Signatures of localised particle acceleration at a global coronal shock wave
Context. Extreme ultraviolet (EUV) waves are global waves in the solar corona that accelerate particles. The efficiency of this acceleration depends on local plasma characteristics such as the Alfvén speed and the geometry of the magnetic field. This shock-driven particle acceleration produces radio...
Kaydedildi:
| Asıl Yazarlar: | , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
EDP Sciences
2026-05-01
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| Seri Bilgileri: | Astronomy & Astrophysics |
| Konular: | |
| Online Erişim: | https://www.aanda.org/articles/aa/full_html/2026/05/aa58124-25/aa58124-25.html |
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