Resonantly Damped Surface and Body MHD Waves in a Solar Coronal Slab with Oblique Propagation
The theory of magnetohydrodynamic (MHD) waves in solar coronal slabs in a zero- β configuration and for parallel propagation of waves does not allow the existence of surface waves. When oblique propagation of perturbations is considered, both surface and body waves are able to propagate. When the perpendicular wavenumber is larger than a certain
Arregui, I. et al.
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2007