Stars are rotating and magnetic bodies. Moreover, more and more constraints are obtained
on such dynamical processes using, for example, seismology and spectropolarimetry …

We discuss recent observational, theoretical and numerical progress made in understanding
the solar global magnetism and its short and long term variability. We discuss the physical …

Context. The discovery of moderate differential rotation between the core and the envelope
of evolved solar-like stars could be the signature of a strong magnetic field trapped inside …

We present MAESTROeX, a massively parallel solver for low Mach number astrophysical
flows. The underlying low Mach number equation set allows for efficient, long-time …

Overshooting of turbulent motions from convective regions into adjacent stably stratified
zones plays a significant role in stellar interior dynamics, as this process may lead to mixing …

We present the first numerical simulations of the solar interior to exhibit a tachocline
consistent with the Gough and McIntyre model. We find non-linear, axisymmetric, steady …

We present a local but fully nonlinear model of the solar tachocline, using three-dimensional
direct numerical simulations. The tachocline forms naturally as a statistically steady balance …

Context. With the progress of observational constraints on dynamical processes in stars, it
becomes necessary to understand the angular momentum and the rotation profile history. In …

The propagation of meridional circulation below the base of the convection zone (CZ) of low-
mass stars may play a crucial role in the transport of angular momentum and also …

Surface observations indicate that the speed of the solar meridional circulation in the
photosphere varies in anti-phase with the solar cycle. The current explanation for the source …