Magnetism science with the square kilometre array
Artikel i vetenskaplig tidskrift, 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

Magnetic fields

Techniques: polarimetric

Telescopes

Instrumentation: interferometers

Författare

G. Heald

CSIRO Astronomy and Space Science

S. A. Mao

Max-Planck-Gesellschaft

V. Vacca

INAF Osservatorio Astronomico di Cagliari

Takuya Akahori

National Astronomical Observatory of Japan

Ancor Damas-Segovia

CSIC - Instituto de Astrofísica de Andalucía (IAA)

B. Gaensler

University of Toronto

M. Hoeft

Thüringer Landessternwarte Tautenburg

I. Agudo

CSIC - Instituto de Astrofísica de Andalucía (IAA)

A. Basu

Universität Bielefeld

R. Beck

Max-Planck-Gesellschaft

M. Birkinshaw

University of Bristol

A. Bonafede

Universita di 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

Institut d'Estudis Espacials de Catalunya (IEEC)

Institut de Ciències de l'Espai (ICE) - CSIC

F. Govoni

INAF Osservatorio Astronomico di Cagliari

J.A. Green

CSIRO Astronomy and Space Science

Jinlin Han

Chinese Academy of Sciences

M. Haverkorn

Radboud Universiteit

Cathy Horellou

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

M. Johnston-Hollitt

Curtin University

Roland Kothes

National Research Council Canada

T. L. Landecker

National Research Council Canada

B. Nikiel-Wroczyński

Uniwersytet Jagiellonski w Krakowie

Shane P. O'Sullivan

Dublin City University

M. Padovani

Osservatorio Astrofisico di Arcetri

Frédérick Poidevin

Universidad de la Laguna

Instituto Astrofisico de Canarias

Luke Pratley

University of Toronto

Marco Regis

Universita degli Studi di Torino

Istituto Nazionale di Fisica Nucleare

C. J. Riseley

Istituto di Radioastronomia

Universita di Bologna

T. Robishaw

National Research Council Canada

L. Rudnick

University of Minnesota

C. Sobey

CSIRO Astronomy and Space Science

J. Stil

University of Calgary

Xiaohui Sun

Yunnan University

Sharanya Sur

Indian Institute of Astrophysics

A. Russell Taylor

University of the Western Cape

Inter-University Institute for Data Intensive Astronomy

University of Cape Town

Alec Thomson

CSIRO Astronomy and Space Science

C.L. Van Eck

University of Toronto

F. Vazza

Istituto di Radioastronomia

Universita di Bologna

Jennifer L. West

University of Toronto

Galaxies

20754434 (eISSN)

Vol. 8 8 53

Ämneskategorier

Tvärvetenskapliga studier

Astronomi, astrofysik och kosmologi

Kommunikationsvetenskap

DOI

10.3390/galaxies8030053

Mer information

Senast uppdaterat

2020-11-13