Magnetic geometry effects on turbulent density fluctuations in Wendelstein 7-X

Abstract Line-integrated density fluctuation measurements from the core of the optimised stellarator Wendelstein 7-X (W7-X) are studied in the context of magnetic field geometry changes. The amplitude as well as the spectral distribution of fluctuations is affected by varying the magnetic field configuration. Weaker turbulent fluctuations are observed in configurations with higher rotational transform and lower magnetic mirror depth. Simulations with the gyrokinetic codes stella and GENE-3D are used to investigate the role of magnetic geometry for the experimental observations. The stabilising effect of the high rational transform configuration is reproduced by simulations and can be associated with stronger shaping of the magnetic field. This leads to increased finite Larmor radius and local shear effects, which limit the toroidal extent of ion temperature gradient (ITG) modes. For W7-X configurations with higher magnetic mirror depth, gyrokinetic theory and simulations predict weaker fluctuations, since they are closer to having the maximum- J property, which has a stabilising effect on trapped-electron mode and ITG. The opposite trend is observed experimentally, which can therefore not be explained by geometry effects on turbulence alone.

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Publication Details

Journal
Nuclear Fusion
Published
2025-10-21
DOI
https://doi.org/10.1088/1741-4326/ae15a3
Citations
1
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
1.15
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Magnetic geometry effects on turbulent density fluctuations in Wendelstein 7-X

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1 citations
Nuclear Fusion
Solar and Space Plasma Dynamics
1.15
article

Magnetic geometry effects on turbulent density fluctuations in Wendelstein 7-X

A. Langenberg, A. Zocco, A. Bañón Navarro, S. Bozhenkov, L. Podavini, O. Grulke, E. Edlund, A. von Stechow, P. Zs. Pölöskei, N. Pablant, J.-P. Bähner, O. Ford, G. Fuchert, S. K. Hansen, F. Jenko, Thilo Romba, M. Porkoláb, E. Pasch
article en
1 citations

Abstract

Abstract Line-integrated density fluctuation measurements from the core of the optimised stellarator Wendelstein 7-X (W7-X) are studied in the context of magnetic field geometry changes. The amplitude as well as the spectral distribution of fluctuations is affected by varying the magnetic field configuration. Weaker turbulent fluctuations are observed in configurations with higher rotational transform and lower magnetic mirror depth. Simulations with the gyrokinetic codes stella and GENE-3D are used to investigate the role of magnetic geometry for the experimental observations. The stabilising effect of the high rational transform configuration is reproduced by simulations and can be associated with stronger shaping of the magnetic field. This leads to increased finite Larmor radius and local shear effects, which limit the toroidal extent of ion temperature gradient (ITG) modes. For W7-X configurations with higher magnetic mirror depth, gyrokinetic theory and simulations predict weaker fluctuations, since they are closer to having the maximum- J property, which has a stabilising effect on trapped-electron mode and ITG. The opposite trend is observed experimentally, which can therefore not be explained by geometry effects on turbulence alone.

Nuclear FusionVol. 66(1)
Princeton Plasma Physics Laboratory (US), Max Planck Institute for Plasma Physics - Greifswald (DE), Fusion (United States) (US), Plasma Technology (United States) (US), Max Planck Institute for Plasma Physics (DE), Fusion Academy (US), SUNY Cortland (US), Technical University of Denmark (DK)
Openalex Percentile: Top 16%
Solar and Space Plasma Dynamics
1.15
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