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We studied the responses of the ionosphere over the southern and northern African sector. A RINEX formatted TEC data obtained from the global positioning system (GPS) was used to study the impact of geomagnetic storms of 23rd June and 20th December on a South African station, SUTM (33.97°N, 6.84°W) and a Moroccan station, RABT (32.41°S, 38.75°E). The storms which occurred in summer and winter (solstice months) were quantified using the Dst data from World Data Center, Kyoto, Japan. The results showed obvious hemispheric and seasonal influences on ionospheric responses to the geomagnetic storms. The substorm-time responses of the ionosphere were always positive across the stations and seasons. This is a result of increased particle and energy depositions occasioned by the proton density (PD). The rates of energy and particles intensifications during substorms were higher in the summer storm event than in winter for both stations. In other words, there was no hemispheric asymmetry observed. In addition to the storm onset time, its peak time and hemispheric location are crucial in storm-time ionospheric responses. Local timing of the orientations of the prompt penetration and disturbance dynamo electric fields during northward interplanetary magnetic fields determined the nature of ionospheric responses in the day and night sides. These results contribute to our understanding of the dynamics and complexities of the ionosphere over African mid latitude ionosphere.
Astrophysics and Space Science – Springer Journals
Published: May 1, 2023
Keywords: Solar quiet (Sq); Disturbance dynamo electric field (DDEF); Total electron content (TEC); Prompt penetration electric (PPEF); Geomagnetic storm event; Interplanetary (CME); Disturbance storm time (Dst); Hemispheric
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