Rankine–Hugoniot relations (RH) connect the upstream and downstream plasma states. They allow us to determine the magnetic compression, the density compression, and the plasma heating as functions of the Mach number, shock angle, and upstream temperature. RH are based on the conservation laws in the hydrodynamical form. In collisionless shocks, the ion distributions behind the shock transition are determined by ion dynamics in the macroscopic fields of the shock front. The ion parameters upon crossing the shock are directly related to the magnetic compression and the cross-shock potential. For given upstream parameters, RH provide the magnetic compression. If there is no substantial overshoot, an analytical estimate provides the cross-shock...
The heating of directly transmitted ions at low Mach number, quasi-perpendicular collisionless shock...
International audienceThe unprecedented high detail of field and plasma measurements by the four MMS...
In a series of earlier papers, we developed expressions for ion and electron velocity distribution f...
Collisionless shock heats ions very efficiently. Ion heating is a nonadiabatic process and the downs...
The only well-developed theory of collisionless shocks is the one-dimensional (1-D) stationary theor...
Context. Observations by Voyager-2 at the crossing of the solar wind termination shock have led to u...
Collisionless shocks channel the energy of the directed plasma flow into the heating of the plasma s...
Collisionless shocks efficiently convert the energy of the directed ion flow into their thermal ener...
This work presents an analysis of the ion outflow from magnetic reconnection throughout fully kineti...
In this work, we compare the spatial distribution of the plasma parameters along the 1999 June 11 co...
Interplanetary shocks are believed to play an important role in the acceleration of charged particle...
Interplanetary shocks are believed to play an important role in the acceleration of charged particle...
The heating of directly transmitted ions at low Mach number, perpendicular and quasi perpendicular s...
In this paper we consider a multi-fluid plasma that describes the upstream solar wind at its passage...
[1] To study MHD shocks in space, it is important to find the shock frame of reference from the obse...
The heating of directly transmitted ions at low Mach number, quasi-perpendicular collisionless shock...
International audienceThe unprecedented high detail of field and plasma measurements by the four MMS...
In a series of earlier papers, we developed expressions for ion and electron velocity distribution f...
Collisionless shock heats ions very efficiently. Ion heating is a nonadiabatic process and the downs...
The only well-developed theory of collisionless shocks is the one-dimensional (1-D) stationary theor...
Context. Observations by Voyager-2 at the crossing of the solar wind termination shock have led to u...
Collisionless shocks channel the energy of the directed plasma flow into the heating of the plasma s...
Collisionless shocks efficiently convert the energy of the directed ion flow into their thermal ener...
This work presents an analysis of the ion outflow from magnetic reconnection throughout fully kineti...
In this work, we compare the spatial distribution of the plasma parameters along the 1999 June 11 co...
Interplanetary shocks are believed to play an important role in the acceleration of charged particle...
Interplanetary shocks are believed to play an important role in the acceleration of charged particle...
The heating of directly transmitted ions at low Mach number, perpendicular and quasi perpendicular s...
In this paper we consider a multi-fluid plasma that describes the upstream solar wind at its passage...
[1] To study MHD shocks in space, it is important to find the shock frame of reference from the obse...
The heating of directly transmitted ions at low Mach number, quasi-perpendicular collisionless shock...
International audienceThe unprecedented high detail of field and plasma measurements by the four MMS...
In a series of earlier papers, we developed expressions for ion and electron velocity distribution f...