Ionospheric F2-Region Characteristics of Profile Parameters at an Equatorial Station During Low Solar Activity

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O. E. Ehinlafa
G. A. Alagbe
M. J. Johnson
S. O. Ige
J. O. Adeniyi

Abstract

The ionospheric characteristics of the F2 region critical frequency (foF2), peak electron density (NmF2) and the height of occurrence of electron density (hmF2), was investigated over Ilorin (lat. 8.31°N, long. 4.34°E, dip lat. 2.95o), a station along the equatorial ionization anomaly trough, during a period of low solar activity (LSA). Diurnally, foF2, NmF2 and hmF2 were found to have two characteristic peaks: pre-noon and post-noon peaks, except hmF2 that has post-sunset peak. The foF2 and NmF2 pre-noon peaks occurred around 0800–0900 LT, hmF2’s peak around 1000 LT. The post-noon peaks of foF2 and NmF2 were observed around 1500 and 1800 LT, while hmF2 was observed around 1800 and 1900 LT. In general, the magnitude of the pre-noon peak is less than that of the post-noon/post-sunset peak for all the parameters, for all the seasons. The highest magnitudes of foF2 and NmF2 were reached in the equinoctial months. The rapid faster electron drift in hmF2 away from the equator is responsible for the sharp drop in foF2 and NmF2 after sunset in all seasons. Seasonal peaks in general are suspected to be controlled by the enhanced E × B drifts and, the atmospheric wind, which is consistent with some earlier results obtained at some stations in the African region during low solar activity periods.

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Ehinlafa, O. E., Alagbe, G. A., Johnson, M. J., Ige, S. O., & Adeniyi, J. O. (2024). Ionospheric F2-Region Characteristics of Profile Parameters at an Equatorial Station During Low Solar Activity. Nigerian Journal of Physics, 32(4), 73–80. https://doi.org/10.62292/njp.v32i4.2023.55
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References

Adebesin, B.O., Adeniyi, J.O., Adimula, I.A., Reinisch, B.W., and Yumoto, K., (2013a) Equatorial vertical plasma drift velocities and electron densities inferred from ground-based ionosonde measurements during low solar activity; J. Atmos. Sol. Terr. Phys. 97, 58–64, doi: 10.1016/j.jastp.2013.02.010.

Adebesin, B. O., Adeniyi, J. O., Adimula, I. A., Reinisch, B. W. and Yumoto, K. (2013b) F2 layer characteristics and electrojet strength over an Equatorial station; Adv. Space Res., 52(5), 791–800, doi: 10.1016/j.asr2013.05.025

Adebesin B O (2012) foF2 variations during geomagnetic disturbances at the rise of solar cycle 23; Indian J. Radio and Space Phys. 41(3), 323–331

Adeniyi, J. O., Oladipo, O. A. and Radicella, S. M. (2007) Variability of foF2 for an equatorial station and comparison with the foF2 maps in IRI model; J. Atmos. Sol. Terr. Phys. 69. 721–733

Alagbe, G. A. (2012) Geomagnetic storm effects on F2 layer peak electron density and other profile parameters at high solar activity at an equatorial station; J. Phys. Sci. Innovation 4, 5–12, ISSN 2277–0119

Anderson, D. N., Anghel, A., Yumoto, K., Ishitsuka, M., Kudeki, E., (2002) Estimating daytime, vertical E B drift velocities in the equatorial F region using ground-based magnetometer observations. Geophys. Res. Lett. 29 (12). http://dx.doi.org/10.1029/ 2001GL014562.

Atac A, Ozguc A and Pektas R (2009) The variability of foF2 in different phases of solar cycle 23; J. Atmos. Sol. Terr. Phys. 71, 583–588.

Babatunde, A., Olamike, R., Teiji, D.F., Nurul, U., Shazana, A.H., and Akimassa, Y. (2017) Longitudinal Variation of Equatorial Electrojet and the Occurrence of Its Counter Electrojet. Annales Geophysicae, 35, 535-545.

Bai, H.; Feng, F.; Wang, J. (2020) A Combination Prediction Model of Long-Term Ionospheric foF2 Based on Entropy Weight Method. Entropy 2020, 22, 442.

Bilitza, D., Altadill, D., Zhang, Y., Mertens, C., Truhlik, V., Richards, P., McKinnell, L.A. and Reinisch, B. (2014) The International Reference Ionosphere 2012—A Model of International Collaboration. Journal of Space Weather and Space Climate, 4, A07.

