Figure 4
From: Hemispheric asymmetry of the dayside aurora due to imbalanced solar insolation
Comparisons of the latitudinal energy flux profile at (a,d) the 1,400–1,600 MLT, (b,e) 1,100–1,300 MLT, and (c,f) 0,900–1,100 MLT sectors for (top panels) all solar wind corresponding to Fig. 2 and (bottom panels) weak solar wind driving corresponding to Fig. 3. In each panel, blue is for sunlit NH, orange is for dark NH, red is for sunlit SH, and cyan is for dark SH. The vertical bar at each latitudinal bin represents standard deviation of the mean. The inserts in each panel are the sunlit-to-dark ratio of latitudinal integrated and peak (in the parenthesis) energy flux.
