Turbulent acceleration of electrons by large-amplitude magnetohydrodynamic waves in solar flares
Context. Solar flares appear as a sudden local enhancement of the emission of electromagnetic waves from the radio to the γ-ray range on the Sun. This radiation is primarily generated by energetic electrons. In addition, these electrons play an important role, since they carry a substantial part of...
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| Hlavní autoři: | , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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EDP Sciences
2026-04-01
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| Edice: | Astronomy & Astrophysics |
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| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/04/aa57249-25/aa57249-25.html |
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