activity
20022005
most citedThe case for a distributed solar dynamo shaped by near-surface shear

406 citations · 1.8k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph200529 cited

Effect of the radiative background flux in convection

A. Brandenburg, K. L. Chan, A. Nordlund +1

Numerical simulations of turbulent stratified convection are used to study models with approximately the same convective flux, but different radiative fluxes. As the radiative flux…

astro-ph2005406 cited

The case for a distributed solar dynamo shaped by near-surface shear

Axel Brandenburg

Arguments for and against the widely accepted picture of a solar dynamo being seated in the tachocline are reviewed and alternative ideas concerning dynamos operating in the bulk o…

q-bio.BM200516 cited

Dissociation in a polymerization model of homochirality

A. Brandenburg, A. C. Andersen, M. Nilsson

A fully self-contained model of homochirality is presented that contains the effects of both polymerization and dissociation. The dissociation fragments are assumed to replenish th…

astro-ph2005

Nonhelical turbulent dynamos: shocks and shear

A. Brandenburg, N. E. L. Haugen, A. J. Mee

Small scale turbulent dynamo action in compressible transonic turbulence is discussed. It is shown that the critical value of the magnetic Reynolds number displays a bimodal behavi…

astro-ph200414 cited

The problem of small and large scale fields in the solar dynamo

A. Brandenburg, N. E. L. Haugen, P. J. Käpylä +1

Three closely related stumbling blocks of solar mean field dynamo theory are discussed: how dominant are the small scale fields, how is the alpha effect quenched, and whether magne…

astro-ph2004240 cited

Magnetic field generation in fully convective rotating spheres

W. Dobler, M. Stix, A. Brandenburg

Magnetohydrodynamic simulations of fully convective, rotating spheres with volume heating near the center and cooling at the surface are presented. The dynamo-generated magnetic fi…