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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2495 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2495 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2495 archive 131 disk0/00/00/06/49 2014-01-27 08:59:30 2015-05-01 06:16:56 2014-01-27 08:59:30 article show Kahniashvili Tina tinatin@iliauni.edu.ge pub QB QC public I present a short review of primordial magnetic helicity effects on Cosmic Microwave Background (CMB) temperature and polarization anisotropies. These effects allow us to test for cosmological magnetic helicity; however, very accurate CMB fluctuation data are required. This scheme for magnetic helicity detection is valid only for a cosmological magnetic field with a present amplitude larger than 10-9-10-10 Gauss. 2006 published Astronomische Nachrichten, 327 414-418 TRUE