期刊
ASTROPHYSICAL JOURNAL
卷 850, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/aa9223
关键词
magnetohydrodynamics (MHD); Sun: activity; Sun: oscillations; Sun: photosphere
资金
- Odysseus type II funding (FWO-Vlaanderen)
- IAP [P7/08 CHARM]
- KU Leuven [GOA-2015-014]
- European Research Council (ERC) under the European Union's Horizon research and innovation programme [724326]
We study the effect of resonant absorption of surface sausage and surface kink modes under photospheric conditions where the slow surface sausage modes undergo resonant damping in the slow continuum and the surface kink modes in the slow and Alfven continua at the transitional layers. We use recently derived analytical formulas to obtain the damping rate (time). By considering linear density and linear pressure profiles for the transitional layers, we show that resonant absorption in the slow continuum could be an efficient mechanism for the wave damping of the slow surface sausage and slow surface kink modes while the damping rate of the slow surface kink mode in the Alfven continuum is weak. It is also found that the resonant damping of the fast surface kink mode is much stronger than that of the slow surface kink mode, showing a similar efficiency as under coronal conditions. It is worth noting that the slow body sausage and kink modes can also resonantly damp in the slow continuum for those linear profiles.
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