May 24 – 26, 2021
Virtual
US/Eastern timezone

The Scaling of Electron Heating in Low-beta Reconnection Exhausts with Kinetic Reconnection Simulations

May 26, 2021, 1:00 PM
40m
Virtual

Virtual

Poster Flare and Nanoflare heating Poster session: SQ3 and SQ6

Speaker

Qile Zhang (Los Alamos National Lab)

Description

Particle heating in reconnection is essential to understand the heating in the solar corona, solar flares and the magnetotail. It plays an important role distributing magnetic energy into different species and between thermal and nonthermal components. Previous observational and theoretical studies on electron heating in reconnection exhausts within the beta~1 regime suggest a simple linear scaling where the electron heating is proportional to the magnetic energy per particle. Using kinetic reconnection simulations in the low-beta regime (with beta down to 0.005), we demonstrate that electron heating follows a sub-linear scaling below beta~0.01, with or without guide fields. As a result, the maximum heating is limited to only ~5 times of upstream electron temperature. This electron heating scaling may be testable by MMS observations at the magnetotail. This new finding has strong implications for the efficiency of electron heating in reconnection at low-beta environments throughout heliosphysics.

Primary authors

Qile Zhang (Los Alamos National Lab) Fan Guo (Los Alamos National Lab) Dr Marit Øieroset (University of California Berkeley) Dr Tai Phan (University of California Berkeley) Michael Shay (University of Delaware) Dr James Drake (University of Maryland College Park) Dr Marc Swisdak (University of Maryland College Park)

Presentation materials