Abstract.
We analyze the effects of the background velocity and the initial magnetic field correlations, and viscosities on the turbulent dynamo and the \(\alpha\)-effect. We calculate the \(\alpha\)-coefficients for arbitrary magnetic and fluid viscosities, background velocity and the initial magnetic field correlations. We explicitly demonstrate that the general features of the initial growth and late-time saturation of the magnetic fields due to the non-linear feedback are qualitatively independent of these correlations. We also examine the hydrodynamic limit of the magnetic field growth in a renormalization group framework and discuss the possibilities of suppression of the dynamo growth below a critical rotation. We demonstrate that for Kolmogorov-(K41) type of spectra the Ekman number \(M \gtrsim 1/2\) for dynamo growth to occur.
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Received: 14 November 2003, Published online: 20 April 2004
PACS:
47.65. + a Magnetohydrodynamics and electrohydrodynamics - 91.25.Cw Origins and models of the magnetic field; dynamo theories
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Basu, A. Dynamo mechanism: Effects of correlations and viscosities. Eur. Phys. J. B 38, 117–126 (2004). https://doi.org/10.1140/epjb/e2004-00107-0
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DOI: https://doi.org/10.1140/epjb/e2004-00107-0