Variability of foE in the equatorial ionosphere with solar activity Original Research Article

This research examined the variability of foE in the equatorial ionosphere with solar activity within the equatorial ionospheric anomaly region. Ionosonde data recorded at Ouagadougou (lat. 12.4°N, long. 1.5°W and magnetic dip 1.43°N) were engaged to study the transient variations of the critical frequency of the E-layer (foE) and its dependence on solar activity. The study revealed that foE increases with the increase in solar intensity of the sun. The variability of the foE decreases with increases in the solar activity. The maximum value of the foE is at local noon when the ionosphere is stable; the variability at this local time is minimal. The minimum value of the foE is at sunrise and sunset, at this period on local time the equatorial ionosphere recorded its maxima variability. Irrespective of the degree of solar activity, foE is observed to be maximum in June solstice, followed by the equinoxes and minimum in December solstice. Equinoctial asymmetry occurred in the variation of the relative standard deviation of foE with maximum in September/March equinox for low/high solar activity.