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Solar and Solar-Like Oscillations: Theory

Published online by Cambridge University Press:  30 March 2016

D.O. Gough
D.O. Gough*
Affiliation:
Institute of Astronomy, and Department of Applied Mathematics and Theoretical Physics, University of Cambridge

Abstract

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Solar five-minute oscillations provide a means of testing theoretical models of the sun. By judiciously combining data from low-degree modes, properties of the central and surface regions of the sun can be inferred separately. In principle, it should be possible to draw similar inferences from other stars, once adequate data are available. Recent solar rotational splitting data imply that in the equatorial regions much of the radiative envelope of the sun is rotating more slowly than the photosphere.

References

Bahcall, J.N., Huebner, W.F., Lubow, S.H., Parker, P.D. and Ulrich, R.K. 1982. Rev. Mod. Phys., 54, 767–799.Google Scholar
Berthomieu, G., Provost, J. and Schatzmann, E. 1984. Nature 308, 254–257.Google Scholar
Brown, T.M. 1985. Nature, 317, 591–594.CrossRefGoogle Scholar
Brown, T.M. 1986. Seismology of the sun and the distant stars (ed. Gough, D.O., NATO ASI Ser., Reidel, Dordrecht), 199–214.CrossRefGoogle Scholar
Christensen-Dalsgaard, J. 1982. Mon.Not.R.astr.Soc., 199, 735–761.Google Scholar
Christensen-Dalsgaard, J. 1984a. Theoretical problems in stellar stability and oscillations (ed. Gabriel, M. and Noels, A., Institut d’Astrophysique, Liège) 155–207.Google Scholar
Christensen-Dalsgaard, J. 1984b. Proc. Workshop on Space research prospects in stellar activity and variability (ed. Praderie, F., Paris Observatory Press) 11–45.Google Scholar
Christensen-Dalsgaard, J. 1986. Seismology of the sun and the distant stars (ed. Gough, D.O., NATO ASI Ser, Reidel, Dordrecht) 23–53.CrossRefGoogle Scholar
Christensen-Dalsgaard, J. and Frandsen, S., 1983. Solar Physics. 82, 469–486.Google Scholar
Christensen-Dalsgaard, J. and Gough, D.O. 1984. Solar seismology from space (ed. Ulrich, R.K. Harvey, J.W. Rhodes, E.J. Jr and Toomre, J., Jet Propulsion Lab. Publ. 84–84, Pasadena) 199–204.Google Scholar
Christensen-Dalsgaard, J., Gough, D.O. and Morgan, J.G. 1979. Astron. Astrophys. 73, 121–128; 79, 260.Google Scholar
Christensen-Dalsgaard, J., Duvall, T. Jr, Gough, D.O., Harvey, J.W. and Rhodes, E.J. Jr 1985. Nature, 315, 378–382.Google Scholar
Claverie, A., Isaak, G.R., McLeod, C.P., van der Raay, H.B. and Roca Cortes, T. 1981. Nature, 293, 443–445.Google Scholar
Cox, A.N. and Kidman, R.B. 1984. Theoretical problems in stellar stability and oscillations (ed. Gabriel, M. and Noels, A., Institute d’Astrophysique, Liège) 259–262.Google Scholar
Däppen, W., Gilliland, R. and Christensen-Dalsgaard, J. 1986. Nature submitted.Google Scholar
Deubner, F-L. and Gough, D.O. 1984. Ann.Rev. Astron.Astrophys. 22, 593–619.Google Scholar
Duvall, T.L. Jr and Harvey, J.W. 1984. Nature 310, 19–22.Google Scholar
Duvall Jr, T.L., Dziembowski, W.A., Goode, P.R., Gough, D.O., Harvey, J.W. and Leibacher, J.W. 1984. Nature, 310, 22–25.Google Scholar
Faulkner, J., Gough, D.O. and Vahia, M.N. 1986. Nature in press.Google Scholar
Fossat, E., Gelly, B. and Grec, G. 1986. Seismology of the sun and the distant stars (ed. Gough, D.O., NATO ASI Ser., Reidei, Dordrecht) 405–416.Google Scholar
Fossat, E., Grec, G., Gelly, B. and Decanini, Y. 1984. Comptes Rendus Acad. Sci. Paris, Ser 2, 229., 17–20.Google Scholar
Gough, D.O. 1983a. Phys. Bull. 34., 502–507.CrossRefGoogle Scholar
Gough, D.O. 1983b. ESO Workshop on primordial helium (ed. Shaver, P.A. Kunth, D. and Kjär, K., European Southern Observatory, Garching) 117–136.Google Scholar
Gough, D.O. 1985. Future missions in solar, heliospheric and space plasma physics (ed. Rolfe, E. and Battrick, B., European Space Agency SP-235, Noordwijk) 183–197.Google Scholar
Grec, G., Fossat, E. and Pomerantz, M. 1983. Solar Phys. 82, 55–66.Google Scholar
Harvey, J.W. and Duvall, T.L. Jr 1984. Solar seismology from space (ed. Ulrich, R.K. Harvey, J.W. Rhodes, E.J. Jr and Toomre, J., Jet Propulsion Lab. Publ. 84–84, Pasadena) 165–172.Google Scholar
Henning, H.M. and Scherrer, P.H. 1986. Seismology of the sun and the distant stars (ed. Gough, D.O., NATO ASI Ser., Reidel, Dordrecht) 55–62.Google Scholar
Kurtz, D. 1986. Seismology of the sun and the distant stars (ed. Gough, D.O., NATO ASI Ser., Reidel, Dordrecht) 417–440.CrossRefGoogle Scholar
Libbrecht, K.G. 1986. Nature submittedGoogle Scholar
Libbrecht, K.G. and Zirin, H. 1986. Astrophys. J. submitted.Google Scholar
Noyes, R.W., Baliunas, S.L., Belserene, E., Duncan, D.K., Horne, J. and Widrow, L. 1984. Astrophys. J., 285, L23–L26.Google Scholar
Provost, J. 1984. Observational tests of stellar evolution theory, Proc. IAU Symp. 105 (ed. Maeder, A. and Renzini, A., Reidel, Dordrecht) 47–64.Google Scholar
Rosner, R. and Weiss, N.O. 1985. Nature 317, 790–792.Google Scholar
Ross, J.E. and Aller, L.H. 1976. Science 191, 1223.Google Scholar
Schatzmann, E., Maeder, A., Angrand, F. and Glowinski, R. 1981. Astron. Astrophys. 96, 1–16.Google Scholar
Shibahashi, H., Noels, A. and Gabriel, M. 1983. Astron. Astrophys. 123, 283–288.Google Scholar
Tassoul, M. 1980. Astrophys. J. Suppl. 43, 469–490.Google Scholar
Ulrich, R.K. 1982. Astrophys. J. 258, 404-413.CrossRefGoogle Scholar
Ulrich, R.K. and Rhodes, E.J. Jr 1983. Astrophys. J. 265, 551–563.Google Scholar
Ulrich, R.K. and Rhodes Jr, E.J. 1984. Solar seismology from space (ed. Ulrich, R.K. Harvey, J.W. Rhodes, E.J. Jr, and Toomre, J., Jet Propulsion Lab. Publ. 84–84, Pasadena) 371–377.Google Scholar
Woodard, M. and Hudson, H.S. 1983. Nature 345, 589–593.Google Scholar