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Published online by Cambridge University Press: 03 August 2017
The purpose of this investigation is to estimate how well the structure of the solar core might be inferred by inverting g-mode frequencies.
Delache and Scherrer (1983), Isaak et al. (1984), Severny et al. (1984) reported detection and identification of solar g modes. Although the results seem not to be complete it is helpful to invert the available data in order to understand what new information on the structure of the solar core can be obtained from g-mode frequencies.