activity
20002020
most cited3D convection simulations of the outer layers of the Sun using realistic physics

101 citations · 316 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020★ 1 cited

Simulating the outer layers of rapidly rotating stars

Frank Robinson, Joel Tanner, Sarbani Basu

This paper presents the results of a set of radiative hydrodynamic (RHD) simulations of convection in the near-surface regions of a rapidly rotating star. The simulations use micro…

astro-ph2006★ 81 cited

On Dissipation inside Turbulent Convection Zones from 3D Simulations of Solar Convection

Kaloyan Penev, Dimitar Sasselov, Frank Robinson +1

The development of 2D and 3D simulations of solar convection has lead to a picture of convection quite unlike the usually assumed Kolmogorov spectrum turbulent flow. We investigate…

astro-ph2005★ 17 cited

Simulating the outer layers of Procyon A: a comparison with the Sun

F. J. Robinson, P. Demarque, D. B. Guenther +2

Compared to the Sun, the atmospheric structure and convective flow in Procyon A exhibit the following characteristics: (1) the highly superadiabatic transition layer (SAL) is locat…

astro-ph2002★ 101 cited

3D convection simulations of the outer layers of the Sun using realistic physics

F. J. Robinson, P. Demarque, L. H. Li +4

This paper describes a series of 3D simulations of shallow inefficient convection in the outer layers of the Sun. The computational domain is a closed box containing the convection…

astro-ph2001★ 64 cited

Inclusion of turbulence in solar modeling

L. H. Li, F. J. Robinson, P. Demarque +2

The general consensus is that in order to reproduce the observed solar p-mode oscillation frequencies, turbulence should be included in solar models. However, until now there has n…

astro-ph2000★ 52 cited

A Large Eddy Simulation of Turbulent Compressible Convection: Differential Rotation in the Solar Convection Zone

Francis J. Robinson, Kwing L. Chan

We present results of two simulations of the convection zone, obtained by solving the full hydrodynamic equations in a section of a spherical shell. The first simulation has cylind…