[1] Directed flow of incident ions provides the free energy which is redistributed in a shock among heated ions and electrons, accelerated particles, and magnetic compression. In low Mach number laminar shock the main channel of conversion is into downstream gyrating ions. Just behind the shock transition the ion distribution is substantially nongyrotropic, which results in spatially periodic variations of the ion pressure and, consequently, in time stationary downstream oscillations of the magnetic field. In the absence of significant level of nonstationarity, gyrotropization is due to the gyrophase mixing and slow. Theoretical analysis of the phenomenon and supporting hybrid simulations are presented. It is shown that these oscillations a...
International audiencePrevious particle-in-cell simulations have evidenced that quasi-perpendicular ...
International audienceMany space missions have already evidenced the existence of the ion foreshock ...
International audienceCollisionless shocks are well-known structures in astrophysical environments w...
Collisionless shocks efficiently convert the energy of the directed ion flow into their thermal ener...
Collisionless shock heats ions very efficiently. Ion heating is a nonadiabatic process and the downs...
Collisionless shocks are ubiquitous throughout the known Universe. They mainly convert the energy of...
The heating of directly transmitted ions at low Mach number, perpendicular and quasi perpendicular s...
We have performed 3 one-dimensional full particle electromagnetic simulations of a quasi-perpendicu...
International audiencePrevious particle-in-cell simulations have evidenced that quasiperpendicular s...
International audienceThe ion foreshock located upstream of the Earth's shock front is populated wit...
We review the ion and electron heating at the quasi-perpendicular collision-less shock front. The sh...
International audienceThe ion foreshock located upstream of the Earth's shock wave is populated with...
International audiencePrevious particle-in-cell simulations have evidenced that quasi-perpendicular ...
International audienceMany space missions have already evidenced the existence of the ion foreshock ...
International audienceCollisionless shocks are well-known structures in astrophysical environments w...
Collisionless shocks efficiently convert the energy of the directed ion flow into their thermal ener...
Collisionless shock heats ions very efficiently. Ion heating is a nonadiabatic process and the downs...
Collisionless shocks are ubiquitous throughout the known Universe. They mainly convert the energy of...
The heating of directly transmitted ions at low Mach number, perpendicular and quasi perpendicular s...
We have performed 3 one-dimensional full particle electromagnetic simulations of a quasi-perpendicu...
International audiencePrevious particle-in-cell simulations have evidenced that quasiperpendicular s...
International audienceThe ion foreshock located upstream of the Earth's shock front is populated wit...
We review the ion and electron heating at the quasi-perpendicular collision-less shock front. The sh...
International audienceThe ion foreshock located upstream of the Earth's shock wave is populated with...
International audiencePrevious particle-in-cell simulations have evidenced that quasi-perpendicular ...
International audienceMany space missions have already evidenced the existence of the ion foreshock ...
International audienceCollisionless shocks are well-known structures in astrophysical environments w...