File: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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Source NASA website; description: [1] high resolution image: [2]
Author NASA
Other versions Image:Sunprominence 304erupt crop.jpg


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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current12:22, 16 October 2008Thumbnail for version as of 12:22, 16 October 20082,400 × 2,400 (423 KB)Elipongo (talk | contribs){{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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