Flux-Surface Shaping in Stellarators and Tokamaks
Analysis
This paper addresses the challenge of characterizing and shaping magnetic fields in stellarators, crucial for achieving quasi-symmetry and efficient plasma confinement. It introduces a novel method using Fourier mode analysis to define and analyze the shapes of flux surfaces, applicable to both axisymmetric and non-axisymmetric configurations. The findings reveal a spatial resonance between shape complexity and rotation, correlating with rotational transform and field periods, offering insights into optimizing stellarator designs.
Key Takeaways
- •Introduces a new method for analyzing flux-surface shapes using Fourier mode analysis.
- •Applicable to both axisymmetric and non-axisymmetric configurations.
- •Identifies a spatial resonance between shape complexity and rotation as key to quasi-symmetry.
- •Findings correlate with rotational transform and field periods, offering design insights.
“Empirically, we find that quasi-symmetry results from a spatial resonance between shape complexity and shape rotation about the magnetic axis.”