Overview
- A paper published Aug. 5, 2026 in Nature reports that the Daniel K. Inouye Solar Telescope captured small plasma vortices in magnetically active regions of the photosphere that match the Kelvin‑Helmholtz instability.
- The observations reached about 19 km spatial resolution using DKIST’s 4‑meter mirror and adaptive optics on Haleakalā, revealing dozens of vortices with characteristic separations near 65 km and sizes between roughly 25 and 170 km.
- Independent magnetohydrodynamic simulations, including runs with the MURaM code, reproduced the same vortex shapes, speeds and spacings, strengthening the identification of the phenomenon.
- Researchers say the vortices can twist and mix magnetic field lines, which could increase magnetic diffusion, feed small-scale energy cascades and contribute to coronal heating and the drivers of space weather.
- Teams led by the NSO plan to build automated detection pipelines and run quantitative energy‑budget studies on DKIST’s growing dataset to measure how much these vortices transport upward and affect solar eruption models.