activity
20102017
most citedApproaching the Asymptotic Regime of Rapidly Rotating Convection: Boundary Layers vs Interior Dynamics

187 citations · 1.3k across the 17 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2015★ 33 cited

A New Model for Mixing By Double-Diffusive Convection (Semi-Convection). III. Thermal and Compositional Transport Through Non-Layered ODDC

Ryan Moll, Pascale Garaud, Stephan Stellmach

Oscillatory double-diffusive convection (ODDC) (also known as semi- convection) refers to a type of double diffusive instability that occurs in regions of planetary and stellar int…

astro-ph.SR2015★ 38 cited

Anelastic Versus Fully Compressible Turbulent Rayleigh-Bénard Convection

Jan Verhoeven, Thomas Wiesehöfer, Stephan Stellmach

Numerical simulations of turbulent Rayleigh-Bénard convection in an ideal gas, using either the anelastic approximation or the fully compressible equations, are compared. Theoretic…

astro-ph.SR2014★ 12 cited

Double-diffusive mixing in stellar interiors in the presence of horizontal gradients

Michael Medrano, Pascale Garaud, Stephan Stellmach

We have identified an important source of mixing in stellar radiation zones, that would arise whenever two conditions are satisfied: (1) the presence of an inverse vertical composi…

astro-ph.SR2012★ 120 cited

Chemical Transport and Spontaneous Layer Formation in Fingering Convection in Astrophysics

Justin M. Brown, Pascale Garaud, Stephan Stellmach

A region of a star that is stable to convection according to the Ledoux criterion may nevertheless undergo additional mixing if the mean molecular weight increases with radius. Thi…

astro-ph.SR2012★ 97 cited

A new model for mixing by double-diffusive convection (semi-convection). II. The transport of heat and composition through layers

Toby S. Wood, Pascale Garaud, Stephan Stellmach

Regions of stellar and planetary interiors that are unstable according to the Schwarzschild criterion, but stable according to the Ledoux criterion, are subject to a form of oscill…

astro-ph.SR2011★ 124 cited

A new model for mixing by double-diffusive convection (semi-convection): I. The conditions for layer formation

Giovanni M. Mirouh, Pascale Garaud, Stephan Stellmach +2

The process referred to as "semi-convection" in astrophysics and "double-diffusive convection in the diffusive regime" in Earth and planetary sciences, occurs in stellar and planet…

astro-ph.SR2010★ 121 cited

Turbulent mixing and layer formation in double-diffusive convection: 3D numerical simulations and theory

Erica Rosenblum, Pascale Garaud, Adrienne Traxler +1

Double-diffusive convection, often referred to as semi-convection in astrophysics, occurs in thermally and compositionally stratified systems which are stable according to the Ledo…

astro-ph.SR2010★ 152 cited

Numerically determined transport laws for fingering ("thermohaline") convection in astrophysics

Adrienne Traxler, Pascale Garaud, Stephan Stellmach

We present the first three-dimensional simulations of fingering convection performed in a parameter regime close to the one relevant for astrophysics, and reveal the existence of s…

astro-ph.SR2010★ 35 cited

A model of the entropy flux and Reynolds stress in turbulent convection

Pascale Garaud, Gordon I. Ogilvie, Neil Miller +1

We propose a closure model for the transport of entropy and momentum in astrophysical turbulence, intended for application to rotating stellar convective regions. Our closure model…