A simplified model of particle transport at a quasiparallel one-dimensional collisionless shock is suggested. In this model the MHD-turbulence behind the shock is dominated by a circularly polarized, large amplitude Alfvén wave originated upstream from the turbulence excited by particles leaking from the downstream medium. It is argued that such a wave having significantly increased its magnetic field during the transmission through the shock interface can effectively trap thermal ions, regulating their leakage upstream. Together with a background turbulence this wave also plays a fundamental role in thermalization of the incoming ion flow. The spectrum of leaking particles and the amplitude of the wave excited by these particles are selfco...
An example is presented from a test particle simulation designed to study ion acceleration at obliqu...
We report the results of 1D particle-in-cell simulations of ultrarelativistic shock waves in proton-...
One of the main features of astrophysical shocks is their ability to accelerate particles to extreme...
The dynamical reaction of the particles accelerated at a shock front by the first order Fermi proces...
The dynamical reaction of the particles accelerated at a shock front by the first-order Fermi proces...
Electron injection process at high Mach number collisionless quasi-perpendicular shock waves is inve...
The dynamical reaction of the particles accelerated at a shock front by the first order Fermi proces...
Within a test-particle description of the acceleration process in parallel nonrelativistic shocks, w...
We consider a phenomenological model for the thermal leakage injection in the diffusive shock accele...
While the theory of shock acceleration has been widely accepted in astrophysical settings, the sourc...
Shock waves propagating in collisionless heliospheric and astrophysical plasmas have been studied ex...
The superthermal ions at a quasi-parallel collisionless shock are considered to be generated during ...
Particle acceleration in collisionless astrophysical shocks, i.e., diffusive shock acceleration (DSA...
We use kinetic hybrid simulations (kinetic ions – fluid electrons) to characterize the fraction of i...
A large number of numerical experiments has been performed in order to study the interaction of inte...
An example is presented from a test particle simulation designed to study ion acceleration at obliqu...
We report the results of 1D particle-in-cell simulations of ultrarelativistic shock waves in proton-...
One of the main features of astrophysical shocks is their ability to accelerate particles to extreme...
The dynamical reaction of the particles accelerated at a shock front by the first order Fermi proces...
The dynamical reaction of the particles accelerated at a shock front by the first-order Fermi proces...
Electron injection process at high Mach number collisionless quasi-perpendicular shock waves is inve...
The dynamical reaction of the particles accelerated at a shock front by the first order Fermi proces...
Within a test-particle description of the acceleration process in parallel nonrelativistic shocks, w...
We consider a phenomenological model for the thermal leakage injection in the diffusive shock accele...
While the theory of shock acceleration has been widely accepted in astrophysical settings, the sourc...
Shock waves propagating in collisionless heliospheric and astrophysical plasmas have been studied ex...
The superthermal ions at a quasi-parallel collisionless shock are considered to be generated during ...
Particle acceleration in collisionless astrophysical shocks, i.e., diffusive shock acceleration (DSA...
We use kinetic hybrid simulations (kinetic ions – fluid electrons) to characterize the fraction of i...
A large number of numerical experiments has been performed in order to study the interaction of inte...
An example is presented from a test particle simulation designed to study ion acceleration at obliqu...
We report the results of 1D particle-in-cell simulations of ultrarelativistic shock waves in proton-...
One of the main features of astrophysical shocks is their ability to accelerate particles to extreme...