Electron Heating in 2D Particle-in-Cell Simulations of Quasi-Perpendicular Low-Beta Shocks
arXiv:2308.16462 · doi:10.3847/1538-4357/ad1f69
Abstract
We measure the thermal electron energization in 1D and 2D particle-in-cell (PIC) simulations of quasi-perpendicular, low-beta () collisionless ion-electron shocks with mass ratio , fast Mach number -, and upstream magnetic field angle - from shock normal . It is known that shock electron heating is described by an ambipolar, -parallel electric potential jump, , that scales roughly linearly with the electron temperature jump. Our simulations have - in units of the pre-shock ions' bulk kinetic energy, in agreement with prior measurements and simulations. Different ways to measure , including the use of de Hoffmann-Teller frame fields, agree to tens-of-percent accuracy. Neglecting off-diagonal electron pressure tensor terms can lead to a systematic underestimate of in our low- shocks. We further focus on two shocks: a () case with a long, precursor of whistler waves along , and a () case with a shorter, precursor of whistlers oblique to both and ; is the ion skin depth. Within the precursors, has a secular rise towards the shock along multiple whistler wavelengths and also has localized spikes within magnetic troughs. In a 1D simulation of the , case, shows a weak dependence on the electron plasma-to-cyclotron frequency ratio , and decreases by a factor of 2 as is raised to the true proton-electron value of 1836.
32 pages, 25 figures; accepted to ApJ. Figures 6, 8, 16, 23 updated to fix Liouville mapping procedure normalization (Equation (8))
References in corpus (11)
- Non-Thermal Electron Acceleration in Low Mach Number Collisionless Shocks. I. Particle Energy Spectra and Acceleration Mechanism
- Relativistic electrons produced by foreshock disturbances
- Observational Evidence for Stochastic Shock Drift Acceleration of Electrons at the Earth's Bow Shock
- Theory of Stochastic Shock Drift Acceleration for Electrons in the Shock Transition Region
- Electrostatic solitary waves in the Earth's bow shock: nature, properties, lifetimes and origin
- Electron Heating in Low Mach Number Perpendicular shocks. I. Heating Mechanism
- Electron-scale reconnection in three-dimensional shock turbulence
- Non-adiabatic electron behaviour due to short-scale electric field structures at collisionless shock waves
- Mach Number Dependence of Electron Heating in High Mach Number Quasiperpendicular Shocks
- Double layers in the Earth's bow shock
- Intense whistler-mode waves at foreshock transients: characteristics and regimes of wave-particle resonant interaction