Learning

Solar Origins of Space Weather

Sun's Structure and Magnetic Field → Space Weather Prediction and Monitoring

This learning path takes undergraduate students from the Sun's internal structure and magnetic field to the origins of space weather phenomena, including solar flares, CMEs, and the solar wind, and their effects on Earth. It covers the solar cycle, geomagnetic storms, and SEP events, and concludes with prediction and monitoring efforts. The path emphasizes the physical connections between solar activity and its impacts on near-Earth space.