We present a suite of models of the coherent magnetic field of the Galaxy based on new
divergence-free parametric functions describing the global structure of the field. The model …

Context. Magnetic fields permeate the diffuse interstellar medium (ISM) of the Milky Way,
and are essential to explain the dynamical evolution and current shape of the Galaxy …

Context. The extreme precision and accuracy of forthcoming observations of the cosmic
microwave background (CMB) temperature and polarisation anisotropies, aiming to detect …

The line-of-sight structure of the Galactic magnetic field (GMF) can be studied using Faraday
rotation measure (RM) grids. We analyze how the choice of interpolation kernel can affect …

Polarimetry of stars at optical and near-infrared wavelengths is an invaluable tool for tracing
interstellar dust and magnetic fields. Recent studies have demonstrated the power of …

We present a multifrequency polarimetric study for the quasar 1604+ 159. The source was
observed at the L band with the American Very Long Baseline Array and the L, X, and U …

Context. A recent catalogue of the Faraday rotation measures (RMs) of extragalactic
sources, together with the synchrotron polarisation data from WMAP and Planck, provide us …

In recent years a number of surveys and telescopes have observed the plane-of-sky
component of magnetic fields associated with molecular clouds. However, observations of …

Using results of numerical simulations and Galactic and galaxy clusters observations, it is
shown that the transition from deterministic chaos to hard turbulence in the Galactic and …

It is shown, using results of numerical simulations and galactic observations that the
transition from deterministic chaos to hard turbulence in the Galactic magnetized plasmas …