4 papers
Non-linear evolution of the horizontal shear instability in stratified rotating fluids under the complete Coriolis acceleration
Camille Moisset, Paul Billant, Junho Park +1
This paper investigates the non-linear dynamics of horizontal shear instability in an incompressible, stratified and rotating fluid in the non-traditional -plane, i.e. with the…
Exploring hydrodynamical stellar tachoclines along stellar evolution
Camille Moisset, Stéphane Mathis, Louis Amard
Stellar tachoclines are thin regions located between the radiative core and the convective envelope of solar-type stars. They are defined as layers where the rotation of the radiat…
Vertical shear instabilities in rotating stellar radiation zones: effects of the full Coriolis acceleration and thermal diffusion
Junho Park, Stéphane Mathis
Rotation deeply impacts the structure and the evolution of stars. To build coherent 1D or multi-D stellar structure and evolution models, we must systematically evaluate the turbul…
The effects of rotation on wave-induced transport in stars: from weakly to strongly stratified radiative zones
Q. André, S. Mathis, L. Amard
Internal waves propagating in stellar radiative zones can lead to efficient angular momentum transport, that should occur throughout the whole lifetime of stars. They thus play a k…