A&A 421, 349-351 (2004)
DOI: 10.1051/0004-6361:20041302
Does the butterfly diagram indicate a solar flux-transport dynamo?
M. Schüssler and D. SchmittMax-Planck-Institut für Sonnensystemforschung (Formerly: Max-Planck-Institut für Aeronomie.) , Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
e-mail: [schuessler,schmitt]@linmpi.mpg.de
(Received 26 February 2004 / Accepted 17 March 2004 )
Abstract
We address the question whether the properties of the observed
latitude-time diagram of sunspot occurrence (the butterfly diagram)
provide evidence for the operation of a flux-transport
dynamo, which explains the migration of the sunspot zones and the
period of the solar cycle in terms of a deep equatorward
meridional flow. We show that the properties of the butterfly diagram
are equally well reproduced by a conventional dynamo model with
migrating dynamo waves, but without transport of magnetic flux by a
flow. These properties seem to be generic for an oscillatory and
migratory field of dipole parity and thus do not permit an
observational distinction between different dynamo approaches.
Key words: magnetohydrodynamics (MHD) -- Sun: activity -- Sun: magnetic fields -- Sun: interior -- Sun: sunspots
Offprint request: M. Schüssler, msch@linmpi.mpg.de
© ESO 2004
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