First-principles based plasma profile predictions for optimized stellarators
A. Ba\~n\'on Navarro, A. Di Siena, J. L. Velasco, F. Wilms, G. Merlo,, T. Windisch, L. L. LoDestro, J. B. Parker, and F. Jenko

TL;DR
This paper presents advanced first-principles simulations of plasma profiles in optimized stellarators, integrating turbulence, neoclassical transport, and external sources to better understand energy confinement and guide stellarator design.
Contribution
It introduces a novel coupling framework combining GENE-3D, KNOSOS, and TANGO for comprehensive plasma profile predictions in stellarators, including turbulence and neoclassical effects.
Findings
Inefficient electron-ion thermal coupling in turbulence regimes explains energy confinement degradation.
Direct ion heating can improve on-axis ion temperature in stellarators.
The framework aids in optimizing stellarator design by accurately modeling transport processes.
Abstract
In the present Letter, first-of-its-kind computer simulations predicting plasma profiles for modern optimized stellarators -- while self-consistently retaining neoclassical transport, turbulent transport with 3D effects, and external physical sources -- are presented. These simulations exploit a newly developed coupling framework involving the global gyrokinetic turbulence code GENE-3D, the neoclassical transport code KNOSOS, and the 1D transport solver TANGO. This framework is used to analyze the recently observed degradation of energy confinement in electron-heated plasmas in the Wendelstein 7-X stellarator, where the central ion temperature was "clamped" to keV regardless of the external heating power. By performing first-principles based simulations, we provide key evidence to understand this effect, namely the inefficient thermal coupling between electrons and…
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Taxonomy
TopicsMagnetic confinement fusion research · Ionosphere and magnetosphere dynamics · Particle accelerators and beam dynamics
