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An attempt to determine the structure of the solar core from observed g-mode frequencies

Published online by Cambridge University Press:  03 August 2017

A.G. Kosovichev
A.G. Kosovichev*
Affiliation:
Crimean Astrophysical Observatory of the USSR Academy of Sciences, Crimea, USSR

Extract

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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.

Type
Chapter 2: Theory of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 141 - 146
Copyright
Copyright © Reidel 1988 

References

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