Planck 2015 results
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Fig. 3

image

Magnetically-induced CMB TT (top left), TE (top right), EE (bottom left), and BB (bottom right) power spectra due to passive tensor modes, compared with the ones that are due to compensated modes. The solid lines represent primary CMB anisotropies, the dotted lines represent magnetically-induced compensated scalar modes (except for the BB panel, where it represents the lensing contribution), the dashed lines represent vector modes, whereas dot-dashed lines represent magnetically-induced passive tensor modes. We consider PMFs with B1 Mpc = 4.5 nG and nB = −2.9.

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