Resonance oscillations in sunspot and transformation of magneto-acoustic-gravity waves

Details Resonance oscillations in sunspot and transformation of magneto-acoustic-gravity waves Resonance oscillations in sunspot and transformation of magneto-acoustic-gravity waves

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..731z&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, April 15, 1984, p. 731-744.

Other

23

Gravity Waves, Magnetoacoustic Waves, Resonance, Solar Atmosphere, Solar Oscillations, Sunspots, Chromosphere, Coupled Modes, Mode Transformers, Solar Magnetic Field

Scientific paper

Sunspots are shown to contain three resonant layers, namely the chromospheric resonator for slow magneto-acoustic waves and two subphotospheric resonators for slow and fast waves. The resonators are coupled to each other through the wave transformation. A qualitative model for combined oscillatory convection in sunspots is proposed. The proposed scheme is used to examine the 3- and 5-min oscillations and the bright dots in sunspots.

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