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arXiv · 1903.09994

Gyrokinetic analysis and simulation of pedestals, to identify the culprits for energy losses using fingerprints

Abstract

Fusion performance in tokamaks hinges critically on the efficacy of the Edge Transport Barrier (ETB) at suppressing energy losses. The new concept of fingerprints is introduced to identify the instabilities that cause the transport losses in the ETB of many of today's experiments, from widely posited candidates. Analysis of the Gyrokinetic-Maxwell equations, and gyrokinetic simulations of experiments, find that each mode type produces characteristic ratios of transport in the various channels: density, heat and impurities. This, together with experimental observations of transport in some channel, or, of the relative size of the driving sources of channels, can identify or determine the dominant modes causing energy transport. In multiple ELMy H-mode cases that are examined, these fingerprints indicate that MHD-like modes are apparently not the dominant agent of energy transport; rather, this role is played by Micro-Tearing Modes (MTM) and Electron Temperature Gradient (ETG) modes, and in addition, possibly Ion Temperature Gradient (ITG)/Trapped Electron Modes (ITG/TEM) on JET. MHD-like modes may dominate the electron particle losses. Fluctuation frequency can also be an important means of identification, and is often closely related to the transport fingerprint. The analytical arguments unify and explain previously disparate experimental observations on multiple devices, including DIII-D, JET and ASDEX-U, and detailed simulations of two DIII-D ETBs also demonstrate and corroborate this.

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BibTeXRIS

M. Kotschenreuther, X. Liu, D. R. Hatch, S. Mahajan, L. Zheng, A. Diallo, R. Groebner, the DIII-D TEAM, J. C. Hillesheim, C. F. Maggi, C. Giroud, F. Koechl, V. Parail, S. Saarelma, E. Solano, JET Contributors, A. Chankin. 2019-03-24. Gyrokinetic analysis and simulation of pedestals, to identify the culprits for energy losses using fingerprints. https://doi.org/10.1088/1741-4326%2Fab1fa2

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