activity
19972012
most citedThe case for a distributed solar dynamo shaped by near-surface shear

406 citations · 3.2k across the 59 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.SR200920 cited

The critical role of magnetic helicity in astrophysical large-scale dynamos

Axel Brandenburg

The role of magnetic helicity in astrophysical large-scale dynamos is reviewed and compared with cases where there is no energy supply and an initial magnetic field can only decay.…

astro-ph.SR200976 cited

Small-scale magnetic helicity losses from a mean-field dynamo

Axel Brandenburg, Simon Candelaresi, Piyali Chatterjee

Using mean-field models with a dynamical quenching formalism we show that in finite domains magnetic helicity fluxes associated with small-scale magnetic fields are able to allevia…

astro-ph.SR200919 cited

The role of the Yoshizawa effect in the Archontis dynamo

Sharanya Sur, Axel Brandenburg

The generation of mean magnetic fields is studied for a simple non-helical flow where a net cross helicity of either sign can emerge. This flow, which is also known as the Archonti…

astro-ph.SR200941 cited

Advances in theory and simulations of large-scale dynamos

Axel Brandenburg

Recent analytical and computational advances in the theory of large-scale dynamos are reviewed. The importance of the magnetic helicity constraint is apparent even without invoking…

astro-ph.SR20092 cited

Paradigm shifts in solar dynamo modeling

Axel Brandenburg

Selected topics in solar dynamo theory are being highlighted. The possible relevance of the near-surface shear layer is discussed. The role of turbulent downward pumping is mention…

astro-ph.SR200936 cited

Turbulent diffusion with rotation or magnetic fields

Axel Brandenburg, Andreas Svedin, Geoffrey M. Vasil

The turbulent diffusion tensor describing the evolution of the mean concentration of a passive scalar is investigated for non-helically forced turbulence in the presence of rotatio…