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首页> 外文期刊>Nuclear fusion >Analysis of resonant fast ion distributions during combined ICRF and NBI heating with transients using neutron emission spectroscopy
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Analysis of resonant fast ion distributions during combined ICRF and NBI heating with transients using neutron emission spectroscopy

机译:使用中子发射光谱分析在瞬态ICRF和NBI联合加热过程中的共振快速离子分布

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摘要

ICRF heating at the fundamental cyclotron frequency of a hydrogen minority ion species also gives rise to a partial power absorption by deuterium ions at their second harmonic resonance. This paper studies the deuterium distributions resulting from such 2nd harmonic heating at JET using neutron emission spectroscopy data from the time of flight spectrometer TOFOR. The fast deuterium distributions are obtained over the energy range 100keV to 2 MeV. Specifically, we study how the fast deuterium distributions vary as ICRF heating is used alone as well as in combination with NBI heating. When comparing the different heating scenarios, we observed both a difference in the shapes of the distributions as well as in their absolute level. The differences are most pronounced below 0.5 MeV. Comparisons are made with corresponding distributions calculated with the code PION. We find a good agreement between the measured distributions and those calculated with PION, both in terms of their shapes as well as their amplitudes. However, we also identified a period with signs of an inverted fast ion distribution, which showed large disagreements between the modeled and measured results. Resonant interactions with tornado modes, i.e. core localized toroidal alfven eigenmodes (TAEs), are put forward as a possible explanation for the inverted distribution.
机译:在少数氢离子物种的基本回旋加速器频率下进行ICRF加热还会导致氘离子在其二次谐波共振时吸收部分功率。本文利用飞行时间光谱仪TOFOR的中子发射光谱数据研究了由JET的二次谐波加热产生的氘分布。在100keV至2 MeV的能量范围内可获得快速的氘分布。具体而言,我们研究了快速的氘分布如何随单独使用ICRF加热以及与NBI加热结合使用而变化。当比较不同的供热方案时,我们观察到分布形状及其绝对水平的差异。差异最明显的是低于0.5 MeV。与使用代码PION计算的相应分布进行比较。在形状和振幅方面,我们发现测得的分布与用PION计算的分布之间有很好的一致性。但是,我们还确定了一个周期,该周期具有快速离子分布反转的迹象,这表明在建模结果和测量结果之间存在很大分歧。提出了与龙卷风模式的共振相互作用,即核心局部环形阿尔文本征模式(TAE),作为对倒转分布的可能解释。

著录项

  • 来源
    《Nuclear fusion》 |2018年第5期|056021.1-056021.11|共11页
  • 作者单位

    Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Barcelona Supercomputing Center (BSC), Barcelona, Spain,ICREA, Pg. Lluis Companys 23, 08010 Barcelona, Spain;

    Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    CCFE, Culham Science Centre, Abingdon, Oxfordshire OX 14 3DB, United Kingdom of Great Britain and Northern Ireland;

    Instituto de Plasmas e Fusao Nuclear, Instituto Superior Tecnico, Universidade de Lisboa, 1049-001 Lisboa, Portugal;

    EUROfusion Consortium, JET, Culham Science Centre, Abingdon, OX14 3DB, United Kingdom of Great Britain and Northern Ireland;

  • 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
  • 中图分类
  • 关键词

    fast ions; radio-frequency heating; neutron spectroscopy; plasma instabilities; plasma heating;

    机译:快速离子射频加热;中子光谱;等离子体不稳定性等离子加热;

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