1976
DOI: 10.1515/zna-1976-1102
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Equilibrium and Stability of a Three-Dimensional Toroidal MHD Configuration Near its Magnetic Axis

Abstract: M onodentate, Semicarbazone, Thiosem icarbazone, But-2-yne, Tungsten(II) Reaction of [W I(C O )(N C M e)(dppm )(772 -M eC2M e)][BF4] {dppm = Ph2 P(C H 2 )PPh2} with an equim olar quantity of L {L = R R 'C N N H C O N H 2 (R = R ' = Me; R = H, R ' = Ph)} or L {L = R R 'C N N H C S N H 2 (R = R ' = Me, Et; R = Me, R ' = E t, Pr", Bu', Ph; R = H, R ' = Ph)} gives the m onodentately coordinated sem icarbazone or thiosem icarbazone products [W I(CO)L(dppm)(?7 2 -M eC2M e)][BF4] (1 -9 ) . 13C N M R spectroscopy sugg… Show more

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Cited by 26 publications
(24 citation statements)
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“…In a quite different region of the W7-X configuration space at low-ῑ a and very high b 01 > 0.2, a vacuum magnetic hill appears [27]. These configurations are predicted to be Mercier unstable similarly to the inward-shifted LHD configurations [14,28].…”
Section: B the Main Fourier Modes Of W7-x Configurationsmentioning
confidence: 99%
“…In a quite different region of the W7-X configuration space at low-ῑ a and very high b 01 > 0.2, a vacuum magnetic hill appears [27]. These configurations are predicted to be Mercier unstable similarly to the inward-shifted LHD configurations [14,28].…”
Section: B the Main Fourier Modes Of W7-x Configurationsmentioning
confidence: 99%
“…From an expansion of Maxwell's equations in the vicinity of the magnetic axis, the average number of poloidal turns of a field line in one toroidal revolution can be expressed as an integral along the length l once around the magnetic axis [4,5],…”
Section: Magnetic Fieldmentioning
confidence: 99%
“…Weights are chosen to combine multiple objectives into a single objective function, and one is left wondering whether a different choice of weights might lead to promising magnetic configurations in a different region of parameter space. An older approach for relating stellarator geometry to physics properties is to make an asymptotic expansion in large local aspect ratio (Mercier 1964; Solov'ev & Shafranov 1970; Mercier & Luc 1974; Lortz & Nührenberg 1976; Garren & Boozer 1991 b ). Such an expansion is accurate in the core of any stellarator, even those for which the aspect ratio of the boundary is low (Landreman 2019).…”
Section: Introductionmentioning
confidence: 99%