International audienceMagneto hydrodynamics is an important tool to study the dynamics of Space Physics. In this context, we introduce a three-dimensional magneto hydrodynamic solver with divergence-cleaning in the adaptive multiresolution CARMEN code. The numerical scheme is based on a finite volume discretization that ensures the conservation of physical quantities. The adaptive multiresolution approach allows for automatic identification of local structures in the numerical solution and thus provides an adaptive mesh refined only in regions where the solution needs more improved resolution. We assess the three dimensional magnetohydrodynamic CARMEN code and compare its results with the ones from the well-known FLASH code
We present the implementation of a three-dimensional, second-order accurate Godunov-type algorithm f...
We present an adaptive parallel solver for the numerical simulation of ideal magnetohydrodynamics in...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
International audienceMagneto hydrodynamics is an important tool to study the dynamics of Space Phys...
We present an adaptive multiresolution method for the numerical simulation of ideal magnetohydrodyna...
International audienceWe present an adaptive multiresolution method for the numerical simulation of ...
We present a new adaptive multiresoltion method for the numerical simulation of ideal magn...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
An adaptive grid technique for use in the solution of multi-dimensional time-dependent PDEs is appli...
An adaptive grid technique for use in the solution of multi-dimensional time-dependent PDEs is appli...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
Abstract—A 3-D parallel adaptive mesh refinement (AMR) scheme is described for solving the partial-d...
International audienceA description is given of the algorithms implemented in the AstroBEAR adaptive...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
Abstract — On this work we present an adaptive bi-dimensional ideal magnetohydrodynamics (MHD) model...
We present the implementation of a three-dimensional, second-order accurate Godunov-type algorithm f...
We present an adaptive parallel solver for the numerical simulation of ideal magnetohydrodynamics in...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
International audienceMagneto hydrodynamics is an important tool to study the dynamics of Space Phys...
We present an adaptive multiresolution method for the numerical simulation of ideal magnetohydrodyna...
International audienceWe present an adaptive multiresolution method for the numerical simulation of ...
We present a new adaptive multiresoltion method for the numerical simulation of ideal magn...
We have developed a modern code to solve the magneto-hydrodynamic (MHD) or hydrodynamic (HD) equatio...
An adaptive grid technique for use in the solution of multi-dimensional time-dependent PDEs is appli...
An adaptive grid technique for use in the solution of multi-dimensional time-dependent PDEs is appli...
A description is given of the algorithms implemented in the AstroBEAR adaptive mesh-refinement code ...
Abstract—A 3-D parallel adaptive mesh refinement (AMR) scheme is described for solving the partial-d...
International audienceA description is given of the algorithms implemented in the AstroBEAR adaptive...
We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for ...
Abstract — On this work we present an adaptive bi-dimensional ideal magnetohydrodynamics (MHD) model...
We present the implementation of a three-dimensional, second-order accurate Godunov-type algorithm f...
We present an adaptive parallel solver for the numerical simulation of ideal magnetohydrodynamics in...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...