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Blazar CTA 102 underwent exceptional optical and high-energy outbursts in 2012 and 2016–2017. We analyze its behaviour during these events, focusing on polarimetry as a tool that allows us to trace changes in the physical conditions and geometric configuration of the emission source close to the central black hole. We also use Fermi    γ   -ray data in conjunction with optical photometry in an effort to localize the origin of the outbursts

Behaviour of the Blazar CTA 102 during Two Giant Outbursts