Prevention of core particle depletion in stellarators by turbulence

In reactor-relevant plasmas, neoclassical transport drives an outward particle flux in the core of large stellarators and predicts strongly hollow density profiles. However, this theoretical prediction is contradicted by experiments. In particular, in Wendelstein 7-X, the first large optimized stell...

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Main Authors: Thienpondt, H, García-Regaña, JM, Calvo, I, Alonso, JA, Velasco, JL, González-Jerez, A, Barnes, M, Brunner, K, Ford, O, Fuchert, G, Knauer, J, Pasch, E, Vanó, L
Format: Journal article
Language:English
Published: American Physical Society 2023
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author Thienpondt, H
García-Regaña, JM
Calvo, I
Alonso, JA
Velasco, JL
González-Jerez, A
Barnes, M
Brunner, K
Ford, O
Fuchert, G
Knauer, J
Pasch, E
Vanó, L
author_facet Thienpondt, H
García-Regaña, JM
Calvo, I
Alonso, JA
Velasco, JL
González-Jerez, A
Barnes, M
Brunner, K
Ford, O
Fuchert, G
Knauer, J
Pasch, E
Vanó, L
author_sort Thienpondt, H
collection OXFORD
description In reactor-relevant plasmas, neoclassical transport drives an outward particle flux in the core of large stellarators and predicts strongly hollow density profiles. However, this theoretical prediction is contradicted by experiments. In particular, in Wendelstein 7-X, the first large optimized stellarator, flat or weakly peaked density profiles are generally measured, indicating that neoclassical theory is not sufficient and that an inward contribution to the particle flux is missing in the core. In this Research Letter, it is shown that the turbulent contribution to the particle flux can explain the difference between experimental measurements and neoclassical predictions. The results of this Research Letter also prove that theoretical and numerical tools are approaching the level of maturity needed for the prediction of equilibrium density profiles in stellarator plasmas, which is a fundamental requirement for the design of operation scenarios of present devices and future reactors.
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spelling oxford-uuid:1cb32525-5b00-47c8-b8a7-b644160dea492023-10-17T09:15:48ZPrevention of core particle depletion in stellarators by turbulenceJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:1cb32525-5b00-47c8-b8a7-b644160dea49EnglishSymplectic ElementsAmerican Physical Society2023Thienpondt, HGarcía-Regaña, JMCalvo, IAlonso, JAVelasco, JLGonzález-Jerez, ABarnes, MBrunner, KFord, OFuchert, GKnauer, JPasch, EVanó, LIn reactor-relevant plasmas, neoclassical transport drives an outward particle flux in the core of large stellarators and predicts strongly hollow density profiles. However, this theoretical prediction is contradicted by experiments. In particular, in Wendelstein 7-X, the first large optimized stellarator, flat or weakly peaked density profiles are generally measured, indicating that neoclassical theory is not sufficient and that an inward contribution to the particle flux is missing in the core. In this Research Letter, it is shown that the turbulent contribution to the particle flux can explain the difference between experimental measurements and neoclassical predictions. The results of this Research Letter also prove that theoretical and numerical tools are approaching the level of maturity needed for the prediction of equilibrium density profiles in stellarator plasmas, which is a fundamental requirement for the design of operation scenarios of present devices and future reactors.
spellingShingle Thienpondt, H
García-Regaña, JM
Calvo, I
Alonso, JA
Velasco, JL
González-Jerez, A
Barnes, M
Brunner, K
Ford, O
Fuchert, G
Knauer, J
Pasch, E
Vanó, L
Prevention of core particle depletion in stellarators by turbulence
title Prevention of core particle depletion in stellarators by turbulence
title_full Prevention of core particle depletion in stellarators by turbulence
title_fullStr Prevention of core particle depletion in stellarators by turbulence
title_full_unstemmed Prevention of core particle depletion in stellarators by turbulence
title_short Prevention of core particle depletion in stellarators by turbulence
title_sort prevention of core particle depletion in stellarators by turbulence
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