The only well-developed theory of collisionless shocks is the one-dimensional (1-D) stationary theory, which explicitly assumes that all variables in the shock front, including electric and magnetic fields, depend only on the coordinate along the shock normal and do not depend on time. These two assumptions are essential for establishing the Rankine-Hugoniot relations [see, e.g., Tidman and Krall, 1971] which connect the upstream and downstream states of plasma and magneti
International audienceStationary shocks (Part 1) represent a first (simplified) approach of collisio...
Equations are derived to describe the evolution of an electron distribution function under the actio...
The thesis investigates ion behaviour at collisionless shocks, with a focus on two areas of interest...
Rankine–Hugoniot relations (RH) connect the upstream and downstream plasma states. They allow us to ...
Collisionless shocks channel the energy of the directed plasma flow into the heating of the plasma s...
A shock-wave model proposed by both Kahn and Parker for the collision of two interstellar gas clouds...
It is widely believed (see Scudder [1995] and references therein) that electron heating in the shock...
International audienceCollisionless shock waves in plasmas are usually considered as stationary nonl...
We review the ion and electron heating at the quasi-perpendicular collision-less shock front. The sh...
The overall structure of quasi-perpendicular, high Mach number collisionless shocks is controlled ...
Almost all existing models of collisionless shocks, starting with the one-fluid MHD models and endin...
Collisionless shocks undergo structural changes with the increase of Mach number. Observations and n...
The paper deals with the structure of collisionless shocks arising from turbulent wave-particle inte...
In typical heliospheric collisionless shocks most of the mass, momentum and energy are carried by io...
[1] To study MHD shocks in space, it is important to find the shock frame of reference from the obse...
International audienceStationary shocks (Part 1) represent a first (simplified) approach of collisio...
Equations are derived to describe the evolution of an electron distribution function under the actio...
The thesis investigates ion behaviour at collisionless shocks, with a focus on two areas of interest...
Rankine–Hugoniot relations (RH) connect the upstream and downstream plasma states. They allow us to ...
Collisionless shocks channel the energy of the directed plasma flow into the heating of the plasma s...
A shock-wave model proposed by both Kahn and Parker for the collision of two interstellar gas clouds...
It is widely believed (see Scudder [1995] and references therein) that electron heating in the shock...
International audienceCollisionless shock waves in plasmas are usually considered as stationary nonl...
We review the ion and electron heating at the quasi-perpendicular collision-less shock front. The sh...
The overall structure of quasi-perpendicular, high Mach number collisionless shocks is controlled ...
Almost all existing models of collisionless shocks, starting with the one-fluid MHD models and endin...
Collisionless shocks undergo structural changes with the increase of Mach number. Observations and n...
The paper deals with the structure of collisionless shocks arising from turbulent wave-particle inte...
In typical heliospheric collisionless shocks most of the mass, momentum and energy are carried by io...
[1] To study MHD shocks in space, it is important to find the shock frame of reference from the obse...
International audienceStationary shocks (Part 1) represent a first (simplified) approach of collisio...
Equations are derived to describe the evolution of an electron distribution function under the actio...
The thesis investigates ion behaviour at collisionless shocks, with a focus on two areas of interest...