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X particles 3.5 torrent7/10/2023 Flares are powered by the sudden (timescales of minutes to tens of minutes) release of magnetic energy stored in the corona. Flares occur in active regions often around sunspots, where intense magnetic fields penetrate the photosphere to link the corona to the solar interior. Most of the energy is spread over frequencies outside the visual range the majority of the flares are not visible to the naked eye and must be observed with special instruments. Flares produce electromagnetic radiation across the electromagnetic spectrum at all wavelengths, from radio waves to gamma rays. ![]() The plasma medium is heated to tens of millions of kelvins, while electrons, protons, and heavier ions are accelerated to near the speed of light. ![]() Solar flares affect all layers of the solar atmosphere ( photosphere, chromosphere, and corona).
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