Observation of avalanche-like transport in Heliotron J and JT-60U plasmas

F. Kin, S. Inagaki, K. Nagasaki, M. Luo, K. Itoh, K. Shinohara, A. Terakado, T. Minami, S. Kado, Shinji Kobayashi, S. Ohshima, T. Bando, N. Oyama, M. Yoshida
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Abstract

The avalanche type of transport can induce a long-radial transport and thus can contribute to the global profile formation. In this study, we observed the heat perturbations exhibiting avalanche-like transport in the stellarator/heliotron device, Heliotron J, and the tokamak device, JT-60U. We found that the electron heat propagation in Heliotron J is mainly generated from the heating source region. The relatively high value of the Hurst exponent, which is a signature of avalanches, depends on the total heating power. On the other hand, the electron and ion heat avalanches measured in JT-60U tend to spread from the local peak of the temperature gradient and are not influenced by the heating source profiles. The contrasting features of avalanches in stellarator/heliotrons and tokamaks potentially imply the difference in the temperature profile formation, such as the presence of stiffness.
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在 Heliotron J 和 JT-60U 等离子体中观测雪崩式输运
雪崩式输运可以诱发长径向输运,从而有助于全局剖面的形成。在这项研究中,我们观测了恒星器/日中子装置 "Heliotron J "和托卡马克装置 "JT-60U "中呈现雪崩式输运的热扰动。我们发现,Heliotron J 中的电子热传播主要来自加热源区域。作为雪崩特征的赫斯特指数值相对较高,这与总加热功率有关。另一方面,在 JT-60U 中测量到的电子和离子热雪崩倾向于从温度梯度的局部峰值扩散,不受加热源剖面的影响。恒星器/日中子和托卡马克中热雪崩的对比特征可能意味着温度曲线形成的不同,例如存在硬度。
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