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

The existence of magnetic fields associated with the intracluster medium in clusters of
galaxies is now well established through different methods of analysis. Magnetic fields are …

This paper describes the identification, modelling, and removal of previously unexplained
systematic effects in the polarization data of the Planck High Frequency Instrument (HFI) on …

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 …

The commonly used classical equipartition or minimum‐energy estimate of total magnetic
fields strengths from radio synchrotron intensities is of limited practical use because it is …

We review observations of extended regions of radio emission in clusters; these include
diffuse emission in 'relics', and the large central regions commonly referred to as 'halos'. The …

Radio synchrotron emission, its polarization and Faraday rotation of the polarization angle
are powerful tools to study the strength and structure of magnetic fields in galaxies …

Recent analyses of 21 cm neutral hydrogen (H i) emission have demonstrated that H i gas is
organized into linear filamentary structures that are preferentially aligned with the local …

We discuss observations of the magnetic field, column density, and turbulence in the cold
neutral medium (CNM). The observed quantities are only indirectly related to the intrinsic …

Most of the visible matter in the Universe is ionized, so that cosmic magnetic fields are quite
easy to generate and due to the lack of magnetic monopoles hard to destroy. Magnetic fields …