On Inverting Asteroseismic Data

Simple item page
dc.creatorThompson, M. J.
dc.creatorChristensen-Dalsgaard, J.
dc.date2001-10-19
dc.date.accessioned2026-07-07T02:00:55Z
dc.date.available2026-07-07T02:00:55Z
dc.descriptionSome 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.
dc.descriptionTo 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0110447
dc.identifierhttp://arxiv.org/abs/astro-ph/0110447
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3570
dc.subjectAstrophysics
dc.titleOn Inverting Asteroseismic Data
dc.typetext

Files

Collections

arXiv