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 solar tachocline is an internal region of the Sun possessing strong radial and latitudinal
shears straddling the base of the convective envelope. Based on helioseismic inversions …

Despite their importance in stellar evolution, little is known about magnetic fields in the
interior of stars. The recent seismic detection of magnetic fields in the core of several red …

The Tayler instability is an important but poorly studied magnetohydrodynamic (MHD)
instability that likely operates in stellar interiors. The non-linear saturation of the Tayler …

ABSTRACT The Tayler–Spruit dynamo is one of the most promising mechanisms proposed
to explain angular momentum transport during stellar evolution. Its development in proto …

Context. Space asteroseismology is revolutionizing our knowledge of the internal structure
and dynamics of stars. A breakthrough is ongoing with the recent discoveries of signatures …

Recent decades have seen enormous progress in the experimental investigation of
fundamental processes that are relevant to geophysical and astrophysical fluid dynamics …

It has recently been shown that a significant slowdown of many stars can be attributed to the
emergence of a strong magnetic field within the radiative region, where heat is transferred …

Context. Tens of thousands of red giant stars in the Kepler data exhibit solar-like oscillations.
The mixed-mode characteristics of their oscillations enable us to study the internal physics …

Red giant stars host solar-like oscillations which have mixed character, being sensitive to
conditions both in the outer convection zone and deep within the interior. The properties of …