Spatial Structure and Field-Line Diffusion in Transverse Magnetic Turbulence

W. H. Matthaeus, P. C. Gray, D. H. Pontius, Jr., and J. W. Bieber
Phys. Rev. Lett. 75, 2136 – Published 11 September 1995
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Abstract

We examine magnetic surfaces and randomization of field lines with fluctuations transverse to a uniform magnetic field. Analogy with passive scalar transport in inviscid 2D flow provides realizations of magnetic surfaces and motivates a nonperturbative statistical approach. The stochastic wandering of magnetic field lines leads to diffusive perpendicular transport. For two-component fluctuations, appropriate for solar wind turbulence, the diffusion coefficient is a nonadditive combination of slab and 2D coefficients, approaching the latter in the small amplitude limit.

  • Received 27 April 1995

DOI:https://doi.org/10.1103/PhysRevLett.75.2136

©1995 American Physical Society

Authors & Affiliations

W. H. Matthaeus, P. C. Gray, D. H. Pontius, Jr., and J. W. Bieber

  • Bartol Research Institute, University of Delaware, Newark, Delaware 19716

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Issue

Vol. 75, Iss. 11 — 11 September 1995

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