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

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

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.159...24k&link_type=abstract

"Communications in Asteroseismology, Vol. 159, p. 24-26. Proceedings of "JENAM 2008 Symposium No 4: Asteroseismology and Stellar

Physics

1

Scientific paper

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.

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