# Optimization of flux-surface density variation in stellarator plasmas   with respect to the transport of collisional impurities

**Authors:** Stefan Buller, H{\aa}kan M. Smith, Albert Moll\'en, Sarah Louise, Newton, Istvan Pusztai

arXiv: 1812.09194 · 2019-04-15

## TL;DR

This paper develops a semi-analytic method to optimize flux-surface impurity density variations in stellarators, aiming to reduce impurity accumulation and improve plasma purity in steady-state operation.

## Contribution

It introduces a numerical optimization approach for impurity density-variations on flux-surfaces, demonstrating significant impurity reduction in stellarator configurations.

## Key findings

- Optimized impurity density-variations can reduce core impurity density by up to 75% in LHD.
- In Wendelstein 7-X, impurity reduction reaches up to 89%.
- Controlling impurity density-variations can significantly influence impurity peaking factors.

## Abstract

Avoiding impurity accumulation is a requirement for steady-state stellarator operation. The accumulation of impurities can be heavily affected by variations in their density on the flux-surface. Using recently derived semi-analytic expressions for the transport of a collisional impurity species with high-$Z$ and flux-surface density-variation in the presence of a low-collisionality bulk ion species, we numerically optimize the impurity density-variation on the flux-surface to minimize the radial peaking factor of the impurities. These optimized density-variations can reduce the core impurity density by $0.75^Z$ (with $Z$ the impurity charge number) in the Large Helical Device case considered here, and by $0.89^Z$ in a Wendelstein 7-X standard configuration case. On the other hand, when the same procedure is used to find density-variations that maximize the peaking factor, it is notably increased compared to the case with no density-variation. This highlights the potential importance of measuring and controlling these variations in experiments.

## Full text

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## Figures

48 figures with captions in the complete paper: https://tomesphere.com/paper/1812.09194/full.md

## References

30 references — full list in the complete paper: https://tomesphere.com/paper/1812.09194/full.md

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Source: https://tomesphere.com/paper/1812.09194