Quasisymmetric stellarator magnetic fields are generated by periodic KdV soliton potentials, with B approaching the 1-soliton reflectionless form near the outermost surface.
We choose the orthogonal triad (ˆx, ˆy, ˆz) such that ˆx is aligned with the unit vector ˆt along the magnetic field Bs
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Periodic Korteweg-de Vries soliton potentials generate quasisymmetric magnetic fields
Quasisymmetric stellarator magnetic fields are generated by periodic KdV soliton potentials, with B approaching the 1-soliton reflectionless form near the outermost surface.