How Does The Magnetic Gradient Scale Length Influence Complexity of Filamentary Coils in Stellarators?
John Kappel, Matt Landreman, Philipp Jura\v{s}i\'c, and Sophia A Henneberg

TL;DR
This study investigates how the magnetic gradient scale length (L_gradB) influences the complexity and proximity of filamentary coils in stellarators, demonstrating that optimizing L_gradB can improve coil design and plasma confinement.
Contribution
The paper shows that the magnetic gradient scale length correlates with coil-surface distance for filament coils and introduces optimization strategies to enhance stellarator coil configurations.
Findings
min(L_gradB) correlates with coil-surface and coil-coil distances
Optimizing min(L_gradB) can improve plasma confinement
Increasing coil-surface distance reduces coil ripple and particle loss
Abstract
The distance between the last closed flux surface (LCFS) and the nearest electromagnetic coils is a dominating factor in the cost, size, and engineering difficulty of stellarators. The smallest magnetic gradient scale length on the LCFS - denoted L_gradB - has been shown to be a good proxy for minimum coil-surface distance in optimizations of a current potential on a winding surface, such as through the REGCOIL method. However, it has not been shown the same is true for filament coils, or that the magnetic gradient scale length is an effective objective function in optimization. In this paper, we explore examples in which min(L_gradB) is correlated with the minimum coil-surface distance for filament coils. First, we analyze a subset of the single-stage-optimized equilibria from the QUASR dataset [Giuliani et al. JPP (2024)]. We find that the majority of configurations have min(L_gradB)…
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Taxonomy
TopicsMagnetic confinement fusion research · Solar and Space Plasma Dynamics · Particle accelerators and beam dynamics
