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

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

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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...

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Xehetasun bibliografikoak
Egile Nagusiak:	Schekochihin, A, Cowley, S, Hammett, G, Maron, J, McWilliams, J
Formatua:	Journal article
Hizkuntza:	English
Argitaratua:	IOP Publishing 2002

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