Systematics of Dynamo Action in a Shell Model for Magnetohydrodynamic Turbulence

Details Systematics of Dynamo Action in a Shell Model for Magnetohydrodynamic Turbulence Systematics of Dynamo Action in a Shell Model for Magnetohydrodynamic Turbulence

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ihy..worke..59s&link_type=abstract

2nd UN/NASA Workshop on International Heliophysical Year and Basic Space Science. Proceedings of the conference held 27 Novembe

Astronomy and Astrophysics

Astrophysics

Scientific paper

We carry out high-resolution studies of the dynamo effect in a shell model for magnetohydrodynamic (MHD) turbulence at low magnetic Prandtl numbers (as low as 105). We present the stability diagram for the formation of a turbulent dynamo in this MHD shell model in magnetic Prandtl number and magnetic Reynolds number plane. Our systematic numerical studies show that a fractal-like boundary separates the dynamo and no dynamo regimes in this plane.

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