Coronal holes appear as dark areas of the corona when viewed in ultraviolet light and in X-rays. Coronal holes are the source of strong solar wind gusts that carry solar particles out to our magnetosphere and beyond. These images are over the span of a week, and are Extreme ultraviolet Imaging Telescope (EIT) of the Solar and Heliospheric Observatory (SOHO), at a wavelength of 284 angstroms. | Stock Photo #4389-1635

Stock Photo #4389-1635, Coronal holes appear as dark areas of the corona when viewed in ultraviolet light and in X-rays. Coronal holes are the source of strong solar wind gusts that carry solar particles out to our magnetosphere and beyond. These images are over the span of a week, and are Extreme ultraviolet Imaging Telescope (EIT) of the Solar and Heliospheric Observatory (SOHO), at a wavelength of 284 angstroms.

Stock Photo - Coronal holes appear as dark areas of the corona when viewed in ultraviolet light and in X-rays. Coronal holes are the source of strong solar wind gusts that carry solar particles out to our magnetosphere and beyond. These images are over the span of a week, and are Extreme ultraviolet Imaging Telescope (EIT) of the Solar and Heliospheric Observatory (SOHO), at a wavelength of 284 angstroms.
Credit: NASA / Science Faction / SuperStock
4389-1635-N-X999 Image availability not guaranteed
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4389-1635
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