On the modal structure of the solar oscillations

Details On the modal structure of the solar oscillations On the modal structure of the solar oscillations

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105..417s&link_type=abstract

Astronomy and Astrophysics, vol. 105, no. 2, Jan. 1982, p. 417, 418. Research supported by the Centre National de la Recherche

Astronomy and Astrophysics

Astrophysics

3

Frequency Response, Modal Response, Solar Oscillations, Stellar Structure, Plasma Oscillations, Solar Interior, Vertical Distribution

Scientific paper

The very different frequency structure of the high and low order modes of the observed solar oscillations is shown to be due to the difference in their cavities. The low order mode cavities extend deep into the solar interior, while the high order mode cavities are confined near the surface of the Sun. As a result the vertical component of the wave vector has a very different dependence on depth in the two cases.

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