Observational study reveals longitudinal day-to-day ionospheric variability across equatorial Africa, suggesting short-period lower-atmospheric forcing drives rapid fluctuations.
The rate of change of the total electron content index (ROTI) is a widely used proxy for phase fluctuations associated with ionospheric irregularities derived from GNSS total electron content measurements. This study investigates the longitudinal day-to-day variability of ionospheric irregularities over the African Equatorial Ionization Anomaly (EIA) region during 2014 using ROTI from six GNSS stations at low latitudes. Day-to-day variability is quantified through differences between consecutive daily ROTI values (ΔROTI), relative ROTI (RROTI), correlation coefficients, daily deviations from climatology, and variability magnitude. The results reveal clear longitudinal day-to-day variability between East and West African sectors, with larger variability in West Africa. Diurnal ROTI peaks reach about 2 TECU/min in East Africa and about 3 TECU/min in West Africa. Correlation coefficients within the same longitude sector range from 0.678 to 0.848, whereas cross-sector correlations range from 0.476 to 0.689. ΔROTI and RROTI indicate that day-to-day variability is driven mainly by short-period lower-atmospheric forcing rather than slow solar forcing. Relative variations range from about -70% to +150%, with predominantly negative values during solstices and positive values during equinoxes.
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Endeshaw et al. (2026) studied this question.
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