1,720,963 research outputs found
Mixing of the electron distribution function in nonlinear 2D magnetic reconnection
The role played by the conservation of the generalized magnetic linking conditions in the nonlinear evolution of the two-dimensional collisionless, magnetic field reconnection is investigated in the framework of a drift-kinetic description of the electron response. The time-evolution of the electron distribution function at fixed parallel canonical momentum allows us to establish a clear analogy between the fluid and the kinetic regimes of the collisionless reconnection instability in terms of the advection and mixing of Lagrangian invariants
Nonlinear drift-kinetic evolution of the electron distribution function in two-dimensional magnetic reconnection
The nonlinear evolution of the electron distribution function in collisionless magnetic field line reconnection is investigated by adopting a drift-kinetic description of the electron response. A two dimensional magnetic configuration with a null line and a strong perpendicular guide magnetic field is considered. Using the conservation of the parallel canonical momentum, the fluid and the drift-kinetic regimes of the collisionless reconnection instability are shown to share common features in terms of the advection and mixing of the Lagrangian invariants
Three-dimensional MHD simulations of forced magnetic reconnection
Results are presented from MHD simulations of three-dimensional flows of a high-conductivity plasma in the vicinity of a null point of a magnetic field. The excitation of an electric current at the boundary of the computation region results in self-consistent plasma flows and change in the structure of the magnetic field. Generally, in the vicinity of a null point, an MHD singularity arises that manifests itself in the formation of locally plane current sheets. It is shown that the current sheet can be oriented either along the separatrix surface of a magnetic configuration or perpendicular to it, except for axisymmetric configurations (or close to them), when the excitation of an electric current in the direction orthogonal to the separatrix surface does not lead to the formation of a current sheet. (C) 2001 MAIK "Nauka/Interperiodica"
Current sheet formation in three-dimensional magnetic configurations
The formation of electric current sheets in a high-conductivity three-dimensional plasma configuration is studied in the neighborhood of the critical points of the magnetic field. First, with the help of a Clebsch variable representation, the propagation of magnetohydrodynamic (MHD) waves in azimuthally symmetric current-free configurations is investigated. Exact solutions of the MHD equations that describe the self-similar evolution of a magnetic configuration near a critical point are presented. Then, the nonlinear plasma evolution is simulated with an MHD code. The excitation of an electric current at the boundary of the computational region results in a self-consistent plasma flow and in the change of the structure of the magnetic field. No electric current sheet is formed when both the equilibrium configuration and the perturbations are azimuthally symmetric. (C) 2002 American Institute of Physics
Formation of current sheets in structurally stable and structurally unstable magnetic configurations with two null lines
The nonlinear dynamics of magnetoacoustic and Alfven Mt-ID perturbations in structurally unstable magnetic configurations with two null lines (X-lines) is studied both analytically and numerically. It is shown that these perturbations cause the electric current to evolve nonlinearly in such a manner that a structurally unstable configuration of the magnetic field transforms into a structurally stable configuration. Such a transformation is forbidden in ideal magnetohydrodynamics but can occur in the process of magnetic field line reconnection. The final magnetic configuration to which the system evolves is shown to contain no separatrices connecting the null lines. (C) 2000 MAIK "Nauka/Interperiodica"
Foliation and mixing of the electron drift-kinetic distribution function in nonlinear two-dimensional magnetic reconnection
The nonlinear evolution of the two-dimensional collisionless magnetic field reconnection in a configuration with a null line and a strong perpendicular guide magnetic field is studied analytically and numerically by adopting a drift-kinetic description of the electron response. The foliation of the electron distribution function at fixed parallel canonical momentum allows us to establish a clear link between the fluid and the kinetic regimes of the collisionless reconnection instability in terms of the advection and mixing of Lagrangian invariants. (C) 2004 American Institute of Physics
Unlimited Ion Acceleration by Radiation Pressure
The energy of ions accelerated by an intense electromagnetic wave in the radiation pressure dominated regime can be greatly enhanced due to a transverse expansion of a thin target. The expansion decreases the number of accelerated ions in the irradiated region resulting in an increase in the ion energy and in the ion longitudinal velocity. In the relativistic limit, the ions become phase locked with respect to the electromagnetic wave resulting in unlimited ion energy gain
Phase-locked ions and foil transparency in the radiation pressure acceleration regime
The transverse expansion of a thin foil accelerated in the RPDA regime can be exploited in order to increase the ion energy and the acceleration efficiency at the expense of decreasing the number of accelerated particles. In the relativistic regime, the ions become phase-locked with respect to the electromagnetic wave. The use of an optimal laser pulse shape makes it possible to keep the expanding foil opaque to the laser radiation. This provides a new approach in order to enhance the energy of laser accelerated ions significantly. (C) 2010 Elsevier B.V. All rights reserved
Dependence of the ion energy on the parameters of the laser pulse and target in the radiation-pressure-dominated regime of acceleration
When the dominant mechanism for ion acceleration is the laser radiation pressure, the conversion efficiency of the laser energy into the energy of relativistic ions may be very high. Stability analysis of a thin plasma layer accelerated by the radiation pressure shows that Raleigh-Taylor instability may enhance plasma inhomogeneity. In the linear stage of instability, the plasma layer decays into separate bunches, which are accelerated by the radiation pressure similarly to clusters accelerated under the action of an electromagnetic wave. The energy and luminosity of an ion beam accelerated in the radiation-pressure-dominated regime are calculated
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