Abstract:
This thesis investigates the impact of geomagnetic storms on the global ionospheric Total
Electron Content (TEC) during selected events from April 2023 to August 2024. The primary
objective is to analyze the dynamic response of the ionosphere to solar and geomagnetic
activities, focusing on the variations in TEC associated with these storm events. The research
utilizes data obtained from the Global Ionospheric Map to evaluate significant fluctuations in
TEC during multiple geomagnetic storm episodes. Notably, the storm event from April 22-25,
2023, resulted in a substantial decrease in TEC, particularly pronounced in the Northern
Hemisphere, highlighting the storm's adverse effects on satellite communication and
navigation. Conversely, the geomagnetic storm in November 2023 led to an increase in TEC
across both hemispheres, illustrating the complexity and variability of ionospheric responses
to geomagnetic disturbances. The findings emphasize the necessity for region-specific
analyses to accurately predict TEC behavior during such disturbances. A critical observation
is the asymmetric response of the Northern and Southern Hemispheres, where contrasting
TEC behaviors were noted during the March 2024 storm. This underscores the intricate
dynamics at play within the ionosphere, indicating that one hemisphere may benefit from
improved conditions while the other may experience detrimental effects during the same
storm. Additionally, the study explores the influence of atmospheric composition on TEC
variations, particularly during storm events. Changes in the oxygen-to-nitrogen ratio were
linked to significant impacts on ionospheric electron density, suggesting that thermospheric
shifts can have profound effects on ionospheric behavior. Overall, the thesis advocates for
continuous monitoring of ionospheric conditions to enhance predictive capabilities and
mitigate the impacts of geomagnetic storms on technological applications. By deepening our
understanding of TEC fluctuations and their underlying mechanisms, this research
contributes to the ongoing efforts to maintain reliable communication and navigation systems
in the face of evolving space weather conditions.