Plasma properties in the vicinity of the last closed flux surface in hydrogen and helium fusion plasma discharges

M. Dimitrova, D. Lopez-Bruna, James Paul Gunn, J. Kovačič, Vojtech Svoboda, Jan Stockel, P. Ivanova, Elmira Vasileva, Embie Hasan, R. Dejarnac, Ulises Losada, Carlos Hidalgo, T. Popov
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Abstract

The origin of the bi-Maxwellian electron energy distribution function (EEDF) observed in the scrape-off layer (SOL) of tokamak plasmas by means of Langmuir probes is still under discussion. It has been assumed that the ionization of hydrogen and deuterium neutrals by thermal electrons penetrating the SOL from the bulk plasma is the main reason for the appearance of a second Maxwellian. To validate this assumption, radial measurements of the electron temperatures and densities, or the plasma properties in helium plasmas in the GOLEM tokamak and the TJ-II stellarator were performed. The radial profiles of the low-temperature electron group densities follow the trend of the calculated radial profiles of the electron sources arising from the ionization of neutrals in both deuterium and helium plasmas in TJ-II. The difference in the radial location where the bi-Maxwellian EEDF appears can be explained by the difference in the rate coefficients for ionization of deuterium and helium. The results of probe measurements in GOLEM and the WEST tokamak divertor, at one radial location in the SOL, are compatible with the hypothesis concerning the ionization of neutral atoms and the type of the EEDF.
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氢和氦聚变等离子体放电中最后一个封闭通量面附近的等离子体特性
通过朗缪尔探针在托卡马克等离子体的刮除层(SOL)中观测到的双麦克斯韦电子能量分布函数(EEDF)的起源仍在讨论之中。人们假定,从主体等离子体穿透 SOL 的热电子使氢和氘中性电离是出现第二个麦克斯韦电子分布函数的主要原因。为了验证这一假设,对 GOLEM 托卡马克和 TJ-II 恒星器中氦等离子体的电子温度和密度或等离子体特性进行了径向测量。低温电子群密度的径向分布与氘等离子体和氦等离子体中中子电离产生的电子源的径向分布的计算结果趋势一致。氘和氦电离速率系数的不同可以解释出现双麦克斯韦EEDF的径向位置的差异。在 GOLEM 和 WEST 托卡马克分流器中对 SOL 的一个径向位置进行的探测测量结果与有关中性原子电离和 EEDF 类型的假设相吻合。
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