A solar prominence is a large, bright feature extending outward from the Sun's surface. These structures are made of hot plasma and are often seen looping and arching above the Sun. Despite appearing to hover above the Sun's surface, solar prominences are actually magnetic phenomena. The immense magnetic fields of the Sun's corona trap the plasma, creating these beautiful and dynamic displays.

Solar prominences are a common sight during solar eclipses when the Moon blocks the bright solar disk, allowing these structures to become more visible against the darkened sky. Studying solar prominences is crucial for understanding the Sun's magnetic activity and its impact on space weather. Scientists monitor these phenomena to predict solar flares and geomagnetic storms that can affect satellites, communication systems, and power grids on Earth.