使用直径6英寸的螺旋源在实验室环境中模拟高超声速大气条件

K. Lemmer, A. Gallimore, T.B. Smith, S. Nguyen, D. R. Austin, D. Morris, C. Davis, J. Zagel
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引用次数: 3

摘要

只提供摘要形式。当航天器重新进入大气层或高超音速飞行器飞行时,低频电磁辐射无法穿透高速飞行器周围形成的等离子体层。这干扰了来自高超音速飞行器的实时遥测,并在大气层再入期间中断了航天器通信。高超声速大气等离子体很难在实验室环境中模拟,因为它们密度高(~109 - 1011 cm-3,取决于海拔高度),温度低(~2 - 5 eV)。密歇根大学等离子动力学和电力推进实验室(PEPL)已经设计、制造并测试了一个直径6厘米的螺旋源,能够产生符合这些要求的等离子体。本文介绍了Langmuir探针、缓速电位分析仪和残余气体分析仪在氩气、氮气和空气条件下运行的数据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Simulating Hypersonic Atmospheric Conditions in a Laboratory Setting using a 6-in-Diameter Helicon Source
Summary form only given. While a spacecraft is reentering the atmosphere or a hypersonic vehicle is in flight, low-frequency electromagnetic radiation cannot penetrate the plasma layer that forms around the high speed vehicle. This interferes with real-time telemetry from hypersonic vehicles and interrupts spacecraft communications during atmospheric reentry. Hypersonic atmospheric plasmas are difficult to simulate in a laboratory setting because they are high density (~109 - 1011 cm-3 depending on altitude) and low temperature (~2 - 5 eV). A 6-cm-diameter helicon source capable of creating plasma with these requirements has been designed, fabricated and tested at the University of Michigan Plasmadynamics and Electric Propulsion Laboratory (PEPL). We present Langmuir probe, retarding potential analyzer and residual gas analyzer data from helicon source operation with argon, nitrogen and air.
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