Phys. Rev. E 51, 4844 - 4859 (1995)

Diffusive processes in a stochastic magnetic field

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Hai-Da Wang, M. Vlad, E. Vanden Eijnden, F. Spineanu, J. H. Misguich, and R. Balescu
Association Euratom-Etat Belge sur la Fusion, Physique Statistique et Plasmas, Code Postal 231, Université Libre de Bruxelles, Campus Plaine, Boulevard du Triomphe, 1050 Bruxelles, Belgium
Association Euratom-Commissariat a l’Energie Atomique sur la Fusion, Département de Recherches sur la Fusion Contrôlé, Centre d’Etudes de Cadarache, 13108 Saint-Paul-lez-Durance Cedex, France

Received 31 October 1994

The statistical representation of a fluctuating (stochastic) magnetic field configuration is studied in detail. The Eulerian correlation functions of the magnetic field are determined, taking into account all geometrical constraints: these objects form a nondiagonal matrix. The Lagrangian correlations, within the reasonable Corrsin approximation, are reduced to a single scalar function, determined by an integral equation. The mean square perpendicular deviation of a geometrical point moving along a perturbed field line is determined by a nonlinear second-order differential equation. The separation of neighboring field lines in a stochastic magnetic field is studied. We find exponentiation lengths of both signs describing, in particular, a decay (on the average) of any initial anisotropy. The vanishing sum of these exponentiation lengths ensures the existence of an invariant which was overlooked in previous works. Next, the separation of a particle’s trajectory from the magnetic field line to which it was initially attached is studied by a similar method. Here too an initial phase of exponential separation appears. Assuming the existence of a final diffusive phase, anomalous diffusion coefficients are found for both weakly and strongly collisional limits. The latter is identical to the well known Rechester-Rosenbluth coefficient, which is obtained here by a more quantitative (though not entirely deductive) treatment than in earlier works.


©1995 The American Physical Society

URL: http://link.aps.org/abstract/PRE/v51/p4844
DOI: 10.1103/PhysRevE.51.4844
PACS: 52.25.Fi, 05.40.+j, 52.25.Gj, 52.35.Ra

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