Cambridge University Press, Proceedings of the International Astronomical Union, S239(2), p. 364-369, 2006
DOI: 10.1017/s1743921307000737
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AbstractWe investigate the possibility of detecting deep convection in the Sun by computing travel-time shifts induced by convective flows interacting with propagating waves. The convection zone is modeled using a velocity profile taken from an Anelastic convection simulation. We present results obtained from a ray calculation of travel-time shifts. We compare these results with a full 3D calculation of the wave-flow interaction.