Abstract
The purpose of this investigation is to estimate how well the structure of the solar core might be inferred by inverting g-mode frequencies.
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© 1988 International Astronomical Union
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Kosovichev, A.G. (1988). An Attempt to Determine the Structure of the Solar Core from Observed G-Mode Frequencies. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_32
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DOI: https://doi.org/10.1007/978-94-009-4009-3_32
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