A multi-scale disk dynamo model

Astronomy and Astrophysics – Astronomy

Scientific paper

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Magnetic Fields, Mhd, Turbulence

Scientific paper

We suggest to combine the mean-field description of the galactic dynamo with a shell description of small-scale turbulence for high values of hydrodynamic and magnetic Reynolds numbers. The model allows us to keep the balance of energy and realizes the kinematic and non-linear regimes of the magnetic field generation. The suggested approach gives a possibility to study the role of magnetic helicity in the generation process.

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