A solar flare is an intense burst of electromagnetic radiation generated in the sun's atmosphere — the layers of sparse but hot gas that lie above its visible surface, or photosphere.
The vast amounts of energy released by a typical solar flare are mostly radiated away in the ultraviolet and X-ray part of the electromagnetic spectrum, at shorter wavelengths with higher energies than visible light. Solar flares can heat nearby material in the sun's atmosphere, launching huge blobs…
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A potential cure
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