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Investigation of EBW thermal emission and mode-conversion physics in the national spherical torus experiment.

机译:国家球形圆环实验中的EBW热发射和模式转换物理研究。

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摘要

NSTX is a spherical tokamak (ST) that operates with ne up to 1020 m-3 and BT less than 0.6 T, cutting off low harmonic electron cyclotron (EC) waves widely used for electron temperature measurements and EC heating and current drive in conventional aspect ratio tokamaks. The electron Bernstein wave (EBW) can propagate in ST plasmas and is readily absorbed and emitted at EC harmonics. Additionally, EBWs do not experience a density dependent cutoff. As such, EBWs may enable local electron temperature measurements and provide local electron heating and current drive. EBWs cannot propagate in vacuum but can couple to electromagnetic waves, so for these applications efficient coupling between the EBWs and electromagnetic waves outside the plasma is needed.;In this thesis, EBW emission via the oblique double mode conversion process to the X- and O-modes (B-X-O) is measured with two remotely steered antennas located outside of the vacuum vessel. These emission measurements have been used to determine the EBW transmission efficiency for a wide range of plasma conditions. The antennas collect fundamental (8-18 GHz), second and third (18-40 GHz) harmonic emission. The remote steering capability allowed detailed measurements (as a function of toroidal and poloidal pointing angle) of the B-X-O transmission window. Peak L-mode B-X-O transmission efficiencies of 90% and 35% for fundamental and second harmonic emission, respectively, were measured. The measured and theoretical optimal pointing angles agreed within 5° of the simulated values. Evidence of strong EBW collisional damping near the fundamental and second harmonic B-X-O conversion region was observed in H-mode discharges, reducing the B-X-O transmission efficiency to nearly 0% in some cases. Edge conditioning, via Li evaporation, successfully reduced this EBW damping and increased transmission efficiencies to 50-60%, agreeing with EBW emission (EBE) simulations. These results provide experimental evidence supporting B-X-O mode conversion theory and provide verification of an EBE simulation code developed at the Czech Institute of Plasma Physics. Additionally, the results presented in this thesis provide the first measurements demonstrating that EBW collisional damping can be successfully reduced with edge conditioning. Except for power dependent effects, the physics of B-X-O emission and O-X-B injection are reciprocal, thus the B-X-O mode conversion measurements support the feasibility of EBW based heating and current drive experiments for future ST devices such as an ST-based Component Test Facility.;Te(R) reconstructions of ST H-mode plasma via EBE measurements are also presented in this thesis and have been quite difficult. The B-X-O process is a complicated process, involving double mode conversion of the emission before it is detected, and an antenna view oblique to the magnetic field near the plasma edge, so that extensive numerical modeling is needed to determine the emission location and reconstruct the Te (R) profile. In contrast to stellarators or conventional aspect ratio tokamaks, reconstruction of the magnetic equilibrium in an ST is strongly affected by time varying internal currents that generate poloidal fields that can be comparable to the toroidal field. Good agreement with the edge Thomson scattering and EBE Te(R) measurements have been observed. Inside a major radius of 140 cm, EBE Te(R) measurements are within 40% of Thomson scattering measurements.
机译:NSTX是一种球形托卡马克(ST),其最大工作频率为1020 m-3,BT小于0.6 T,切断了低谐波电子回旋加速器(EC)波,该波广泛用于电子温度测量以及EC加热和常规电流驱动比托卡马克。电子伯恩斯坦波(EBW)可以在ST等离子体中传播,并且容易被EC谐波吸收和发射。此外,EBW不会遇到密度依赖的临界值。这样,EBW可以实现局部电子温度测量并提供局部电子加热和电流驱动。 EBW不能在真空中传播,但可以耦合到电磁波,因此对于这些应用,需要在EBW与等离子体外部的电磁波之间进行有效耦合。;本文中,通过斜双模转换过程将EBW发射到X和O -模式(BXO)使用位于真空容器外部的两个远程操纵天线进行测量。这些发射测量已用于确定各种等离子体条件下的EBW传输效率。天线收集基本(8-18 GHz),第二和第三(18-40 GHz)谐波发射。远程转向功能允许对B-X-O传输窗口进行详细的测量(作为环形和多角形指向角的函数)。测得基波和二次谐波的峰值L模式B-X-O传输效率分别为90%和35%。测量值和理论上的最佳指向角在模拟值的5°之内。在H型放电中,观察到在基波和二次谐波B-X-O转换区域附近有很强的EBW碰撞阻尼,这在某些情况下将B-X-O的传输效率降低到接近0%。通过锂离子蒸发进行的边缘调节成功地将EBW阻尼降低了,并将传输效率提高到50-60%,与EBW排放(EBE)模拟相吻合。这些结果提供了支持B-X-O模式转换理论的实验证据,并提供了捷克等离子物理研究所开发的EBE仿真代码的验证。此外,本文提出的结果提供了首次测量结果,证明了通过边沿调节可以成功降低EBW碰撞阻尼。除了功率相关的影响外,BXO发射和OXB注入的物理原理是相反的,因此BXO模式转换测量支持基于EBW的加热和电流驱动实验的可行性,以用于未来的ST设备,例如基于ST的组件测试设备。本文还介绍了通过EBE测量对ST H模式等离子体进行的(R)重建,而且非常困难。 BXO过程是一个复杂的过程,涉及到在检测到发射之前进行发射的双模转换,并且天线视图倾斜于等离子体边缘附近的磁场,因此需要进行广泛的数值建模来确定发射位置并重建Te (R)个人资料。与恒星器或传统的长宽比托卡马克相反,ST中磁平衡的重建受到时变内部电流的强烈影响,内部电流会产生可与环形场媲美的极向场。已经观察到与边缘Thomson散射和EBE Te(R)测量的良好一致性。在140厘米的主半径内,EBE Te(R)测量值在Thomson散射测量值的40%以内。

著录项

  • 作者

    Diem, Stephanie Josephine.;

  • 作者单位

    Princeton University.;

  • 授予单位 Princeton University.;
  • 学科 Physics Fluid and Plasma.
  • 学位 Ph.D.
  • 年度 2008
  • 页码 178 p.
  • 总页数 178
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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