Magnetism in the Square Kilometre Array Era
S. A. Mao (MPIfR)
TL;DR
The paper discusses how the Square Kilometre Array (SKA) will revolutionize cosmic magnetism studies through its advanced radio polarimetric capabilities, enabling detailed mapping and evolution tracking of magnetic fields across the universe.
Contribution
It highlights the unique capabilities of SKA for mapping cosmic magnetic fields and addressing longstanding questions in cosmic magnetism science.
Findings
SKA will map the warm hot intergalactic medium.
It will reveal 3D structures of magnetic fields in local galaxies.
It will trace the redshift evolution of galactic magnetic fields.
Abstract
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.
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