PPPS-2013:重气体θ箍缩线圈中初始等离子体形成的光学发射光谱

W. Meeks, J. Rovey
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摘要

只提供摘要形式。脉冲感应等离子体器件,如常见的theta-pinch,已成为研究和工业中标准的高能等离子体源。目前,核聚变和空间推进领域正在研究的脉冲感应等离子体分别利用氘和氙,并提供了有希望的新结果。然而,在早期等离子体形成时期(即初始电感耦合期间)的能量转换过程中,很少有人做得更好。这项研究的广泛努力是阐明在10-8到10-6秒的初始等离子体形成过程中,电到粒子的能量转换过程。在这项工作中,光谱发射数据的分析是在一个用于现场反向配置(FRC)研究的theta夹点测试文章上进行的。测试在脉冲氙等离子体上进行,能量约为80焦耳,中性回填压力为10-2托,RLC放电频率为500 kHz。同一实验的磁场研究(b点探针、磁回路)与这些工作并行。利用先前为分析氙霍尔效应推力器而开发的碰撞辐射模型,线发射强度比被用来近似与等离子体密度无关的电子温度。使用普林斯顿仪器SP2300i光谱仪与PI-MAX 1024×1024像素iCCD相机,门时间为10-9至10-8秒,可变延迟,以允许时间分辨光谱数据。
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PPPS-2013: Optical emission spectroscopy of initial plasma formation in a heavy gas theta pinch coil
Summary form only given. Pulsed inductive plasma devices such as the common theta-pinch have become a standard high energy plasma source in research and industry. Recent pulsed inductive plasmas currently being investigated by the fusion and space propulsion communities utilize deuterium and xenon, respectively, and have provided promising new results. However, little has been done to better understand the energy conversion processes during early plasma formation times (i.e., during the initial inductive coupling). The broad efforts of this research are to elucidate the electric-to-particle energy conversion processes during initial plasma formation over time scales of 10-8 to 10-6 seconds. In this work an analysis of spectral emission data is performed on a theta pinch test article intended for use in field reversed configuration (FRC) studies. Testing is performed on a pulsed xenon plasma at energies of around 80 joules, neutral back-fill pressures of 10-2 Torr, and an RLC discharge frequency of 500 kHz. Efforts are paralleled by magnetic field studies (B-dot probes, flux loops) of the same experiment. Using a collisional-radiative model previously developed for analysis on xenon Hall effect thrusters, line emission intensity ratios are used to approximate electron temperatures independent of plasma density. A Princeton Instruments SP2300i spectrometer with PI-MAX 1024×1024 pixel iCCD camera is used with gate times of 10-9 to 10-8 seconds and variable delay to allow for time-resolved spectral data.
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