High-$\beta$ equilibrium and ballooning stability of the low aspect ratio CNT stellarator
K. C. Hammond, S. A. Lazerson, and F. A. Volpe

TL;DR
This study predicts the existence and stability limits of low aspect ratio CNT stellarator equilibria at high plasma beta, using numerical tools to explore ballooning stability and test computational codes in such regimes.
Contribution
It provides the first numerical analysis of ballooning stability limits in low aspect ratio CNT stellarators at high beta, and evaluates the performance of stellarator codes like VMEC under these conditions.
Findings
Expected beta limits of 0.9-3.0% depending on configuration.
Indications of a second stable ballooning region.
Stability varies with aspect ratio and configuration.
Abstract
The existence and ballooning-stability of low aspect ratio stellarator equilibria is predicted for CNT with the aid of 3D numerical tools. In addition to having a low aspect ratio, CNT is characterized by a low magnetic field and small plasma volume. Also, highly overdense plasmas were recently heated in CNT by means of microwaves. These characteristics suggest that CNT might attain relatively high values of plasma and thus be of use in the experimental study of stellarator stability to high- instabilities such as ballooning modes. As a first step in that direction, here the ballooning stability limit is found numerically. Depending on the particular magnetic configuration we expect volume-averaged limits in the range 0.9-3.0%, and possibly higher, and observe indications of a second region of ballooning stability. As the aspect ratio is reduced, stability is…
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