On the Sun, turbulent eddies could take place inside a coronal mass ejection as the plasma interacts with the solar wind in the background. “The turbulence that gives rise to KHI plays a fundamental role in regulating the dynamics of CMEs flowing through the ambient solar wind,” Evangelos Paouris, a member of the Wide-field Imager for Parker Solar Probe (WISPR) Science Team, and lead author of the new paper, said in a statement. “Hence, understanding turbulence is key in achieving a deeper understanding of CME evolution and kinematics.”