Statistical methods for the analysis of rotation measure grids in large
  scale structures in the SKA era
  To better understand the origin and properties of cosmological magnetic
fields, a detailed knowledge of magnetic fields in the large-scale structure of
the Universe (galaxy clusters, filaments) is crucial. We propose a new
statistical approach to study magnetic fields on large scales with the rotation
measure grid data that will be obtained with the new generation of radio
interferometers.
