Assessment of long-term impact of solar activity on the ionosphere over an African equatorial GNSS station

Moses, Mefe; Panda, Sampad Kumar; Dodo, Joseph D.; Ojigi, Lazarus Mustapha; Lawal, K. M.

doi:10.1007/s12145-022-00863-y

Cited by 2 publications

(1 citation statement)

References 26 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…However, the ionization at the F 2 region peak seems to be more complex. The level of solar activity and its influence on ionospheric variability in the TEC during the solar cycle 24 also was recently discussed by [7]. It was mentioned that the decrease in the ultraviolet ray intensity and solar ionization during the solar maximum period (2013 to 2014) of solar cycle 24 was the key factor for driving the decreasing trend in TEC between 1999 and 2017.…”

Section: Introductionmentioning

confidence: 97%

Ionospheric Variability over the Brazilian Equatorial Region during the Minima Solar Cycles 1996 and 2009: Comparison between Observational Data and the IRI Model

et al. 2022

View full text Add to dashboard Cite

The behavior of the Brazilian equatorial ionosphere during the solar minimum periods, 1996 and 2009, which cover the solar cycles 22/23 and 23/24, respectively, is investigated. For this, the F2 layer critical frequency (foF2) and peak height (hmF2) registered by a Digisonde operated at São Luis (2.33° S; 44° W) are carefully analyzed. The results show that the seasonal mean values of the foF2 and the hmF2 in the equinoxes and winter during 2009 were lower than in 1996. In the summer, an anomalous response to solar variability was observed. In this case, the hmF2 in 2009 is higher than in 1996 during a specific daytime interval. Besides that, it was verified that the prereversal enhancement of the zonal electric field (PRE) during the equinoxes in 2009 occurred a few minutes earlier than in 1996. Additionally, a Fast Fourier Transform (FFT) analysis was used to investigate the impacts of solar atmospheric tides (amplitude, diurnal, semidiurnal, and terdiurnal modes) on foF2 and hmF2 parameters with respect to its seasonality. Significant differences were observed between their values during the two minima, mainly in the amplitude of hmF2, which was higher in 1996 than in 2009 for all days analyzed. Moreover, the seasonality in the diurnal and semidiurnal modes for both periods presented an annual variability, while the terdiurnal mode exhibited annual and semiannual components. The results are compared with the International Reference Ionosphere (IRI) model, and the main differences between the observation and the model results are discussed in this work.

show abstract

Section: Introductionmentioning

confidence: 97%