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Enhancement and Suppression of Heat Transfer by MHD Turbulence
Author(s) -
A. Lazarian
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/505796
Subject(s) - turbulence , physics , magnetohydrodynamics , advection , thermal diffusivity , heat transfer , mechanics , thermal conductivity , plasma , turbulence kinetic energy , mean free path , intracluster medium , k epsilon turbulence model , electron , astrophysics , computational physics , thermodynamics , galaxy cluster , nuclear physics , galaxy
We study of the effect of turbulence on heat transfer within magnetizedplasmas for energy injection velocities both larger and smaller that the Alfvenspeed. We find that in the latter regime the heat transfer is partiallysuppressed, while in the former regime the effects of turbulence depend on theintensity of driving. In fact, the scale l at which the turbulent velocity isequal the Alfven velocity is a new important parameter. When the electron meanfree path is larger than l, the stronger the the turbulence, the lower thermalconductivity by electrons is. The turbulent motions, however, induces their ownadvective heat transport, which, for the parameters of intracluster medium(ICM) provides effective heat diffusivity that exceeds the classical Spitzervalue.Comment: 4 pages, misprint corrected, published ApJL version is correc

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