Shear layer instability in a highly diffusive stably stratified atmosphere

被引:0
作者
Lignières, F [1 ]
Califano, F
Mangeney, A
机构
[1] Observ Paris, Dept Rech Spatiale, F-92195 Meudon, France
[2] Observ Paris, CNRS, URA 264, F-92195 Meudon, France
[3] Univ London Queen Mary & Westfield Coll, Astron Unit, London E1 4NS, England
[4] Univ Pisa, Ist Nazl Fis Mat, Sez A, I-56100 Pisa, Italy
关键词
instabilities; hydrodynamics; stars : interiors;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The linear stability of a shear layer in a highly diffusive stably stratified atmosphere has been investigated. This study completes and extends previous works by Dudis (1974) and Jones (1977). We show that (i) an asymptotic regime is reached in the limit of large thermal diffusivity, (ii) there exists two different types of unstable modes. The slowest growing modes correspond to predominantly horizontal motions and the fast growing ones to isotropic motions, (iii) the physical interpretation of the stability properties in this asymptotic regime is simple. Applications to the dynamics of stellar radiative zone are discussed.
引用
收藏
页码:1027 / 1036
页数:10
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