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JOURNALS // Uspekhi Fizicheskikh Nauk // Archive

UFN, 1993 Volume 163, Number 11, Pages 19–56 (Mi ufn7214)

This article is cited in 97 papers

REVIEWS OF TOPICAL PROBLEMS

Particle kinetics in highly turbulent plasmas (renormalization and self-consistent field methods)

A. M. Bykova, I. N. Toptyginb

a Ioffe Institute, St. Petersburg
b Saint-Petersburg State Technical University

Abstract: This review presents methods available for calculating transport coefficients for impurity particles in plasmas with strong long-wave MHD-type velocity and magnetic-field fluctuations, and random ensembles of strong shock fronts. The renormalization of the coefficients of the mean-field equation of turbulent dynamo theory is also considered. Particular attention is devoted to the renormalization method developed by the authors in which the renormalized transport coefficients are calculated from a nonlinear transcendental equation (or a set of such equations) and are expressed in the form of explicit functions of pair correlation tensors describing turbulence. Numerical calculations are reproduced for different turbulence spectra. Spatial transport in a magnetic field and particle acceleration by strong turbulence are investigated. The theory can be used in a wide range of practical problems in plasma physics, atmospheric physics, ocean physics, astrophysics, cosmic-ray physics, and so on.

PACS: 52.35.Ra, 52.25.Fi, 52.25.Gj, 52.25.Vy, 52.30.Cv, 52.65.Vv

Received: June 25, 1993
Revised: September 30, 1993

DOI: 10.3367/UFNr.0163.199311b.0019


 English version:
Physics–Uspekhi, 1993, 36:11, 1020–1052


© Steklov Math. Inst. of RAS, 2026