Electromagnetic electron Kelvin–Helmholtz instability

Author:

Che H.12ORCID,Zank G. P.12ORCID

Affiliation:

1. Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville , Huntsville, Alabama 35805, USA and , Huntsville, Alabama 35899, USA

2. Department of Space Science, University of Alabama in Huntsville , Huntsville, Alabama 35805, USA and , Huntsville, Alabama 35899, USA

Abstract

On electron kinetic scales, ions and electrons decouple, and electron velocity shear on electron inertial length ∼de can trigger electromagnetic (EM) electron Kelvin–Helmholtz instability (EKHI). In this paper, we present an analytic study of EM EKHI in an inviscid collisionless plasma with a step-function electron shear flow. We show that in incompressible collisionless plasma, the ideal electron frozen-in condition E+ve×B/c=0 must be broken for the EM EKHI to occur. In a step-function electron shear flow, the ideal electron frozen-in condition is replaced by magnetic flux conservation, i.e., ∇×(E+ve×B/c)=0, resulting in a dispersion relation similar to that of the standard ideal and incompressible magnetohydrodynamics KHI. The magnetic field parallel to the electron streaming suppresses the EM EKHI due to magnetic tension. The threshold for the EM mode of the EKHI is (k·ΔUe)2>ne1+ne2ne1ne2[ne1(vAe1·k)2+ne2(vAe2·k)2], where vAe=B/(4πmene)1/2, ΔUe, and ne are the electron streaming velocity shear and densities, respectively. The growth rate of the EM mode is γem∼Ωce, which is the electron gyro-frequency.

Funder

Division of Physics

Division of Atmospheric and Geospace Sciences

Office of Experimental Program to Stimulate Competitive Research

NASA Headquarters

Alabama EPSCoR

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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