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20012023
most citedAnalytical protostellar disk models 1: the effect of internal dissipation and surface irradiation on the structure of disks and the location of the snow line around Sun-like stars

265 citations · 1.8k across the 46 of their papers we have counts for

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physics.flu-dyn2022★ 5 cited

Resistive instabilities in sinusoidal shear flows with a streamwise magnetic field

Adrian E. Fraser, Imogen G. Cresswell, Pascale Garaud

We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) wit…

physics.flu-dyn2021

Journey to the center of stars: the realm of low Prandtl number fluid dynamics

Pascale Garaud

The dynamics of fluids deep in stellar interiors is a subject that bears many similarities with geophysical fluid dynamics, with one crucial difference: the Prandtl number. The rat…

physics.flu-dyn2021★ 2 cited

Preferential concentration by mechanically-driven turbulence in the two-fluid formalism

Sara Nasab, Pascale Garaud

Preferential concentration is thought to play a key role in promoting particle growth, which is crucial to processes such as warm rain formation in clouds, planet formation, and in…

physics.flu-dyn2020★ 4 cited

Preferential concentration in the particle-induced convective instability

Sara Nasab, Pascale Garaud

Heavy particles in turbulent flows have been shown to accumulate in regions of high strain rate or low vorticity, a process otherwise known as preferential concentration. This can…

physics.flu-dyn2019★ 37 cited

The dynamics of stratified horizontal shear flows at low Péclet number

L. Cope, P. Garaud, C. P. Caulfield

We consider the dynamics of a vertically stratified, horizontally-forced Kolmogorov flow. Motivated by astrophysical systems where the Prandtl number is often asymptotically small,…

physics.flu-dyn2017★ 15 cited

Weakly non-Boussinesq convection in a gaseous spherical shell

Lydia Korre, Nicholas Brummell, Pascale Garaud

We examine the dynamics associated with weakly compressible convection in a spherical shell by running 3D direct numerical simulations using the Boussinesq formalism [1]. Motivated…