In a collisionless plasma, when reconnection instability takes place, strong shear flows may develop. Under appropriate conditions these shear flows become unstable to the Kelvin-Helmholtz instability. Here, we investigate the coupling between these instabilities in the framework of a four-field model. Firstly, we recover the known results in the low beta limit, beta being the ratio between the plasma and the magnetic pressure. We concentrate our attention on the dynamical evolution of the current density and vorticity sheets which evolve coupled together according to a laminar or a turbulent regime. A three-dimensional extension in this limit is also discussed. Secondly, we consider finite values of the beta parameter, allowing for compres...
We investigate the Kelvin-Helmholtz instability occurring at the interface of a shear-flow configura...
The nonlinear evolution of collisionless plasmas is typically a multi-scale process, where the energ...
The plasma state is usually referred as the fourth state of matter. In practice it is a collection o...
The role of magnetic reconnection on the evolution of the Kelvin-Helmholtz instability is investigat...
The understanding of the dynamics at play at the Earth's Magnetopause, the boundary separating the E...
International audienceIn this paper we present the numerical investigation of a three-dimensional fo...
The turbulence developing inside Kelvin-Helmholtz vortices has been studied using a two-fluid numeri...
We explore, via analytical and numerical methods, the Kelvin-Helmholtz instability in relativistic m...
The fast collisionless reconnection process typical of fusion relevant plasma regimes is analyzed wi...
We explore, via analytical and numerical methods, the Kelvin-Helmholtz (KH) instability in relativis...
At the Earth\u27s magnetopause, both magnetic reconnection and the Kelvin‐Helmholtz (KH) instability...
The interplay between the Kelvin-Helmholtz, the Rayleigh-Taylor and the Magnetic Re-connection insta...
A typical property of magnetopause reconnection is a significant perpendicular shear flow due to the...
Context. The magnetic Kelvin-Helmholtz instability (KHI) has been proposed as a means of generating ...
We investigate both large- and small-scale properties of a Kelvin-Helmholtz (KH) event at the dusk f...
We investigate the Kelvin-Helmholtz instability occurring at the interface of a shear-flow configura...
The nonlinear evolution of collisionless plasmas is typically a multi-scale process, where the energ...
The plasma state is usually referred as the fourth state of matter. In practice it is a collection o...
The role of magnetic reconnection on the evolution of the Kelvin-Helmholtz instability is investigat...
The understanding of the dynamics at play at the Earth's Magnetopause, the boundary separating the E...
International audienceIn this paper we present the numerical investigation of a three-dimensional fo...
The turbulence developing inside Kelvin-Helmholtz vortices has been studied using a two-fluid numeri...
We explore, via analytical and numerical methods, the Kelvin-Helmholtz instability in relativistic m...
The fast collisionless reconnection process typical of fusion relevant plasma regimes is analyzed wi...
We explore, via analytical and numerical methods, the Kelvin-Helmholtz (KH) instability in relativis...
At the Earth\u27s magnetopause, both magnetic reconnection and the Kelvin‐Helmholtz (KH) instability...
The interplay between the Kelvin-Helmholtz, the Rayleigh-Taylor and the Magnetic Re-connection insta...
A typical property of magnetopause reconnection is a significant perpendicular shear flow due to the...
Context. The magnetic Kelvin-Helmholtz instability (KHI) has been proposed as a means of generating ...
We investigate both large- and small-scale properties of a Kelvin-Helmholtz (KH) event at the dusk f...
We investigate the Kelvin-Helmholtz instability occurring at the interface of a shear-flow configura...
The nonlinear evolution of collisionless plasmas is typically a multi-scale process, where the energ...
The plasma state is usually referred as the fourth state of matter. In practice it is a collection o...