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First experiments on ICRF discharge generation by a W7-X-like antenna in the Uragan-2M stellarator
Journal of Plasma Physics ( IF 2.1 ) Pub Date : 2020-10-28 , DOI: 10.1017/s0022377820001099
V. E. Moiseenko , Yu. V. Kovtun , T. Wauters , A. Goriaev , A. I. Lyssoivan , A. V. Lozin , R. O. Pavlichenko , A. N. Shapoval , S. M. Maznichenko , V. B. Korovin , E. D. Kramskoy , M. M. Kozulya , N. V. Zamanov , Y. V. Siusko , A. Yu. Krasiuk , V. S. Romanov , A. Alonso , R. Brakel , A. Dinklage , D. Hartmann , Ye. Kazakov , H. Laqua , J. Ongena , T. Stange ,

In support of the ICRF experiments planned on the Wendelstein 7-X (W7-X) stellarator, i.e. fast ion generation, wall conditioning, target plasma production and heating, a first experimental study on plasma production has been made in the Uragan-2M (U-2M) stellarator using W7-X-like two-strap antenna. In all the experiments, antenna monopole phasing was used. The W7-X-like antenna operation with launched radiofrequency power of ~100 kW have been performed in helium (p = (4–14) × 10−2 Pa) with the vacuum vessel walls pre-loaded with hydrogen. Production of plasma with a density higher than 1012 cm−3 was observed near the first harmonic of the hydrogen cyclotron frequency. Operation at first hydrogen harmonic is feasible in W7-X future ICRF experiments.



中文翻译:

在Uragan-2M恒星发生器中通过类似W7-X的天线产生ICRF放电的首次实验

为了支持计划在Wendelstein 7-X(W7-X)恒星仪上进行的ICRF实验(即快速离子产生,壁调节,目标等离子体产生和加热),已在Uragan-2M中进行了等离子体产生的第一项实验研究( U-2M)恒星器,使用类似W7-X的两带天线。在所有实验中,均使用天线单极定相。已在氦气中(p  =(4-14)×10 -2 Pa)在真空容器壁中预装了氢气的情况下,发射了约100 kW的射频功率,类似W7-X的天线运行。产生密度高于10 12 cm -3的等离子体在氢回旋加速器频率的一次谐波附近观察到。在W7-X未来的ICRF实验中,第一次氢谐波操作是可行的。

更新日期:2020-10-30
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