Fig. 9From: Initial performance of the radio occultation experiment in the Venus orbiter mission AkatsukiElectron density profile obtained from the ingress occultation (solid) that sampled an illuminate region (SZA = 78°) and the profile from the egress occultation (blue dashed) that sampled an unilluminated region (SZA = 102°) conducted on May 6, 2016Back to article page