Analysing the occurrence of sunspots

Abstract

This study focuses on analyzing the occurrence of sunspots over a specific period to understand their temporal patterns and potential correlations with solar cycles. Using historical data, the analysis employed statistical methods to identify trends, periodicity, and anomalies in sunspot activity. The results highlight the cyclical nature of sunspot occurrence, confirming the presence of the approximately 11-year solar cycle. Additionally, the study explores the implications of sunspot activity on space weather and its broader impact on technological systems. These findings contribute to a deeper understanding of solar dynamics and their significance in astrophysical and terrestrial contexts.