# Multiscale interaction between a large scale magnetic island and small   scale turbulence

**Authors:** M. J. Choi (1), J. Kim (1), J.-M. Kwon (1), H. K. Park (1, 2), Y., In (1), W. Lee (1), K. D. Lee (1), G. S. Yun (3), J. Lee (2), M. Kim (2),, W.-H. Ko (1), J. H. Lee (1), Y. S. Park (4), Y.-S. Na (5), N. C. Luhmann Jr, (6), B. H. Park (1) ((1) National Fusion Research Institute, (2) Ulsan, National Institute of Science, Technology, (3) Pohang University of, Science, Technology, (4) Columbia University, (5) Seoul National, University, (6) University of California at Davis)

arXiv: 1705.09487 · 2017-11-22

## TL;DR

This study demonstrates the complex multiscale interactions between magnetic islands and turbulence, revealing how they influence electron heat transport and can lead to disruptions in plasma confinement.

## Contribution

It provides the first detailed measurement-based analysis of the coupled dynamics between magnetic islands and turbulence at multiple scales.

## Key findings

- Magnetic islands modify the electron temperature gradient distribution.
- T_e turbulence correlates with regions of increased T_e gradient.
- Critical levels of gradient, turbulence, and flow shear can trigger rapid heat transport and disruptions.

## Abstract

Multiscale interaction between the magnetic island and turbulence has been demonstrated through simultaneous two-dimensional measurements of turbulence and temperature and flow profiles. The magnetic island and turbulence mutually interact via the coupling between the electron temperature ($T_e$) gradient, the $T_e$ turbulence, and the poloidal flow. The $T_e$ gradient altered by the magnetic island is peaked outside and flattened inside the island. The $T_e$ turbulence can appear in the increased $T_e$ gradient regions. The combined effects of the $T_e$ gradient and the the poloidal flow shear determine two-dimensional distribution of the $T_e$ turbulence. When the reversed poloidal flow forms, it can maintain the steepest $T_e$ gradient and the magnetic island acts more like a electron heat transport barrier. Interestingly, when the $T_e$ gradient, the $T_e$ turbulence, and the flow shear increase beyond critical levels, the magnetic island turns into a fast electron heat transport channel, which directly leads to the minor disruption.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1705.09487/full.md

## References

58 references — full list in the complete paper: https://tomesphere.com/paper/1705.09487/full.md

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Source: https://tomesphere.com/paper/1705.09487