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dc.contributor.authorBattaner, Eduardo-
dc.contributor.authorAgudo, Iván-
dc.contributor.authorAlberdi, Antxón-
dc.contributor.authorFlorido, Estrella-
dc.contributor.authorGuijarro, Ana-
dc.contributor.authorRuiz-Granados, Beatriz-
dc.contributor.authorRubiño-Martín, J. A.-
dc.date.accessioned2016-12-14T13:09:26Z-
dc.date.available2016-12-14T13:09:26Z-
dc.date.issued2015-
dc.identifierisbn: 978-84-606-8955-3-
dc.identifier.citationThe Spanish Square Kilometre Array White Book: 141-145 (2015)-
dc.identifier.urihttp://hdl.handle.net/10261/141438-
dc.description.abstractHigh–sensitivity, linear and circular polarization, large frequency range and good angular resolution are characteristics of the SKA which will allow a much deeper insight in all topics of Cosmic Magnetism. More specific goals will be: magnetism and cosmology, nearby galaxies, the so called fan region, the physics of AGN jets and cosmic ray anisotropies.-
dc.description.sponsorshipEB, EF, AG, BRG and JARM acknowledge support from the Spanish Ministry of Economy and Competitiveness (MINECO) through grants AYA2011-24728 and the Consolider-Ingenio project CSD2010-00064 (EPI: Exploring the Physics of Infation), and from Junta de Andalucía (CEIC) through the FQM-108 project. IA research is supported by a Ramón y Cajal grant of the Spanish MINECO. IA also acknowledges funding support by MINECO through grant AYA2013-40825-P.-
dc.publisherSociedad Española de Astronomía-
dc.relationMINECO/ICTI2013-2016/AYA2013-40825-P-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleCosmic magnetism-
dc.typeCapítulo de libro-
dc.date.updated2016-12-14T13:09:26Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.contributor.funderJunta de Andalucía-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
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