Abstract
The theory of acoustic wave propagation in a structured moving atmosphere is presented. It is shown that the phase velocity of acoustic waves in the atmosphere differs from the sound speed and depends on the frequency and the direction of propagation. The effect of the dispersion and anisotropy of waves on p-modes in the convection zone is discussed.
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Zhugzhda, Y.D., Stix, M. (1994), AA 291, 310
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© 1997 Springer Science+Business Media Dordrecht
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Zhugzhda, Y.D. (1997). The Theory of Anisotropic P-Mode Propagation in the Solar Convection Zone. In: Pijpers, F.P., Christensen-Dalsgaard, J., Rosenthal, C.S. (eds) SCORe ’96: Solar Convection and Oscillations and their Relationship. Astrophysics and Space Science Library, vol 225. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5167-2_19
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DOI: https://doi.org/10.1007/978-94-011-5167-2_19
Publisher Name: Springer, Dordrecht
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