On the interplay between plasma triangularity and micro-tearing turbulence

Abstract In this work, we study the interplay between triangularity and micro-tearing turbulence using linear and nonlinear flux tube GENE simulations. We consider scenarios with negative and positive triangularity (PT) plasma shaping taken from existing tokamaks (TCV, DIII-D, MAST-U and SMART) and EU-DEMO. The study of all these tokamaks reveals a coherent picture. Negative triangularity (NT) geometry is more susceptible to micro-tearing modes (MTMs), which, when present, make transport much worse than in PT. At sufficiently large β (the ratio of plasma pressure over magnetic pressure), magnetic shear and ratio of electron to ion temperature gradient, all the scenarios with NT are dominated by MTM turbulence. In contrast, the corresponding scenarios with PT remain dominated by electrostatic turbulence and MTMs are subdominant or stable. We observe that conventional tokamaks usually operate in a parameter space far away from the onset of this MTM-dominated regime in NT, thus preserving the beneficial effect of NT on turbulent transport. In contrast, spherical tokamaks (ST) operate close to this regime and may ultimately exhibit worse transport at NT than PT. We find that lowering the magnetic shear in STs can preserve the beneficial effect of NT on electrostatic turbulence and prevent strong MTM transport. Finally, linear and nonlinear simulations reveal the reason for stronger MTMs: the magnetic drifts are faster in the NT geometry.

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Publication Details

Journal
Plasma Physics and Controlled Fusion
Published
2025-10-14
DOI
https://doi.org/10.1088/1361-6587/ae1327
Citations
2
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
2.31

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article

On the interplay between plasma triangularity and micro-tearing turbulence

S. Coda, Justin Ball, A. Balestri
2 citations
Plasma Physics and Controlled Fusion
Solar and Space Plasma Dynamics
2.31
article

On the interplay between plasma triangularity and micro-tearing turbulence

S. Coda, Justin Ball, A. Balestri
article en
2 citations

Abstract

Abstract In this work, we study the interplay between triangularity and micro-tearing turbulence using linear and nonlinear flux tube GENE simulations. We consider scenarios with negative and positive triangularity (PT) plasma shaping taken from existing tokamaks (TCV, DIII-D, MAST-U and SMART) and EU-DEMO. The study of all these tokamaks reveals a coherent picture. Negative triangularity (NT) geometry is more susceptible to micro-tearing modes (MTMs), which, when present, make transport much worse than in PT. At sufficiently large β (the ratio of plasma pressure over magnetic pressure), magnetic shear and ratio of electron to ion temperature gradient, all the scenarios with NT are dominated by MTM turbulence. In contrast, the corresponding scenarios with PT remain dominated by electrostatic turbulence and MTMs are subdominant or stable. We observe that conventional tokamaks usually operate in a parameter space far away from the onset of this MTM-dominated regime in NT, thus preserving the beneficial effect of NT on turbulent transport. In contrast, spherical tokamaks (ST) operate close to this regime and may ultimately exhibit worse transport at NT than PT. We find that lowering the magnetic shear in STs can preserve the beneficial effect of NT on electrostatic turbulence and prevent strong MTM transport. Finally, linear and nonlinear simulations reveal the reason for stronger MTMs: the magnetic drifts are faster in the NT geometry.

Plasma Physics and Controlled FusionVol. 67(10)
École Polytechnique Fédérale de Lausanne (CH)
National Science Foundation, EUROfusion, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, China Scholarship Council, Centro Svizzero di Calcolo Scientifico, National Supercomputing Centre Singapore, Euratom Research and Training Programme, Staatssekretariat für Bildung, Forschung und Innovation, FP7 Fusion Energy Research
Openalex Percentile: Top 10%
Solar and Space Plasma Dynamics
2.31
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