Literature DB >> 12484833

New dynamical mean-field dynamo theory and closure approach.

Eric G Blackman1, George B Field.   

Abstract

We develop a new nonlinear mean field dynamo theory that couples field growth to the time evolution of the magnetic helicity and the turbulent electromotive force, E. We show that the difference between kinetic and current helicities emerges naturally as the growth driver when the time derivative of E is coupled into the theory. The solutions predict significant field growth in a kinematic phase and a saturation rate/strength that is magnetic Reynolds number dependent/independent in agreement with numerical simulations. The amplitude of early time oscillations provides a diagnostic for the closure.

Year:  2002        PMID: 12484833     DOI: 10.1103/PhysRevLett.89.265007

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  1 in total

1.  Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF.

Authors:  Piyush Sharda; Christoph Federrath; Mark R Krumholz; Dominik R G Schleicher
Journal:  Mon Not R Astron Soc       Date:  2021-02-25       Impact factor: 5.287

  1 in total

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