International audienceThe dynamics of long oblique MHD waves in a collisionless plasma permeated by a uniform magnetic field is addressed using a Landau-fluid model that includes Hall effect and electron-pressure gradient in a generalized Ohm's law and retains ion finite Larmor radius (FLR) corrections to the gyrotropic pressure (Phys. Plasmas 10, 3906, 2003). This one-fluid model, built to reproduce the weakly nonlinear dynamics of long dispersive Alfvén waves propagating along an ambient field, is shown to correctly capture the Landau damping of oblique magnetosonic waves predicted by a kinetic theory based on the Vlasov-Maxwell system. For oblique and kinetic Alfvén waves (for which second order FLR corrections are to be retained), the l...
International audienceThe present work examines the effects arising from the nonlinear Landau dampin...
The linear wave equation (sixth order in space and time) and the corresponding dispersion relation...
The linear wave equation (sixth order in space and time) and the corresponding dispersion relation...
International audienceA dispersive Landau-fluid model is used to study the decay and modulational in...
A dispersive Landau-fluid model is used to study the decay and modulational instabilities of circula...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
The damping phenomenon is studied due to the collisions of ions and neutral particles and Landau app...
In order to describe correctly the heating rate of the interstellar medium by plasma wave energy los...
In order to describe correctly the heating rate of the interstellar medium by plasma wave energy los...
International audienceWe review the basic approximations underlying magnetohydrodynamic (MHD) theory...
The limitations of Hall MHD as a model for turbulence in weakly collisional plasmas are explored usi...
Aims. In the approximation of linear dissipative magnetohydrodynamics (MHD), it can be shown that dr...
International audienceThe present work examines the effects arising from the nonlinear Landau dampin...
The linear wave equation (sixth order in space and time) and the corresponding dispersion relation...
The linear wave equation (sixth order in space and time) and the corresponding dispersion relation...
International audienceA dispersive Landau-fluid model is used to study the decay and modulational in...
A dispersive Landau-fluid model is used to study the decay and modulational instabilities of circula...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
International audienceReduced models are derived for a strongly magnetized collisionless plasma at s...
The damping phenomenon is studied due to the collisions of ions and neutral particles and Landau app...
In order to describe correctly the heating rate of the interstellar medium by plasma wave energy los...
In order to describe correctly the heating rate of the interstellar medium by plasma wave energy los...
International audienceWe review the basic approximations underlying magnetohydrodynamic (MHD) theory...
The limitations of Hall MHD as a model for turbulence in weakly collisional plasmas are explored usi...
Aims. In the approximation of linear dissipative magnetohydrodynamics (MHD), it can be shown that dr...
International audienceThe present work examines the effects arising from the nonlinear Landau dampin...
The linear wave equation (sixth order in space and time) and the corresponding dispersion relation...
The linear wave equation (sixth order in space and time) and the corresponding dispersion relation...