Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-23T15:15:12.059Z Has data issue: false hasContentIssue false

Helioseismological Determination of Stratification and Dynamic Processes in the Solar Core

Published online by Cambridge University Press:  19 July 2016

A.G. Kosovichev*
Affiliation:
Crimean Astrophysical Observatory 334413, Nauchny, Crimea, USSR

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Brown, T.M. & Morrow, C.A. 1987. Astrophys. J. Lett. , 314, L21.Google Scholar
Christensen-Dalsgaard, J. 1988, Seismology of the Sun & sun-like stars , ESA Publ. SP-286, p. 431.Google Scholar
Duvall, T.L. Jr & Harvey, J.W. 1984. Nature, 310, 19.Google Scholar
Duvall, T.L. Jr et al. 1988. Astrophys. J. , 324, 1158.Google Scholar
Gough, D.O. & Kosovichev, A.G. 1989, Inside the Sun. (in press).Google Scholar
Dziembowski, W. & Kosovichev, A.G. 1987. Acta Astron. , 37, 341.Google Scholar
Kosovichev, A.G. 1988. Sov. Astron. Lett. , 14, 145.Google Scholar