Least-elongated stellarator plasma boundary
Find the least elongated stellarator plasma boundary with aspect ratio at most 4, average triangularity at most −0.5 and edge iota per period at least 0.3.
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| 1 | +# Least-elongated stellarator plasma boundary | |
| 2 | + | |
| 3 | +Find the outer shape of a stellarator plasma whose cross-sections are as round as possible while meeting fixed targets on compactness, triangularity and the twist of the magnetic field lines. It is the entry-level problem of the ConStellaration benchmark, posed to lower the entry barrier to stellarator design for optimization and machine-learning researchers. | |
| 4 | + | |
| 5 | +## Task | |
| 6 | + | |
| 7 | +A candidate is a stellarator-symmetric plasma boundary, written as a truncated Fourier series in cylindrical coordinates $(R,\phi,Z)$: | |
| 8 | + | |
| 9 | +$$R(\theta,\phi)=\sum_{m,n}R_{mn}\cos(m\theta-N_{\mathrm{fp}}n\phi),\qquad Z(\theta,\phi)=\sum_{m,n}Z_{mn}\sin(m\theta-N_{\mathrm{fp}}n\phi),$$ | |
| 10 | + | |
| 11 | +where $\theta$ and $\phi$ are poloidal and toroidal angles and $N_{\mathrm{fp}}$, the number of field periods, is also chosen by the designer. The forward model computes the vacuum ideal-MHD equilibrium inside the boundary with VMEC++ and returns the metrics used below. The problem is | |
| 12 | + | |
| 13 | +$$\min\ \epsilon_{\max}\quad\text{subject to}\quad A\le 4,\qquad \bar\delta\le-0.5,\qquad \lvert\tilde\iota\rvert\ge 0.3,$$ | |
| 14 | + | |
| 15 | +where $\epsilon_{\max}$ is the largest elongation among the boundary cross-sections, $A$ the aspect ratio (major over minor radius), $\bar\delta$ the triangularity averaged over the two symmetric cross-sections $\phi=0$ and $\phi=\pi/N_{\mathrm{fp}}$, and $\tilde\iota$ the edge rotational transform divided by $N_{\mathrm{fp}}$. A design is feasible when every normalized constraint violation $(c_i-c_i^*)/\lvert c_i^*\rvert$ is at most $0.01$. The score is | |
| 16 | + | |
| 17 | +$$s=\min\Big(1,\ \max\Big(0,\ 1-\frac{\epsilon_{\max}-1}{9}\Big)\Big)$$ | |
| 18 | + | |
| 19 | +for a feasible design and $0$ otherwise; higher is better, and circular cross-sections would score 1. | |
| 20 | + | |
| 21 | +## Background | |
| 22 | + | |
| 23 | +Stellarators confine a fusion plasma with external coils alone, which shape twisted magnetic surfaces, so they need no large plasma current and avoid current-driven disruptions; the price is a hard, high-dimensional shape-design problem. ConStellaration (Cadena et al., NeurIPS 2025) was released by Proxima Fusion with a dataset of about 158,000 quasi-isodynamic-like boundaries and their equilibria, and three optimization problems of increasing difficulty. This first one is purely geometric: no confinement or stability property is imposed, so it isolates the optimizer and the choice of boundary parameterization, and it shares its forward model with the two physics problems. | |
| 24 | + | |
| 25 | +## Data and evaluation | |
| 26 | + | |
| 27 | +- **Instances:** one fixed problem. The [dataset](https://huggingface.co/datasets/proxima-fusion/constellaration) and all public leaderboard submissions ([results dataset](https://huggingface.co/datasets/proxima-fusion/constellaration-bench-results)) can serve as starting points. | |
| 28 | +- **Evaluation code:** `constellaration==0.2.6`, `problems.GeometricalProblem().evaluate(boundary)`, which runs VMEC++ at its high-fidelity setting. The [leaderboard](https://huggingface.co/spaces/proxima-fusion/constellaration-bench) scores every submission with exactly this release; later releases give different numbers. A submission is one boundary as `SurfaceRZFourier` JSON. | |
| 29 | +- **Hardware:** none assumed; the score does not depend on run time. | |
| 30 | + | |
| 31 | +## What is known | |
| 32 | + | |
| 33 | +- Paper baseline (Cadena et al., 2025): an augmented-Lagrangian method with the NGOpt optimizer, seeded from a rotating ellipse with three field periods and Fourier modes up to 4, reached $\epsilon_{\max}=1.27$ and a score of 0.969 after 18 hours on 96 vCPUs. SciPy's trust-constr and COBYQA found no feasible design. | |
| 34 | +- Weißberg et al. (2026) refined the top leaderboard designs with an augmented-Lagrangian loop around L-BFGS, using finite-difference gradients through VMEC++; one refined design scored 0.9763 in their study, and their submitted entry (0.97440 on the leaderboard) took first place in May 2026. | |
| 35 | +- Best on the leaderboard on 2026-10-20: 0.98048 (user canyon-ant, September 2026), which corresponds to $\epsilon_{\max}\approx1.176$. | |
| 36 | + | |
| 37 | +## What would count as progress | |
| 38 | + | |
| 39 | +- A boundary scoring above 0.98048 under `constellaration==0.2.6`, submitted as JSON; the check is a single forward-model evaluation that anyone can rerun. | |
| 40 | +- A method that reaches at least 0.98 from a rotating-ellipse start, without seeding from published leaderboard designs, with its code. | |
| 41 | +- A study of how the best achievable $\epsilon_{\max}$ depends on $N_{\mathrm{fp}}$, with the best boundary for each value. | |
| 42 | + | |
| 43 | +## References | |
| 44 | + | |
| 45 | +1. S. A. Cadena, A. Merlo, E. Laude, et al. ConStellaration: A dataset of QI-like stellarator plasma boundaries and optimization benchmarks. NeurIPS 2025 Datasets and Benchmarks Track. [arXiv:2506.19583](https://arxiv.org/abs/2506.19583) | |
| 46 | +2. J. Schilling. The numerics of VMEC++. 2025. [arXiv:2502.04374](https://arxiv.org/abs/2502.04374) | |
| 47 | +3. T. Weißberg, M. Heep, Z. Lähner, F. Bernard. Towards stellarator geometry optimisation for nuclear fusion. 2026. [arXiv:2608.28224](https://arxiv.org/abs/2608.28224) | |
| 48 | +4. Proxima Fusion. ConStellaration code, release v0.2.6. [GitHub](https://github.com/proximafusion/constellaration/releases/tag/v0.2.6) | |
| 49 | + | |
| 50 | +## Source | |
| 51 | + | |
| 52 | +Imported from [ConStellaration geometrical problem](https://github.com/proximafusion/constellaration/blob/v0.2.6/src/constellaration/problems.py#L113), curated by Proxima Fusion. Open according to the source as of 2026-10-20. The statement above is written in our own words; see the source for the original wording, history and discussion. | |