Author:
Odeyemi Olumide Olayinka,Adeniyi Jacob,Oladipo Olushola,Olawepo Olayinka,Adimula Isaac,Oyeyemi Elijah
Abstract
Abstract. We investigated total electron content (TEC) at Ilorin (8.50∘ N
4.65∘ E, dip lat. 2.95) for the year 2010, a year of low solar
activity in 2010 with Rz=15.8. The investigation involved the use of TEC
derived from GPS, estimated TEC from digisonde portable sounder data (DPS),
and the International Reference Ionosphere (IRI) and NeQuick 2 (NeQ) models.
During the sunrise period, we found that the rate of increase in DPS TEC, IRI
TEC, and NeQ TEC was higher compared with GPS TEC. One reason for this can be
attributed to an overestimation of plasmaspheric electron content (PEC)
contribution in modeled TEC and DPS TEC. A correction factor around the
sunrise, where our finding showed a significant percentage deviation between
the modeled TEC and GPS TEC, will correct the differences. Our finding
revealed that during the daytime when PEC contribution is known to be absent
or insignificant, GPS TEC and DPS TEC in April, September, and December
predict TEC very well. The lowest discrepancies were observed in May, June,
and July (June solstice) between the observed values and all the model values
at all hours. There is an overestimation in DPS TEC that could be due to
extrapolation error while integrating from the peak electron density of F2
(NmF2) to around ∼1000 km in the Ne profile. The
underestimation observed in NeQ TEC must have come from the inadequate
representation of contribution from PEC on the topside of the NeQ model
profile, whereas the exaggeration of PEC contribution in IRI TEC amounts to
overestimation in GPS TEC. The excess bite-out observed in DPS TEC and
modeled TEC indicates over-prediction of the fountain effect in these models.
Therefore, the daytime bite-out observed in these models requires a modifier
that could moderate the perceived fountain effect morphology in the models
accordingly. The daytime DPS TEC performs better than the daytime IRI TEC and
NeQ TEC in all the months. However, the dusk period requires attention due to
the highest percentage deviation recorded, especially for the models, in
March, November, and December. Seasonally, we found that all the TECs
maximize and minimize during the March equinox and June solstice,
respectively. Therefore, GPS TEC and modeled TEC reveal the semiannual
variations in TEC.
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geology,Astronomy and Astrophysics
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