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Issue A&A
Volume 427, Number 1, November III 2004
Page(s) 13 - 21
Section Astrophysical processes
DOI http://dx.doi.org/10.1051/0004-6361:20047086



A&A 427, 13-21 (2004)
DOI: 10.1051/0004-6361:20047086

Catastrophic alpha quenching alleviated by helicity flux and shear

A. Brandenburg1 and C. Sandin2

1  NORDITA, Blegdamsvej 17, 2100 Copenhagen Ø, Denmark
    e-mail: brandenb@nordita.dk
2  Astrophysical Institute Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
    e-mail: CSandin@aip.de

(Received 16 January 2004 / Accepted 21 July 2004)

Abstract
A new simulation set-up is proposed for studying mean field dynamo action. The model combines the computational advantages of local Cartesian geometry with the ability to include a shear profile that resembles the sun's differential rotation at low latitudes. It is shown that in a two-dimensional mean field model this geometry produces cyclic solutions with dynamo waves traveling away from the equator - as expected for a positive alpha effect in the northern hemisphere. In three dimensions with turbulence driven by a helical forcing function, an alpha effect is self-consistently generated in the presence of a finite imposed toroidal magnetic field. The results suggest that, due to a finite flux of current helicity out of the domain, alpha quenching appears to be non-catastrophic - at least for intermediate values of the magnetic Reynolds number. For larger values of the magnetic Reynolds number, however, there is evidence for a reversal of the trend and that $\alpha$ may decrease with increasing magnetic Reynolds number. Control experiments with closed boundaries confirm that in the absence of a current helicity flux, but with shear as before, alpha quenching is always catastrophic and alpha decreases inversely proportional to the magnetic Reynolds number. For solar parameters, our results suggest a current helicity flux of about $0.001\,{\rm G^2\!/s}$. This corresponds to a magnetic helicity flux, integrated over the northern hemisphere and over the 11 year solar cycle, of about $10^{46}\,{\rm Mx}^2$.


Key words: magnetohydrodynamics (MHD) -- turbulence -- Sun: magnetic fields




© ESO 2004


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