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Resistive instabilities in rapidly rotating fluids: Linear theory of the convective modes

 

作者: Weijia Kuang,   PaulH. Roberts,  

 

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

页码: 129-162

 

ISSN:0309-1929

 

年代: 1992

 

DOI:10.1080/03091929208201841

 

出版商: Taylor & Francis Group

 

关键词: Resistive instability;tearing mode;rotating magnetohydrodynamics

 

数据来源: Taylor

 

摘要:

This paper analyzes the linear stability of a rapidly-rotating, stratified sheet pinch in a gravitational field, g, perpendicular to the sheet. The sheet pinch is a layer (O ⩽ z ⩽ d) of inviscid, Boussinesq fluid of electrical conductivity σ, magnetic permeability μ, and almost uniform densityρo; z is height. The prevailing magnetic field.Bo(z), is horizontal at each z level, but varies in direction with z. The angular velocity,Ω, is vertical and large (Ω ≫ VA/d, where VA= B0√(μρ0) is the Alfvén velocity). The Elsasser number, Λ = σB20/2Ωρ0, measures σ. A (modified) Rayleigh number, R = gβd2/ρ0V2A, measures the buoyancy force, where β is the imposed density gradient, antiparallel tog. A Prandtl number, PK= μσK, measures the diffusivity, k, of density differences.

 

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