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 …

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 …

ABSTRACT The 3D MHD Anelastic Spherical Harmonic code, using slope-limited diffusion,
is employed to capture convective and dynamo processes achieved in a global-scale stellar …

The variable magnetic field of the solar photosphere exhibits periodic reversals as a result of
dynamo activity occurring within the solar interior. We decompose the surface field as …

We present an analysis of 21 global MHD simulations of the dynamo action taking place in
the interiors of fully convective M4 stars. We leverage our past work involving 45 simulations …

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 …

The discovery of Mercury's unusually axisymmetric, anomalously axially offset dipolar
magnetic field reveals a new regime of planetary magnetic fields. The cause of the offset …

In this paper, we argue that the solar activity record, as revealed by telescopic observations
and proxy data from the abundances of cosmogenic isotopes, is consistent with the action of …

Aims. In this study, we analyse the magnetic field properties of a set of 15 global
magnetohydrodynamic (MHD) simulations of solar-type star dynamos conducted using the …

We present a study of several systems in which a large-scale field is generated over a
turbulent background. These large-scale fields break a symmetry of the forcing by selecting …