1980
DOI: 10.1017/s0022377800010400
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Plasma equilibrium in toroidal l = 3 stellarators

Abstract: The equations of MHD equilibrium are solved by including plasma pressure and current in a large aspect-ratio ordering scheme for the calculation of toroidal, l = 3 stellarator vacuum fields. The extended ordering unifies the low-beta equilibrium theory for tokamaks and l = 3 stellarators, and allows solutions to be obtained simply for arbitrarily prescribed pressure and current density profiles. Expressions are given for the equilibrium magnetic field and the equation for the flux surfaces is calculated, inclu… Show more

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Cited by 12 publications
(12 citation statements)
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“…An attractive coil configuration having been decided on, it was possible to check that the values of N c , p and t were consistent by field line following. An MHD equilibrium calculation [5,6] provided confirmation that the assumed beta value could be sustained in equilibrium.…”
Section: Introductionmentioning
confidence: 87%
“…An attractive coil configuration having been decided on, it was possible to check that the values of N c , p and t were consistent by field line following. An MHD equilibrium calculation [5,6] provided confirmation that the assumed beta value could be sustained in equilibrium.…”
Section: Introductionmentioning
confidence: 87%
“…Hitchon and Fielding [32] applied a large-aspect-ratio ordering scheme to the problem of low-beta MHD equilibrium in an £ = 3 stellarator and obtained solutions for arbitrarily prescribed pressure and current density profiles. The results were used to calculate equilibria for the CLEO stellarator parameters [33 ]; also, the role of the vertical field in reducing pressure-induced flux surface distortion was examined. Experimentally, it had been found necessary to apply a vertical field to obtain the high-beta plasma with neutral injection.…”
Section: Further Theory and Reactor Studymentioning
confidence: 99%
“…( 2), we begin by rewriting it as 6. = p 6 ( s i n n (cose -hp ) -cosn s i n e } (11) which is oscillatory in p0 and the amplitude of which is (hp ) 2 -2h P cose] 1 / 2 (12) We have already noted that the ripple vanishes at p 0 = h" 1 , 6 = 0; let us define a dimensionless length z 0 = h" 1 . Then Eq.…”
Section: Model Fieldmentioning
confidence: 99%