output
19912026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2019 · astro-ph.SRShow all

6 papers · 2 filters

astro-ph.SR2019★ 9 cited

Magnetic helicity dissipation and production in an ideal MHD code

Axel Brandenburg, Evan Scannapieco

We study a turbulent helical dynamo in a periodic domain by solving the ideal magnetohydrodynamic (MHD) equations with the FLASH code using the divergence-cleaning eight-wave metho…

astro-ph.SR2019★ 20 cited

Topological changes in the magnetic field of LQ Hya during an activity minimum

Jyri J. Lehtinen, Maarit J. Käpylä, Thomas Hackman +6

Previous studies have related surface temperature maps, obtained with the Doppler imaging (DI) technique, of LQ Hya with long-term photometry. We compare surface magnetic field map…

astro-ph.SR2019★ 3 cited

Exploring helical dynamos with machine learning

Farrukh Nauman, Joonas Nättilä

We use ensemble machine learning algorithms to study the evolution of magnetic fields in magnetohydrodynamic (MHD) turbulence that is helically forced. We perform direct numerical…

astro-ph.SR2019★ 27 cited

Reversed dynamo at small scales and large magnetic Prandtl number

Axel Brandenburg, Matthias Rempel

We show that at large magnetic Prandtl numbers, the Lorentz force does work on the flow at small scales and drives fluid motions, whose energy is dissipated viscously. This situati…

astro-ph.SR2019★ 17 cited

Spectral magnetic helicity of solar active regions between 2006 and 2017

Sanjay Gosain, Axel Brandenburg

We compute magnetic helicity and energy spectra from about 2485 patches of about 100 megameters (Mm) side length on the solar surface using data from Hinode during 2006--2017. An e…

astro-ph.SR2019★ 18 cited

Turbulent viscosity and effective magnetic Prandtl number from simulations of isotropically forced turbulence

Petri J. Käpylä, Matthias Rheinhardt, Axel Brandenburg +1

(abridged) Context: Turbulent diffusion of large-scale flows and magnetic fields play major roles in many astrophysical systems. Aims: Our goal is to compute turbulent viscosity an…