Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-24T07:20:35.879Z Has data issue: false hasContentIssue false
  • English
  • Français

Cosmic magnetic field observations with next generation instrumentation

Published online by Cambridge University Press:  21 October 2010

Rainer Beck
Rainer Beck*
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The origin of magnetic fields in the Universe is an open problem in astrophysics and fundamental physics. Forthcoming radio telescopes will open a new era in studying cosmic magnetic fields. Low-frequency radio waves will reveal the structure of weak magnetic fields in the outer regions and halos of galaxies and in intracluster media. At higher frequencies, the EVLA and the SKA will map the structure of magnetic fields in galaxies in unprecedented detail. All-sky surveys of Faraday rotation measures (RM) towards a huge number of polarized background sources with the SKA and its pathfinders will allow us to model the structure and strength of the regular magnetic fields in the Milky Way, the interstellar medium of galaxies, in galaxy clusters and the intergalactic medium.

Keywords

Techniques: polarimetricgalaxies: clustersgalaxies: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 430 - 431
Copyright
Copyright © International Astronomical Union 2010

References

Arshakian, T. G., Beck, R., Krause, M., & Sokoloff, D. 2009, A&A, 494, 21Google Scholar
Beck, R. 2009, Rev. Mex. AyA 36, 1Google Scholar
Beck, R., Brandenburg, A., Moss, D., Shukurov, A., & Sokoloff, D. 1996, ARAA 34, 155CrossRefGoogle Scholar
Brandenburg, A. & Subramanian, K. 2005, Phys. Rep. 417, 1CrossRefGoogle Scholar
Brentjens, M. A. & de Bruyn, A. G. 2005, A&A 441, 1217Google Scholar
Gaensler, B. M., Beck, R., & Feretti, L. 2004, New Astr. Rev. 48, 1003CrossRefGoogle Scholar
Krause, M., Alexander, P., Bolton, R., et al. 2009, MNRAS, in pressGoogle Scholar
Kronberg, P. P., Bernet, M. L., Miniati, F., et al. 2008, ApJ 676, 70CrossRefGoogle Scholar
Lazar, M., Schlickeiser, R., Wielebinski, R., & Poedts, S. 2009, ApJ 693, 1133CrossRefGoogle Scholar
Rees, M. J. 2005, in: Wielebinski, R., & Beck, R. (eds.), Cosmic Magnetic Fields (Berlin: Springer), p. 1Google Scholar
Ryu, D., Kang, H., Cho, J., & Das, S. 2008, Science 320, 909CrossRefGoogle Scholar
Widrow, L. M. 2002, Rev. Mod. Phys. 74, 775CrossRefGoogle Scholar