Abstract
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.
Original language | English |
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Journal | Advancing Astrophysics with the Square Kilometre Array (AASKA14) |
Publication status | Published - 2015 |