The effect of alternative propellants on the electron drift instability in Hall-effect thrusters: Insight from 2D Particle-In-Cell simulations
Vivien Croes (LPP), Antoine Tavant (LPP), Romain Lucken (LPP), Roberto, Martorelli (LPP), Trevor Lafleur, Anne Bourdon (LPP), Pascal Chabert (LPP)

TL;DR
This study uses 2D PIC/MCC simulations to analyze how different noble gas propellants affect the electron drift instability in Hall-effect thrusters, revealing that instability frequency depends on propellant mass while electron mobility does not.
Contribution
It provides the first detailed comparison of EDI characteristics across multiple noble gases in HETs using advanced simulation techniques.
Findings
EDI occurs with all studied propellants.
Instability frequency depends on propellant mass.
Electron mobility is nearly independent of propellant choice.
Abstract
Hall-effect thrusters (HETs) operated with xenon are one of the most commonly used electric propulsion technologies for a wide range of space missions, including drag compensation in low Earth orbit, station-keeping, and orbital insertion, as access to space becomes more affordable. Although anomalous electron transport, the electron drift instability (EDI), and secondary electron emission (SEE) have been studied experimentally and numerically in xenon-based HETs, the impact of alternative propellants is still poorly characterized. In this work, a two-dimensional particle-in-cell/Monte Carlo collision (PIC/MCC) code is used to model the (r -- ) plane of a HET operated separately with four different noble gases: xenon, krypton, argon, and helium. Models for electron induced secondary electron emission (SEE) and dielectric walls are implemented in order to investigate the coupling…
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Taxonomy
TopicsPlasma Diagnostics and Applications · Ionosphere and magnetosphere dynamics · Electrohydrodynamics and Fluid Dynamics
