Characterization of GPS-TEC over African equatorial ionization anomaly (EIA) region during 2009–2016. Issue 1 (1st January 2019)

• Record Type: Journal Article
• Authors: Oluwadare, Temitope Seun; Nguyen Thai, Chinh; Akala, Andrew Oke-Ovie; Heise, Stefan; Alizadeh, Mahdi; Schuh, Harald
• Is Part Of: Advances in space research. Volume 63:Issue 1(2019)
• Page Start: 282
• Page End: 301
• Publication Date: 2019-01-01
• Subjects: African equatorial ionosphere -- Global Positioning System (GPS) – TEC -- Solar activity and cycle 24; Space sciences -- Periodicals; Astronautics -- Periodicals; Geophysics -- Periodicals; 500.505
• DOI: 10.1016/j.asr.2018.08.044
• Languages: English
• ISSNs: 0273-1177

Abstract

Abstract: This study characterizes total electron content (TEC) measured by Global Positioning System (GPS) over African equatorial ionization anomaly (EIA) region for 2009–2016 period during both quiet geomagnetic conditions (Kp ≤ 1) and normal conditions (1 > Kp ≤ 4). GPS-TEC data from four equatorial/low-latitude stations, namely, Addis Ababa (ADIS: 9.04°N, 38.77°E, mag. lat: 0.2°N) [Ethiopia]; Yamoussoukro (YKRO: 6.87°N, 5.24°W, mag. lat: 2.6°S) [Ivory Coast]; Malindi (MAL2; 3.00°S, 40.19°E, mag. lat: 12.4°S) [Kenya] and Libreville (NKLG; 0.35°N, 9.67°W, mag. lat: 13.5°S) [Gabon] were used for this study. Interesting features like noontime TEC bite-out, winter anomaly during the ascending and maximum phases of solar cycle 24, diurnal and seasonal variations with solar activity have been observed and investigated in this study. The day-to-day variations exhibited ionospheric TEC asymmetry on an annual scale. TEC observed at equatorial stations (EIA-trough) and EIA-crest reach maximum values between ∼1300–1600 LT and ∼1300–1600 LT, respectively. About 76% of the high TEC values were recorded in equinoctial months while the June solstice predominantly exhibited low TEC values. Yearly, the estimated TEC values increases or decreases with solar activity, with 2014 having the highest TEC value. Solar activity dependence of TEC within the EIA zone reveals that both F10.7 cm index and EUV flux (24–36 nm) gives a stronger correlation with TEC than Sunspot Number (SSN). A slightly higher degree of dependence is on EUV flux with the mean highest correlation coefficient (R) value of 0.70, 0.83, 0.82 and 0.88 for quiet geomagnetic conditions (Kp ≤ 1) at stations ADIS, MAL2, NKLG, and YKRO, respectively. The correlation results for the entire period consequently reveals that SSN and solar flux F10.7 cm index might not be an ideal index as a proxy for EUV flux as well as to measure the variability of TEC strength within the EIA zone. The estimated TEC along the EIA crest (MAL2 and NKLG) exhibited double-hump maximum, as well as post-sunset peaks (night time enhancement of TEC) between ∼2100 and 2300 LT. EIA formation was prominent during evening/post-noon hours.