In this lecture note, we make the case for new (spectro)polarimetric measurements of changing-look AGNs (CLAGNs), a subclass of the AGN family tree that shows long-term (months to years) large flux variability associated with the appearance or disappearance of optical broad emission lines. We discuss how polarization measurements could help to distinguish which of the several scenarios proposed to explain such variations is/are the most likely. We collected past polarization measurements of nearby, Seyfert-like CLAGNs and take stock that almost all polarimetric information we have on those fascinating objects dates from the 80s and 90s. We thus explain how polarization could help us understand the physical processes happening in the first parsecs of CLAGNs and why new polarization monitoring campaigns are strongly needed.
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