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On the variations of ionospheric parameters made at a near equatorial station in the African longitude sector: IRI validation with the experimental observations
Author(s) -
O. S. Oyekola,
P. R. Fagundes
Publication year - 2012
Publication title -
earth planets and space
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.835
H-Index - 74
eISSN - 1880-5981
pISSN - 1343-8832
DOI - 10.5047/eps.2011.10.004
Subject(s) - ionosonde , ionosphere , longitude , altitude (triangle) , latitude , international reference ionosphere , atmospheric sciences , electron density , f region , total electron content , environmental science , physics , meteorology , geodesy , electron , geography , mathematics , geophysics , geometry , quantum mechanics , tec
We examine the main morphological patterns and climatological behaviour of equatorial F2 region over African sector using hourly observational values of F2 peak height of maximum electron density (h m F2), F2 layer peak electron density (N m F2/ foF2), and propagation factor (M3000F2) hitherto made by the Ibadan ionosonde at 7.4°N, 3.9°E, dip latitude 2.3°S, in Nigeria; between January to December 1958, during a period of high solar activity (yearly averaged Rz12 = 190 units) and magnetically quiet conditions (Kp ≤ 3). A direct comparison between these measurements and the International Reference Ionosphere 2007 (IRI-2007) model-predictions are also made. The results of comparisons illustrate that good advancement has been made but reveal some important discrepancies. The trends in the experimental data are found to be in excellent agreement with the trends in the simulation results for maximum electron density and propagation factor, but fair-to-good for F2 layer peak altitude. The model is unable to capture the sharp postsunset and predawn enhancements in h m F2 and M3000F2, respectively. The model results have errors ranging from approximately 8–15%, 9–17%, and 3–5%, respectively, for h m F2, N m F2, and M3000F2. On average, the percent absolute relative difference of the model from the experimental observations varies from about 0–20%, 0–30%, and 0–10% for h m F2, N m F2, and M3000F2, in that order. Our results are essentially consistent with other equatorial and low-latitude ground-based measurements over South America, India, and Southeast Asia.

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