Magnetism science with the square kilometre array
Journal article, 2020
The Square Kilometre Array (SKA) will answer fundamental questions about the origin, evolution, properties, and influence of magnetic fields throughout the Universe. Magnetic fields can illuminate and influence phenomena as diverse as star formation, galactic dynamics, fast radio bursts, active galactic nuclei, large-scale structure, and dark matter annihilation. Preparations for the SKA are swiftly continuing worldwide, and the community is making tremendous observational progress in the field of cosmic magnetism using data from a powerful international suite of SKA pathfinder and precursor telescopes. In this contribution, we revisit community plans for magnetism research using the SKA, in light of these recent rapid developments. We focus in particular on the impact that new radio telescope instrumentation is generating, thus advancing our understanding of key SKA magnetism science areas, as well as the new techniques that are required for processing and interpreting the data. We discuss these recent developments in the context of the ultimate scientific goals for the SKA era.
Polarization
Techniques: polarimetric
Instrumentation: interferometers
Magnetic fields
Telescopes
Author
G. Heald
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
S. A. Mao
Max Planck Society
V. Vacca
Istituto nazionale di astrofisica (INAF)
Takuya Akahori
National Astronomical Observatory of Japan
Ancor Damas-Segovia
Spanish National Research Council (CSIC)
B. Gaensler
University of Toronto
M. Hoeft
Thüringer Landessternwarte Tautenburg
I. Agudo
Spanish National Research Council (CSIC)
A. Basu
Bielefeld University
R. Beck
Max Planck Society
M. Birkinshaw
University of Bristol
A. Bonafede
University of Bologna
Istituto di Radioastronomia
T. L. Bourke
SKA Organisation
Andrea Bracco
Ruder Boskovic Institute
E. Carretti
Istituto di Radioastronomia
L. Feretti
Istituto di Radioastronomia
J. M. Girart
Spanish National Research Council (CSIC)
Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)
F. Govoni
Istituto nazionale di astrofisica (INAF)
J.A. Green
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
Jinlin Han
Chinese Academy of Sciences
M. Haverkorn
Radboud University
Cathy Horellou
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
M. Johnston-Hollitt
Curtin University
Roland Kothes
National Research Council Canada
T. L. Landecker
National Research Council Canada
B. Nikiel-Wroczyński
Jagiellonian University in Kraków
Shane P. O'Sullivan
Dublin City University
M. Padovani
Arcetri Astrophysical Observatory
Frédérick Poidevin
Instituto de Astrofísica de Canarias
University of La Laguna
Luke Pratley
University of Toronto
Marco Regis
University of Turin
National Institute for Nuclear Physics
C. J. Riseley
University of Bologna
Istituto di Radioastronomia
T. Robishaw
National Research Council Canada
L. Rudnick
University of Minnesota
C. Sobey
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
J. Stil
University of Calgary
Xiaohui Sun
Yunnan University
Sharanya Sur
Indian Institute of Astrophysics
A. Russell Taylor
University of the Western Cape
University of Cape Town
Alec Thomson
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
C.L. Van Eck
University of Toronto
F. Vazza
University of Bologna
Istituto di Radioastronomia
Jennifer L. West
University of Toronto
Galaxies
20754434 (eISSN)
Vol. 8 8 53Subject Categories (SSIF 2011)
Social Sciences Interdisciplinary
Astronomy, Astrophysics and Cosmology
Communication Studies
DOI
10.3390/GALAXIES8030053