Relation of Solar Flares, CMEs And Sunspot Number from Solar Minimum (Dec.2019) To Predicted Solar Maximum (April 2025)

The ongoing Solar Cycle 25 presents a crucial opportunity to study coronal mass ejections (CMEs) solar flares and Sunspot numbers, key drivers of space weather that significantly impact Earth's magnetosphere and technological systems. From the solar minimum phase to the predicted solar maximum, this study examines the properties, occurrence, and severity of CMEs and solar flares. Utilizing information from space-based observatories like the Parker Solar Probe, the Solar Dynamics Observatory, and the Solar and Heliospheric Observatory (SOHO), we examine patterns in magnetic field fluctuations, plasma dynamics, and solar activity. In this work, we seek to establish relationships between flare activity, CME occurrence rates, and solar magnetic field changes in order to enhance prediction models for space weather forecasting. By improving our knowledge of solar energetic events and their possible effects on Earth's space environment, the findings will help create mitigation plans for communication and satellite operations.