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- W200076514 abstract "Two posters concerning solar and stellar oscillations were presented at the meeting by L. A. M. Nejad. The first, by Gough and Nejad, concerned inversion experiments with model helioseismic data: “The dependence of solar oscillation frequencies on the solar interior can be used by means of inversion techniques to provide information about the internal structure of the sun. Our experiments are part of a programme to develop inversion procedures for real data, and currently address only the spherically symmetrical component of the structure.” They construct two models: a simple model that will take the place of a real star, and a “trial model” that will be used to deduce the structure of the original model by iteration. So far, they have concentrated on using data only from low-degree modes. They have found that “to resolve the structure of the innermost region of the sun p modes alone are inadequate, though the addition of only a few f and g modes leads to substantial improvement. This is in accord with previous investigations using different inversion procedures (Cooper, A. J. 1981, PhD dissertation, University of Cambridge; Gough, D. O. 1984, in Solar Seismology from Space, R. K. Ulrich, J. Harvey, E. J. Rhodes Jr, and J. Toomre, eds, JPL Publ. 84-84, NASA, 49–78).” KeywordsSpherical SymmetryInversion TechniqueInversion ProcedureSymmetrical ComponentSolar InteriorThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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- W200076514 date "1988-01-01" @default.
- W200076514 modified "2023-09-26" @default.
- W200076514 title "Summary by S. Jordan and L. A. Willson of Selected Contributions on Helio- and Astero- Seismology" @default.
- W200076514 doi "https://doi.org/10.1007/978-94-009-3029-2_12" @default.
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