Other
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242..353c&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Feb. 1, 1990, p. 353-369.
Other
71
Helioseismology, Solar Interior, Solar Oscillations, Asymptotic Properties, Error Analysis, Least Squares Method, Solar Spectra
Scientific paper
Consideration is given to the inversion techniques used to study the properties of the solar interior with observed frequencies of solar oscillation. Linear inversion schemes for helioseismic problems are compared in terms of resolutions and error properties. Measures of the error amplification resulting from the inversion and the resolution achieved are defined. Although the study includes only inversions for a spherically symmetric angular velocity distribution, it is suggested that the methods may be used to study kernels for other properties of the solar interior.
Christensen-Dalsgaard Joergen
Schou Jepser
Thompson Michael J.
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