Constructing precisely quasi-isodynamic magnetic fields
arXiv:2211.09829 · doi:10.1017/S002237782300065X
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.
25 pages, 10 figures
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- Energetic Particle Tracing in Optimized Quasisymmetric Stellarator Equilibria
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- Piecewise omnigenous stellarators with zero bootstrap current
- Omnigenous umbilic stellarators
- Efficient Computation of Stellarator Coils with an Augmented Lagrangian Optimization Method
- Near-axis quasi-isodynamic database