The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …

The current understanding of astrophysical magnetic fields is reviewed, focusing on their
generation and maintenance by turbulence. In the astrophysical context this generation is …

These lecture notes are based on a tutorial given in 2017 at a plasma physics winter school
in Les Houches. Their aim is to provide a self-contained graduate-student level introduction …

This book presents an introduction to, and modern account of, magnetohydrodynamic
(MHD) turbulence, an active field both in general turbulence theory and in various areas of …

The nonlinear evolution of magnetized Keplerian shear flows is simulated in a local, three-
dimensional model, including the effects of compressibility and stratification. Supersonic …

We present numerical simulations and explore scalings and anisotropy of compressible
magnetohydrodynamic (MHD) turbulence. Our study covers both gas-pressure-dominated …

The solar dynamo continues to pose a challenge to observers and theoreticians.
Observations of the solar surface reveal a magnetic field with a complex, hierarchical …

We report the results of an extensive numerical study of the small-scale turbulent dynamo.
The primary focus is on the case of large magnetic Prandtl numbers Pr m, which is relevant …

A numerical model of isotropic homogeneous turbulence with helical forcing is investigated.
The resulting flow, which is essentially the prototype of the α 2 dynamo of mean field …

We use the anelastic spherical harmonic code to model the convective dynamo of solar-type
stars. Based on a series of 15 3D MHD simulations spanning four bins in rotation and mass …