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arXiv · 2211.09829

Constructing precisely quasi-isodynamic magnetic fields

Alan Goodman·Katia Camacho Mata·Sophia A Henneberg·Rogerio Jorge·Matt Landreman·Gabriel Plunk·Hakan Smith·Ralf Mackenbach·Per Helander
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Abstract

We present a novel method for numerically finding quasi-isodynamic stellarator magnetic fields with excellent fast-particle confinement and extremely small neoclassical transport. The method works particularly well in configurations with only one field period. We examine the properties of these newfound quasi-isodynamic configurations, including their bootstrap currents, particle confinement, and available energy for trapped-electron driven turbulence, as well as the degree to which they change when a finite pressure profile is added. We finally discuss the differences between the magnetic axes of the optimized solutions and their respective initial conditions, and conclude with the prospects for future quasi-isodynamic optimization.

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Alan Goodman, Katia Camacho Mata, Sophia A Henneberg, Rogerio Jorge, Matt Landreman, Gabriel Plunk, Hakan Smith, Ralf Mackenbach, Per Helander. 2022-11-17. Constructing precisely quasi-isodynamic magnetic fields. https://doi.org/10.1017/s002237782300065x

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