Learning

Understanding the Generation and Propagation of Coronal Mass Ejections

Solar Atmosphere and Corona → Shock Formation and Particle Acceleration

This learning path provides a systematic, advanced-level introduction to coronal mass ejections (CMEs), covering their physical origins, structure, kinematics, and evolution from the Sun through interplanetary space. It integrates necessary background in magnetohydrodynamics, plasma physics, and shock physics, and emphasizes the connection between CMEs and solar flares. Designed for undergraduate students in solar physics, the path builds from foundational concepts to current research topics, preparing learners for further study or research.