Effects of magnetic field gradient and secondary electron emission on instabilities and transport in an ExB plasma configuration

TL;DR

This study investigates how magnetic field gradients and secondary electron emission influence plasma instabilities and transport in ExB configurations, with implications for improving Hall thruster performance.

Contribution

The paper presents novel simulation results on the effects of magnetic field gradients and secondary electron emission on plasma behavior in Hall thrusters.

Findings

Inverse energy cascade forms high-frequency azimuthal modes at high plasma densities.

Strong magnetic field gradients enhance electron cross-field transport.

Plasma heating and instability characteristics are significantly affected by these factors.

Abstract

Today, partially magnetized low-temperature plasmas (LTP) in an ExB configuration, where the applied magnetic field is perpendicular to the self-consistent electric field, have important industrial applications. Hall thrusters, a type of electrostatic plasma propulsion, are one of the main LTP technologies whose advancement is hindered by the not-fully-understood underlying physics of operation, particularly, with respect to the plasma instabilities and the associated electron cross-field transport. The development of Hall thrusters with unconventional magnetic field topologies has imposed further questions regarding the instabilities' characteristics and the electrons' dynamics in these modern cross-field configurations. Accordingly, we present in this effort a series of studies on the influence of four factors on the plasma processes in the radial-azimuthal coordinates of a Hall thruster, namely, the magnetic field gradient, Secondary Electron Emission, electron-neutral collisions, and plasma number density. The studies are carried out using the reduced-order particle-in-cell (PIC) code developed by the authors. The setup of the radial-azimuthal simulations largely follows a well-defined benchmark case from the literature in which the magnetic field is oriented along the radius and a constant axial electric field is applied perpendicular to the simulation plane. The salient finding from our investigations is that, in the studied cases corresponding to elevated plasma densities, an inverse energy cascade leads to the formation of a long-wavelength, high-frequency azimuthal mode. Moreover, in the presence of strong magnetic field gradients, this mode is fully developed and induces a significant electron cross-field transport as well as a notable heating of the ion population.