Observational Evidence of Large-Scale Kelvin-Helmholtz Instability in Coronal Mass Ejections

This research provides valuable insight into the dynamics of coronal mass ejections (CMEs) and their interaction with the surrounding solar wind. The study's focus on the Kelvin-Helmholtz instability offers a unique perspective on energy transfer and plasma behavior during these events.

• •Identifies large-scale Kelvin-Helmholtz instability waves.
• •Provides observational evidence supporting theoretical models of CME dynamics.
• •Contributes to a better understanding of space weather phenomena.