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[en] We obtain the value of the mirror magnetic field during different stages of cosmological evolution. We consider the magnetic field generation in the radiation-dominated era and the post-recombination epoch. We also estimate its galactic low-scale value in the process of dynamo amplification. We discuss a possible effect of the mirror magnetic field on the mirror matter distribution in a galaxy. The model can be generalized by assuming the existence of kinetic mixing between ordinary and mirror particles.
Journal
Journal of Experimental and Theoretical Physics; ISSN 1063-7761; 
; CODEN JTPHES; v. 129(1); p. 19-27
; CODEN JTPHES; v. 129(1); p. 19-27