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Communication Dans Un Congrès Année : 2009

Using p-mode excitation rates for probing convection in solar-like stars

Résumé

We discuss how the possibility to measure mode excitation rates through means of helio- and asteroseismology has improved our capabilities to test convection models and numerical simulations of surface convection and avoids ambiguities that have limited previous approaches.

Dates et versions

hal-03734555 , version 1 (21-07-2022)

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Friedrich Kupka, Kevin Belkacem, Marie-José Goupil, Davoud-Reza Samadi. Using p-mode excitation rates for probing convection in solar-like stars. Proceedings of "38th Liege International Astrophysical Colloquium: Evolution and Pulsation of Massive Stars on the Main Sequence and Close to it", Jul 2013, Liège, Belgium. pp.24-26, ⟨10.1553/cia159s24⟩. ⟨hal-03734555⟩
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