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Lookup NU author(s): Dr Christopher Hales
This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0).
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. 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.
Author(s): Vacca V, Oppermann N, Ensslin T, Selig M, Junklewitz H, Greiner M, Jasche J, Hales CA, Reinecke M, Carretti E, Feretti L, Ferrari C, Giovannini G, Govoni F, Horellou C, Ideguchi S, Johnston-Hollitt M, Murgia M, Paladino R, Pizzo RF, Scaife A
Publication type: Conference Proceedings (inc. Abstract)
Publication status: Published
Conference Name: Advancing Astrophysics with the Square Kilometre Array
Year of Conference: 2014
Online publication date: 09/06/2014
Acceptance date: 01/01/1900
Date deposited: 30/06/2017
Publisher: Proceedings of Science (PoS)
Notes: Paper presented at the conference Advancing Astrophysics with the Square Kilometre Array, June 8-13, 2014, Giardini Naxos, Italy
Series Title: Proceedings of Science