Astronomy and Astrophysics – Astrophysics
Conducting Fluids, Dynamo Theory, Magnetohydrodynamic Turbulence, Velocity Distribution, High Reynolds Number, Magnetic Fields
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.
Carvalho Joel C.
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