activity
20032008
most citedGlobal-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope

481 citations · 1k across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph2008

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…

astro-ph2008146 cited

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…

astro-ph2007222 cited

Structure and Evolution of Giant Cells in Global Models of Solar Convection

Mark S. Miesch, Allan Sacha Brun, Marc L. Derosa +1

The global scales of solar convection are studied through three-dimensional simulations of compressible convection carried out in spherical shells of rotating fluid which extend fr…

astro-ph2006481 cited

Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope

Allan Sacha Brun, Mark S. Miesch, Juri Toomre

The operation of the solar global dynamo appears to involve many dynamical elements. Self-consistent MHD simulations which realistically incorporate all of these processes are not…

astro-ph2006178 cited

Simulations of core convection in rotating A-type stars: Magnetic dynamo action

Allan Sacha Brun, Matthew K. Browning, Juri Toomre

Core convection and dynamo activity deep within rotating A-type stars of 2 solar masses are studied with 3--D nonlinear simulations. Our modeling considers the inner 30% by radius…

astro-ph2004

Simulations of core convection and resulting dynamo action in rotating A-type stars

Matthew Browning, Allan Sacha Brun, Juri Toomre

We present the results of 3--D nonlinear simulations of magnetic dynamo action by core convection within A-type stars of 2 solar masses, at a range of rotation rates. We consider t…