The DESC Stellarator Code Suite Part II: Perturbation and continuation methods
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Abstract (arXiv)
A new perturbation and continuation method is presented for computing and analyzing stellarator equilibria. The method is formally derived from a series expansion about the equilibrium condition F equiv J × B - nabla p = 0, and an efficient algorithm for computing solutions to 2nd and 3rd order perturbations is developed. The method has been implemented in the DESC stellarator equilibrium code, using automatic differentiation to compute the required derivatives. Examples are shown demonstrating its use for computing complicated equilibria, perturbing a tokamak into a stellarator, and performing parameter scans in pressure, rotational transform and boundary shape in a fraction of the time required for a full solution.
Key facts. Cited by 4 papers in the map (data through 14 Oct 2026). First posted on arXiv 29 Mar 2022.
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Citing papers per year: 2022: 1; 2023: 0; 2024: 0; 2025: 2; 2026: 1.
4 papers.
- 2022Unsupervised Discovery of Inertial-Fusion Plasma Physics using Differentiable Kinetic Simulations and a Maximum Entropy Loss Functioncited by 1
- 2025Improving ideal MHD equilibrium accuracy with physics-informed neural networkscited by 1
- 2025Narrow Operator Models of Stellarator Equilibria in Fourier Zernike Basiscited by 0
- 2026A proof-of-concept for automated AI-driven stellarator coil optimization with in-the-loop finite-element calculationscited by 0
- 2026A proof-of-concept for automated AI-driven stellarator coil optimization with in-the-loop finite-element calculations16 Mar 2026
- 2025Narrow Operator Models of Stellarator Equilibria in Fourier Zernike Basis15 Oct 2025
- 2025Improving ideal MHD equilibrium accuracy with physics-informed neural networks3 Jul 2025
- 2022Unsupervised Discovery of Inertial-Fusion Plasma Physics using Differentiable Kinetic Simulations and a Maximum Entropy Loss Function3 Jun 2022