Image:SOHO EIT ultraviolet corona image.gif

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An image taken by the Solar and Heliospheric Observatory (SOHO) spacecraft's EIT instrument showing the corona in deep UV at 17.1 nm. The UV wavelength corresponds to resonance lines of eight and nine times ionized iron (Fe IX/X) which is churning in the hot coronal plasma at about 1 million kelvin.

SOHO Copyright Notice: The use of SOHO images or data for public education efforts and non-commercial purposes is strongly encouraged and requires no expressed authorization. It is requested, however, that any such use properly attributes the source of the images or data as: "Courtesy of SOHO/[instrument] consortium. SOHO is a project of international cooperation between ESA and NASA." Where [instrument] stands for the name of the instrument that acquired the data (i.e. SOHO/EIT, SOHO/LASCO, etc).

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(del) (cur) 23:42, 11 August 2004 . . Deglr6328 (Talk | contribs) . . 1024×1024 (828,710 bytes) (An image taken by the Solar and Heliospheric Observatory (SOHO) spacecraft's EIT instrument showing the corona in deep UV at 17.1 nm {{PD-USGov}})