Fig. 14

Three degree smoothed map of the difference between the main and side arm of LFI25 before (top) and after (bottom) ADC non-linearity correction. Stripes can seen which are stronger in the region where the solar dipole peaks, as a result of residuals from calibration uncertainties. This relative uncertainty between radiometer arms directly affects polarization as shown here, since the main and side arm difference represents a pseudo-polarization.
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