Quasisymmetric stellarator magnetic fields are generated by periodic KdV soliton potentials, with B approaching the 1-soliton reflectionless form near the outermost surface.
Since the QS condition has not appeared directly in the form (24c) to the best of our knowledge, let us point out its relation to one of the standard forms of QS
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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.