activity
20062026
most citedMagnetism, rotation, and nonthermal emission in cool stars -- Average magnetic field measurements in 292 M dwarfs

177 citations · 2.4k across the 68 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 61 cited

Large-scale dynamos in rigidly rotating turbulent convection

P. J. Käpylä, M. J. Korpi, A. Brandenburg

The existence of large-scale dynamos in rigidly rotating turbulent convection without shear is studied using three-dimensional numerical simulations of penetrative rotating compres…

astro-ph2008★ 60 cited

Turbulent dynamos with shear and fractional helicity

P. J. Käpylä, A. Brandenburg

Dynamo action owing to helically forced turbulence and large-scale shear is studied using direct numerical simulations. The resulting magnetic field displays propagating wave-like…

astro-ph2007★ 9 cited

The helicity constraint in spherical shell dynamos

A. Brandenburg, P. J. Käpylä, D. Mitra +2

The motivation for considering distributed large scale dynamos in the solar context is reviewed in connection with the magnetic helicity constraint. Preliminary accounts of 3-dimen…

astro-ph2007★ 5 cited

Turbulent viscosity and Lambda-effect from numerical turbulence models

P. J. Käpylä, A. Brandenburg

Homogeneous anisotropic turbulence simulations are used to determine off-diagonal components of the Reynolds stress tensor and its parameterization in terms of turbulent viscosity…

astro-ph2007★ 171 cited

Magnetic diffusivity tensor and dynamo effects in rotating and shearing turbulence

A. Brandenburg, K. -H. Rädler, M. Rheinhardt +1

The turbulent magnetic diffusivity tensor is determined in the presence of rotation or shear. The question is addressed whether dynamo action from the shear-current effect can expl…

astro-ph2006★ 5 cited

Effects of Rotation and Input Energy Flux on Convective Overshooting

P. J. Käpylä, M. J. Korpi, M. Stix +1

We study convective overshooting by means of local 3D convection calculations. Using a mixing length model of the solar convection zone (CZ) as a guide, we determine the Coriolis n…