File:Our Sun.jpg

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English: Extreme Ultraviolet Imaging Telescope (EIT) image of a huge, handle-shaped prominence taken on Sept. 14,1999 taken in the 304 angstrom wavelength - Prominences are huge clouds of relatively cool dense plasmasuspended in the Sun's hot, thin corona. At times, they can erupt,escaping the Sun's atmosphere. Emission in this spectral line shows theupper chromosphere at a temperature of about 60,000 degrees K. Everyfeature in the image traces magnetic field structure. The hottest areasappear almost white, while the darker red areas indicate coolertemperatures. Courtesy of SOHO/Extreme Ultraviolet Imaging Telescope (EIT) consortium. SOHO is a project of international cooperation between ESA and NASA.
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Xigasho https://www.nasa.gov/multimedia/imagegallery/image_feature_21.html
Qoraa NASA

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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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Our Sun

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