Electron-scale Kelvin–Helmholtz Instabilities in Magnetized Shear Flows

Electron-scale Kelvin–Helmholtz instabilities (ESKHIs) are found in several astrophysical scenarios. Naturally, ESKHIs are subject to a background magnetic field, but an analytical dispersion relation and an accurate growth rate of ESKHI under this circumstance have remained open because former magn...

Full description

Saved in:
Bibliographic Details
Main Authors: Yao Guo, Dong Wu, Jie Zhang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ade3cf
Tags: Add Tag
No Tags, Be the first to tag this record!