The inner structure of collisionless magnetic reconnection: The electron-frame dissipation measure and Hall fields
Abstract
It was recently proposed that the electron-frame dissipation measure, the energy transfer from the electromagnetic field to plasmas in the electron's rest frame, identifies the dissipation region of collisionless magnetic reconnection [Zenitani et al., Phys. Rev. Lett. 106, 195003 (2011)]. The measure is further applied to the electron-scale structures of antiparallel reconnection, by using two-dimensional particle-in-cell simulations. The size of the central dissipation region is controlled by the electron-ion mass ratio, suggesting that electron physics is essential. A narrow electron jet extends along the outflow direction until it reaches an electron shock. The jet region appears to be anti-dissipative. At the shock, electron heating is relevant to a magnetic cavity signature. The results are summarized to a unified picture of the single dissipation region in a Hall magnetic geometry.
- Publication:
-
Physics of Plasmas
- Pub Date:
- December 2011
- DOI:
- 10.1063/1.3662430
- arXiv:
- arXiv:1110.3103
- Bibcode:
- 2011PhPl...18l2108Z
- Keywords:
-
- astrophysical plasma;
- diffusion;
- magnetic reconnection;
- plasma jets;
- plasma kinetic theory;
- plasma magnetohydrodynamics;
- plasma shock waves;
- plasma simulation;
- plasma transport processes;
- 95.30.Qd;
- 52.25.Dg;
- 52.25.Fi;
- 52.30.Cv;
- 52.35.Tc;
- 52.65.Rr;
- Magnetohydrodynamics and plasmas;
- Plasma kinetic equations;
- Transport properties;
- Magnetohydrodynamics;
- Shock waves and discontinuities;
- Particle-in-cell method;
- Astrophysics - Solar and Stellar Astrophysics;
- Physics - Plasma Physics;
- Physics - Space Physics
- E-Print:
- 10 pages, 9 figures