File:CoronalMassEjection.jpg
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A composite image from observations by the SOHO satellite observatory. This combines (red) a coronagraphic view using visible light and (brown) a direct view using EUV radiation at 17.1 nm. The solar disk is not bright at this wavelength, so that an occulter is not necessary for coronal viewing.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:59, 29 December 2007 | | 1,875 × 2,100 (1.44 MB) | Hugh Hudson (Talk | contribs) | A composite image from observations by the SOHO satellite observatory. This combines (red) a coronagraphic view using visible light and (green) a direct view using EUV radiation at 17.1 nm. The solar disk is not bright at this wavelength, so that an occu |
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