Fig. 4
Mean (solid lines) and standard (dashed lines) deviation profiles towards the Galactic disk (5° ≲|b|≲ 10°) for the |∇P|/|P| intensity as a function of Galactic longitude. The ranges of Galactic longitudes corresponding to the main Galactic features and spiral arms are also indicated. Data points are obtained from square regions of size 5°.
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