Possible effects of subphotospheric flows on helio-seismic g-modes

Details Possible effects of subphotospheric flows on helio-seismic g-modes Possible effects of subphotospheric flows on helio-seismic g-modes

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pobeo..80...53c&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, Vol. 80, p. 53-56

Physics

Fluid Dynamics

Helioseismology, Doppler Resonance, Wave Amplification

Scientific paper

Non-uniform subphotospheric horizontal flows may arise from differential rotation of the sun's interior as well as from a global meridional plasma circulation. The fluid dynamics equations for a model of solar interior with the convective zone reveal a second order singularity at locations where a non-uniform flow and eigen-modes of solar global oscillations are in resonance. This indicates a possibility for a local resonant amplification of internal g-modes which makes them easier for observational detection.

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