2004
DOI: 10.1103/physreve.70.046409
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Intrinsic trapping of stochastic sheared magnetic field lines

Abstract: The decorrelation trajectory method is applied to the diffusion of magnetic field lines in a perturbed sheared slab magnetic configuration. Some interesting decorrelation trajectories for several values of the magnetic Kubo number and of the shear parameter are exhibited. The asymmetry of the decorrelation trajectories appears in comparison with those obtained in the purely electrostatic case studied in earlier work. The running and asymptotic diffusion tensor components are calculated and displayed.

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Cited by 14 publications
(24 citation statements)
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“…In [13] this method was applied to calculate the diffusion coefficients in the slab geometry. It is interesting that for a relatively small magnetic turbulence (Kubo number = 0.1) and a shearless situation, the results obtained by the authors of [13] are similar with those obtained by us. The influence of the magnetic shear on the thermal diffusivity should be explored.…”
Section: Discussionmentioning
confidence: 99%
“…In [13] this method was applied to calculate the diffusion coefficients in the slab geometry. It is interesting that for a relatively small magnetic turbulence (Kubo number = 0.1) and a shearless situation, the results obtained by the authors of [13] are similar with those obtained by us. The influence of the magnetic shear on the thermal diffusivity should be explored.…”
Section: Discussionmentioning
confidence: 99%
“…is taken as a Gaussian random field, spatially homogeneous (in the statistical sense) in the (X, Y )-plane, and stationary (again in the statistical sense). The Eulerian auto-correlation function is taken as [23] M(X; Z) = (0; 0) (X;…”
Section: B(x; Z)mentioning
confidence: 99%
“…the appearance of spatially coherent structures in the radial or poloidal direction, such as zonal flows or streamers (see, e.g., [3]). We thus determine the diffusion coefficients for different levels of magnetic turbulence, whose intensity can be measured by the dimensionless magnetic Kubo number K m (see, e.g., [19,20,[22][23][24]), different plasma temperatures (expressed in terms of the dimensionless drift Kubo number K dr ) and different degrees of anisotropy in the magnetic fluctuations (described by the stochastic anisotropy parameter ). The impurities considered here are He, Be, Ne and W, all assumed to be fully ionized.…”
Section: Introductionmentioning
confidence: 99%
“…The stabilizing effect produced by a sheared magnetic field on bound eigenmodes [44], or, alternatively, the instability for wavelengths below the ion Larmor scale [45] are not considered here. The effects of the magnetic shear on transport were studied using DTM in [46], which enables the extension of the present study to more complex confining configuration.…”
Section: Test Modesmentioning
confidence: 99%