1994
DOI: 10.1088/0741-3335/36/2/007
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Ripple transport in helical-axis advanced stellarators: a comparison with classical stellarator/torsatrons

Abstract: Calculations of the neoclassical tEUiSpofi rates due to particles trapped in the helical ripples of a stellarator's magnetic field are carried out based on solutions of the bounce-averaged kinetic equation. These calculations employ amodel forthe magnetic field strength, B, whichir. m accurate approximation to the actual B far a wide variety of stellarator-type devices, amone, which are Helical-Axis Advanced Stellmtors (Hdizs) as well as conventional stellarators and torsatrons. Comparisons are cmied out in wh… Show more

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Cited by 65 publications
(60 citation statements)
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“…The simulation results are 15%-50% lower than that in the experimental values which include both the anomalous and neoclassical contributions to the transport. If we subtract the neoclassical part calculated by the GSRAKE code, 23 the simulation results agree well with the anomalous part of P i , such that the observed differences are less than 10% for q ¼ 0:46; 0:65, and about 30% for q ¼ 0:83 (see also Table I for the ion heat diffusivity v i ). Figure 3 shows the poloidal wavenumber spectra of the turbulent density fluctuation obtained from the PCI measurement and the simulation, where k y is treated as the poloidal wavenumber in the coordinates used in the simulation.…”
Section: -2supporting
confidence: 54%
“…The simulation results are 15%-50% lower than that in the experimental values which include both the anomalous and neoclassical contributions to the transport. If we subtract the neoclassical part calculated by the GSRAKE code, 23 the simulation results agree well with the anomalous part of P i , such that the observed differences are less than 10% for q ¼ 0:46; 0:65, and about 30% for q ¼ 0:83 (see also Table I for the ion heat diffusivity v i ). Figure 3 shows the poloidal wavenumber spectra of the turbulent density fluctuation obtained from the PCI measurement and the simulation, where k y is treated as the poloidal wavenumber in the coordinates used in the simulation.…”
Section: -2supporting
confidence: 54%
“…Power balance analysis was conducted using the PROCTR code [4], and neoclassical transport coefficients were calculated using the GSRAKE code [5]. In stellarator/heliotron devices, neoclassical transport is strongly af- fected by the radial electric field (E r ).…”
Section: Transport Analysis Of High T I Dischargementioning
confidence: 99%
“…For the simplest picture of helical devices, the transport scales either as ν 1/2 or ν, depending on whether collisions or drifts are responsible for removing the particles from local ripples. It is possible to determine the mono-energetic diffusion coefficient, D, in each of these three lmfp regimes from asymptotic solutions of the kinetic equation and the scalings obtained may be summarized as [6,12,13] , , ,…”
Section: Neoclassical Transport Theory In Low-collisional Helical Plamentioning
confidence: 99%