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Fig. 18


Same as in Fig. 17 but for two fields at intermediate Galactic latitudes sampling the diffuse ISM. The central pixel for the top panels corresponds to (l,b) = (6°,37°). The central pixel for the bottom panels corresponds to (l,b) = (295°, −40°). The Magellanic Clouds in the bottom extinction map (left) are masked. Most of the structures in the relative orientation maps appear as parallel to the magnetic field.

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