X-ray of a filament in the solar corona
Numéro d’image : 11884088
| Solar corona. X-ray image of the Sun taken by the YOHKOH satellite of the eruption of a filament. The filament has a complex shape and is visible at upper and middle centre; it is formed in a region where a strong magnetic field bottles and accelerates coronal gases at high speed causing them to release a huge amount of energy in a relatively short period of time. This filament disappeared after only a few hours. The other bright areas are active regions in the corona where sunspots would be seen in visible light. The gas forming the corona has a very low density but high temperature (1 to 5 million degrees Kelvin) which causes the intense X-ray emission | |
| Licence : | Droits gérés |
| Crédit: | Science Photo Library / Jisas / Lockheed |
| Taille de l’image : | 4370 px × 4552 px |
| Model Release : | Non requis |
| Property Release : | Non requis |
| Restrictions : | - |
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