dc.description.abstract |
Ionosphere, is a thin layer of plasma that occupies the upper layer of the Earth's atmosphere,
affecting radio communications, satellite navigation, and space weather. For this reason,
monitoring changes in the ionosphere is quite vital. One of the crucial parameters expressing
the characteristic of the ionosphere is the total electron content (TEC), which is a function of
electron density. This study investigat es the variations in vertical total electron Content
(vTEC) of the ionosphere during solar cycle 24, particularly focusing on the solar maximum
period (2014 and 2015), over Africa. Its variations during this cycle are essential for
enhancing space weather prediction and improving communication and navigation systems.
The observational data from ground-based Global Positioning System (GPS), inferred from
dual-frequency GPS receivers established at Rabat, Malindi, Zambia, and Yamoussoukro
over Africa in the years 2014 and 2015 were used. It was used to study the hourly, diurnal,
seasonal, and latitudinal variations in ionospheric vTEC at these GPS stations as insufficient
research results of ionospheric variations are available for these areas.
Our findings reveal distinct diurnal patterns: vTEC reaches its minimum morning, gradually
increases throughout the day, peaks in the afternoon, and then declines after sunset. This
behavior is primarily driven by photoionization due to solar radiation. Conversely, nighttime
electron loss processes lead to decreased vTEC values. Seasonal variations were also
observed, with the highest vTEC recorded during the equinoxes, intermediate values during
the June solstice, and the lowest during the December solstice. Additionally, vTEC values
were influenced by the latitudinal position of the GPS receivers; higher electron
concentrations were found at lower latitudes, diminishing toward the poles. For future
research, we want to recommend others use, as far as possible, complete data and consider
the long-term studies of these GPS receiver stations to enhance our understanding of
ionospheric dynamics. |
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