The F2 region critical frequency ( f o F2 ) and peak electron density ( N m F2 ) morphology was investigated over Ilorin (latitude 8.31°N, longitude 4.34°E) during a Low Solar Epochs (LSE), a station along the equator anomaly trough. Diurnally, f o F2 and N m F2 are visibly more prominent during the day than at night with two characteristic peaks: pre-noon and post-noon peaks. The f o F2 and N m F2 pre-noon peak magnitude range: (7.7–8.3 MHz) and (7.3–8.6) × 10 11 /m -3 respectively is less compared to the f o F2 and N m F2 post-noon peak magnitude range: (7.3–9.7 MHz) and (6.7–11.7) ×10 11 /m -3 respectively. Seasonally, the highest values were attained during the post-noon peak in the equinoctial months compared to the solstices months, and also, annually, the post-noon peak is higher than the pre-noon peak. The rapid electron drift away from the equator is responsible for the sharp drop in f o F2 and N m F2 after sunset in all seasons. Seasonal peaks in f o F2 and N m F2 are suspected to be controlled by the enhanced E × B drifts and the onset and turn-off of solar ionization, which is consistent with some earlier results obtained at some stations in the African region during low solar epoch periods.
