial-d...
The interaction between magnetized space plasmas and obstacles like comets, asteroids or planets is ...
MPI-AMRVAC version 2.0 is an open-source framework for parallel, grid-adaptive simulations of hydrod...
Techniques that have become common in aerodynamics codes have recently begun to be implemented in sp...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
A parallel adaptive mesh refinement (AMR) scheme is described for solving the governing equations of...
International audienceWe report our implementation of the magneto-frictional method in the Message P...
ARMS is a robust code for solving the single-fluid, fully compressible equations of magnetohydrodyna...
Relativistic hydro and magnetohydrodynamics provide continuum fluid descriptions for gas and plasma ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/77232/1/AIAA-1999-3273-200.pd
In this thesis, we develop an adaptive mesh refinement (AMR) code including magnetic fields, and use...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...