Direct construction of optimized stellarator shapes. Part 3. Omnigenity near the magnetic axis
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The condition of omnigenity is investigated, and applied to the near-axis expansion of Garren & Boozer (Phys. Fluids B, vol. 3 (10), 1991a, pp. 2805–2821). Due in part to the particular analyticity requirements of the near-axis expansion, we find that, excluding quasi-symmetric solutions, only one type of omnigenity, namely quasi-isodynamicity, can be satisfied at first order in the distance from the magnetic axis. Our construction provides a parameterization of the space of such solutions, and the cylindrical reformulation and numerical method of Landreman & Sengupta (J. Plasma Phys., vol. 84 (6), 2018, 905840616); Landreman et al. (J. Plasma Phys., vol. 85 (1), 2019, 905850103), enables their efficient numerical construction.
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1984 ◽
Vol 35
(4)
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pp. 217-225
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2020 ◽
Vol 25
(6)
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pp. 997-1014
1992 ◽
Vol 03
(05)
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pp. 1019-1023
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1988 ◽
Vol 15
(6-8)
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pp. 595-602
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2020 ◽
Vol 08
(09)
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pp. 1729-1735