Solar Physics paper

Abstract This study examines the complex relationships among high-energy solar particle events (SEPs), solar flares, and coronal mass ejections (CMEs) at the onset of Solar Cycle 25. We investigate the sources and characteristics of high-energy solar particles and explore the dynamics of solar flares and CMEs within this evolving solar cycle. While CMEs are often associated with SEPs, their occurrence isn't guaranteed due to the intricate interplay of magnetic fields and propagation conditions. Understanding this variability is crucial for improving predictive capabilities related to space weather events. We leverage advanced observational techniques to analyze CMEs and assess their correlations with solar cycle activity. Our research also considers the potential impacts of these solar events on Earth's space weather and technology infrastructure. Comparisons with previous solar cycles provide valuable insights into the evolving nature of solar activity. We conclude by discussing the current state of predictive modeling and forecasting, emphasizing the need for continued advancements in space weather prediction models. Overall, this study contributes to our understanding of solar physics and space weather, particularly regarding the dynamics of high-energy solar particle events and their relationships with flares and CMEs during Solar Cycle 25's early stages.