Magnetic field and α-effect in model Z
- 1 December 1992
- journal article
- research article
- Published by Taylor & Francis in Geophysical & Astrophysical Fluid Dynamics
- Vol. 67 (1-4) , 87-97
- https://doi.org/10.1080/03091929208201838
Abstract
The main subject of the paper is to show how the shape and thickness of an α-layer and the amplitude of the α-effect influence the solution of model Z, especially the magnetic field energy (MFE). Solution of model Z with different input parameters allows us to conclude that the larger the thickness of the α-layer, the greater the ratio of the MFE of the meridional to the MFE of the azimuthal field and, therefore, the greater the efficiency of the α-effect, although the appropriate value of the amplitude of the α-effect is more difficult to find. The MFE tends to oscillate for a sufficiently thick α-layer if the amplitude of the α-effect is changed, but the oscillations are suppressed and MFE is again stabilized. If the thickness of the α-layer does not vary, the MFE of the azimuthal field relative to the MFE of the meridional field decreases with increasing amplitude of the α-effect in certain narrow limits. The geostrophic shear does not change its character, and its maximum follows the maximum of α-effect in the layer.Keywords
This publication has 4 references indexed in Scilit:
- On the computation of a model-Zwith electromagnetic core-mantle couplingGeophysical & Astrophysical Fluid Dynamics, 1989
- From taylor state to model-Z?Geophysical & Astrophysical Fluid Dynamics, 1989
- A model-Z geodynamoGeophysical & Astrophysical Fluid Dynamics, 1987
- Z-model of the nearly symmetric hydromagnetic dynamo with electromagnetic core-mantle couplingStudia Geophysica et Geodaetica, 1985