Bittencourt, J. A. and Abdu, M. A. (1981) A theoretical comparison between apparent and real vertical ionization drift velocities in the equatorial Fregion. J. Geophys. Res., 86, 2451–2454.

Chen, C. H., Liu, J. Y., Yumoto, K., Lin, C. H., Fang, T. W. (2008) Equatorial ionization anomaly of the total electron content and equatorial electrojet of ground-based geomagnetic field strength J. Atmos. Sol. Terr. Phys., 70, 2172–2183.

Chen, C.; Wu, Z.S.; Xu, Z.W.; Sun, S.J.; Ding, Z.H.; Ban, P.P. (2010) Forecasting the local ionospheric foF2 parameter 1 hour ahead during disturbed geomagnetic conditions. J. Geophys. Res. Space Phys. 2010, 115, 135–146.

Chou Y. T. and Lee C. C. (2008) Ionospheric variability at Taiwan low latitude station: Comparison between observations and IRI 2001 model; Adv. Space Res. 42, 673–681.

Diabaté, A., Zerbo, J.-L. and Ouattara, F. (2019) Variation of the foF2 Parameter during Fluctuating Activity: Prediction with IRI-2012 Compared to Measured Data from Ouagadougou Ionosonde Station during Solar Cycles 21 and 22. Vietnam Journal of Earth Sciences, 41, 69-78.

Fejer, B. G., Scherliess, L., de Paula, E. R. (1999) Effects of the vertical plasma drift velocity on the generation and evolution of equatorial spread F. J. Geophys. Res., 104, 19854–19869.

Fejer B G (1997) The electrodynamics of the low latitude ionosphere recent results and future challenges; J. Atmos. Sol. Terr. Phys. 59, 1465–1482.

Fejer B G, de Paula E R, Heelis R A and Hanson W B (1995) Global equatorial ionosphere vertical plasma drifts measured by the AE-E Satellite; J. Geophys. Res. 100, 5769–5776.

Jayachandran, B., Balachandran, N.R., Balan, N. and Rao, P.B., (1995): Short time variability of the ionospheric electron content and peak electron density during solar cycles for a low latitude station, J. Atmos. Sol. Terr. Phys.,52, 1599-1605.

Lastovcka, J., Yue, X. and Wan, W. (2008) Long-Term Trends in foF2: Their Estimating and Origin. Annales Geophysicae, 26, 593-598.

Oladipo O A, Adeniyi J O, Radicella S M and Obrou O K (2008) Variability of equatorial ionospheric electron density at fixed heights below the F2 peak; J. Atmos. Sol. Terr. Phys. 70, 1056–1065.

Oladipo O A, Adeniyi J O and Radicella S M 2009 Electron density distribution at fixed heights N(h): Gaussian distribution test; J. Atmos. Sol. Terr. Phys. 71, 1–10

Olga, M., (2021) The Influence of Space Weather on the Relationship between the Parameters TEC and foF2 of the Ionosphere, IEEE J. Radio Freq. Identify, 5, 261 - 268

Ouattara, F. (2013) IRI-2007 foF2 Predictions at Ouagadougou Station during Quiet Time Periods from 1985 to 1995. Archives of Physics Research, 4, 12-18.

Ouattara, F. and Zerbo, J.L. (2011) Ouagadougou Station F2 Layer Parameters, Yearly and Seasonal Variations during Severe Geomagnetic Storms Generated by Coronal Mass Ejections (CMEs) and Fluctuating Wind Streams. International Journal of the Physical Sciences, 6, 4854-4860.

Radicella, S.M. and Adeniyi, J.O., (1999) Equatorial ionospheric electron density below the F2 peak. Radio Science, 34(5), 1153- 1163.

Sawadogo, W.E., Zerbo, J.-L. and Ouattara, F. (2019) Diurnal Variation of F2-Layer Critical Frequency under Solar Activity Recurrent Conditions during Solar Cycles 21 and 22 at Ouagadougou Station: Prediction with IRI-2012. Scientific Research and Essays, 14, 111-118.

Tariku, Y.A. (2015) TEC Prediction Performance of the IRI-2012 Model over Ethiopia during the Rising Phase of Solar Cycle 24 (2009-2011). Earth, Planets and Space, 67, 140.