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.

RT Journal
T1 Particle kinetics in highly turbulent plasmas (renormalization and self-consistent field methods)
A1 Bykov,A.M.
A1 Toptygin,I.N.
PB Physics-Uspekhi
PY 1993
FD 10 Nov, 1993
JF Physics-Uspekhi
JO Phys. Usp.
VO 36
IS 11
SP 1020-1052
DO 10.1070/PU1993v036n11ABEH002179
LK https://ufn.ru/en/articles/1993/11/b/