activity
19942023
most citedThe inverse cascade and nonlinear alpha-effect in simulations of isotropic helical hydromagnetic turbulence

604 citations · 12.7k across the 343 of their papers we have counts for

collaborators
Showing 2009Show all

18 papers · 1 filter

astro-ph.SR2009★ 91 cited

Astrophysical turbulence modeling

Axel Brandenburg, Aake Nordlund

The role of turbulence in various astrophysical settings is reviewed. Among the differences to laboratory and atmospheric turbulence we highlight the ubiquitous presence of magneti…

astro-ph.SR2009★ 81 cited

Equatorial magnetic helicity flux in simulations with different gauges

Dhrubaditya Mitra, Simon Candelaresi, Piyali Chatterjee +2

We use direct numerical simulations of forced MHD turbulence with a forcing function that produces two different signs of kinetic helicity in the upper and lower parts of the domai…

astro-ph.SR2009★ 46 cited

Large-scale magnetic flux concentrations from turbulent stresses

Axel Brandenburg, Nathan Kleeorin, Igor Rogachevskii

In this study we provide the first numerical demonstration of the effects of turbulence on the mean Lorentz force and the resulting formation of large-scale magnetic structures. Us…

astro-ph.SR2009★ 41 cited

Magnetic field decay of three interlocked flux rings with zero linking number

Fabio Del Sordo, Simon Candelaresi, Axel Brandenburg

The resistive decay of chains of three interlocked magnetic flux rings is considered. Depending on the relative orientation of the magnetic field in the three rings, the late-time…

astro-ph.GA2009★ 4 cited

Turbulent diffusion and galactic magnetism

Axel Brandenburg, Fabio Del Sordo

Using the test-field method for nearly irrotational turbulence driven by spherical expansion waves it is shown that the turbulent magnetic diffusivity increases with magnetic Reyno…

astro-ph.SR2009★ 20 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.…