Large- and Small-Scale Dynamo Action

Details Large- and Small-Scale Dynamo Action Large- and Small-Scale Dynamo Action

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..429...79h&link_type=abstract

Numerical Modeling of Space Plasma Flows, Astronum-2009, proceedings of a conference held 29 June through 3 July 2009 in Chamoni

Physics

Fluid Dynamics

Scientific paper

Providing a theoretical explanation of the generation of large-scale magnetic fields, as observed in many cosmical bodies, is a central and long-standing problem in astrophysical fluid dynamics. Traditionally it is investigated within the framework of mean field electrodynamics. Here I focus on one of the difficulties with this standard mean field formulation, namely the presence of a competing, and probably dominant, small-scale dynamo.

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