Experiments on the Electrostatic Transport of Charged Anorthite Particles under Electron Beam Irradiation

TL;DR

This study investigates how secondary electron emission influences the electrostatic charging and vertical transport of micron-sized anorthite particles, serving as lunar regolith analogs, under electron beam irradiation, revealing velocity-diameter relationships and charging mechanisms.

Contribution

First experimental measurement of micron-sized anorthite particle transport under electron beam irradiation, providing new insights into dust charging and movement mechanisms on airless celestial bodies.

Findings

Vertical transport dominates particle movement.

High vertical velocities up to 9.74 m/s observed.

Velocity depends linearly on inverse square of diameter.

Abstract

To reveal the effect of secondary electron emission on the charging properties of a surface covered by micron-sized insulating dust particles and the migration characteristics of these particles, for the first time, we used a laser Doppler method to measure the diameters and velocities of micron-sized anorthite particles under electron beam irradiation with an incident energy of 350 eV. Here, anorthite particles are being treated as a proxy for lunar regolith. We experimentally confirm that the vertical transport of anorthite particles is always dominant, although the horizontal transport occurs. In our experiments, some anorthite particles were observed to have large vertical velocities up to 9.74 m~s$^{-1}$ at the measurement point. The upper boundary of the vertical velocities $V_{\rm{z}}$ of these high-speed anorthite particles are well constrained by its diameter $D$, that is, $V_{\rm{z}}^2$ linearly depends on $D^{-2}$. These velocity-diameter data provide strong constraints on the dust charging and transportation mechanisms. The shared charge model could not explain the observed velocity-diameter data. Both the isolated charge model and patched charge model appear to require a large dust charging potential of $-$350 to $-$78 V to reproduce the observed data. The micro-structures of the dusty surface may play an important role in producing this charging potential and in understanding the pulse migration phenomenon observed in our experiment. The presented results and analysis in this paper are helpful for understanding the dust charging and electrostatic transport mechanisms in airless celestial bodies such as the Moon and asteroids in various plasma conditions.