次世代の宇宙ロケットを後押しする研究 (New UVA Professor’s Research May Boost Next-Generation Space Rockets)

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2025-01-02 アメリカ合衆国・バージニア大学 (UVA)

次世代の宇宙ロケットを後押しする研究 (New UVA Professor’s Research May Boost Next-Generation Space Rockets)
Pictured is a 6 kW Hall thruster in operation at the NASA Jet Propulsion Laboratory. (Courtesy of NASA-JPL/CalTech)

バージニア大学の新任助教授であるChen Cui氏は、電気推進(EP)スラスターのプラズマビーム内の電子の運動を詳細に研究し、EPスラスターの性能向上に寄与する新たな知見を得ました。この研究は、EPスラスターが長期間の宇宙ミッションで安定的かつ効率的に動作するための基盤となり、将来的な宇宙探査ミッションの成功に貢献することが期待されます。

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電気推進ビームのブラゾフシミュレーション Vlasov simulations of electric propulsion beam

Chen Cui and Joseph Wang
Plasma Sources Science and Technology  Published: 11 December 2024
DOI:10.1088/1361-6595/ad98c0

Abstract

A grid-based Vlasov simulation model is developed to simulate the two-dimensional unmagnetized electric propulsion (EP) plasma beam emission process. Comparing to the standard fully kinetic Particle-in-Cell simulation, the grid-based Vlasov simulation method eliminates the interference of particle noise and is capable of resolving higher-order velocity moment, such as electron heat flux, accurately. Vlasov simulations are carried out to investigate the effects of microscopic electron kinetics on macroscopic electron thermodynamics in EP beam. We find that the electron velocity distribution function (eVDF) exhibits a near-Maxwellian shape but with a depleted negative velocity tail in the beam direction and a ‘top-hat’ shape in the transverse direction. Macroscopically, the electrons confined within the quasi-neutral beam core region has a near constant temperature along the beam direction but follow a near-adiabatic cooling process as they expand outward in the transverse direction. The electron heat flux is dominated by the x-direction tensor component. The connection between the eVDF skewness and the electron heat flux suggests a pathway to develop a microscopic physics based electron closure relation for macroscopic electron thermodynamic process in unmagnetized plasma beam expansion.

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