Polarization of decayless kink oscillations in a 3D MHD coronal loop model
Decayless kink oscillations are frequently observed in solar coronal loops and are considered potential contributors to coronal heating. Despite the ubiquity of this wave phenomenon, its driving mechanism remains unclear. Studies to derive the polarization state of these oscillations, which would be...
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| Hauptverfasser: | , , |
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| Format: | Artigo |
| Sprache: | Inglês |
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EDP Sciences
2026-03-01
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| Schriftenreihe: | Astronomy & Astrophysics |
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| Online-Zugang: | https://www.aanda.org/articles/aa/full_html/2026/03/aa58203-25/aa58203-25.html |
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