Scientists discover Kelvin-Helmholtz Instability on the surface of the Sun
Scientists using the NSF Daniel K. Inouye Solar Telescope have identified Kelvin-Helmholtz instability on the Sun's surface. These swirling patterns may explain how magnetic energy builds up to fuel solar flares and atmospheric heating.
Why it matters
Understanding these solar mechanisms is critical for predicting space weather that can disrupt satellites, power grids, and global communication infrastructure.
Scientists using the U.S. National Science Foundation Daniel K. Inouye Solar Telescope have made a major breakthrough in solar physics, discovering Kelvin-Helmholtz Instability on the surface of the Sun — a finding that could help explain explosive solar activity and other solar phenomena.
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