Compressibility has a strong influence on the stability of velocity shear layers when the difference of velocity ΔV across the flow becomes supersonic. The flanks of the Earth's magnetopause are normally supersonic Ms > 1, and super-Alfvénic MA > 1, depending on the distance from the dayside terminator (Ms and MA are the sonic and Alfvén Mach numbers of the magnetosheath plasma, respectively). The stability of MHD supersonic flows depends, also on several other features, such as the finite thickness Δ of the boundary layer, the relative orientation of velocity and magnetic fields, the density jump across the boundary and the magnetic shear angle. We analyze the MHD stability of some representative flank sites modeled after data from s...
The compressible magnetohydrodynamic Kelvin-Helmholtz instability occurs in two varieties, one that ...
A magnetohydrodynamic simulation of Kelvin-Helmholtz instabilities in a compressible plasma has been...
We have performed 13 three-dimensional global magnetohydrodynamic (MHD) simulations of the magnetosh...
Two examples of stability analysis of the supersonic magnetopause (MP) flanks, based on compressible...
It has recently been demonstrated, by means of a two-dimensional MHD simulation, that a finite thick...
It is demonstrated by means of a MHD simulation that a finite thick velocity shear layer with super‐...
The effect of the finite thickness of the shear layer on the Kelvin-Helmholtz instability of the Ear...
International audienceA study is made of the influence of the longitudinal magnetic field and densit...
We study the Kelvin-Helmholtz (KH) instability at the dayside magnetopause, modeling the flow, the m...
The understanding of the dynamics at play at the Earth's Magnetopause, the boundary separating the E...
International audienceOn 14 June 2001 the four Cluster spacecraft recorded multiple encounters of th...
The Kelvin-Helmoltz instability (KH) with formation of vortices appears in a wide variety of terrest...
The aim of this paper is to model for the first time the variation of field and flow parameters in t...
A magnetohydrodynamic simulation of Kelvin-Helmholtz instabilities in a compressible plasma has been...
A two-dimensional magnetohydrodynamic simulation of Kelvin-Helmholtz instability at the terrestrial ...
The compressible magnetohydrodynamic Kelvin-Helmholtz instability occurs in two varieties, one that ...
A magnetohydrodynamic simulation of Kelvin-Helmholtz instabilities in a compressible plasma has been...
We have performed 13 three-dimensional global magnetohydrodynamic (MHD) simulations of the magnetosh...
Two examples of stability analysis of the supersonic magnetopause (MP) flanks, based on compressible...
It has recently been demonstrated, by means of a two-dimensional MHD simulation, that a finite thick...
It is demonstrated by means of a MHD simulation that a finite thick velocity shear layer with super‐...
The effect of the finite thickness of the shear layer on the Kelvin-Helmholtz instability of the Ear...
International audienceA study is made of the influence of the longitudinal magnetic field and densit...
We study the Kelvin-Helmholtz (KH) instability at the dayside magnetopause, modeling the flow, the m...
The understanding of the dynamics at play at the Earth's Magnetopause, the boundary separating the E...
International audienceOn 14 June 2001 the four Cluster spacecraft recorded multiple encounters of th...
The Kelvin-Helmoltz instability (KH) with formation of vortices appears in a wide variety of terrest...
The aim of this paper is to model for the first time the variation of field and flow parameters in t...
A magnetohydrodynamic simulation of Kelvin-Helmholtz instabilities in a compressible plasma has been...
A two-dimensional magnetohydrodynamic simulation of Kelvin-Helmholtz instability at the terrestrial ...
The compressible magnetohydrodynamic Kelvin-Helmholtz instability occurs in two varieties, one that ...
A magnetohydrodynamic simulation of Kelvin-Helmholtz instabilities in a compressible plasma has been...
We have performed 13 three-dimensional global magnetohydrodynamic (MHD) simulations of the magnetosh...