Plasma in the solar corona condenses and falls into the Sun, being transported along magnetic field lines.

Schmidt, D., Schad, T.A., Yurchyshyn, V. et al. Observations of fine coronal structures with high-order solar adaptive optics. Nat Astron 9, 1148–1157 (2025). https://doi.org/10.1038/s41550-025-02564-0