A particular class of exact solutions of the two-dimensional time-dependent magnetohydrodynamic equations for an ideal isothermal plasma is presented. The associated flows have non-vanishing acceleration. A special form of the mapping between Eulerian and Lagrangian coordinates is assumed and the acceleration term has to have the form of a potential force. The class of potentials compatible with these assumptions is derived and the constraints imposed by the vanishing resistivity then lead to a restriction of the admissible flow fields. Some explicit solutions are constructed and their properties are investigated.</p
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
This work describes the theoretical background and the implementation of OpenFOAM solvers suitable f...
© 2018 The Author(s). In certain astrophysical systems, the commonly employed ideal magnetohydrodyna...
It is shown that a special class of time-dependent solutions of the ideal two-dimensional magnetohyd...
A special method is presented to construct exact time-dependent solutions of the two-dimensional ide...
AbstractThe magnetohydrodynamic (or MHD) equations of an incompressible and homogeneous plasma are c...
This is a dissertation on the motion of incompressible charged and non charged particles in a fluid....
This talk presents recent work on the two-dimensional (2D) magnetohydrodynamic (MHD) equations with ...
The plasma flow past a blunt obstacle in an ideal magnetohydrodynamic (MHD) model is studied, taking...
It is shown that the ideal MHD equilibrium states of an axisymmetric plasma with incompressible flow...
SubmittedInternational audienceThe ideal magnetohydrodynamic equations are, roughly speaking, a quas...
The ideal MagnetoHydroDynamic (MHD) equations accurately describe the macroscopic dynamics of a perf...
The techniques developed in Part 1 of the present series are here applied to two-dimensional solutio...
Numerical methods for solving the ideal magnetohydrodynamic (MHD) equa-tions in more than one space ...
AbstractIn analog to the Irvine's tetrads of a rotating reference system, a tetrad field associated ...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
This work describes the theoretical background and the implementation of OpenFOAM solvers suitable f...
© 2018 The Author(s). In certain astrophysical systems, the commonly employed ideal magnetohydrodyna...
It is shown that a special class of time-dependent solutions of the ideal two-dimensional magnetohyd...
A special method is presented to construct exact time-dependent solutions of the two-dimensional ide...
AbstractThe magnetohydrodynamic (or MHD) equations of an incompressible and homogeneous plasma are c...
This is a dissertation on the motion of incompressible charged and non charged particles in a fluid....
This talk presents recent work on the two-dimensional (2D) magnetohydrodynamic (MHD) equations with ...
The plasma flow past a blunt obstacle in an ideal magnetohydrodynamic (MHD) model is studied, taking...
It is shown that the ideal MHD equilibrium states of an axisymmetric plasma with incompressible flow...
SubmittedInternational audienceThe ideal magnetohydrodynamic equations are, roughly speaking, a quas...
The ideal MagnetoHydroDynamic (MHD) equations accurately describe the macroscopic dynamics of a perf...
The techniques developed in Part 1 of the present series are here applied to two-dimensional solutio...
Numerical methods for solving the ideal magnetohydrodynamic (MHD) equa-tions in more than one space ...
AbstractIn analog to the Irvine's tetrads of a rotating reference system, a tetrad field associated ...
In this, the second of a series of three papers, we continue a detailed description of ZEUS-2D, a nu...
This work describes the theoretical background and the implementation of OpenFOAM solvers suitable f...
© 2018 The Author(s). In certain astrophysical systems, the commonly employed ideal magnetohydrodyna...