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Electron kinetic effects on interferometry and polarimetry in high temperature fusion plasmas

机译:电子动力学对高温聚变等离子体中干涉和极化的影响

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摘要

At anticipated high electron temperatures in ITER, the effects of electron thermal motion on phase measurements made by the toroidal interferometer/polarimeter (TIP) and poloidal polarimeter (PoPola) diagnostics will be significant and must be precisely treated or the measurement accuracy will fail to meet the specified requirements for ITER operation. We calculate electron thermal corrections to the interferometric phase and polarization state of an electromagnetic wave propagating along tangential and poloidal chords (Faraday and Cotton-Mouton polarimetry) and incorporate them into the Stokes vector equation for evolution of polarization. Although these corrections are small at electron temperatures T_e ∽ = 1 keV, they become sizable at T_e≥ 10 keV. The precision of the previous lowest order linear in the τ = T_e/m_ec~2 model may be insufficient; we present a more precise model with τ~2-order corrections to satisfy the high accuracy required for ITER TIP and PoPola diagnostics. Proper treatment of temperature effects will ensure more accurate interpretation of interferometric and polarimetric measurements in fusion devices like ITER and DEMO. The use of precise analytic expressions is especially important for burning plasmas where various interferometric techniques will be used for direct real time feedback control of device operations with time resolution ~1 ms to regulate the rate of the thermonuclear burn and monitor/control the safety factor profile.
机译:在预期的ITER中较高的电子温度下,电子热运动对环形干涉仪/旋光仪(TIP)和多极化旋光仪(PoPola)诊断所进行的相位测量的影响将非常显着,必须对其进行精确处理,否则测量精度将无法满足ITER操作的规定要求。我们计算沿切线和多极弦传播的电磁波的干涉相和极化状态的电子热校正(法拉第和棉木木顿极化),并将它们合并到斯托克斯矢量方程中以进行极化演化。尽管这些校正在电子温度T_e∽= 1 keV时很小,但在T_e≥10 keV时变得相当大。 τ= T_e / m_ec〜2模型中先前最低阶线性的精度可能不足;我们提出了一种具有τ〜2阶校正的更精确模型,以满足ITER TIP和PoPola诊断所需的高精度。正确处理温度效应将确保更准确地解释ITER和DEMO等聚变设备中的干涉测量和偏振测量。使用精确的解析表达式对于燃烧等离子体尤其重要,在燃烧等离子体中,各种干涉技术将用于对设备操作进行直接实时反馈控制,时间分辨率约为1 ms,以调节热核燃烧的速率并监控/控制安全系数曲线。

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  • 来源
    《Nuclear fusion》 |2013年第11期|113005.1-113005.9|共9页
  • 作者单位

    University of Wisconsin - Madison, Madison, Wisconsin, USA,Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, USA;

    University of California Los Angeles, Los Angeles, CA, USA,Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, USA;

    University of Wisconsin - Madison, Madison, Wisconsin, USA,Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, USA;

    University of California Los Angeles, Los Angeles, CA, USA,Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, USA;

    University of Wisconsin - Madison, Madison, Wisconsin, USA;

    University of Wisconsin - Madison, Madison, Wisconsin, USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);
  • 原文格式 PDF
  • 正文语种 eng
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