ABSTRACT: The validation of IRI-2012 modelwas carriedout on experimental data obtained at an equatorial station [12.4°N, 1.5°W,dip latitude: 5.9°N]. Four ionosphericparameters, namely, the F2 layer peak electron density (NmF2), the corresponding height (hmF2), the bottom-side parameter (B0) and the shape parameter (B1), were used. The observed data were compared with the data generated from IRI-2012 model, using the two coefficients, URSI and CCIR options of the model.Both the URSI and CCIR options of theIRI-2012 modeleither underestimated or overestimated NmF2 during the period considered, at almost all the hours of the day..
Keywords: Equatorial ionosphere, low solar activity, electron density.
[1]. Adeniyi, J.O., S.M. Radicella, I.A. Adimula, A.A. Willoughby, O.A. Oladipo, and O. Olawepo (2008), Validation of B0 and B1 in the IRI 2001 model at low solar activity for Ilorin an equatorial station, Advances in Space Research 42 (2008) 691–694.
[2]. Altadill, D., J.M. Torta, and E. Blanch, (2009), Proposal of new models of the bottom-side B0 and B1 parameters for IRI, Adv. Space Res., 4, 1825–1834, DOI:10.1016/j.asr.2008.08.014
[3]. Asmare, Y., T. Kassa, and M. Nigussie (2014), Validation of IRI-2012 TEC model over Ethiopia during solar minimum (2009) and solar maximum (2013) phases, Advances in Space Research 53 (2014) 1582–1594.
[4]. Bertoni, F., Y. Sahai, W. L. C. Lima, P. R. Fagundes, V. G. Pillat, F. Becker-Guedes, and J. R. Abalde (2006), IRI-2001 model predictions compared with ionospheric data observed at Brazilian low latitude stations, Ann. Geophys., 24, 2191–2200.
[5]. Bilitza, D. (2001), International Reference Ionosphere 2000, Radio Science, Volume 36, Number 2, Pages 261-275..