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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2829 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2829 http://eprints.org/relation/ismediumThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2829 2840 2 8101 document 2840 small.jpg image/png 2b10791dab01da55e685c3eec7701833 MD5 1714 2014-01-27 20:55:02 http://eprints.iliauni.edu.ge/731/6/small.jpg 731 6 6 image/png other Thumbnails conversion from text to thumbnail_small ge public

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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2829 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2829 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2829 archive 131 disk0/00/00/07/31 2014-01-30 12:34:52 2015-03-27 06:51:42 2014-01-30 12:34:52 article show Durrer Ruth Kahniashvili Tina tinatin@iliauni.edu.ge Yates Andrew pub QC public We investigate microwave background anisotropies in the presence of primordial magnetic fields. We show that a homogeneous field with fixed direction can amplify vector perturbations. We calculate the correlations of δT/T explicitly and show that a large scale coherent field induces correlations between al-1,m and al+1,m. We discuss constraints on the amplitude and spectrum of a primordial magnetic field imposed by observations of CMB anisotropies. 1998 published Microwave background anisotropies from Alfvén waves 58 123004 TRUE