Fig. 8From: On a simple, data-aided analytic description of the morphology of equatorial F-region zonal plasma driftsComparison of the local time dependence of the Pedersen conductance (left), Hall conductance (middle), and Hall-to-Pedersen ratio (right) during June solstice at an apex height of 240 km. The solid (dashed) lines correspond to HSF (LSF) conditionsBack to article page