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Magnetic field and α-effect in model Z

 

作者: I. Cupal,   P. Hejda,  

 

期刊: Geophysical & Astrophysical Fluid Dynamics  (Taylor Available online 1992)
卷期: Volume 67, issue 1-4  

页码: 87-97

 

ISSN:0309-1929

 

年代: 1992

 

DOI:10.1080/03091929208201838

 

出版商: Taylor & Francis Group

 

关键词: Hydromagnetic dynamo;α-effect;model-Z

 

数据来源: Taylor

 

摘要:

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.

 

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