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 …

Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …

We study the behavior of magnetorotational turbulence in shearing box simulations with a
radial and azimuthal extent up to 10 scale heights. Maxwell and Reynolds stresses are …

The mean plane-of-sky magnetic field strength is traditionally obtained from the combination
of polarization and spectroscopic data using the Davis–Chandrasekhar–Fermi (DCF) …

Kinetic and magnetic energy spectra in the ecliptic plane near 1 AU are found to exhibit
different power-law behaviors in the inertial range, with the magnetic spectrum often having …

Magnetic fields on small scales are ubiquitous in the Universe. Although they can often be
observed in detail, their generation mechanisms are not fully understood. One possibility is …

We present numerical simulations of driven magnetohydrodynamic (MHD) turbulence with
weak/moderate imposed magnetic fields. The main goal is to clarify dynamics of magnetic …

We demonstrate that a magneto-convection simulation incorporating essential physical
processes governing solar surface convection exhibits turbulent small-scale dynamo action …

Magnetic fields grow quickly, even at early cosmological times, suggesting the action of a
small-scale dynamo (SSD) in the interstellar medium (ISM) of galaxies. Many studies have …

Quantifying the efficiency of dust destruction in the interstellar medium (ISM) due to
supernovae (SNe) is crucial for the understanding of galactic dust evolution. We present 3D …