Preprints
https://doi.org/10.5194/egusphere-2026-5194
https://doi.org/10.5194/egusphere-2026-5194
04 Sep 2026
 | 04 Sep 2026
Status: this preprint is open for discussion and under review for Annales Geophysicae (ANGEO).

Multifractal characterization of daily maximum and minimum ionospheric TEC at African equatorial stations

Babatunde Rabiu, Samuel Ogunjo, and Ayomide Olabode

Abstract. The temporal scaling structure of the ionospheric vertical total electron content (vTEC) carries fundamental information about the intrinsic dynamics of the equatorial and low-latitude plasma system. This study applies Multifractal Detrended Fluctuation Analysis (MFDFA) to investigate the intrinsic dynamics of the variability of the ionosphere over African equatorial stations using the daily maximum and minimum vTEC time series recorded at three GNSS stations (Dakar (DAKR), Libreville (NKLG), and Djibouti (DJIG) spanning the equatorial ionisation anomaly (EIA) crest and its flanks. Seasonal trend components are isolated using Seasonal and Trend decomposition with Loess (STL) to separate the contribution of the seasonal cycle from intrinsic ionospheric dynamics. The raw maximum vTEC series exhibit clear semi-annual modulation and multifractality at all stations, with generalised Hurst exponents 0.104 ≤h(q=2)0.193 and statistically significant singularity spectral widths. A crossover in scaling behaviour near n150 days reveals scale-dependent persistence that is stronger at sub-annual scales. The raw minimum vTEC series confirm multifractality but with consistently narrower singularity spectra and weaker q-dependence, reflecting the reduced dynamic range of the nighttime ionosphere in the absence of photo-ionisation. These results reveal a clear daytime-nighttime asymmetry in ionospheric scaling dynamics and establish the EIA crest as a region of persistent, non-seasonal nonlinear variability that manifests across both the daytime and nighttime ionosphere. The findings demonstrate that MFDFA applied to the diurnal extremes of vTEC provides a sensitive and physically interpretable diagnostic of equatorial ionospheric complexity that is not accessible through conventional spectral or trend-based analyses.

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Babatunde Rabiu, Samuel Ogunjo, and Ayomide Olabode

Status: open (until 16 Oct 2026)

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Babatunde Rabiu, Samuel Ogunjo, and Ayomide Olabode
Babatunde Rabiu, Samuel Ogunjo, and Ayomide Olabode
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Short summary
The upper atmosphere over Africa, despite is importance in communication and navigation, is poorly understood. We studied the  daily maximum and minimum of the total electron content above three African stations near the equator, applying a technique that reveals hidden patterns across many timescales. Daytime values proved far more variable than nighttime ones, reflecting how sunlight drives this activity. The findings help improve forecasts of communication over Africa.
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