146 citations · 234 across the 4 of their papers we have counts for
4 papers
Heat Transport and Dissipation in 2.5D Rotating Internally Heated and Cooled Convection
Tom Joshi-Hartley, Matthew K. Browning, Laura K. Currie +3
Models of astrophysical convection, such as mixing length theory, typically assume that the heat transport is independent of microphysical diffusivities. Such 'diffusion-free' beha…
Exploring the vs relation with flux transport dynamo models of solar-like stars
L. Jouve, B. P. Brown, A. S. Brun
Aims: To understand stellar magnetism and to test the validity of the Babcock-Leighton flux transport mean field dynamo models with stellar activity observations Methods: 2-D mean…
Three-Dimensional Simulations of Solar and Stellar Dynamos: The Influence of a Tachocline
M. S. Miesch, M. K. Browning, A. S. Brun +2
We review recent advances in modeling global-scale convection and dynamo processes with the Anelastic Spherical Harmonic (ASH) code. In particular, we have recently achieved the fi…
Rapidly Rotating Suns and Active Nests of Convection
Benjamin P. Brown, Matthew K. Browning, Allan Sacha Brun +2
In the solar convection zone, rotation couples with intensely turbulent convection to drive a strong differential rotation and achieve complex magnetic dynamo action. Our sun must…