Analysis of Density Profile Peaking during On-Axis ECR-Heating in the T-10 Tokamak

IF 0.5 4区 物理与天体物理 Q4 PHYSICS, NUCLEAR
V. F. Andreev, A. S. Aseev, A. A. Borshchegovskij, S. E. Lysenko, T. B. Myalton, I. N. Roy, D. S. Sergeev
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Abstract

The article presents the results of the analysis of the density profile peaking factor and the inverse density gradient scale length (IDGSL) after switching-on the on-axis electron cyclotron resonance heating (ECRH) in the T-10 tokamak. Two series of experiments with different chord-averaged densities in the ohmic regime before the ECRH switching-on are considered. In each series, the total plasma current was changed from shot to shot at a fixed chord-averaged density and the ECRH power. In this case, the ECRH power was several times higher than the ohmic heating power. It was shown that at the ECRH stage, the density profile peaking factor and the IDGSL become almost the same in each series of experiments. This circumstance indicates the formation of the “stiff” IDGSL with high-power on-axis ECRH. Such property of stiffness for the IDGSL requires its consideration in transport models, when we analyzing the density evolution.

Abstract Image

T-10托卡马克轴上ecr加热过程中密度曲线峰值分析
本文介绍了T-10型托卡马克轴向电子回旋共振加热(ECRH)开启后的密度剖面峰值因子和密度梯度尺度逆长度(IDGSL)的分析结果。在ECRH开启前,考虑了两组不同弦平均密度的欧姆区实验。在每个系列中,总等离子体电流在固定的弦平均密度和ECRH功率下从一个镜头到另一个镜头变化。在这种情况下,ECRH功率比欧姆加热功率高几倍。结果表明,在ECRH阶段,密度剖面峰值因子和IDGSL在各系列试验中几乎相同。这种情况表明具有高功率轴上ECRH的“刚性”IDGSL的形成。在分析密度演化时,这种刚度特性需要在输运模型中加以考虑。
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来源期刊
Physics of Atomic Nuclei
Physics of Atomic Nuclei 物理-物理:核物理
CiteScore
0.60
自引率
25.00%
发文量
56
审稿时长
3-6 weeks
期刊介绍: Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.
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