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...

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Bibliografische Detailangaben

Hauptverfasser:	Liu Jing, Li Bo, Shi Mijie, Guo Mingzhe, Yu Hui
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	EDP Sciences 2026-03-01
Schriftenreihe:	Astronomy & Astrophysics
Schlagworte:	magnetohydrodynamics (mhd) waves sun: corona sun: magnetic fields
Online-Zugang:	https://www.aanda.org/articles/aa/full_html/2026/03/aa57221-25/aa57221-25.html
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