About structure inversions of simulated COROT data for a solar like star

Details About structure inversions of simulated COROT data for a solar like star About structure inversions of simulated COROT data for a solar like star

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..411b&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Physics

6

Stars: Oscillations

Scientific paper

We study the potential of exploring the internal structure of solar like stars which could be observed by COROT. We consider a solar like star of mass and age which allows stochastically excited oscillations according to the results of Houdek et al (1999). Taking into account COROT observational constraints we estimate a set of observable modes with the uncertainties on their frequencies; then, in the same way followed by Gough and Kosovichev (1993), we evaluate the possibility of inferring structure properties of the star using inversion techniques.

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