Fig. 6
From: Scale analysis of equatorial plasma irregularities derived from Swarm constellation
Variation of R max with Δt in the a northern and b southern hemispheres during the second study period, but only for the pair Swarm A and C. Frames c and d represent the dependence of R max on local time. The gray triangles and vertical lines are the mean values and standard deviation of R max for each local time bin (1 h). Frames e and f show local time distribution of the occurrence ratio for those EPI events with R max > 0.7 between Swarm A and C