A solar flare is a tremendous explosion of electromagnetic radiation that occurs in the atmosphere of the sun. Flares can be seen in active locations and are frequently, but not always, linked to coronal mass ejections, solar particle events, and other solar occurrences. Solar flares have a power-law magnitude spectrum; an energy release of 1020 joules is usually enough to produce a clearly observable event, but a large event can emit up to 1025 joules. They were first discovered in the visible electromagnetic spectrum, namely in the hydrogen H-alpha emission line, but they can now be identified in everything from radio waves to gamma rays.
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