Ubiquitous Kelvin-Helmholtz instabilities driving plasma mixing on the Sun.

The interaction between the magnetic field and turbulent convection in the Sun's photosphere drives the dynamics, evolution and structuring of its magnetized atmosphere.

The interaction between the magnetic field and turbulent convection in the Sun's photosphere drives the dynamics, evolution and structuring of its magnetized atmosphere. This interaction often takes place at or below the spatial resolution of modern-day observations. Here we…