This thesis examines the occurrence of strong geomagnetic storms and how they have been reflected in the visibility of the aurora borealis in Slovenia between 1932 and 2024. The thesis first defines the basic concepts necessary for understanding the underlying physical processes. It then investigates the temporal and cyclical occurrence of individual solar cycles and geomagnetic storms, followed by a comparison of theoretical conditions with actual cases of auroral visibility over Slovenian territory. The second part focuses on actual observations of the aurora borealis in Slovenia and the ways in which the phenomenon has been detected and documented. Particular attention is given to the impact of modern technological advances and digital photography, which have significantly changed the methods of documenting the phenomenon as well as the frequency of recorded observations compared to the past. Finally, the thesis presents the concept of a comprehensive interpretation of physical data and field observations, emphasizing the importance of incorporating space weather into contemporary geographical research.
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