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SYGP: Symposium Gemeinsame Probleme in Fusions- und astrophysikalischen Plasmen
SYGP 3: Contributed Talks
SYGP 3.1: Vortrag
Montag, 12. März 2012, 16:30–16:45, V55.22
Dynamos in convectively driven turbulence — •Wolf-Christian Müller1 and Manfred Schüssler2 — 1Max-Planck-Institut für Plasmaphysik, Boltzmannstr. 2, 85748 Garching — 2Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau
Different efforts to increase the understanding of magnetic field amplification in magnetohydrodynamic turbulence in the framework of the inter-institutional research initiative of the Max-Planck-Institutes for Plasma Physics and Solar System Research are presented. This talk focuses on basic turbulence properties which are also of importance from an astrophysical viewpoint, like the impact of physical modelling on turbulent dynamos, turbulent energy transport, and Lagrangian as well as dynamo-related characteristics of convective MHD turbulence.