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The propagation and stability of linear wave motions in rapidly rotating spherical shells: Weak magnetic fields

 

作者: I.A. Eltayeb,  

 

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

页码: 211-239

 

ISSN:0309-1929

 

年代: 1992

 

DOI:10.1080/03091929208201845

 

出版商: Taylor & Francis Group

 

关键词: Hydromagnetic-rotating fluids;planetary dynamos;Rossby buoyancy waves;slow MHD waves

 

数据来源: Taylor

 

摘要:

The propagation properties and stability of wave motions in a spherical fluid shell, rotating uniformly in a co-rotating zonal magnetic field, are studied. Various profils of magnetic field and temperature gradient are examined. The fluid is viscous and electrically and thermally conducting. The analysis is applicable when the rotation rate is very high and the Elsasser number Λ ≪ 1. (Λ measures the ratio of Lorentz to Coriolis forces). The wave motions occur in the form of annular cylindrical cells whose thickness is determined by the rotation rate and magnetic field amplitude (Eltayeb and Kumar, 1977).

 

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