等离子体启动过程中的电子回旋共振

IF 2.1 3区 物理与天体物理 Q2 PHYSICS, FLUIDS & PLASMAS Journal of Plasma Physics Pub Date : 2024-01-15 DOI:10.1017/s0022377823001423
C. Albert Johansson, Pavel Aleynikov
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引用次数: 0

摘要

电子-回旋共振加热(ECRH)是温德斯坦 7-X 恒星器(W7-X)的主要加热机制。虽然二次谐波 ECRH(X2)已被常规用于等离子体的启动,但已知三次谐波(X3)的启动要困难得多。在这项工作中,我们针对 W7-X 中二次和三次谐波启动的相关条件,研究了粒子在非线性波粒相互作用过程中的能量增益。我们同时考虑了光束和环境磁场的不均匀性。结果表明,环境磁场不均匀会显著增加单个波粒共振相互作用产生的平均能量增益。在类似 W7-X 的条件下,最大增益能量的提高幅度是类比均匀磁场情况下的 4 倍。然而,这种改进不足以确保 X3 启动。研究发现,在类似 W7-X 的条件下,平均能量增益和启动的最佳磁场不均匀长度尺度在 1 美元到 3 美元之间。还考虑了使用具有相邻共振的多束的可能性。结果表明,能量增益显著提高。
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Electron cyclotron resonance during plasma initiation

Electron-cyclotron resonance heating (ECRH) is the main heating mechanism in the Wendelstein 7-X (W7-X) stellarator. Although second-harmonic ECRH (X2) has been used routinely for plasma startup, startup at third harmonic (X3) is known to be much more difficult. In this work, we investigate the energy gain of particles during nonlinear wave–particle interaction for conditions relevant to second- and third-harmonic startups in W7-X. We take into account both the beam and the ambient magnetic field inhomogeneities. The latter is shown to significantly increase the mean energy gain resulting from a single wave–particle resonant interaction. In W7-X-like conditions, the improvement in maximum gained energy is up to 4 times the analogous uniform magnetic field case. However, this improvement is not enough to ensure X3 startup. The optimal magnetic field inhomogeneity length scale for average energy gain and start up in W7-X-like conditions is found to be in the range of $1$ to $3\ {\rm km}^{-1}$. A possibility of using multiple beams with neighbouring resonances is also considered. A considerable enhancement of the energy gain is demonstrated.

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来源期刊
Journal of Plasma Physics
Journal of Plasma Physics 物理-物理:流体与等离子体
CiteScore
3.50
自引率
16.00%
发文量
106
审稿时长
6-12 weeks
期刊介绍: JPP aspires to be the intellectual home of those who think of plasma physics as a fundamental discipline. The journal focuses on publishing research on laboratory plasmas (including magnetically confined and inertial fusion plasmas), space physics and plasma astrophysics that takes advantage of the rapid ongoing progress in instrumentation and computing to advance fundamental understanding of multiscale plasma physics. The Journal welcomes submissions of analytical, numerical, observational and experimental work: both original research and tutorial- or review-style papers, as well as proposals for its Lecture Notes series.
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