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On gravity waves in the Sun

Abstract : We briefly present our recent progress to model in 3-D the excitation and propagation of internal waves in the deep solar radiative interior. By modeling a rotating spherical convection zone on top of a radiative interior with a realistic seismically calibrated stable stratification (i.e solar-like Brunt-Väisälä frequency), we are able to generate a large spectrum of internal waves and modes thanks to the continuous pummeling of convective plumes. When comparing with an adiabatic oscillation code we find a good overall agreement and confirm that those waves are gravity waves.
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Contributor : Bruno Savelli Connect in order to contact the contributor
Submitted on : Tuesday, May 20, 2014 - 4:07:43 PM
Last modification on : Wednesday, October 27, 2021 - 2:45:34 PM

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A.S. Brun, Antoine Strugarek, S. Mathis, R.A. Garcia. On gravity waves in the Sun. Journal of Physics: Conference Series, IOP Publishing, 2013, 440, pp.012043. ⟨10.1088/1742-6596/440/1/012043⟩. ⟨cea-00993755⟩



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