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      Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era

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          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.

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          Journal
          2015-01-02
          Article
          1501.00415
          b9fe60a0-4611-4aab-b017-90371fd62976

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          9 pages; to appear as part of 'Cosmic Magnetism' in Proceedings 'Advancing Astrophysics with the SKA (AASKA14)', PoS(AASKA14)114
          astro-ph.CO

          Cosmology & Extragalactic astrophysics
          Cosmology & Extragalactic astrophysics

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