## Abstract We propose a model of magneticβfield growth in galaxy clusters whereby the field is ampli.fied by a factor of about 10^8^ over a cosmologically short time of βΌ 10^8^ yr. Our model is based on the idea that the viscosity of the intracluster medium during the fieldβamplification epoch is
Magnetic fields in clusters of galaxies
β Scribed by L. Feretti; M. Johnston-Hollitt
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 358 KB
- Volume
- 48
- Category
- Article
- ISSN
- 1387-6473
No coin nor oath required. For personal study only.
β¦ Synopsis
An important area of study of cosmic magnetic fields is on the largest scales, those of clusters of galaxies. In the last decade it has become clear that the intra-cluster medium in clusters of galaxies is magnetized and that magnetic fields play a critical role in the cluster formation and evolution. The observational evidence for the existence of cluster magnetic fields is obtained by the diffuse cluster-wide synchrotron radio emission and from rotation measure studies of extragalactic radio sources located within or behind the clusters. A significant breakthrough in the knowledge of the cluster magnetic fields will be reached through the SKA, owing to its capabilities, in particular the deep sensitivity and the polarization purity.
π SIMILAR VOLUMES
## Abstract The analysis of Faraday rotation measurements (RM) gives insight into the properties of cluster magnetic fields. Recently, Kolmogorovβlike magnetic turbulence was reported for the cool core of the Hydra A galaxy cluster which was derived using a maximum likelihood analysis of an RM map