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Helioseismology with High Degree p-Modes*

Published online by Cambridge University Press:  12 April 2016

F.-L. Deubner
F.-L. Deubner*
Affiliation:
Institut für Astronomie und Astrophysik, D-8700 Würzburg, F.R.G.

Abstract

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The value of p-modes of high degree l as a diagnostic for the structure and dynamics of the solar envelope is reviewed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 66: Problems of Solar and Stellar Oscillations , 1983 , pp. 103 - 109
Copyright
Copyright © Reidel 1983

Footnotes

*

Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1-5 September, 1981.

References

Aime, C. and Ricort, G.: 1975, Astron. Astrophys. 39, 319.Google Scholar
Christensen-Dalsgaard, J.: 1980, private communication.Google Scholar
Claverie, A., Isaak, G.R., 1McLeod, C.P., van der Raay, H.B., and Roca Cortes, T. :1983, Solar Phys. 82, 233 (this volume).CrossRefGoogle Scholar
Deubner, F.-L.: 1972, Solar Phys. 22, 263.CrossRefGoogle Scholar
Deubner, F.-L.: 1975, Astron. Astrophys. 44, 371.Google Scholar
Deubner, F.-L.: 1981, in Jordan, S. (ed.), The Sun as a Star, NASA/CNRS monograph series on Nonthermal Phenomena in Stellar-Atmospheres, Washington, Paris, p. 65.Google Scholar
Deubner, F.-L., Ulrich, R.K., and Rhodes, E.J. Jr.: 1979, Astron. Astrophys. 72, 177.Google Scholar
Gough, D.: 1981, private communication.Google Scholar
Gouttebroze, P. and Leibacher, J.W.: 1980, Astrophys. J. 238, 1134.CrossRefGoogle Scholar
Grec, G., Fossat, E., and Pomeranz, M.: 1980, Nature 288, 541.CrossRefGoogle Scholar
Hill, F., Toomre, J., and November, L.J.: 1983, Solar Phys. 82, 411 (this volume).CrossRefGoogle Scholar
Howard, R.: 1967, Solar Phys, 2, 3.CrossRefGoogle Scholar
Leibacher, J.W. and Stein, R.F.: 1971, Astrophys. Letters 7, 191.Google Scholar
Leibacher, J.W. and Stein, R.F.: 1981, in Jordan, S. (ed.), The Sun as a Star, NASA/CNRS monograph series on Nonthermal Phenomena in Stellar Atmospheres, Washington, Paris, p. 263.Google Scholar
Leibacher, J.W., Gouttebroze, P., and Stein, R.F.: 1982, Astrophys. J. 258, 393.CrossRefGoogle Scholar
Leighton, R.B., Noyes, R.W., and Simon, G.W.: 1962, Astrophys. J. 135, 474.CrossRefGoogle Scholar
Lubow, S.H., Rhodes, E.J. Jr., and Ulrich, R.J.: 1980, in Hill, H. and Dziembowski, W. (eds.), Non-Radial and Non-Linear Stellar Oscillation, Springer Verlag, Berlin, p. 300.Google Scholar
Mein, .N.: 1977, Solar Phys. 52, 283.CrossRefGoogle Scholar
Rhodes, E.J. Jr., Harvey, J.W., and Duvall, T.L. Jr.: Solar Phys. 82, 111 (this volume).CrossRefGoogle Scholar
Rhodes, E.J. Jr. Deubner, F.-L., and Ulrich, R.K.: 1979, Astrophys. J. 227, 629.CrossRefGoogle Scholar
Schmieder, B.: 1978, Solar Phys. 57, 245.CrossRefGoogle Scholar
Ulrich, R.K.: 1970, Astrophys. J. 162, 993.CrossRefGoogle Scholar
Ulrich, R.K. and Rhodes, E.J. Jr.: 1977, Astrophys. J. 218, 521.CrossRefGoogle Scholar
Ulrich, R.K., Rhodes, E.J. Jr., and Deubner, F.-L.: 1979, Astrophys. J. 227, 638.CrossRefGoogle Scholar
White, O.R. and Cha, M.Y.: 1973, Solar Phys. 31, 23.CrossRefGoogle Scholar
Wolff, C.L.: 1972, Astrophys. J. 176, 833.CrossRefGoogle Scholar