Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.168..183c&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 168, no. 2, June 1990, p. 183-191.
Astronomy and Astrophysics
Astrophysics
1
Conducting Fluids, Dynamo Theory, Magnetohydrodynamic Turbulence, Velocity Distribution, High Reynolds Number, Magnetic Fields
Scientific paper
The kinematic turbulent dynamo equations are studied in the presence of a large-scale velocity field. The two length-scales approach is employed, and solutions of the equations are found in the limit of small bulk motion and shear, and for large Reynolds number Rm. The regeneration term is calculated up to second-order in 1/Rm using cyclonic convective turbulent velocity field.
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