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Glossary

Quasi-Symmetry

A mathematical property of optimized stellarator magnetic fields that makes particle confinement nearly as good as in a tokamak — the theoretical breakthrough enabling the modern stellarator renaissance.

Reviewed Last reviewed: 9 Aug 2026 · Category: Glossary

The Problem

In a tokamak, the magnetic field strength depends only on the major radius (it is axisymmetric). This symmetry ensures that trapped-particle orbits are well-confined. In a general stellarator, the three-dimensional magnetic field breaks this symmetry, causing trapped particles to drift out of the plasma — leading to unacceptable neoclassical transport losses.[1]

The insight: In 1988, Juergen Nührenberg and Rainer Zille showed that it is possible to design stellarator magnetic fields where the field strength B, expressed in Boozer coordinates, depends on only one angular coordinate — even though the field geometry is fully three-dimensional. This “quasi-symmetry” restores the good confinement properties of axisymmetry.

Types of Quasi-Symmetry

Quasi-helical symmetry (QHS): B depends on a helical angle. Demonstrated in the HSX stellarator at the University of Wisconsin. Quasi-axisymmetry (QA): B depends on the toroidal angle (like a tokamak). Being pursued by CFQS and Princeton Stellarators. Quasi-isodynamicity (QI): All trapped particles have zero average drift. Implemented in Wendelstein 7-X.[2]

Impact

Quasi-symmetry has transformed the stellarator from a historical curiosity into a serious reactor candidate. Several private companies (Type One Energy, Princeton Stellarators, Proxima Fusion) are building on quasi-symmetric optimization for commercial stellarator designs.[3]

Sources

  1. Nührenberg, J. and Zille, R. "Quasi-helically symmetric toroidal stellarators." Physics Letters A, 129, 113, 1988.
  2. Helander, P. "Theory of plasma confinement in non-axisymmetric magnetic fields." Reports on Progress in Physics, 77, 087001, 2014.
  3. Landreman, M. and Paul, E. "Magnetic fields with precise quasisymmetry for plasma confinement." Physical Review Letters, 128, 035001, 2022.

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