International audienceA higher-order multiscale analysis of the dissipation range of collisionless plasma turbulence is presented using in situ high-frequency magnetic field measurements from the Cluster spacecraft in a stationary interval of fast ambient solar wind. The observations, spanning five decades in temporal scales, show a crossover from multifractal intermittent turbulence in the inertial range to non-Gaussian monoscaling in the dissipation range. This presents a strong observational constraint on theories of dissipation mechanisms in turbulent collisionless plasmas
In this paper we give a formulation of two-dimensional (2D) collisionless magnetohydrodynamic (MHD) ...
This HDR is devoted to solar wind turbulence from MHD to kinetic plasma scales. Solar wind turbulenc...
International audienceRecent studies of kinetic scales solar wind turbulence have revealed new featu...
International audienceA higher-order multiscale analysis of the dissipation range of collisionless p...
A higher-order multiscale analysis of the dissipation range of collisionless plasma turbulence is pr...
A robust multiscale analysis of high-frequency magnetic field measurements from the Cluster spacecra...
In several different contexts space plasmas display intermittent turbulence at magneto-hydro-dynamic...
The physics of turbulence in incompressible hydrodynamics follows a clear scheme: energy is injected...
International audienceTo investigate the universality of magnetic turbulence in space plasmas, we an...
Many plasmas throughout the Universe undergo complex turbulent dynamics, which transfer energy from ...
International audienceSolar wind is a turbulent magnetized collisionless plasma. Kolmogorov's turbul...
In this paper we give a formulation of two-dimensional (2D) collisionless magnetohydrodynamic (MHD) ...
High resolution kinetic simulations of collisionless plasma driven by shear show the development of ...
International audienceTurbulent spectrum of magnetic fluctuations in the solar wind nearly follows K...
International audienceTurbulent spectra of magnetic fluctuations in the free solar wind are studied ...
In this paper we give a formulation of two-dimensional (2D) collisionless magnetohydrodynamic (MHD) ...
This HDR is devoted to solar wind turbulence from MHD to kinetic plasma scales. Solar wind turbulenc...
International audienceRecent studies of kinetic scales solar wind turbulence have revealed new featu...
International audienceA higher-order multiscale analysis of the dissipation range of collisionless p...
A higher-order multiscale analysis of the dissipation range of collisionless plasma turbulence is pr...
A robust multiscale analysis of high-frequency magnetic field measurements from the Cluster spacecra...
In several different contexts space plasmas display intermittent turbulence at magneto-hydro-dynamic...
The physics of turbulence in incompressible hydrodynamics follows a clear scheme: energy is injected...
International audienceTo investigate the universality of magnetic turbulence in space plasmas, we an...
Many plasmas throughout the Universe undergo complex turbulent dynamics, which transfer energy from ...
International audienceSolar wind is a turbulent magnetized collisionless plasma. Kolmogorov's turbul...
In this paper we give a formulation of two-dimensional (2D) collisionless magnetohydrodynamic (MHD) ...
High resolution kinetic simulations of collisionless plasma driven by shear show the development of ...
International audienceTurbulent spectrum of magnetic fluctuations in the solar wind nearly follows K...
International audienceTurbulent spectra of magnetic fluctuations in the free solar wind are studied ...
In this paper we give a formulation of two-dimensional (2D) collisionless magnetohydrodynamic (MHD) ...
This HDR is devoted to solar wind turbulence from MHD to kinetic plasma scales. Solar wind turbulenc...
International audienceRecent studies of kinetic scales solar wind turbulence have revealed new featu...