Electron acceleration and heating in collisionless magnetic reconnection
arXiv:astro-ph/0305081 · doi:10.1063/1.1598207
Abstract
We discuss electron acceleration and heating during collisionless magnetic reconnection by using the results of implicit kinetic simulations of Harris current sheets. We consider and compare electron dynamics in plasmas with different βvalues and perform simulations up to the physical mass ratio. We analyze the typical trajectory of electrons passing through the reconnection region, we study the electron velocity, focusing on the out-of-plane velocity, and we discuss the electron heating along the in-plane and out-of-plane directions.
References in corpus (1)
Cited by in corpus (9)
- The Role of the Guide Field in Relativistic Pair Plasma Reconnection
- Relativistic magnetic reconnection in collisionless ion-electron plasmas explored with particle-in-cell simulations
- Three Dimensional Evolution of a Relativistic Current Sheet : Triggering of Magnetic Reconnection by the Guide Field
- Electron and Proton Heating in Transrelativistic Guide Field Reconnection
- Two-Stage Bulk Electron Heating in the Diffusion Region of Anti-Parallel Symmetric Reconnection
- Non-linear Waves and Instabilities Leading to Secondary Reconnection in Reconnection Outflows
- Magnetic guide field generation in thin collisionless current sheets
- Drifting Pulsation Structure at the Very Beginning of the 2017 September 10 Limb Flare
- Direct Measurement of Electron Heating in Electron-Only Reconnection in a Laboratory Mini-Magnetosphere