Total solar eclipse. The last rays of the sun and solar prominences as seen during a total solar eclipse. The disc of the moon has moved over the disc of the Sun. At totality the Moon fits over the Sun and only the sun's corona (atmosphere) is visible. The moment of totality lasts for only a few minutes. Total solar eclipses usually occur less than once a year and can only be seen from a small area of the Earth's surface. Photographed in March 2006 from Turkey | |
Licence : | Droits gérés |
Crédit: | Science Photo Library / Tafreshi, Babak |
Taille de l’image : | 3500 px × 2581 px |
Model Release : | Non requis |
Property Release : | Non requis |
Restrictions : | - |