Tiny vortex storms revealed on the Sun by the world’s largest solar telescope

Researchers using the 4‑meter Daniel K. Inouye Solar Telescope imaged Kelvin‑Helmholtz vortexes at 416 nm on the Sun’s surface, showing 60–100 km spacing and 25–170 km-diameter structures that can grow quickly and travel 0.67–3 km/s. The observations, aided by high-speed imaging and advanced deconvolution, suggest a new mechanism for heat, mass, and magnetic-energy transport in the solar atmosphere and may affect convection and corona heating models. The study combines telescope data with simulations to confirm the effect, but is based on a short (about 3 minutes) observation window and calls for longer, magnetic-field–map measurements to fully quantify energy budgets.