We review the state of the art of three dimensional numerical simulations of solar and stellar
dynamos. We summarize fundamental constraints of numerical modelling and the …

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

We report on simulations of turbulent, rotating, stratified, magnetohydrodynamic convection
in spherical wedge geometry. An initially small-scale, random, weak-amplitude magnetic …

Recent advances in mean-field theory are reviewed and applications to the Sun, late-type
stars, accretion disks, galaxies and the early Universe are discussed. We focus particularly …

To explore the physics of large-scale flows in solar-like stars, we perform three-dimensional
anelastic simulations of rotating convection for global models with stratification resembling …

Context. Late-type stars such as the Sun rotate differentially due to the interaction of
turbulent convection and rotation. Aims. The aim of the study is to investigate the effects of …

Context. Solar-like differential rotation is characterized by a rapidly rotating equator and
slower poles. However, theoretical models and numerical simulations can also result in a …

We present results from simulations of rotating magnetized turbulent convection in spherical
wedge geometry representing parts of the latitudinal and longitudinal extents of a star. Here …

In this work the authors draw upon their expertise in geophysical and astrophysical MHD to
explore the motion of electrically conducting fluids, the so-called dynamo effect, and …

Context. Turbulent fluxes of angular momentum and enthalpy or heat due to rotationally
affected convection play a key role in determining differential rotation of stars. Their …