1. Impact of Magnetic Field Configuration on Heat Transport in Stellarators and Heliotrons
- Author
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Felix, Warmer, K, Tanaka, P, Xanthopoulos, M, Nunami, M, Nakata, C D, Beidler, S A, Bozhenkov, M N A, Beurskens, K J, Brunner, O P, Ford, G, Fuchert, H, Funaba, J, Geiger, D, Gradic, K, Ida, H, Igami, S, Kubo, A, Langenberg, H P, Laqua, S, Lazerson, T, Morisaki, M, Osakabe, N, Pablant, E, Pasch, B, Peterson, S, Satake, R, Seki, T, Shimozuma, H M, Smith, T, Stange, A V, Stechow, H, Sugama, Y, Suzuki, H, Takahashi, T, Tokuzawa, T, Tsujimura, Y, Turkin, R C, Wolf, I, Yamada, R, Yanai, R, Yasuhara, M, Yokoyama, Y, Yoshimura, M, Yoshinuma, D, Zhang, W-X Team, Lhd Experimental Group, W7-X Team, Max Planck Institute for Plasma Physics, Max Planck Society, and LHD Experimental Group
- Subjects
Physics ,Condensed matter physics ,0103 physical sciences ,General Physics and Astronomy ,010306 general physics ,01 natural sciences ,010305 fluids & plasmas ,Magnetic field - Abstract
We assess the magnetic field configuration in modern fusion devices by comparing experiments with the same heating power, between a stellarator and a heliotron. The key role of turbulence is evident in the optimized stellarator, while neoclassical processes largely determine the transport in the heliotron device. Gyrokinetic simulations elucidate the underlying mechanisms promoting stronger ion scale turbulence in the stellarator. Similar plasma performances in these experiments suggests that neoclassical and turbulent transport should both be optimized in next step reactor designs.
- Published
- 2021