New Insights into Dissipation in the Electron Layer During Magnetic Reconnection
arXiv:1001.0082 · doi:10.1029/2008GL034538
Abstract
Detailed comparisons are reported between laboratory observations of electron-scale dissipation layers near a reconnecting X-line and direct two-dimensional full-particle simulations. Many experimental features of the electron layers, such as insensitivity to the ion mass, are reproduced by the simulations; the layer thickness, however, is about 3-5 times larger than the predictions. Consequently, the leading candidate 2D mechanism based on collisionless electron nongyrotropic pressure is insufficient to explain the observed reconnection rates. These results suggest that, in addition to the residual collisions, 3D effects play an important role in electron-scale dissipation during fast reconnection.
17 pages, 4 figures
References in corpus (2)
Cited by in corpus (11)
- Phase Diagram for Magnetic Reconnection in Heliophysical, Astrophysical and Laboratory Plasmas
- Magnetic reconnection in the era of exascale computing and multiscale experiments
- Laboratory Space Physics: Investigating the Physics of Space Plasmas in the Laboratory
- Onset of Fast Magnetic Reconnection in Partially Ionized Gases
- First observation of magnetic flux rope inside electron diffusion region
- Ion and Electron Acoustic Bursts during Anti-Parallel Magnetic Reconnection Driven by Lasers
- Laboratory verification of electron-scale reconnection regions modulated by a three-dimensional instability
- Model of two-fluid reconnection
- Nonlinear Resistivity for Magnetohydrodynamical Models
- A new fast reconnection model in a collisionless regime
- Fast and slow two-fluid magnetic reconnection