UNDERSTANDING GEOMAGNETIC STORM IN RELATION TO THE SUNSPOT NUMBER DURING SOLAR CYCLE 24 AND 25

Abstract

Geomagnetic storms, caused by disturbances in Earth’s magnetosphere due to solar activity, are significant drivers of space weather and have profound effects on technological systems and infrastructure. This study investigates the relationship between geomagnetic storms and sunspot numbers, a primary indicator of solar activity, during solar cycles 24 and 25. Solar cycle 24, marked by historically low sunspot numbers and subdued solar activity, contrasts with solar cycle 25, which is projected to exhibit increased solar intensity. The research employs a multi-faceted approach, analyzing data from solar wind parameters, interplanetary magnetic fields, and geomagnetic indices such as Dst and Kp. Through statistical analysis and correlation studies, it examines the influence of sunspot number variations on the frequency, intensity, and duration of geomagnetic storms. Additionally, the study explores the distinct characteristics of geomagnetic activity during these two solar cycles, identifying key patterns and trends. By establishing a clearer understanding of the connection between sunspot numbers and geomagnetic storms, this research contributes to the development of more accurate predictive models for space weather events. These findings hold significant implications for improving preparedness and mitigation strategies to safeguard satellite operations, communication systems, and power grid stability against space weather impacts.