Fig. 5From: Estimation of the emission altitude of pulsating aurora using the five-wavelength photometera MLT distribution of intervals of pulsating aurora sampled from 37 nights of observations. b Dependence of the altitude of pulsating aurora on magnetic local time. The red cross marks and vertical bars respectively indicate the average and standard deviation of the altitude of pulsating aurora calculated every 1-h magnetic local time binBack to article page