The surface of the sun churns with energy and frequently ejects masses of highly-magnetized plasma towards Earth.
Sometimes these ejections are strong enough to crash through the magnetosphere—the natural magnetic shield that protects the Earth—damaging satellites or electrical grids.
Such space weather events can be catastrophic.
Turbulence plays a key role in the dynamics of the solar wind and coronal mass ejections.
This complex phenomenon has many facets, including the role of shock-turbulence interaction and ion acceleration.
Source
Sometimes these ejections are strong enough to crash through the magnetosphere—the natural magnetic shield that protects the Earth—damaging satellites or electrical grids.
Such space weather events can be catastrophic.
Turbulence plays a key role in the dynamics of the solar wind and coronal mass ejections.
This complex phenomenon has many facets, including the role of shock-turbulence interaction and ion acceleration.
Source