Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era
Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden changes in the magnetic field of stars with high energy release through magnetic reconnection, which can be observed across a wide range of the electromagnetic spectrum from radio waves to the optical range to X...
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| Päätekijät: | , , , , , , , , |
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| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
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MDPI AG
2024-07-01
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| Sarja: | Universe |
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| Linkit: | https://www.mdpi.com/2218-1997/10/8/313 |
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