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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. Sandin21 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
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
.
This corresponds to a magnetic helicity flux, integrated over the northern
hemisphere and over the 11 year solar cycle, of about
.
Key words: magnetohydrodynamics (MHD) -- turbulence -- Sun: magnetic fields
© ESO 2004
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