Published June 9, 2014
| Version v1
Conference paper
Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era
Contributors
Others:
- Max Planck Institute for Astrophysics ; Max-Planck-Gesellschaft
- Institut d'Astrophysique de Paris (IAP) ; Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
- Université Paris Cité (UPCité)
- Joseph Louis LAGRANGE (LAGRANGE) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS) ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
- Services généraux (SGDG) ; Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)
- Department of Earth and Space Sciences [Göteborg] ; Chalmers University of Technology [Göteborg]
- Victoria University of Wellington
- Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)
- Netherlands Institute for Radio Astronomy (ASTRON)
Description
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.
Abstract
International audienceAdditional details
Identifiers
- URL
- https://hal.archives-ouvertes.fr/hal-03648705
- URN
- urn:oai:HAL:hal-03648705v1
Origin repository
- Origin repository
- UNICA