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Radiation zone
From Wikipedia, the free encyclopedia
The radiation zone is the middle zone in the sun's interior. Energy travels out of the core into the radiation zone. Energy travels through the radiation zone in the form of electromagnetic radiation. The radiation zone is so dense that the waves bounce around. The energy might not get out of the radiation zone for millions of years.
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| Structure: Solar Core - Radiation Zone - Convection Zone |
| Atmosphere - Photosphere - Chromosphere - Transition region - Corona |
| Extended Structure: Termination Shock - Heliosphere - Heliopause - Heliosheath - Bow Shock |
| Solar Phenomena: Sunspots - Faculae - Granules - Supergranulation - Solar Wind - Spicules |
| Coronal loops - Solar Flares - Solar Prominences - Coronal Mass Ejections |
| Moreton Waves - Coronal Holes |
| Other: Solar System - Solar Variation - Solar Dynamo - Heliospheric Current Sheet - Solar Radiation - Solar Eclipse |
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