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
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceThis work presents numerical results on the transport of heat and chemical spe...
The stability characteristics of a Helmholtz velocity profile in a stably stratified, compressible a...
The stability characteristics of a Helmholtz velocity profile in a stably stratified, compressible a...
The stability characteristics of a Helmholtz velocity profile in a stably stratified, compressible a...
The linear stability of a double-diffusively stratified, inflectional shear flow is investigated. Do...
We discuss the possibility that astrophysical accretion disks are dynamically unstable to non-axisym...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
Shear flows have a significant impact on the dynamics in an assortment of different astrophysical ob...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceThis work presents numerical results on the transport of heat and chemical spe...
The stability characteristics of a Helmholtz velocity profile in a stably stratified, compressible a...
The stability characteristics of a Helmholtz velocity profile in a stably stratified, compressible a...
The stability characteristics of a Helmholtz velocity profile in a stably stratified, compressible a...
The linear stability of a double-diffusively stratified, inflectional shear flow is investigated. Do...
We discuss the possibility that astrophysical accretion disks are dynamically unstable to non-axisym...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
Shear flows have a significant impact on the dynamics in an assortment of different astrophysical ob...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceThis work addresses the question of the stability of stratified, spatially per...
International audienceWe discuss the possibility that astrophysical accretion disks are dynamically ...