Sensitivity of five minute eigenfrequencies to the structure of the sun-Reference-Cited by-同舟云学术

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Sensitivity of five minute eigenfrequencies to the structure of the sun

Published: Issue: Volume: Page:307-312
ISSN:
Container-title:Nonradial and Nonlinear Stellar Pulsation
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Author:

Berthomieu G.,Cooper A. J.,Gough D. O.,Osaki Y.,Provost J.,Rocca A.

Publisher

Springer Berlin Heidelberg

Link

http://link.springer.com/content/pdf/10.1007/3-540-09994-8_29.pdf

Reference24 articles.

1. Ando, H. and Osaki, Y. 1975, Pub. Astr. Soc. Japan, 27, 581.

2. Ando, H. and Osaki, Y. 1977, Pub. Astr. Soc. Japan, 29, 221.

3. Baker, N.H., Moore, D.W. and Spiegel, E.A. 1971, Quart. J. Mech. Appl. Math., 24, 391.

4. Baker, N.H. and Temesvary, S. 1966, Tables of convective stellar envelopes (Goddard Institute for Space Studies, New York).

5. Brown, T.M. and Harrison, R.L. 1980, these proceedings.

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