2005/11/30 by Torsten A. Ensslin, T. A. Enßlin, Corina Vogt +5 · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Cosmology and Gravitation Theories #Solar and Space Plasma Dynamics #astro-ph
paper · pdf · doi:10.1002/asna.200610607
invited talk at conference on `The Origin and Evolution of Cosmic Magnetism' in Bologna 2005, eds. R. Beck, G. Brunetti, L. Feretti, and B. Gaensler, to appear in Astronomische Nachrichten, 6 pages, 3 figures, typo corrected
arxiv created 2006/01/04 · openalex publication_date 2006/05/16 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
Abstract The Planck mission will permit measurements of the polarization of the cosmic microwave background and of polarized foregrounds such as our own Galaxy with an unprecedented combination of accuracy and completeness. This will provide information on cosmological and galactic magnetic fields. The latter can be studied in detail via nearly Faraday‐rotation free synchrotron and polarized dust emission. Methods are discussed to extract physically relevant information on the magnetic turbulence from Planck data and other measurements. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)