Three-dimensional kink modes in solar coronal slabs: Group velocities and their implications for impulsively excited waves
Context. Little attention has been paid to group velocities of three-dimensional (3D) magnetohydrodynamic (MHD) waves in solar coronal seismology. Aims. This study presents a comprehensive examination of the group velocities of trapped 3D kink modes in coronal slabs, emphasizing the connection of mo...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
EDP Sciences
2026-03-01
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| Σειρά: | Astronomy & Astrophysics |
| Θέματα: | |
| Διαθέσιμο Online: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57221-25/aa57221-25.html |
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