Restr:Solar prominence from STEREO spacecraft September 29, 2008.jpg

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English: The STEREO (Ahead) spacecraft observed this visually stunning solar prominence eruption on September 29, 2008, in the 304 angstrom wavelength of extreme UV light. Prominences are relatively cool clouds of gas suspended above the sun and controlled by magnetic forces. The prominence rose and cascaded to the right over several hours, appearing something like a flag unfurling, as it broke apart and headed into space. The prominence is composed of ionized Helium that is about 60,000 degrees Kelvin.
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29 Gwe 2008

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red16 Her 2008 da 12:22Munud eus stumm an 16 Her 2008 da 12:222 400 × 2 400 (423 Kio)Elipongo{{Information |Description={{en|1=The STEREO (Ahead) spacecraft observed this visually stunning solar prominence eruption on September 29, 2008, in the 304 angstrom wavelength of extreme UV light. Prominences are relatively cool clouds of gas

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