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Magnetism in the Square Kilometre Array Era

Published online by Cambridge University Press:  03 March 2020

S. A. Mao
S. A. Mao*
Affiliation:
Max Planck Institute for Radio Astronomy, Auf dem Hügel 69, D-53121 Bonn, Germany email: mao@mpifr-bonn.mpg.de
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Abstract

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The unprecedented sensitivity, angular resolution and broad bandwidth coverage of Square Kilometre Array (SKA) radio polarimetric observations will allow us to address many long-standing mysteries in cosmic magnetism science. I will highlight the unique capabilities of the SKA to map the warm hot intergalactic medium, reveal detailed 3-dimensional structures of magnetic fields in local galaxies and trace the redshift evolution of galactic magnetic fields.

Keywords

polarizationcosmology: large-scale structure of universegalaxies: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 307 - 310
Copyright
© International Astronomical Union 2020

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