Dust profiles in latitude for the models as in Fig. 4. The top shows the inner Galaxy (i.e., −90° <l< 90°), while the bottom shows the third quadrant (180° <l< 270°, i.e., the outer Galaxy excluding the Fan region). For total intensity on the left, the Commander dust solution in solid black is compared to the Planck 2013 dust model of Planck Collaboration XI (2014) (black dashed), but the difference is not generally visible. (Since the models shown in colour differ only in the magnetic field, which has no impact on the dust total intensity, these curves are not distinguishable.)