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Plasma Potential and Langmuir Probe Measurements in the Near-field Plume of the NASA 300M Hall Thruster

机译:NASA 300M霍尔推进器近场羽流中的等离子体电势和Langmuir探针测量

摘要

In order to aid in the design of high-power Hall thrusters and provide experimental validation for existing modeling efforts, plasma potential and Langmuir probe measurements were performed in the near-field plume of the NASA 300M Hall thruster. A probe array consisting of a Faraday probe, Langmuir probe, and emissive probe was used to interrogate the plume from approximately 0.1 - 2.0 DT,m downstream of the thruster exit plane at four operating conditions: 300 V, 400 V, and 500 V at 20 kW as well as 300 V at 10 kW. Results show that the acceleration zone and high-temperature region were contained within 0.3 DT,m from the exit plane at all operating conditions. Isothermal lines were shown to strongly follow magnetic field lines in the nearfield, with maximum temperatures ranging from 19 - 27 eV. The electron temperature spatial distribution created large drops in measured floating potentials in front of the magnetic pole surfaces where the plasma density was small, which suggests strong sheaths at these surfaces. The data taken have provided valuable information for future design and modeling validation, and complements ongoing internal measurement efforts on the NASA 300 M.
机译:为了帮助设计大功率霍尔推力器并为现有的建模工作提供实验验证,在NASA 300M霍尔推力器的近场羽流中进行了等离子体电势和Langmuir探针测量。由法拉第探针,Langmuir探针和发射探针组成的探针阵列用于在以下四个操作条件下从推进器出口平面下游约0.1-2.0 DT,m处探查羽流:300 V,400 V和500 V 20 kW以及10 kW时为300V。结果表明,在所有工作条件下,加速区和高温区域均位于离出口平面0.3 DT,m之内。等温线显示在近场中强烈跟随磁场线,最高温度范围为19-27 eV。电子温度空间分布在等离子密度小的磁极表面前面产生了很大的测量浮动电位下降,这表明在这些表面上有坚固的鞘层。所获取的数据为将来的设计和建模验证提供了有价值的信息,并补充了NASA 300 M上正在进行的内部测量工作。

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