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.
点击下载:
PDF (1329KB)
返 回