Solar prominence Ultraviolet SOHO Solar and Heliospheric Observatory satellite image of a solar prominence top right The prominence is erupting from the chromosphere orange which lies above the Suns visible surface the photosp here Prominences are dense clouds of plasma or ionised gas in the Suns outer layer the corona They are typically at temperatures of Kelvin much cooler than the several million Kelvin of the corona Active regions white mark areas of high solar activity The Suns activity peaks every years Image produced by SOHOs Extreme Ultraviolet Imaging Telescope EIT on September as the Sun approached such a time
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Product ID: 22109359002A