On Inverting Asteroseismic Data
M. J. Thompson, J. Christensen-Dalsgaard
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.
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