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Helioseismic Investigation of Solar Internal Structure

Published online by Cambridge University Press:  12 April 2016

Jørgen Christensen-Dalsgaard*
Affiliation:
Astronomisk Institut, Aarhus Universitet,DK-8000 Aarhus C, Denmark

Abstract

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The solar oscillation frequencies provide our only means of obtaining detailed information about conditions inside the Sun. Here I give a brief overview of the relevant properties of solar models and solar oscillations, and present examples of the dependence of the oscillation frequencies on the structure of the model. Furthermore I discuss some results obtained so far from analysis of observed frequencies.

Type
Part 3: Helioseismology
Copyright
Copyright © Kluwer 1990

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