On Inverting Asteroseismic Data
Astrophysics
2007-05-23 v1
Abstract
Some issues of inverting asteroseismic frequency data are discussed, including the use of model calibration and linearized inversion. An illustrative inversion of artificial data for solar-type stars, using least-squares fitting of a small set of basis functions, is presented. A few details of kernel construction are also given.
Cite
@article{arxiv.astro-ph/0110447,
title = {On Inverting Asteroseismic Data},
author = {M. J. Thompson and J. Christensen-Dalsgaard},
journal= {arXiv preprint arXiv:astro-ph/0110447},
year = {2007}
}
Comments
To appear in Proc. 1st Eddington Workshop, `Stellar Structure and Habitable Planet Finding' (ESA SP-485), eds F. Favata, I. W. Roxburgh and D. Galadi. Processed with ESASPStyle