Magellanic Clouds in our results and as seen with different observables, respectively: panels a and b show the Faraday rotation (with a 20 rad m⁻² offset) and the underlying amplitude field as inferred in this work. Panels c and d show the clouds in H α emission (Finkbeiner 2003; Gaustad et al. 2001), and in emission measure (EM), as obtained by the Planck satellite (Planck Collaboration X 2016), respectively. Panel c indicates the locations of the clouds.