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Helioseismological Determination of Stratification and Dynamic Processes in the Solar Core
Published online by Cambridge University Press: 19 July 2016
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Helioseismology provides a powerful tool for investigating stratification and dynamics of plasma in the Sun's interior. The observed frequencies of the 5-min oscillations depend on density, sound speed, chemical abundances and angular velocity distributions inside the Sun. These parameters are estimated using inversion techniques.
- Type
- II. The Solar Interior
- Information
- Copyright
- Copyright © Kluwer 1990
References
REFERENCES
Christensen-Dalsgaard, J.
1988,
Seismology of the Sun & sun-like stars
, ESA Publ. SP-286, p. 431.Google Scholar