Scientists have identified a mechanism on the Sun's surface that may explain the heating of its outer atmosphere, utilizing the advanced capabilities of the Daniel K. Inouye Solar Telescope.
Recent images from the Inouye Solar Telescope showcase the Kelvin-Helmholtz instability on the Sun's surface, providing insights into solar dynamics.
For decades, the Moon's sporadic magnetic field spikes, known as lunar external magnetic enhancements (LEMEs), have puzzled scientists. A new study reveals that these phenomena are likely caused by a novel form of the Kelvin-Helmholtz instability.
