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Solar flare accelerates nearly all electrons in a large coronal volume
Solar flares, driven by prompt release of free magnetic energy in the solar corona(1,2), are known to accelerate a substantial portion (ten per cent or more)(3,4) of available electrons to high energies. Hard X-rays, produced by high-energy electrons accelerated in the flare(5), require a high ambie...
| Autores principales: | , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2022
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9217745/ https://www.ncbi.nlm.nih.gov/pubmed/35676480 http://dx.doi.org/10.1038/s41586-022-04728-8 |