1992
DOI: 10.1088/0741-3335/34/6/010
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Collisionless alpha -particle confinement in stellarators

Abstract: In many stellarators-envisagcd as fusion deviccs--any a-particle which cver gets reflected (all = 0) is collisionlcssly lost in a time which is orders ofmagnitude smaller than the typical slowing-down time of =IO-' s. Two classes of stellarators to which this general picture docs not apply arc dcscribcd: quasi-helically symmetric stellarators and a class ofstellarators with vanishing bootstrap current in which the collisionless r-particle confinement sufficiently improves at finile 8. The influence of the modu… Show more

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Cited by 82 publications
(97 citation statements)
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“…Losses induced by collisionless stochastic diffusion of fast ions was introduced in Ref. [1] and further developed in Ref. [2].…”
Section: Introductionmentioning
confidence: 99%
“…Losses induced by collisionless stochastic diffusion of fast ions was introduced in Ref. [1] and further developed in Ref. [2].…”
Section: Introductionmentioning
confidence: 99%
“…Hence, closure of separatrix shapes within the plasma could be added as an additional criterion during the optimization of stellarator configurations. Minimization of fast particle loss calculated with a Monte Carlo code is often included in the set of criteria in the process of the stellarator optimization (see, e.g., [13]). However, closure of separatrix shapes within the plasma is a criterion evaluated much faster than the particle loss with a Monte Carlo code (although, admittedly, the latter criterion takes into account loss channels other than stochastic diffusion of transitioning particles).…”
Section: Discussionmentioning
confidence: 99%
“…Numerical simulations of the alpha particle behaviour [13] have shown that the alpha particle confinement in optimized configurations is indeed much better than that in traditional stellarators. Most particles in the optimized configurations, including a majority of trapped particles, are confined for times much longer than the characteristic times of the orbital motion.…”
Section: Introductionmentioning
confidence: 99%
“…For thermal particles, the problem is mitigated by collisionless detrapping associated with poloidal ExB drift, but for fast particles this helpful process is weak due to the smaller ratio of ExB to parallel speed. The scale of the fast-particle confinement problem is clearly shown in [29], which found all trapped alpha particles to be lost in ∼ 10 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 reactor parameters can be estimated as ≥ 0.1s. Fast particle confinement in modern optimized designs such as W7-X and NCSX is much improved compared to conventional stellarators [30], but remains one of the main challenges for the concept.…”
Section: Energetic Ion Confinementmentioning
confidence: 99%