Non-Maxwellian electron distribution functions due to self-generated turbulence in collisionless guide-field reconnection
arXiv:1608.03110 · doi:10.1063/1.4963773
Abstract
Non-Maxwellian electron velocity space distribution functions (EVDF) are useful signatures of plasma conditions and non-local consequences of collisionless magnetic reconnection. In the past, EVDFs were obtained mainly for antiparallel reconnection and under the influence of weak guide-fields in the direction perpendicular to the reconnection plane. EVDFs are, however, not well known, yet, for oblique (or component-) reconnection in dependence on stronger guide-magnetic fields and for the exhaust (outflow) region of reconnection away from the diffusion region. In view of the multi-spacecraft Magnetospheric Multiscale Mission (MMS), we derived the non-Maxwellian EVDFs of collisionless magnetic reconnection in dependence on the guide-field strength from small () to very strong () guide-fields, taking into account the feedback of the self-generated turbulence. For this sake, we carried out 2.5D fully-kinetic Particle-in-Cell simulations using the ACRONYM code. We obtained anisotropic EVDFs and electron beams propagating along the separatrices as well as in the exhaust region of reconnection. The beams are anisotropic with a higher temperature in the direction perpendicular rather than parallel to the local magnetic field. The beams propagate in the direction opposite to the background electrons and cause instabilities. We also obtained the guide-field dependence of the relative electron-beam drift speed, threshold and properties of the resulting streaming instabilities including the strongly non-linear saturation of the self-generated plasma turbulence. This turbulence and its non-linear feedback cause non-adiabatic parallel electron acceleration and EVDFs well beyond the limits of the quasi-linear approximation, producing phase space holes and an isotropizing pitch-angle scattering.
21 pages, 8 figures. Revised to match with the version published in Physics of Plasmas. An abridged version of the abstract is shown here
References in corpus (16)
- Instability of current sheets and formation of plasmoid chains
- Fast Reconnection in High-Lundquist-Number Plasmas Due to Secondary Tearing Instabilities
- Spontaneous current-layer fragmentation and cascading reconnection in solar flares: I. Model and analysis
- Kinetic signatures of the region surrounding the X-line in asymmetric (magnetopause) reconnection
- The Transition from Anti-Parallel to Component Magnetic Reconnection
- Electron Holes and Heating in the Reconnection Dissipation Region
- Spacecraft observations and analytic theory of crescent-shaped electron distributions in asymmetric magnetic reconnection
- Bipolar Electric Field Signatures of Reconnection Separatrices for a Hydrogen Plasma at Realistic Guide Fields
- Jet deflection by very weak guide fields during magnetic reconnection
- Spontaneous current-layer fragmentation and cascading reconnection in solar flares: II. Relation to observations
- Apar-T: code, validation, and physical interpretation of particle-in-cell results
- Nonlinear Development of Streaming Instabilities In Strongly Magnetized Plasmas
- Electron acceleration by cascading reconnection in the solar corona I Magnetic gradient and curvature effects
- Particle dynamics in the electron current layer in collisionless magnetic reconnection
- Separatrices: the crux of reconnection
- Three dimensional density cavities in guide field collisionless magnetic reconnection
Cited by in corpus (11)
- How Anomalous Resistivity Accelerates Magnetic Reconnection
- Kinetic turbulence in fast 3D collisionless guide-field magnetic reconnection
- A new hybrid code (CHIEF) implementing the inertial electron fluid equation without approximation
- Wave excitation by energetic ring-distributed electron beams in the solar corona
- Turbulent transport in 2D collisionless guide field reconnection
- The effects of density inhomogeneities on the radio wave emission in electron beam plasmas
- Instabilities and Turbulence in Low- Guide Field Reconnection Exhausts with Kinetic Riemann Simulations
- Nonlinear evolution of electron shear flow instabilities in the presence of an external guide magnetic field
- Wave emission of non-thermal electron beams generated by magnetic reconnection
- Nonthermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions
- Anisotropic Heating and Parallel Heat Flux in Electron-only Magnetic Reconnection with Intense Guide Fields