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Published on: February 22, 2018
Distinct Turbulence Saturation Regimes in Stellarators
G G Plunk1, P Xanthopoulos1, P Helander1
1Max-Planck-Institut für Plasmaphysik, Wendelsteinstrasse 1, 17491 Greifswald, Germany.
Ion-temperature-gradient turbulence in stellarators exhibits two saturation regimes. Petascale simulations reveal a new regime with weaker heat flux, controlled by magnetic geometry.
Area of Science:
- Plasma physics
- Fusion energy research
- Computational fluid dynamics
Background:
- Ion-temperature-gradient (ITG) turbulence is a key driver of energy loss in fusion devices.
- Previous studies in tokamaks identified a single saturation regime for ITG turbulence.
- Stellarators, with their complex 3D magnetic fields, present unique challenges for understanding plasma turbulence.
Purpose of the Study:
- To investigate the behavior of ITG turbulence in stellarator magnetic fields.
- To identify distinct saturation regimes of ITG turbulence in stellarators.
- To develop a theoretical explanation for observed turbulence behaviors.
Main Methods:
- Petascale numerical simulations of plasma turbulence in stellarator geometries.
- Development of a simplified turbulence theory to explain simulation results.
- Comparison of simulation findings with existing tokamak turbulence observations.
Main Results:
- Two distinct saturation regimes for ITG turbulence were identified in stellarators.
- The first regime, characterized by strong zonal flows, aligns with tokamak observations.
- A novel second regime was discovered, featuring quasi-two-dimensional turbulence, weak zonal flows, and reduced heat flux scaling.
Conclusions:
- Stellarator magnetic geometry significantly influences ITG turbulence dynamics.
- The newly identified second regime offers insights into optimizing stellarator performance.
- Understanding these regimes is crucial for advancing fusion energy development.
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