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Cosmic Magnetism (1911.02108v1)

Published 5 Nov 2019 in astro-ph.GA and astro-ph.IM

Abstract: Magnetic fields are involved in every astrophysical process on every scale: from planetary and stellar interiors to neutron stars, stellar wind bubbles and supernova remnants; from the interstellar medium in galactic disks, nuclei, spiral arms and halos to the intracluster and intergalactic media. They are involved in essentially every particle acceleration process and are thus fundamental to non-thermal physics in the Universe. Key questions include the origin of magnetic fields, their evolution over cosmic time, the amplification and decay processes that modify their strength, and their impact on other processes such as star formation and galaxy evolution. Astrophysical plasmas provide a unique laboratory for testing magnetic dynamo theory. The study of magnetic fields requires observations that span the wavelength range from radio through infrared, optical, UV, X-ray, and gamma-ray. Canada has an extremely strong record of research in cosmic magnetism, and has a significant leadership role in several ongoing and upcoming global programs. This white paper will review the science questions to be addressed in the study of cosmic magnetic fields and will describe the observational and theoretical opportunities and challenges afforded by the telescopes and modelling capabilities of today and tomorrow.

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Summary

  • The paper demonstrates that magnetic fields critically influence astrophysical processes from star formation to galaxy evolution.
  • It employs advanced radio methods, including polarization and Faraday rotation synthesis, to robustly characterize cosmic magnetism.
  • Canadian initiatives like POSSUM, VLASS, and CIRADA drive innovative research and set future directions in cosmic magnetism studies.

An Essay on the Comprehensive Study of Cosmic Magnetism

The paper "Cosmic Magnetism" provides an extensive review of the fundamental roles that magnetic fields play across a myriad of astrophysical processes and environments, covering scales from planetary bodies to cosmic structures. The authors—from a collection of Canadian institutions with a robust history in astrophysical research—aim to articulate both the prevailing questions and future directions in the paper of cosmic magnetic fields. Their work highlights how Canadian scholars are contributing to a global understanding and advancement in this specialized domain.

Executive Summary and Key Science Questions

The paper sets the stage by emphasizing that magnetic fields, though invisible and difficult to detect directly, are integral to all astrophysical environments. These fields are crucial for processes such as particle acceleration, non-thermal phenomena, star formation, and galaxy evolution. The authors highlight critical questions regarding the origin, evolution, strength, and interaction of magnetic fields with different cosmic processes. Specifically, the research focuses on the impact of magnetic fields on stellar evolution, the structure in interstellar medium drivers, the small and large-scale structures of magnetic fields in the Milky Way and other galaxies, cosmic ray propagation, AGN feedback, and the evolution of these fields over cosmic time.

Observational Techniques and Methodologies

The paper discusses the use of radio observations, particularly radio polarization and synchrotron radiation, as powerful probes for understanding magnetic fields. Techniques such as Faraday rotation measure synthesis are presented as invaluable tools to discern the characteristics of magnetic fields across the universe. The authors explore methods for observing magnetic structures within the Milky Way and nearby galaxies, emphasizing the importance of combining low frequencies with wide bandwidths for effective magnetic studies.

Canadian Contributions and Future Directions

Canadians have historically taken leading roles in identifying and analyzing cosmic magnetic fields. Several achievements are mentioned, including the first detections in various stellar objects and the largest catalogue of extragalactic rotation measures. The paper outlines Canada's leadership in international projects like the Polarisation Sky Survey of the Universe's Magnetism (POSSUM), Very Large Array Sky Survey (VLASS), and Global Magneto-Ionic Medium Survey (GMIMS). Each project is designed to answer specific science questions leveraging Canada's investments in cutting-edge radio astronomy technology.

Canadian efforts are additionally supported by initiatives like the Canadian Initiative for Radio Astronomy Data Analysis (CIRADA), focusing on processing large-scale radio survey data and developing innovative data products from facilities such as the ASKAP, LOFAR, and MeerKAT telescopes. The Square Kilometre Array (SKA), slated to significantly advance cosmic magnetism studies, promises a noteworthy enhancement of rotation measures due to its high sensitivity.

Archiving Cosmic Magnetism

This paper frames the necessity for further technological advancements and the involvement of Canadian facilities to sustain contributions in the cosmic magnetism field. In terms of future prospects, projects like CHORD and SKA are anticipated to provide unprecedented insights into magnetic field structures, thereby attracting a new cadre of scientists and stakeholders.

Conclusion

While the paper explores numerous scientific explorations, its underlying theme remains steadfast—advancing our knowledge of cosmic magnetism demands broad collaboration, continual technological upgrades, and strategic leadership. Through initiatives outlined, Canadian researchers are well-positioned to address vital questions and forge ahead in understanding the dynamic and complex nature of cosmic magnetic fields. The potential transformational gains in fundamental astrophysical knowledge implicit in this research are foundational for the broader pursuit of understanding the universe's interconnected systems.

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