C. Kutzner, U.R. Christensen
Institute of Geophysics, University of Goettingen, Goettingen, Germany
We use a 3D convection-driven numerical dynamo model without hyperdiffusivity to study the characteristic structure and time variability of the magnetic field in dependence of the Rayleigh number (Ra) for values up to about 40 times supercritical. We also compare a variety of ways to drive the convection and basically find two dynamo regimes. At low Ra the magnetic field at the surface of the model is dominated by the non-reversing axial dipole component. At high Ra the dipole part becomes small in comparison to higher multipole components. At transitional values of the Rayleigh number the dynamo vacillates between the dipole-dominated and the multipolar regime, which includes excursions and reversals of the dipole axis. For suitable choices of the driving mode and the non-dimensional numbers the mean dipole moment and the temporal evolution of the magnetic field resemble the known properties of the Earth's field from paleomagnetic data.