14–18 Feb 2011
Wenner Gren Center
Europe/Stockholm timezone

Session

Session 9

16 Feb 2011, 09:00
Wenner-Gren Center, floor 7, Hörsalen (Wenner Gren Center)

Wenner-Gren Center, floor 7, Hörsalen

Wenner Gren Center

Sveavägen 164 SE-113 46 Stockholm Sweden

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  1. Dr Andre Giesecke
    16/02/2011, 09:00
    A simple way to interpret the reversal mechanism of the Earth's magnetic field has been achieved in theoretical models based on the interplay between very few magnetic modes. Motivated by the temporal behavior of elementary multipolar components of the Earth's magnetic field during the last reversal 780ka ago, (Leonhardt & Fabian 2007) the possibility of interacting magnetic modes is...
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  2. Dhrubaditya Mitra
    16/02/2011, 09:30
    We present direct numerical simulations with helical forcing in spherical coordinates which generates a dynamo which shows oscillations and equatorward migration. This DNS can be described by a mean field model with an alpha square dynamo where the alpha has different signs on the two hemispheres.
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  3. Dr Martin Schrinner
    16/02/2011, 10:00
    Under which conditions are convection-driven dynamo models oscillatory and do these models provide any implications for the solar dynamo? We perform global direct numerical simulations varying the governing parameters as well as the mechanical boundary conditions and build a sample of oscillatory dynamo models. We identify common characteristics responsible for the oscillatory nature...
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