Loops of hot plasma in this multiple image show where a powerful coronal mass ejection (CME) has left the Sun. Solar physicists believe such loops are the signature of 'magnetic reconnection,' which accelerates charged particles in the coronal plasma to energies well above that of the already hot, coronal gas.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of Loops of hot plasma in this multiple image show where a powerful coronal mass ejection (CME) has left the Sun. Solar physicists believe such loops are the signature of 'magnetic reconnection,' which accelerates charged particles in the coronal plasma to energies well above that of the already hot, coronal gas. by NASA is available for licensing today.
Looking for a license?
Click here, and we'll help you find it! Questions? Just ask!
Click here, and we'll help you find it! Questions? Just ask!
DETAILS
Image Number: 4389-1615Rights ManagedCredit Line:NASA/SuperStockCollection:NASA Model Release:NoProperty Release:NoResolution:6880×2808
