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

We review the present theoretical and numerical understanding of magnetic field
amplification in cosmic large-scale structure, on length scales of galaxy clusters and beyond …

Understanding the physics of turbulence is crucial for many applications, including weather,
industry and astrophysics. In the interstellar medium,, supersonic turbulence plays a crucial …

We study the growth rate and saturation level of the turbulent dynamo in
magnetohydrodynamical simulations of turbulence, driven with solenoidal (divergence-free) …

Magnetic fields play an important role in astrophysical accretion discs and in the interstellar
and intergalactic medium. They drive jets, suppress fragmentation in star-forming clouds and …

We show that supersonic MHD turbulence yields a star formation rate (SFR) as low as
observed in molecular clouds, for characteristic values of the free-fall time divided by the …

Several recent advances in turbulent dynamo theory are reviewed. High resolution
simulations of small-scale and large-scale dynamo action in periodic domains are compared …

The ideal MHD equations are a central model in astrophysics, and their solution relies upon
stable numerical schemes. We present an implementation of a new method, which …

We explore the amplification of magnetic seeds during the formation of the first stars and
galaxies. During gravitational collapse, turbulence is created from accretion shocks, which …

We present the first results from SPHINX-MHD, a suite of cosmological radiation-
magnetohydrodynamics simulations designed to study the impact of primordial magnetic …