Electron-only reconnection in plasma turbulence
Abstract
Hybrid-Vlasov-Maxwell simulations of magnetized plasma turbulence including non-linear electron-inertia effects in a generalized Ohm's law are presented. When fluctuation energy is injected on scales sufficiently close to ion-kinetic scales, the ions efficiently become demagnetized and electron-scale current sheets largely dominate the distribution of the emerging current structures, in contrast to the usual picture, where a full hierarchy of structure sizes is generally observed. These current sheets are shown to be the sites of electron-only reconnection (e-rec), in which the usual electron exhausts are unaccompanied by ion outflows and which are in qualitative agreement with those recently observed by MMS in the Earth's turbulent magnetosheath, downstream of the bow shock. Some features of the e-rec phenomenology are shown to be consistent with an electron magnetohydrodynamic description. Simulations suggest that this regime of collisionless reconnection may be found in turbulent systems where plasma processes, such as micro-instabilities and/or shocks, overpower the more customary turbulent cascade by directly injecting energy close to the ion-kinetic scales.
- Publication:
-
Frontiers in Physics
- Pub Date:
- September 2020
- DOI:
- 10.3389/fphy.2020.00317
- arXiv:
- arXiv:1810.03957
- Bibcode:
- 2020FrP.....8..317C
- Keywords:
-
- Magnetic Fields;
- magnetic reconnection;
- Plasma turbulence;
- Solar wind;
- Earth magnetosheath;
- kinetic plasma simulations;
- Physics - Plasma Physics;
- Astrophysics - Solar and Stellar Astrophysics;
- Physics - Space Physics
- E-Print:
- 20 pages, 8 figures