HIGHLIGHTS
- What: The authors propose a more general model that is applicable to both quasiaxisymmetric and quasi-helically symmetric stellarators far from axisymmetry. The former corresponds to the equilibrium limit of the Strauss equations, and so the authors focus on the latter. Having derived the model, the authors now show that adding an O( ) correction to χ will not change it. Next, the authors show that (3.3) is equivalent to the σ -equation of Jorge et_al .
- Who: Nikita Nikulsin and colleagues from the Published by Cambridge University Press , Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA . . .
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