A model of nonlinear evolution and saturation of the turbulent MHD dynamo

The growth and saturation of magnetic field in conducting turbulent media with large magnetic Prandtl numbers are investigated. This regime is very common in low-density hot astrophysical plasmas. During the early (kinematic) stage, weak magnetic fluctuations grow exponentially and concentrate at th...

תיאור מלא

מידע ביבליוגרפי
Main Authors: Schekochihin, A, Cowley, S, Hammett, G, Maron, J, McWilliams, J
פורמט: Journal article
שפה:English
יצא לאור: IOP Publishing 2002